tag:blogger.com,1999:blog-71557779714552537062024-02-18T23:48:02.823-08:00Da Terra ao Céu e ao Infinito - Algumas das 88 ConstelaçõesJanine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comBlogger75125tag:blogger.com,1999:blog-7155777971455253706.post-67267136467919303482013-08-24T06:42:00.000-07:002015-06-19T08:21:20.224-07:00MEU AMOR PELAS ESTRELAS...<div class="separator" style="clear: both; text-align: center;">
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiJfwAAUnGDZ-gYDD5VzNzYeHe0ukbr6w4io7z9VVD2QopuTRHimcmQMvjxhRvL4Mr3JsLVVOtGEELW17xo3qJxIREi7rvp1ctt8HZmgGUgg3MwxcXdp8YLa7eHb4v05VgC-76bSQ4PbG23/s1600/eu.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiJfwAAUnGDZ-gYDD5VzNzYeHe0ukbr6w4io7z9VVD2QopuTRHimcmQMvjxhRvL4Mr3JsLVVOtGEELW17xo3qJxIREi7rvp1ctt8HZmgGUgg3MwxcXdp8YLa7eHb4v05VgC-76bSQ4PbG23/s1600/eu.png" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 14px; text-align: left;"><span style="background-color: white;"><span style="font-size: x-small;">Stellarium</span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 14px; text-align: left;"><b style="background-color: white;">Olharmos para o céu e nos comover </b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif; line-height: 14px; text-align: left;"><b style="background-color: white;">é o primeiro passo. </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="background-color: white; line-height: 14px; text-align: left;"><br /></span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="line-height: 14px; text-align: left;"><br /></span></span><span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="line-height: 14px; text-align: left;">Janine Milward</span></span></span><br />
<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="line-height: 14px; text-align: left;"><br /></span></span><span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="line-height: 14px; text-align: left;"><br /></span></span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="background-color: white; line-height: 14px; text-align: left;"><br /></span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="background-color: white; line-height: 14px; text-align: left;">Olhar para o céu noturno é algo que sempre me comoveu, </span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="background-color: white; line-height: 14px; text-align: left;">desde pequena, com meus irmãos e eu indo parar no alto da caixa de água, </span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="background-color: white; line-height: 14px; text-align: left;">em noites escuras, para ficarmos conversando sob as estrelas .... </span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="background-color: white; line-height: 14px; text-align: left;">e sobre as estrelas. </span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="background-color: white; line-height: 14px; text-align: left;"><br /></span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="background-color: white; line-height: 14px; text-align: left;"> Naqueles tempos do passado - metade do século XX -, </span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="background-color: white; line-height: 14px; text-align: left;">a Nova Friburgo que morávamos era ainda uma cidade de luzes poucas</span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="background-color: white; line-height: 14px; text-align: left;"> e voltadas, amareladamente pálidas,</span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="background-color: white; line-height: 14px; text-align: left;"> somente para o chão das ruas simples e provincianas, que bom.</span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="background-color: white; line-height: 14px; text-align: left;"><br /></span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="background-color: white; line-height: 14px; text-align: left;">Havia também um livrão antigo de astronomia, em francês </span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="background-color: white; line-height: 14px; text-align: left;">(que mais tarde descobri que é uma verdadeira relíquia </span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="background-color: white; line-height: 14px; text-align: left;">e que minha mãe deixou para mim, como herança:</span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="background-color: white; line-height: 14px; text-align: left;">Camille Flammarion, Astronomie Populaire, edição de 1922!),</span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="line-height: 14px; text-align: left;"> e sempre meus irmãos e eu estávamos folheando </span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="line-height: 14px; text-align: left;">e lendo (tentando entender o francês aliado às fotos black and white, </span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[0]" style="line-height: 14px; text-align: left;">do passado, de mais de um século atrás!).</span><br data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[1]" style="line-height: 14px; text-align: left;" /><b><br data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[2]" style="line-height: 14px; text-align: left;" /><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[3]" style="line-height: 14px; text-align: left;">Olharmos para o céu e nos comover é o primeiro passo. </span></b></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[3]" style="background-color: white; line-height: 14px; text-align: left;"><b><br /></b></span></span></div>
<b><span style="background-color: white;"></span><br /></b>
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<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[3]" style="line-height: 14px; text-align: left;"><b>O segundo passo é decidirmos se vamos ficar felizes e contentes </b></span></span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[3]" style="line-height: 14px; text-align: left;"><b>dentro do Caos </b></span></span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[3]" style="line-height: 14px; text-align: left;"><b>ou se vamos tentar trazer o Caos para dentro do Cosmos.,.</b></span></span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[3]" style="line-height: 14px; text-align: left;"><b> Cosmos quer dizer ORDENAÇÃO</b></span></span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><b><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[3]" style="line-height: 14px; text-align: left;"> e Caos quer dizer caos mesmo....</span></b><br data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[5]" style="line-height: 14px; text-align: left;" /><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[6]" style="line-height: 14px; text-align: left;">Acho que dá para começar tentando saber quem é quem</span></span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[6]" style="line-height: 14px; text-align: left;"> - dentro das estrelas mais brilhantes, é claro, </span></span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[6]" style="line-height: 14px; text-align: left;">ou através pedacinhos de constelações</span></span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[6]" style="line-height: 14px; text-align: left;"> (como o Cinturão de Órion conhecido como As Três Marias), </span></span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[6]" style="line-height: 14px; text-align: left;">ou mesmo através constelações inteiras </span></span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[6]" style="line-height: 14px; text-align: left;">(quem não sabe apontar para o Cruzeiro do Sul?).</span><br data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[7]" style="line-height: 14px; text-align: left;" /><br data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[8]" style="line-height: 14px; text-align: left;" /><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[9]" style="line-height: 14px; text-align: left;">Enfim, é preciso se estar em lugar de céu mais escuro e transparente,</span></span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[9]" style="line-height: 14px; text-align: left;"> longe das luzes poluentes das cidades, grandes, médias, pequenas...</span></span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[9]" style="line-height: 14px; text-align: left;"><br /></span></span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[9]" style="line-height: 14px; text-align: left;"> Luzes são luzes em qualquer lugar </span></span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[9]" style="line-height: 14px; text-align: left;">e poluem nossa visão do céu estrelado, </span></span></span></div>
<div style="background-color: #fefafb; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[9]" style="line-height: 14px; text-align: left;">escondem as estrelas.</span></span></span></div>
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<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><span data-reactid=".r[2cpfg].[1][3][1]{comment615871251803838_5807971}.[0].{right}.[0].{left}.[0].[0].[0][3].[0].[9]" style="line-height: 14px; text-align: left;"><br /></span></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<tr><td style="text-align: center;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhQCm0iCY_TUhbqNyKVtSsY2MDixSbjNT43o_i8ndOzJkIw1TogBZ7GQNdwCa8zYAo4D54jDX4SS_apMBTvEEolhg8p7XtTfIjaZO6bq4jSEBSZ_rkK993Pjt4Pm-XyqTk6djxM5S6eu9mM/s1600/mapa+do+universo+que+vemos+em+positivo.gif" imageanchor="1" style="margin-left: auto; margin-right: auto;"><span style="background-color: white; color: #073763;"><img border="0" height="480" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhQCm0iCY_TUhbqNyKVtSsY2MDixSbjNT43o_i8ndOzJkIw1TogBZ7GQNdwCa8zYAo4D54jDX4SS_apMBTvEEolhg8p7XtTfIjaZO6bq4jSEBSZ_rkK993Pjt4Pm-XyqTk6djxM5S6eu9mM/s640/mapa+do+universo+que+vemos+em+positivo.gif" width="640" /></span></a></td></tr>
<tr><td class="tr-caption" style="text-align: center;"><span style="background-color: white; color: #073763;"><span style="font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 14px; text-align: start;">Fonte da Imagem: http://www.atlasoftheuniverse.com/galchart.html</span><span style="font-family: Arial, Helvetica, sans-serif; font-size: xx-small; text-align: start;"> </span><a href="http://www.atlasoftheuniverse.com/me.html" style="font-family: Arial, Helvetica, sans-serif; font-size: medium; text-align: start;">Richard Powell</a><span style="font-family: Arial, Helvetica, sans-serif; font-size: xx-small; text-align: start;">.</span><span style="font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 14px; text-align: start;"><br /></span></span></td></tr>
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<tr><td style="text-align: center;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgA_mbgMRJPJASW6cXU0O1lB_eNWkUUldXU4qhiVl4XNVT2Vl9AgMF19CN4qncrcRlGKm1_Kw7lVtNbD_aYHpXEPuNSXEs48uztumtfFIiZnQwSEY-rItSuK1rOgEA66jW-jMBKqv09b4hn/s1600/800px-Earth's_Location_in_the_Universe_SMALLER_(JPEG).jpg" imageanchor="1" style="margin-left: auto; margin-right: auto;"><span style="background-color: white; color: #073763;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgA_mbgMRJPJASW6cXU0O1lB_eNWkUUldXU4qhiVl4XNVT2Vl9AgMF19CN4qncrcRlGKm1_Kw7lVtNbD_aYHpXEPuNSXEs48uztumtfFIiZnQwSEY-rItSuK1rOgEA66jW-jMBKqv09b4hn/s1600/800px-Earth's_Location_in_the_Universe_SMALLER_(JPEG).jpg" /></span></a></td></tr>
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<a href="http://commons.wikimedia.org/wiki/File:Earth%27s_Location_in_the_Universe_SMALLER_(JPEG).jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">http://commons.wikimedia.org/wiki/File:Earth%27s_Location_in_the_Universe_SMALLER_(JPEG).jpg</span></a></div>
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<span style="font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;"></span><br />
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<span lang="PT" style="line-height: 48px;"><b><span style="background-color: white; color: #073763; font-family: Helvetica Neue, Arial, Helvetica, sans-serif; font-size: large;">Da Terra ao Céu .......................<o:p></o:p></span></b></span></div>
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<b><span style="background-color: white; color: #073763; font-family: Helvetica Neue, Arial, Helvetica, sans-serif; font-size: large;"><span lang="PT" style="line-height: 36px;">.........................................................................................</span><span lang="PT" style="line-height: 36px;"><o:p></o:p></span></span></b></div>
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<span lang="PT" style="line-height: 48px;"><b><span style="background-color: white; color: #073763;"><span style="font-family: Helvetica Neue, Arial, Helvetica, sans-serif; font-size: large;">................................ e ao Infinito ...................</span><span style="font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><o:p></o:p></span></span></b></span><br />
<span lang="PT" style="line-height: 48px;"><b><span style="background-color: white; color: #073763;"><span style="font-family: Helvetica Neue, Arial, Helvetica, sans-serif; font-size: large;"><br /></span></span></b></span>
<span lang="PT" style="line-height: 48px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 14px; line-height: normal; text-align: start;">PÁGINA AINDA EM CONSTRUÇÃO... </span></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 48px;">e certamente assim continuará por um longo tempo... até que as 88 Constelações estejam prontas. Obrigada pela paciência, caro Leitor!</span><br />
<span lang="PT" style="line-height: 48px;"><span style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 14px; line-height: normal; text-align: start;"><br /></span></span></div>
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<span lang="PT" style="line-height: 22px;"><b><span style="background-color: white; color: #073763;">CONSTELAÇÕES, ESTRELAS E OBJETOS CELESTES<o:p></o:p></span></b></span></div>
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<span lang="PT" style="line-height: 22px;"><b><span style="background-color: white; color: #073763;">(sob o ponto de vista do Mundo Ocidental)<o:p></o:p></span></b></span></div>
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<span lang="PT" style="line-height: 22px;"><b><span style="background-color: white; color: #073763;"> SUAS HISTÓRIAS, SEUS MITOS, SEUS SIGNIFICADOS<o:p></o:p></span></b></span></div>
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<span lang="PT" style="line-height: 22px;"><b><span style="background-color: white; color: #073763;">E SUAS SINTETIZADAS DESCRIÇÕES<o:p></o:p></span></b></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763;">Reunião das Informações,<o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763;">suas traduções para a língua portuguesa (quando necessário),<o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763;"> Compilação bem como Comentários Pessoais:<o:p></o:p></span></span></div>
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<div style="font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;">
<div style="text-align: left;">
<i><span lang="PT"><span style="background-color: white; color: #073763;">Janine Milward</span></span></i></div>
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<span style="background-color: white; color: #073763;"><i><span lang="PT"><br /></span></i>
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<ul class="posts" style="border-width: 0px; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 14px; line-height: 16.7999992370605px; list-style: none none; margin: 0px; padding: 0px;">
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-style: none; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/sobre-nosso-passeio-atraves-o-ceu.html" style="background-color: white; color: #274e13; text-decoration: none;">Sobre Nosso Passeio através o Céu Estrelado</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/algumas-referencias-bibliograficas.html" style="background-color: white; color: #274e13; text-decoration: none;">REFERÊNCIAS BIBLIOGRÁFICAS Impressas e Virtuais</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/as-nuvens-de-magalhaes.html" style="background-color: white; color: #274e13; text-decoration: none;">AS NUVENS DE MAGALHÃES</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/andromeda-princesa-acorrentada.html" style="background-color: white; color: #274e13; text-decoration: none;">ANDROMEDA, A PRINCESA ACORRENTADA</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/antlia-pneumatica-maquina-pneumatica.html" style="background-color: white; color: #274e13; text-decoration: none;">ANTLIA PNEUMATICA, A MÁQUINA PNEUMÁTICA</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/apus-ave-do-paraiso.html" style="background-color: white; color: #274e13; text-decoration: none;">APUS, AVE-DO-PARAÍSO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/aquarius-o-aguadeiro.html" style="background-color: white; color: #274e13; text-decoration: none;">AQUARIUS, O AGUADEIRO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/aquila-aguia.html" style="background-color: white; color: #274e13; text-decoration: none;">AQUILA, A ÁGUIA</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/ara-altar.html" style="background-color: white; color: #274e13; text-decoration: none;">ARA, ALTAR</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/auriga-o-cocheiro.html" style="background-color: white; color: #274e13; text-decoration: none;">AURIGA, O COCHEIRO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/bootes-o-boieiro.html" style="background-color: white; color: #274e13; text-decoration: none;">BOOTES, O BOIEIRO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/argo-navis-o-navo-argus.html" style="background-color: white; color: #274e13; text-decoration: none;">ARGO NAVIS, O NAVIO ARGUS</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/cancer-o-caranguejo.html" style="background-color: white; color: #274e13; text-decoration: none;">CANCER, O CARANGUEJO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/canes-venatici-os-caes-de-caca.html" style="background-color: white; color: #274e13; text-decoration: none;">CANES VENATICI, OS CÃES DE CAÇA</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/canis-major-o-cao-maior.html" style="background-color: white; color: #274e13; text-decoration: none;">CANIS MAJOR, O CÃO MAIOR</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/canis-minor-o-cao-menor.html" style="background-color: white; color: #274e13; text-decoration: none;">CANIS MINOR, O CÃO MENOR</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/capricornus-cabra.html" style="background-color: white; color: #274e13; text-decoration: none;">CAPRICORNUS, A CABRA</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/carina-quilha-do-navio.html" style="background-color: white; color: #274e13; text-decoration: none;">CARINA, A QUILHA DO NAVIO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/cassiopeia-mulher-sentada.html" style="background-color: white; color: #274e13; text-decoration: none;">CASSIOPEIA, A MULHER SENTADA</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/centaurus-o-centauro.html" style="background-color: white; color: #274e13; text-decoration: none;">CENTAURUS, O CENTAURO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/cepheus-cefeu-o-rei.html" style="background-color: white; color: #274e13; text-decoration: none;">CEPHEUS, CEFEU, O REI</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; color: #376307; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-indent: -15px;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/cetus-baleia-o-monstro-marinho.html" style="color: #274e13; text-decoration: none;">CETUS, A BALEIA, O MONSTRO MARINHO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-indent: -15px;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/circinus-o-compasso.html"><span style="color: #274e13;">CIRCINUS, O COMPASSO</span></a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-indent: -15px;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/chamaleon-o-camaleao.html" style="color: #274e13; text-decoration: none;">CHAMALEON, O CAMALEÃO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/columba-noe-pomba-de-noe.html" style="background-color: white; color: #274e13; text-decoration: none;">COLUMBA NOE, A POMBA DE NOÉ</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/coma-berenices-cabeleira-de-berenice.html" style="background-color: white; color: #274e13; text-decoration: none;">COMA BERENICES, A CABELEIRA DE BERENICE</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/corona-australis-coroa-austral.html" style="background-color: white; color: #274e13; text-decoration: none;">CORONA AUSTRALIS, A COROA AUSTRAL</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/corona-borealis-coroa-boreal.html" style="background-color: white; color: #274e13; text-decoration: none;">CORONA BOREALIS, A COROA BOREAL</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/corvus-o-corvo.html" style="background-color: white; color: #274e13; text-decoration: none;">CORVUS, O CORVO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/crux-cruz-o-cruzeiro-do-sul.html" style="background-color: white; color: #274e13; text-decoration: none;">CRUX, A CRUZ, O CRUZEIRO DO SUL</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/cygnus-o-cisne.html" style="background-color: white; color: #274e13; text-decoration: none;">CYGNUS, O CISNE</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/delphinus-o-delfim.html" style="background-color: white; color: #274e13; text-decoration: none;">DELPHINUS, O DELFIM</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/dorado-o-peixe-dourado_19.html" style="background-color: white; color: #274e13; text-decoration: none;">DORADO, O PEIXE DOURADO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/equuleus-cavalo-menor.html" style="background-color: white; color: #274e13; text-decoration: none;">EQUULEUS, CAVALO MENOR</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/eridanus-o-rio-eridano_19.html" style="background-color: white; color: #274e13; text-decoration: none;">ERIDANUS, O RIO ERIDANO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/grus-o-grou.html" style="background-color: white; color: #274e13; text-decoration: none;">GRUS, O GROU</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/gemini-os-gemeos.html" style="background-color: white; color: #274e13; text-decoration: none;">GEMINI, OS GÊMEOS</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/hydra-hidra-femea.html" style="background-color: white; color: #274e13; text-decoration: none;">HYDRA, A HIDRA FÊMEA</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/hydrus-hidra-macho.html" style="background-color: white; color: #274e13; text-decoration: none;">HYDRUS, HIDRA MACHO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/indus-o-indio.html" style="background-color: white; color: #274e13; text-decoration: none;">INDUS, O ÍNDIO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/lacerta-o-lagarto.html" style="background-color: white; color: #274e13; text-decoration: none;">LACERTA, O LAGARTO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/leo-o-leao.html" style="background-color: white; color: #274e13; text-decoration: none;">LEO, O LEÃO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/lyra-lira_19.html" style="background-color: white; color: #274e13; text-decoration: none;">LYRA, A LIRA</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/mons-mensa-montanha-da-mesa-mesa.html" style="background-color: white; color: #274e13; text-decoration: none;">MONS MENSA, A MONTANHA DA MESA, A MESA</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/monoceros-o-unicornio.html" style="background-color: white; color: #274e13; text-decoration: none;">MONOCEROS, O UNICÓRNIO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center; text-indent: -15px;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/musca-australis-mosca-do-sul.html" style="color: #274e13; text-decoration: none;">MUSCA AUSTRALIS, A MOSCA DO SUL</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; color: #376307; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-indent: -15px;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/norma-et-regula-o-esquadro-e-regua.html" style="color: #274e13; text-decoration: none;">NORMA ET REGULA, O ESQUADRO E A RÉGUA</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-indent: -15px;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/octans-o-oitante.html"><span style="color: #274e13;">OCTANS, O OITANTE</span></a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/ophiucus-ofiuco.html" style="background-color: white; color: #274e13; text-decoration: none;">OPHIUCUS, OFIÚCO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/orion-o-gigante-cacador.html" style="background-color: white; color: #274e13; line-height: 16.7999992370605px; text-decoration: none;">ORION, O GIGANTE CAÇADOR</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/pavo-o-pavao.html" style="background-color: white; color: #274e13; text-decoration: none;">PAVO, O PAVÃO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/perseus-o-campeao.html" style="background-color: white; color: #274e13; text-decoration: none;">PERSEUS, O CAMPEÃO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/phoenix-fenix.html" style="background-color: white; color: #274e13; text-decoration: none;">PHOENIX, A FÊNIX</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/pisces-os-peixes.html" style="background-color: white; color: #274e13; text-decoration: none;">PISCES, OS PEIXES</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/pisces-australis-o-peixe-austral.html" style="background-color: white; color: #274e13; text-decoration: none;">PISCES AUSTRALIS, O PEIXE AUSTRAL</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/puppis-popa-em-argo-navis-o-navio.html" style="background-color: white; color: #274e13; text-decoration: none;">PUPPIS, A POPA EM ARGO NAVIS, O NAVIO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/sagitta-flecha.html" style="background-color: white; color: #274e13; text-decoration: none;">SAGITTA, A FLECHA</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/sagittarius-o-arqueiro.html" style="background-color: white; color: #274e13; text-decoration: none;">SAGITTARIUS, O ARQUEIRO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/scorpius-o-escorpiao.html" style="background-color: white; color: #274e13; text-decoration: none;">SCORPIUS, O ESCORPIÃO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/serpens-serpente.html" style="background-color: white; color: #274e13; text-decoration: none;">SERPENS, A SERPENTE</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/taurus-o-touro.html" style="background-color: white; color: #274e13; text-decoration: none;">TAURUS, O TOURO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/telescopium-o-telescopio.html" style="background-color: white; color: #274e13; text-decoration: none;">TELESCOPIUM, O TELESCÓPIO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/triangulum-o-triangulo.html" style="background-color: white; color: #274e13; text-decoration: none;">TRIANGULUM, O TRIÂNGULO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-indent: -15px;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/triangulum-australis-o-triangulo-do-sul.html" style="color: #274e13; text-decoration: none;">TRIANGULUM AUSTRALIS, O TRIÂNGULO DO SUL</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/tucana-o-tucano.html" style="background-color: white; color: #274e13; text-decoration: none;">TUCANA, O TUCANO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/vela-em-argo-navis-o-navio_20.html" style="background-color: white; color: #274e13; text-decoration: none;">VELA, EM ARGO NAVIS, O NAVIO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/virgo-virgem.html" style="background-color: white; color: #274e13; text-decoration: none;">VIRGO, A VIRGEM</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/pisces-volans-o-peixe-voador.html" style="background-color: white; color: #274e13; line-height: 16.7999992370605px; text-decoration: none;">VOLANS, O PEIXE VOADOR</a></li>
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<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/scutum-o-escudo.html" style="background-color: white; color: #274e13; text-decoration: none;">SCUTUM, O ESCUDO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/vulpecula-et-anser-raposa-e-o-ganso.html" style="background-color: white; color: #274e13; text-decoration: none;">VULPECULA ET ANSER, A RAPOSA E O GANSO</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/algumas-constelacoes-mais-recentes-e.html" style="background-color: white; color: #274e13; text-decoration: none;">Constelações Atuais</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/constelacoes-apresentadas-partir-do.html" style="background-color: white; color: #274e13; text-decoration: none;">Constelações apresentadas a partir do Ponto Vernal...</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(241, 194, 50); border-bottom-style: solid; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/breve-roteiro-de-viagem-celeste-para-os.html" style="background-color: white; color: #274e13; text-decoration: none;">Breve Roteiro de Viagem Celeste para os tempos do ...</a></li>
<li style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-style: none; border-top-color: rgb(241, 194, 50); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em; text-align: center;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/da-terra-ao-ceu-e-ao-infinito_24.html" style="background-color: white; color: #274e13; text-decoration: none;">MEU AMOR PELAS ESTRELAS...</a></li>
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<span style="background-color: white;"><span lang="PT" style="color: #660000; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px;"><b>MEU AMOR PELAS ESTRELAS...</b></span></span><br />
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<b style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal;"><span style="font-size: large;">The Old Astronomer to His Pupil</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: large;">Though my soul may set in darkness, it will rise in perfect light;<br />I have loved the stars too fondly to be fearful of the night.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> (traduzindo livremente) :</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: large;">Apesar de minha alma permanecer na escuridão, ela ascenderá plenamente iluminada,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: large;">Meu amor pelas estrelas tem sido grande demais para que eu tema a (escuridão da) noite</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: large;">.......ou .. para que eu tema a morte)."</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Este poema é o grande companheiro das noites solitárias dos amantes das estrelas.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Momento de Reverência à Astronomia</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Transcrevo o belíssimo poema de SARAH WILLIAMS</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> que tão bem descreve o amor à Astronomia, o respeito à passagem do conhecimento do mestre para o discípulo, a tristeza do não-reconhecimento dos pares contemporâneos a respeito do trabalho realizado, a emoção de se unir ao mestre reverenciado e às estrelas quando chega o momento da morte... Morte que nunca é temida por todos aqueles que amaram a escuridão da noite e as luzes das estrelas...</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">The Old Astronomer to His Pupil</b></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br />
<i>Sarah Williams</i></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Reach me down my Tycho Brahe, I would know him when we meet,<br />When I share my later science, sitting humbly at his feet;<br />He may know the law of all things, yet be ignorant of how<br />We are working to completion, working on from then to now.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Pray remember that I leave you all my theory complete,<br />Lacking only certain data for your adding, as is meet,<br />And remember men will scorn it, 'tis original and true,<br />And the obliquy of newness may fall bitterly on you.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">But, my pupil, as my pupil you have learned the worth of scorn,<br />You have laughed with me at pity, we have enjoyed to be forlorn,<br />What for us are all distractions of men's fellowship and smiles;<br />What for us the Goddess Pleasure with her meretricious smiles.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">You may tell that German College that their honor comes too late,<br />But they must not waste repentance on the grizzly savant's fate.<br />Though my soul may set in darkness, it will rise in perfect light;<br />I have loved the stars too fondly to be fearful of the night.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">"Reach me down my Tycho Brahe, I would know him when we meet"</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A poeta Sarah Williams nestes versos bem descreveu o sentimento do velho astrônomo em seu leito de morte, deixando seu conhecimento como herança para seu discípulo...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ele pede ao seu discípulo para lhe trazer o retrato pintado de Tycho Brahe, o grande mestre astrônomo anterior a Kepler, a Galileu....para reconhecê-lo quando se encontrarem... E o velho astrônomo tem certeza de que – apesar de Tycho Brahe saber a lei sobre todas as coisas, ainda assim não sabe o que o velho astrônomo já acumulou de conhecimentos, dando continuidade ao trabalho da astronomia desde aquele tempo mais antigo até aquele momento...trabalho esse que, humildemente, o velho astrônomo anseia por compartilhar com o antigo mestre..... Essa é a primeira estrofe.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A segunda estrofe começa com o velho astrônomo deixando como herança ao seu discípulo sua teoria já completa, ao mesmo tempo que fazendo seu herdeiro saber que a esta teoria ele deverá acrescentar mais e mais informações. E o avisa: os homens zombarão dele – apesar de sua teoria se provar original e verdadeira. E sentencia: a ignorância em relação ao novo conhecimento cairá como fel sobre o discípulo.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Na terceira estrofe e nos dois primeiros versos da quarta estrofe, o velho astrônomo devaneia sobre as zombarias e o não-reconhecimento que o discípulo teve oportunidade de vivenciar junto ao seu mestre e sobre o bom-humor e temperança com que ambos tiveram que enfrentar tais vicissitudes...... Também assinala que qualquer honraria agora chegaria tarde demais...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os dois últimos versos da última estrofe são de uma beleza ímpar:</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">"Though my soul may set in darkness, it will rise in perfect light;</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">I have loved the stars too fondly to be fearful of the night."</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Assim, o velho astrônomo termina sua vida dizendo (traduzindo livremente) :</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">"Apesar de minha alma permanecer na escuridão, ela ascenderá plenamente iluminada,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Meu amor pelas estrelas tem sido grande demais para que eu tema a (escuridão da) noite</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">.......ou .. para que eu tema a morte)."</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esse último verso tem sido o grande companheiro de todos aqueles que amam verdadeiramente as estrelas, sejam astrônomos ou não....</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">FONTES:</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The Old Astronomer to his Pupil</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- Poema de Sarah Williams</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">"Best Loved Poems of the American People"</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Hazel Felleman, ed. Garden City Publishing Co.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Garden City, NY. 1936, pp. 613-614</span></div>
<a href="http://www.3ap.org/sarahWilliams.shtml"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.3ap.org/sarahWilliams.shtml</span></a><br />
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<b><span lang="EN-US" style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763;">ATLAS DO UNIVERSO</span></span></b></div>
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<a href="http://www.atlasoftheuniverse.com/index.html"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763;">http://www.atlasoftheuniverse.com/index.html</span></span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763;">This website belongs to <a href="http://www.atlasoftheuniverse.com/me.html" style="text-decoration: none;">Richard Powell</a>.</span></span></div>
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<span style="text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.atlasoftheuniverse.com/galchart.html</span></span></div>
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<span lang="PT" style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">WIKIPEDIA</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US"> </span><span lang="EN-US">- </span><b><span lang="EN"><span lang="EN-US"><a href="http://en.wikipedia.org/wiki/Supercluster" style="text-decoration: none;">http://en.wikipedia.org/wiki/</a></span></span></b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://commons.wikimedia.org/wiki/File:Earth%27s_Location_in_the_Universe_SMALLER_(JPEG).jpg" style="background-color: white;">http://commons.wikimedia.org/wiki/File:Earth%27s_Location_in_the_Universe_SMALLER_(JPEG).jpg</a></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Programa Stellarium</b></span><br />
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-45875414154099931432013-08-21T12:25:00.002-07:002014-04-28T11:28:09.499-07:00Breve Roteiro de Viagem Celeste para os tempos do Outono, Inverno, Primavera e Verão no Sítio das Estrelas Latitude 21s52 e da Longitude 43w00<div class="MsoBodyText2" style="font-size: 14px; line-height: 21px; text-align: center;">
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiu_rLBu81j65Tvoz4Aa9zWPjEJuDYpEiZvw-GJzI1RcIVUChcbnClem9sXL4-aO97RwvNjtSPYW7hfIXrm1yx96IFSaCRlQHvPYTzwAf9UcmbzjLHFYnGXY0NCPY9DznsUwVNHnx6gT58o/s1600/png.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiu_rLBu81j65Tvoz4Aa9zWPjEJuDYpEiZvw-GJzI1RcIVUChcbnClem9sXL4-aO97RwvNjtSPYW7hfIXrm1yx96IFSaCRlQHvPYTzwAf9UcmbzjLHFYnGXY0NCPY9DznsUwVNHnx6gT58o/s640/png.png" height="624" width="640" /></span></a></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Um Passeio pelo Céu Noturno do Sítio das Estrelas</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">OBSERVAÇÃO DE CONSTELAÇÕES E ESTRELAS</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">À VISTA DESARMADA OU ATRAVÉS DE BINÓCULOS</span></b></div>
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<b><i><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></i></b></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">Breve Roteiro de Viagem Celeste</span></b></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">para os tempos do Outono, Inverno, Primavera e Verão</span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">no Sítio das Estrelas</span></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">Latitude 21s52 e da Longitude 43w00</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dois Dedos Iniciais de Prosa sobre o Céu no Sítio das Estrelas</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando eu pensei em me afastar da cidade grande, do Rio de Janeiro, meu desejo era o de morar sob as estrelas, num lugar aonde eu pudesse sempre estar comungando com suas luzes e com suas (quase) eternidades... E logo ao chegar ao pedaço de terra que me apareceu para ser por mim adquirido, o nome <i>Sítio das Estrelas</i> me veio de imediato à mente.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Sítio das Estrelas é um lugar bastante apropriado para se olhar o céu estrelado.<span style="mso-spacerun: yes;"> </span>A bem da verdade, já foi melhor...<span style="mso-spacerun: yes;"> </span>Quando aqui cheguei, em 1998, a provinciana cidadezinha ainda abrigava uma população pequena.<span style="mso-spacerun: yes;"> </span>Com o tempo, a cidade foi crescendo e casas foram sendo construídas para abrigar as novas famílias, os bairros surgiram e a iluminação feérica também!<span style="mso-spacerun: yes;"> </span>Sendo assim, no Sítio das Estrelas, nosso norte não é nada bom pela presença da cidade próxima<span style="mso-spacerun: yes;"> </span>e também nosso noroeste, da mesma forma, porque ali podemos ver a iluminação crescente advinda da cidade de Juiz de Fora, distante a cerca de 60 quilômetros!<span style="mso-spacerun: yes;"> </span>Portanto, norte e noroeste acabam ficando comprometidos com a poluição luminosa... mas, mesmo assim, sempre podemos observar grandes espetáculos. No entanto, nosso leste e nosso sul e o zênite são bem mais interessantes, sem dúvida alguma... por enquanto...<span style="mso-spacerun: yes;"> </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="mso-spacerun: yes;"> </span>Aqui podemos ver a olho nú as duas Nuvens de Magalhães, a Cabeleira de Berenice, A Colmeia de Abelhas (M-44) ou Presépio, a Caixinha de Jóias, A Espada do Órion (M-42).... Também podemos acompanhar alguns serpenteados nos céus: o rio Eridanus começando bem ao sul e terminando aos pés do Gigante e Caçador Órion; a Hydra com sua cabeça triangular começando bem próxima ao Presépio e caminhando delicadamente, delineando, algumas constelações como a Taça, o Corvo, a Virgem, indo se esconder na Balança; a Cabeça da Serpente guardando as maravilhosas estrelas da Corona Borealis; a preciosidade e delicadeza das estrelinhas que compõem a Corona Australis; a Cabeleira de Berenice, quase um enxame de estrelas extremamente tímidas entre o Leão garboso e o Boieiro... Felicidade indescritível também é podermos nadar junto aos dois Peixes em seu mar celeste após termos quase que surfado nas ondas marolantes das estrelinhas tímidas e em ziguezague do Aquário, o Aguadeiro, advindos do Capricórnio que mais parece uma fraldinha de nenê... Infelizmente não dá para ver Andrômeda, a galáxia, a olho nu porque para os lados do norte e noroeste situa-se a cidade de Mar de Hespanha.... e um tantinho mais adiante, ocupando o noroeste e parte do oeste, situa-se a cidade de Juiz de Fora.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Bem, caro Caminhante, para o leitor que entende um pouquinho do céu estrelado, os nomes acima mencionados evocam emoção, estremecimento e felicidade: ver tudo isso a olho nú significa que o céu desse lugar é bem escuro e transparente..... Para o leigo, tudo isso significa o tanto que podemos ainda aprender juntos, realizando um verdadeiro Passeio pelo Céu Noturno do Sítio das Estrelas!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Confesso ao Caminhante que sinto um imenso prazer em morar num lugar onde posso jantar olhando para algum Planeta caindo no oeste... (no carnaval passado, a Caminhante que aqui esteve, levantou seus olhos do prato e se viu ‘pega’ por uma luz intensa, no oeste..., e me perguntou: “que luz é aquela?”<span style="mso-spacerun: yes;"> </span>Eu respondi: “é Júpiter!”); posso acordar sob o albedo de Vênus ou de Júpiter resvalando por sobre minha cama; posso dormir sob a mira dos raios luminosos da Lua Cheia ou de outras Luas mais tímidas; posso, sempre que quero, sair para o gramado para saudar as estrelas, os planetas, me deixar surpreender por um risco cruzando os céus, uma estrela cadente... e fazer um pedido...; posso suspirar ao apontar para Omega Centauri com meus simples binóculos e então, em noites <i>verdadeiramente escuras</i> e transparentes, <i>tentar</i> divisar este belíssimo objeto, com a visão enviesada...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eu diria, caro Caminhante, que me encanta o céu estrelado e é por isso que vim viver no Sítio das Estrelas.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Grande parte de minha vida noturna é dedicada a me deixar ser coberta pelo manto estrelado da nossa Via Láctea... e observar as luzes piscantes das estrelas observadas a olho nú – algumas vezes bem sumidas, fugidias (como aquelas da Cabeleira de Berenice, Aquário, Presépio, Hidra, Rio Eridano, por exemplo); a lâmpada acesa dos Planetas movendo-se para frente e para trás contra o pano de fundo das constelações, o caminho que a Lua, doce e mutável Lua vai traçando noite após noite, dia após dia; os chumaços de algodão que vão percorrendo os céus nos revelando a Galáxia onde vivemos e seu revirão na cauda do Escorpião..., bem como outras galáxias... agrupamentos, nebulosas...; um rasgo de luz de um meteoro cruzando o céu.... - todos marchando através da abóbada celeste, revelando seus segredos e sua beleza!</span></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">O CÉU DO OUTONO</span></b></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">no Sítio das Estrelas</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">OBSERVAÇÃO DE CONSTELAÇÕES E ESTRELAS</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">À VISTA DESARMADA OU ATRAVÉS DE BINÓCULOS</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando o outono chega, aqui na Zona da Mata das Minas Gerais, as chuvas do verão vão escasseando de tal forma até se tornarem apenas uma lembrança... As noites voltam a mostrar suas estrelas em céu sem nuvens e o ar bem mais seco permite que suas luzes fiquem bem mais brilhantes e piscantes contra o pano de fundo da escuridão da abóbada celeste. Por que não aproveitarmos esses tempos de início seca do outono para observarmos o céu noturno, em belo passeio?</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ao começar nosso <i>tour</i> celeste, nestes dias de março, podemos ainda bem observar o adeus dos mares aonde a Baleia Cetus e os Peixes nadam vigorosamente... Também já nos despedimos do grande quadrado do cavalo alado Pégasus colado à constelação de Andrômeda e entre ambos, a luz fugidia e a olho nú bem enviesado da Galáxia com o nome da donzela que se apresenta maravilhosamente a nossos olhos revestidos com um simples par de binóculos e melhor ainda, através das lentes do telescópio.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Vale a pena observarmos um dos dois círculos formados pelas estrelas dos Peixes quase ao centro do grande quadrado formado pela constelação de Pegasus, imensa constelação, realmente.<span style="mso-spacerun: yes;"> </span>É bem neste ponto que encontra-se o Ponto Vernal, o equinócio da primavera.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Olhando em linha quase reta para o sul, poderemos ainda ver a Pequena Nuvem já quase caindo no oeste enquanto a Grande Nuvem de Magalhães ainda a acompanha de longe, permanecendo um pouco mais de tempo nos céus. Aqui na roça, um antigo caseiro meu, as chamava de as Mulas do Presépio! Pobre Fernão de Magalhães que nos perdoe!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando o céu escurece por todo, já também o Carneiro, Áries,<span style="mso-spacerun: yes;"> </span>se coloca em posição de caída no horizonte oeste, levando consigo, mais ao norte, o herói Perseus que caminha juntamente com aquelas que nos chamam a atenção e nos trazem seus suspiros: as Plêiades que sempre me parecem um tercinho, um rosário.... por que não contá-las? Quatro, cinco, seis, sete.... doze....?</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Estamos entrando, então, nos campos aonde o Touro pasta... e encontramos Aldebarã, o Olho do Touro, sua alfa - como é avermelhada, esta gigante.... será que algum dia poderemos vê-la explodindo em supernova? E as Hyades, não parecem uma arvorezinha de natal? Visto do sul, o Touro fica de cabeça para baixo...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Já quase caindo no oeste e bem mais ao sul de Cetus, ainda nos atrai a beleza de Achernar, o começo (ou o fim) do Rio Eridanus. O Eridanus corre sinuoso e tímido através dos céus até se encontrar com Rigel, o pé do Gigante Órion. Esse Rio tão belo pode apenas ser observado em céus escuros e transparentes, longe das luzes urbanas... assim como no Sítio das Estrelas.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Órion é reconhecidamente uma das mais belas constelação do céu estrelado. Seu Cinturão, as chamadas Três Marias (Alnilan, Mintaka e Alnitak), carregam a linha do equador celeste, ou seja, ao vermos o Gigante, podemos distinguir aquilo que pertence mais ao norte e aquilo que pertence mais ao sul.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Nesse momento de preciosa escuridão, por que não divisarmos todos os detalhes da figura do Gigante poderoso dos céus? Adoro ver seu Escudo, desafiadoramente enfrentando o Olho do Touro, Aldebarã. Sua cabeça é simples porém seus ombros trazem duas preciosidades: Belatrix e Betelgeuse. Porém, o melhor de Órion pode ser divisado a olho nú, apreciado através de binóculos e transformando o sonho em realidade através de bons telescópios: M42, seu berço de estrelas, parte da Espada do Gigante Caçador dos céus.<span style="mso-spacerun: yes;"> </span>Rigel é a estrela-beta desta constelação e é a seus pés que o Rio Eridanus começa a acontecer, já tendo sido anunciado anteriormente (pois caminha de volta ao leste) por sua Foz realizada pela estrela-alfa Achernar</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Não podemos nos esquecer que os Cães seguem o Gigante Órion em suas caçadas: O Cão Maior e o Cão Menor. Sírius, a mais bela e mais brilhante do céu, é sem dúvida, sempre esperada com ansiedade. Ainda no Cão Maior, binóculos podem ajudar no achado de chumaços simpáticos de estrelas, algumas que pertencem ao Cão Maior e outras que já fazem parte da Popa do Navio. Procyon, alfa do Cão Menor, vem sempre quase junto a Sírius, porém um tantinho atrás, como se fosse uma dama de companhia e já fazendo parte da côrte dos irmãos gêmeos Castor e Pollux.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela pisca bem ao norte... quem será? É Capela, alfa do Cocheiro! Realmente, esta estrela sempre nos chama a atenção pois que se encontra num lugar do céu do norte pouco habitado por grandes luzes.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Se bem percebermos, Já desde Perseus, passando pelo Cocheiro, caminhando entre o Touro e os pés dos Gêmeos e inundando o Cão Maior com seu brilho esfumaçado, realçando Sírius e navegando o Navio capitaneado por Canopus adentro (o Navio foi desmembrado em Popa, Vela, Carina)... e mergulhando no Cruzeiro do Sul (que volta a nos encantar com sua presença no céu do outono), enfim, marcando sua presença inefavelmente e inegavelmente, eis que vemos a Via Láctea com sua mancha esbranquiçada, algodão divino, leite derramado por tantas e tantas estrelas.... Em céus escuros como aqui no Sítio das Estrelas, bem podemos divisar o Saco de Carvão e outras manchas escuras na via esbranquiçada ao longo do Cruzeiro e redondezas e também enxames de algodão brilhante - como a Caixinha de Jóias, por exemplo.<span style="mso-spacerun: yes;"> </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E, ajudados por um bom par de binóculos, podemos nos deixar<span style="mso-spacerun: yes;"> </span>deslumbrar com a visão de Omega Centauri, um chumaço de estrelas conjugadas e formando um brilhante grande círculo!<span style="mso-spacerun: yes;"> </span>Falando em Centauro, por que não apreciarmos suas estrelas ponteadoras de<span style="mso-spacerun: yes;"> </span>seus pés, Alfa e Beta Centauri - sendo que a primeira nos apresenta o lugar onde se encontra Próxima Centauri, assim nomeada por ser a estrela mais próxima de nós, terráqueos, de nosso sistema solar.<span style="mso-spacerun: yes;"> </span>A bem da verdade, Alfa Centauri - também conhecida como Bungula ou Rigelkent - é um sistema triplo acolhendo a estrela mais perto de nós..</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Também outros belíssimos tesouros podem ser vistos entre o Cão Maior e o Cruzeiro do Sul (muitos deles na Popa do Navio), chumaços de estrelas formando belíssimos aglomerados que podem ser divisados a olho nú em lugares de céu bem escuros e transparentes.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Em abril, o tempo se afirma em sua secura e quando a noite cai, podemos sempre observar os dois Gêmeos celestes, Castor e Pólux caminhando, literalmente pisando sobre a Via Láctea. É bem nos Gêmeos, na altura do ombro de Pólux, que se encontra o ponto do solstício de junho, trazendo o inverno para o sul e o verão para o norte, o ponto aonde a Terra se encontra mais distante em seu <i>tour</i> ao redor do Sol. As estrelinhas de Castor e Pólux podem ser estudadas bem esmiuçadamente porque aparecem bem distintamente em céus da roça escura, sem luz elétrica.<span style="mso-spacerun: yes;"> </span>(Confesso a você, Caminhante dos Céus, que o Sol transitava pelas pernas dos Gêmeos quando eu nasci!).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A ausência de luz elétrica e de poluição da atmosfera nesses tempos de abril e maio e junho, nos deixam entrever a constelação tímida de Câncer, o Caranguejo. Aqui no Sítio das Estrelas certamente podemos ver (e ver bem) M-44, o Presépio, ou a Colmeia de Abelhas, um verdadeiro berço de estrelas-crianças que viajam juntas e formam para nossos olhos uma lua cheia de luzes fugazes.<span style="mso-spacerun: yes;"> </span>É interessantes sabermos que o Caminho da Eclíptica passa pelo Presépio e é sempre uma grande honra podermos observar Planetas - ou mesmo a Lua crescendo ou minguando, sem muita luminosidade, é claro - sendo aconchegados pela grande lua cheia de estrelinhas tímidas que compõem o berço do Presépio!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Junto ao Caranguejo, em direção ao sul, podemos ver a Cabeça da Hydra e seu corpo sinuoso de estrelas pouco cintilantes rastejando pelos céus, enredilhando-se na Taça, no Corvo, na Virgem, finalizando, aparentemente, nas duas estrelas ponteadoras da Balança... Alfard, a alfa e o Coração da Hydra, bate avermelhadamente na noite escura e silenciosa.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Estamos agora nos dirigindo para nosso encontro com o garboso Leão, com suas estrelas alpha e beta, Regulus e Denébola, uma das patas dianteiras e a cauda do vigoroso felino.<span style="mso-spacerun: yes;"> </span>Mais ao norte do Leão, podemos com certeza, nos deliciar com grande parte do corpo da Ursa Maior, constelação norteante que aponta também para a Ursa Menor, que traz em sua cauda, a Estrela Polar (longe de nossos olhos do sul).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Bem ao sul, o Cruzeiro chega mais cedo a cada noite, sendo devidamente anunciado pelas duas estrelas que formam os pés do Centauro. A estrela alpha do Centauro, Rigel Kent, é um conjunto de três estrelas sendo que uma delas é a chamada Próxima Centauro... e por que? Porque é a estrela mais próxima de nós, de nosso Sistema Solar!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Aproveite as noites de maio para melhor observar as estrelas do sul ainda mais ao sul do que o Cruzeiro. A Mosca é perfeitamente divisada assim como o Triângulo Austral. Por que não procurarmos pelo ponto do sul verdadeiro, o pólo sul? Não é difícil de chegarmos ao polo sul quando estamos sob um céu escuro e transparente porque as constelações que o rodeiam, mesmo que compostas de tímidas estrelas, podem ser bem delineadas.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É realmente interessante observarmos o fato de que todo o céu mais ao sul tende a ir se concentrando, concentrando, como se estivesse passando por um funil.... Assim, as constelações e suas estrelas mais ao sul parecem deslizar ao longo da abóbada celeste como se fizessem uma elipse alongada, começando no sudeste, passando pelo zênite voltado para o sul e finalizando no sudoeste.<span style="mso-spacerun: yes;"> </span>Constelações como o Escorpião e o Corvo, por exemplo, apresentam seu rastejar e seu vôo, respectivamente, inteiramente contidos dentro dessa elipse alongada.<span style="mso-spacerun: yes;"> </span>O Navio também parece navegar nos mares celestes realizando esse trajeto, porém de maneira bem mais aproximada ao pólo sul, realmente. Podemos pensar, como num exemplo, o sul como uma vasilha em seu ponto de encontro com a mesa, em sua base, e a abertura da vasilha, seu vazio, como representativo do norte (será que me expliquei bem?)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="mso-spacerun: yes;"> </span>Ah, eu gostaria de poder um dia ir a algum ponto bem ao sul do Planeta para poder observar o Cruzeiro do Sul e o Navio, por exemplo, durante toda a noite, assim como se dançassem uma roda de cantigas celestes!<span style="mso-spacerun: yes;"> </span>Ah, eu gostaria de um dia poder ir a algum ponto bem ao norte do Planeta para poder observar o Navio navegando alhures, distante, e espraiando-se pelo oceano sem fim!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tenho sempre um imenso prazer quando o Corvo começa a fazer seu vôo pelos céus, cruzando o leste mais o sul, fazendo quase uma meia-girada simbolizando um real vôo, até desaparecer no horizonte oeste, ao longo de sua passagem de alguns meses no ano.... Já desde final de março, início de abril, que podemos ver este pássaro nos céus, radioso, voando, voando, deslizando com seu vôo suave pela abóbada dos céus do sul.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">No entanto, não podemos nos esquecer que o Leão também já vem rugindo desde há bastante tempo nos céus... Visto do sul, o Leão está de cabeça para baixo porém sempre nos deixando entrever sua juba, seu pé Régulus, seu corpo iluminado por estrelas simpáticas e finalmente, sua cauda vibrante, Denébola.<span style="mso-spacerun: yes;"> </span>O Caminho da Eclíptica passa por Regulus e então é muito comum que possamos observar esta estrela sendo conjugada com a Lua ou com algum Planeta!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A noite vai andando, maio vai seguindo seu rumo e o céu também vai andando, como num carrossel iluminado.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mais ao norte do Leão, podemos ver o Leão Menor e umas poucas estrelinhas dos pés da Ursa Maior.... Mais ao sul, o chumaço de algodão, o leite derramado das estrelas da Via Láctea, continua invadindo o sul, sempre brilhante, enquanto que ao norte, vai desaparecendo sua luz tímida como um sonho desvanecedor... Noite adentrada, essa Via Láctea e luminosa nos traz o Escorpião, surgindo vagarosamente no leste mais ao sul, trazendo em sua cauda o revirão da Galáxia, o ponto de mutação, onde a cobra morde a cauda....</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Porém, ainda no céu do começo da noite do meses de maio e junho e acompanhando o vôo do Corvo bem de perto, a Virgem chega radiosa com sua alfa, a estrela Spica. O Caminho da Eclíptica passa por Spica e é bem comum podermos observar a Lua ou algum Planeta conjugando-se à esta estrela.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Um dedinho antes da constelação da Virgem, encontra-se o ponto de interseção das linhas da eclíptica e do equador, o equinócio. Virgem traz consigo a Balança, com suas duas estrelas perfazendo os dois pratos: Zubenelgenubi e Zubenelschamalli (que antigamente eram consideradas as Garras do animalzinho rastejante dos céus e, sem dúvida alguma, isso faz o maior sentido).<span style="mso-spacerun: yes;"> </span>O Caminho da Eclíptica passa pelas estrelas ponteadoras da Balança e, da mesma forma, passa bem próxima à Antares, a estrela alfa do Escorpião.<span style="mso-spacerun: yes;"> </span>Depois de passar próxima<span style="mso-spacerun: yes;"> </span>à Antares, o Caminho da Eclíptica adentra a 13<sup>a</sup>. constelação do Zodíaco, Ophiúco, aquele que segura a Serpente que pode ser delineada em sua cauda e também em sua cabeça (esta última terminando aos pés da Coroa Boreal, como se quisesse guardá-la.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Olhando mais ao norte, podemos nos deliciar com a presença de Arcturus, no Boieiro. Em locais de céu escuro – assim como no Sítio das Estrelas -, podemos divisar as tímidas estrelinhas que formam as mechas da Cabeleira de Berenice, constelação quase apagada, entre o Leão e o Boieiro. Ver a olho nú as mechas dos cabelos da bela egípcia é um real privilégio.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Em junho, quando cai a noite, já temos a figura maravilhante do Escorpião toda desenhada entre o algodão doce da Via Láctea... Como já dissemos, o Escorpião é antecedido por suas duas garras, as estrelas alpha e beta da Balança.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A cabeça deste animalzinho rastejante sobre a Via Láctea é realmente incrível, levando até seu coração batendo avermelhadamente, Antares, a rival de Ars, Marte.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É realmente belo o desenho que as estrelas do Escorpião vão nos mostrando... várias estrelas duplas que disputam a acuracidade de nossa visão... (me lembro de meu primeiro namorado me dizendo que éramos tão próximos um do outro quanto aquelas duas estrelas que formam uma das curvas do Escorpião.... palavras ao vento.... não o vejo há mais de 45 anos...). A cauda do Escorpião é realmente assustadora com a presença fulminante de Schaula... finalizando com alguns objetos maravilhosos, M-7, M-8, M-6, chumaços de algodão, bom de olhar a olho nú, melhor ainda de binóculos e telescópio.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Nesta região do céu entre o Escorpião e o Sagitário, naquela direção e além daquela poeira de estrelas, encontra-se o chamado Centro de nossa Galáxia, a Via Láctea. E como tudo no universo realiza um movimento de rotação em torno de si mesmo e em torno de algum outro objeto magnetizador, também nossa Via-Láctea realiza esse movimento.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Não podemos deixar de mencionar a imperdível visão da Coroa Austral sendo enlaçada pelo Sagitário!<span style="mso-spacerun: yes;"> </span>A Coroa Austral é de uma delicadeza ímpar, realmente.<span style="mso-spacerun: yes;"> </span>Se mantivermos quase a mesma direção do céu, estaremos encontrando, bem mais ao norte, a Coroa Boreal, tão bela quanto a outra Coroa e encontrando-se bem situada entre estrelas de primeiríssima grandeza como Arcturus, a alfa do Boieiro, e Vega, a alfa da Lira e próxima ao herói Hercules.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Com o andar da noite e das estrelas, outras constelações vão se aprontando, por assim dizer, para entrarem no palco da vida...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Não será tempo de irmos dormir?! Ah, eu diria para você passar uma noite em claro apenas para observar a girada da Via Láctea enquanto o céu vai caminhando todo de leste para oeste, carregando suas estrelas, planetas, constelações.... A visão do girar da Via Láctea é algo que nos deixa sem palavras....</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Se você tiver a oportunidade de estar num lugar onde o céu seja escuro e transparente, poderá observar a imensa pavimentação de algodão de estrelas - a Via-Láctea - aparentemente centralizando-se no Escorpião e cobrindo o céu estrelado em direção ao norte, passando por Sagitário, pela Águia até alcançar o Cisne..., e em direção ao sul encontrando-se com nosso Cruzeiro do Sul, com o Navio, com o Cão Maior seguido do Gigante Órion e aparentemente concluindo-se no Cocheiro....<span style="mso-spacerun: yes;"> </span>Deste ponto bem ao sul e se você estiver em Latitude bem mais ao norte do Planeta, poderá ainda comungar com a pavimentação de algodão de estrelas fazendo parte do Mito de Andromeda, a donzela acorrentada, enredilhando Perseus, seu herói salvador,<span style="mso-spacerun: yes;"> </span>Cassiopéia, sua malvada madrasta, e seu pai, o Rei Cepheus - todas constelações bem ao norte - e, finalmente a Via Lactea realiza seu<span style="mso-spacerun: yes;"> </span>encontro com o Cisne.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Obviamente que aquilo que vemos e acompanhamos como o Revirão da Via Láctea durante a passagem noturna do Escorpião aliado ao Sagitário é um movimento aparente – pois que, na realidade, esse aparente movimento se dá em função do movimento de rotação da nossa Terra, nosso tão querido Planeta.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Revirão da Via Láctea é um espetáculo imperdível e inesquecível e que nos traz uma realidade da mecânica celeste que vai além à realidade que vemos do caminhar das constelações e suas estrelas, todas advindas do horizonte leste, galgando as alturas dos céus e concluindo seu passear no horizonte oeste - com as constelações e estrelas mais ao sul realizando seu caminhar em elipse do sudeste ao sudoeste e com as constelações e estrelas mais ao norte realizando seu caminhar de maneira mais espraiada, digamos assim.<span style="mso-spacerun: yes;"> </span>A realidade do Revirão da Via Láctea parece varrer os céus, como se essa varrição viesse do sul em direção ao norte ou vice-versa..., como se fosse uma hélice, algo assim, cobrindo todas as direções, ao longo da noite e ao longo do caminhar do Escorpião, fundamentalmente.<span style="mso-spacerun: yes;"> </span>A realidade do Revirão da Via Láctea, quando o percebemos realmente - em lugares de céus escuros e transparentes e que nos apresentem o chumaço de algodão do caminho desta Via iluminada em bom estilo!<span style="mso-spacerun: yes;"> </span>-, nos faz tremer não somente de emoção como também em nosso labirinto interior, é quase como se perdêssemos o chão, ficamos zonzos, tontos, quase caímos, quase perdemos o equilíbrio.<span style="mso-spacerun: yes;"> </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os braços da Via Láctea, centralizados no corpo do Escorpião, vão varrendo o céu vindo do sudeste, caminhando para o leste, passando pelo noroeste, pelo norte, pelo noroeste, pelo oeste... e ainda pelo sudoeste, pelo sul, novamente pelo sudeste, noite após noite.<span style="mso-spacerun: yes;"> </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Não deixe de dar uma olhada no Céu do Inverno, se você estiver desejoso de passar a noite inteira observado as constelações e suas estrelas em marcha céu adentro céu afora... ou se você estiver retornando de um programa noturno e perder o sono... ou se você gostar de acordar bem cedo, já com o canto do galo...</span></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">O CÉU DO INVERNO</span></b></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">No Sítio das Estrelas</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">OBSERVAÇÃO DE CONSTELAÇÕES E ESTRELAS</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">À VISTA DESARMADA OU ATRAVÉS DE BINÓCULOS</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Aqui na Zona da Mata das Minas Gerais, o inverno traz tempo frio, chás, cafés, casacos, gorros, meias, cobertores.... e muita vontade de olhar as estrelas porque ainda o céu está seco (antes das queimadas se aventurarem a maltratar as matas, normalmente a partir do final de julho e cobrindo os meses de agosto e setembro... até que as benditas chuvas retornem, mais para o outubro).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Certamente, é ainda o Escorpião e o ponto que leva à centralidade da Via Láctea que nos chama a atenção....<span style="mso-spacerun: yes;"> </span>Portanto, eu aconselharia você, Caminhante dos Céus, a retornar o ponto anterior onde eu tentei descrever o Revirão da Via Láctea.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Porém, com o contínuo andamento do céu (a cada noite, tudo chega mais cedo 4 minutos), podemos agora ver bem o Sagitário, quando a noite cai. É sempre interessante observarmos o fato de que esta constelação também é denominada de Bule de Chá..., porque se parece mesmo com um!<span style="mso-spacerun: yes;"> </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">No ponto entre o Escorpião e o Sagitário, em lugares de céu escuro como o Sítio das Estrelas e em noites secas e transparentes, podemos ver que a Via Láctea vai recebendo vários buracos imensos de puro negrume.... verdadeiras belezas de luz e vazio para serem fotografadas!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A Via de Chumaço de Algodão, a Via Láctea, encontra a Águia que voa sempre orientada por sua estrela alfa, Altair, e este pássaro acaba sendo avizinhado por constelações pequenas e muitíssimo simpáticas, Sagitta, a Flecha, e o Delfim, por exemplo, que também são enredilhadas pelo caminho leitoso.<span style="mso-spacerun: yes;"> </span>Ainda em direção mais ao norte, a Via Láctea parece, a meus olhos, encontrar o Cisne que traz sua cauda a estrela alfa, Deneb, e ali se esfumaçar mais e mais, rumo norte mais aprofundado e distanciado de meus olhos.<span style="mso-spacerun: yes;"> </span>A Via Láctea estará iluminando os caminhos de constelação bem ao norte, como Cepheus, Cassiopéia, Perseus (e passando próxima à Andromeda e ao Cavalo Pegasus) e novamente retornando aos nossos olhos do sul através o Cocheiro, com sua belíssima estrela-alfa Capella, e então retomando a conversa com os Gêmeos Castor e Pollux, acompanhando o Gigante Òrion conduzindo seus dois Cães e já nos enleando a visão com a bela Sirius acompanhada da tímida Procium... até que o clarão dos raios avermelhados do Sol começam a inundar o horizonte leste....</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A Via Láctea pode bem ser vista até Deneb, aqui no Sítio das Estrelas... Quando a noite cai, o revirão dessa Via parece ter chegado à sua conclusão.... porém ainda podemos acompanhá-lo varrendo a noite, quase com puxando as estrelas que chegam no leste e empurrando as estrelas do meio do céu para caírem no horizonte oeste....<span style="mso-spacerun: yes;"> </span>Os braços da Via Láctea, centralizados no corpo do Escorpião, vão varrendo o céu vindo do sudeste, caminhando para o leste, passando pelo noroeste, pelo norte, pelo noroeste, pelo oeste... e ainda pelo sudoeste, pelo sul, novamente pelo sudeste, noite após noite.<span style="mso-spacerun: yes;"> </span>É um girar intenso, como se fosse um dançarino sufi, girando e girando e girando e nos trazendo o êxtase.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Cruzeiro do Sul aparece bem alto, o mais alto que consegue chegar, acompanhando a caída do Navio no horizonte oeste e trazendo maior brilho às presenças do Escorpião, do Sagitário.... e certamente, da Via Láctea que continua fazendo seu revirão noite a dentro.<span style="mso-spacerun: yes;"> </span>Não se esqueça, Caminhante, de bem observar os Sacos de Carvão e dos conjuntos brilhantes de estrelas juntinhas que vão se formando após o Cruzeiro e indo em direção ao Navio que navega bem mais distanciado, em mares longínquos, buscando por outras paragens e retornando apenas na madrugada anunciadora das estrelas e suas constelações que vão surgir no leste.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Arcturus também continua encantando nossa visão.... e para aqueles que possuem um norte escuro e de horizonte baixo, a Ursa Maior se insinua querendo também trazer consigo o Dragão (desaparecido nesta latitude).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Porém, os céus do norte estão felizes com a presença da Coroa Boreal, que parece um colar que todas as mulheres gostariam de usar! Porém, cautela! Esse valoroso colar é guardado por Hércules que ainda mal se articula em sua figura engraçada surgindo no horizonte leste mais ao norte...<span style="mso-spacerun: yes;"> </span>E também guardado pela cabeça da cobra que o Ofiúco segura.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando agosto entra trazendo suas queimadas e já uma certa poluição tirando a escuridão plena e a transparência cristalina dos céus da roça, com sorte, ainda podemos nos deliciar com as travessuras do desajeitado Hércules, agora mais alto no céu do norte, acompanhado, em lugares de horizonte bem baixo, pelo Dragão que guarda as estrelas que rodeiam o polo norte, longe de nossa visão.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Digo que o Hércules é todo desajeitado porque é assim que o vejo. Lembro-me bem da primeira vez que o delineei, eu até ri, mesmo!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Cada vez mais o Cruzeiro do Sul cai em direção ao horizonte oeste mais ao sul ao mesmo tempo que também o Escorpião vai alcançando o meio do céu seguido do Sagitário, com seu Bule de Chá,<span style="mso-spacerun: yes;"> </span>que dá lugar ao Capricórnio que começa a querer se levantar no horizonte leste, ainda ao sul.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Nesse tempo do inverno já bem andado, eu adoro ver minha estrela preferida, Vega, tocando sua Lyra e surgindo atrás dos morros do leste mais ao norte....<span style="mso-spacerun: yes;"> </span>Sempre que eu me vejo diante da Lyra segurada por Vega,sua alfa, eu me flagro suspirando, inteiramente enleada, como se pudesse escutar o doce som das cordas desta constelação!<span style="mso-spacerun: yes;"> </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A bem da verdade, o céu do inverno nos presenteia com um triângulo de estrelas muito interessantes: Altair, alfa da Águia, Vega, alfa da Lyra, e Deneb, alfa do Cisne.<span style="mso-spacerun: yes;"> </span>São estrelas belíssimas que fazem parte de belíssimas constelações!<span style="mso-spacerun: yes;"> </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Cisne é de uma perfeição incrível em seu vôo, parece estar sempre alçando vôo, abrindo suas asas imensas, buscando as alturas, sempre.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A Águia sempre surge apresentando três estrelas - uma delas, Altair, sua alfa - que caminham sempre juntas e que podem ser vistas após a conclusão de todo o corpo do Capricórnio, com seu aspecto de fraldinha tecida por estrelas suaves que delineiam a figura desta constelação.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É bom também observarmos, ainda entre o Sagitário e seu Bule de Chá e o Capricórnio, um pequeno grupo de estrelas que sugere uma pequena cruz, um tímido diamante, algo assim, verdadeira maravilha para ser visto em lugares de céus bem escuros e transparentes.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eu aconselharia o Caminhante dos Céus aguardar a chegada do Capricórnio e da Águia para então olhar mais ao norte e se encantar com a Lira... e um tantinho mais tarde ainda, suspirar com o Cisne voando amplamente nos céus estrelados.<span style="mso-spacerun: yes;"> </span>E, olhando mais ao sul, observarmos o vôo do Grou balizado por sua estrela-alfa, Al Nair.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A partir de então, podemos olhar para os lados do sul e observarmos a chegada do Peixe Austral com sua estrela-alfa, Fomalhaut.<span style="mso-spacerun: yes;"> </span>Estamos bem já sendo colhidos pelas ondas marolantes e em verdadeiro zigue-zague formadas pelo Aguadeiro, Aquário!<span style="mso-spacerun: yes;"> </span>A meu ver, esta constelação é um dos eventos mais interessantes a ser observado nos céus estrelados e isso somente pode acontecer em lugares de céus realmente escuros e transparentes!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Bem ao sul, podemos observar pássaros voando, Fênix e Tucano.<span style="mso-spacerun: yes;"> </span>No entanto, a estrela que realmente nos chama a atenção é Achernar, a alfa do Rio Erídano, sua Foz, e este Rio vai correndo sinuosamente e através suas tímidas estrelas até encontrar os pés do Gigante Órion, em Rigel, sua estrela-beta, já em terra firme.<span style="mso-spacerun: yes;"> </span>É interessante repararmos o fato de que o Rio Erídano caminha em direção ao leste e neste momento de inverno, podemos acompanhar seu desaguar junto ao Gigante caçador do Escorpião porque a constelação de Órion ainda pode ser vista em todo seu esplendor de estrelas ao final da noite, quando o galo desentrelaça suas asas e começa a cantar anunciando um novo dia que não tarda a chegar!<span style="mso-spacerun: yes;"> </span>(Aqui no Sítio das Estrelas meu simpático galo nos acorda com seu canto por volta das quatro horas da matina!).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Nos céus do norte, é interessante observarmos que as estrelinhas marolantes do Aguadeiro parecem querer se entrelaçar com as estrelas também tímidas dos Peixes.<span style="mso-spacerun: yes;"> </span>Nesse momento estamos diante de um mito realmente encantador que apresenta no céu estrelado do norte todos os componentes de sua estória, começando pelo Cavalo Pegasus em seu grande quadrado sendo seguido por Andromeda, a donzela acorrentada numa ilha por sua madrasta Cassiopéia esposa de Cepheus.<span style="mso-spacerun: yes;"> </span>Andromeda será salva pelo herói Perseus.<span style="mso-spacerun: yes;"> </span>A Via Láctea ilumina com seu leite as constelações do pai, da madrasta e do herói salvador, todas bem ao norte e não muito facilmente identificáveis aqui, no Sítio das Estrelas (porque para estes lados fica a cidadezinha de Mar de Hespanha e sua iluminação pouco generosa com o céu estrelado).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">... ‘Stamos em pleno mar... - como diria o poeta português, Camões.<span style="mso-spacerun: yes;"> </span>Ao sul dos Peixes nos deparamos com a imensidade da constelação de Cetus, a Baleia que quer devorar a bela donzela acorrentada, Andromeda.<span style="mso-spacerun: yes;"> </span>Este é um mar interessante pois que também apresenta a Foz do Rio Erídano e todo seu correr sinuoso, desde o sul até o sudeste, para encontrar os pés do Gigante Órion, já em terra firme.<span style="mso-spacerun: yes;"> </span>No entanto, este mar interessante nos apresenta, bem ao fundo (do ponto de vista de quem está bem ao norte, certamente) a estrela maravihosa e alfa do Navio, seu capitão Canopus!<span style="mso-spacerun: yes;"> </span>Sempre que virmos Canopus podemos ter a certeza de que Sirius chegará logo depois!<span style="mso-spacerun: yes;"> </span>E Sirius faz parte da comitiva do Gigante Órion, com seus Cães Maior e Menor, todos já em terra firme.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Não podemos deixar de divisar os dois círculos formados pelas cabeças dos dois Peixes.<span style="mso-spacerun: yes;"> </span>Um destes circulo encontra-se logo ao norte do grande quadrado do Cavalo Pegasus e é bem ali que podemos encontrar o chamado Ponto Vernal, o lugar onde a Eclíptica encontra-se com o Equador Celeste.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Olhando para o sul, poderemos ver a Pequena Nuvem seguida<span style="mso-spacerun: yes;"> </span>pela Grande Nuvem de Magalhães. Aqui na roça, um antigo caseiro meu, as chamava de as Mulas do Presépio de Jesus! Fernão de Magalhães que nos perdoe!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os mares terminam deixando entrar em cena as duas estrelas ponteadoras de Áries, o Carneiro, e depois, surge o campo onde o Touro pasta, sempre antecedido pelas estrelas que choram, as Pleiades, um tercinho de estrelas, verdadeira maravilha sempre a ser visitada por nossos olhos...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Já estamos na madrugada sonolenta quando entra em cena o Gigante Órion acompanhado do Cão Maior e este embelezando os céus com a presença de Sirius, a bela das belas.<span style="mso-spacerun: yes;"> </span>A Via Láctea já retorna à nossa visão, o Navio vai se mostrando por inteiro, os Gêmeos já se mostram conversantes, como sempre...<span style="mso-spacerun: yes;"> </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Não deixe de dar uma olhada no Céu da Primavera, se você estiver desejoso/a de passar a noite inteira observado as constelações e suas estrelas em marcha céu adentro céu afora... ou se você estiver retornando de um programa noturno e perder o sono... ou se você gostar de acordar bem cedo, já com o canto do galo...</span></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">O CÉU DA PRIMAVERA</span></b></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">No Sítio das Estrelas</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">OBSERVAÇÃO DE CONSTELAÇÕES E ESTRELAS</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">À VISTA DESARMADA OU ATRAVÉS DE BINÓCULOS</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Cruzeiro do Sul já se despede de nossas noites quando chega outubro. E num movimento de seguimento, o Escorpião também desliza em seu caminho rumo ao sudoeste, carregando consigo o Sagitário, a Coroa Boreal, Hércules...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A côrte do céu, no entanto, está formada pelo triângulo do norte, a maravilhosa Vega tocando sua Lyra, a esplendorosa Altair voando a Águia e a não menos formosa, Deneb, a cauda do belo Cisne.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ainda rodeando Altair, encontramos algumas pequeninas constelações que são verdadeiras preciosidades: Sagitta, a Flecha, o Delfim, Equuleus - constelações compostas por tímidas estrelas que podem ser vistas apenas em locais de céus escuros e transparentes.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É bom tempo para estudarmos as estrelas que formam o grande triângulo do Capricórnio e também nos prepararmos para mergulhar dentre as estrelinhas marolantes do Aquário.... já entrevendo a chegada do cavalo alado Pégasus, no horizonte leste mais ao norte.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Também já surge no leste, mais ao sul, o pássaro Grou, uma verdadeira beleza voadora nos céus balizado por sua estrela alfa Al Nair, ao mesmo tempo, que já no mar ao sul do Aquário, podemos ver o Peixe Austral com sua bela estrela Fomalhaut.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Se o tempo ajudar e se a seca comprometida pelas queimadas não estiver maculando nosso céu, por que não continuarmos a estudar os Peixes?<span style="mso-spacerun: yes;"> </span>Por que não nos embevecermos com a visão das Nuvens de Magalhães?</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Com novembro chegam as chuvas... tão ansiadas chuvas - aqui na Zona da Mata das Minas Gerais! Benditas águas que caem dos céus, despencadas, quem sabe, pelas águas do Aquário, do Peixe Austral, e também com o aparecimento dos Peixes que nadam juntos com a Baleia Cetus.... Entre o Aquário e os Peixes, existe o ponto da interseção da eclíptica com o equador celeste, o ponto vernal trazendo o equinócio.<span style="mso-spacerun: yes;"> </span>Este ponto também apresenta-se bem próximo ao grande quadrado de estrelas que formam o Pegasus, o cavalo alado que carrega Perseus em sua intenção de salvar Andromeda, a bela - e é interessante observarmos que também esta Galáxia nossa irmã encontra-se nos arredores do ponto vernal.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O cavalo alado Pégasus já salva a heroína acorrentada, Andrômeda, um tanto que antecedidos, em norte bem baixo, por Cepheus.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Cruzeiro do Sul bem como o Escorpião se despedem do palco dos céus do anoitecer... Porém, Achernar, a foz do Rio Eridanus novamente surge, brilhante e maviosa, no leste do sul bem sul mesmo!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Em dezembro, se as chuvas nos derem alguma trégua, podemos nos deixar maravilhar com a linha sinuosa do caminho que o Rio Eridanus segue... mesmo que ainda não possamos ver o gigante caçador Órion, ao anoitecer, apenas um tanto mais tarde em noite de já quase verão quente.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ao norte, em horizonte bem baixo, Cassiopéia nos deixa ver algumas de suas estrelinhas. Andrômeda e o cavalo alado Pégasus surgem imponentes no meio do céu. Por que não procurarmos por Andromeda, a Galáxia? Mesmo com um simples par de binóculos, esta visão se faz encantadora: é uma emoção imensa, realmente, observarmos nossa querida irmã... porque mais dia menos dia possivelmente nos uniremos a ela de maneira a nos tornamos irmãs siamesas... No horizonte leste, mais ao norte, entra Áries, o Carneiro, ao lado do Triângulo.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A noite vai seguindo seu curso e novamente podemos nos deixar encantar pela via leitosa, a Via Láctea, fazendo parte dos céus do norte, vindo de Perseus e ladeando as Pleiades (que bom, assim essa preciosidade da constelação do Touro não fica comprometida pelo chumaço de algodão) bem como a cabeça do Touro sempre nos mostrando seu Olho Iluminado, Aldebarã.<span style="mso-spacerun: yes;"> </span>A Via Láctea abençoa o Cocheiro e sua<span style="mso-spacerun: yes;"> </span>bela estrela-alfa, Capella, e então segue rumando mais ao sul, encostando no Gigante Órion, sempre garboso e pronto para caçar o Escorpião (que mora do outro lado do céu exatamente para não ser caçado!)<span style="mso-spacerun: yes;"> </span>e enchendo de luz esfumaçada, esbranquiçada, o Cão Maior que nos brinda com a majestosa presença da mais bela da noite, Sirius, a mais brilhante dos céus e também tão próxima a nós (somente 8 anos-luz de distância).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O mito da donzela acorrentada, Andromeda, começa a desaparecer de nossas vistas, com o horizonte oeste engolindo Cepheu, o Cavalo Alado Pegasus, Andromeda, a Baleia Cetus, Cassiopéia... e, com a entrada em cena de Áries e do Touro, também Perseus começa a se despedir de nós.<span style="mso-spacerun: yes;"> </span>Aquário e Peixes também saem do palco estelar.<span style="mso-spacerun: yes;"> </span>O belo Triangulo formado pelos três pássaros, Águia, Cisne e Vultur (outra denominação para a Lira), também podem ser vistos apenas no começo das noites de dezembro, caindo no horizonte oeste logo depois.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ao longo da noite, Achernar começa a carregar o sinuoso Rio Erídano consigo, caindo no horizonte oeste, enquanto Canopus vai capitaneando o Navio que vai surgindo cada vez mais belo, mais imponente, silenciosamente singrando as águas celestes.<span style="mso-spacerun: yes;"> </span>Também o Navio acaba sendo encontrado pela Via Láctea que busca encantar nossa visão acendendo o Cruzeiro do Sul, o Centauro, todos ao sul...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Caminho da Eclíptica já nos deixou ver os Gêmeos conversadores, o Presépio no Caranguejo sendo guardado pela cabeça da Hydra e emocionado por seu coração laranja, Alfard, e esta cobra da água já se mostrou rastejando através a Taça e o Corvo, saudando o Leão, a Virgem, e encontrando a Balança.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Não deixe de dar uma olhada no Céu do Verão, se você estiver desejoso/a de passar a noite inteira observado as constelações e suas estrelas em marcha céu adentro céu afora... ou se você estiver retornando de um programa noturno e perder o sono... ou se você gostar de acordar bem cedo, já com o canto do galo...</span></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">O CÉU DO VERÃO</span></b></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">No Sítio das Estrelas</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">OBSERVAÇÃO DE CONSTELAÇÕES E ESTRELAS</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">À VISTA DESARMADA OU ATRAVÉS DE BINÓCULOS</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Em janeiro, se as chuvas nos derem uma trégua – pelo menos durante o anoitecer... aqui na Zona da Mata das Minas Gerais – podemos nos deitar no deck em frente ao grande lago do Sítio das Estrelas e nos deixar levar pelas estrelas e suas histórias celestes....</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Todo o mito de Andrômeda salva por Perseus cavalgando seu cavalo alado Pégasus está no céu, na ilha do céu, onde a donzela foi acorrentada por sua madrasta Cassiopéia que não pode ser vista adequadamente nesta latitude... Nesse mar, estão o Aguadeiro (Aquário), o Peixe Austral, os Peixes juntamente com Cetus, a Baleia... ao mesmo tempo que voam nos céus celestes os pássaros Grou e Fênix, mais ao norte. Com a entrada do Carneiro, Áries, parece que pisamos em terra e no entanto, já nos deparamos com um rio, o Eridanus, que agora, em janeiro, já nos leva a ver o gigante caçador Órion, em cujas pernas suas águas começam, em terra firme...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sempre que vemos o Órion surgindo ao anoitecer, também estaremos revendo as Plêiades, irmãs chorosas, o Touro com seu belo olho avermelhado, Aldebarã, as Hyades.... ao norte, novamente Capela nos chama a atenção, como se fosse um farol!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sem dúvida alguma, essa parte dos céus estrelados nos deixa absolutamente enleados, quase que sem respiração... porque a Via Láctea nos abençoa com sua presença esfumaçada e escondendo vários pontos interessantes a serem observados através nossos binóculos.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sírius, a rainha da noite, também nos encanta a visão nesse já quase final de verão, fevereiro de nossos carnavais... Procyon segue Sírius, como sempre, e ambas estrelas seguem o caçador gigante Órion... Canopus volta a capitanear seu imenso Navio (desmembrado em Popa, Vela e Carina - não sei por qual razão....) E eis que ao leste, bem ao sul, bem ao sul... retorna o Cruzeiro aos nossos céus da noite!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mais ao norte,<span style="mso-spacerun: yes;"> </span>podemos ver os dois Gêmeos conversando animadamente a caminho do meio do céu. Câncer continua protegendo em seu ventre seu ninho de estrelinhas-crianças, o Presépio. A Hydra também re-aparece em sua cabeça triangular, mostrando depois seu coração, Alphard.... e com o andar da noite e dos meses, todo o seu corpo serpenteando várias constelações...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Leão surge garboso como sempre com suas estrelas Regulus e Denebola - a primeira na pata e a segunda, na cauda -, dando lugar à Virgem que surge antecipada pelo vôo do Corvo.<span style="mso-spacerun: yes;"> </span>Sempre a Virgem nos faz voltar nossa visão para a encantadora Spica, sua estrela-alfa.<span style="mso-spacerun: yes;"> </span>E sempre também a Virgem nos faz voltar nosso desejo de observarmos a luz amarelada e intensíssima advinda de Arcturus, a estrela-alfa do Boeiro.<span style="mso-spacerun: yes;"> </span>Não podemos nos esquecer que entre o Leão e o Boieiro existe a Cabeleira de Berenice, um presente dos céus escuros e transparentes, realmente.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Se olharmos para os céus do norte, poderemos divisar o Leão Menor, os Cães de Caça, e com muita sorte, as patas da Ursa Maior.<span style="mso-spacerun: yes;"> </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Se olharmos para os céus do sul, estaremos suspirando mais e mais com a visão encantadora, cativante, maravilhante, da Via Láctea realizando seu caminho através o Navio, a Cruz, o Centauro e preenchendo todos os espaços que unem estas duas últimas constelações ao Escorpião que entra em cena trazendo nossos olhares mais e mais ao sul, sendo antecedido por suas duas Garras, ou seja, a constelação da Balança.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sempre que o Cruzeiro do Sul aponta para seu momento máximo de zênite possível para uma constelação muitíssimo ao sul e muito próxima ao pólo sul..., entra em cena a majestosa constelação do Escorpião!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Entrando no palco celeste o Escorpião, é tempo de nos deixarmos maravilhar com a Via Láctea encontrando seu ponto máximo de concentração, digamos assim, pois aos pés desse rastejante animal celeste encontra-se o ponto para onde podemos dirigir nossos pensamentos para encontrarem o centro de nossa Galáxia!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Para enfeitarmos e saudarmos esse evento, sempre podemos nos brindar com a doce visão da Coroa Austral, já bem próxima a Sagitário, e da Coroa Boreal, entre o Boieiro e Hercules e guardado pela cabeça da serpente que o Ofiuco segura.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Se o Caminhante estiver num lugar de norte bem baixo, realmente, poderá tentar observar algumas estrelas que compõem o Dragão que guarda o norte dos céus estrelados, o pólo norte.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando o galo estiver cantando, ainda antes do Sol surgir no horizonte leste anunciado por clarões avermelhados..., com sorte poderemos novamente nos fazer felizes como a entrada em cena do Capricórnio apontando para o norte que acolhe a estrela Vega, a alfa da doce e bela e sutil Lyra, e nos trazendo a esperança da chegada próxima da Águia, também acolhida pela Via Láctea, e sempre nos mostrando suas três estrelas que voam juntas!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Não deixe de dar uma olhada no Céu do Outono, se você estiver desejoso/a de passar a noite inteira observado as constelações e suas estrelas em marcha céu adentro céu afora... ou se você estiver retornando de um programa noturno e perder o sono... ou se você gostar de acordar bem cedo, já com o canto do galo...</span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Março marca o final do verão e o início do outono...</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando o outono chega, aqui na Zona da Mata das Minas Gerais, as chuvas do verão vão escasseando de tal forma até se tornarem apenas uma lembrança... As noites voltam a mostrar suas estrelas em céu sem nuvens e o ar bem mais seco permite que suas luzes fiquem bem mais brilhantes e piscantes contra o pano de fundo da escuridão da abóbada celeste. Por que não aproveitarmos esses tempos de início seca do outono para observarmos o céu noturno, em belo passeio?</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ao começar nosso <i>tour</i> celeste, nestes dias de final de março.......................................................................................................................................................................................................................................................... (você pode retornar ao começo de nosso texto.... porém, já certamente sabedor de alguns dos tesouros dos céus estrelados!)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-63398903522054603542013-08-21T12:20:00.004-07:002014-04-27T13:17:58.076-07:00Constelações apresentadas a partir do Ponto Vernal<div class="MsoNormal">
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<b><span lang="PT" style="font-family: 'Monotype Corsiva'; font-size: 18pt; line-height: 150%;"><span style="background-color: white; color: #073763;">Da Terra ao Céu<o:p></o:p></span></span></b></div>
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<b><span lang="PT" style="font-family: 'Monotype Corsiva'; font-size: 18pt; line-height: 150%;"><span style="background-color: white; color: #073763;">e ao Infinito <o:p></o:p></span></span></b></div>
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<b><span lang="PT" style="font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">CONSTELAÇÕES, ESTRELAS E OBJETOS CELESTES<o:p></o:p></span></span></b></div>
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<b><span lang="PT" style="font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">(sob o ponto de vista do Mundo Ocidental)<o:p></o:p></span></span></b></div>
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<b><span lang="PT" style="font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">SUAS HISTÓRIAS, SEUS MITOS, SEUS SIGNIFICADOS<o:p></o:p></span></span></b></div>
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<b><span lang="PT" style="font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">E SUAS SINTETIZADAS DESCRIÇÕES<o:p></o:p></span></span></b></div>
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<b><span lang="PT" style="font-size: 11pt;"><span style="background-color: white; color: #073763;">Reunião das Informações, <o:p></o:p></span></span></b></div>
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<b><span lang="PT" style="font-size: 11pt;"><span style="background-color: white; color: #073763;">suas traduções para a língua portuguesa (quando necessário) <o:p></o:p></span></span></b></div>
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<b><span lang="PT" style="font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">e Compilação: <o:p></o:p></span></span></b></div>
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<b><i><span lang="PT" style="font-size: 11pt;"><span style="background-color: white; color: #073763;">Janine Milward<o:p></o:p></span></span></i></b></div>
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<span lang="PT" style="font-size: 11pt;"><span style="background-color: white; color: #073763;"><b>Esse passeio através o
céu estrelado estará começando a partir das constelações que
circundam o Ponto Vernal, o ponto de interseção entre o Equador e a Eclíptica
apontando para o equinócio da primavera.</b><o:p></o:p></span></span></div>
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<span lang="PT" style="font-size: 11pt;"><span style="background-color: white; color: #073763;">Se acaso você tiver em mãos um mapa celeste, certamente irá bem
acompanhar o andamento da descrição das constelações e das estrelas, vagueando
de norte a sul, rodeando os céus estrelados, encantando-se, maravilhando-se,
aprendendo e apreendendo sobre a magia que existe nos desenhos das constelações
e nas luzes de suas estrelas... E
deixando sua alma, sua mente e seu coração voarem mais e mais longe, infinitamente
distante, seja através sua visão a olho nú, direta ou enviesada, seja através
um bom par de binóculos, através um simpático telescópio, através imensos
telescópios ou mesmo através instrumentos que nos revelam a infinitude de um
universo que ainda vem sendo descoberto, não mais coberto, desvelado, não mais
velado.<o:p></o:p></span></span></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Dados referentes à época 1980, coletados no Atlas Celeste de
R.R.de Freitas Mourão, 6<sup>a</sup>. edição.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: 'Comic Sans MS';">Visitando os
Sites abaixo,</span><span style="font-family: 'Comic Sans MS';"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: 'Comic Sans MS';"> você
conseguirá informações atualizadas e preciosas</span><span style="font-family: 'Comic Sans MS';"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: 'Comic Sans MS';">sobre os
Objetos Celestiais de seu interesse:</span><span style="font-family: 'Comic Sans MS';"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><b><span style="background-position: initial initial; background-repeat: initial initial; font-family: 'Comic Sans MS';">NASA/IPAC</span></b><b><span style="background-position: initial initial; background-repeat: initial initial; font-family: 'Comic Sans MS';"> EXTRAGALACTIC DATABASE –</span></b><span style="font-family: 'Comic Sans MS';"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://ned.ipac.caltech.edu/"><span style="background-position: initial initial; background-repeat: initial initial; font-family: 'Comic Sans MS';">http://ned.ipac.caltech.edu/</span></a><span style="background-position: initial initial; background-repeat: initial initial; font-family: 'Comic Sans MS';"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://ned.ipac.caltech.edu/forms/byname.html"><span style="background-position: initial initial; background-repeat: initial initial; font-family: 'Comic Sans MS';">http://ned.ipac.caltech.edu/forms/byname.html</span></a><span style="background-position: initial initial; background-repeat: initial initial; font-family: 'Comic Sans MS';"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><em><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: 'Comic Sans MS';">NASA/IPAC Extragalactic Database
(NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: 'Comic Sans MS';"> </span></i></span><em><span lang="EN-US" style="font-family: 'Comic Sans MS';"> operated by the Jet Propulsion Laboratory,
California Institute of Technology, under contract with the National
Aeronautics and Space Administration.</span></em><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: 'Comic Sans MS';"><o:p></o:p></span></b></span></div>
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<b><span lang="EN-US" style="font-family: 'Comic Sans MS';"><span style="background-color: white; color: #073763;">THE NIGHT SKY
ATLAS<o:p></o:p></span></span></b></div>
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<span style="color: #073763;"><b style="background-color: white;"><a href="http://www.nightskyatlas.com/index.jsp"><span lang="EN-US" style="font-family: 'Comic Sans MS';">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: 'Comic Sans MS';"><o:p></o:p></span></b></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span lang="EN-US" style="font-family: 'Comic Sans MS';"><span style="background-color: white; color: #073763;">The night sky atlas creates images
of any part of the night sky, allowing easy location of any object. Detailed
chart images show all stars visible to the naked eye, the constellations,
Messier objects, and names of the brightest stars.<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763;"><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: 'Comic Sans MS';">The</span></b><span class="apple-converted-space"><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: 'Comic Sans MS';"> </span></b></span><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: 'Comic Sans MS';">Internet STELLAR
DATABASE</span></b><span lang="EN-US" style="font-family: 'Comic Sans MS';"><o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763;"><a href="http://www.stellar-database.com/"><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: 'Comic Sans MS';">http://www.stellar-database.com/</span></a><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: 'Comic Sans MS';"><o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span lang="EN-US" style="font-family: 'Comic Sans MS';"><span style="background-color: white; color: #073763;">- stars within 75
light-years. (Plus some of the more well-known "name brand"
stars farther away.)<b><o:p></o:p></b></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span lang="EN-US" style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">DORADO, O PEIXE DOURADO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 3h52m / 6h36m
Declinação -48<sup>o</sup>.8 / -70<sup>o</sup>.1<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div class="MsoNormal">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div class="MsoNormal">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Frederici Honores, Honras de Frederico<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Uma constelação obsoleta formada por Bode em 1787, em honra a
Frederick II, da Prússia, através as estrelas pertencentes a Cepheus,
Andromeda, Cassiopeia e Cisne.<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">FORNAX CHEMICA, O FORNO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 1h44m / 3h48m
Declinação -24<sup>o</sup>.0 / 39<sup>o</sup>.8<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">ANDROMEDA, A PRINCESA ACORRENTADA<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">Ascensão Reta 22h56m / 2h36m Declinação +21<sup>o</sup> 4’ a +52<sup>o</sup>
9’<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Nubecula Minor, a Nuvem Pequena, a Pequena Nuvem de Magalhães <o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">História:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Provavelmente adicionada por Bayer, 1604.<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div class="MsoNormal">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div class="MsoNormal">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div class="MsoNormal">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">ARIES, O CARNEIRO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 1h44m / 3h27m
- Declinação +10<sup>o</sup> 2’ /
+30<sup>o</sup> 9’<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">CASSIOPEIA, A MULHER SENTADA<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">Ascensão Reta 22h56m / 3h36m Declinação
+46<sup>o</sup>.4 / +77<sup>o</sup>.5<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span lang="PT" style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">TRIANGULUM, O TRIÂNGULO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">Ascensão Reta 1h29m / 2h48m Declinação +25<sup>o</sup>.4 / +37<sup>o</sup>.0<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Triangulum Minor, o Triângulo Menor<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">História:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Constelação formada por Hevelius, em 1690.<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">PERSEUS, O CAMPEÃO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 1h26m / 4h46m
Declinação +30<sup>o</sup>.9 / +58<sup>o</sup>.9<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div class="MsoNormal">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div class="MsoNormal">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">CAELUM, O BURIL<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 4h18m / 5h3m
- Declinação -27<sup>o</sup> 1’ /
-48<sup>o</sup> 8’<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Musca Borealis, a Mosca do Norte<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">História:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Constelação adicionada por Bartschius, 1624.<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Psalterium Georgianum, a Harpa de George<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">História:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Formada pelo Abade Hell em 1781 em honra a George II da
Inglaterra - porém obsoleta nos dias de hoje.<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">TAURUS, O TOURO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 3h20m / 5h58m
Declinação +0<sup>o</sup>.1 / +30<sup>o</sup>.9<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Custos Messium, o Guardião da Colheita.<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">História:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Constelação formada por La Lande em 1775 sob o nome de Le
Messieur, O Senhor, mas não é mais reconhecida.<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Tarandus, a Rena<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">História:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Constelação formada por Monnier, em 1776.<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Sceptrum Brandenburgicum, o Cetro<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">História:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Constelação adicionada por Gottfried Kirch, 1688.<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">EQUULEUS PICTORIS, O PINTOR<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 4h32m /
6h51m Declinação -43<sup>o</sup>.1 / -64<sup>o</sup>.1<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763;"><br /></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">CAMELOPARDALIS, A GIRAFA<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 3h11m / 14h25m
Declinação +52<sup>O</sup>.8 / +85<sup>o</sup>.1<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span lang="PT" style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Nubecula Major, a Grande Nuvem<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">História:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Provavelmente adicionada por Bayer, 1604.<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">LEPUS, O COELHO, A LEBRE<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 4h54m / 6h9m
Declinação -11<sup>o</sup>.0 / +27<sup>o</sup>.1<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">COLUMBA NOE, A POMBA DE NOÉ<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 5h3m / 6h28
Declinação -27<sup>o</sup>.2 / -43<sup>o</sup>.0<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">ORION, O GIGANTE CAÇADOR<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 4h41m /
6h23m Declinação -11<sup>o</sup>.0 /
+23<sup>o</sup>.0<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">AURIGA, O COCHEIRO <o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 4h25m /
7h27m - Declinação +27<sup>o</sup> 9’ / +56<sup>o</sup>
1’ <o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">URSA MINOR, A URSA MENOR<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">Ascensão Reta 0h0m / 24h0m Declinação +65<sup>o</sup>.6 / +90<sup>o</sup>.0<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">MONOCEROS, O UNICÓRNIO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 5h54m / 8h8m
Declinação -11<sup>o</sup>.0 / +11<sup>o</sup>.9<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">LYNX, O LINCE<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 6h13m / 9h40m
Declinação +33<sup>o</sup>.4 / +62<sup>o</sup>.0<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">CANIS MAJOR, O CÃO MAIOR<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 6h9m / 7h26m
Declinação -11<sup>o</sup>.o / -33<sup>o</sup>.2<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span lang="PT" style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">GEMINI, OS GÊMEOS <o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 5h57m /
8h6m Declinação +10<sup>o</sup>.0 /
+35<sup>o</sup>.4<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div class="MsoNormal">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Telescopium Herschell, o Telescópio de Herschell<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">História:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Constelação formada pelo Abade Hell em 1781, em honra a Sir
William Herschell (o descobridor de Urano).<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">URSA MAJOR, A URSA MAIOR<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">Ascensão Reta
8h5m / 14h27m Declinação +28<sup>o</sup>.8
/ +73<sup>o</sup>.3<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">ARGO NAVIS, O NAVIO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763;"><br /></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Esta constelação, o Navio, fazia parte do grupo de 48
constelações relacionado por Ptolomeu.
Porém, La Caille dividiu o Navio em<b><o:p></o:p></b></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Carina, Vela e Puppis: Quilha, Vela e Popa<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763;"><br /></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">CARINA, QUILHA<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 200h4m / 21h57m Declinação -8<sup>o</sup>.7 / - 27<sup>o</sup>.8<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">VELA<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"> Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 8h2m /
11h24m Declinação -37<sup>o</sup>.0 /
-57<sup>o</sup>.0<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">PUPPIS, POPA<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763;"><b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"> </span></b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 6h2m / 8h26m
Declinação -11<sup>o</sup>.0 / -50<sup>o</sup>.8<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">CANIS MINOR, O CÃO MENOR <o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 7h4m / 8h9m
Declinação -o’0<sup>o</sup>.1 / +13<sup>o</sup>.2<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Officina Typographica<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Constelação formada por Bode em 1800, porém obsoleta nos dias de
hoje.<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">CANCER, O CARANGUEJO <o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 7h53m / 9h19m
Declinação +6<sup>o</sup>.8 / +33<sup>o</sup>.3<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">HYDRA, A HIDRA FÊMEA<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 8h8m /
14h58m Declinação +6<sup>o</sup>.8 /
-35<sup>o</sup>.3<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span lang="PT" style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span lang="PT" style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">LEO MINOR, O LEÃO MENOR<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">Ascensão Reta 9h19m / 11h4m Declinação +22<sup>o</sup>.1 / +41<sup>o</sup>.7<o:p></o:p></span></span></div>
<div class="MsoNormal">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div class="MsoNormal">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div class="MsoNormal">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div class="MsoNormal">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">LEO, O LEÃO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 9h18m /
11h56m Declinação -6<sup>o</sup>.4 /
+33<sup>o</sup>.3<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">SEXTANS URANIAE, O SEXTANTE<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 9h39m / 10h49
Declinação -6<sup>o</sup>.6 / -11<sup>o</sup>.3<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Felix, o Gato<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Constelação formada por La Lande em 1805, porém obsoleta, hoje
em dia.<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">ANTLIA PNEUMATICA, A MÁQUINA PNEUMÁTICA <o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 9h23m / 11h3m
Declinação - 24<sup>o</sup> 3’ a
- 40<sup>o</sup> 1’<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">LIBRA, A BALANÇA<o:p></o:p></span></span></b></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 14h18m /
15h59m Declinação -0<sup>o</sup>.3 /
-29<sup>o</sup>.9<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white; color: #073763;"><b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;">CANES VENATICI, OS CÃES DE CAÇA</span></b><b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"> <o:p></o:p></span></b></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">Ascensão Reta 12h4m / 14h5m Declinação +28<sup>o</sup>.o / +52<sup>o</sup>.7<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">CRATER, A TAÇA<o:p></o:p></span></span></b></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 10h48m /
11h54m Declinação -6<sup>o</sup>.5 /
-24<sup>o</sup>.9<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">COMA BERENICES, A CABELEIRA DE BERENICE<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 11h57 / 13h33m
Declinação +13<sup>o</sup>.8 / +33<sup>o</sup>.7<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS';"><span style="background-color: white; color: #073763;">VIRGO, A VIRGEM<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS';"><span style="background-color: white; color: #073763;">Posicionamento:<b><o:p></o:p></b></span></span></div>
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<span style="font-family: 'Comic Sans MS';"><span style="background-color: white; color: #073763;">Ascensão Reta 11h35m / 15h8m Declinação +16<sup>o</sup>.6 / -22<sup>o</sup>.2<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">PISCES VOLANS, OS PEIXES VOADORES<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">Ascensão Reta
6h36m / 9h2m Declinação -64<sup>o</sup>.2
/ -75<sup>o</sup>.0<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">SCORPIUS, O ESCORPIÃO<o:p></o:p></span></span></b></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 15h44m / 17h55m
Declinação -8<sup>o</sup>.1 / -45<sup>o</sup>.6<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Robur Carolinum, o Carvalho de Charles<o:p></o:p></span></span></b></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">História:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Constelação formada por Halley, 1679, em comemoração ao carvalho<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">onde Charles II escondeu-se.<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">BOOTES, O BOIEIRO <o:p></o:p></span></span></b></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 13h33m / 15h47m
- Declinação +7<sup>o</sup> 6’ /
+55<sup>o</sup> 2’<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763;"><b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;">Quadrans Muralis, o Quadrante</span></b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">História:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Constelação formada por La Lande em 1795 porém obsoleta nos dias
de hoje.<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">CENTAURUS, O CENTAURO <o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 11h3m / 14h59m
Declinação -29<sup>o</sup>.9 / -64<sup>o</sup>.5<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">CORVUS, O CORVO<o:p></o:p></span></span></b></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 11h54m / 12h54m Declinação -11<sup>o</sup>.3 / -24<sup>o</sup>.9<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Mons Maenalus, o Monte Maenalus<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"> 10 Norte a 18 Norte<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Constelação formada por Hevelius, 1690.<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div class="MsoNormal">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">HERCULES, O HOMEM AJOELHADO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 15h47m / 18h56m Declinação +3<sup>o</sup>.9 / +51<sup>o</sup>.3<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">CRUX, A CRUZ, O CRUZEIRO DO SUL<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 11h53m /
12h55m Declinação -55<sup>o</sup>.5 /
-64<sup>o</sup>.5<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">CORONA BOREALIS, A COROA BOREAL<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 15h14m /
16h22m Declinação +25<sup>o</sup>.8 /
+39<sup>o</sup>.8<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Noctua, a Coruja<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Uma constelação obsoleta que ocupava a parte final da cauda da
Hydra.<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">MUSCA AUSTRALIS, A MOSCA DO SUL<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 11h17m / 13h46m Declinação -64<sup>o</sup>.5 / -75<sup>o</sup>.2<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">CHAMALEON, O CAMALEÃO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 7h32m /
13h48m Declinação -75<sup>o</sup>.2 /
-82<sup>o</sup>.8 <o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Constelação adicionada por Bayer, em 1604.<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">SERPENS, A SERPENTE <o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Serpens Cauda et Serpens Caput - a Cauda e a Cabeça da Serpente<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 15h8m /
18h56m Declinação +25<sup>o</sup>.7 /
-16<sup>o</sup>.0<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div class="MsoNormal">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">LUPUS, O LÔBO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 14h13m / 16h5m
Declinação -29<sup>o</sup>.8 / -55<sup>o</sup>.3<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">OPHIUCUS, OFIÚCO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">ou Serpentarius, aquele que Segura a Serpente<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 15h58m / 18h42m Declinação +14<sup>o</sup>.3 / -30<sup>o</sup>.1<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">SERPENS, A SERPENTE <o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Serpens Cauda et Serpens Caput - a Cauda e a Cabeça da Serpente<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 15h8m /
18h56m Declinação +25<sup>o</sup>.7 /
-16<sup>o</sup>.0<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">CIRCINUS, O COMPASSO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 13h35m /
15h26m Declinação -54<sup>o</sup>.3 / -70<sup>o</sup>.4<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">APUS, AVE-DO-PARAÍSO <o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 13h45m / 18h17m
- Declinação - 67<sup>o</sup> 5’
a - 82<sup>o</sup> 9’<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">NORMA ET REGULA, O ESQUADRO E A RÉGUA<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 15h25m / 16h31m Declinação -42<sup>o</sup>.2 / -60<sup>o</sup>.2<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">TRIANGULUM AUSTRALIS, O TRIÂNGULO DO SUL<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 14h50m / 17h9m
Declinação -60<sup>o</sup>.3 / -70<sup>o</sup>.3<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">OCTANS, O OITANTE<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 0h0m / 24h0m
Declinação -74<sup>o</sup>.7 / -90<sup>o</sup>.0<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">MONS MENSA, A MONTANHA DA MESA, A MESA<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 3h20m /
7h37m Declinação -69<sup>o</sup>.9 /
85<sup>o</sup>.0<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">ARA, ALTAR <o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 16h31m / 18h 6m
- Declinação -45<sup>o</sup> 5’ /
-67<sup>o</sup> 6’<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Cerberus, o Cão Cérbero<o:p></o:p></span></span></b></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">História:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Esta constelação não é mais reconhecida nos dias de hoje e teria
sido provavelmente adicionada por Hevelius in 1690. <o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white; color: #073763;"><br /></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Taurus Poniatovii, o Touro de Poniatowski<o:p></o:p></span></span></b></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">História:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Constelação formada pelo Abade Poczobut, em honra ao Rei da Polônia.<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div class="MsoNormal">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">TELESCOPIUM, O TELESCÓPIO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h6m / 20h26m
Declinação -45<sup>o</sup>.4 / -56<sup>o</sup>.9<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">SAGITTARIUS, O ARQUEIRO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 17h41m / 20h15m
Declinação -11<sup>o</sup>.8 / -45<sup>o</sup>.4<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<b><span lang="PT" style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span lang="PT" style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
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<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">SCUTUM, O ESCUDO<o:p></o:p></span></span></b></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h18m / 18h56m
Declinação -4<sup>o</sup>.0 / -16<sup>o</sup>.0<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">CORONA AUSTRALIS, A COROA AUSTRAL<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 17h55m / 19h15m
Declinação -37<sup>o</sup>.0 / -45<sup>o</sup>.6<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
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<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">HYDRUS, HIDRA MACHO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta oh2m / 4h33m
Declinação -58<sup>o</sup>.1 / -82<sup>o</sup>.1<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">LYRA, A LIRA<o:p></o:p></span></span></b></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h12m /
19h26m Declinação +25<sup>o</sup>.6 /
+47<sup>o</sup>.7<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
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<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">INDUS, O ÍNDIO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 20h25m /
23h25m Declinação -45<sup>o</sup>.4 /
-74<sup>o</sup>.7<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">AQUILA, A ÁGUIA <o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h38m/20h36m
Declinação -11<sup>o</sup> 9’ a
-18<sup>o</sup> 6’<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Antinous <o:p></o:p></span></span></b></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">História:<o:p></o:p></span></span></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Hoje em dia esta constelação faz parte de Aquila, a Águia.<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
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<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">SAGITTA, A FLECHA<o:p></o:p></span></span></b></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h56m / 20h18m
Declinação +16<sup>o</sup>.0 / +21<sup>o</sup>.4<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div class="MsoNormal">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">VULPECULA ET ANSER, A RAPOSA E O GANSO<o:p></o:p></span></span></b></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h56m / 21h28m
Declinação +19<sup>o</sup>.5 / +29<sup>o</sup>.4<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">CAPRICORNUS, A CABRA <o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 20h4m / 21h57m
Declinação -8<sup>o</sup>.7 / -27<sup>o</sup>.8<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">CYGNUS, O CISNE<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 19h7m / 22h1m
Declinação +27<sup>o</sup>.7 / +61<sup>o</sup>.2<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div class="MsoNormal">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">MICROSCOPIUM, O MICROSCÓPIO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">Ascensão Reta 20h25m / 21h25m Declinação -27<sup>o</sup>.7 / -45<sup>o</sup>.4<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">TUCANA, O TUCANO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">Ascensão Reta 22h5m / 1h22m Declinação -56<sup>o</sup>.7 / -75<sup>o</sup>.7<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">GRUS, O GROU<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">Ascensão Reta 21h25m / 23h25m Declinação -36<sup>o</sup>.6 / -56<sup>o</sup>.6<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Globus Aerostaticus, o Balão<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Constelação formada por La Lande em 1798, porém obsoleta, nos
dias de hoje.<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">AQUARIUS, O AGUADEIRO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 20h36m / 23h54
- Declinação + 3<sup>o</sup> 1’ a
- 25<sup>o</sup> 2’<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">DELPHINUS, O DELFIM<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 20h13m / 21h6m
Declinação +2<sup>o</sup>.2 / +20<sup>o</sup>.8<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div class="MsoNormal">
<span style="background-color: white; color: #073763;"><a href="http://en.wikipedia.org/wiki/File:Cirta_mosaic.jpg"><span style="font-family: Arial, sans-serif; font-size: 5.5pt;"><br />
</span></a><o:p></o:p></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">PISCES AUSTRALIS, O PEIXE AUSTRAL<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 21h25m / 23h4m
Declinação -25<sup>o</sup>.2 / -36<sup>o</sup>.7<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">PHOENIX, A FÊNIX<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">Ascensão Reta
23h24m / 2h24m Declinação -39<sup>o</sup>.8
/ -58<sup>o</sup>.2<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">EQUULEUS, O CAVALO MENOR<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">Ascensão Reta 20h54m / 21h23m Declinação +2<sup>o</sup>.2 / _12<sup>o</sup>.9<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">PEGASUS, O CAVALO ALADO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 21h5m / 0h13m
Declinação +2<sup>o</sup>.2 / +36<sup>o</sup>.3<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">SCULPTOR, O ESCULTOR<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 23h4m / 1h4m
Declinação -25<sup>o</sup>.2 / -39<sup>o</sup>.8<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">HOROLOGIUM OSCILLATORIUM, O
RELÓGIO <o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 2h12m / 4h18m
Declinação -30<sup>o</sup>.8 / -67<sup>o</sup>.2<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span lang="EN-US" style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">RETICULUM, RETÍCULO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 3h14m / 4h35m
Declinação -53<sup>o</sup>.0 / -67<sup>o</sup>.3<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">PISCES, OS PEIXES<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 22h49m /
2h4m Declinação -6<sup>o</sup>.6 / +33<sup>o</sup>.4<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span lang="PT" style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span lang="PT" style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">ERIDANUS, O RIO ERIDANO<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 1h22m / 5h9m
Declinação +0<sup>o</sup>.1 / -58<sup>o</sup>.1<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span></b></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">CEPHEUS, CEFEU, O REI<o:p></o:p></span></span></b></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
<div align="center" class="MsoNormal" style="line-height: 150%; text-align: center;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">Ascensão Reta 20h1m / 8h30m Declinação +53<sup>o</sup>.1 / +88<sup>o</sup>.5<o:p></o:p></span></span></div>
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<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">CETUS, A BALEIA, O MONSTRO MARINHO<o:p></o:p></span></span></b></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 23h55m / 3h21m
Declinação -25<sup>o</sup>.2 / +10<sup>o</sup>.2<o:p></o:p></span></span></div>
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<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">LACERTA, O LAGARTO<o:p></o:p></span></span></b></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">Ascensão Reta 21h55m / 22h56 Declinação +34<sup>o</sup>.3 / +56<sup>o</sup>.8<o:p></o:p></span></span></div>
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<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Machina Electrica<o:p></o:p></span></span></b></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Uma constelação obsoleta, formada por Bode em 1800.<o:p></o:p></span></span></div>
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<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">DRACO, O DRAGÃO<o:p></o:p></span></span></b></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;"> Situa-se em semi-torno do
Pólo Norte<o:p></o:p></span></span></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt; line-height: 150%;"><span style="background-color: white; color: #073763;">Ascensão Reta 9h18m / 21hom Declinação +47<sup>o</sup>.7 / - 86<sup>o</sup>.0<o:p></o:p></span></span></div>
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<b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">VIA LACTEA<o:p></o:p></span></span></b></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">A Via Láctea foi causada por um derramamento do leite que
Mercúrio era nutrido. De acordo com
outros mitos, Saturno, querendo devorar seus filhos, recebeu uma pedra de sua
mulher e teria engasgado, caso ela não tivesse derramado leite através sua
garganta... e parte desse leite derramou, formando a Via Láctea.<o:p></o:p></span></span></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Os persas achavam que um grande rio corria nos céus, e que nas
margens da Via Láctea pastavam rebanhos de gazelas de patas finas, camelos,
cavalos e avestruzes. Perto das tendas,
estendiam-se oásis com tamareiras e, no centro do paraíso de Alah,
encontrava-se um tesouro de pedras preciosas: a caixa de jóias, perto do
Cruzeiro do Sul.<o:p></o:p></span></span></div>
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<b><span style="background-color: white; color: #073763; font-family: 'Comic Sans MS'; font-size: 11pt;">REFERÊNCIAS BIBLIOGRÁFICAS:<o:p></o:p></span></b></div>
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<span lang="PT" style="font-size: 11pt;"><span style="background-color: white; color: #073763;">COMPILAÇÃO E TRADUÇÃO literal (quando necessária) de Janine Milward:<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="EN-US" style="font-size: 11pt;">- </span><b><span lang="EN-US" style="font-size: 11pt;">Wil Tirion - Atlas of the Night Sky</span></b><span lang="EN-US" style="font-size: 11pt;"> - The Hamlyn
Publishing Group Limited, London, England<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="EN-US" style="font-size: 11pt;">- </span><b><span lang="EN-US" style="font-size: 11pt;">Antonin Rükl - The Hamlyn Encyclopedia of Stars & Planets</span></b><span lang="EN-US" style="font-size: 11pt;">
- The Hamlyn Publishng Group Limited, London, England<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="EN-US" style="font-family: 'Comic Sans MS'; font-size: 11pt;">-
</span><b><span lang="EN" style="font-family: 'Comic Sans MS'; font-size: 11pt;"><a href="http://en.wikipedia.org/wiki/Supercluster"><span lang="EN-US" style="text-decoration: none;">http://en.wikipedia.org/wiki/Supercluster</span></a></span></b><span lang="EN" style="font-family: 'Comic Sans MS'; font-size: 11pt;"><o:p></o:p></span></span></div>
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<span lang="EN" style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">- <b>http://www.atlasoftheuniverse.com</b><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="EN-US" style="font-size: 11pt;">- </span><b><span lang="EN-US" style="font-size: 11pt;">Richard Hinckley Allen, Star
Names, Their Lore and Meaning</span></b><span lang="EN-US" style="font-size: 11pt;">, Dover Publications, Inc, New York, USA <o:p></o:p></span></span></div>
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<span lang="PT" style="font-size: 11pt;"><span style="background-color: white; color: #073763;">-
<b>Bernard Pellequer - Pequeno Guia do Céu</b> - Editora Martins Fontes,
São Paulo, Brasil<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div class="MsoNormal" style="text-align: justify;">
<span style="background-color: white; color: #073763;"><span style="font-family: 'Comic Sans MS'; font-size: 11pt;">- </span><b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;">Identificação do Céu</span></b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"> (Livro
que foi sendo revisado e reeditado algumas vezes) de autoria de <b>Fernando
Vieira</b>, <o:p></o:p></span></span></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Secretaria
Municipal de Cultura, Fundação Planetário da Cidade do Rio de Janeiro<o:p></o:p></span></span></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">(com
dedicatória do próprio autor para mim em Curso de Identificação do Céu, <o:p></o:p></span></span></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">em
30/07/1999))<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">- 6<sup>a</sup>.
Edição do <b>Atlas Celeste</b> <o:p></o:p></span></span></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">de autoria
de <b>Ronaldo Rogério de Freitas Mourão</b>, <o:p></o:p></span></span></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Editora
Vozes, Petrópolis, ano de 1986 <o:p></o:p></span></span></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">(com
dedicatória do próprio autor para mim <o:p></o:p></span></span></div>
<div class="MsoNormal" style="text-align: justify;">
<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">em evento
realizado no Museu de Astronomia do Rio de Janeiro, <o:p></o:p></span></span></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">em
16/06/1989)<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="PT" style="font-family: 'Comic Sans MS'; font-size: 11pt;">- </span><b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;">Mario Jaci
Monteiro</span></b><span style="font-family: 'Comic Sans MS'; font-size: 11pt;"> , <b>As Constelações, Cartas
Celestes</b> - <o:p></o:p></span></span></div>
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<span style="font-family: 'Comic Sans MS'; font-size: 11pt;"><span style="background-color: white; color: #073763;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC - com
dedicatória do autor para mim, em março de 2004 (quando Mário Jaci
generosamente me presenteou com um instrumento de observação (kepleriano)
artesanalmente construído por ele).<o:p></o:p></span></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-32839594418143924052013-08-20T09:07:00.002-07:002014-04-27T13:19:13.090-07:00 Constelações Atuais <div class="MsoNormal" style="text-align: center;">
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</span></span><br />
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<span lang="PT" style="font-family: Arial, sans-serif; line-height: 150%;"><span style="background-color: white; color: #073763; font-size: large;">Da Terra ao Céu
.......................<o:p></o:p></span></span></div>
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<span lang="PT" style="font-family: Arial, sans-serif; line-height: 150%;"><span style="background-color: white; color: #073763; font-size: large;">.........................................................................................<o:p></o:p></span></span></div>
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<span lang="PT" style="font-family: Arial, sans-serif; line-height: 150%;"><span style="background-color: white; color: #073763; font-size: large;">................................
e ao Infinito ...................</span></span><br />
<span lang="PT" style="font-family: Arial, sans-serif; line-height: 150%;"><span style="background-color: white; color: #073763; font-size: large;"><br /></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, sans-serif; font-size: 11pt;"><b>Dois Dedos Iniciais de Prosa</b><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Em primeiríssimo lugar, eu gostaria de dizer que sou apaixonada
pelo céu estrelado, literalmente falando - apaixonada - pelo céu -
estrelado. E foi por essa razão que vim
morar e trabalhar num pedaço de chão um tantinho mais distanciado das luzes
poluentes das grandes cidades e mesmo da pequena e provinciana cidade onde meu
Sítio das Estrelas é situado. Rendo meu
total respeito a Tycho Brahe, por exemplo, que soube olhar para o céu estrelado
e descrevê-lo como ninguém - a julgar pelo fato de que em sua época
instrumentos ópticos ou não existiam ou eram raridades rudimentares (a nosso
ver), ainda engatinhando seus primeiros passos.<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Eu realmente lamento o fato de que a grande maioria dos
Caminhantes dos Céus, dos Amigos das Estrelas, não mora em lugares distantes da
poluição luminosa da Terra sendo levada até os céus, escondendo as estrelas de
tal forma que pensam todos que existem apenas estrelas de primeira ou, no
máximo, de segunda grandezas para serem olhadas!.... e, com sorte, Planetas como
Mercúrio, Vênus, Marte, Júpiter e Saturno, que sorte (pelo menos os Planetas
estão salvos!).<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div class="MsoNormal" style="text-align: justify; text-indent: 35.4pt;">
<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">E, em continuidade ao meu pensamento, eu lamento o fato de que a
grande maioria dos Caminhantes dos Céus não possa usufruir do embevecimento que
a visão a olho nú sempre o céu estrelado nos traz: não existe tédio algum,
jamais, sempre algo no Cenário Celeste muda, sempre a Lua, doce e mutável Lua,
vai avançando de oeste para leste sempre inchando... e meio que <i>aparentemente</i>
saindo do leste em direção ao oeste quando vai sempre desinchando... Sempre podemos ver uma estrela cadente caindo
ali atrás do morro... Sempre podemos nos
surpreender em encontrar alguma constelação que ainda não havíamos
divisado... Sempre nos maravilhamos
diante da visão do Presépio - berço de estrelas-crianças, da Cabeça da Serpente
tomando conta da Coroa Boreal, das duas Nuvens de Magalhães, da Cabeleira de
Berenice, da Hidra enredilhando-se através várias constelações, do Rio Erídano
com sua cabeceira aos pés do Gigante Órion e com sua foz bem ao sul, das
estrelinhas tímidas e ziguezagueantes do Aquário, da Flecha e do Dolfim, da
delicadeza das cordas da Lira, do mito de Andromeda sendo salva por seu Herói
Perseus montado no cavalo alado Pegasus e ainda nos deixando perceber, com visão
enviesada, a Galáxia nossa irmã com nome de Princesa, do tercinho encantador
formado pelas Pleiades, do saco de carvão aos pés da Cruz, do revirão da Via
Láctea acontecendo na cauda do Escorpião que ainda nos faz surpreender com a
visão encantadora da Coroa Austral, com o Caminho de Algodão Leitoso espraiado
pelos céus através estrelas e constelações, nossa Galáxia amada...., Sempre
podemos exalar um suspiro de felicidade ao visualizarmos uma estrela piscando
no oeste, ao cair da noite... quem será, ali, naquele lugar e naquela hora?....
Mercúrio! Não é estrela porém pisca como
uma estrela... você já notou isso?...É preciso olhar literalmente para o céu
estrelado e com a visão desarmada, olho nu, noite após noite, para percebermos
estes pequenos tesouros.<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div class="MsoNormal" style="text-align: justify; text-indent: 35.4pt;">
<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">E ainda em continuidade ao meu pensamento exposto nos dois
parágrafos imediatamente acima, eu lamento que o Caminhante do Céu não
literalmente caminhe no céu... e sim somente
caminhe através as fotografias maravilhosamente maravilhosas que nos são
apresentadas pelas revistas e pelos sites virtuais ou caminhe através os
instrumentos ópticos disponíveis no mercado ou caminhe através os conhecimentos
oferecidos pelos alfarrábios, talvez sendo bem-sucedido em preencher o vazio
instaurado pelo seu não-olhar as estrelas do céu a olho nú, despido de qualquer
outra questão e trajando apenas sua paixão pelo céu estrelado.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">De qualquer forma, todos os Caminhantes do Céu são sempre
privilegiados por serem apaixonadas pelas estrelas - seja pela maneira que for
que vivenciem esta paixão. O Céu sempre
nos traz um sentimento de infinitude da vida... mesmo que saibamos que mesmo a
vida no Céu está sempre em constante mutação, em constante movimentação, em
constante transmutação.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">................ É por
esta e por outras tantas razões, que venho nomeando este meu Trabalho de DA TERRA AO CÉU E AO INFINITO. <o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Este meu Trabalho pressupõe trazer ao conhecimento do Caminhante
do Céu, do Amigo das Estrelas, as 88 Constelações acolhendo seus dados, seus
mitos, suas histórias, suas estrelas, suas nebulosas, seus aglomerados
globulares e abertos, seus aglomerados de galáxias, seus superaglomerados....,
suas muralhas de luz e de sombra...., enfim, tudo aquilo que astronomicamente
pode caber em nossos alfarrábios - ou pelo menos, tudo aquilo que eu, Janine,
simples amante dos céus estrelados, conseguir amealhar a partir de minha
compreensão ainda e sempre simplesmente amadora e respeitosamente braheana.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Com um abraço estrelado,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Janine Milward<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #660000; font-family: Arial, sans-serif; font-size: 11pt;"><b>Uma Breve Visão da Formação das 88 Constelações
Atuais</b></span><span style="color: #073763; font-family: Arial, sans-serif; font-size: 11pt;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;"><b><span style="font-size: large;">Ptolomeu,</span></b> </span><span style="font-family: Arial, sans-serif; font-size: 11pt;">século 11 d.c., matemático e astrônomo. Obra: Almagesto, catálogo que relaciona 1022
estrelas de 48 constelações: 12 zodiacais, 21 ao norte e 15 ao sul.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Andromeda, Aquário, Águia, Altar, Navio Argo, Carneiro,
Cocheiro, Boieiro, Caranguejo, Cão Maior, Cão Menor, Capricórnio, Cassiopéia,
Centauro, Cefeu, Baleia, Coroa Austral, Coroa Boreal, Corvo, Taça, Cisne,
Delfim, Dragão, Cavalo Menor, Erídano, Gêmeos, Hercules, Hidra Fêmea, Leão,
Lebre, Balança, Lobo, Lira, Ofiúco, Orion, Pegaso, Perseu, Peixes, Peixe
Astral, Flecha, Sagitário, Escorpião, Serpente, Touro, Triângulo, Ujrsa Maior,
Ursa Menor, Virgem<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;"><b><span style="font-size: large;">Bayer</span></b></span><span style="font-family: Arial, sans-serif; font-size: 11pt;">,
1603, astrônomo. Obra: Uranometria.
Relaciona 60 constelações, incluindo as circumpolares Sul, cuja
nomenclatura conclui e unifica. </span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Acrescenta 12 constelações.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ave-do-Paraíso, Camaleão, Dourado, Grou, Hidra Macho, Índio,
Mosca, Pavão, Fênix, Triângulo Austral, Tucano, Peixe-Voador<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;"><span style="font-size: large;"><b>Hevelius</b></span></span><span style="font-family: Arial, sans-serif; font-size: 11pt;">,
1690, astrônomo amador, selenógrafo.
Obra: Sete Cartas Celestes. </span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Dá nome a 9 constelações:<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Girafa, Cães de Caça, Lagarto, Leão Menor, Lince, Unicórnio,
Escudo, Sextante, Raposa<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;"><b><span style="font-size: large;">Royer</span></b></span><span style="font-family: Arial, sans-serif; font-size: 11pt;">,
1697, navegante francês. Obra: Carta
Celeste. Desmembra a Cruz Australis da
constelação do Centauro. Cruzeiro do Sul<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif; font-size: 11pt;">Bartschius</span><span style="font-family: Arial, sans-serif; font-size: 11pt;">, 1624. </span><span lang="ES-TRAD" style="font-family: Arial, sans-serif; font-size: 11pt;">Pomba<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="ES-TRAD" style="font-family: Arial, sans-serif;"><b><span style="font-size: large;">La Caille</span></b></span><span lang="ES-TRAD" style="font-family: Arial, sans-serif; font-size: 11pt;">, 1752,
astrônomo. </span><span style="font-family: Arial, sans-serif; font-size: 11pt;">Obras: Memórias e Céu Estrelado. </span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Introduz 14 novas constelações:</span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;"> Máquina Pneumática, Buril, Compasso,
Forno, Relógio, Mesa, Microscópio, Esquadro, Oitante, Pintor, Bússula,
Retículo, Escultor, Telescópio<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">E divide a extensa constelação ptolomaica Argo, o Navio, em
Carina, Puppis e Vela.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Quilha, Popa, Vela<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Algumas Constelações</b></span></span></span><br />
<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">que não fazem parte das 88 Constelações atualmente aceitas</b></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Frederici Honores, Honras de Frederico<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma constelação obsoleta formada por Bode em 1787, em honra a
Frederick II, da Prússia, através as estrelas pertencentes a Cepheus,
Andromeda, Cassiopeia e Cisne.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Nubecula Minor, a Nuvem Pequena, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">a Pequena Nuvem de Magalhães <o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">História:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Provavelmente adicionada por Bayer, 1604.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma das galáxias mais próximas ao nosso próprio sistema da Via
Láctea, considerada como galáxia-satélite, assim como M32 o é em relação à
Grande Nebulosa de Andromeda, M31.
Encontra-se a cerca de 220.000 anos-luz da nossa galáxia. <o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 150%;">Observação a olho nú ou através binóculos e/ou
telescópios:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É visível a olho nú em lugares de céus escuros e transparentes não
muito distante da Grande Nuvem de Magalhães, como se fossem dois pedaços da Via
Láctea. Com um bom par de binóculos,
podemos observar aglomerados como NGC 346 (globular) e NGC 371 (aberto).<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Na roça, as pessoas chamam as duas Nuvens de mulas do presépio de
Jesus.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As Nuvens de Magalhães<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Existem duas pequenas nuvens esfumaçadas que pareciam ser
fragmentos da Via Láctea e que formam um quase triangulo com o pólo sul
celestial. Estas nuvens foram primeiramente
descritas pelo navegante português Fernando de Magalhães, no começo do século
dezesseis. Porém, somente nos anos de
1920, os astrônomos determinaram que as Nuvens de Magalhães são galáxias,
irregulares, pequena e próximas.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As Nuvens de Magalhães são ligadas entre si e à nossa Galáxia não
somente pela força de gravidade mas também pela ponte gigantesca de hidrogênio
neutro e frio. O brilho azulado das
Nuvens de Magalhães revelam a presença de um imenso número de estrelas jovens,
quentes e gigantes muito luminosas.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Se pudéssemos olhar para nossa Galáxia de um ponto externo à mesma,
veríamos três pequenos e próximos satélites (galáxias-satélites), as Nuvens de
Magalhães. Um sistema similar acontece
com a Galáxia de assiopéi, onde podemos observar várias pequenas galáxias
satélites. <o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A Pequena Nuvem de Magalhães<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta é uma galáxia irregular e próxima e que, juntamente com a
Grande Nuvem de Magalhães, órbita nossa Galáxia como se ambas fossem nossos
satélites. <o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A maior parte da massa da Pequena Nuvem de Magalhães consiste de nuvens interestelares de hidrogênio, o
material básico de formação das estrelas - que nesta galáxia acontecem em larga
escala. Prova disso é o grande numero de
estrelas jovens e quentes - gigantes azuis - que trazem à Nuvem esta sua
coloração azulada.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Em 1984, radio-astronomos australianos descobriram que a Pequena
Nuvem de Magalhães consiste, na verdade, de duas galáxias separadas, uma atrás da outra, uma
sendo ocultada de forma que vemos apenas um único objeto no céu. Estas duas
galáxias estão se separando uma da outra e foi exatamente a diferença de
velocidade entre ambas que revelou o fato de a Pequena Nuvem ser, na verdade,
duas galáxias separadas.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Triangulum Minor, o Triângulo Menor<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">História:<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelação formada por Hevelius, em 1690.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Musca Borealis, a Mosca do Norte<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">História:<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelação adicionada por Bartschius, 1624.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Psalterium Georgianum, a Harpa de George<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">História:<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Formada pelo Abade Hell em 1781 em honra a George II da Inglaterra
- porém obsoleta nos dias de hoje.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Custos Messium, o Guardião da Colheita</span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">História:<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelação formada por La Lande em 1775 sob o nome de Le Messieur,
O Senhor, mas não é mais reconhecida.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tarandus, a Rena<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">História:<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelação formada por Monnier, em 1776.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sceptrum Brandenburgicum, o Cetro<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">História:<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelação adicionada por Gottfried Kirch, 1688.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Nubecula Major,</span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> a Grande Nuvem<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">História:<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Provavelmente adicionada por Bayer, 1604.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Juntamente com a Pequena Nuvem de Magalhães, ela forma o par de
galáxias mais próximas à Via Láctea. Estima-se sua distância em 180.000
anos-luz. Os seus inúmeros aglomerados
constituem um notável espetáculo para um simples telescópio. Entre esses objetos, destacam-se a Nebulosa
de Tarântula (30 Doradus), a NGC 1850, a NGC 1854, etc.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As Nuvens de Magalhães<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Existem duas pequenas nuvens esfumaçadas que pareciam ser
fragmentos da Via Láctea e que formam um quase triangulo com o pólo sul
celestial. Estas nuvens foram
primeiramente descritas pelo navegante português Fernando de Magalhães, no
começo do século dezesseis. Porém,
somente nos anos de 1920, os astrônomos determinaram que as Nuvens de Magalhães
são galáxias, irregulares, pequena e próximas.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As Nuvens de Magalhães são ligadas entre si e à nossa Galáxia não
somente pela força de gravidade mas também pela ponte gigantesca de hidrogênio
neutro e frio. O brilho azulado das
Nuvens de Magalhães revelam a presença de um imenso número de estrelas jovens,
quentes e gigantes muito luminosas.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Se pudéssemos olhar para nossa Galáxia de um ponto externo à mesma,
veríamos três pequenos e próximos satélites (galáxias-satélites), as Nuvens de
Magalhães. Um sistema similar acontece
com a Galáxia de ndrômeda, onde podemos observar várias pequenas galáxias
satélites. <o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A Grande Nuvem de Magalhães<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Inicialmente, a Grande Nuvem de Magalhães foi classificada como uma
galáxia irregular. No entanto, mais
tarde foram descobertos sinais de estrutura espiralada e alguma relação com
espirais barrados. A barra é a parte
mais interessante da galáxia e se parece com uma nuvem estelar brilhante e
alongada e ao longo dessa barra, existem numerosas nebulosas avermelhadas por
hidrogênio ionizado, e estimuladas pela radiação de estrelas quentes e
jovens. Nestas regiões são formadas
novas estrelas. <o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Telescopium Herschell, o Telescópio de Herschell<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">História:<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelação formada pelo Abade Hell em 1781, em honra a Sir William
Herschell (o descobridor de Urano).<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Officina Typographica<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelação formada por Bode em 1800, porém obsoleta nos dias de
hoje.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Robur Carolinum, o Carvalho de Charles<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">História:<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelação formada por Halley, 1679, em comemoração ao carvalho<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">onde Charles II escondeu-se.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mons Maenalus, o Monte Maenalus<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> 10 Norte a 18 Norte<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelação formada por Hevelius, 1690.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quadrans Muralis, o Quadrante<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">História:<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelação formada por La Lande em 1795 porém obsoleta nos dias de
hoje.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Noctua, a Coruja<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma constelação obsoleta que ocupava a parte final da cauda da
Hydra.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Cerberus, o Cão Cérbero<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">História:<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação não é mais reconhecida nos dias de hoje e teria
sido provavelmente adicionada por Hevelius in 1690. <o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mito:<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Representa o monstro de três cabeças que guardava o portão do
Hades, os mundos ínferos. Este monstro
foi trazido para a terra por Hercules - e inclusive figura sendo segurado por
Hercules, em cuja constelação agora está fusionado.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Taurus Poniatovii, o Touro de Poniatowski<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">História:<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelação formada pelo Abade Poczobut, em honra ao Rei da Polônia.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Antinous <o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">História:<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Hoje em dia esta constelação faz parte de Aquila, a Águia.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mito:<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Antinous era uma jovem de extraordinária beleza e era a favorita do
Imperador Hadrian. Dizem que a jovem afogou-se no Rio Nilo, na crença que essa
ação estaria prolongando a vida do Imperador - que, em sua honra, colocou-a no
céu no ano de 132 d.c. Antinous também
foi associado a Ganimedes, que foi levado por uma águia e encarregado de servir
uma taça a Júpiter.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Globus Aerostaticus, o Balão<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelação formada por La Lande em 1798, porém obsoleta, nos dias
de hoje.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Machina Electrica<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma constelação obsoleta, formada por Bode em 1800.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">VIA LACTEA<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A Via Láctea foi causada por um derramamento do leite que Mercúrio
era nutrido. De acordo com outros mitos,
Saturno, querendo devorar seus filhos, recebeu uma pedra de sua mulher e teria
engasgado, caso ela não tivesse derramado leite através sua garganta... e parte
desse leite derramou, formando a Via Láctea.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os persas achavam que um grande rio corria nos céus, e que nas
margens da Via Láctea pastavam rebanhos de gazelas de patas finas, camelos,
cavalos e avestruzes. Perto das tendas,
estendiam-se oásis com tamareiras e, no centro do paraíso de Alah,
encontrava-se um tesouro de pedras preciosas: a caixa de jóias, perto do Cruzeiro
do Sul.<o:p></o:p></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
</div>
<div class="MsoNormal" style="text-align: center;">
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br />
</span><br />
<div style="text-align: justify;">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; background-position: initial initial; background-repeat: initial initial; color: #073763; font-family: "Arial","sans-serif";">Os desenhos formados pelas estrelas – As
Constelações - são como janelas que se abrem para a infinitude do universo e
que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o
céu e a terra bem como percebendo que o caos, vagarosamente, vai se tornando
Cosmos e sendo por nossa mente conscientizado. </span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="background-position: initial initial; background-repeat: initial initial; font-family: "Arial","sans-serif";"> Quer dizer, nossa mente é
tão infinita quanto infinito é o Cosmos.</span><span style="font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">COM UM
ABRAÇO ESTRELADO,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine
Milward<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>REFERÊNCIAS BIBLIOGRÁFICAS:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">COMPILAÇÃO E TRADUÇÃO literal (quando necessária)
de Janine Milward:</span><o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- Wil Tirion - Atlas of the Night Sky -
The Hamlyn Publishing Group Limited, London, England<o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- Antonin Rükl - The Hamlyn
Encyclopedia of Stars & Planets - The Hamlyn Publishng Group
Limited, London, England<o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- V. E. Robson - Stars and
Constellations and Their Mythology – Samuel Weiser Inc., York Beach,
Maine, USA<o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- Richard Hinckley Allen, Star Names, Their
Lore and Meaning, Dover Publications, Inc, New York, USA<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- Bernard Pellequer - Pequeno Guia do
Céu - Editora Martins Fontes, São Paulo, Brasil</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- Identificação do Céu (Livro que foi sendo
revisado e reeditado algumas vezes) de autoria de Fernando Vieira,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Secretaria Municipal de Cultura, Fundação Planetário da Cidade do Rio de
Janeiro<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(com dedicatória do próprio autor para mim em Curso de Identificação do
Céu,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em 30/07/1999))<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(com dedicatória do próprio autor para mim<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em evento realizado no Museu de Astronomia do Rio de Janeiro,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em 16/06/1989)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- </span>Mario Jaci Monteiro , As Constelações,
Cartas Celestes -<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC - com dedicatória
do autor para mim, em março de 2004 (quando Mário Jaci generosamente me
presenteou com um instrumento de observação (kepleriano) artesanalmente
construído por ele).<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">COM UM ABRAÇO ESTRELADO,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span><span style="color: navy; font-family: Comic Sans MS; font-size: 11pt;"><o:p></o:p></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-47472374912961888852013-08-20T08:47:00.000-07:002014-08-22T11:38:20.639-07:00VULPECULA ET ANSER, A RAPOSA E O GANSO<div align="center" class="MsoNormal" style="text-align: center;">
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px; text-align: start;">Meu Projeto</span><br />
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;"><span style="font-size: large;">Da Terra ao Céu ....</span></span></span></a></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;"><span style="font-size: large;">.....<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;">e ao Infinito </a></span></span></span></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><span style="color: #660000;"><span style="font-size: large;">- As 88 Constelações</span></span></a></span></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;">http://daterraaoceueaoinfinito.blogspot.com.br/</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<img src="http://www.raremaps.com/maps/medium/30252.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px; padding: 8px;" /><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 22.399999618530273px;">http://www.raremaps.com/gallery/detail/30252/Aquila_and_Antinous_Stars_heightened_in_gold/Hevelius.html</span><br />
<div class="productDetailItem" style="background-color: white; border: 0px; color: #073763; font-family: verdana, arial, georgia, sans-serif; font-size: 16px; line-height: 22.399999618530273px; margin-bottom: 1em; padding: 0px 0px 10px;">
<strong>Title: </strong>Aquila and Antinous (Stars heightened in gold)</div>
<div class="productDetailItem" style="background-color: white; border: 0px; color: #073763; font-family: verdana, arial, georgia, sans-serif; font-size: 16px; line-height: 22.399999618530273px; margin-bottom: 1em; padding: 0px 0px 10px;">
<strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/2813" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; text-decoration: none;">Johannes Hevelius</a></div>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">VULPECULA ET ANSER, A RAPOSA E O GANSO</span></b></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Estivemos em Postagens anteriores</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> comentando sobre o quão rica em vizinhança estrelada</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e de constelações pequenas porém encantadoras</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">é a maravilhosa constelação Aquila, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">a Águia em seu voo balizado por suas três estrelas</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- Alshain, Terazed e Altair, estrela-alpha Aquilae!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Na descrição sobre esta vizinhança estrelada </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">que visualmente apreciamos </span><span style="font-family: Arial, Helvetica, sans-serif;">ao redor da belíssima Águia,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">viemos comentando sobre a delicadeza de figura de um diamante polido</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">que </span><span style="font-family: Arial, Helvetica, sans-serif;"> Delphinus, o Delfim, nos revela!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(veja em h<a href="ttp://oceudomes.blogspot.com.br/2014/08/a-delicada-constelacao-delphinuso-delfim.html" style="color: #274e13;">ttp://oceudomes.blogspot.com.br/2014/08/a-delicada-constelacao-delphinuso-delfim.html</a>)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">E também estivemos apresentando a você, Caro Leitor,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">um tantinho de informações sobre a pequena porém encantadora</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Flecha dos céus estrelados, Sagitta!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(veja em http://oceudomes.blogspot.com.br/2014/08/sagitta-estrelada-flecha-certeira.html)</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Bem grudada à Flecha, a Seta, Sagitta,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">encontra-se uma constelação criada por Hevelius, em 1690,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">na intenção de ocupar um espaço no céu</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">com um animal (a Raposa caçando o Ganso)</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">tão astuto e voraz e corajoso quanto a Águia, Aquila, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e como o Corvo Caído, Vultur Cadens (outra denominação para a Lyra!):</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">entrou em cena, então, a constelação Vulpecula et Anser, a Raposa e o Ganso.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A bem da verdade </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(e como nos diz Ronaldo Rogério de Freitas Mourão),</span></div>
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><i>a Via Láctea passa por Vulpécula,</i></span></span><br />
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><i> o que faz com que suas estrelas não apareçam de maneira proeminente.</i></span></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><i>Esta constelação pode ser encontrada ao longo de Sagitta </i></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><i>ou a partir da estrela Beta Cygni, Albireo</i></span></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">. </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">De qualquer forma, </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">mesmo não sendo uma constelação de estrelas expressivas a olho nu, </span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">bem ao contrário... porém nos trazendo Exoplanetas e</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">nos brindando com a belíssima M27, Dumbbell Nebula </span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">(a Nebulosa da Bolha do Sabão ou do Halteres)....,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e mesmo que ocupe uma área extensa nos céus estrelados do norte,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Vulpecula et Anser ajudam a enriquecer</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">a vizinhança estelar em torno à Águia</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e estas constelações vicinais nos trazem muito prazer</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">em buscar visualizá-las e divisá-las</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">- sempre em noites sem-Lua e em lugares de céus escuros e transparentes.</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">(Aliás, a noite de ontem ofereceu-me um céu translúcido</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e cheio de emoções...</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">- inclusive a boa oportunidade de poder, finalmente!,</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">encontrar e contemplar a tímida constelação </span></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">da valente Raposa!)</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A "dica" é sempre nos orientarmos, num primeiro momento,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">a partir das três estrelas da Águia (Altair, estrela-alpha Aquilae, é inconfundível!)</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e então buscarmos pela figura indubitável da Flecha certeira e estrelada, Sagitta.</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Assim como as cartas celestes nos mostram, Vulpecula encontra-se</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">praticamente grudada à Sagitta </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e ambas constelações situando-se na Grande Fenda, The Great Rift, o Rio do Vazio,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">a bifurcação que acontece naquele ponto da Via Lactea</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> entre as estrelas Altair e Deneb, estrelas-alpha Aquilae e Cygni, respectivamente.... </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- porém é preciso que estejamos em lugar realmente de céus transparentes</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">para bem visualizarmos esses pormenores na Via Lactea...</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Realmente, não é nada fácil divisar e visualizar Vulpecula em bons termos</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- porém eu penso que existe a boa ajuda </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">da imensa e belíssima constelação do Cisne, Cygnus,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> que se espraia em seu voo </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">como se estivesse recém sendo alçado </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">através os céus mais ao norte! </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A estrela-beta Cygni, Albireo</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- que é sugerida ora como o Olho do Cisne e ora como o Bico do Cisne -,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">aponta para a vicinitude da Raposa com o Ganso.</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É bem interessante também percebermos</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">que as constelações Sagitta, a Flecha, e Vulpecula, a Raposa,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">encontram-se bem no caminho do meio</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">da deslumbrante imagem que nomeamos de Grande Triângulo do Norte</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(do Verão, no hemisfério norte, e do Inverno, no hemisfério sul)</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">realizado a partir das estrelas Alpha das constelações Aquila, Lyra e Cygnus,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">quer dizer, das belíssimas estrelas Altair, Vega e Deneb!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Com um abraço estrelado,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Janine Milward</span></span></div>
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<a href="http://www.raremaps.com/gallery/enlarge/33140" style="color: #274e13; text-decoration: none;"><span style="font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/enlarge/33140</span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/33140/Aquila_Sagitta_Vulpecula_and_Anser_Delphinus/Flamsteed.html</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><strong>Title: </strong>Aquila, Sagitta, Vulpecula & Anser Delphinus.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1260" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; text-decoration: none;">John Flamsteed</a></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span><span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></span><span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">VULPECULA ET ANSER, </span></b></span></span><br />
<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">A RAPOSA E O GANSO</span></b><span style="color: #073763;"><o:p></o:p></span></span></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Posicionamento:<o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Ascensão Reta 18h56m / 21h28m Declinação +19<sup>o</sup>.5 / +29<sup>o</sup>.4<o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">História:<o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Constelação formada por Hevelius em 1690 </span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">porém hoje em dia abreviada para Vulpecula.<o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Algumas Informações Interessantes acerca esta Constelação:<o:p></o:p></span></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Esta constelação pode ser encontrada ao longo de Sagitta </span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">ou a partir da estrela Beta Cygni, Albireo. </span></span><br />
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">A Via Láctea passa por Vulpécula,</span></span><br />
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"> o que faz com que suas estrelas não apareçam de maneira proeminente.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp?rightAscension=20.3&declination=23.6">http://www.nightskyatlas.com/index.jsp?rightAscension=20.3&declination=23.6</a></span></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Fronteiras:<o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Vulpecula situa-se entre as constelações </span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Sagitta, Delphinus, Pegasus Cignus Lyra, Hercules<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">I Vulpeculae - Estrela Variável<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Ascensão Reta 20h49m Declinação +28<sup>o</sup>.03<o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Magnitudes: Max 5,9 Min 6,8 Período 4,4<o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Tipo CEP Espectro F8v<o:p></o:p></span></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif; font-size: x-small;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; font-size: x-small;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<a href="http://www.amazon.com/dp/0486210790/ref=rdr_ext_tmb" style="color: #274e13; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">http://www.amazon.com/dp/0486210790/ref=rdr_ext_tmb</span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="font-size: small;"><span lang="EN-US">- </span><b><span lang="EN-US">Richard Hinckley Allen, Star Names, Their Lore and Meaning</span></b><span lang="EN-US">, Dover Publications, Inc, New York, USA <o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="font-size: small;">Richard Hinckley Allen, em seu famoso e importantíssimo livro<br />Star Names — Their Lore and Meaning -,</span></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="font-size: small;">nos fala bem sobre</span></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="font-size: small;">VULPECULA CUM ANSERE</span></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="font-size: small;">A raposa e o Ganso</span></b></span></div>
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<span style="background-color: transparent; color: #000066; font-family: 'Palatino Linotype', Palatino, 'Gentium Plus', serif; font-size: small;"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Vulpecula*.html">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Vulpecula*.html</a></span></div>
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Vulpecula cum Ansere, the Little Fox with the Goose,</h2>
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is known in Italy as <b><span class="Italian" style="color: rgb(0, 102, 0) !important;">Volpe colla Oca</span></b>; in Germany as <b><span class="German" style="color: rgb(51, 153, 153) !important;">Fuchs</span></b>, or <b><span class="German" style="color: rgb(51, 153, 153) !important;">Füchschen</span></b>, <b><span class="German" style="color: rgb(51, 153, 153) !important;">mit der Gans</span></b>; and in France as <b><span class="French" style="color: rgb(0, 153, 51) !important;">Petit Renard avec l'Oie</span></b>.</div>
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Smyth wrote that this is</div>
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a modern constellation, crowded in by Hevelius to occupy a space between the Arrow and the Swan, where the Via Lactea divides into two branches. For this purpose he ransacked the <span class="Latin" style="color: rgb(153, 0, 0) !important;">informes</span> of this bifurcation, and was so satisfied with the result, that the effigies figure in the elaborate print of his offerings to Urania. He selected it on account of the Eagle, Cerberus and Vultur Cadens. "I wished," said he, "to place a fox and a goose in the space of the sky well fitted to it; because such an animal is very cunning, voracious and fierce. Aquila and Vultur are of the same nature, rapacious and greedy."<br />
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The two members are sometimes given separately; indeed the <b>Anser</b> is often omitted. Flamsteed's <i>Atlas</i> shows both, but separates the titles; and Proctor arbitrarily combined both in his <b>Vulpes</b>. Astronomers now call the whole <b>Vulpecula</b>.</div>
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Its inventor saw 27 stars here, but Argelander catalogued 37, and Heis 62. They come to the meridian toward the end of August.</div>
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Although I have elsewhere found no named star in Vulpecula, and its <a href="https://www.blogger.com/null" id="p474"></a><span class="pagenum" style="color: rgb(255, 51, 0) !important; font-size: x-small; position: absolute; right: 1.5em; text-align: right; top: auto; width: 70px;">p474</span>general faintness would render it doubtful whether there ever has been one, yet the<i>Standard Dictionary</i> says of it under the word <b>Anser</b>:</div>
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a small star in the constellation of the Fox and the Goose;<br />
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and the <i>Century Dictionary</i> has much the same. This may have been <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14px; font-style: italic;">α</span>, the <i>lucida</i>, a 4.4‑magnitude just west of the Fox's head.</div>
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A meteor stream, the <b>Vulpeculids</b>, appearing from the 13th of June to the 7th of July, radiates from a point in this constellation; but the latter's most noteworthy object is the <b>Double-headed Shot</b>, or <b>Dumb-bell</b>, <b>Nebula</b>, <a href="http://spider.seds.org/ngc/ngc.cgi?M27" style="color: rgb(204, 0, 0) !important; text-decoration: none;" target="offsite"><span class="star" style="color: rgb(51, 102, 255) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14px; font-style: italic;">NGC 6853, 27 M.</span></a>, just visible in a 1¼‑inch finder, 7° southeast from the star Albireo.</div>
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Smyth wrote that this is</div>
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a modern constellation, crowded in by Hevelius to occupy a space between the Arrow and the Swan, where the Via Lactea divides into two branches. For this purpose he ransacked the <span class="Latin" style="color: rgb(153, 0, 0) !important;">informes</span> of this bifurcation, and was so satisfied with the result, that the effigies figure in the elaborate print of his offerings to Urania. He selected it on account of the Eagle, Cerberus and Vultur Cadens. "I wished," said he, "to place a fox and a goose in the space of the sky well fitted to it; because such an animal is very cunning, voracious and fierce. Aquila and Vultur are of the same nature, rapacious and greedy."</div>
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<span style="background-color: white; font-family: 'Palatino Linotype', Palatino, 'Gentium Plus', serif; font-size: small; line-height: 22.399999618530273px; text-align: center;"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Vulpecula*.html">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Vulpecula*.html</a></span></div>
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<span style="background-color: white; line-height: 22.399999618530273px; text-align: center;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Minha (Janine) simples e direta tradução:</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Smyth escreveu que (esta constelação) é</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="hps">uma constelação</span> <span class="hps">moderna</span>, realizada por <span class="hps">Hevelius</span> na intenção de<span class="hps"> ocupar um espaço</span> <span class="hps">entre a</span> Flecha e o<span class="hps"> Cisne</span>, onde a <span class="hps">Via</span> <span class="hps">Lactea</span> <span class="hps">divide-se em duas vertentes</span>. <span class="hps">Para tanto,</span> não levou em conta esta bifgurcação que ofertou à Urânia sua realização. Hevelius pensou em termos da Águia, do cão Cérbero e do Vultur Cadens,o Corvo Caído. Ele (Hevelius) disse: "Eu queria colocar uma raposa e um ganso num espaço do céu bem propício para isso - porque a raposa é astuta, voraz e feroz e da mesma natureza da Águia e do Vultur, o Corvo" (possivelmente falando sobre a Lyra - nota da tradutora).</span></div>
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<img src="http://www.iau.org/static/public/constellations/gif/VUL.gif" /><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span><span style="background-color: white; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"><span style="color: #252525; font-family: sans-serif;"><a href="http://www.iau.org/static/public/constellations/gif/VUL.gif">http://www.iau.org/static/public/constellations/gif/VUL.gif</a></span></span><br />
<span style="background-color: white; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"><span style="color: #252525; font-family: sans-serif;"><b><br /></b></span></span><b style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"><br /></b><b style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"><br /></b><b style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"><br /></b><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">Vulpecula</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> (Vul), a </span><a href="http://pt.wikipedia.org/wiki/Raposa" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Raposa">Raposa</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">, é uma </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> do </span><a href="http://pt.wikipedia.org/wiki/Hemisf%C3%A9rio_celestial_norte" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Hemisfério celestial norte">hemisfério celestial norte</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. O genitivo, usado para formar nomes de estrelas, é </span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">Vulpeculae</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">.</span><br />
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<span class="mw-headline" id="Estrelas"><span style="font-size: small;">Estrelas</span></span></h3>
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Não há <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a> mais brilhantes que <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude</a> 4 em Vulpecula. <b>A estrela mais brilhante da constelação é <a href="http://pt.wikipedia.org/wiki/Alpha_Vulpeculae" style="background: none; color: #0b0080; text-decoration: none;" title="Alpha Vulpeculae">α Vulpeculae</a>, uma <a href="http://pt.wikipedia.org/wiki/Gigante_vermelha" style="background: none; color: #0b0080; text-decoration: none;" title="Gigante vermelha">gigante vermelha</a> com uma magnitude aparente de apenas 4,44 situada a 297 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> da Terra</b>. Ela forma uma <a href="http://pt.wikipedia.org/wiki/Estrela_dupla" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela dupla">binária óptica</a> com <a class="new" href="http://pt.wikipedia.org/w/index.php?title=8_Vulpeculae&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="8 Vulpeculae (página não existe)">8 Vulpeculae</a>, com uma separação de cerca de 7 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a>.<span class="reference" id="cite_ref-anser_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Vulpecula#cite_note-anser-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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http://pt.wikipedia.org/wiki/Vulpecula</div>
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<b>Alpha Vulpeculae</b> (α Vul / α Vulpeculae) é a <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a> mais brilhante da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Vulpecula" style="background: none; color: #0b0080; text-decoration: none;" title="Vulpecula">Vulpecula</a>. Tem os nomes tradicionais <b>Lukida</b>, <b>Lucida Anseris</b> ou <b>Anser</b>.</div>
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Alpha Vulpeculae é uma <a href="http://pt.wikipedia.org/wiki/Gigante_vermelha" style="background: none; color: #0b0080; text-decoration: none;" title="Gigante vermelha">gigante vermelha</a> de <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">classe espectral</a> M0 que está a aproximadamente 297 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>. Ela forma uma <a href="http://pt.wikipedia.org/wiki/Estrela_dupla" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela dupla">binária óptica</a> com <a class="new" href="http://pt.wikipedia.org/w/index.php?title=8_Vulpeculae&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="8 Vulpeculae (página não existe)">8 Vulpeculae</a>.</div>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">http://pt.wikipedia.org/wiki/Alpha_Vulpeculae</span></span><br />
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<b><span style="font-size: large;">Em 1967, o primeiro <a href="http://pt.wikipedia.org/wiki/Pulsar" style="background: none; color: #0b0080; text-decoration: none;" title="Pulsar">pulsar</a>, <a href="http://pt.wikipedia.org/wiki/PSR_B1919%2B21" style="background: none; color: #0b0080; text-decoration: none;" title="PSR B1919+21">PSR B1919+21</a>, foi descoberto em Vulpecula</span></b> por <a href="http://pt.wikipedia.org/wiki/Antony_Hewish" style="background: none; color: #0b0080; text-decoration: none;" title="Antony Hewish">Antony Hewish</a> e <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Jocelyn_Bell&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Jocelyn Bell (página não existe)">Jocelyn Bell</a>, em <a href="http://pt.wikipedia.org/wiki/Cambridge" style="background: none; color: #0b0080; text-decoration: none;" title="Cambridge">Cambridge</a>. Enquanto eles estavam procurando cintilações de sinais de rádio de <a href="http://pt.wikipedia.org/wiki/Quasar" style="background: none; color: #0b0080; text-decoration: none;" title="Quasar">quasares</a>, eles observaram pulsos que se repetiam com um período de 1,3373 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a>.<span class="reference" id="cite_ref-hewish_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Vulpecula#cite_note-hewish-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> Essa anomalia foi identificada como o sinal de uma <a href="http://pt.wikipedia.org/wiki/Estrela_de_n%C3%AAutrons" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela de nêutrons">estrela de nêutrons</a> de rápida rotação. 15 anos depois da descoberto desse pulsar, foi descoberto também em Vulpecula o primeiro <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Pulsar_milissegundo&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Pulsar milissegundo (página não existe)">pulsar milissegundo</a>, <a href="http://pt.wikipedia.org/wiki/PSR_B1937%2B21" style="background: none; color: #0b0080; text-decoration: none;" title="PSR B1937+21">PSR B1937+21</a>, a poucos graus de distância no céu de PSR B1919+21.<span class="reference" id="cite_ref-backer_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Vulpecula#cite_note-backer-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></div>
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http://pt.wikipedia.org/wiki/Vulpecula</div>
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<span style="font-size: large;"><b>PSR B1919 +21'</b> é um <a href="http://pt.wikipedia.org/wiki/Pulsar" style="background: none; color: #0b0080; text-decoration: none;" title="Pulsar">pulsar</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Vulpecula" style="background: none; color: #0b0080; text-decoration: none;" title="Vulpecula">Vulpecula</a></span> com um período de 1,3373 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a><span class="reference" id="cite_ref-Arzoumanian1994_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/PSR_B1919%2B21#cite_note-Arzoumanian1994-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> e uma largura de pulso de 0,04 segundos. Descoberto em julho de <a href="http://pt.wikipedia.org/wiki/1967" style="background: none; color: #0b0080; text-decoration: none;" title="1967">1967</a>, foi o primeiro pulsar a ser descoberto com ondas de rádio. Sua designação original era <b>CP 1919</b> e ele também é conhecido como <b>PSR J1921+2153</b>.</div>
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<span class="mw-headline" id="Descoberta"><span style="font-size: small;">..................</span></span></h2>
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Antes que natureza do sinal foi determinada, os investigadores, Bell e seu supervisor Ph.D <a href="http://pt.wikipedia.org/wiki/Antony_Hewish" style="background: none; color: #0b0080; text-decoration: none;" title="Antony Hewish">Antony Hewish</a>, consideraram seriamente a possibilidade de vida extraterrestre:</div>
<dl style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; margin-bottom: 0.5em; margin-top: 0.2em; text-align: start;"><dd style="line-height: 1.5em; margin-bottom: 0.1em; margin-left: 1.6em; margin-right: 0px;"><i>"Nós não acreditamos realmente que tínhamos pego sinais de outra civilização, mas é evidente que a ideia havia atravessado nossas mentes e nós não tínhamos qualquer prova de que foi uma emissão de rádio totalmente natural. É um problema interessante - se um pensa que pode ter detectado uma vida em outros pontos do universo como anunciar o resultado responsavelmente? Quem faz um dizer primeiro?"</i><span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/PSR_B1919%2B21#cite_note-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></dd></dl>
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A observação recebeu a designação <i><a href="http://pt.wikipedia.org/wiki/LGM-1" style="background: none; color: #0b0080; text-decoration: none;" title="LGM-1">Little green men 1</a></i>, até que os pesquisadores <a href="http://pt.wikipedia.org/wiki/Thomas_Gold" style="background: none; color: #0b0080; text-decoration: none;" title="Thomas Gold">Thomas Gold</a> e <a href="http://pt.wikipedia.org/wiki/Fred_Hoyle" style="background: none; color: #0b0080; text-decoration: none;" title="Fred Hoyle">Fred Hoyle</a> terem corretamente identificados esses sinais como uma<a href="http://pt.wikipedia.org/wiki/Estrela_de_n%C3%AAutrons" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela de nêutrons">estrela de nêutrons</a> de rápida rotação com um campo magnético forte.</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/PSR_B1919%2B21</span></span></div>
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<b><span style="font-size: large;">Na constelação de Vulpecula também se encontra o <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Planeta_extrassolar" style="background: none; color: #0b0080; text-decoration: none;" title="Planeta extrassolar">planeta extrassolar</a> <a href="http://pt.wikipedia.org/wiki/HD_189733_b" style="background: none; color: #0b0080; text-decoration: none;" title="HD 189733 b">HD 189733 b</a></span></b>. Esse planeta tem uma massa de 1,14 <a href="http://pt.wikipedia.org/wiki/Massa_de_J%C3%BApiter" style="background: none; color: #0b0080; text-decoration: none;" title="Massa de Júpiter">massas de Júpiter</a> e um <a href="http://pt.wikipedia.org/wiki/Per%C3%ADodo_orbital" style="background: none; color: #0b0080; text-decoration: none;" title="Período orbital">período orbital</a> de 2,22 dias,<span class="reference" id="cite_ref-epe_4-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Vulpecula#cite_note-epe-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> o que o torna um <a href="http://pt.wikipedia.org/wiki/J%C3%BApiter_quente" style="background: none; color: #0b0080; text-decoration: none;" title="Júpiter quente">Júpiter quente</a>. Em 2007, análises espectroscópicas revelaram grandes quantidades de <a href="http://pt.wikipedia.org/wiki/Vapor_de_%C3%A1gua" style="background: none; color: #0b0080; text-decoration: none;" title="Vapor de água">vapor de água</a> nele,<span class="reference" id="cite_ref-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Vulpecula#cite_note-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> e também em 2007 foi criado um mapa de temperatura de HD 189733 b a partir de dados do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Spitzer" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Spitzer">Telescópio Espacial Spitzer</a>, o primeiro mapa de um planeta extrassolar.<span class="reference" id="cite_ref-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Vulpecula#cite_note-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span></div>
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http://pt.wikipedia.org/wiki/Vulpecula</div>
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<b>HD 189733b</b> é um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Planeta_extrassolar" style="background: none; color: #0b0080; text-decoration: none;" title="Planeta extrassolar">planeta extrassolar</a> gigante, parecido com <a href="http://pt.wikipedia.org/wiki/J%C3%BApiter_(planeta)" style="background: none; color: #0b0080; text-decoration: none;" title="Júpiter (planeta)">Júpiter</a>. Está situado a cerca de 63 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>. Foi descoberto em <a href="http://pt.wikipedia.org/wiki/2005" style="background: none; color: #0b0080; text-decoration: none;" title="2005">2005</a>, porém foi recentemente descoberta a existência de <a href="http://pt.wikipedia.org/wiki/Vapor_de_%C3%A1gua" style="background: none; color: #0b0080; text-decoration: none;" title="Vapor de água">vapor de água</a> em sua <a href="http://pt.wikipedia.org/wiki/Atmosfera" style="background: none; color: #0b0080; text-decoration: none;" title="Atmosfera">atmosfera</a> .</div>
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A massa de HD 189733b é cerca de 15% maior que a de <a href="http://pt.wikipedia.org/wiki/J%C3%BApiter" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Júpiter">Júpiter</a>. Em 2013 o <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio espacial Hubble">telescópio espacial Hubble</a> revelou que o exoplaneta HD 189733 B é azul, porém acredita-se que o azul dele não vem da reflexão de um oceano, mas deve-se a uma atmosfera gasosa e turbulenta, composta principalmente por <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Hidrog%C3%AAnio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hidrogênio">hidrogênio</a> e carregada por partículas de <a href="http://pt.wikipedia.org/wiki/Silicato" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Silicato">silicato</a>, transmitindo assim luz azul.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/HD_189733_b#cite_note-1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
<table class="toccolours" style="background-color: #f9f9f9; border: 1px solid rgb(170, 170, 170); clear: right; color: #252525; font-family: sans-serif; font-size: 12px; margin: 0px 0px 1em 1em; padding: 5px;"><caption style="font-size: 16px; margin-left: inherit;"><b>HD 189733 b</b></caption><tbody>
<tr><th colspan="2" style="background-color: #a0b0ff;" width="140px"><small><a href="http://pt.wikipedia.org/wiki/Exoplaneta" style="background: none; color: #0b0080; text-decoration: none;" title="Exoplaneta">Exoplaneta</a></small></th><td align="center" width="160px"><small><a href="http://pt.wikipedia.org/wiki/Anexo:Lista_de_estrelas_com_exoplaneta" style="background: none; color: #0b0080; text-decoration: none;" title="Anexo:Lista de estrelas com exoplaneta">Lista de exoplanetas</a></small></td></tr>
<tr><td colspan="3" style="text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Exoplanet_Comparison_HD_189733_b.png" style="background: none; color: #0b0080; text-decoration: none;"><img alt="Exoplanet Comparison HD 189733 b.png" data-file-height="480" data-file-width="1040" src="http://upload.wikimedia.org/wikipedia/commons/thumb/9/9d/Exoplanet_Comparison_HD_189733_b.png/300px-Exoplanet_Comparison_HD_189733_b.png" height="138" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/9/9d/Exoplanet_Comparison_HD_189733_b.png/450px-Exoplanet_Comparison_HD_189733_b.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/9/9d/Exoplanet_Comparison_HD_189733_b.png/600px-Exoplanet_Comparison_HD_189733_b.png 2x" style="border: none; vertical-align: middle;" width="300" /></a><br />
<center>
<small>Comparação de tamanho entre HD 189733 b e Júpiter.</small></center>
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<tr><th colspan="3" style="background-color: #a0b0ff;">Estrela mãe</th></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">Estrela</a></b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/HD_189733" style="background: none; color: #0b0080; text-decoration: none;" title="HD 189733">HD 189733</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/Vulpecula" style="background: none; color: #0b0080; text-decoration: none;" title="Vulpecula">Vulpecula</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Ascensão reta</a></b></td><td align="left">20<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 00<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 43,8<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></b></td><td align="left">22° 42′ 39,1″</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnitude aparente</a></b></td><td align="left">7,66</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Dist%C3%A2ncia" style="background: none; color: #0b0080; text-decoration: none;" title="Distância">Distância</a></b></td><td align="left">62,9 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (19,3 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</td></tr>
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<span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/HD_189733_b</span></span></div>
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<b>HD 188015 b</b> é um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Planeta_extrassolar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Planeta extrassolar">planeta extrassolar</a> que orbita a <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a> <a href="http://pt.wikipedia.org/wiki/HD_188015" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="HD 188015">HD 188015</a>. Como a maioria dos planetas extrassolares, ele foi descoberto usando o método da<a href="http://pt.wikipedia.org/wiki/Velocidade_radial" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Velocidade radial">velocidade radial</a>. A massa mínima do planeta é de cerca de um quarto a mais do que a <a href="http://pt.wikipedia.org/wiki/Massa_de_J%C3%BApiter" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080;" title="Massa de Júpiter">massa de Júpiter</a>. Ele orbita HD 188015 em uma <a href="http://pt.wikipedia.org/wiki/%C3%93rbita" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Órbita">órbita</a> um pouco<a href="http://pt.wikipedia.org/wiki/Excentricidade_orbital" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Excentricidade orbital">excêntrica</a>, em uma distância média de aproximadamente 20% a mais da distância da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> ao <a href="http://pt.wikipedia.org/wiki/Sol" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sol">Sol</a>.</div>
<table class="toccolours" style="background-color: #f9f9f9; border: 1px solid rgb(170, 170, 170); clear: right; color: #252525; font-family: sans-serif; font-size: 12px; margin: 0px 0px 1em 1em; padding: 5px;"><caption style="font-size: 16px; margin-left: inherit;"><b>HD 188015 b</b></caption><tbody>
<tr><th colspan="2" style="background-color: #a0b0ff;" width="140px"><small><a href="http://pt.wikipedia.org/wiki/Exoplaneta" style="background: none; color: #0b0080; text-decoration: none;" title="Exoplaneta">Exoplaneta</a></small></th><td align="center" width="160px"><small><a href="http://pt.wikipedia.org/wiki/Anexo:Lista_de_estrelas_com_exoplaneta" style="background: none; color: #0b0080; text-decoration: none;" title="Anexo:Lista de estrelas com exoplaneta">Lista de exoplanetas</a></small></td></tr>
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<tr><th colspan="3" style="background-color: #a0b0ff;">Estrela mãe</th></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">Estrela</a></b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/HD_188015" style="background: none; color: #0b0080; text-decoration: none;" title="HD 188015">HD 188015</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/Vulpecula" style="background: none; color: #0b0080; text-decoration: none;" title="Vulpecula">Vulpecula</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Ascensão reta</a></b></td><td align="left">19<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 52<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 04,5<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></b></td><td align="left">28° 06′ 01,3″</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnitude aparente</a></b></td><td align="left">8,242</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Dist%C3%A2ncia" style="background: none; color: #0b0080; text-decoration: none;" title="Distância">Distância</a></b></td><td align="left">171,66 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (52,63 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</td></tr>
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<span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/HD_188015_b</span></span></div>
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<b style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">HD 190228</b><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Planeta_extrassolar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Planeta extrassolar">planeta extrassolar</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> que orbita a </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Estrela">estrela</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> </span><a href="http://pt.wikipedia.org/wiki/HD_190228" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="HD 190228">HD 190228</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">. Sua massa mínima é de 4,49 </span><a href="http://pt.wikipedia.org/wiki/Massa_de_J%C3%BApiter" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Massa de Júpiter">massas de Júpiter</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">. Ele orbita a estrela a uma distância que varia entre 1,13 </span><a href="http://pt.wikipedia.org/wiki/Unidade_astron%C3%B4mica" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Unidade astronômica">UA</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> a 3,37 UA. Assim como a maioria dos planetas extrassolares, foi descoberto usando o método da </span><a href="http://pt.wikipedia.org/wiki/Velocidade_radial" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Velocidade radial">velocidade radial</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">.</span></div>
<table class="toccolours" style="background-color: #f9f9f9; border: 1px solid rgb(170, 170, 170); clear: right; color: #252525; font-family: sans-serif; font-size: 12px; margin: 0px 0px 1em 1em; padding: 5px;"><caption style="font-size: 16px; margin-left: inherit;"><b>HD 190228 b</b></caption><tbody>
<tr><th colspan="2" style="background-color: #a0b0ff;" width="140px"><small><a href="http://pt.wikipedia.org/wiki/Exoplaneta" style="background: none; color: #0b0080; text-decoration: none;" title="Exoplaneta">Exoplaneta</a></small></th><td align="center" width="160px"><small><a href="http://pt.wikipedia.org/wiki/Anexo:Lista_de_estrelas_com_exoplaneta" style="background: none; color: #0b0080; text-decoration: none;" title="Anexo:Lista de estrelas com exoplaneta">Lista de exoplanetas</a></small></td></tr>
<tr><td colspan="3" style="text-align: center;"></td></tr>
<tr><th colspan="3" style="background-color: #a0b0ff;">Estrela mãe</th></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">Estrela</a></b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/HD_190228" style="background: none; color: #0b0080; text-decoration: none;" title="HD 190228">HD 190228</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/Vulpecula" style="background: none; color: #0b0080; text-decoration: none;" title="Vulpecula">Vulpecula</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Ascensão reta</a></b></td><td align="left">20<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 03<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 00,8<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></b></td><td align="left">28° 18′ 24,7″</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnitude aparente</a></b></td><td align="left">7,307</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Dist%C3%A2ncia" style="background: none; color: #0b0080; text-decoration: none;" title="Distância">Distância</a></b></td><td align="left">202,58 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (62,11 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</td></tr>
<tr><td align="left" colspan="2"><b><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Tipo_espectral" style="background: none; color: #0b0080; text-decoration: none;" title="Tipo espectral">Tipo espectral</a></b></td><td align="left">G5IV</td></tr>
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<span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/HD_190228_b</span></span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/7/71/Vulpecula_constellation_map.png/1024px-Vulpecula_constellation_map.png" /></div>
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<span class="mw-headline" style="font-weight: normal;"><span style="font-size: small;">http://pt.wikipedia.org/wiki/Vulpecula#mediaviewer/Ficheiro:Vulpecula_constellation_map.png</span></span></h3>
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<span class="mw-headline">Objetos de céu profundo</span></h3>
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Dois bem conhecidos objetos de <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Céu profundo">céu profundo</a> podem ser achados em Vulpecula.<b> A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa do Haltere">nebulosa do Haltere</a> (M27) </b>é uma grande e brilhante <a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa planetária">nebulosa planetária</a>. Ela foi descoberta por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em <a href="http://pt.wikipedia.org/wiki/1764" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1764">1764</a>, sendo a primeira nebulosa planetária descoberta.<span class="reference" id="cite_ref-7" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Vulpecula#cite_note-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span> <b>O <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Aglomerado_de_Brocchi&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Aglomerado de Brocchi (página não existe)">Aglomerado de Brocchi</a> (Collinder 399</b>) é um grupo de cerca de 40 estrelas descoberto pelo astrônomo da Pérsia <a href="http://pt.wikipedia.org/wiki/Al_Sufi" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Al Sufi">Al Sufi</a> no ano de 964 e mais tarde redescoberto independentemente pelo astrônomo italiano <a href="http://pt.wikipedia.org/wiki/Giovanni_Battista_Hodierna" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Giovanni Battista Hodierna">Giovanni Battista Hodierna</a>. A classificação desse aglomerado mudou muito, mas observações recentes feitas pelo satélite <a href="http://pt.wikipedia.org/wiki/Hipparcos" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hipparcos">Hipparcos</a> indicam que ele é um <a href="http://pt.wikipedia.org/wiki/Asterismo_(astronomia)" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Asterismo (astronomia)">asterismo</a>, sem ligação física.<span class="reference" id="cite_ref-8" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Vulpecula#cite_note-8" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">8</a></span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Vulpecula</span></span></div>
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<b style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">NGC 6802</b><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Vulpecula" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Vulpecula">constelação de Vulpecula</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="William Herschel">William Herschel</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> em 1784, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> (+8,8), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> amadores ou com equipamentos superiores.</span></div>
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<span style="font-size: 14px; line-height: 22.399999618530273px; text-align: start;"><span style="color: #252525; font-family: sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_6802">http://pt.wikipedia.org/wiki/NGC_6802</a></span></span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/9/9d/Ngc_6802_ver.jpg" /></div>
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http://pt.wikipedia.org/wiki/NGC_6802#mediaviewer/Ficheiro:Ngc_6802_ver.jpg</div>
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<span style="background-color: white;"><span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Ngc 6802 </span></span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span class="mw-mmv-author"><a class="new" href="http://commons.wikimedia.org/w/index.php?title=User:Irchans&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="User:Irchans (página não existe)">Irchans</a></span> - <span class="mw-mmv-source"><span class="int-own-work">Obra do próprio</span></span></span></div>
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<span style="background-color: white;"><b style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">NGC 6940</b><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Vulpecula" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Vulpecula">constelação de Vulpecula</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="William Herschel">William Herschel</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> em 1784, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> (+6,3), é visível apenas com telescópios amadores ou com equipamentos superiores.</span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><a href="http://pt.wikipedia.org/wiki/NGC_6940">http://pt.wikipedia.org/wiki/NGC_6940</a></span></span><br />
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">NGC 6830</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;" title="Aglomerado aberto">aglomerado aberto</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Vulpecula" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Vulpecula">constelação de Vulpecula</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="William Herschel">William Herschel</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> em 1784, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> (+7,9), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> amadores ou com equipamentos superiores.</span><br />
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<span style="background-color: white; line-height: 22.399999618530273px; text-align: start;"><span style="color: #252525; font-family: sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_6830">http://pt.wikipedia.org/wiki/NGC_6830</a></span></span><br />
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<span style="background-color: white;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span><img src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e8/M27_-_Dumbbell_Nebula.jpg/800px-M27_-_Dumbbell_Nebula.jpg" /><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">http://en.wikipedia.org/wiki/Dumbbell_Nebula#mediaviewer/File:M27_-_Dumbbell_Nebula.jpg</span></span><br />
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<span style="background-color: white;"><span class="mw-mmv-title" original-title="File name" style="font-size: 1.2em; max-width: 60%;">M27 - Dumbbell Nebula</span></span></div>
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<span class="mw-mmv-source-author" original-title="Author and source information" style="background-color: white;"><span class="mw-mmv-author">ESO</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.eso.org/public/images/eso9846a/" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://www.eso.org/public/images/eso9846a/</a></span></span></div>
<span style="background-color: white;"><span style="color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start;">The </span><a class="extiw" href="http://en.wikipedia.org/wiki/Dumbbell_Nebula" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start; text-decoration: none;" title="en:Dumbbell Nebula">Dumbbell Nebula</a><span style="color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start;"> — also known as Messier 27 or NGC 6853 — is a typical planetary nebula and is located in the constellation </span><a class="extiw" href="http://en.wikipedia.org/wiki/Vulpecula" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start; text-decoration: none;" title="en:Vulpecula">Vulpecula</a><span style="color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start;"> (The Fox). The distance is rather uncertain, but is believed to be around 1200 light-years. It was first described by the French astronomer and comet hunter </span><a class="extiw" href="http://en.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start; text-decoration: none;" title="en:Charles Messier">Charles Messier</a><span style="color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start;"> who found it in 1764 and included it as no. 27 in his famous list of extended sky objects. Despite its class, the Dumbbell Nebula has nothing to do with planets. It consists of very rarified gas that has been ejected from the hot central star now in one of its last evolutionary stages. Colours & filters Band Wavelength Telescope Optical B 429 nm Very Large Telescope FORS1 Optical Oiii 501 nm Very Large Telescope FORS1 Optical H-alpha 656 nm Very Large Telescope FORS1 .</span></span><br />
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">NGC 6853 - M 27 - Vulpecula - Nebulosa Planetária - Bolha de Sabão</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Ascensão Reta 19h58m Declinação +22<sup>o</sup>.40<o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Tipo Nebulosa Planetária NP Dimensão 7,0 Magnitude 20<o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Magnitude da Estrela associada 13 Distância em anos-luz 3,5<o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Encontrada mais ao sul e na fronteira com Sagitta.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> É uma nebulosa planetária e conhecida como Dumbbell.<o:p></o:p></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif; font-size: x-small;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; font-size: x-small;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<tr><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="See Explanation. Clicking on the picture will download
the highest resolution version available." src="http://apod.nasa.gov/apod/image/1112/m27_snyder_900.jpg" height="477" style="margin-left: auto; margin-right: auto;" width="640" /></span></td></tr>
<tr><td class="tr-caption" style="font-size: 13px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://apod.nasa.gov/apod/ap111227.html">http://apod.nasa.gov/apod/ap111227.html</a></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">M27: The Dumbbell Nebula<br />Image Credit & Copyright: <a href="http://billsnyderastrophotography.com/?page_id=2">Bill Snyder</a> (<a href="http://billsnyderastrophotography.com/">Bill Snyder Photography</a>) </span></td></tr>
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<b> Explanation: </b>The first hint of what will become of our <a href="http://www.nineplanets.org/sol.html">Sun</a> was discovered inadvertently in <a href="http://en.wikipedia.org/wiki/1764">1764</a>. At that time, <a href="http://www.seds.org/messier/xtra/history/biograph.html">Charles Messier</a> was compiling a list of diffuse objects not to be confused with comets. The 27th object on <a href="http://apod.nasa.gov/apod/ap960626.html">Messier's list</a>, now known as <a href="http://www.seds.org/messier/m/m027.html">M27</a> or the Dumbbell Nebula, is a <a href="http://apod.nasa.gov/apod/planetary_nebulae.html">planetary nebula</a>, the type of nebula our <a href="http://asterisk.apod.com/viewtopic.php?f=24&t=18012">Sun</a> will produce when <a href="http://fusedweb.pppl.gov/">nuclear fusion</a> stops in its core. <a href="http://apod.nasa.gov/apod/ap020302.html">M27</a> is one of the brightest <a href="http://www.seds.org/messier/planetar.html">planetary nebulae</a> on the sky, and can be seen toward the <a href="http://www.astro.wisc.edu/~dolan/constellations/extra/constellations.html">constellation</a> of the Fox (<a href="http://en.wikipedia.org/wiki/Vulpecula">Vulpecula</a>) with binoculars. It takes light about 1000 years to reach us from M27, <a href="http://billsnyderastrophotography.com/?page_id=1767">shown above</a> in colors emitted by <a href="http://en.wikipedia.org/wiki/H-alpha">hydrogen</a> and <a href="http://periodic.lanl.gov/8.shtml">oxygen</a>. Understanding the physics and significance of <a href="http://apod.nasa.gov/apod/ap100826.html">M27</a> was well beyond 18th century science. Even today, many things remain mysterious about <a href="http://apod.nasa.gov/apod/ap040201.html">bipolar planetary nebula</a> like M27, including the physical mechanism that expels a low-mass star's gaseous outer-envelope, leaving an <a href="http://science.hq.nasa.gov/kids/imagers/ems/xrays.html">X-ray</a> hot <a href="http://imagine.gsfc.nasa.gov/docs/science/know_l2/dwarfs.html">white dwarf</a>.<br />
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A <b>Nebulosa do Haltere</b> (Messier 27, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6853</a>), foi a primeira <a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa planetária">nebulosa planetária</a> descoberta. Está localizada a cerca de mil e duzentos <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> de distância da <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>, na direção da <a href="http://pt.wikipedia.org/wiki/Vulpecula" style="background: none; color: #0b0080; text-decoration: none;" title="Vulpecula">Constelação da Raposa</a>.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere#cite_note-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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Foi descoberta em <a href="http://pt.wikipedia.org/wiki/1764" style="background: none; color: #0b0080; text-decoration: none;" title="1764">1764</a>, por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a>. Com seu brilho de magnitude aparente 7,5 e com <a href="http://pt.wikipedia.org/wiki/Di%C3%A2metro" style="background: none; color: #0b0080; text-decoration: none;" title="Diâmetro">diâmetro</a> aparente de cerca de 8 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a>, é facilmente visível com<a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background: none; color: #0b0080; text-decoration: none;" title="Binóculo">binóculos</a> e bastante observada por <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background: none; color: #0b0080; text-decoration: none;" title="Astronomia">astrônomos</a> amadores. Situa-se aproximadamente a 1000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> e sua idade, cerca de 10 000 anos, é extremamente pequena em termos astrônomicos, embora comum para nebulosas planetárias.</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere</span></span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/d/d7/Weighing_in_on_the_Dumbbell_Nebula.jpg/1920px-Weighing_in_on_the_Dumbbell_Nebula.jpg" /></div>
<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Dumbbell_Nebula#mediaviewer/File:Weighing_in_on_the_Dumbbell_Nebula.jpg">http://en.wikipedia.org/wiki/Dumbbell_Nebula#mediaviewer/File:Weighing_in_on_the_Dumbbell_Nebula.jpg</a></span><br />
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<span style="background-color: white;"><span style="color: #073763;"><span class="mw-mmv-title" original-title="File name" style="font-size: 1.2em; max-width: 60%;">Weighing in on the Dumbbell Nebula</span></span></span></div>
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<span class="mw-mmv-source-author" original-title="Author and source information" style="background-color: white;"><span style="color: #073763;"><span class="mw-mmv-author">NASA/JPL-Caltech/J. Hora (Harvard-Smithsonian CfA)</span> - <span class="mw-mmv-source"><a class="external text" href="http://www.spitzer.caltech.edu/images/4409-sig11-011-Weighing-in-on-the-Dumbbell-Nebula" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;">JPL</a></span></span></span></div>
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<span style="background-color: white;">Image from the <a href="http://en.wikipedia.org/wiki/Spitzer_Space_Telescope" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Spitzer Space Telescope">Spitzer Space Telescope</a>.</span></div>
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<span style="background-color: white;">The Dumbbell nebula, also known as Messier 27, pumps out <a href="http://commons.wikimedia.org/wiki/Category:Infrared" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Category:Infrared">infrared</a> light in this image from NASAs <a href="http://commons.wikimedia.org/wiki/Category:Spitzer_space_telescope" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Category:Spitzer space telescope">Spitzer Space Telescope</a>. Spitzers infrared view shows a different side of this recycled stellar material. It is interesting how different Spitzers view of the Dumbbell looks compared to optical images, comments Dr. Joseph Hora of the <a href="http://commons.wikimedia.org/wiki/Category:Harvard-Smithsonian_Center_for_Astrophysics" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Category:Harvard-Smithsonian Center for Astrophysics">Harvard Smithsonian Center for Astrophysics</a>. The diffuse <a href="http://commons.wikimedia.org/wiki/Green" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Green">green</a> glow, which is brightest near the center, is probably showing us hot gas atoms being heated by the ultraviolet <a href="http://commons.wikimedia.org/wiki/Light" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Light">light</a> from the central white dwarf. A collection of clumps fill the central part of the nebula, and <a class="mw-redirect" href="http://commons.wikimedia.org/wiki/Red" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Red">red</a>-coloured radial spokes extend well beyond. Astronomers think these features represent molecules of <a href="http://commons.wikimedia.org/wiki/Hydrogen" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hydrogen">hydrogen</a> gas, mixed with traces of heavier elements</span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/e/e3/TwoDumbbells.JPG" height="400" width="335" /><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Dumbbell#mediaviewer/File:TwoDumbbells.JPG">http://en.wikipedia.org/wiki/Dumbbell#mediaviewer/File:TwoDumbbells.JPG</a></span><br />
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/d/db/Halteres_from_ancient_Greece.JPG/1024px-Halteres_from_ancient_Greece.JPG" height="425" width="640" /><br />
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<span class="mw-mmv-title" original-title="File name" style="line-height: 24px; max-width: 60%; white-space: nowrap;"><span style="font-family: sans-serif;"><span style="background-color: #fbfbfb; color: #333333;">http://en.wi</span><span style="background-color: white;"><span style="color: #073763;">kipedia.org/wiki/Dumbbell#mediaviewer/File:Halteres_from_an<span style="font-size: 19px;">cient_Greece.JPG</span></span></span></span></span></div>
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<span class="mw-mmv-title" original-title="File name" style="background-color: white; font-size: 1.2em; max-width: 60%;"><span style="color: #073763;">Halteres from ancient Greece</span></span></div>
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<span class="mw-mmv-source-author mw-mmv-reduce-toolong" original-title="Author and source information" style="font-size: 0.8em;"><span class="mw-mmv-author" style="background-color: white;"><span style="color: #073763;"><a class="extiw" href="http://en.wikipedia.org/wiki/User:Portum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="en:User:Portum">Portum</a> (<a class="extiw" href="http://en.wikipedia.org/wiki/User_talk:Portum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="en:User talk:Portum">talk</a>). Original uploader was <a class="extiw" href="http://en.wikipedia.org/wiki/User:Portum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="en:User:Portum">Portum</a> at <a class="external text" href="http://en.wikipedia.org/" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;">en.wikipedia</a></span></span></span></div>
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Foi a primeira <a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa planetária">nebulosa planetária</a> a ser descoberta e o primeiro a visualizá-la foi o astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a>, em 12 de julho de 1764. Ele descreveu o objeto como uma nebulosa oval sem estrelas. O nome "haltere" foi dado por <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background: none; color: #0b0080; text-decoration: none;" title="John Herschel">John Herschel</a>, que o comparou-o a uma "marca de dois tiros próximos".<span class="reference" id="cite_ref-seds_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere#cite_note-seds-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span></div>
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A partir da <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>, tem-se a vista equatorial da nebulosa planetária, de forma semelhante à vista de outra nebulosa planetária, a<a href="http://pt.wikipedia.org/wiki/Pequena_Nebulosa_do_Haltere" style="background: none; color: #0b0080; text-decoration: none;" title="Pequena Nebulosa do Haltere">Pequena Nebulosa do Haltere</a> (Messier 76). Posicionando-se em um dos polos da nebulosa, seria possível visualizar sua forma de um anel, forma semelhante a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Anel" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa do Anel">nebulosa do Anel</a> (Messier 57).<span class="reference" id="cite_ref-seds_5-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere#cite_note-seds-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiB2wtoQgQCzX7jZvIWxLkba2XCJZbTzFYdD9Vt6mg99TRDX72XMUl3cRwenMH3Q2jOcBB6iRO0oqO3ejy_ibcuWsqZ23ZjrrLg0JEALGCcOEVktfCKBUf_F4PQXA4g5imwZjCxmvsNJ30/s1600/Messier27.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiB2wtoQgQCzX7jZvIWxLkba2XCJZbTzFYdD9Vt6mg99TRDX72XMUl3cRwenMH3Q2jOcBB6iRO0oqO3ejy_ibcuWsqZ23ZjrrLg0JEALGCcOEVktfCKBUf_F4PQXA4g5imwZjCxmvsNJ30/s1600/Messier27.jpg" height="480" width="640" /></a></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.399999618530273px;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere#mediaviewer/Ficheiro:Messier27.jpg">http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere#mediaviewer/Ficheiro:Messier27.jpg</a></span></span></div>
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<span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">Like many nearby planetary nebulae, <b>the Dumbbell contains knots</b>. Its central region is marked by a pattern of dark and bright cusped knots and their associated dark tails (see picture). The knots vary in appearance from symmetric objects with tails to rather irregular tail-less objects. Similarly to the </span><a href="http://en.wikipedia.org/wiki/Helix_Nebula" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Helix Nebula">Helix Nebula</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> and the </span><a href="http://en.wikipedia.org/wiki/Eskimo_Nebula" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Eskimo Nebula">Eskimo Nebula</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">, the heads of the knots have bright cusps which are local </span><a href="http://en.wikipedia.org/wiki/Photoionization" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Photoionization">photoionization</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> fronts.</span><sup class="reference" id="cite_ref-ODelletal2003_5-1" style="color: #252525; font-family: sans-serif; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Dumbbell_Nebula#cite_note-ODelletal2003-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[5]</a></sup></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Dumbbell_Nebula">http://en.wikipedia.org/wiki/Dumbbell_Nebula</a></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiIU3Qa8HRi436zzatsyjoMYPqNo69xR3f5efqJI_j_8ChbpmfxIVDpUCXh15HwFS6OE-Z-R9U8iJbaJtFfTzHg5cKzs1hsJX-kMjgTzszlS7PQlSDMFrNZHubpnMlxQaJdfrXjMVvccN8/s1600/M27_Knots.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiIU3Qa8HRi436zzatsyjoMYPqNo69xR3f5efqJI_j_8ChbpmfxIVDpUCXh15HwFS6OE-Z-R9U8iJbaJtFfTzHg5cKzs1hsJX-kMjgTzszlS7PQlSDMFrNZHubpnMlxQaJdfrXjMVvccN8/s1600/M27_Knots.jpg" /></a></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/6/6e/M27_Knots.jpg/220px-M27_Knots.jpg" height="381" width="640" /><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Dumbbell_Nebula#mediaviewer/File:M27_Knots.jpg">http://en.wikipedia.org/wiki/Dumbbell_Nebula#mediaviewer/File:M27_Knots.jpg</a></span><br />
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<span class="mw-mmv-title" original-title="File name" style="background-color: white; font-size: 1.2em; max-width: 60%;">M27 Knots</span></div>
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<span class="mw-mmv-source-author" original-title="Author and source information" style="background-color: white;"><span class="mw-mmv-author">C.R. O'Dell (Vanderbilt University)</span> - <span class="mw-mmv-source"><a class="external free" href="http://hubblesite.org/newscenter/archive/releases/2003/06/image/a" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://hubblesite.org/newscenter/archive/releases/2003/06/image/a</a> (<a class="external text" href="http://imgsrc.hubblesite.org/hu/db/2003/06/images/a/formats/full_jpg.jpg" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">direct link</a>)</span></span></div>
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A estrela central de M27 é uma <a href="http://pt.wikipedia.org/wiki/Estrela_an%C3%A3" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela anã">estrela anã</a> brilhante, de magnitude aparente 13,5, e é extremamente quente, azul, com <a href="http://pt.wikipedia.org/wiki/Temperatura" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Temperatura">temperatura</a>superficial de 85 000 <a href="http://pt.wikipedia.org/wiki/Kelvin" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Kelvin">K</a>, pertencente à <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Classificação estelar">classe espectral</a> O7, com uma provável companheira de magnitude aparente 17.<span class="reference" id="cite_ref-seds_5-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere#cite_note-seds-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span></div>
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Adotando-se um valor médio para sua distância em 1 200 anos-luz, a luminosidade intrínseca da nebulosa é cerca de 100 vezes mais do que a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Luminosidade_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Luminosidade solar">luminosidade solar</a> (-0,5 de<a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a>), embora a estrela geradora da nebulosa tenha apenas um terço da luminosidade solar e sua companheira apenas um centésimo, considerando-se o<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Espectro_visual" style="background: none; color: #0b0080; text-decoration: none;" title="Espectro visual">espectro visual</a>. A grande luminosidade da nebulosa deve-se a absorção radiação de alta energia da estrela central e na sua reemissão no espectro visível, sendo a maior parte emitida em apenas uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Linha_espectral" style="background: none; color: #0b0080; text-decoration: none;" title="Linha espectral">linha espectral</a> centrada no verde, conhecida como a linha 5007 Ångström, gerada pela dupla ionização do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Oxig%C3%AAnio" style="background: none; color: #0b0080; text-decoration: none;" title="Oxigênio">oxigênio</a>.<span class="reference" id="cite_ref-seds_5-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere#cite_note-seds-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span></div>
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Praticamente nos limites da nebulosa, existe uma <a href="http://pt.wikipedia.org/wiki/Estrela_vari%C3%A1vel" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela variável">estrela variável</a>, em correlações com a nebulosa, chamada variável de Goldilocks. Esta nebulosa planetária apresenta uma aparência de <a href="http://pt.wikipedia.org/wiki/Esferoide" style="background: none; color: #0b0080; text-decoration: none;" title="Esferoide">esferoide</a> dilatada e é visível da perspetiva terrestre ao longo do plano de seu <a href="http://pt.wikipedia.org/wiki/Linha_do_equador" style="background: none; color: #0b0080; text-decoration: none;" title="Linha do equador">equador</a>.<span class="reference" id="cite_ref-seds_5-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere#cite_note-seds-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span></div>
<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere">http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere</a></span><br />
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<span style="color: #660000; font-size: large;"><b style="background-color: white; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">NGC 6885</b><span style="background-color: white; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">, also </span><b style="background-color: white; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"><a href="http://en.wikipedia.org/wiki/Caldwell_catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Caldwell catalogue">Caldwell</a> 37</b></span><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">, is an </span><a href="http://en.wikipedia.org/wiki/Open_cluster" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Open cluster">open cluster</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> in the constellation </span><a href="http://en.wikipedia.org/wiki/Vulpecula" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Vulpecula">Vulpecula</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. It shines at magnitude +5.7/+8.1.</span><sup class="reference" id="cite_ref-earth_1-0" style="background-color: white; color: #252525; font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/NGC_6885#cite_note-earth-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> Its celestial coordinates are RA 20</span><sup style="background-color: white; color: #252525; font-family: sans-serif; line-height: 1; text-align: start;">h</sup><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> 12.0</span><sup style="background-color: white; color: #252525; font-family: sans-serif; line-height: 1; text-align: start;">m</sup><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">, dec +26° 29′. It surrounds a naked-eye O or B-class star, and is located near </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Messier_27" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Messier 27">M27</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> (Dumbbell nebula), the nebula </span><a class="new" href="http://en.wikipedia.org/w/index.php?title=IC_4954&action=edit&redlink=1" style="background: none rgb(255, 255, 255); color: #a55858; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="IC 4954 (page does not exist)">IC 4954</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">, and open clusters </span><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_6882&action=edit&redlink=1" style="background: none rgb(255, 255, 255); color: #a55858; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="NGC 6882 (page does not exist)">NGC 6882</a><sup class="reference" id="cite_ref-earth_1-1" style="background-color: white; color: #252525; font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/NGC_6885#cite_note-earth-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> and </span><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_6940&action=edit&redlink=1" style="background: none rgb(255, 255, 255); color: #a55858; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="NGC 6940 (page does not exist)">NGC 6940</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. It is 7'/18' across.</span><sup class="reference" id="cite_ref-earth_1-2" style="background-color: white; color: #252525; font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/NGC_6885#cite_note-earth-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/NGC_6885">http://en.wikipedia.org/wiki/NGC_6885</a></span><br />
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">NGC 6885</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">, também chamado de </span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">Caldwell 37</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">, é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado estelar aberto</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/Vulpecula" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Vulpecula">Vulpecula</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. Ele possui diversas </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Estrela">estrelas</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> azuis de </span><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Classificação estelar">classe espectral</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> O ou B</span><br />
<span style="background-color: white; line-height: 22.399999618530273px; text-align: start;"><span style="color: #252525; font-family: sans-serif;">http://pt.wikipedia.org/wiki/NGC_6885</span></span><br />
<span style="background-color: white; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"><span style="color: #252525; font-family: sans-serif;"><br /></span></span><span style="background-color: white; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"><span style="color: #252525; font-family: sans-serif;"><br /></span></span><img src="http://upload.wikimedia.org/wikipedia/commons/1/16/NGC_6885.png" /><br />
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<span style="background-color: white; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"><span style="color: #252525; font-family: sans-serif;">http://pt.wikipedia.org/wiki/NGC_6885#mediaviewer/Ficheiro:NGC_6885.png</span></span></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="background-color: white; font-size: 1.2em; max-width: 60%;">NGC 6885</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span class="mw-mmv-author"><a href="http://commons.wikimedia.org/wiki/User:Roberto_Mura" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="User:Roberto Mura">Roberto Mura</a></span> - <span class="mw-mmv-source"><span class="int-own-work">Obra do próprio</span></span></span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span class="mw-mmv-source"><span class="int-own-work"><br /></span></span></span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span class="mw-mmv-source"><span class="int-own-work"><br /></span></span></span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span class="mw-mmv-source"><span class="int-own-work"><br /></span></span></span></div>
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<h1>
<span style="color: #660000; font-size: large; font-weight: normal;">Brocchi's Cluster, Collinder 399</span></h1>
<i><a href="http://messier.seds.org/cluster.html">Open Cluster</a> Collinder 399</i> in <a href="http://messier.seds.org/map/Vul.html">Vulpecula</a>Brocchi's Cluster; Al Sufi's Cluster; The Coathanger Cluster</center>
<div style="text-align: start;">
<a href="http://messier.seds.org/Pics/Ngc/cr399.jpg"><img align="right" alt="[Cr 399, Credner/Kohle]" border="0" src="http://messier.seds.org/Pics/Ngc/cr399.jpg" /></a></div>
<table border="2" cellpadding="5" cellspacing="0"><tbody>
<tr><th align="left"><span style="font-weight: normal;">Right Ascension</span></th><td align="center">19 : 25.4 (h:m)</td></tr>
<tr><th align="left"><span style="font-weight: normal;">Declination</span></th><td align="center">+20 : 11 (deg:m)</td></tr>
<tr><th align="left"><span style="font-weight: normal;">Distance</span></th><td align="center">0.42 (kly)</td></tr>
<tr><th align="left"><span style="font-weight: normal;">Visual Brightness</span></th><td align="center">3.6 (mag)</td></tr>
<tr><th align="left"><span style="font-weight: normal;">Apparent Dimension</span></th><td align="center">60 (arc min)</td></tr>
</tbody></table>
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Discovered before 964 AD by Al Sufi.</div>
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<div style="text-align: start;">
This cluster of about 40 stars was discovered by <a href="http://messier.seds.org/xtra/Bios/alsufi.html">Al Sufi</a> and described in 964 AD. It was independently rediscovered by <a href="http://messier.seds.org/xtra/similar/hodierna.html">Hodierna</a>. Messier, the Herschels and the NGC did not assign it a number, probably because of the cluster's size: Even at moderate power, it doesn't match in one field of view, and is best seen in a good pair of binoculars. Also, its appearance suggests it might be an asterism only.</div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span class="mw-mmv-source"><span class="int-own-work"></span></span></span></div>
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This object is sometimes named <i>Brocchi's Cluster</i> after American amateur astronomer D.F. Brocchi, who created a map of it in the 1920s, for calibrating photometers. It was included in <a href="http://messier.seds.org/xtra/supp/cats.html#Cr">Per Collinder's 1931 catalog</a> of open clusters.</div>
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<span style="font-size: large;"><br /></span></div>
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<a href="http://messier.seds.org/xtra/ngc/brocchi.html">http://messier.seds.org/xtra/ngc/brocchi.html</a></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgbD-LwNr2RXzQEaQiezYWmnD0wKyl-gNjLWfHMF56-jvdA8TMmII12By4Pt_YjI0ySunBJ8R2DLvuKWd75fmtQD1CTGTczvfaRe_On37P6gz0nJ_XAmtAk9tFF3730ehd7KUlnx9UlfRo/s1600/urania14+(1).jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgbD-LwNr2RXzQEaQiezYWmnD0wKyl-gNjLWfHMF56-jvdA8TMmII12By4Pt_YjI0ySunBJ8R2DLvuKWd75fmtQD1CTGTczvfaRe_On37P6gz0nJ_XAmtAk9tFF3730ehd7KUlnx9UlfRo/s1600/urania14+(1).jpg" height="445" width="640" /></a></div>
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<a href="http://www.ianridpath.com/atlases/urania/urania14.jpg">http://www.ianridpath.com/atlases/urania/urania14.jpg</a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas </span></div>
<div align="center" style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 16.8pt; margin: 0cm;">
<span style="font-family: Arial, Helvetica, sans-serif;">- AS CONSTELAÇÕES -</span></div>
<div align="center" style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 16.8pt; margin: 0cm;">
<span style="font-family: Arial, Helvetica, sans-serif;"> são como janelas que se abrem para a infinitude do universo</span></div>
<div align="center" style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 16.8pt; margin: 0cm;">
<span style="font-family: Arial, Helvetica, sans-serif;"> e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, </span></div>
<div align="center" style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 16.8pt; margin: 0cm;">
<span style="font-family: Arial, Helvetica, sans-serif;">entre o céu e a terra..., bem como percebendo que o caos, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">vagarosamente, </span></div>
<div align="center" style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 16.8pt; margin: 0cm;">
<span style="font-family: Arial, Helvetica, sans-serif;">vai se tornando Cosmos </span></div>
<div align="center" style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 16.8pt; margin: 0cm;">
<span style="font-family: Arial, Helvetica, sans-serif;">e este por nossa mente sendo conscientizado.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,<o:p></o:p></span></div>
<div align="center" style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 16.8pt; margin: 0cm;">
<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">Janine Milward<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div align="center" style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 16.8pt; margin: 0cm;">
<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">VISITE MINHA PÁGINA<o:p></o:p></span></div>
<div align="center" style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 16.8pt; margin: 0cm;">
<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">DA TERRA AO CÉU E AO INFINITO<o:p></o:p></span></div>
<div align="center" style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 16.8pt; margin: 0cm;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #274e13;">http://daterraaoceueaoinfinito.blogspot.com.br/</span></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-18651831027048694442013-08-20T08:44:00.005-07:002017-04-09T10:52:47.341-07:00PISCES VOLANS, O PEIXE VOADOR<div align="center" class="MsoNormal" style="text-align: center;">
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span>
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<span style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px; line-height: 14.25pt;"></span><br />
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<span style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px; line-height: 14.25pt;"><br class="Apple-interchange-newline" />Olá!</span></div>
</div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 14.25pt;"></span><br /></div>
<div style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px;">
<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 14.25pt;">O Peixe Voador foi primeiramente conhecido como Piscis Volans</span></div>
<div style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px;">
<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 14.25pt;">e mais tarde simplesmente como Volans</span></div>
<div style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px;">
<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 14.25pt;">e sua primeira apresentação num atlas celeste</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 14.25pt;"></span><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 14.25pt;"></span></div>
<div style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px;">
<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 14.25pt;">aconteceu através Bayer em sua Uranometria, em 1603.</span></div>
<span style="font-family: arial, tahoma, helvetica, freesans, sans-serif; line-height: 14.25pt;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 14.25pt;"></span></span><div style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px;">
</div>
<div style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px;">
<br /></div>
<div style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px;">
<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 14.25pt;">É interessante percebermos que o Peixe Voador acompanha o Navio Argo</span></div>
<div style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px;">
<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 14.25pt;">(assim como também a Pomba de Nóe, Columba)</span></div>
<div style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px;">
<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 14.25pt;">e também nada e voa bem próximo ao peixe Dourado, Dorado.</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 14.25pt;"></span><br /></div>
<div style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px;">
<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 14.25pt;">A bem da verdade, </span></div>
<div style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px;">
<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 14.25pt;">o Peixe Voador serve de comida tanto para Dorado</span></div>
<div style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px;">
<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 14.25pt;">(que vem até a tona para pescá-lo!)</span></div>
<div style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px;">
<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 14.25pt;"></span><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 14.25pt;"></span></div>
<div style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px;">
<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 14.25pt;">como para os tripulantes do Navio Argos</span></div>
<span style="font-family: arial, tahoma, helvetica, freesans, sans-serif; line-height: 14.25pt;"><div>
<span style="color: #073763; font-size: 16px; line-height: 14.25pt;">- por conseguir voar tão alto para escapar do peixe devorador....</span><span style="color: #073763; font-size: 16px; line-height: 14.25pt;"> até alcançar a Quilha, Carina </span><span style="color: #073763; font-size: 16px; line-height: 14.25pt;">(onde os marinheiros avidamente o agarram....)</span><span style="color: #073763; font-size: 16px; line-height: 14.25pt;">com cuja </span></div>
<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 14.25pt;"></span></span><span style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px; line-height: normal;"><div style="text-align: left;">
(mais tarde desmembrada de Argo Navis, o Navio)</div>
</span><span style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px; line-height: normal;"><div style="text-align: left;">
parece quase ser adjuntado</div>
</span><span style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px; line-height: normal;"><div style="text-align: left;">
e por o Peixe Voador ser bem encontrado</div>
</span><span style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px; line-height: normal;"><div style="text-align: left;">
situando-se entre as estrelas Beta (Miaplacidus) e Epsilon Carinae (Avior).</div>
</span><span style="background-color: white; color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px;"><div style="text-align: left;">
<span style="color: #073763; font-family: "arial" , sans-serif;"><br /></span></div>
</span><span style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px; line-height: normal;"><div style="text-align: left;">
O Peixe Voador, Volans,<br />
encontra-se também em excelente vizinhança,</div>
</span><span style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px; line-height: normal;"><div style="text-align: left;">
quer dizer,</div>
</span><span style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px; line-height: normal;"><div style="text-align: left;">
situando-se bem entre aquilo que poderia ser considerado </div>
</span><span style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px; line-height: normal;"><div style="text-align: left;">
como a Proa de Argo Navis, o Navio</div>
</span><span style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px; line-height: normal;"><div style="text-align: left;">
....., mas que desfaz-se em nuvens de estrelas e mais estrelas </div>
</span><span style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px; line-height: normal;"><div style="text-align: left;">
e mais estrelas esfumaçadas </div>
</span><span style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px; line-height: normal;"><div style="text-align: left;">
que permeiam a fantástica Nebulosa Carina<br />
bem como As Pleiades do Sul....</div>
</span><span style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px; line-height: normal;"><div style="text-align: left;">
e a maravilhosa Grande Nuvem de Magalhães ...</div>
</span><span style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px; line-height: normal;"><div style="text-align: left;">
em cuja direção encontram-se o peixe Dorado<br />
e a Montanha da Mesa, Mons Mensa</div>
</span><span style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px; line-height: normal;"><div style="text-align: left;">
(sendo que em Dourado, o caçador de Volans,<br />
é acolhida a belíssima Nebulosa da Tarântula!).</div>
</span><span style="background-color: white; color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px;"><div style="text-align: left;">
<span style="color: #073763; font-family: "arial" , sans-serif;"><br /></span></div>
</span><span style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px; line-height: normal;"><div style="text-align: left;">
Enfim,<br />
nos mares onde o Peixe Voador nada e voa</div>
</span><span style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px; line-height: normal;"><div style="text-align: left;">
de tédio não se morre!</div>
</span><span style="background-color: white; color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px;"><div style="text-align: left;">
<span style="color: #073763; font-family: "arial" , sans-serif;"><br /></span></div>
</span><span style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px; line-height: normal;"><div style="text-align: left;">
Com um abraço estrelado,</div>
</span><span style="color: #073763; font-family: arial, tahoma, helvetica, freesans, sans-serif; font-size: 16px; line-height: normal;"><div style="text-align: left;">
Janine Milward<br />
<br />
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="font-size: medium;"><span style="background-color: #f9f9f9; color: #252525; font-family: sans-serif;">The "Southern Birds", </span><a class="extiw" href="https://en.wikipedia.org/wiki/Pavo_(constellation)" style="background: none rgb(249, 249, 249); color: #663366; font-family: sans-serif; text-decoration-line: none;" title="en:Pavo (constellation)">Pavo</a><span style="background-color: #f9f9f9; color: #252525; font-family: sans-serif;">, </span><a class="extiw" href="https://en.wikipedia.org/wiki/Phoenix_(constellation)" style="background: none rgb(249, 249, 249); color: #663366; font-family: sans-serif; text-decoration-line: none;" title="en:Phoenix (constellation)">Phoenix</a><span style="background-color: #f9f9f9; color: #252525; font-family: sans-serif;">, </span><a class="extiw" href="https://en.wikipedia.org/wiki/Grus_(constellation)" style="background: none rgb(249, 249, 249); color: #663366; font-family: sans-serif; text-decoration-line: none;" title="en:Grus (constellation)">Grus</a><span style="background-color: #f9f9f9; color: #252525; font-family: sans-serif;">, and </span><a class="extiw" href="https://en.wikipedia.org/wiki/Tucana_(constellation)" style="background: none rgb(249, 249, 249); color: #663366; font-family: sans-serif; text-decoration-line: none;" title="en:Tucana (constellation)">Tucana</a><span style="background-color: #f9f9f9; color: #252525; font-family: sans-serif;"> from </span><a class="extiw" href="https://en.wikipedia.org/wiki/Johann_Bayer" style="background: none rgb(249, 249, 249); color: #663366; font-family: sans-serif; text-decoration-line: none;" title="en:Johann Bayer">Johann Bayer</a><span style="background-color: #f9f9f9; color: #252525; font-family: sans-serif;">'s </span><i style="background-color: #f9f9f9; color: #252525; font-family: sans-serif;"><a class="extiw" href="https://en.wikipedia.org/wiki/Uranometria" style="background: none; color: #663366; text-decoration-line: none;" title="en:Uranometria">Uranometria</a></i><span style="background-color: #f9f9f9; color: #252525; font-family: sans-serif;"> of 1603, the first celestial atlas to include the southern constellations. </span><a class="extiw" href="https://en.wikipedia.org/wiki/Indus_(constellation)" style="background: none rgb(249, 249, 249); color: #663366; font-family: sans-serif; text-decoration-line: none;" title="en:Indus (constellation)">Indus</a><span style="background-color: #f9f9f9; color: #252525; font-family: sans-serif;"> and </span><a class="extiw" href="https://en.wikipedia.org/wiki/Hydrus_(constellation)" style="background: none rgb(249, 249, 249); color: #663366; font-family: sans-serif; text-decoration-line: none;" title="en:Hydrus (constellation)">Hydrus</a><span style="background-color: #f9f9f9; color: #252525; font-family: sans-serif;"> also appear.</span></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><img alt="Resultado de imagem para Johann Bayer" src="https://upload.wikimedia.org/wikipedia/commons/thumb/b/b5/Johann_Bayer_-_Uraniometria_-_Southern_Birds.jpg/838px-Johann_Bayer_-_Uraniometria_-_Southern_Birds.jpg" style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">https://upload.wikimedia.org/wikipedia/commons/thumb/b/b5/<b><span style="font-size: medium;">Johann_Bayer_-_Uraniometria_-_Southern_Birds.</span></b>jpg/838px-Johann_Bayer_-_Uraniometria_-_Southern_Birds.jpg</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Caro Leitor,</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">É interessante percebermos o fato de que</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">muitas das constelações mais ao sul</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">foram figuradas e nomeadas </span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;">nos Séculos XVI (bem ao final), XVII e XVIII.</span><br />
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>Petrus Plancius</b></span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;"><b><br /></b></span><b style="color: #252525; font-family: sans-serif;">Petrus Plancius</b><span style="color: #252525; font-family: sans-serif;"> (1552 – May 15, 1622) was a </span><a href="https://en.wikipedia.org/wiki/Flanders" style="background-image: none; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Flanders">Flemish</a><span style="color: #252525; font-family: sans-serif;"> </span><a href="https://en.wikipedia.org/wiki/Astronomer" style="background-image: none; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Astronomer">astronomer</a><span style="color: #252525; font-family: sans-serif;">, </span><a href="https://en.wikipedia.org/wiki/Cartography" style="background-image: none; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Cartography">cartographer</a><span style="color: #252525; font-family: sans-serif;"> and </span><a class="mw-redirect" href="https://en.wikipedia.org/wiki/Clergyman" style="background-image: none; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Clergyman">clergyman</a><span style="color: #252525; font-family: sans-serif;">. He was born as </span><b style="color: #252525; font-family: sans-serif;">Pieter Platevoet</b><span style="color: #252525; font-family: sans-serif;"> in </span><a href="https://en.wikipedia.org/wiki/Dranouter" style="background-image: none; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Dranouter">Dranouter</a><span style="color: #252525; font-family: sans-serif;">, now in </span><a href="https://en.wikipedia.org/wiki/Heuvelland" style="background-image: none; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Heuvelland">Heuvelland</a><span style="color: #252525; font-family: sans-serif;">, </span><a href="https://en.wikipedia.org/wiki/West_Flanders" style="background-image: none; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="West Flanders">West Flanders</a><span style="color: #252525; font-family: sans-serif;">. He studied </span><a href="https://en.wikipedia.org/wiki/Theology" style="background-image: none; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Theology">theology</a><span style="color: #252525; font-family: sans-serif;"> in Germany and England. At the age of 24 he became a </span><a class="mw-redirect" href="https://en.wikipedia.org/wiki/Religious_minister" style="background-image: none; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Religious minister">minister</a><span style="color: #252525; font-family: sans-serif;"> in the </span><a href="https://en.wikipedia.org/wiki/Dutch_Reformed_Church" style="background-image: none; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Dutch Reformed Church">Dutch Reformed Church</a><span style="color: #252525; font-family: sans-serif;">.</span><br />
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In 1589 Plancius collaborated with the Amsterdam cartographer <a href="https://en.wikipedia.org/wiki/Jacob_Floris_van_Langren" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Jacob Floris van Langren">Jacob Floris van Langren</a> on a 32.5-cm celestial globe, which, using the sparse information available about southern celestial features, for the first time depicted: <a href="https://en.wikipedia.org/wiki/Crux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Crux">Crux</a> the southern cross, <a href="https://en.wikipedia.org/wiki/Triangulum_Australe" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Triangulum Australe">Triangulum Australe</a> the southern triangle, and the <a href="https://en.wikipedia.org/wiki/Ferdinand_Magellan" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Ferdinand Magellan">Magellanic Clouds</a>, <a href="https://en.wikipedia.org/wiki/Large_Magellanic_Cloud" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Large Magellanic Cloud">Nubecula Major</a> and <a href="https://en.wikipedia.org/wiki/Small_Magellanic_Cloud" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Small Magellanic Cloud">Minor</a>.</div>
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In 1595 Plancius asked <a href="https://en.wikipedia.org/wiki/Pieter_Dirkszoon_Keyser" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Pieter Dirkszoon Keyser">Pieter Dirkszoon Keyser</a>, the chief pilot on the <i>Hollandia</i>, to make observations to fill in the blank area around the south celestial pole on European maps of the southern sky. Keyser died in <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Java_(island)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Java (island)">Java</a> the following year – the expedition had many casualties – but his catalogue of 135 <a href="https://en.wikipedia.org/wiki/Star" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Star">stars</a>,<sup class="reference" id="cite_ref-knobel_dehoutman_3-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Petrus_Plancius#cite_note-knobel_dehoutman-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;">[3]</a></sup> probably measured up with the help of explorer-colleague <a href="https://en.wikipedia.org/wiki/Frederick_de_Houtman" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Frederick de Houtman">Frederick de Houtman</a>,<sup class="reference" id="cite_ref-ridpath_ch1_c_4-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Petrus_Plancius#cite_note-ridpath_ch1_c-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;">[4]</a></sup> was delivered to Plancius. These stars appear as 12 new southern <a href="https://en.wikipedia.org/wiki/Constellation" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Constellation">constellations</a>,<sup class="reference" id="cite_ref-ridpath_ch1_c_4-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Petrus_Plancius#cite_note-ridpath_ch1_c-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;">[4]</a></sup> on a 35-cm celestial globe designed by Plancius in late 1597 (or early 1598) and produced in collaboration with the Amsterdam cartographer <a href="https://en.wikipedia.org/wiki/Jodocus_Hondius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Jodocus Hondius">Jodocus Hondius the Elder</a>. The 12 new constellations (mostly referring to animals and subjects described in natural history books and travellers' journals of his day) are <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Apis_(constellation)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Apis (constellation)">Apis</a> the Bee (later changed to <a href="https://en.wikipedia.org/wiki/Musca" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Musca">Musca</a> by <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Lacaille">Lacaille</a>), <b><a href="https://en.wikipedia.org/wiki/Apus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Apus">Apus</a> the Bird of Paradise</b>, <a href="https://en.wikipedia.org/wiki/Chamaeleon" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Chamaeleon">Chamaeleon</a>, <a href="https://en.wikipedia.org/wiki/Dorado" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Dorado">Dorado</a> the Goldfish (or Swordfish), <b><a href="https://en.wikipedia.org/wiki/Grus_(constellation)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Grus (constellation)">Grus</a> the Crane</b>, <a href="https://en.wikipedia.org/wiki/Hydrus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Hydrus">Hydrus</a>the Small Water Snake, <a href="https://en.wikipedia.org/wiki/Indus_(constellation)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Indus (constellation)">Indus</a> the Indian,<b> <a href="https://en.wikipedia.org/wiki/Pavo_(constellation)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Pavo (constellation)">Pavo</a> the Peacock, <a href="https://en.wikipedia.org/wiki/Phoenix_(constellation)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Phoenix (constellation)">Phoenix</a></b>, <a href="https://en.wikipedia.org/wiki/Triangulum_Australe" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Triangulum Australe">Triangulum Australe</a> the Southern Triangle, <b><a href="https://en.wikipedia.org/wiki/Tucana" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Tucana">Tucana</a> the Toucan, and <a href="https://en.wikipedia.org/wiki/Volans" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Volans">Volans</a> the Flying Fish</b>. (The Southern Triangle and Southern Cross were reported as asterisms by earlier navigators and appear on earlier charts,<sup class="reference" id="cite_ref-Dekker_5-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Petrus_Plancius#cite_note-Dekker-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;">[5]</a></sup> but the globe of 1598 is the first surviving source that plots their locations reasonably accurately.) Also notable is the inclusion of Achernar as Alpha Eridani.</div>
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These constellations, together with the constellation <a href="https://en.wikipedia.org/wiki/Columba_(constellation)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Columba (constellation)"><b>Columba</b></a> illustrated by Plancius on his large wall map of the world of 1592, were then incorporated in 1603 by <a href="https://en.wikipedia.org/wiki/Johann_Bayer" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Johann Bayer">Johann Bayer</a> in his sky atlas, the <i><a href="https://en.wikipedia.org/wiki/Uranometria" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Uranometria">Uranometria</a></i>.</div>
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<span style="color: #252525; font-family: sans-serif;"><a href="https://en.wikipedia.org/wiki/Petrus_Plancius" style="color: #274e13; text-decoration-line: none;">https://en.wikipedia.org/wiki/Petrus_Plancius</a></span></div>
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<img src="http://www.atlascoelestis.com/globo_completo.jpg" height="396" style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="400" /></div>
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<span style="color: #252525; font-family: sans-serif;"><a href="http://www.atlascoelestis.com/desu%20Plancius.htm" style="color: #274e13; text-decoration-line: none;">http://www.atlascoelestis.com/desu%20Plancius.htm</a></span></div>
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<span style="font-family: "arial" , sans-serif;"><b>Johann Bayer</b></span><span style="font-family: "arial" , sans-serif; font-size: 11pt;">, 1603, astrônomo. Obra: Uranometria. </span></div>
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<span style="font-family: "arial" , sans-serif; font-size: 11pt;">Relaciona 60 constelações, incluindo as circumpolares Sul, cuja nomenclatura conclui e unifica. </span></div>
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<span style="font-family: "arial" , sans-serif; font-size: 11pt;">Acrescenta 12 constelações.<o:p></o:p></span></div>
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<span style="font-family: "arial" , sans-serif; font-size: 11pt;"><b>Ave-do-Paraíso</b>, Camaleão, Dourado, <b>Grou</b>, Hidra Macho, Índio, Mosca, <b>Pavão, Fênix</b>, Triângulo Austral, <b>Tucano, Peixe-Voador<o:p></o:p></b></span></div>
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<span style="font-family: "arial" , sans-serif; font-size: 11pt;"><b>??? Jacob Bartsch</b></span><span style="font-family: "arial" , sans-serif; font-size: 11pt;">, 1624. </span><span lang="ES-TRAD" style="font-family: "arial" , sans-serif; font-size: 11pt;"><b>Pomba ??</b></span><br />
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<span lang="ES-TRAD"><span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="font-family: sans-serif; font-size: 14px;"><b><span style="color: #660000;">Bayer</span></b><span style="color: #252525;"> é mais famoso pelo seu </span></span><a class="mw-redirect" href="https://pt.wikipedia.org/wiki/Atlas_estelar" style="background-image: none; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Atlas estelar">atlas estelar</a><span style="color: #252525; font-family: sans-serif; font-size: 14px;"> </span><i style="color: #252525; font-family: sans-serif;"><a href="https://pt.wikipedia.org/wiki/Uranometria" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Uranometria">Uranometria</a></i><span style="color: #252525; font-family: sans-serif; font-size: 14px;">, publicado em </span><a href="https://pt.wikipedia.org/wiki/1603" style="background-image: none; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="1603">1603</a><span style="color: #252525; font-family: sans-serif; font-size: 14px;"> e que foi o primeiro </span><a href="https://pt.wikipedia.org/wiki/Atlas_(cartografia)" style="background-image: none; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Atlas (cartografia)">atlas</a><span style="color: #252525; font-family: sans-serif; font-size: 14px;"> a cobrir toda a </span><a href="https://pt.wikipedia.org/wiki/Esfera_celeste" style="background-image: none; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Esfera celeste">esfera celeste</a><span style="color: #252525; font-family: sans-serif; font-size: 14px;">. Este trabalho introduziu um novo sistema para designar as estrelas, usando a notação grega e latina, que se tornou conhecido com nomenclatura, ou </span><a href="https://pt.wikipedia.org/wiki/Designa%C3%A7%C3%A3o_de_Bayer" style="background-image: none; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Designação de Bayer">designação, de Bayer</a><span style="color: #252525; font-family: sans-serif; font-size: 14px;">. A maioria das notações atribuídas por Bayer e por astrónomos posteriores que adoptaram o seu sistema permanece em uso até aos dias de hoje.</span></span></span></div>
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<span lang="ES-TRAD"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #252525; font-family: sans-serif; font-size: 14px;"><a href="https://pt.wikipedia.org/wiki/Johann_Bayer" style="color: #274e13; text-decoration-line: none;">https://pt.wikipedia.org/wiki/Johann_Bayer</a></span></span></span></div>
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<img height="320" src="https://upload.wikimedia.org/wikipedia/commons/thumb/1/16/Uranometria_titlepage.jpg/200px-Uranometria_titlepage.jpg" style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="223" /></div>
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<a href="https://pt.wikipedia.org/wiki/Uranometria#/media/File:Uranometria_titlepage.jpg" style="color: #274e13; text-decoration-line: none;">https://pt.wikipedia.org/wiki/Uranometria#/media/File:Uranometria_titlepage.jpg</a></div>
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E vamos encontrar</div>
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Hevelius, Royer e La Caille </div>
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nomeando e reafirmando<br />
várias outras constelações,</div>
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algumas mais ao sul e outras não:</div>
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<span style="font-family: "arial" , sans-serif;"><span style="font-size: small;"><b>Hevelius</b></span></span><span style="font-family: "arial" , sans-serif; font-size: 11pt;">, 1690, astrônomo amador, selenógrafo. Obra: Sete Cartas Celestes. </span></div>
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<span style="font-family: "arial" , sans-serif; font-size: 11pt;">Dá nome a 9 constelações:<o:p></o:p></span></div>
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<span style="font-family: "arial" , sans-serif; font-size: 11pt;">Girafa, Cães de Caça, Lagarto, Leão Menor, Lince, Unicórnio, Escudo, Sextante, Raposa<o:p></o:p></span></div>
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<span style="font-family: "arial" , sans-serif;"><b>Royer</b></span><span style="font-family: "arial" , sans-serif; font-size: 11pt;">, 1697, navegante francês. Obra: Carta Celeste. Desmembra a Cruz Australis da constelação do Centauro. Cruzeiro do Sul<o:p></o:p></span></div>
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<span lang="ES-TRAD" style="font-family: "arial" , sans-serif;"><b>La Caille</b></span><span lang="ES-TRAD" style="font-family: "arial" , sans-serif; font-size: 11pt;">, 1752, astrônomo. </span><span style="font-family: "arial" , sans-serif; font-size: 11pt;">Obras: Memórias e Céu Estrelado. </span></div>
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<span style="font-family: "arial" , sans-serif; font-size: 11pt;">Introduz 14 novas constelações:</span></div>
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<span style="font-family: "arial" , sans-serif; font-size: 11pt;"> Máquina Pneumática, Buril, Compasso, Forno, Relógio, Mesa, Microscópio, Esquadro, Oitante, Pintor, Bússula, Retículo, Escultor, Telescópio<o:p></o:p></span></div>
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<span style="font-family: "arial" , sans-serif; font-size: 11pt;">E divide a extensa constelação ptolomaica Argo, o Navio, em Carina, Puppis e Vela.<o:p></o:p></span></div>
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<span style="font-family: "arial" , sans-serif; font-size: 11pt;">Quilha, Popa, Vela<o:p></o:p></span></div>
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<span style="background-color: white;"><span style="font-size: small;">O que são peixes-voadores? Como eles voam?</span></span><iframe allowtransparency="true" class="twitter-share-button twitter-tweet-button twitter-share-button twitter-count-horizontal" data-twttr-rendered="true" frameborder="0" id="twitter-widget-0" scrolling="no" src="http://platform.twitter.com/widgets/tweet_button.b169aa788731255dd55f1bb243b660e1.pt.html#_=1431955793105&count=horizontal&dnt=false&id=twitter-widget-0&lang=pt&original_referer=http%3A%2F%2Fmundoestranho.abril.com.br%2Fmateria%2Fo-que-sao-peixesvoadores-como-eles-voam&size=m&text=O%20que%20s%C3%A3o%20peixes-voadores%3F%20Como%20eles%20voam%3F%20-%20Mundo%20Estranho&url=http%3A%2F%2Fmundoestranho.abril.com.br%2Fmateria%2Fo-que-sao-peixesvoadores-como-eles-voam&via=mundoestranho" style="font-size: medium; height: 20px; line-height: normal; margin: 0px; padding: 0px; position: static; visibility: visible; widows: auto; width: 88px;" title="Twitter Tweet Button"></iframe></h1>
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<span style="background-color: white;">Esses curiosos animais compreendem cerca de 40 espécies de peixes carnívoros e herbívoros da família Exocoetidae, encontrados apenas em mares de águas mornas. Todos eles têm o corpo fino e crescem pouco, atingindo no máximo 45 centímetros. Ao contrário do que se possa imaginar, esses bichos não voam como as aves, batendo asas para cima e para baixo. O que eles fazem, na verdade, é ganhar impulso para dar grandes saltos. Depois, abrem suas barbatanas para planar, ficando no ar por até 15 segundos. No vôo, o mais comum é que as espécies cubram uma distância de, no máximo, 180 metros. Mas em saltos múltiplos os tipos recordistas conseguem planar por 400 metros. Em geral, os peixes utilizam esse recurso para fugir de seus predadores, principalmente tubarões, atuns e golfinhos. O Brasil não tem os tipos tradicionais de peixes-voadores, mas as águas amazônicas abrigam uma espécie parecida: é o peixe-machadinha, que faz vôos bem mais curtos, de 1,50 metro de distância.</span></div>
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<strong style="display: block; font-family: 'lucida grande', 'lucida sans unicode', verdana, sans-serif; margin: 0px; padding: 0px;"><span style="background-color: white;">Acrobacia aquática</span></strong><em style="display: block; font-family: 'lucida grande', 'lucida sans unicode', verdana, sans-serif; margin: 0px; padding: 0px;"><span style="background-color: white;">A decolagem atinge 1 metro de altura e pode se prolongar por 180 metros</span></em><br />
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<span style="background-color: white;">1. O vôo do peixe-voador é um recurso para escapar de predadores. Ao ser perseguido por um peixe maior, a espécie cruza o mar velozmente com as barbatanas coladas ao corpo, nada para cima e se prepara para voar</span></div>
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<span style="background-color: white;">2. Ao atingir a superfície, o peixe dá um impulso final, batendo freneticamente o rabo na água. Quando o empurrão já é suficiente, ele levanta o rabo e decola</span></div>
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<span style="background-color: white;">3. No ar, o peixe abre as barbatanas, obtendo a sustentação necessária para planar por cima da água. Ele consegue realizar sua decolagem em uma inclinação de 15 graus em relação à superfície líquida</span></div>
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<span style="background-color: white;">4. Durante sua aventura aérea, o peixe-voador atinge 1 metro de altura, chegando a voar por até 180 metros em um único vôo ou 400 metros em vôos múltiplos. Mas os passeios são rápidos: costumam durar, em média, de 2 a 15 segundos</span></div>
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<span style="font-size: 14px; line-height: 24px;"><span style="font-family: "lucida grande" , "lucida sans unicode" , "verdana" , sans-serif;"><a href="http://mundoestranho.abril.com.br/materia/o-que-sao-peixesvoadores-como-eles-voam" style="color: #274e13; text-decoration-line: none;">http://mundoestranho.abril.com.br/materia/o-que-sao-peixesvoadores-como-eles-voam</a></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">"Exvol u0". Licenciado sob Domínio público, via Wikimedia Commons - http://commons.wikimedia.org/wiki/File:Exvol_u0.gif#/media/File:Exvol_u0.gif</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiGsBZSKTCb4_nufbFtjS4aMK_fr9kuZGghpefylQ3FuKlnUWEq46UeHJe59hyphenhyphenKGejqHijYNLGgZ0ZHIp8EXvTOFmjTone8M069JbppqJFSlU4LsM7242Ouc-4lW0wRVAFqsRHy3OTR3XiY/s1600/Volans,+Mario+Jaci.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration-line: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiGsBZSKTCb4_nufbFtjS4aMK_fr9kuZGghpefylQ3FuKlnUWEq46UeHJe59hyphenhyphenKGejqHijYNLGgZ0ZHIp8EXvTOFmjTone8M069JbppqJFSlU4LsM7242Ouc-4lW0wRVAFqsRHy3OTR3XiY/s1600/Volans,+Mario+Jaci.jpg" style="background: rgb(250, 242, 217); border-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<span style="color: #20124d; font-family: "arial" , "helvetica" , sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes - CARJ</span></div>
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<span style="background-color: white; font-family: "arial" , sans-serif;"><b><span style="color: #660000;">PISCES VOLANS, OS PEIXES VOADORES</span></b><span style="color: #073763;"><o:p></o:p></span></span><br />
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<span style="background-color: white; color: #073763; font-family: "arial" , sans-serif;">Ascensão Reta 6h36m / 9h2m Declinação -64<sup>o</sup>.2 / -75<sup>o</sup>.0<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: "arial" , sans-serif;">Constelação adicionada por Bayer, 1604.<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: "arial" , sans-serif;">Esta é uma constelação que parece quase ser adjuntada à Carina </span><br />
<span style="background-color: white; color: #073763; font-family: "arial" , sans-serif;">e pode ser bem encontrada </span><br />
<span style="background-color: white; color: #073763; font-family: "arial" , sans-serif;">situando-se entre as estrelas Beta (Miaplacidus) </span><br />
<span style="background-color: white; color: #073763; font-family: "arial" , sans-serif;">e Epsilon Carinae (Avior).<o:p></o:p></span></div>
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<span style="color: #274e13; font-family: "arial" , "helvetica" , sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #274e13; font-family: "arial" , "helvetica" , sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="color: #274e13; font-family: "arial" , "helvetica" , sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="background-color: white;"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/home.html" style="color: #cc0000; text-decoration-line: none;" target="index"><b><span class="larger" style="font-size: 17.92px;">Star Names<br /><span class="small" style="font-size: 15.232px;">Their Lore and Meaning </span></span><br />by<br /><span class="larger" style="font-size: 17.92px;">Richard Hinckley Allen </span></b></a><br />as reprinted<br />in the Dover edition, 1963</span></div>
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<span style="background-color: white;">The text is in the public domain.</span><br />
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<span style="color: #000066; font-family: "palatino linotype" , "palatino" , "gentium plus" , serif; font-size: 19.2px;">Piscis Volans, the Flying Fish,</span></div>
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now known by astronomers as <b>Volans</b>, is the <b><span class="French" style="color: rgb(0 , 153 , 51);">Poisson Volant</span></b> of the French and the <b><span class="German" style="color: rgb(51 , 153 , 153);">Fliegende Fisch</span></b> of the Germans. The <i>Rudolphine Tables</i> have it<b><span class="Latin" style="color: rgb(153 , 0 , 0);">Passer</span></b>, the Sparrow, and, as such, it is translated <b><span class="Chinese" style="color: rgb(218 , 83 , 0);">Fe Yu</span></b> by the Chinese. This is another of the new southern constellations formally introduced by Bayer, comprising forty-six stars south of Canopus and Miaplacidus, — <span class="star" style="color: rgb(136 , 0 , 204); font-family: "verdana" , "ariel" , "helvetica" , sans-serif; font-size: 14.4px; font-style: italic;">α</span> and <span class="star" style="color: rgb(136 , 0 , 204); font-family: "verdana" , "ariel" , "helvetica" , sans-serif; font-size: 14.4px; font-style: italic;">β</span> Argūs.</div>
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Julius Schiller included it with <a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Dorado*.html" style="color: #cc0000; text-decoration-line: none;">Dorado </a>and the <a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Nubecula_Major*.html" style="color: #cc0000; text-decoration-line: none;">Nubecula Major</a> in his biblical figure of <b>Abel the Just</b>.</div>
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The <i>lucida</i> is <span class="star" style="color: rgb(136 , 0 , 204); font-family: "verdana" , "ariel" , "helvetica" , sans-serif; font-size: 14.4px; font-style: italic;">β</span>, a colored 3.9‑magnitude, culminating on the 12th of March.</div>
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<span style="color: #000066; font-family: "palatino linotype" , "palatino" , "gentium plus" , serif;"><span style="line-height: 24px;"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Piscis_Volans*.html" style="color: #274e13; text-decoration-line: none;">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Piscis_Volans*.html</a></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><a href="http://www.iau.org/static/public/constellations/gif/VOL.gif" style="color: #274e13; text-decoration-line: none;">http://www.iau.org/static/public/constellations/gif/VOL.gif</a></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>Volans</b> (Vol), o Peixe voador, é uma <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Constelação">constelação</a> do <a href="http://pt.wikipedia.org/wiki/Hemisf%C3%A9rio_celestial_sul" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Hemisfério celestial sul">hemisfério celestial sul</a>. O genitivo, usado para formar nomes de estrelas, é <b>Volantis</b>.</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">As constelações vizinhas são <a href="http://pt.wikipedia.org/wiki/Carina_(constela%C3%A7%C3%A3o)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Carina (constelação)">Carina</a>, <a href="http://pt.wikipedia.org/wiki/Pictor" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Pictor">Pictor</a>, <a href="http://pt.wikipedia.org/wiki/Dorado" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Dorado">Dorado</a>, <a href="http://pt.wikipedia.org/wiki/Mensa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Mensa">Mensa</a> e <a href="http://pt.wikipedia.org/wiki/Chamaeleon" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Chamaeleon">Chamaeleon</a>.</span></div>
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<span class="mw-headline" id="Hist.C3.B3ria" style="font-size: medium;">História</span></h2>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">O nome Volans é uma forma abreviada do nome original da constelação, <b>Piscis Volans</b>.<span class="reference" id="cite_ref-Staal1988_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Volans#cite_note-Staal1988-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">1</a></span> Volans foi uma das 12 constelações criadas por <a href="http://pt.wikipedia.org/wiki/Petrus_Plancius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Petrus Plancius">Petrus Plancius</a> a partir de observações de <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Pieter_Dirkszoon_Keyser&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration-line: none;" title="Pieter Dirkszoon Keyser (página não existe)">Pieter Dirkszoon Keyser</a> e <a href="http://pt.wikipedia.org/wiki/Frederick_de_Houtman" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Frederick de Houtman">Frederick de Houtman</a> e apareceu pela primeira vez num globo celestial de 35 cm de diâmetro publicado em 1597 (ou 1598) em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Amsterd%C3%A3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Amsterdã">Amsterdã</a> por Plancius com <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Jodocus_Hondius&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration-line: none;" title="Jodocus Hondius (página não existe)">Jodocus Hondius</a>. A primeira representação da constelação num atlas celestial foi em <i><a href="http://pt.wikipedia.org/wiki/Uranometria" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Uranometria">Uranometria</a></i> de <a href="http://pt.wikipedia.org/wiki/Johann_Bayer" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Johann Bayer">Johann Bayer</a>, em 1603.<span class="reference" id="cite_ref-Staal1988_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Volans#cite_note-Staal1988-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">1</a></span></span></div>
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<span class="mw-headline" id="Objetos" style="font-size: medium;">Objetos</span></h2>
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<span class="mw-headline" id="Estrelas" style="font-size: medium;">Estrelas</span></h3>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Há duas <a href="http://pt.wikipedia.org/wiki/Estrela_dupla" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Estrela dupla">estrelas duplas</a> na constelação que podem ser observadas utilizando um <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Telescópio">telescópio</a> pequeno, <a href="http://pt.wikipedia.org/wiki/Gamma_Volantis" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Gamma Volantis">Gamma Volantis</a> e <a href="http://pt.wikipedia.org/wiki/Epsilon_Volantis" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Epsilon Volantis">Epsilon Volantis</a>. As magnitudes das estrelas de Gamma Volantis são 4 e 6, e das de Epsilon Volantis são 4 e 8<span class="reference" id="cite_ref-FOOTNOTERidpathTirion2007_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Volans#cite_note-FOOTNOTERidpathTirion2007-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">2</a></span> .</span></div>
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<span class="mw-headline" id="C.C3.A9u_profundo" style="font-size: medium;">Céu profundo</span></h3>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Volans possui vários objetos de <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Céu profundo">céu profundo</a>. O anel de Lindsay-Shapley, categorizado com o código <a class="new" href="http://pt.wikipedia.org/w/index.php?title=AM_0644-741&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration-line: none;" title="AM 0644-741 (página não existe)">AM 0644-741</a>, é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_em_anel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Galáxia em anel">galáxia em anel</a> localizada a 300 milhões de<a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Ano-luz">anos-luz</a> da Terra. Foi encontrada próxima à <a href="http://pt.wikipedia.org/wiki/Grande_Nuvem_de_Magalh%C3%A3es" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Grande Nuvem de Magalhães">Grande Nuvem de Magalhães</a> em <a href="http://pt.wikipedia.org/wiki/1960" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="1960">1960</a> e recebeu o nome de seus descobridores. Seu formato pouco usual é resultado de uma colisão há muitos milhões de anos atrás. O anel azul que possui 150 mil anos-luz de diâmetro foi formado quando uma <a href="http://pt.wikipedia.org/wiki/Onda_de_choque" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Onda de choque">onda de choque</a> da colisão criou o anel de estrelas azuis e quentes; o núcleo amarelo é uma fusão dos núcleos das galáxias progenitoras<span class="reference" id="cite_ref-FOOTNOTEWilkinsDunn2006_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Volans#cite_note-FOOTNOTEWilkinsDunn2006-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">3</a></span> . <a href="http://pt.wikipedia.org/wiki/NGC_2442" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="NGC 2442">NGC 2442</a>, uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Galáxia espiral">galáxia espiral</a>, está localizada a uma distância de 50 milhões de anos-luz da Terra.</span></div>
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<span style="color: #333333; font-family: sans-serif; line-height: 18px;"><span style="line-height: 24px; white-space: nowrap;">http://pt.wikipedia.org/wiki/Volans#/media/File:Volans_constellation_map.png</span></span></div>
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Stellarium</div>
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<b>Alpha Volantis</b> (α Vol, α Volantis) é uma <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Estrela">estrela</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Volans" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Volans">Volans</a>. Com uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Magnitude aparente">magnitude aparente</a> de 4,00,<span class="reference" id="cite_ref-simbad_1-8" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Volantis#cite_note-simbad-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">1</a></span> é a quinta estrela mais brilhante da constelação, mesmo tendo a designação "Alpha" (que normalmente é dada à estrela mais brilhante da constelação).<span class="reference" id="cite_ref-stars_4-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Volantis#cite_note-stars-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">4</a></span> Com base em medições de <a href="http://pt.wikipedia.org/wiki/Paralaxe" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Paralaxe">paralaxe</a>, está localizada a aproximadamente 124,9 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Ano-luz">anos-luz</a> (38,3 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Parsec">parsecs</a>) da Terra.<span class="reference" id="cite_ref-simbad_1-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Volantis#cite_note-simbad-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">1</a></span></div>
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Alpha Volantis é uma <a href="http://pt.wikipedia.org/wiki/Estrela_peculiar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Estrela peculiar">estrela peculiar</a> do grupo das <a href="http://pt.wikipedia.org/wiki/Estrela_com_linhas_met%C3%A1licas" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Estrela com linhas metálicas">estrelas Am</a>, tendo uma <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Classificação estelar">classificação estelar</a> de kA3hA5mA5 V.<span class="reference" id="cite_ref-aj132_1_161_2-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Volantis#cite_note-aj132_1_161-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">2</a></span> É uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Estrela_de_classe_A_da_sequ%C3%AAncia_principal" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Estrela de classe A da sequência principal">estrela de classe A da sequência principal</a>com uma <a href="http://pt.wikipedia.org/wiki/Temperatura_efetiva" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Temperatura efetiva">temperatura efetiva</a> de 8 198 <a href="http://pt.wikipedia.org/wiki/Kelvin" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Kelvin">K</a><span class="reference" id="cite_ref-aj132_1_161_2-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Volantis#cite_note-aj132_1_161-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">2</a></span> Tem uma massa de 2,2 vezes a <a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Massa solar">massa do Sol</a> e um raio de 2,5 vezes o <a href="http://pt.wikipedia.org/wiki/Raio_solar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Raio solar">raio solar</a>.<span class="reference" id="cite_ref-stars_4-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Volantis#cite_note-stars-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">4</a></span> Sua idade estimada é de 420 milhões de anos.<span class="reference" id="cite_ref-Vican2012_6-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Volantis#cite_note-Vican2012-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; 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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.4px;">http://pt.wikipedia.org/wiki/Alpha_Volantis</span></span></div>
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<b>Beta Volantis</b> (β Vol, β Volantis) é a <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Estrela">estrela</a> mais brilhante da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Volans" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Volans">Volans</a>, com uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Magnitude aparente">magnitude aparente</a> de 3,78.<span class="reference" id="cite_ref-simbad_1-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Volantis#cite_note-simbad-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">1</a></span> Medições de <a href="http://pt.wikipedia.org/wiki/Paralaxe" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Paralaxe">paralaxe</a> mostram que está uma distância de aproximadamente 107,5 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Ano-luz">anos-luz</a> (33 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Parsec">parsecs</a>) da Terra.<span class="reference" id="cite_ref-simbad_1-10" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Volantis#cite_note-simbad-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">1</a></span></div>
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O espectro de Beta Volantis corresponde a uma <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Classificação estelar">classificação estelar</a> de K2 III.<span class="reference" id="cite_ref-simbad_1-11" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Volantis#cite_note-simbad-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">1</a></span> A classe de luminosidade 'III' indica que é uma <a href="http://pt.wikipedia.org/wiki/Estrela_gigante" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Estrela gigante">estrela gigante</a> que já consumiu todo o hidrogênio de seu núcleo e saiu da <a href="http://pt.wikipedia.org/wiki/Sequ%C3%AAncia_principal" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Sequência principal">sequência principal</a>. Tem uma massa de 1,62 vezes a <a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Massa solar">massa do Sol</a><span class="reference" id="cite_ref-Stello2008_3-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Volantis#cite_note-Stello2008-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">3</a></span> e um raio de 16 vezes o <a href="http://pt.wikipedia.org/wiki/Raio_solar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Raio solar">raio solar</a>.<span class="reference" id="cite_ref-aaa367_521_4-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Volantis#cite_note-aaa367_521-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">4</a></span> Está irradiando 41 vezes mais energia que o Sol<span class="reference" id="cite_ref-Stello2008_3-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Volantis#cite_note-Stello2008-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">3</a></span> de sua <a href="http://pt.wikipedia.org/wiki/Atmosfera_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Atmosfera estelar">atmosfera externa</a> a uma <a href="http://pt.wikipedia.org/wiki/Temperatura_efetiva" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Temperatura efetiva">temperatura efetiva</a> de 4 736 <a href="http://pt.wikipedia.org/wiki/Kelvin" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Kelvin">K</a>,<span class="reference" id="cite_ref-Morel2012_5-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Volantis#cite_note-Morel2012-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">5</a></span> o que lhe dá a coloração alaranjada típica de estrelas de classe K.<span class="reference" id="cite_ref-csiro_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Volantis#cite_note-csiro-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">6</a></span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.4px;">http://pt.wikipedia.org/wiki/Beta_Volantis</span></span></div>
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<b>Gamma Volantis</b> (γ Vol, γ Volantis) é uma <a href="http://pt.wikipedia.org/wiki/Estrela_bin%C3%A1ria" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Estrela binária">estrela binária</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Volans" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Volans">Volans</a>. As duas estrelas do sistema são inseparáveis a olho nu e têm uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Magnitude aparente">magnitude aparente</a> conjunta de 3,60, o que torna esse sistema o mais brilhante da constelação, embora <a href="http://pt.wikipedia.org/wiki/Beta_Volantis" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Beta Volantis">Beta Volantis</a> seja a estrela individual mais brilhante. Está a uma distância de aproximadamente 142 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Ano-luz">anos-luz</a> (43 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Parsec">parsecs</a>) da Terra.<span class="reference" id="cite_ref-stars_3-7" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Volantis#cite_note-stars-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">3</a></span></div>
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O sistema é composto por Gamma<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">1</span> Volantis, a estrela menos brilhante de magnitude 5,67, e Gamma<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">2</span> Volantis, o componente primário de magnitude 3,78. Gamma<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">2</span>Volantis é uma <a href="http://pt.wikipedia.org/wiki/Estrela_gigante" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Estrela gigante">estrela gigante</a> com uma <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Classificação estelar">classificação estelar</a> de K0 III, o que significa que é uma estrela <a href="http://pt.wikipedia.org/wiki/Evolu%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Evolução estelar">evoluída</a> que já queimou todo o hidrogênio de seu núcleo. Irradia 71 vezes mais energia que o Sol a uma <a href="http://pt.wikipedia.org/wiki/Temperatura_efetiva" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Temperatura efetiva">temperatura efetiva</a> de 4 700 <a href="http://pt.wikipedia.org/wiki/Kelvin" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Kelvin">K</a>. Tem uma massa de 2,5 vezes a <a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Massa solar">massa do Sol</a> e um raio de 12,7 vezes o <a href="http://pt.wikipedia.org/wiki/Raio_solar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Raio solar">raio solar</a>.<span class="reference" id="cite_ref-stars_3-8" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Volantis#cite_note-stars-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">3</a></span>Sua companheira, Gamma<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">1</span> Volantis, é uma <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Estrela_de_classe_F_da_sequ%C3%AAncia_principal&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration-line: none;" title="Estrela de classe F da sequência principal (página não existe)">estrela de classe F da sequência principal</a> com classificação de F2 V e temperatura efetiva de 6 541 K.<span class="reference" id="cite_ref-Eiff2012_4-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Volantis#cite_note-Eiff2012-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">4</a></span> Tem uma massa de 1,69 vezes a massa solar<span class="reference" id="cite_ref-Casagrande2011_5-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Volantis#cite_note-Casagrande2011-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">5</a></span> e um raio de 1,9 vezes o raio solar. Suspeita-se que seja uma <a href="http://pt.wikipedia.org/wiki/Estrela_vari%C3%A1vel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Estrela variável">variável pulsante</a> levemente irregular.<span class="reference" id="cite_ref-stars_3-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Volantis#cite_note-stars-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">3</a></span></div>
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O sistema tem uma idade estimada de 600 milhões de anos<span class="reference" id="cite_ref-stars_3-10" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Volantis#cite_note-stars-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">3</a></span> a 1,8 bilhão de anos.<span class="reference" id="cite_ref-Casagrande2011_5-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Volantis#cite_note-Casagrande2011-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">5</a></span> As duas estrelas estão separadas no céu por 14,1 <a href="http://pt.wikipedia.org/wiki/Segundo_de_arco" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Segundo de arco">segundos de arco</a>, o que corresponde a uma separação de no mínimo 600 <a href="http://pt.wikipedia.org/wiki/Unidade_astron%C3%B4mica" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Unidade astronômica">UA</a> e um <a href="http://pt.wikipedia.org/wiki/Per%C3%ADodo_orbital" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Período orbital">período orbital</a> de pelo menos 7 500 anos.<span class="reference" id="cite_ref-stars_3-11" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Volantis#cite_note-stars-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">3</a></span></div>
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<b style="line-height: 22.4px;">Delta Volantis</b><span style="line-height: 22.4px;"> (δ Vol, δ Volantis) é a quarta </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-image: none; color: #0b0080; line-height: 22.4px; text-decoration-line: none;" title="Estrela">estrela</a><span style="line-height: 22.4px;"> mais brilhante da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; color: #0b0080; line-height: 22.4px; text-decoration-line: none;" title="Constelação">constelação</a><span style="line-height: 22.4px;"> de </span><a href="http://pt.wikipedia.org/wiki/Volans" style="background-image: none; color: #0b0080; line-height: 22.4px; text-decoration-line: none;" title="Volans">Volans</a><span style="line-height: 22.4px;">, com uma </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; color: #0b0080; line-height: 22.4px; text-decoration-line: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 22.4px;"> de 3,98.</span><span class="reference" id="cite_ref-stars_5-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Delta_Volantis#cite_note-stars-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">5</a></span><span style="line-height: 22.4px;"> Tem uma </span><a href="http://pt.wikipedia.org/wiki/Paralaxe" style="background-image: none; color: #0b0080; line-height: 22.4px; text-decoration-line: none;" title="Paralaxe">paralaxe</a><span style="line-height: 22.4px;"> de 4,42 ± 0,11 </span><a href="http://pt.wikipedia.org/wiki/Segundo_de_arco" style="background-image: none; color: #0b0080; line-height: 22.4px; text-decoration-line: none;" title="Segundo de arco">milissegundos de arco</a><span style="line-height: 22.4px;">, o que corresponde a uma distância de aproximadamente 740 </span><a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-image: none; color: #0b0080; line-height: 22.4px; text-decoration-line: none;" title="Ano-luz">anos-luz</a><span style="line-height: 22.4px;"> (226 </span><a href="http://pt.wikipedia.org/wiki/Parsec" style="background-image: none; color: #0b0080; line-height: 22.4px; text-decoration-line: none;" title="Parsec">parsecs</a><span style="line-height: 22.4px;">) da Terra.</span><span class="reference" id="cite_ref-simbad_1-8" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Delta_Volantis#cite_note-simbad-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">1</a></span><span style="line-height: 22.4px;"> É uma </span><a href="http://pt.wikipedia.org/wiki/Estrela_gigante_luminosa" style="background-image: none; color: #0b0080; line-height: 22.4px; text-decoration-line: none;" title="Estrela gigante luminosa">gigante luminosa</a><span style="line-height: 22.4px;"> com uma</span><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-image: none; color: #0b0080; line-height: 22.4px; text-decoration-line: none;" title="Classificação estelar">classificação estelar</a><span style="line-height: 22.4px;"> de F6 II.</span><span class="reference" id="cite_ref-simbad_1-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Delta_Volantis#cite_note-simbad-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">1</a></span><span style="line-height: 22.4px;"> Tem uma massa de cerca de 6 </span><a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background-image: none; color: #0b0080; line-height: 22.4px; text-decoration-line: none;" title="Massa solar">massas solares</a><span style="line-height: 22.4px;"> e um raio de 50 </span><a href="http://pt.wikipedia.org/wiki/Raio_solar" style="background-image: none; color: #0b0080; line-height: 22.4px; text-decoration-line: none;" title="Raio solar">raios solares</a><span style="line-height: 22.4px;">.</span><span class="reference" id="cite_ref-stars_5-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Delta_Volantis#cite_note-stars-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">5</a></span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.4px;">http://pt.wikipedia.org/wiki/Delta_Volantis</span></span></div>
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<b>Epsilon Volantis</b> (ε Vol, ε Volantis) é um <a href="http://pt.wikipedia.org/wiki/Sistema_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Sistema estelar">sistema estelar triplo</a><span class="reference" id="cite_ref-mnras389_2_869_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Volantis#cite_note-mnras389_2_869-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">3</a></span> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Volans" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Volans">Volans</a>. Possui uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Magnitude aparente">magnitude aparente</a> visual de 4,40,<span class="reference" id="cite_ref-simbad_1-11" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Volantis#cite_note-simbad-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">1</a></span> sendo visível a <a href="http://pt.wikipedia.org/wiki/Vis%C3%A3o#A_olho_nu" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Visão">olho nu</a> em boas condições de visualização. Com base em sua <a href="http://pt.wikipedia.org/wiki/Paralaxe" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Paralaxe">paralaxe</a> de 5,80 <a href="http://pt.wikipedia.org/wiki/Segundo_de_arco" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Segundo de arco">milissegundos de arco</a>, está localizado a uma distância de aproximadamente 560 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Ano-luz">anos-luz</a>(170 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Parsec">parsecs</a>) da Terra.<span class="reference" id="cite_ref-simbad_1-12" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Volantis#cite_note-simbad-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">1</a></span></div>
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O componente primário do sistema Epsilon Volantis é uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Bin%C3%A1ria_espectrosc%C3%B3pica" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Binária espectroscópica">binária espectroscópica</a> de linha dupla<span class="reference" id="cite_ref-Chini2012_4-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Volantis#cite_note-Chini2012-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">4</a></span> com um <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Classificação estelar">tipo espectral</a> de B6 IV<span class="reference" id="cite_ref-simbad_1-13" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Volantis#cite_note-simbad-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">1</a></span> e <a href="http://pt.wikipedia.org/wiki/Per%C3%ADodo_orbital" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Período orbital">período orbital</a> de 14,1683 dias.<span class="reference" id="cite_ref-Pourbaix2004_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Volantis#cite_note-Pourbaix2004-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">5</a></span>A uma distância angular de 6,1 segundos de arco na <a href="http://pt.wikipedia.org/wiki/Esfera_celeste" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Esfera celeste">esfera celeste</a> está a terceira estrela do sistema, de magnitude aparente 7,48.<span class="reference" id="cite_ref-mnras389_2_869_3-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Volantis#cite_note-mnras389_2_869-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">3</a></span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.4px;">http://pt.wikipedia.org/wiki/Epsilon_Volantis</span></span></div>
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<b>Zeta Volantis</b> (ζ Vol, ζ Volantis) é a terceira <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Estrela">estrela</a> mais brilhante da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Volans" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Volans">Volans</a>, com uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Magnitude aparente">magnitude aparente</a> de 3,96.<span class="reference" id="cite_ref-simbad_1-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Zeta_Volantis#cite_note-simbad-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">1</a></span> Com base em medições de<a href="http://pt.wikipedia.org/wiki/Paralaxe" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Paralaxe">paralaxe</a>, está localizada a aproximadamente 141 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Ano-luz">anos-luz</a> (43,2 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Parsec">parsecs</a>) da Terra.<span class="reference" id="cite_ref-simbad_1-10" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Zeta_Volantis#cite_note-simbad-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">1</a></span></div>
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Zeta Volantis é uma <a href="http://pt.wikipedia.org/wiki/Estrela_gigante" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Estrela gigante">estrela gigante</a> <a href="http://pt.wikipedia.org/wiki/Evolu%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Evolução estelar">evoluída</a> com uma <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Classificação estelar">classificação estelar</a> de K0 III.<span class="reference" id="cite_ref-simbad_1-11" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Zeta_Volantis#cite_note-simbad-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">1</a></span> Estrelas desse tipo tipicamente têm uma <a href="http://pt.wikipedia.org/wiki/Temperatura_efetiva" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Temperatura efetiva">temperatura efetiva</a> de cerca de 4 900 <a href="http://pt.wikipedia.org/wiki/Kelvin" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Kelvin">K</a>, o que lhes dá a coloração alaranjada típica de estrelas de classe K.<span class="reference" id="cite_ref-csiro_4-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Zeta_Volantis#cite_note-csiro-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">4</a></span> O <a href="http://pt.wikipedia.org/wiki/Di%C3%A2metro_angular" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Diâmetro angular">diâmetro angular</a> de Zeta Volantis, após correções de <a href="http://pt.wikipedia.org/wiki/Escurecimento_de_bordo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Escurecimento de bordo">escurecimento de bordo</a>, é de 2,32 ± 0,06 <a href="http://pt.wikipedia.org/wiki/Segundo_de_arco" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Segundo de arco">milissegundos de arco</a>,<span class="reference" id="cite_ref-aaa431_773_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Zeta_Volantis#cite_note-aaa431_773-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">5</a></span> o que pode ser usado para calcular um raio de aproximadamente 11 vezes o <a href="http://pt.wikipedia.org/wiki/Raio_solar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Raio solar">raio solar</a>.<span class="reference" id="cite_ref-lang2006_3-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Zeta_Volantis#cite_note-lang2006-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">3</a></span> Zeta Volantis forma um <a href="http://pt.wikipedia.org/wiki/Estrela_bin%C3%A1ria" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Estrela binária">sistema estelar binário</a> com uma estrela de magnitude 9,7 localizada a uma separação de 16,7 segundos de arco no céu.<span class="reference" id="cite_ref-mnras389_2_869_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Zeta_Volantis#cite_note-mnras389_2_869-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none; white-space: nowrap;">6</a></span></div>
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<span style="line-height: 18px;"><span style="font-family: "arial" , "helvetica" , sans-serif;"><a href="http://www.raremaps.com/gallery/enlarge/28535" style="color: #274e13; text-decoration-line: none;">http://www.raremaps.com/gallery/enlarge/28535</a></span></span></div>
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<span style="color: #073763;"><a href="http://www.raremaps.com/gallery/detail/28535/The_Consellations_Southern_Hemisphere/Burritt.html" style="color: #274e13; text-decoration-line: none;">http://www.raremaps.com/gallery/detail/28535/The_Consellations_Southern_Hemisphere/Burritt.html</a></span></div>
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<span style="color: #274e13; font-family: "arial" , "helvetica" , sans-serif;">The Consellations (Southern Hemisphere) </span><strong style="color: #274e13; font-family: arial, helvetica, sans-serif;">Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/808" style="border-bottom: 0px solid rgb(255, 255, 255); color: #274e13; font-family: arial, helvetica, sans-serif; text-decoration-line: none;">Elijah J. Burritt</a></div>
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<span style="color: #274e13; font-family: "arial" , "helvetica" , sans-serif;">Decorative chart of the southern skies, with a chart at the bottom left, identifying the magnitude of the various stars. </span><span style="color: #274e13; font-family: "arial" , "helvetica" , sans-serif;">The constellations and major stars are named within the image. From Burritt's </span><em style="color: #274e13; font-family: arial, helvetica, sans-serif;">Atlas Designed to Illustrate the Geography of the Heavens.</em><br />
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<span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif; line-height: 22.4px;"><b>Caro Leitor,</b></span></div>
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<span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif; line-height: 22.4px;"><b>Os Objetos Celestes abaixo apresentados</b></span></div>
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<span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif; line-height: 22.4px;"><b>e que são encontrados na direção do Peixe Voador, Volans,</b></span></div>
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<span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif; line-height: 22.4px;"><b>foram descobertos por Jonh Herschel</b></span></div>
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<span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif; line-height: 22.4px;"><b>quando de sua estada no Cabo da Boa Esperança, África do Sul.</b></span></div>
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<span style="color: #000099; font-family: "times new roman"; font-size: x-small; line-height: normal;"><span style="font-family: "arial" , "helvetica";"><b>John Frederick William Herschel</b>, <i>Sir</i></span></span></div>
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<span style="color: #000099; font-family: "arial" , "helvetica" , sans-serif; line-height: normal;"><i></i><b>(1792 - 1871)</b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #000099; line-height: normal;"><b><img align="LEFT" src="http://www.dec.ufcg.edu.br/biografias/johnfrew.jpg" height="284" style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="199" /></b> Astrônomo inglês nascido em Slough, Buckinghamshire, filho único do famosíssimo astrônomo e construtor de telescópios <b>William Frederick Herschel</b>, continuador das observações do pai sobre nebulosas e estrelas duplas, e com o qual catalogou a descoberta de 525 nebulosas. Estudou na Universidade de Cambridge e, em Londres, iniciou um curso de direito que não chegou a concluir, optando por trabalhar com o pai (1816) desenvolvendo seus conhecimentos sobre astronomia. Desenvolveu também notáveis descobertas em pesquisas sobre a luz e a astrofísica, como o primeiro telescópio para levantamento dos céus do sul. Decidido a estudar o firmamento do hemisfério sul, transferiu-se para o cabo da Boa Esperança (1833), na África do Sul, onde completou um catálogo de quase setenta mil corpos celestes e desenvolveu um método para o cálculo de sua órbita real no espaço. Fez notáveis descobertas sobre técnicas fotográficas, como a invenção de um processo de fotografia sobre papel sensibilizador. Pioneiro no uso dos termos positivo e negativo (foto) em relação às imagens fotográficas, descobriu a capacidade do <i>hipossulfito de sódio </i>(1819) para diluição de sais de prata, o que abriu caminho para a fabricação de <i>fixadores em fotografia</i>. Contribuiu, além disso, para o progresso das ciências exatas, foi autor de trabalhos sobre cálculo diferencial e teoria das séries e, em física, publicou um conceituado tratado de óptica. Foi um dos fundadores, juntamente com <b>Charles Babage</b> e<b>George Peacock</b>, da Analitical Society of the Trinity College, em Cambridge, e morreu em Collingwood, Kent (1871).</span><span style="line-height: normal;"></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><i><span style="color: #000099;">Figura copiada do site da UNIV. TEXAS / PORTRAIT GALERY :</span></i><br /><span style="color: #000099;"><a href="http://www.lib.utexas.edu/photodraw/portraits/#F" style="color: #274e13; text-decoration-line: none;">http://www.lib.utexas.edu/photodraw/portraits/</a></span></span></div>
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<span style="color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.4px;"><a href="http://www.dec.ufcg.edu.br/biografias/JohnFreW.html" style="color: #274e13; text-decoration-line: none;">http://www.dec.ufcg.edu.br/biografias/JohnFreW.html</a></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Programa Stellarium</span></div>
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<b>NGC 2601</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral_barrada" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Galáxia espiral barrada">espiral barrada</a> (SBa) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Volans" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Volans">Volans</a>. Possui uma declinação de -68° 07' 04" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Ascensão recta">ascensão recta</a> de 8 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Hora">horas</a>, 25 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Minuto">minutos</a> e 30,4 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Segundo">segundos</a>.</div>
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A galáxia <b>NGC 2601</b> foi descoberta em <a href="http://pt.wikipedia.org/wiki/1835" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="1835">1835</a> por <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="John Herschel">John Herschel</a>.</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.4px;">http://pt.wikipedia.org/wiki/NGC_2601</span></span><br />
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Stellarium</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.4px;">"NGC 2397 by HST" por NASA, ESA & Stephen Smartt (Queen's University Belfast, UK) - European Hubble site. Licenciado sob CC BY-SA 3.0, via Wikimedia Commons - http://commons.wikimedia.org/wiki/File:NGC_2397_by_HST.jpg#/media/File:NGC_2397_by_HST.jpg</span></span></div>
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<b>NGC 2397</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Galáxia espiral">espiral</a> (Sb) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Volans" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Volans">Volans</a>. Possui uma declinação de -69° 00' 05" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Ascensão recta">ascensão recta</a> de 7 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Hora">horas</a>, 21<a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Minuto">minutos</a> e 19,5 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Segundo">segundos</a>.</div>
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A galáxia <b>NGC 2397</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/21_de_Fevereiro" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="21 de Fevereiro">21 de Fevereiro</a> de <a href="http://pt.wikipedia.org/wiki/1835" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="1835">1835</a> por <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="John Herschel">John Herschel</a>.</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.4px;">http://pt.wikipedia.org/wiki/NGC_2397</span></span></div>
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Stellarium</div>
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<img alt="Ngc2442 potw.jpg" src="http://upload.wikimedia.org/wikipedia/commons/thumb/4/4e/Ngc2442_potw.jpg/800px-Ngc2442_potw.jpg" style="background: rgb(250, 242, 217); border-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.4px;">"Ngc2442 potw" por ESO/IDA/Danish 1.5 m/R. Gendler, J.-E. Ovaldsen, C. C. Thöne and C. Féron - <a href="http://www.eso.org/gallery/v/ESOPIA/Galaxies/ngc2442_potw.tif.html" style="color: #274e13; text-decoration-line: none;">http://www.eso.org/gallery/v/ESOPIA/Galaxies/ngc2442_potw.tif.html</a>. Licenciado sob CC BY 4.0, via Wikimedia Commons - http://commons.wikimedia.org/wiki/File:Ngc2442_potw.jpg#/media/File:Ngc2442_potw.jpg</span></span></div>
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<span style="color: #333333; font-family: sans-serif; line-height: 22px;">The distorted galaxy NGC 2442, also known as the Meathook Galaxy, is located some 50 million light-years away in the constellation of Volans (the Flying Fish). The galaxy is 75 000 light-years wide and features two dusty spiral arms extending from a pronounced central bar that give it a hook-like appearance, hence its nickname. The galaxy’s distorted shape is most likely the result of a close encounter with a smaller, unseen galaxy. This image is based on data acquired with the 1.5-metre Danish telescope at ESO’s La Silla Observatory in Chile, through three filters (B: 250 s, V: 187 s, R: 150 s). ID: ngc2442 Credit: ESO/IDA/Danish 1.5 m/R. Gendler, J.-E. Ovaldsen, C. C. Thöne and C. Féron</span></div>
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<span class="mw-mmv-author" style="background-color: whitesmoke; color: #555555; font-family: sans-serif; font-size: 13.6px; line-height: 24.48px;">Féron</span><span style="background-color: whitesmoke; color: #555555; font-family: sans-serif; font-size: 13.6px; line-height: 24.48px;"> - </span><span class="mw-mmv-source" style="background-color: whitesmoke; color: #555555; font-family: sans-serif; font-size: 13.6px; line-height: 24.48px;"><a class="external free" href="http://www.eso.org/gallery/v/ESOPIA/Galaxies/ngc2442_potw.tif.html" rel="nofollow" style="background: none; color: #0b0080; text-decoration-line: none;">http://www.eso.org/gallery/v/ESOPIA/Galaxies/ngc2442_potw.tif.html</a></span></div>
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<b style="color: #252525; font-family: sans-serif; line-height: 22.4px;">NGC 2442</b><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"> é</span><span style="color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.4px;"> uma </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral_barrada" style="background-image: none; color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.4px; text-decoration-line: none;" title="Galáxia espiral barrada">galáxia espiral barrada</a><span style="color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.4px;"> situada na direção da </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o_do_Peixe_Voador" style="background-image: none; color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.4px; text-decoration-line: none;" title="Constelação do Peixe Voador">constelação do Peixe Voador</a><span style="color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.4px;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.4px; text-decoration-line: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.4px;"> de 10,4, uma declinação de -69º 32' 31" e uma</span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-image: none; color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.4px; text-decoration-line: none;" title="Ascensão reta">ascensão reta</a><span style="color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.4px;"> de 07 </span><a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.4px; text-decoration-line: none;" title="Hora">horas</a><span style="color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.4px;">, 36 </span><a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.4px; text-decoration-line: none;" title="Minuto">minutos</a><span style="color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.4px;"> e 19,7 </span><a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.4px; text-decoration-line: none;" title="Segundo">segundos</a><span style="color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.4px;">.</span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.4px;">http://pt.wikipedia.org/wiki/NGC_2442</span></span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/9/98/NGC_2442.jpg/640px-NGC_2442.jpg" style="background: rgb(250, 242, 217); border-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></div>
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"NGC 2442" by NASA, ESA - http://www.spacetelescope.org/images/heic1108a/. Licensed under Public Domain via Wikimedia Commons - http://commons.wikimedia.org/wiki/File:NGC_2442.jpg#/media/File:NGC_2442.jpg</div>
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<span class="mw-mmv-source-author" original-title="" style="line-height: 1.8em;"><span class="mw-mmv-author">NASA, ESA</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.spacetelescope.org/images/heic1108a/" rel="nofollow" style="background: none; color: #0b0080; text-decoration-line: none;">http://www.spacetelescope.org/images/heic1108a/</a></span></span></div>
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This close-up Hubble view of the Meathook Galaxy (NGC 2442) focuses on the more compact of its two asymmetric spiral arms as well as the central regions. The spiral arm was the location of a supernova that exploded in 1999. These Hubble observations were made in 2006 in order to study the aftermath of this supernova. Ground-based data from MPG/ESO 2.2-metre telescope were used to fill out parts of the edges of this image.</div>
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<b style="color: #252525; font-family: sans-serif; line-height: 22.4px;">NGC 2442 / 2443</b><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"> or commonly known as the </span><b style="color: #252525; font-family: sans-serif; line-height: 22.4px;">Meathook Galaxy</b><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"> is an </span><a href="http://en.wikipedia.org/wiki/Intermediate_spiral_galaxy" style="background-image: none; color: #0b0080; font-family: sans-serif; line-height: 22.4px; text-decoration-line: none;" title="Intermediate spiral galaxy">intermediate spiral galaxy</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"> about 50 million </span><a href="http://en.wikipedia.org/wiki/Light-year" style="background-image: none; color: #0b0080; font-family: sans-serif; line-height: 22.4px; text-decoration-line: none;" title="Light-year">light-years</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"> away in the </span><a href="http://en.wikipedia.org/wiki/Constellation" style="background-image: none; color: #0b0080; font-family: sans-serif; line-height: 22.4px; text-decoration-line: none;" title="Constellation">constellation</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"> </span><a href="http://en.wikipedia.org/wiki/Volans" style="background-image: none; color: #0b0080; font-family: sans-serif; line-height: 22.4px; text-decoration-line: none;" title="Volans">Volans</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;">. It was discovered by Sir </span><a href="http://en.wikipedia.org/wiki/John_Herschel" style="background-image: none; color: #0b0080; font-family: sans-serif; line-height: 22.4px; text-decoration-line: none;" title="John Herschel">John Herschel</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;">.</span><sup class="noprint Inline-Template Template-Fact" style="color: #252525; font-family: sans-serif; line-height: 1; white-space: nowrap;">[<i><a href="http://en.wikipedia.org/wiki/Wikipedia:Citation_needed" style="background: none; color: #0b0080; text-decoration-line: none;" title="Wikipedia:Citation needed"><span title="This claim needs references to reliable sources. (February 2007)">citation needed</span></a></i>]</sup><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"> Associated with this galaxy is HIPASS J0731-69, a cloud of gas devoid of any stars.</span><sup class="reference" id="cite_ref-Ryder_2-0" style="color: #252525; font-family: sans-serif; line-height: 1;"><a href="http://en.wikipedia.org/wiki/NGC_2442/2443#cite_note-Ryder-2" style="background: none; color: #0b0080; text-decoration-line: none; white-space: nowrap;">[2]</a></sup><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"> It is likely that the cloud was torn loose from NGC 2442 by a companion.</span><sup class="reference" id="cite_ref-Ryder_2-1" style="color: #252525; font-family: sans-serif; line-height: 1;"><a href="http://en.wikipedia.org/wiki/NGC_2442/2443#cite_note-Ryder-2" style="background: none; color: #0b0080; text-decoration-line: none; white-space: nowrap;">[2]</a></sup></div>
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http://en.wikipedia.org/wiki/NGC_2442/2443</div>
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<span class="title" style="font-size: 14pt;">NGC2442/2443 (Meathook Galaxy) & NGC 2434</span></h3>
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<span style="background-color: white;">NGC 2442/2443 (near centre of image, commonly known as the Meathook Galaxy or the Cobra and Mouse), is an intermediate spiral galaxy about 50 million light-years away in the constellation Volans. The galaxy’s distorted shape is most likely the result of a close encounter with a smaller, unseen galaxy. NGC 2442 is the name for SW part, while NGC 2443 is NE part.<br /><br />NGC 2434 is an elliptical galaxy also in Volans (upper left in image).<br /><br />They were both discovered by Sir John Herschel.</span></div>
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<span style="background-color: white;"><span class="exif">Lum-18x15m, R-8x15m, G-10x15m, B-10x15m<br />Image data taken with the "Bunyip 12.5" Newtonian Astrograph / STL11000M / Paramount ME <a href="http://www.pbase.com/david_fitz_henry/image/155933057&exif=Y" rel="nofollow" style="color: #274e13; text-decoration-line: none;">full exif</a> </span></span></div>
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<span style="font-size: 12px;"><span style="font-family: "arial" , "helvetica" , sans-serif;"><b><a href="http://www.pbase.com/david_fitz_henry/image/155933057" style="color: #274e13; text-decoration-line: none;">http://www.pbase.com/david_fitz_henry/image/155933057</a></b></span></span></div>
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<b>NGC 2434</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_el%C3%ADptica" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Galáxia elíptica">elíptica</a> (E) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Volans" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Volans">Volans</a>. Possui uma declinação de -69° 17' 04" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Ascensão recta">ascensão recta</a> de 7 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Hora">horas</a>, 34<a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Minuto">minutos</a> e 51,5 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; color: #0b0080; text-decoration-line: none;" title="Segundo">segundos</a>.</div>
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A galáxia <b>NGC 2434</b> foi descoberta em <a href="http://pt.wikipedia.org/wiki/1834" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="1834">1834</a> por <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="John Herschel">John Herschel</a>.</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.4px;">http://pt.wikipedia.org/wiki/NGC_2434</span></span></div>
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<a href="http://cseligman.com/text/atlas/ngc24.htm" style="color: #274e13; text-decoration-line: none;">http://cseligman.com/text/atlas/ngc24.htm</a></div>
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<span style="color: #252525; font-family: sans-serif; line-height: 22.4px;">http://cseligman.com/text/atlas/ngc24.htm</span></div>
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<a href="https://www.blogger.com/null" name="2434" style="background-color: #f9fcff; color: #274e13; font-family: georgia; text-decoration-line: none;"><big><b>NGC 2434 (= PGC 21325)</b></big><br />Discovered (Dec 23, 1834) by </a><a href="http://cseligman.com/text/atlas/discoverers.htm#jfwherschel" style="background-color: #f9fcff; color: #274e13; font-family: georgia; text-decoration-line: none;">John Herschel</a><br />
<span style="background-color: #f9fcff; font-family: "georgia";">An 11th-magnitude elliptical galaxy (type E1?) in </span><a href="http://cseligman.com/text/atlas/volans.htm#2434" style="background-color: #f9fcff; color: #274e13; font-family: georgia; text-decoration-line: none;">Volans</a><span style="background-color: #f9fcff; font-family: "georgia";"> (RA 07 34 51.5, Dec -69 17 04)</span></div>
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Per Dreyer, NGC 2434 (= John Herschel's GC 1561, 1860 RA 07 35 10, NPD 158 58.1) is "pretty bright, small, round, pretty much brighter middle, three 11th-magnitude stars to north". The position precesses to RA 07 34 51.2, Dec -69 16 57, almost dead center on the galaxy, and there are three stars just to the north, so the identification is certain. Based on a recessional velocity of 1390 km/sec, NGC 2434 is about 65 million light years away, in good agreement with redshift-independent distance estimates of 55 to 80 million light years. Given that and its apparent size of 2.5 by 2.3 arcmin, it is about 45 thousand light years across.</div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;"><a href="http://www.raremaps.com/gallery/detail/33613/Celestial_Map_of_the_Southern_Hemisphere/Pardies.html" style="color: #274e13; text-decoration-line: none;">http://www.raremaps.com/gallery/detail/33613/Celestial_Map_of_the_Southern_Hemisphere/Pardies.html</a></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><strong style="color: #073763;">Title: </strong><span style="color: #073763;">[Celestial Map of the Southern Hemisphere] </span><strong><span style="color: #073763;">Map</span><span style="color: #274e13;"> Maker: </span></strong><a href="https://www.raremaps.com/gallery/browse/creator_id/3418" style="border-bottom: 0px solid rgb(255, 255, 255); color: #274e13; text-decoration-line: none;">Ignace Gaston Pardies</a></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white; color: #274e13;">Fine fully colored example of this rare 17th Century map of the Southern Celestial Hemisphere, </span></span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white; color: #274e13;">originally issued in 1674 by Ignace Gastone Pardies in Paris and revised in 1690, </span></span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white; color: #274e13;">based in part on the work of the French Jesuit mathematician and astronomer Thomas Gouye (1650-1725).</span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>Os desenhos formados pelas estrelas </b></span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>- AS CONSTELAÇÕES -</b></span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, </b></span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>entre o céu e a terra... </b></span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos </b></span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>e sendo por nossa mente conscientizado. </b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>Quer dizer, </b></span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>COM UM ABRAÇO ESTRELADO,<o:p></o:p></b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>Janine Milward</b><o:p></o:p></span></div>
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<span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif;"><b>VISITE MINHA PÁGINA</b><o:p></o:p></span></div>
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<span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif;"><b>DA TERRA AO CÉU E AO INFINITO</b><o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b><span style="color: #660000;">http://daterraaoceueaoinfinito.blogspot.com.br/</span></b></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-17817526128367363942013-08-20T08:44:00.003-07:002014-10-14T05:15:37.089-07:00SCUTUM, O ESCUDO<div align="center" class="MsoNormal" style="text-align: center;">
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px; text-align: start;">Meu Projeto</span></div>
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="text-decoration: none;"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000; font-size: large;">Da Terra ao Céu ....</span></span></a></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000; font-size: large;">.....<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="text-decoration: none;">e ao Infinito </a></span></span></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="text-decoration: none;"><span style="color: #660000; font-size: large;">- As 88 Constelações</span></a></span></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000; font-size: large; text-decoration: none;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="text-decoration: none;">http://daterraaoceueaoinfinito.blogspot.com.br/</a></span><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<img src="http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_021.jpg" /><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_021.jpg</span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">O Escudo, Scutum, é uma constelação interessante</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">pois que não exatamente faz parte do Zodíaco</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">mas está sempre acolhendo a Lua e Planetas e Planetóides</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(neste momento - e já por algum bom tempo -, </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Scutum vem praticamente abrigando</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Plutão, aquele que já foi rei (Planeta) e que jamais perde sua majestade.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Leia mais em http://oceudomes.blogspot.com.br/2014/07/lua-plutao-e-new-horizons.html).</span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Scutum, o Escudo, é abrigado, digamos assim, por apenas três constelações,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">quer dizer, de um lado existe o imenso Serpentário, Ophiucus, </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e a parte da Cauda da Serpente;</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">ao norte, encontramos a belíssima Águia, Aquila;</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e, finalmente, ao sul o Escudo pode sempre tomar seu chá das cinco</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">junto ao Bule de Chá que o Sagitário, o Arqueiro, apresenta.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(Veja em</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/07/lua-e-o-bule-de-cha-em-sagitario.html)</span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgeyYgRgWbA-FcjykrwfzKhAx_as9jNY1rHtT94H3ADPL7s53uBuVuKnZB9pKRcnXmWA8UaZNP_LAzUFTAA9SZioj21NmglBHs1j884AYpa4nGfUhh53NW9vbstqRoEU_UhsbtDCU5YwG9O/s1600/scutum+e+sagit%C3%A1rio,+invertidos.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgeyYgRgWbA-FcjykrwfzKhAx_as9jNY1rHtT94H3ADPL7s53uBuVuKnZB9pKRcnXmWA8UaZNP_LAzUFTAA9SZioj21NmglBHs1j884AYpa4nGfUhh53NW9vbstqRoEU_UhsbtDCU5YwG9O/s1600/scutum+e+sagit%C3%A1rio,+invertidos.jpg" /></a></div>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_021.jpg</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Imagem invertida em suas cores originais por Janine</span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Scutum, o Escudo, é uma constelação que homenageia um rei,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é uma herança a todos nós legada até os dias de hoje.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span><br />
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<span style="color: #0f243e; font-family: Arial, sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">Ascensão Reta 18h18m / 18h56m Declinação -4<sup>o</sup>.0 / -16<sup>o</sup>.0<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">Constelação formada por Hevelius em 1690 em honra ao rei da Polônia.<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">Scutum situa-se entre as constelações Sagittarius, Aquila, Serpens</span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">R Scuti - Estrela Variável<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">Ascensão Reta 18h44m Declinação -05<sup>o</sup>.46<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">Magnitudes: Max 5,4 Min 9,0 Período 142,0<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">Tipo SPE Espectro K2v<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- </span><b><span lang="EN-US">Richard Hinckley Allen, Star Names, Their Lore and Meaning</span></b><span lang="EN-US">, Dover Publications, Inc, New York, USA <o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Richard Hinckley Allen, em seu famoso e importantíssimo livro<br />Star Names — Their Lore and Meaning -,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nos fala bem sinteticamente sobre SCUTUM:</b></span></div>
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It is pictured as the <b>Coat of Arms</b> of the third John Sobieski, king of Poland, who so distinguished himself in the defensive wars of his native land, as well as in his successful resistance of the Turks in their march on Vienna when turned back at the Kalenberg on the 12th of September, 1683. It was just after this, when he had made his triumphal entry into the city, that at the cathedral service of thanksgiving the officiating priest read the passage:</div>
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There was a man sent from God, whose name was John.<br />
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Seven years subsequently this new constellation was named for him by Hewel, with a glowing tribute to his merit and heroic deeds; the sign of the Cross for which he fought being emblazoned on his Shield as we have it to‑day. Some identify this <b>Cross</b>, however, with that of the fighting Franciscan friar, Saint John Capistrano, famous at Belgrade in 1456, and now honored by a colossal statue on the exterior of the Vienna cathedral. The four stars on the border of the Shield are for the four sons of the king.</div>
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Although Scutum is a recent creation with us, it has long been known in China as <b><span class="Chinese" style="color: rgb(218, 83, 0) !important;">Tien Pien</span></b>, the Heavenly Casque, but in this are included some components of Antinoüs.</div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;"><span style="font-size: 15px;">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Scutum_Sobiescianum*.html</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgZKHn9ml91B7lyMegM_NjCrpx5wwkEAiMLJH00AJ2Ih1orjhEnQt6vZBuFLFkagnkcF1GAjgeVX2IfrEYHuHRjWWxbGqpdaRbeH-GraOHPHX7RiGbeX9miPprm-ZfNSOMtFRL1M66dOSQv/s1600/Scutum_Sobiescianum.PNG" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgZKHn9ml91B7lyMegM_NjCrpx5wwkEAiMLJH00AJ2Ih1orjhEnQt6vZBuFLFkagnkcF1GAjgeVX2IfrEYHuHRjWWxbGqpdaRbeH-GraOHPHX7RiGbeX9miPprm-ZfNSOMtFRL1M66dOSQv/s1600/Scutum_Sobiescianum.PNG" height="509" width="640" /></a></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;"><span style="font-size: 15px;">http://en.wikipedia.org/wiki/John_III_Sobieski#mediaviewer/File:Scutum_Sobiescianum.PNG</span></span></div>
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<span class="mw-mmv-title" original-title="File name" style="background-color: white; font-size: 1.2em; max-width: 60%;">Scutum Sobiescianum</span></div>
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<span class="mw-mmv-source-author" original-title="Author and source information" style="background-color: white;"><span class="mw-mmv-author">Johannes Hevelius</span> - <span class="mw-mmv-source"><a class="external text" href="http://contentdm.lindahall.org/cdm4/document.php?CISOROOT=/star_atlas&CISOPTR=479" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">Atlas Coelestis</a>. Johannes Hevelius drew the constellation in Uranographia, his celestial catalogue in 1690.</span></span></div>
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<b>Scutum</b> (Sct), o <a href="http://pt.wikipedia.org/wiki/Escudo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Escudo">Escudo</a>, é uma <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> do <a href="http://pt.wikipedia.org/wiki/Hemisf%C3%A9rio_celestial_sul" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hemisfério celestial sul">hemisfério celestial sul</a>. O genitivo, usado para formar nomes de estrelas, é <b>Scuti</b>. Representa o escudo do rei <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Jan_III_Sobieski" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Jan III Sobieski">João III Sobieski da Polônia</a>.</div>
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As constelações vizinhas são <a href="http://pt.wikipedia.org/wiki/Aquila" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aquila">Aquila</a>, <a href="http://pt.wikipedia.org/wiki/Serpens" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Serpens">Serpens</a> (Cauda) e <a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagittarius</a>.</div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 15px; line-height: normal;">http://pt.wikipedia.org/wiki/Aglomerado_do_Pato_Selvagem</span></div>
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<b>Alpha Scuti</b> (14 Scuti) é uma <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a> na direção da <a href="http://pt.wikipedia.org/wiki/Scutum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Scutum">Scutum</a>. Possui uma <a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080;" title="Ascensão reta">ascensão reta</a> de 18h 35m 12.44s e uma <a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">declinação</a> de −08° 14′ 35.9″. Sua <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> é igual a 3.85. Considerando sua distância de 174 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>, sua <a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a> é igual a 0.21. Pertence à <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Classificação estelar">classe espectral</a> K2III.</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Alpha_Scuti</span></span></div>
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<b style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">Beta Scuti</b><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> (24 Scuti) é uma </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Estrela">estrela</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Scutum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Scutum">Scutum</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> de 18h 47m 10.48s e uma </span><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Declinação">declinação</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> de −04° 44′ 52.2″. Sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> é igual a 4.22. Considerando sua distância de 689 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> em relação à </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Terra">Terra</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">, sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> é igual a −2.41. Pertence à </span><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Classificação estelar">classe espectral</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> G5II....</span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Beta_Scuti</span></span></div>
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<b style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">Gamma Scuti</b><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> (6 Scuti) é uma </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Estrela">estrela</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Constelação">constelação</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> de </span><a href="http://pt.wikipedia.org/wiki/Scutum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Scutum">Scutum</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> de 18h 29m 11.85s e uma </span><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Declinação">declinação</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> de −14° 33′ 56.9″. Sua</span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> é igual a 4.67. Considerando sua distância de 291 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px;" title="Anos-luz">anos-luz</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> em relação à </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Terra">Terra</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">, sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> é igual a −0.09. Pertence à </span><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Classificação estelar">classe espectral</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> A1IV/V.</span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Gamma_Scuti</span></span></div>
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Em <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background: none; color: #0b0080; text-decoration: none;" title="Astronomia">astronomia</a>, as <b>variáveis δ Scuti</b> são uma classe de <a href="http://pt.wikipedia.org/wiki/Estrela_vari%C3%A1vel" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela variável">estrelas variáveis</a> com <a href="http://pt.wikipedia.org/wiki/Massa" style="background: none; color: #0b0080; text-decoration: none;" title="Massa">massas</a> entre 1,5 e 2,5 <a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Massa solar">massas solares</a>, cuja localização no <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Diagrama_HR" style="background: none; color: #0b0080; text-decoration: none;" title="Diagrama HR">diagrama HR</a> é a região de intersecção da <a href="http://pt.wikipedia.org/wiki/Sequ%C3%AAncia_principal" style="background: none; color: #0b0080; text-decoration: none;" title="Sequência principal">sequência principal</a> com a parte inferior da <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Faixa_de_instabilidade" style="background: none; color: #0b0080; text-decoration: none;" title="Faixa de instabilidade">faixa de instabilidade</a> das estrelas <a href="http://pt.wikipedia.org/wiki/Cefeida" style="background: none; color: #0b0080; text-decoration: none;" title="Cefeida">Cefeidas</a>.<span class="reference" id="cite_ref-Philip_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Delta_Scuti#cite_note-Philip-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> Esta classe estelar inclui estrelas da <a href="http://pt.wikipedia.org/wiki/Sequ%C3%AAncia_principal" style="background: none; color: #0b0080; text-decoration: none;" title="Sequência principal">sequência principal</a>, bem como estrelas que já saíram da <a href="http://pt.wikipedia.org/wiki/Sequ%C3%AAncia_principal" style="background: none; color: #0b0080; text-decoration: none;" title="Sequência principal">sequência principal</a>, mas que ainda possuem uma camada de queima de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Hidrog%C3%AAnio" style="background: none; color: #0b0080; text-decoration: none;" title="Hidrogênio">hidrogênio</a>.</div>
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São estrelas dos tipos espectrais A0–F6 e das classes de luminosidade III–V.<span class="reference" id="cite_ref-Philip_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Delta_Scuti#cite_note-Philip-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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A maioria das variáveis δ Scuti são <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Estrela_pulsante&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Estrela pulsante (página não existe)">estrelas pulsantes</a> multiperiódicas, tal como as estrelas <a href="http://pt.wikipedia.org/wiki/An%C3%A3_branca" style="background: none; color: #0b0080; text-decoration: none;" title="Anã branca">anãs brancas pulsantes</a>, porém com <a href="http://pt.wikipedia.org/wiki/Frequ%C3%AAncia" style="background: none; color: #0b0080; text-decoration: none;" title="Frequência">frequências</a> de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Pulsa%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Pulsação">pulsação</a> mais baixas, entre 50 e 600 μHz. Os <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Modo_de_pulsa%C3%A7%C3%A3o&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Modo de pulsação (página não existe)">modos de pulsação</a> são tanto <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Modo_radial&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Modo radial (página não existe)">radiais</a> quanto <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Modo_n%C3%A3o-radial&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Modo não-radial (página não existe)">não-radiais</a><span class="reference" id="cite_ref-Philip_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Delta_Scuti#cite_note-Philip-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> e são produzidos pelo <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Mecanismo_kappa&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Mecanismo kappa (página não existe)">mecanismo-κ</a> associado com a zona onde o <a href="http://pt.wikipedia.org/wiki/H%C3%A9lio" style="background: none; color: #0b0080; text-decoration: none;" title="Hélio">hélio</a> está parcialmente <a href="http://pt.wikipedia.org/wiki/Ioniza%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Ionização">ionizado</a>.</div>
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Estrelas delta Scuti oferencem uma boa oportunidade para se aplicar as ferramentas da <a href="http://pt.wikipedia.org/wiki/Asterosismologia" style="background: none; color: #0b0080; text-decoration: none;" title="Asterosismologia">asterosismologia</a> para estudar mecanismos físicos chaves que atuam durante a fase na sequência principal, como o transporte de <a href="http://pt.wikipedia.org/wiki/Momento_angular" style="background: none; color: #0b0080; text-decoration: none;" title="Momento angular">momento angular</a> e o <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Transporte_de_mat%C3%A9ria&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Transporte de matéria (página não existe)">transporte de matéria</a> nas camadas <a href="http://pt.wikipedia.org/wiki/Convec%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Convecção">convectivas</a> da estrela.</div>
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Podem também ser denominadas de por <b>cefeidas de período ultra curto</b> ou <b>cefeidas anãs</b>.<span class="reference" id="cite_ref-Philip_1-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Delta_Scuti#cite_note-Philip-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Delta_Scuti</span></span></div>
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<b style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">Epsilon Scuti</b><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> (21 Scuti) é uma </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Estrela">estrela</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Constelação">constelação</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> de </span><a href="http://pt.wikipedia.org/wiki/Scutum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Scutum">Scutum</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> de 18h 43m 31.24s e uma </span><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Declinação">declinação</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> de −08° 16′ 30.9″. Sua</span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> é igual a 4.88. Considerando sua distância de 522 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> em relação à </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Terra">Terra</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">, sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> é igual a −1.14. Pertence à </span><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Classificação estelar">classe espectral</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> G8II.</span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Epsilon_Scuti</span></span></div>
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<b style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">Zeta Scuti</b><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> (3 Scuti) é uma </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px;" title="Estrela">estrela</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Constelação">constelação</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> de </span><a href="http://pt.wikipedia.org/wiki/Scutum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Scutum">Scutum</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> de 18h 23m 39.55s e uma </span><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Declinação">declinação</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> de −08° 56′ 04.2″. Sua</span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> é igual a 4.66. Considerando sua distância de 191 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> em relação à </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Terra">Terra</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">, sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> é igual a 0.82. Pertence à </span><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Classificação estelar">classe espectral</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> K0III.</span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Zeta_Scuti</span></span></div>
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<b style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">Eta Scuti</b><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> (33 Scuti) é uma </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Estrela">estrela</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Constelação">constelação</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> de </span><a href="http://pt.wikipedia.org/wiki/Scutum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Scutum">Scutum</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> de 18h 57m 03.63s e uma </span><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Declinação">declinação</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> de −05° 50′ 46.4″. Sua</span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> é igual a 4.83. Considerando sua distância de 207 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> em relação à </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Terra">Terra</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">, sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> é igual a 0.82. Pertence à </span><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Classificação estelar">classe espectral</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> K1III.</span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Eta_Scuti</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjDYGma5O5SbfgUu9rtEIegEXWpsScGnAnMBHsdmuky6Bq-4qz6zmWmmgGy4a-23AzYWk_9sOh0UHPe-gV1EwGW04oAJX_lppSWbAaQTjw-foRuNQ-IZJIIPfS1-F9fqGatOHwB5sIJ7sg/s1600/250px-Scutum_constellation_map.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjDYGma5O5SbfgUu9rtEIegEXWpsScGnAnMBHsdmuky6Bq-4qz6zmWmmgGy4a-23AzYWk_9sOh0UHPe-gV1EwGW04oAJX_lppSWbAaQTjw-foRuNQ-IZJIIPfS1-F9fqGatOHwB5sIJ7sg/s1600/250px-Scutum_constellation_map.png" height="611" width="640" /></a></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;"><span style="font-size: 15px;">http://pt.wikipedia.org/wiki/Aglomerado_do_Pato_Selvagem</span></span></div>
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m11atlas.jpg" /></div>
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<a href="https://www.blogger.com/null" name="m81">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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Messier 11</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Open Cluster</a> M11 (NGC 6705)</i>, type 'g', in <a href="http://messier.obspm.fr/map/Sct.html">Scutum</a></center>
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<br /><b><span style="font-size: large;">Wild Duck Cluster</span></b><br /><b><span style="font-size: large;"><br /></span></b><div>
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<a href="http://messier.obspm.fr/Jpg/m11.jpg"><img align="right" alt="[m11.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m11.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">18 : 51.1 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-06 : 16 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">6.0 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">6.3 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">14.0 (arc min)</td></tr>
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Discovered 1681 by Gottfried Kirch.</div>
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Messier 11 (M11, NGC 6705) is "One of the richest and most compact of the galactic (open) clusters," to say it with Robert Burnham, Jr. ..............................</div>
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M11 was discovered by the German astronomer <a href="http://messier.obspm.fr/xtra/Bios/kirch.html">Gottfried Kirch</a> of the Berlin observatory in 1681. It was apparently first resolved into stars by <a href="http://messier.obspm.fr/xtra/similar/derham.html">William Derham</a> about 1733. <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> included it in <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M11">his catalog</a> on May 30, 1764.</div>
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LEIA MAIS</div>
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em</div>
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http://messier.obspm.fr/m/m011.html</div>
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<span style="font-family: Arial, sans-serif;"><b><span style="color: #660000;">M11 - NGC 6705 - Aglomerado Aberto, o Pato Selvagem</span></b><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Um dos aglomerados mais interessantes e ricos. </span><br />
<span style="font-family: Arial, sans-serif;">É visível na extremidade norte da Nuvem de Estrelas em Scutum, </span><br />
<span style="font-family: Arial, sans-serif;">que é parte da Via Láctea e muito mais distante do que M11.</span></div>
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<span style="font-family: Arial, sans-serif;">Ascensão Reta 18h50 Declinação -06<sup>o</sup>.08<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Magnitude fotográfica global 6,8 Magnitude fotográfica da mais brilhante estrela 12,0<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;"> Distância kpc 1,70 Diâmetro 13’ Tipo Espectral B8<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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http://pt.wikipedia.org/wiki/Aglomerado_do_Pato_Selvagem#mediaviewer/Ficheiro:Messier11.jpg</div>
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<span style="color: #660000;">O <b>Aglomerado do Pato Selvagem</b> (Messier 11, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">NGC 6705</a>)</span><span style="color: #252525;"> é um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Scutum" style="background: none; color: #0b0080; text-decoration: none;" title="Scutum">Escudo</a>. Foi descoberto pelo astrônomo alemão<a href="http://pt.wikipedia.org/wiki/Gottfried_Kirch" style="background: none; color: #0b0080; text-decoration: none;" title="Gottfried Kirch">Gottfried Kirch</a> em 1681, e o francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> incluiu o objeto em seu catálogo em 1764.</span></div>
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É um dos mais ricos e compactos aglomerados abertos conhecidos, contendo cerca de 2 900 estrelas. Sua idade é estimada em cerca de 220 milhões de anos e seu nome deriva-se de suas estrelas mais brilhantes, que formam um triângulo que podem representar um bando de <a href="http://pt.wikipedia.org/wiki/Pato" style="background: none; color: #0b0080; text-decoration: none;" title="Pato">patos</a> em formação de voo. Tem <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 6,3, sendo visível a <a href="http://pt.wikipedia.org/wiki/Olho_nu" style="background: none; color: #0b0080; text-decoration: none;" title="Olho nu">olho nu</a> apenas sob excelentes condições de observação. Suas estrelas mais brilhantes podem ser observadas em <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background: none; color: #0b0080; text-decoration: none;" title="Binóculo">binóculos</a> ou pequenos <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a>. Situa-se a 6 200 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>.</div>
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O <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> foi descoberto pelo astrônomo alemão <a href="http://pt.wikipedia.org/wiki/Gottfried_Kirch" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Gottfried Kirch">Gottfried Kirch</a>, no <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Observat%C3%B3rio_de_Berlim&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Observatório de Berlim (página não existe)">observatório de Berlim</a> em 1681. Suas estrelas mais brilhantes foram <a href="http://pt.wikipedia.org/wiki/Resolu%C3%A7%C3%A3o_de_imagem" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Resolução de imagem">resolvidas</a> por <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="William Derham">William Derham</a> em 1733. Foi listado por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> como a décima primeira entrada de seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catálogo</a> em 30 de maio de 1764.<span class="reference" id="cite_ref-seds_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Aglomerado_do_Pato_Selvagem#cite_note-seds-1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Aglomerado do Pato Selvagem</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier11.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 11"><img alt="Messier 11" data-file-height="387" data-file-width="516" src="http://upload.wikimedia.org/wikipedia/commons/thumb/d/da/Messier11.jpg/250px-Messier11.jpg" height="188" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/d/da/Messier11.jpg/375px-Messier11.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/d/da/Messier11.jpg/500px-Messier11.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Messier 11</td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Gottfried_Kirch" style="background: none; color: #0b0080; text-decoration: none;" title="Gottfried Kirch">Gottfried Kirch</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1681" style="background: none; color: #0b0080; text-decoration: none;" title="1681">1681</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Scutum" style="background: none; color: #0b0080; text-decoration: none;" title="Scutum">Scutum</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">18<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 51<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 06,00<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">-06° 16′ 00,0″</td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">6 200 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (1.9 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">6,3</td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">14',0</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Idade estimada</td><td style="background-color: #f8f8f8;">220 milhões de anos</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 6705</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado do Pato Selvagem"><img alt="Aglomerado do Pato Selvagem" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; vertical-align: middle;" width="15" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Scutum_constellation_map.png" style="background: none; color: #0b0080; text-decoration: none;"><img alt="Scutum constellation map.png" data-file-height="1709" data-file-width="1789" src="http://upload.wikimedia.org/wikipedia/commons/thumb/2/22/Scutum_constellation_map.png/250px-Scutum_constellation_map.png" height="239" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/22/Scutum_constellation_map.png/375px-Scutum_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/22/Scutum_constellation_map.png/500px-Scutum_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/Aglomerado_do_Pato_Selvagem">http://pt.wikipedia.org/wiki/Aglomerado_do_Pato_Selvagem</a></span></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;"><span style="font-size: 15px;">http://pt.wikipedia.org/wiki/Aglomerado_do_Pato_Selvagem#mediaviewer/Ficheiro:PSM_V60_D304_Star_cluster_messier_11_and_the_surrounding_milky_way.png</span></span><span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;"> </span></div>
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<a href="https://www.blogger.com/null" name="m81" style="color: black; font-family: 'Times New Roman'; font-size: medium; line-height: normal;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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<h1>
Messier 26</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Open Cluster</a> M26 (NGC 6694)</i>, type 'f', in <a href="http://messier.obspm.fr/map/Sct.html">Scutum</a></center>
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<a href="http://messier.obspm.fr/Jpg/m26.jpg"><img align="right" alt="[m26.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m26.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">18 : 45.2 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-09 : 24 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">5.0 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">8.0 (mag)</td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">15.0 (arc min)</td></tr>
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Discovered by Charles Messier in 1764.</div>
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Open cluster Messier 26 (M26, NGC 6694) is not so impressive as its apparent neighbor, <a href="http://messier.obspm.fr/m/m011.html">M11</a>. Its discoverer <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, who <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M26">cataloged it</a> on June 20, 1764, even noted that it was "not distinguished in a 3.5 foot (FL) telescope and needed a better instrument."</div>
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LEIA MAIS</div>
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em</div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;"><span style="font-size: 15px; line-height: 22.3999996185303px;">http://messier.obspm.fr/m/m026.html</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiJ5Nv9-LLd7YfLbYUa6elnPsUE-HayTLmdS3H_xXHjhdI5SRUO9ROSe5IJteOcxyVoazIXJ3upSbSxLAJto5sejLyfIHQ92SLE0Yw-k9w2O4lyKVLXKnBz0Pe6UuTBklynD4B2lXoyhgY/s1600/m26.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiJ5Nv9-LLd7YfLbYUa6elnPsUE-HayTLmdS3H_xXHjhdI5SRUO9ROSe5IJteOcxyVoazIXJ3upSbSxLAJto5sejLyfIHQ92SLE0Yw-k9w2O4lyKVLXKnBz0Pe6UuTBklynD4B2lXoyhgY/s1600/m26.png" /></a></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;"><span style="font-size: 15px; line-height: 22.3999996185303px;">http://www.stellarium.org/pt/</span></span><br />
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<span style="color: #660000;"><b>Messier 26</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">NGC 6694</a>)</span><span style="color: #252525;"> é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado estelar aberto</a>, integrante do <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo Messier">Catálogo Messier</a>. Ésta localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Scutum" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Scutum">Escudo</a> e foi descoberto por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a>em <a href="http://pt.wikipedia.org/wiki/1764" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1764">1764</a>.</span></div>
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O aglomerado estende-se por 22 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> e está a uma distância de 5 000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>. Sua estrela mais brilhante tem <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 11,9 e tem aproximadamente 89 milhões de anos..</div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Messier 26</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_026_2MASS.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 26, projeto 2MASS"><img alt="Messier 26, projeto 2MASS" data-file-height="1204" data-file-width="842" src="http://upload.wikimedia.org/wikipedia/commons/thumb/1/1b/Messier_026_2MASS.jpg/250px-Messier_026_2MASS.jpg" height="357" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/1b/Messier_026_2MASS.jpg/375px-Messier_026_2MASS.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/1/1b/Messier_026_2MASS.jpg/500px-Messier_026_2MASS.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Messier 26, projeto <a href="http://pt.wikipedia.org/wiki/2MASS" style="background: none; color: #0b0080; text-decoration: none;" title="2MASS">2MASS</a></td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1764" style="background: none; color: #0b0080; text-decoration: none;" title="1764">1764</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Scutum" style="background: none; color: #0b0080; text-decoration: none;" title="Scutum">Scutum</a></td></tr>
<tr style="vertical-align: top;"><td>Tipo</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">Aglomerado estelar aberto</a> (II,2,r)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">18<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 45<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 12,00<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">-9° 24′ 00,0″</td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">5 000 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (1 533 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">parsecs</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">8,0</td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">15',0</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">22 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a></td></tr>
<tr style="vertical-align: top;"><td>Idade estimada</td><td style="background-color: #f8f8f8;">89 milhões de anos</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 6694</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 26"><img alt="Messier 26" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; vertical-align: middle;" width="15" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Scutum_constellation_map.png" style="background: none; color: #0b0080; text-decoration: none;"><img alt="Scutum constellation map.png" data-file-height="1709" data-file-width="1789" src="http://upload.wikimedia.org/wikipedia/commons/thumb/2/22/Scutum_constellation_map.png/250px-Scutum_constellation_map.png" height="239" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/22/Scutum_constellation_map.png/375px-Scutum_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/22/Scutum_constellation_map.png/500px-Scutum_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_26</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiCFqeDrP-ycY7LR4v0v99h6YeF9MtxWPSrdjlkjiHNCNNVSKlAApadEp7P_UkB6KWqq7ovpnReHVmXXbDTI_-4LXiv33hBRUi-EGP3X8P2UdlD-wudbRai75ev0YQtrPY5ltnDIUBoxfg/s1600/250px-Messier_026_2MASS.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiCFqeDrP-ycY7LR4v0v99h6YeF9MtxWPSrdjlkjiHNCNNVSKlAApadEp7P_UkB6KWqq7ovpnReHVmXXbDTI_-4LXiv33hBRUi-EGP3X8P2UdlD-wudbRai75ev0YQtrPY5ltnDIUBoxfg/s1600/250px-Messier_026_2MASS.jpg" height="640" width="448" /></a></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Messier_26#mediaviewer/Ficheiro:Messier_026_2MASS.jpg</span></span></div>
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<span class="mw-mmv-author" style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; font-size: 13px; line-height: 24px;">Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation.</span><span style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; font-size: 13px; line-height: 24px;"> - </span><span class="mw-mmv-source" style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; font-size: 13px; line-height: 24px;"><a class="external text" href="http://www.ipac.caltech.edu/2mass/gallery/messiercat.html" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">2MASS Atlas Image Gallery: The Messier Catalog</a></span></div>
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<b style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">NGC 6683</b><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Scutum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Scutum">constelação de Scutum</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="John Herschel">John Herschel</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> em 1827, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Telescópio">telescópio</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> (+9,4), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Telescópio">telescópios</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> amadores ou com equipamentos superiores.</span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/NGC_6683</span></span></div>
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<b style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">NGC 6625</b><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Scutum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Scutum">constelação de Scutum</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px;" title="John Herschel">John Herschel</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> em 1826, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Telescópio">telescópio</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> (+9), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Telescópio">telescópios</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> amadores ou com equipamentos superiores.</span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/NGC_6625</span></span></div>
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<b style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">NGC 6704</b><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado estelar aberto</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Scutum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Scutum">constelação do Estudo</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">. Foi descoberto pelo astrônomo alemão </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Friedrich_August_Theodor_Winnecke&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Friedrich August Theodor Winnecke (página não existe)">Friedrich August Theodor Winnecke</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> em 1854. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> (+9,2), é visto mesmo com pequenos </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Telescópio">telescópios</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> amadores ou com equipamentos maiores.</span></div>
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http://pt.wikipedia.org/wiki/NGC_6704</div>
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<b style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">NGC 6664</b><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Scutum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Scutum">constelação de Scutum</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px;" title="William Herschel">William Herschel</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> em 1784, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Telescópio">telescópio</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> (+7,8), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Telescópio">telescópios</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> amadores ou com equipamentos superiores.</span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/NGC_6664</span></span></div>
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<b style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">NGC 6649</b><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Scutum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Scutum">constelação de Scutum</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="John Herschel">John Herschel</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> em 1835, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Telescópio">telescópio</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> (+8,9), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Telescópio">telescópios</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> amadores ou com equipamentos superiores.</span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/NGC_6649</span></span></div>
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<b style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">NGC 6712</b><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Scutum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Scutum">constelação de Scutum</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="William Herschel">William Herschel</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> em 1784, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Telescópio">telescópio</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> (+8,1), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Telescópio">telescópios</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> amadores ou com equipamentos superiores</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC 6712: Galactic Globular Cluster </b><br /><b>Credit: </b>G. De Marchi, F. Paresce, B. Leibundgut, L. Pulone, (<a href="http://www.eso.org/">European Southern Observatory</a>)</span></center>
<span style="font-family: Arial, Helvetica, sans-serif;"><b>Explanation: </b>Following orbits which loop <a href="http://www.limber.org/globs.html">high above the galactic plane</a>, globular star clusters are probably 12 to 14 billion years old - <a href="http://apod.nasa.gov/apod/ap990117.html">truly ancient denizens</a> of our Milky Way Galaxy. After analyzing these new <a href="http://apod.nasa.gov/apod/ap960901.html">ESO/VLT</a> images of portions of the globular cluster NGC 6712, <a href="http://www.eso.org/outreach/press-rel/pr-1999/pr-04-99.html">astronomers report that</a> this dense grouping of about 1 million stars seems to be slowly dissolving - steadily loosing fainter, lower mass stars into our Galaxy's halo. Their results offer strong evidence for <a href="http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1997ApJ...474..223G&db_key=AST&high=34f6e1de7f29652">gravitational stripping</a> of stars from clusters which pass through the plane and central regions of the Galaxy. One of <a href="http://physun.physics.mcmaster.ca/GC/mwgc.dat">about 150 globular clusters</a> known to be members of the Milky Way, NGC 6712 is thought to have <a href="http://www.eso.org/outreach/press-rel/pr-1999/phot-06c-99-preview.jpg">crossed through</a> the crowded galactic plane only a few million years ago. NGC 6712 is about 23,000 light-years away in the <a href="http://www.astro.wisc.edu/~dolan/constellations/constellations/Scutum.html">southern constellation Scutum</a>.</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">http://www.astro.wisc.edu/~dolan/constellations/skycharts/sct.gif</span><br />
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<b><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas são como janelas que se abrem para a infinitude do universo </span></b><br />
<b><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, </span></b><br />
<b><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">entre o céu e a terra...; </span></b><br />
<b><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">bem como percebendo que o caos, vagarosamente, </span></b><br />
<b><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">vai se tornando Cosmos e sendo por nossa mente conscientizado. </span></b></div>
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<b><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></b></div>
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<b><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">COM UM ABRAÇO ESTRELADO,</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Pata selvagem/domesticada</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">no Sítio das Estrelas</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">photo by Janine</span></div>
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The Wide Field Imager (WFI) on the MPG/ESO 2.2-metre telescope at the La Silla Observatory in Chile has taken this beautiful image of the open Wild Duck Cluster, Messier 11, or NGC 6705. The blue stars in the centre of the image are the young, hot stars of the cluster. The surrounding redder stars are older, cooler background stars.</div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-8462745163618223962013-08-20T08:42:00.000-07:002014-10-20T11:01:18.297-07:00VIRGO, A VIRGEM<div align="center" class="MsoNormal" style="text-align: center;">
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Meu Projeto DA TERRA AO CÉU E AO INFINITO</span></span></h3>
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<b><i><span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763;">Janine Milward</span></span></i></b></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><b>Da Terra ao Céu e ao Infinito</b> </span><span style="font-family: Arial, Helvetica, sans-serif;">é um Projeto meu que se propõe trazer ao conhecimento do Caminhante do Céu, do Amigo das Estrelas, as 88 Constelações acolhendo seus dados, seus mitos, suas histórias, suas estrelas, suas nebulosas, seus aglomerados globulares e abertos, seus aglomerados de galáxias, seus superaglomerados...., suas muralhas de luz e de sombra...., enfim, tudo aquilo que astronomicamente pode caber em nossos alfarrábios - ou pelo menos, tudo aquilo que eu, Janine, simples amante dos céus estrelados, conseguir amealhar a partir de minha compreensão ainda e sempre simplesmente amadora e respeitosamente braheana.</span></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="text-align: start;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo </span><span style="text-align: start;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...; </span>bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; text-align: start;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.atlasoftheuniverse.com/galchart.html" style="text-decoration: none;"> </a><img src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhQCm0iCY_TUhbqNyKVtSsY2MDixSbjNT43o_i8ndOzJkIw1TogBZ7GQNdwCa8zYAo4D54jDX4SS_apMBTvEEolhg8p7XtTfIjaZO6bq4jSEBSZ_rkK993Pjt4Pm-XyqTk6djxM5S6eu9mM/s400/mapa+do+universo+que+vemos+em+positivo.gif" height="300" style="-webkit-box-shadow: rgba(0, 0, 0, 0.498039) 1px 1px 5px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.498039) 1px 1px 5px; padding: 8px;" width="400" /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Fonte da Imagem: </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.atlasoftheuniverse.com/galchart.html<span style="text-align: start;"> </span><a href="http://www.atlasoftheuniverse.com/me.html" style="text-align: start; text-decoration: none;">Richard Powell</a><span style="text-align: start;">.</span></span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">VIRGO, A VIRGEM</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Acessando o Link abaixo, o Leitor encontrará uma Página própria</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">acolhendo Virgo, a Virgem:</span></div>
<span style="background-color: white; color: #073763;"><a href="http://sobrevirgo.blogspot.com/" style="font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 15px; font-weight: bold; line-height: 23px; text-decoration: none;"><b><span style="font-family: Arial, sans-serif;">http://sobrevirgo.blogspot.com/</span></b></a><span style="font-family: Arial, sans-serif; font-size: 15px; font-weight: bold; line-height: 23px;"> </span></span><br />
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><strong><span style="font-family: Arial, Helvetica, sans-serif; font-size: large;">O Mito</span></strong></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Compilação</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e Tradução (quando necessário)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e escrita (em alguns comentários):</span></div>
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<i><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></i></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação representa Erigone, filha de Icarius, que se enforcou por causa da grande dor causada pela morte de seu pai. Outros dizem que é Astraea, filha de um dos Titans, e que lutou com alguns deuses contra seu próprio pai.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Em outra versão, esta constelação representa Perséfone, filha da irmã de Júpiter, Ceres, (Demeter). Ceres é a deusa da agricultura e aquela que ensinou aos homens plantarem o trigo, colherem e fazerem o pão que os alimenta. (A Estrela-Alpha Virgo representa a espiga de trigo, é Spica). </span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Um belo dia, Perséfone estava colhendo flores no campo e foi avistada por Plutão, o deus dos mundos ínferos, que por ela se apaixonou perdidamente e com ela quis se casar e de tal forma que a raptou e a levou para os mundos ínferos, onde habitava.</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando Ceres descobriu que Plutão havia raptado sua filha, foi até os mundos ínferos para busca-la e traze-la de volta à Terra, porém em vão.</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ceres ficou tão entristecida que não mais quis tomar conta da agricultura da Terra e nada cresceu no solo naquele tempo e os homens ficaram famintos, à beira da morte.</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Júpiter, então, teve que intervir nesta situação e anunciou à Ceres que sua filha poderia retornar ao seu lado - desde que não comesse absolutamente nada enquanto ainda estivesse nos mundos ínferos. No entanto, Plutão ofereceu alguns grãos de romã à Perséfone e que os comesse de maneira que levasse uma boa memória de seu marido e de sua vida nos mundos ínferos. </span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando Ceres soube do ocorrido, Perséfone já havia sido trazida dos mundos ínferos por Mercúrio e encontrado-se com sua mãe. Neste caso, Ceres foi informada que estaria sendo acompanhada por sua filha durante 8 meses no ano - Primavera, Verão e Outono - e os demais 4 meses, sofreria a ausência de Perséfone que estaria retornando aos mundos ínferos e ao encontro de seu marido Plutão: é o Inverno.</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">De qualquer forma, Ceres ficou feliz e trouxe a vida da alimentação novamente à Terra e aos homens.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">No vale do Eufrates, onde foram criadas as constelações, a Virgem simbolizava a deusa Istar, filha do céu e rainha das estrelas. Representada com uma espiga na mão, constituía o símbolo da fertilidade. </span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Erastosthenes identificou a Virgem com Isis, a deusa de mil-nomes, com a espiga de trigo em sua mão e que foi mais tarde deixada cair de maneira a formar a Via Láctea, ou segurando em seus braços seu filho Horus, o deus do sol, o último dos reis divinos. </span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Este simbolismo antigo reapareceu na Idade Média como a Virgem Maria com seu filho Jesus e através as palavras eternas de Shakespeare: <i>Good Boy in Virgo’s lap (O Bom Menino no Colo da Virgem).</i></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Na Índia, Virgo era Kanya, a mãe do grande Krishna, e representada como deusa sentada diante do fogo. </span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">No Zodíaco Cingalês, era a Mulher no Navio e segurando um ramo de trigo em sua mão. Possivelmente, o navio era nomeado a partir das estrelas Beta, Eta, Gamma, Delta e Epsilon, representando a quilha do navio.</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Na Pérsia, Virgo era Khosha, o ramo de trigo, bem como nomeada como a Virgem inteiramente Pura.</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os turcomanos conheciam esta constelação como a Pura Virgem, Dufhiza Pakhiza. Os chineses a conheciam como She Sang Neu, a Donzela Frígida.</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">No pais dos Judeus, a Virgem era Bethulah e sempre associada com a idéia de abundância na colheita.</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Virgem tem sempre sido a figura dos céus mais nomeada e mais simbolizada!</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Virgem representa a mais antiga e puramente alegórica representação de inocência e de virtude.</span></div>
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<tr><td><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhk9jh5sGZbeAgRzWPHZkAlUzRGMYrHtzoPZgMcxsMewvovUMQyY06SDPd2Y2mMT7uN6D9xDWdqAASuLjPiFcvm-LT4b4xbijmi8OtvXk9_e_U64nK05I8-kzSabK1mThXSLnuJZQYPzkE/s1600/VIRGEM++deitada.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhk9jh5sGZbeAgRzWPHZkAlUzRGMYrHtzoPZgMcxsMewvovUMQyY06SDPd2Y2mMT7uN6D9xDWdqAASuLjPiFcvm-LT4b4xbijmi8OtvXk9_e_U64nK05I8-kzSabK1mThXSLnuJZQYPzkE/s640/VIRGEM++deitada.jpg" hca="true" height="456" width="640" /></span></a></td></tr>
<tr><td class="tr-caption" style="font-size: 13px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Carta Celeste realizada por Mario Jaci Monteiro - CARJ</span></td></tr>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Algumas Informações Interessantes acerca a</span></b><br />
<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">CONSTELAÇÃO DA VIRGEM</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação é imensa e cortada pelas Linhas da Eclíptica e pela do Equador Celestial. Existe o entrelaçamento destas duas Linhas - o que podemos traduzir como o Ponto do Equinócio de Outono, que acontece bem próximo à estrela Beta Virginis, Zavijava, situada na cabeça da Virgem. (É interessante conhecermos o fato de que o eclipse solar de 21 de setembro de 1922, aconteceu próximo a esta estrela e que foi por Einstein usada para confirmar sua teoria).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Em termos da Linha da Eclíptica e advindos da constelação do Leão, realizam seus caminhos aparentes o Sol e a Lua e os Planetas, adentrando todos pela Cabeça da Virgem, bem próximos à estrela Beta, Zavijava, e então passando pelo ombro e pelo peito, encontrando Zaniah, e, já na altura da Cintura, situa-se a belíssima Porrima. Todas essas situações são testemunhadas pelas constelações da Taça e do Corvo, na fronteira ao sul. Spica, o ramo de trigo na mão da Virgem, é praticamente o último momento em que a linha da Eclíptica toca realmente o corpo virginal, seguindo em direção à constelação da Balança e tendo a Hydra como fronteira ao sul. </span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Em termos da Linha do Equador, é interessante observarmos o fato de que esta corta praticamente ao meio a figura delineada da Virgem, desde sua cabeça, seus cabelos, passando por seu rosto, por seu pescoço e ombros e entre seus peitos e avançando até encontrar a cintura e ainda descendo por uma de suas pernas até situar-se no entrecruzamento de suas panturrilhas e deixando a Virgem depois de tocar em um de seus pés.</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O ponto de entrecruzamento das Linhas da Eclíptica e do Equador perfaz o Equinócio do Outono e isso acontece no lugar que aponta bem proximamente entre o cabelo e o rosto da Virgem.</span><br />
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<tr><td class="tr-caption" style="font-size: 13px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ilustração realizada no Programa Stellarium e trabalhada no Corel</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Primavera para o hemisfério sul, em setembro 2013</span></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Para que bem possamos compreender a figura delineada da Virgem, algumas estrelas poderão nos servir como referência: Spica, Alpha Virginis, apresenta o ramo de trigo carregado pela mão já ao sul da linha da Eclíptica, com a Hidra como testemunha; Zavijava, Beta Virginis, aponta para o alto de sua cabeça, possivelmente já na altura da testa, com o Leão como testemunha; Zaniah situa-se em um de seus peitos e Porrima, em sua cintura. Caphir situa-se no cotovelo do braço esquerdo da Virgem e Vindemiatrix no ponto onde a mão esquerda segura seus longos cabelos, com a Cabeleira de Berenice como testemunha. Heze situa-se na coxa da perna esquerda e Syrma, entre o joelho e a panturilha da perna direita. Finalmente, Shambaliah situa-se ao pé da Virgem. O Boeiro e a Cabeça da Serpente testemunham a perna esquerda e os pés da Virgem, respectivamente.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Existe também a interpretação de um Canil, formado pelas estrelas Beta, Eta, Gamma, Alpha, Zeta, Epsilon e Delta Virginis. Eu diria que esta figura formada também pode ser compreendida como uma pandorga, papagaio, pipa soltada ao vento e ganhando os céus...</span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">A CONSTELAÇÃO DA VIRGEM</span></b><br />
<strong><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Posicionamento e Fronteiras</span></strong><br />
<strong><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Observação a Olho Nú, através Binóculos e Telescópios </span></strong></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">POSICIONAMENTO:</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 11h35m / 15h8m Declinação +16<sup>o</sup>.6 / -22<sup>o</sup>.2</span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Fronteiras:</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Virgo situa-se entre as constelações</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Libra, Serpens, Bootes, Coma Berenices, Leo, Crater, Corvo, Hydra</span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Observação a olho nú ou através binóculos e/ou telescópios:</span></b><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Virgem é uma constelação muitíssimo interessante de ser observada, por várias razões:</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A olho nú e em lugares de céus escuros e transparentes, podemos observar a presença de muitas estrelinhas pouco luminosas espraiadas ao longo de uma imensa região do céu ocupada por esta constelação - com a exceção de suas estrelas Alpha, Beta e Gamma - Spica, Zavijavah e Porrima -, respectivamente, todas três situadas bem próximas à Linha da Eclíptica e, dessa forma, sendo visitadas com freqüência pela Lua bem como pelo Sol uma vez ao ano e pelos Planetas em suas trajetórias ao longo do Zodíaco. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Spica é uma estrela que sempre chama atenção por seu brilho e sua altivez. Um tantinho ao norte, outra estrela acompanha e rivaliza com Spica: é Arcturus, a estrela Alpha do Boieiro. Ainda antes da chegada de Spica, o Corvo, em seu vôo elipsal voltado para o sul, vem anunciando a Virgem. Em termos das constelações do Zodíaco, o garboso Leão antecede a Virgem e realmente seu desenho de estrelas é bem impressionante e bem marcado pela estrela Alpha Regulus, o pé do rei dos animais, e pela estrela Beta Denebola, sua cauda. Entre o Leão e o Boeiro, encontraremos um pedaço do céu que é verdadeiramente maravilhoso: a Cabeleira de Berenice, com suas tímidas estrelinhas formando suas sedosas mechas - espetáculo que pode ser visualizado somente em lugares de céus escuros e transparentes, com toda a certeza. E a Virgem é seguida pela Balança, constelação que se evidencia por suas duas estrelas ponteadoras dos pratos a serem bem equilibrados, Zubenelzenubi e Zubenelschemalli. A Balança marca a presença do Escorpião - de tal forma que, antigamente, as estrelas Alpha e Beta Librae eram consideradas como as Garras do Escorpião. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Para quem pode usufruir de morar ou visitar lugares de céus escuros e transparentes, é sempre muito interessante se poder acompanhar o enredilhado rastejador das tímidas estrelinhas da Hydra, com sua cabeça apontando para a também tímida constelação de Câncer acolhendo seu maravilhoso Presépio, berço de estrelas-bebês que viajam juntas, e com seu coração batendo intensamente através sua estrela Alpha, Alphard, e seu corpo seguindo enredilhando e rastejando apresentando o sul para o Leão, para a Taça, para o Corvo, para a Virgem..., indo terminar na Balança.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Alguns mapas celestes nos mostram um dos pés da Virgem já adentrando a constelação da Balança e é interessantíssimo se notar o fato de que neste lado do céu surge a figura estranha da Cabeça da Serpente, belíssimo asterismo a ser observado apenas em lugares de céus escuros e transparentes. A Cabeça da Serpente parece estar guardando tanto os pés da Virgem quanto, e fundamentalmente, a Coroa Boreal, espetáculo de retirar o fôlego, pequeno arco de estrelas situado entre o Boeiro e o Herói Sentado, Hercules.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Como vimos, a observação a olho nú da Virgem e seus arredores é realmente muito interessante e nos apresenta um belíssimo canto dos céus estrelados!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Virgem é a maior constelação dentre as 13 que fazem parte do Zodíaco, a Roda dos Animais: o Sol caminha pela Virgem do dia 14 de setembro ao dia 29 de outubro.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mal o Sol, em seu aparente percurso, deixa a constelação do Leão e adentra a constelação da Virgem, acontece o ponto de entrelaçamento das Linhas do Equador Celestial e da Eclíptica e esse é o momento da chegada da Primavera para o hemisfério sul e do Outono para o hemisfério norte. Este ponto encontra-se bem próximo à estrela Beta Virginis, Zavijavah. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mesmo que não vejamos esse momento - a não ser que aconteça algum eclipse total do Sol.... - é sempre interessante que possamos ter esse conhecimento sobre a constelação da Virgem. Sorte teve Albert Einstein: esta foi a estrela por ele usada para confirmar sua teoria, durante o eclipse solar de 21 de setembro de 1922, que aconteceu próximo a esta estrela. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Em termos de uso de binóculos, penso que possivelmente muitos daqueles objetos mencionados mais adiante neste Trabalho estarão se apresentando mais como nebulosas ou aglomerados abertos e globulares... do que como galáxias ou conjunto/aglomerados de galáxias...., mas sei dizer com toda a certeza que, através telescópios - amadores e menos potentes e/ou profissionais e mais e mais potentes e ainda todo um cabedal de infraestrutura tecnológica sempre modernizada e atualizada e disposta a exercer o avanço do conhecimento do espaço profundo - esta é a região mais rica, mais provocante, mais desafiadora e mais densa dos céus estrelados em termos de observação de suas tantas e tantas Galáxias e, fundamentalmente, do Aglomerado de Galáxias de Virgem, o mais próximo a nós!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Richard H. Allen nos diz que Sir William Herschel, em seu tempo de um passado ainda não tão distante de nós, encontrou entre a estrela Denebola, Beta Leonis, e as estrelas Beta, Gamma, Eta e Delta Virginis nada menos do que 323 nebulosas, que mais tarde foram acrescidas para mais de 500 - ou seja, muito mais nebulosas do que as estrelas vistas a olho nu nesta constelação. Ao longo dos tempos, a maior parte dessas ‘nebulosas’ vêm se transformando em aglomerados, em galáxias, em conjunto de galáxias... (Eu, Janine, tive a felicidade de visitar Bath, na Inglaterra, cidade adotada por Herschel para morar e para apontar seu telescópio para o céu estrelado e descobrir Urano!).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A bem da verdade, a Virgem vem sempre nos surpreendendo a respeito dos objetos que, a partir de seu delineamento enquanto constelação, são buscados, encontrados, catalogados. A cada avanço na tecnologia de busca no espaço profundo - lentes gravitacionais, redshifts, telescópios poderosos na Terra e no Céu..., etc., etc., etc. -, mais e mais objetos são trazidos à tona do nosso conhecimento, para nosso total embevecimento. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Em relação a aquilo que podemos nomear enquanto Aglomerado de Galáxias de Virgem, existe já a insistência de não somente acolher este Aglomerado junto a alguns tantos outros pertencentes ao nosso Grupo Local e formar aquilo que denominamos enquanto Superaglomerado Local..., como a de se fazer este ser conhecido como Superaglomerado Virgo!... - mesmo que este Superaglomerado não seja estimado como pertencente ao rank dos grandes superaglomerados.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">De tal forma a astronomia nos surpreende com seus passos avançando astronomicamente através o tempo e o espaço, que começa a surgir em nossa mente a possibilidade de que possam existir Aglomerados de Superaglomerados em nosso Universo! </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O que me comove na ciência da Astronomia é o fato de que não existem nem começo nem fim..., ou seja, jamais poderemos literalmente ver o Big Bang (porque estamos nele inseridos!) e jamais poderemos literalmente ver todas as possíveis e as também impossíveis, imaginadas ou inimaginadas, transmutações que o Universo vai sempre fazendo acontecer! Na Astronomia, não existem passado, presente e futuro... existe apenas o aqui-e-agora nesse tempo e nesse espaço que ora vivenciamos, apenas isso. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(Sonhando.....) Se um dia eu puder me evadir do Planeta Terra e viajar ainda para além do nosso quintal do nosso Sistema Solar..., levarei comigo não Beethoven e sim Mozart (com todo meu respeito a Beethoven) e uma pequena edição (com a tradução de Wu Jyh Cherng do chinês para o português) dos 81 capítulos do Livro do Caminho e da Virtude, de Lao Tse, o Mestre do Tao. A meu ver, Mozart e Lao Tse fazem parte da música e da compreensão da vida despidas de passado, presente e futuro, apenas esta interseção do tempo e do espaço nesse momento de minha vida, sempre.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">................ É por esta e por outras tantas razões, que venho nomeando este meu Trabalho de <b>Da Terra ao Céu e ao Infinito</b>. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Este meu Trabalho pressupõe trazer ao conhecimento do Caminhante do Céu, do Amigo das Estrelas, as 88 Constelações acolhendo seus dados, seus mitos, suas histórias, suas estrelas, suas nebulosas, seus aglomerados globulares e abertos, seus aglomerados de galáxias, seus superaglomerados...., muralhas de luz e de sombra..., etc., etc., etc., enfim, tudo aquilo que astronomicamente pode caber em nossos alfarrábios - ou pelo menos, tudo aquilo que eu, Janine, simples amante dos céus estrelados, conseguir amealhar a partir de minha compreensão ainda e sempre amadora e braheana.</span></div>
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<span style="background-color: white; line-height: 22.3999996185303px;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>em Virgem</b></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Spica</b>. Alpha Virginis. </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 13h 24,1m Declinação -11<sup>o</sup> 03’</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual 1,21 - Distância 220 anos-luz
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela binária branco brilhante no ramo de trigo que a Virgem carrega em sua mão voltada para o sul.
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Freqüentemente chamada de <b>Arista </b>(nome também usado para designar esta constelação) e também conhecida como Azimech.
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> Os hindus a conheciam como Citrã, a 12<sup>a</sup>. Nakshatra, como se fosse uma Lâmpada ou uma Pérola.
Na Babilônia e representando toda a constelação, era personifica como a Esposa de Bel ou a Guirlanda da Virgem.
Para os chineses, Spica significava a grande favorita, Kió, a estrela da primavera.
Era conhecida no Egito como Repã, o Senhor, e em tempos 3200 AC, um templo em Tebas foi erigido orientada através o poente de Spica.
Da mesma forma, já em 2000 AC, assim aconteceu para o templo do Sol. Também assim aconteceu para dois templos na Grécia construídos quase tocando um ao outro, erigidos em 1092 e 747 AC. Outros templos na Grécia antiga apresentaram a mesma orientação.</span></span></div>
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Foi através da observação desta estrela bem como de Regulus em cerca de 300 AC, anotada pelo alexandrino Timochares, que, após comparação com seus próprios apontamentos 150 anos mais tarde, Hiparchos trouxe para si o crédito de sua grande descoberta acerca a precessão dos equinócios - mesmo que os apontamentos da Babilônia e as orientações de construção dos templos no Egito e na Grécia, indicaram um conhecimento prático sobre esta questão.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Zavijava</b>. Beta Virginis. </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude 3.8</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela amarelo pálido situada na cabeça da Virgem. </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">De Al Zawiah, o Ângulo, o Canil, o Recanto dos dois Vigias (possivelmente pelo fato de se encontrar bem próxima ao ponto do Equinócio do Outono) - porém também nomeada como A Gloriosa, A Bela. </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Os árabes chamavam esta estrela como Mashaha e os chineses, de Yew Chi Fa, a Mão Direita do Mantenedor da Lei.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta foi a estrela usada por Einstein para confirmar sua teoria, durante o eclipse solar de 21 de setembro de 1922, que aconteceu próximo a esta estrela. </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Porrima</b> - Gamma Virginis - <b>Estrela Dupla</b></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">AR 12h39m Dec. - 01<sup>o</sup>.11</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Nome latino da deusa da Profecia. Os Latinos a chamavam também de Antevorta ou mesmo algumas vezes Postvorta, nomes de duas antigas deusas da profecia, irmãs e assistentes de Carmentis, venerado e invocado por suas mulheres.
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta estrela Gamma foi especialmente menciondo como sendo Zaviat al Awwã, o Ângulo ou Esquina - Gamma situando-se a meio caminho entre Spica e Denebola, os lados do Canil estendendo-se ao norte e ao oeste e sendo marcado pelas estrelas Eta e Beta, Delta e Epsilone.
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Na Babilônia era Kakkab Dan-nu, a Estrela do Herói - como um ponto de referência em seus anais de observação de Saturno, no primeiro dia de março do ano 228 AC, a primeira menção sobre este planeta e anotada por Ptolomeu.
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Os chineses conheciam esta estrela como Shang Seang, o Alto (Primeiro) Ministro de Estado.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Caphir</b>. Delta Virginis. </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela branca (em outra versão, amarelo dourado) binária e vagamente variável no braço esquerdo (cotovelo) da Virgem. Também chamada de Uma Inesperada Oferta ou Aquela que é Submissa. Esta estrela é conhecida como Auva ou Minelauva.
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">No Eufrates, era conhecida como Lü Lim, a Gazela, a Cabra - ou mesmo o Rei. Os hindus a chamavam Apa, as Águas, e os chineses, Tsze Seang, o Segundo Ministro de Estado.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Vindemiatrix</b>. Epsilon Virginis. </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude 2.86 Distância 90 anos-luz</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">É uma estrela que situa-se na mão esquerda da Virgem segurando seus longos cabelos.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Vindemiatrix ou Vindemiator, A Vindimadora, Aquele que Colhe Uvas, representa Ampelos, filho de um sátiro e de uma ninfa, a quem Baco presenteou com uma vindima. Enquanto colhia as uvas, Ampelos caiu e quebrou o pescoço, e por isso, Baco colocou-o entre as estrelas em lembrança de seu afeto. A Vindimadora, nome de origem latina registrado nas Tábuas Afonsinas. Também conhecida como Almuredin.
Na China, era conhecida como Tsze Tseang, o Segundo General.
No Eufrates, Kakkb Mulu-izi, a Estrela do Homem de Fogo, possivelmente simbolizando os deus Laterak, o Divino Rei do Deserto.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Heze</b><b> </b>- Zeta Virginis</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Estrela situada na coxa da perna esquerda da Virgem, exatamente no ponto por onde passa o Equador Celestial.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Zaniah</b>. Eta Virginis. </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude 3,9</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela variável situada na asa sul da Virgem. Zaniah vem de Al Zawaih. Alguns a nomeiam como a Prostituta. Na China, era conhecida como Tso Chih Fa, a Mão Esquerda do Mantenedor da Lei. Os Chineses também a nomeavam de Tien Mun, o Portão do Céu - por se situar próxima ao Equinócio Outonal. Juntamente com a estrela Zeta, Heze, marca exatamente a linha do equador celestial.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Theta Virginis</b> - Estrela Tripla</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Branco pálido, vileta e escurecida.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Sem exatamente ser nomeada, foi conhecida como a Criança das Águas.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Syrma</b> - Iota Virginis</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude 4,1</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A Cauda, nome de origem grega usado por Ptolomeu para designar a cauda do vestido da Virgem. Na figura delineada do corpo da Virgem, esta estrela aponta para um ponto entre seu joelho direito e sua panturrilha.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Os árabes consideravam esta estrela como a mais afortunada de suas estações lunares, situando-se entre os demoníacos dentes e as mandíbulas do Leão de um dos lados e da cauda e veneno do Escorpião, do outro lado.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Khambalia</b>. Lambda Virginis. </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela pequena situada no pé esquerdo da Virgem.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>R Virginis</b><b> - Estrela Variável</b></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h35m Declinação +07<sup>o</sup>.16</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitudes: Max 6,2 Min 12,0 Período 144,6</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo PLG Espectro M4e</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>S Virginis</b><b> - Estrela Variável</b></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 13h03m Declinação -06<sup>o</sup>.56</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitudes: Max 6,0 Min 12,9 Período 383,7</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo PLG Espectro M6e</span></span></div>
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<tr><td class="tr-caption" style="font-size: 13px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">carta celeste realizada por Mario Jaci Monteiro - CARJ</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; line-height: 18px;">The Virgo Cluster</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 18px;">[JLC] </span><a href="http://asterisk.apod.com/viewtopic.php?f=29&t=31295&start=125#p199678" rel="nofollow nofollow" style="cursor: pointer; line-height: 18px;" target="_blank">http://asterisk.apod.com/<wbr></wbr><span class="word_break" style="display: inline-block;"></span>viewtopic.php?f=29&t=31295&<wbr></wbr><span class="word_break" style="display: inline-block;"></span>start=125#p199678</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; line-height: 18px;">Copyright: Stephen Mounioloux</span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Aglomerado Virgo</b></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>Este é o mais famoso aglomerado de galáxias. É bem maior do que qualquer outro grupo dentre 100 milhões de anos-luz. Existem cerca de 150 grandes galáxias nesse aglomerado e, pelo menos, mil conhecidas galáxias anãs. Este aglomerado domina completamente nosso pequeno pedaço do Universo e até nosso Grupo Local de galáxias vem sendo gravitacionalmente atraído por este aglomerado. No centro do aglomerado Virgo, encontram-se três grandes galáxias elípticas: M84, M86 e M87. Estas galáxias provavelmente formaram a partir da fusão de muitas galáxias menores e são bem mais massivas do que nossa própria galáxia.</i></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(minha simples e direta tradução para o texto abaixo)</span><br />
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<tr><th colspan="2" style="vertical-align: middle;"><a href="http://www.atlasoftheuniverse.com/galgrps/vir.html" style="background-color: white;"><span style="color: #073763;">Virgo Cluster</span></a></th></tr>
<tr><td style="vertical-align: middle;"><a href="http://www.atlasoftheuniverse.com/galgrps/vir.html" style="background-color: white;"><span style="color: #073763;"></span></a></td><td style="vertical-align: middle;"><span style="background-color: white;"><span style="color: #073763;">This is the most famous cluster of galaxies. It is much larger than any other group within 100 million light years. There are about 150 large galaxies in this cluster and at least a thousand known dwarf galaxies. This cluster completely dominates our tiny corner of the Universe, and even our Local Group of galaxies is being gravitationally pulled by this cluster. At the core of the Virgo cluster lie the three large elliptical galaxies M84, M86 and M87. These galaxies probably formed from the merger of many smaller galaxies and are much more massive than our own galaxy.<br /><br /><a href="http://www.atlasoftheuniverse.com/virgo.html">http://www.atlasoftheuniverse.com/virgo.html</a> - </span></span><span style="color: #073763;">This website belongs to </span><a href="http://www.atlasoftheuniverse.com/me.html" style="text-decoration: none;">Richard Powell</a><span style="color: #073763;">.</span><span style="background-color: white;"><span style="color: #073763;"><br /></span></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>O Aglomerado Virgem é um aglomerado massivo de galáxias que dominam o superaglomerado Virgo. Existem cerca de 2.000 galáxias nesse aglomerado (embora noventa por cento das mesmas sejam galáxias anãs). Este algomerado possui um diâmetro de aproximadamente 15 milhões de anos-luz - e o que não é tão maior do que nosso Grupo Local, porém contém cinquenta vezes mais galáxias. Este mapa mostra 600 das mais brilhantes galáxias dentro de 7.5 graus a partir do centro do aglomerado - essa é uma divisa arbitrária, existem muitas outras galáxias para além desse limite, especialmente em direção ao sul do aglomerado, onde existem vários outros grupos de galáxias adcionais. As 160 maiores galáxias são apresentadas neste mapa.</i></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(tradução simples e literal de Janine para o texto abaixo)</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal; text-align: start;">The Virgo cluster is a massive cluster of galaxies which dominates the Virgo supercluster. There are roughly 2000 galaxies in this cluster (although ninety percent of them are dwarf galaxies). This cluster has a diameter of approximately 15 million light years which is not much larger than our Local Group but it contains fifty times the number of galaxies. This map shows 600 of the brightest galaxies within 7.5 degrees of the centre of the cluster - this is an arbitary border, there are many other galaxies beyond this limit especially to the south of the cluster where there are several additional galaxy groups. The 160 largest galaxies are labelled on this map. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763;">LEIA MAIS EM</span></span></div>
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<span lang="PT" style="line-height: 22px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><a href="http://www.atlasoftheuniverse.com/galgrps/vir.html">http://www.atlasoftheuniverse.com/galgrps/vir.html</a></span></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: normal; text-align: start;">This website belongs to </span><a href="http://www.atlasoftheuniverse.com/me.html" style="line-height: normal; text-align: start; text-decoration: none;">Richard Powell</a><span style="line-height: normal; text-align: start;">.</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal; text-align: start;">This website belongs to </span><a href="http://www.atlasoftheuniverse.com/me.html" style="font-family: Arial, Helvetica, sans-serif; line-height: normal; text-align: start; text-decoration: none;">Richard Powell</a><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal; text-align: start;">.</span></div>
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<span style="background-color: white;"><span style="color: #073763;"><b style="color: black; font-family: 'Times New Roman';">Virgo Cluster Galaxies</b></span></span></div>
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<b>Virgo Cluster Galaxies </b><br /><b>Image Credit & <a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply">Copyright</a>: </b><a href="http://blog.deepskycolors.com/about.html">Rogelio Bernal Andreo</a></center>
<b>Explanation: </b>Well over a thousand galaxies are known members of <a href="http://www.seds.org/messier/more/virgo.html">the Virgo Cluster</a>, the closest large cluster of galaxies to our own <a href="http://www.atlasoftheuniverse.com/localgr.html">local group</a>. In fact, the galaxy cluster is difficult <a href="http://www.atlasoftheuniverse.com/galgrps/vir.html">to appreciate</a> all at once because it covers such a large area on the sky. Spanning about 5x3 degrees, this careful <a href="http://blog.deepskycolors.com/archive/2011/03/18/virgo-Cluster-Deep-Widefield.html">mosaic of telescopic images</a> clearly records the central region of the Virgo Cluster through faint <a href="http://www.galaxyimages.com/UNP1.html">foreground dust</a> clouds lingering above the plane of our own Milky Way galaxy. The cluster's dominant giant elliptical <a href="http://apod.nasa.gov/apod/ap100520.html">galaxy M87</a>, is just below center in the frame. Above M87 is the famous interacting galaxy pair NGC 4438, also known <a href="http://apod.nasa.gov/apod/ap070608.html">as The Eyes</a>. A closer examination of the image will reveal many Virgo cluster member galaxies as small fuzzy patches. Sliding your cursor over the image will label the larger galaxies using <a href="http://apod.nasa.gov/apod/ap990429.html">NGC catalog</a> designations. Galaxies are also shown with <a href="http://www.seds.org/messier/xtra/history/m-cat-i.html">Messier catalog</a> numbers, including <a href="http://apod.nasa.gov/apod/ap080425.html">M84, M86</a>, and prominent colorful spirals <a href="http://apod.nasa.gov/apod/ap100130.html">M88</a>, <a href="http://apod.nasa.gov/apod/ap960316.html">M90</a>, and M91. On average, Virgo Cluster galaxies are measured to be about 48 million light-years away. <a href="http://adsbit.harvard.edu/cgi-bin/nph-iarticle_query?1996PASP%2E%2E108%2E1091V">The Virgo Cluster distance</a> has been used to give an important determination of the Hubble Constant and <a href="http://antwrp.gsfc.nasa.gov/diamond_jubilee/debate96.html">the scale of the Universe</a>. (<i>Editor's Note:</i> Labels courtesy of <a href="http://astrometry.net/">Astrometry.net</a>.)<br />
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<b>Virgo Cluster Galaxies </b><br />Image Credit & <a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply">Copyright</a>:<b> </b><a href="http://blog.deepskycolors.com/about.html">Rogelio Bernal Andreo</a></center>
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(<i>Editor's Note:</i> Labels courtesy of <a href="http://astrometry.net/">Astrometry.net</a>.)</center>
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<span style="background-color: white;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b> O mundo fantástico que se esconde </b></span></span><br />
<span style="background-color: white;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>por detrás do corpo da constelação da Virgem</b></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Virgo é o mais próximo dos grandes Aglomerados de Galáxias</b> de forma que muitas de suas brilhantes galáxias podem ser observadas por telescópios amadores</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(como por exemplo M84 e M86). </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">As galáxias podem ser consideradas como os blocos de construção básica do universo. Elas não são isoladas, independente em suas vizinhanças, porém ocorrem em sistemas que constam de dezenas, centenas ou mesmo milhares de membros que se atraem por suas forças gravitacionais. Esses sistemas são denominados de Aglomerados de Galáxias - os Superaglomerados</span></span></div>
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<tr><td class="tr-caption" style="font-size: 13px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Carta Celeste realizada por Mario Jaci Monteiro - CARJ<br />(a imagem ao inverso foi realizada por Janine)</span></td></tr>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><span lang="PT" style="line-height: 22px;">O AGLOMERADO DE GALÁXIAS EM VIRGEM</span></b></span></div>
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<b><span lang="PT"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">ALGUMAS GALÁXIAS, EM VIRGEM</span></span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">As galáxias podem ser consideradas como os blocos de construção básica do universo. Elas não são isoladas, independente em suas vizinhanças, porém ocorrem em sistemas que constam de dezenas, centenas ou mesmo milhares de membros que se atraem por suas forças gravitacionais. Esses sistemas são denominados de Aglomerados de Galáxias - os Superclusters.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC 5746 - Galáxia Espiral Barrada</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo Sb Ascensão Reta 14h45m0 Declinação +01<sup>o</sup>.49</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude visual 12.3 Dimensões 7.4x1.1</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Nota: próxima a Estrela 109 Virginis<b></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Localizada na parte mais ao leste da Virgem - Estrela 109 Virginis, de magnitude 3.8. Esta galáxia espiral possui uma magnitude de 11.6 e carregando brilho em direção ao seu núcleo bem pronunciado. Telescópios de ampla abertura (<metricconverter productid="14”" w:st="on">14”</metricconverter> e além) podem visualizar um plano mais escuro nesta galáxia quando em lugares apropriados para esta observação (céus escuros e transparentes).</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC 5740 - Galáxia</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">ascensão reta 14h44m24 declinação +01<sup>o</sup>. 40 46</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">tipo eg magnitude 11.86:12.56 dimensões 2.95x1.51 160<b></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Esta Galáxia situa-se cerca de <metricconverter productid="18’" w:st="on">18’</metricconverter> a sudoeste de <b>NGC5746</b>, é bem brilhante apresentando uma magnitude de 12.7. Telescópios com abertura a partir de <metricconverter productid="12”" w:st="on">12”</metricconverter>podem bem resolver este objeto.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC 5634 - Aglomerado Globular</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 14h29m36 Declinação - 05<sup>o</sup>.59<b></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Localizado na parte leste da Virgem, a meio caminho entre as estrelas Mu e Iota Virginis. Possui brilho através a magnitude 9.6 e é bem ampla (<metricconverter productid="4.9’" w:st="on">4.9’</metricconverter>), arredondada e com o miolo gradualmente mais brilhante. Pode ser bem resolvida através suas estrelas de magnitude 19. Existe uma estrela de magnitude 8 situada a sudeste. Telescópios com abertura entre <metricconverter productid="16’" w:st="on">16’</metricconverter> e <metricconverter productid="20’" w:st="on">20’</metricconverter> poderão melhor observar este aglomerado.</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>NGC 5257 e NGC 5258 (ARP 240) </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">são duas galáxias espirais enteragindo entre si, a cerca de 300 milhões de anos-luz, em Virgem. Ambas as galáxias estão distorcidas em função da interação gravitacional e estão ambas conectadas por uma ponte.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(traduzido por Janine <a href="http://annesastronomynews.com/photo-gallery-ii/galaxies-clusters/ngc-5257-and-ngc-5258-arp-240-are-two-interacting-spiral-galaxies-300-million-light-years-away-in-virgo-both-galaxies-are-distorted-by-the-gravitational-interaction-and-both-are-connected-by-a-t/" style="color: #274e13; text-decoration: none;">http://annesastronomynews.com/photo-gallery-ii/galaxies-clusters/ngc-5257-and-ngc-5258-arp-240-are-two-interacting-spiral-galaxies-300-million-light-years-away-in-virgo-both-galaxies-are-distorted-by-the-gravitational-interaction-and-both-are-connected-by-a-t/</a>)</span></div>
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<tr><td><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj3AHB_hKYUeCm83zdJ3E6RXJI7vMojarNUwC2H8o714ymmjNBbNbbIXRVgHnSflxeMW5JNu2pCtOU5uayIzKohJAXVMqieJ_esRmhTCPvsguRyaz9Wlpl0mnZDeEdqGoemwGk20fgIXPQ/s1600/NGC-5257-and-NGC-5258-Arp-240-are-two-interacting-spiral-galaxies-300-million-light-years-away-in-Virgo.-Both-galaxies-are-distorted-by-the-gravitati.jpg" imageanchor="1" style="color: #274e13; margin-left: auto; margin-right: auto; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj3AHB_hKYUeCm83zdJ3E6RXJI7vMojarNUwC2H8o714ymmjNBbNbbIXRVgHnSflxeMW5JNu2pCtOU5uayIzKohJAXVMqieJ_esRmhTCPvsguRyaz9Wlpl0mnZDeEdqGoemwGk20fgIXPQ/s640/NGC-5257-and-NGC-5258-Arp-240-are-two-interacting-spiral-galaxies-300-million-light-years-away-in-Virgo.-Both-galaxies-are-distorted-by-the-gravitati.jpg" height="430" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></td></tr>
<tr><td class="tr-caption" style="font-size: 13px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://pt.wikipedia.org/wiki/NGC_5257" style="background-image: none; color: #274e13; line-height: 15.828125px; text-align: left; text-decoration: none;" title="NGC 5257">NGC 5257</a><span style="line-height: 15.828125px; text-align: left;"> e </span><a href="http://pt.wikipedia.org/wiki/NGC_5258" style="background-image: none; color: #274e13; line-height: 15.828125px; text-align: left; text-decoration: none;" title="NGC 5258">NGC 5258</a><span style="line-height: 15.828125px; text-align: left;"> (Arp 240), Par de galáxias espirais interagindo. Imagem do</span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-image: none; color: #274e13; line-height: 15.828125px; text-align: left; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a></span></td></tr>
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<span style="line-height: 19.2000007629395px; text-align: start;"><span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC 5257</b> is a <a href="http://en.wikipedia.org/wiki/Spiral_galaxy" style="background-image: none; color: #274e13; text-decoration: none;" title="Spiral galaxy">spiral galaxy</a> located in the <a href="http://en.wikipedia.org/wiki/Constellation" style="background-image: none; color: #274e13; text-decoration: none;" title="Constellation">constellation</a> <a href="http://en.wikipedia.org/wiki/Virgo_(constellation)" style="background-image: none; color: #274e13; text-decoration: none;" title="Virgo (constellation)">Virgo</a>. The galaxy is notably <a href="http://en.wikipedia.org/wiki/Interacting_galaxy" style="background-image: none; color: #274e13; text-decoration: none;" title="Interacting galaxy">interacting</a> with the spiral galaxy <a href="http://en.wikipedia.org/wiki/NGC_5258" style="background-image: none; color: #274e13; text-decoration: none;" title="NGC 5258"><b>NGC 5258</b></a>. The two galaxies are listed together as <i><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Arp_240_(disambiguation)" style="background-image: none; color: #274e13; text-decoration: none;" title="Arp 240 (disambiguation)">Arp 240</a></i> in the <i><a href="http://en.wikipedia.org/wiki/Atlas_of_Peculiar_Galaxies" style="background-image: none; color: #274e13; text-decoration: none;" title="Atlas of Peculiar Galaxies">Atlas of Peculiar Galaxies</a></i>.<sup class="reference" id="cite_ref-arp1966_2-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/NGC_5257#cite_note-arp1966-2" style="background-image: none; color: #274e13; text-decoration: none; white-space: nowrap;">[2]</a></sup> Both galaxies are distorted by the gravitational interaction, and both are connected by a tidal bridge, as can be seen in images of these galaxies<b>.</b></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiH0waks0a5kz3UG-iDJFkzPJBAU_OjAoLQVZdIN9Dee1En9iHafbGyW6K_l-IczMNB3SONnhunwi0rKMC5CsIi9V7-E9vl6j1VviYxdAPqq9KhcYB9hyphenhyphenWkbPxu6lNGTORQysRPjJ7ILMk/s1600/Virgo_cluster_052012_overlay.jpg" imageanchor="1" style="color: #274e13; font-family: 'Times New Roman'; line-height: normal; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiH0waks0a5kz3UG-iDJFkzPJBAU_OjAoLQVZdIN9Dee1En9iHafbGyW6K_l-IczMNB3SONnhunwi0rKMC5CsIi9V7-E9vl6j1VviYxdAPqq9KhcYB9hyphenhyphenWkbPxu6lNGTORQysRPjJ7ILMk/s1600/Virgo_cluster_052012_overlay.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></span></div>
<span style="font-family: Arial, Helvetica, sans-serif;"><br /><span style="line-height: 18.2000007629395px;">http://upload.wikimedia.org/wikipedia/commons/4/44/Virgo_cluster_052012_overlay.jpg</span></span><br />
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_desc" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Description</span></td><td class="description"><div class="description mw-content-ltr it" dir="ltr" lang="it" style="direction: ltr;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="language it" title=""><b>Italiano:</b></span> Ammasso di galassie della Vergine con l'indicazione delle galassie visibili. Immagine ripresa presso l'osservatorio Serafino Zani, durante una prova in campo per i componenti del gruppo iscritti al corso di fotografia astronomica del 2012 Somma di 59 immagini da un minuto di posa ciascuna. Elaborazione con stretching logaritmico e rinforzo di A. Soffiantini</span></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_date" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Date</span></td><td><time class="dtstart" datetime="2012-05-12" style="display: inline;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">12 May 2012</span></time></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Source</span></td><td><span class="int-own-work"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Own work</span></span></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Author</span></td><td><a class="new" href="http://commons.wikimedia.org/w/index.php?title=User:Hyperion130&action=edit&redlink=1" style="background-image: none; color: #274e13; text-decoration: none;" title="User:Hyperion130 (page does not exist)"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Hyperion130</span></a></td></tr>
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<span style="font-family: Arial, Helvetica, sans-serif;">Immagine ripresa presso l'osservatorio Serafino Zani, durante una prova in campo per i componenti del gruppo iscritti al corso di fotografia astronomica del 2012 Somma di 59 immagini da un minuto di posa ciascuna. Elaborazione con stretching logaritmico e rinforzo di A. Soffiantini Telescopio FLT98 a 495mm di focale CCD ST8</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj5BbQByLSCxRLst_OrJfxs10i7_-S6wpgzh3k3dDU5fvHANXPxLNgc6Pa41S8OGs6XTCrTo_QmZX4N1LgBcBhyphenhyphennaOebd-TJE3L6Zvg2MrsyhqmHbaqZNtzTb5F9UvBy7MtMzzHhU43U4A/s1600/Virgo_cluster_052012_overlay.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"></span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC 4697</b> - Ascensão Reta 12h48m36 Declinação -05<sup>o</sup>.48</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">È uma galáxia elíptica localizada a 4.7<sup>o</sup>. SSE de Porrima (Gamma Virginis). Possui magnitude de 9.9 e largura de 6’x3.8’, comprimento de 45<sup>o</sup>, contendo um núcleo bem pronunciado. É uma galáxia circundada por várias outras, bem mais pálidas.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4731 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h51 01 declinação -06<sup>o</sup>.2329</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 11.47:11.90 dimensões 6.61x3.24 85</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC 4731</b> é uma galáxia bem pálida, de magnitude 11.6, porém bastante grande (6.5’x3.4’).</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>M60 - NGC 4649 e M59 - MGC 4621</b> são duas galáxias bem brilhantes.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">M 60 - NGC 4649</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão reta 12h43m40 declinação +11<sup>o</sup>.32 58</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 8.84:9.81 dimensões 7,31x5.03</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">M60 é uma galáxia elíptica que possui magnitude 9.6 e é bem grande (3’x2.5’).</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">M 59 NGC 4621</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h41m Declinação + 11<sup>o</sup>.47 Tipo Galáxia Elíptica</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">M59 é uma galáxia elíptica de magnitude 10.6, bem grande (4.5’x3.5’).</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4638 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">12h42m47 Declinação 11<sup>o</sup>.2635</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">tipo eg magnitude 11.19:12.13 dimensões 2.24x1.38 125</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4637 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h42m54 Declinação 11<sup>o</sup>.26 12</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 14.82 dimensões 1.17x0.49 97</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Entre essas duas galáxias e um tantinho ao sul, encontram-se <b>NGC4638</b> (mag 12.2) e <b>NGC 4637</b> (mag 14.8). Um tanto mais ao norte, situam-se as galáxias<b>NGC4607</b> (mag. 13.9) e <b>NGC 4606</b> (mag. 12.5).</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4606 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h40m57 Declinação +11<sup>o</sup>.54 41</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 11.83:12.67 dimensões 3.24x1...62 33</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4607 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h41m 12 Declinação +11<sup>o</sup>.53 09</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 12.83:13.75 dimensões 2.88x0.66 2</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4754 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">ascensão Reta 12h52m17 declinação +11<sup>o</sup>.18 49</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">tipo eg magnitude 10.60:11.52 dimensões 4.57x2.45 23</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC 4754 e NGC 4762</b> formam um par de galáxias a leste de M60 e a oeste de Vindemiatrix (Epsilon Virginis).</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NGC 4754 é uma galáxia espiral de magnitude 10.6 e tamanho 4.6’x2.5’, com um brilho que acelera em direção ao seu centro.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NGC 4762 possui magnitude 10.3 e um tamanho de 8.7’x1.7’, galáxia espiral.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC 4762 -</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo SO Ascensão Reta 12h53m0 Declinação +11<sup>o</sup>.14</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude visual 11.1 Dimensões 9.0x2.0</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Nota: a galáxia mais achatada conhecida</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC 4753 - Galáxia em Virgem</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h52m24 Declinação -01<sup>o</sup>.12</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC 4753</b> é uma galáxia estranha e pequena e cheia de planos escuros e entortados, localizada a 2..7<sup>o</sup> leste de Porrima, bela estrela dupla Gamma Virginis. Em instrumentos de abertura de <metricconverter productid="8”" w:st="on">8”</metricconverter>, é possível se observar, com visão enviesada, um núcleo - que se torna mais pronunciado quando avistado em instrumentos mais potentes.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">M 58 - NGC 4579</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h36m Declinação +11<sup>o</sup>.56</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude 9,9 Tipo Galáxia Espiral</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">M 58 é uma galáxia espiral com aquilo que podemos denominar de barra central. Com magnitude de 11, é uma galáxia irregular e bem condensada de maneira que pode ser observada mais facilmente do que sua magnitude poderia indicar.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4564 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h36m27 Declinação +11<sup>o</sup>.2621</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 11.12:12.05 dimensões 3..55x1.48 47</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC 4564</b> - situa-se a <metricconverter productid="30’" w:st="on">30’</metricconverter> sudoeste de M58, com magnitude 11.9, pequena (3.5’x’.5’) e apresentando um pequeno alongamento.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">M58 - NGC 4579</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12H37M44 Declinação +11<sup>O</sup>.49 11</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude 9.66:1.48 dimensões 5.89x4.68</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Gêmeos Siamenses ou Galáxias Borboletas!</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">NGC 4567 and NGC 4568</span></b> (nicknamed the <i><b>Siamese Twins</b></i> or the <i><b>Butterfly Galaxies</b></i>) are a set of <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Spiral_galaxies" style="background-image: none; color: #073763; text-decoration: none;" title="Spiral galaxies">spiral galaxies</a> about 60 million <a href="http://en.wikipedia.org/wiki/Light-year" style="background-image: none; color: #073763; text-decoration: none;" title="Light-year">light-years</a> away<sup class="reference" id="cite_ref-ned-dist_1-1" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/NGC_4567_and_NGC_4568#cite_note-ned-dist-1" style="background-image: none; color: #274e13; text-decoration: none; white-space: nowrap;">[1]</a></sup> in the <a href="http://en.wikipedia.org/wiki/Constellation" style="background-image: none; color: #073763; text-decoration: none;" title="Constellation">constellation</a> <a href="http://en.wikipedia.org/wiki/Virgo_(constellation)" style="background-image: none; color: #073763; text-decoration: none;" title="Virgo (constellation)">Virgo</a>. They were both discovered by <a href="http://en.wikipedia.org/wiki/William_Herschel" style="background-image: none; color: #073763; text-decoration: none;" title="William Herschel">William Herschel</a> in 1784. They are part of the <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Virgo_cluster_of_galaxies" style="background-image: none; color: #073763; text-decoration: none;" title="Virgo cluster of galaxies">Virgo cluster of galaxies</a>. Only one <a href="http://en.wikipedia.org/wiki/Supernova" style="background-image: none; color: #073763; text-decoration: none;" title="Supernova">supernova</a> (<a class="new" href="http://en.wikipedia.org/w/index.php?title=SN_2004cc&action=edit&redlink=1" style="background-image: none; color: #073763; text-decoration: none;" title="SN 2004cc (page does not exist)">SN 2004cc</a>) was observed in the Siamese Twins.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">These galaxies are in the process of <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Colliding_and_merging" style="background-image: none; color: #274e13; text-decoration: none;" title="Colliding and merging">colliding and merging</a> with each other, as studies of their distributions of <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Neutral_hydrogen" style="background-image: none; color: #274e13; text-decoration: none;" title="Neutral hydrogen">neutral</a> and <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Molecular_hydrogen" style="background-image: none; color: #274e13; text-decoration: none;" title="Molecular hydrogen">molecular</a> hydrogen show, with the highest <a href="http://en.wikipedia.org/wiki/Star_formation" style="background-image: none; color: #274e13; text-decoration: none;" title="Star formation">star formation</a>activity in the part where they overlap. However the system is still in an early phase of interaction.<sup class="reference" id="cite_ref-Kaneko2010_2-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/NGC_4567_and_NGC_4568#cite_note-Kaneko2010-2" style="background-image: none; color: #274e13; text-decoration: none; white-space: nowrap;">[2]</a></sup></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">They were named "<a class="mw-redirect" href="http://en.wikipedia.org/wiki/Siamese_Twins" style="background-image: none; color: #274e13; text-decoration: none;" title="Siamese Twins">Siamese Twins</a>" because they appear to be connected.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://en.wikipedia.org/wiki/NGC_4567_and_NGC_4568</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg-VQNygLN_RcktTKloogFCzjDpiBbkMq3DuHA9870z6Yw6JnxWuBNIRNSGKzPUGCHczD9FHJZ13okfwkrYmgQ9zKSvHRuM6MknnfxLhvEJtxnY2lJeq3Y8mt786NuAz6CLZQ0NCsV0HaU/s1600/788px-NGC4568.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg-VQNygLN_RcktTKloogFCzjDpiBbkMq3DuHA9870z6Yw6JnxWuBNIRNSGKzPUGCHczD9FHJZ13okfwkrYmgQ9zKSvHRuM6MknnfxLhvEJtxnY2lJeq3Y8mt786NuAz6CLZQ0NCsV0HaU/s1600/788px-NGC4568.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18.2000007629395px;">http://pt.wikipedia.org/wiki/NGC_4568</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Existe um par de galáxias nomeado de Gêmeos Siameses, situado a <metricconverter productid="11’" w:st="on">11’</metricconverter> sul de NGC4564: são <b>NGC 4567 e NGC 4568</b> e são descritas como muito pálidas (magnitude 12) porém grandes (4’x3’, ao todo). Podem ser visualizadas através a abertura telescópica de <metricconverter productid="8”" w:st="on">8”</metricconverter> e o par surgirá como uma curva brilhante e singular, única. </span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4567 - Galáxia Espiral Barrada</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h36m32 Declinação +11<sup>o</sup>.15 31</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 11.31:12.06 dimensões 2.95x2.00 85</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Nota: Gêmeos Siameses, par de galáxias</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4568 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h36m34 Declinação + 11<sup>o</sup>.14 15</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 10.81:11.68 dimensões 4.57x2.00 23</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>M 89 - NGC 4552 - e M90 - NGC 4569</b> - são duas galáxias brilhantes, sendo que M90 possui uma magnitude de 11 e é bem grande (11’x5’) e apresentando-se como uma galáxia espiral com uma barra difusa. Situa-se a 2.2<sup>o</sup>. a leste dos Olhos. Um tantinho ao norte de M90, situa-se <b>IC 3583</b> (magnitude 13.8)</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">I3583 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h36m43 Declinação +13<sup>o</sup>.15 31</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 13.31 dimensões 2.19x1.12 0</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">M89 é uma galáxia elíptica brilhante (magnitude 10.5), pequena (5’x5’) e e situada a <metricconverter productid="40’" w:st="on">40’</metricconverter> sudoeste de M90. </span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">M 89 - NGC 4552</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão reta 12h53m39 declinação +12<sup>o</sup>.33 25</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 9.75:10.73 dimensões 5.13x4.68</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">M 90 - NGC 4569</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão reta 12h36m50 declinação +13<sup>o</sup>.09 48</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 9.54:10.26 dimensões 9.55x4.37</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEi-o8YB1wy_BxYfRnuS0Bp9OSVatLyor22PBqWWmrHYVAXdcpKFNHrJiZH8xAjFhuMD_uj7gZMGPggnc2EaQQIZJKZoS5UOtB-vf1BEV-0MIG0a15tu-isoF-DzW-Q-dXpxpp_2S232J6k/s1600/NGC4438_NGC4435_crawford_rc720.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEi-o8YB1wy_BxYfRnuS0Bp9OSVatLyor22PBqWWmrHYVAXdcpKFNHrJiZH8xAjFhuMD_uj7gZMGPggnc2EaQQIZJKZoS5UOtB-vf1BEV-0MIG0a15tu-isoF-DzW-Q-dXpxpp_2S232J6k/s1600/NGC4438_NGC4435_crawford_rc720.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
<span style="font-family: Arial, Helvetica, sans-serif;"><br />http://apod.nasa.gov/apod/ap070608.html</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">Markarian's Eyes </span></b><br /><b>Credit & Copyright: </b><a href="http://rdelsol.com/mailme.htm" style="color: #073763; text-decoration: none;">Ken Crawford</a> (<a href="http://rdelsol.com/" style="color: #073763; text-decoration: none;">Rancho Del Sol Observatory</a>)</span></center>
<span style="font-family: Arial, Helvetica, sans-serif;"><b>Explanation: </b>Across the heart of the Virgo Galaxy Cluster lies a string of galaxies known as <a href="http://apod.nasa.gov/apod/ap061011.html" style="color: #274e13; text-decoration: none;">Markarian's Chain</a>. Prominent in Markarian's Chain are these two interacting galaxies, NGC 4438 (left) and NGC 4435 - also known as The Eyes. About 50 million light-years away, the two <a href="http://www.messier45.com/cgi-bin/dsdb/dsb.pl?str=NGC+4438" style="color: #274e13; text-decoration: none;">galaxies appear</a> to be about 100,000 light-years apart in <a href="http://www.rdelsol.com/Galaxy/NGC4435_NGC4438.html" style="color: #274e13; text-decoration: none;">this sharp close-up</a>, but have likely approached to within an estimated 16,000 light-years of each other in their <a href="http://chandra.harvard.edu/photo/cosmic_lookback.html" style="color: #274e13; text-decoration: none;">cosmic past</a>. Gravitational tides from <a href="http://chandra.harvard.edu/photo/2003/ngc4438/" style="color: #274e13; text-decoration: none;">the close encounter</a> have ripped away at their stars, gas, and dust. The more massive NGC 4438 managed to hold on to much of the material torn out in the<a href="http://burro.cwru.edu/JavaLab/GalCrashWeb/main.html" style="color: #274e13; text-decoration: none;">collision</a>, while material from the smaller NGC 4435 was more <a href="http://www.astropix.com/wp/2007/05/13/ngc-4438-and-ngc-4435/" style="color: #274e13; text-decoration: none;">easily lost</a>. The remarkably deep image of this crowded region <a href="http://bigpicture.caltech.edu/" style="color: #274e13; text-decoration: none;">of the universe</a> also includes many more distant background galaxies.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Existe The Markarian Chain, a Corrente Markarian, encontrada a meio caminho entre Denebola, a estrela Beta Leonis, e Vindemiatrix, a estrela Epsilon Virginis (a mão da Virgem segurando a ponta anelada de seus longos cabelos).</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000; font-size: medium;">Os Olhos</span></b> são um par de galáxias situadas bem neste ponto central:</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC4438</b>, um dos dois Olhos, é uma galáxia brilhante e razoavelmente grande, enquanto <b>NGC 4435</b>, um tantinho ao norte, é bem brilhante (magnitude 11.7) e bem grande e arredondada (2.8’x2’).</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC 4438 - Galáxia</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo Sap Ascensão Reta 12h27m8 Declinação +13<sup>o</sup>.01</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude visual 12 Dimensões 9.7x3.9</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Nota: <b>faz par com NGC4435</b></span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4435 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h27m40 declinação +13<sup>o</sup>.04 48</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 10.80:11.74 dimensões 2.75x2.00.13</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A <metricconverter productid="23’" w:st="on">23’</metricconverter> oeste dos Olhos, situam-se a galáxia elíptica <b>M86 - NGC 4406</b> -, com magnitude 9.8 e tamanho de 9’x6’ e a galáxia <b>M84 - NGC 4374</b> -, com magnitude 10, tamanho 6.4’x5.6’.</span></div>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">M84 - NGC 4374</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão reta 12h25m03 declinação +12<sup>o</sup>.53 15</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 9.11:10.09 dimensões 6.46x5.62</span></div>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">M86 - NGC 4406</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão reta 12h26m11 declinação +12<sup>o</sup>.56 49</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 8.90:9.83 dimensões 8.91x5.75</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">M86 apresenta um anel de galáxias formando um colar e estes objetos podem ser vistos em telescópios de abertura <metricconverter productid="8”" w:st="on">8”</metricconverter> ou 10”: NGC 4402, NGC 4387, NGC 4388, NGC 4413, NGC 4425.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4387 Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h25mm41 Declinação +12<sup>o</sup>.48 42</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 12.12:13.01 dimensões 1.78x1.0140</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4402 Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h26m07 Declinação +13<sup>o</sup>.06 46</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 11.73:12.55 dimensões 3.89x1.10 90</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4413 Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h16m31 Declinação +12<sup>o</sup>.3635</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 12.25:12.99 dimensões 2.34x1.51 60</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4425 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h27m13 Declinação +12<sup>o</sup>.44 09</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 11.83:12.73 dimensões 2.95x1.00 27</span></div>
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<b><span lang="PT"><span style="font-family: Arial, Helvetica, sans-serif;">NGC 4388 - tipo SBc</span></span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h25m8 Declinação +12<sup>o</sup>.40</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude visual 12.2 Dimensões 6.2x1.7 Nota: próxima à M85 e M86</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Nota: faz par com NGC 4435</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4486a - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h30m9 Declinação +12<sup>o</sup>.16</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 11.2 dimensões 1.3x1.1</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A <metricconverter productid="58’" w:st="on">58’</metricconverter> sudoeste dos Olhos, situa-se a galáxia gigante elíptica <b>M 87 - NGC 4486</b>, com magnitude 9.6 e tamanho 7’x7’. Existem três galáxias associadas a este objeto e são NGC 4486, NGC 4478 e NGC 4476.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4478 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h30m17 Declinação +12<sup>o</sup>.19 44</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 11.45:12.36 dimensões 1.91x1.62 140</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4476 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h29m58 Declinação +12<sup>o</sup>.20 53</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 12.19:13.01 dimensões 1.70x1.17 25</span></div>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">M87 - NGC 4486 - Galáxia</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h30m49 declinação +12<sup>o</sup>.23 24</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 8.63:9.59 dimensões 8.32x6.61</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Um dos maiores membros do Aglomerado de Galáxias em Virgem, é uma galáxia brilhante e eliptical e uma das mais massivas e luminosas galáxias conhecidas. Ao mesmo tempo, é uma das mais vigorosas fontes de radiação de radio, designada como Virgo A ou pelo número <metricconverter productid="3C" w:st="on">3C</metricconverter> 274 (Catálogo de Fontes de Radio). Sua poderosa radiação de rádio e também a poderosa emissão de raio-x acontecem como um jato luminoso que se extende para mais de 4 mil anos-luz para fóra do núcleo da galáxia. Dentro do núcleo podemos encontrar um jato de elétrons, acelerado por um campo magnético bem forte e para velocidade imensa: isso faz acontecer uma radiação extremamente enérgica e estes processos podem ter sido causados, por exemplo, por um supermassivo buraco negro no núcleo da galáxia.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A Corrente, The Chain, estende-se ao leste e ao norte dos Olhos e então encontraremos outro par de galáxias:</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4461 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h29m03 declinação +13<sup>o</sup>.11 08</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 11.19:12.09 dimensões 3.55x1.45 9</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC 4461</b> é pálida (magnitude 12) e espiral alongada, podendo ser visualizada em grandes telescópios (3.5’x1.4’).</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC 4458</b> situa-se bem ao seu norte e mais difícil de ser visualizada (magnitude 13) do que seu par.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4458 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h28 57 declinação +13<sup>o</sup>.14 35</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 12.07:12.93 dimensões 1.74x1.58</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4473 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h29m48 declinação +13<sup>o</sup>.25 49</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 10.20:11.16 dimensões 4.47x2.51 100</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Olhando para o nordeste em <metricconverter productid="18’" w:st="on">18’</metricconverter>, a Corrente ainda nos revela <b>NGC 4473</b>, com magnitude de 11.1 e tamanho de 4.4’x2.5’. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Certamente esta é a região mais rica do Superaglomerado de Galáxias da Virgem.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">M 61 - NGC 4303</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão reta 12h21m54 declinação +04<sup>o</sup>.28 20</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 9.65:10.18 dimensões 6.46x5....75</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> M 61 é uma galáxia espiral com magnitude 10.1 e bem grande (7’x6’).</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Outra galáxia espiral é <b>NGC 4303 <sup> </sup>A</b>, com magnitude de 13.6.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC4292</b>, magnitude 13.6.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4292 Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12.21m16 Declinação +04<sup>o</sup>.35 47</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg Magnitude 12.21 : 13.09 dimensões 1.66x 1.15 7<sup>o</sup>.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC 4216 - Galáxia Espiral Barrada</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h15m9 Declinação +13<sup>o</sup>.09</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude visual 11.2 Dimensões 8.5x1.7 Notas: próxima à NGCs 4206 e 4222</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC 4216</b> situa-se quase na fronteira com Coma Berenices e encontra-se a 1.5<sup>o</sup>. SSW de <b>M99</b>, a 1.8<sup>o</sup>. SSE de <b>M98</b> e 2.3<sup>o</sup>. oeste de <b>M84</b> e aglutina uma série de galáxias.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A meio caminho entre M84 e NGC 4216, situa-se <b>NGC 4267</b> e com magnitude de 11.8, tamanho de 3.2’x3.0’.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC 4206 Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h15m16 Declinação +13<sup>o</sup>.01 30</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg Magnitude 12.15:12.82 Dimensões 6.17x 1.17.0<sup>o</sup>.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4267 Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h19.45 Declinação +12<sup>o</sup>.47 57</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg Magnitude 10.93:11.86 dimensões 3.24x3.02</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">M84 - NGC 4374</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h24m Declinação +13<sup>o</sup>.00 Tipo Galáxia Elíptica Magnitude 9,8</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A descrição de NGC 4216 é de que é uma galáxia bem brilhante, com magnitude 11 e muito grande (8.2’x1.8’), com grande alongamento - 17<sup>o</sup>. - e um brilho inesperado levando ao núcleo central.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">No mesmo campo de visão de NGC 4216, pode-se observar <b>NGC 4222</b> (magnitude 14, medindo 3.3’x0.5’) e <b>NGC 4206</b> (magnitude 13, medindo 5.1’x1.0’ - esta última mais fácil de ser visualizada.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4222 Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h16mmmm22 Declinação +13<sup>o</sup>.18 31</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg Magnitude 13.86 Dimensões 3.31x0.46.56<sup>o</sup>.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A <metricconverter productid="29’" w:st="on">29’</metricconverter> oeste de NGC4216, encontramos <b>NGC 4193</b> (magnitude 13, medindo 2.0’x1.1’).</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC 4193 Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h13m53 Declinação +13<sup>o</sup>.10 28</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg Magnitude 12.31:13.18 Dimensão 2.04x1.05.93<sup>o</sup>.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><metricconverter productid="15’" w:st="on">15’</metricconverter> ao norte de NGC4193, situa-se <b>NGC4189</b> (magnitude 12.6, medindo 2.4’x1.7’, já <personname productid="em Coma Berenices. A" w:st="on">em Coma Berenices. A</personname> <metricconverter productid="24’" w:st="on">24’</metricconverter> oeste de NGC 4193, encontramos <b>NGC 4168</b>, uma galáxia irregular, pálida e brilhando um tantinho em direção ao seu centro.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4168 Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h12m16 Declinação +13<sup>o</sup>.12.24</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg Magnitude 11.18:12,11 Dimensão 2.7x2.29</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC 4212</b> é uma galáxia brilhante, grande e alongada e já situando-se <personname productid="em Coma Berenices" w:st="on">em Coma Berenices</personname>, <metricconverter productid="45’" w:st="on">45’</metricconverter> ao norte de NGC 4216.</span></div>
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<tr><td><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj7CWY7A2URi_OfV42RRrWyeyc5XzOYqN8Us2zam7M2hggmCoztEIYaraGtqu78HhNdoFLkyUPIVtrQRmYs21swyDYfGdw0rjahQyvCynGWUY-OTZdhhZv0Tj9pv6HUufSIs59qEM7qszU/s1600/outra+virgo+cluster.jpg" imageanchor="1" style="color: #274e13; margin-left: auto; margin-right: auto; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj7CWY7A2URi_OfV42RRrWyeyc5XzOYqN8Us2zam7M2hggmCoztEIYaraGtqu78HhNdoFLkyUPIVtrQRmYs21swyDYfGdw0rjahQyvCynGWUY-OTZdhhZv0Tj9pv6HUufSIs59qEM7qszU/s640/outra+virgo+cluster.jpg" height="388" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></td></tr>
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<span style="line-height: 18px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">The Virgo Cluster</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><span style="line-height: 18px;">[JLC] </span><a href="http://asterisk.apod.com/viewtopic.php?f=29&t=31295&start=125#p199678" rel="nofollow nofollow" style="color: #274e13; cursor: pointer; line-height: 18px; text-decoration: none;" target="_blank">http://asterisk.apod.com/<wbr></wbr><span class="word_break" style="display: inline-block;"></span>viewtopic.php?f=29&t=31295&<wbr></wbr><span class="word_break" style="display: inline-block;"></span>start=125#p199678</a></span></div>
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<span style="line-height: 18px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Copyright: Stephen Mounioloux</span></span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">Galáxias mais ao Sul da Virgem:</span></b></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC 4699 -</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo Sa Ascensão Reta 12h49m1 Declinação -09<sup>o</sup>.40</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude visual 10.5 Dimensões 3.5x2.7 Nota: pequena e brilhante</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC 4699</b>, localizada a 1..6<sup>o</sup>. noroeste de Psi Virginis, acolhe um campo de galáxias. É descrita como uma galáxia bem brilhante (magnitude 10.7), arredondada (3.8’x2.6’) e com o centro bem mais brilhante.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">4759/n4764 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">ascensão reta 12h53m05 declinação -09<sup>o</sup>.15 29</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">tipo eg magnitude :15.98 dimensões 0.10x0.10</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC 4759</b> é descrita como magnitude 12.2 e razoavelmente grande (2..6’x2.0’) e faz dupla com outra galáxia (<b>NGC4764</b>).</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">4739 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">ascensão Reta 12h51m37 declinação -08<sup>o</sup>.24 37</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">tipo eg magnitude:14p dimensões 1.62x1..41</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Mais desafiadoras ainda são as galáxias <b>NGC4739 </b>(localizada a <metricconverter productid="41’" w:st="on">41’</metricconverter> ENE de <b>NGC4699</b>; e <b>IC3826 e NGC4703</b>, ambas também próximas a NGC4699.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">I3826 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">ascensão Reta 12h51m37 Declinação -08<sup>o</sup>.224 37</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">tipo eg magnitude :15p dimensões 1.91x0.78 3</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4703 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h49m19 Declinação -09<sup>o</sup>.06 32</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 14.5 dimensões 2.95x0.58 30</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>M 49 - NGC 4472</b> - é uma galáxia elíptica, com magnitude 9.1 e tamanho de 8’x7’, localizada a 5<sup>o</sup>. ao sul de M87. </span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC 4472 - M49 - Galáxia</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h28m Declinação +08<sup>o</sup>.08</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo (Classificação Hubble) E - Galáxia Elíptica Magnitude fotográfica aparente 9,33</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Dimensões Angulares 9,8 X 6,6 Distância (milhões de anos-luz) 37,0</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Uma das galáxias mais brilhantes do grupo de Virgo, situada a 4/7 da reta imaginária que vai de Denebola a Delta da Virgem, a cerca de 4<sup>o</sup>. a oeste de 32 Virginis e próxima a uma estrela de quinta magnitude.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Em sua vizinhança encontramos <b>NGC 4535 e NGC 4526 e NGC 4365</b>. Ainda outras tantas galáxias rodeiam M 49.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4365 Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h24m27 Declinação +07<sup>o</sup>.19 06</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 9.56:10.52 dimensões 6.92x5.01.40</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC 4526 - Galáxia de forma Elíptica</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo E7 Ascensão Reta 12h34m1 Declinação + 07<sup>o</sup>.43</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude visual 10.6 Dimensões 7.0x2.7</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC 4535 - Galáxia Espiral Barrada</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo SBc Ascensão Reta 12h34m4 Declinação +08<sup>o</sup>.13</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude visual 11.1 Dimensões 7.8x7.0 Nota: próxima à M49</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Localizada a 5<sup>o</sup>. sul de M87 e a 1.1<sup>o</sup>. ESE de M49, encontra-se a galáxia <b>NGC 4536</b>, com ao magnitude 9.6 e com tamanho de 5’x2’. É uma galáxia brilhante e alongada (posição angulada a 120<sup>o</sup>) e inesperado brilho em direção ao centro.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC4570 - Virgo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h36m53 Declinação +07<sup>o</sup>.14 52</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 10.90:11.84 dimensões 3.80x1.15 159</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC 4570</b> é uma galáxia espiral localizada a <metricconverter productid="50’" w:st="on">50’</metricconverter> sudeste de NGC4526, com magnitude de 11.9 e tamanho de 8’x1.1’.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC 4365</b> é outra galáxia elíptica que acolhe outras tantas galáxias mais pálidas. Situando a 1.5<sup>o</sup>. WSW de M49, é descrita como bastante brilhante (magnitude 10.3) e razoavelmente grande (7.0’x5.1’).</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;"><span lang="ES-TRAD">NGC 4594 - </span><b><span lang="ES-TRAD">M 104 - </span></b><span lang="ES-TRAD">- <b>Galáxia Sombrero</b>:</span></span><span lang="ES-TRAD"></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h40m00 Declinação - 11<sup>o</sup>.37</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>M 104</b>: é uma galáxia com magnitude 8.6 e tamanho de 9’x4’. Vista de lado, com um simples telescópio de abertura <metricconverter productid="4”" w:st="on">4”</metricconverter>, poderá apresentar um plano de poeira correndo em direção ao seu centro. Esta galáxia situa-se na fronteira com o Corvo.</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEitfQt8-4ouxmA3_0lVm4VHTRGIjyG-sapKSI7m7_B_9U71FO7LnDiFQ10HroO9BNertd1w4EyegJEwLgPeEJddGNntfZSTypdppBknIU92k7XdCezyPiahQStSYzrsO1f1ZjK_lAz1rC0/s1600/M104_ngc4594_sombrero_galaxy_hi-res.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEitfQt8-4ouxmA3_0lVm4VHTRGIjyG-sapKSI7m7_B_9U71FO7LnDiFQ10HroO9BNertd1w4EyegJEwLgPeEJddGNntfZSTypdppBknIU92k7XdCezyPiahQStSYzrsO1f1ZjK_lAz1rC0/s1600/M104_ngc4594_sombrero_galaxy_hi-res.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<span style="line-height: 18.2000007629395px;"><span style="font-family: Arial, Helvetica, sans-serif;">http://upload.wikimedia.org/wikipedia/commons/thumb/5/5e/M104_ngc4594_sombrero_galaxy_hi-res.jpg/1280px-M104_ngc4594_sombrero_galaxy_hi-res.jpg</span></span></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Autor</span></td><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">NASA/ESA and The Hubble Heritage Team (STScI/AURA)</span></td></tr>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiJARWpVVFivRGQD68BGpzm-3RAeM8EjdNUurDecp7gchKELVv81FFoCzrNmp51CbOWlODsEDOSizjQlflK-PJJjX6aQkA6C66zZyPMtHUzC8ihH8rSIXXO8M2Oy4eZvs-4hBufeYz3dw8/s1600/galaxia-do-sombrero.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"></span></a></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC5068 - Galáxia em Virgem</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 13h18m54 Declinação -21<sup>o</sup>.02</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC 5068</b> acolhe um trio de galáxias próximas à fronteira com a Hydra, 2<sup>o</sup>. ao norte de Gamma Hydrae. É uma galáxia irregularmente arredondada, com magnitude de 10.4 e medidas de 7.2’x6.3’, com um centro mais brilhante.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC 5077</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">ascensão reta 13h20m25 declinação -20<sup>o</sup>.3637</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">tipo eg magnitude 11.39:12.40 dimensões 2.34x1.70 10</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC 5087</b> situa-se a meio grau nordeste de NGC 5068 e pode ser descrita como uma galáxia irregularmente formatada e bem pálida (magnitude 12) e bem pequena (2.3’x1..7’). Pode ser visualizada em telescópio com aberturas <metricconverter productid="8”" w:st="on">8”</metricconverter> a <metricconverter productid="10”" w:st="on">10”</metricconverter>.</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC 5084</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">ascensão reta 13h20m16 declinação -21<sup>o</sup>.49 37</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">tipo eg magnitude 10.52:11.63 dimensões 9.33x1.74 80<b></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> situa-se a <metricconverter productid="51’" w:st="on">51’</metricconverter> SSE de NGC 5068 e é uma galáxia espiralada com magnitude 11.3 e de tamanho 9.3’x1.8’ - estendida a 80<sup>o</sup>.</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjn8AxQKJg_SSBxNPw6VC_LNY6qijq1qKS9soFLZi226fqsyRb3-X-arxWgVgpG3Nz1aWeH_uwrw6R5S-aHF8sNqHo7WW09RWkMUvfkfZAJvlihYNqopZs_FNd0HdrAMsr2HahU43zB5as/s1600/MakariansChain+%25281%2529.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjn8AxQKJg_SSBxNPw6VC_LNY6qijq1qKS9soFLZi226fqsyRb3-X-arxWgVgpG3Nz1aWeH_uwrw6R5S-aHF8sNqHo7WW09RWkMUvfkfZAJvlihYNqopZs_FNd0HdrAMsr2HahU43zB5as/s1600/MakariansChain+%25281%2529.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span lang="EN-US"> Coma-Virgo Galaxy Cluster is home to multiple galaxies visible through binoculars, including M87, M86, and M84.<o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">Philippe Barraud<o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">http://www.astronomy.com/observing/sky-this-week/2014/03/march-1423-2014<o:p></o:p></span></span></div>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">Outros Aglomerados de Galáxias ou Superaglomerados e um Void,</span></b></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>classificados como direcionados a partir da constelação Virgo</b>:</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Abell 1689</b> - Um dos maiores e mais massivos aglomerados de galáxias conhecido, atuando como lente gravitacional.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Abell 1835</b> - Atrás daquela que é candidata de galáxia mais distante conhecida, Galáxia Abell 1835 IR1916, vista através lente gravitacionais.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Abell 2029</b> - Próxima à fronteira com Serpens Caput</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">Leo-Virgo Superaglomerado SCI 107</span></b></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">Virgo-Coma Superaglomerado SCI 111</span></b></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">Virgo Void</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Coordenadas Equatoriais: Ascensão Reta 13.5 Declinação +10</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Coordenadas Supergalacticas: L” 109 B” +11</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Redshift z: 0.0100</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Distância em milhões de anos-luz: 140</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Diâmetro em milhões de anos-luz: 115</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">Superaglomerado Leo-Virgo:</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Coordenadas Equatoriais: Ascensão Reta 11.5 Declinação - 4</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Coordenadas Supergalacticas: L” 115 B” - 22</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Redshift z: 0.052</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Distância em milhões de anos-luz: 708</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Dimensão em milhões de anos-luz: 100</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Constelação na qual a maior parte do Superaglomerado se situa: Leo-Virgo</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Aglomerados Abell no Superaglomerado: Abell 1216, Abell 1308, Abell 1334</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">Superaglomerado Virgo-Serpens:</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Coordenadas Equatoriais: Ascensão Reta 15.2 Declinação +6</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Coordenadas Supergalacticas: L” 120 B” +34</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Redshift z: 0.052</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Distância em milhões de anos-luz: 708</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Dimensão em milhões de anos-luz: 150</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Constelação na qual a maior parte do Superaglomerado se situa: Virgo-Serpens</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Aglomerados Abell no Superaglomerado: Abell 2020, Abell 2023, Abell 2040, Abell 2055</span></div>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">O AGLOMERADO DE GALÁXIAS, EM VIRGEM,</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>faz parte daquilo que nomeamos como Local Supercluster ou Superaglomerado Local que contém o Grupo Local acolhendo nossa Galáxia, a Via Láctea, e contém o Aglomerado de Virgem, bem próximo ao centro: o Superaglomerado Virgo.</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Coordenadas Equatoriais: Ascensão Reta 12h29.6 Declinação +11<sup>o</sup>.49</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Coordenadas Supergalacticas: L” 103.3 B” -2.8</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Riqueza 1</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Redshift .0037</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Distância em milhões de anos-luz: 52</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Começando a partir de uma imensa lista de nebulosas publicada por William e John Herschel em 1863, foi conhecido o fato de que existia um excesso marcante de campos nebulosos na constelação de Virgem. Nos anos 1950, o astrônomo Gerard Henri de Vaucouleurs foi o primeiro a comentar sobre este excesso representado por um tipo de galáxia de escala grandiosa - o que lhe garantiu o nome de Supergaláxia Local, em 1953 e que foi mudado para Superaglomerado Local, em 1958. O debate continuou durante os anos 60 e 70 em termos de se o Superaglomerado Local era verdadeiramente uma estrutura ou um alinhamento de galáxias tão somente. Esta questão foi resolvida através as buscas usando redshift ao final dos anos 70 e começo dos anos 80, que, convincentemente apontou para a concentração de galáxias ao longo do plano supergaláctico.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Virgo Cluster ou Aglomerado de Galáxias, em Virgem, faz parte daquilo que nomeamos como Local Supercluster ou Superaglomerado Local que contém o Grupo Local acolhendo nossa Galáxia, a Via Láctea, e contém o Aglomerado de Virgem, bem próximo ao centro.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Também esta questão pode ser conhecida como o Superaglomerado Virgo ou Superaglomerado Local que se apresenta como um superaglomerado irregular e que contém o Aglomerado Virgo bem como o Grupo Local (que acolhe nossa Via Láctea e a galáxia Andromeda). Acredita-se que pelo menos 100 grupos de galáxias e aglomerados situam-se dentro de seu diâmetro de 33 megaparsecs (110 milhões de anos-luz). E este Superaglomerado é um dos milhões de superaglomerados que existem no Universo observável.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">O Superaglomerado Local contém o Grupo Local com nossa Galáxia, a Via Láctea, e também contém o Aglomerado de Galáxias Virgo próximo a seu centro - e, algumas vezes, é chamado de Virgo Superaglomerado. Dimensão de 33 megaparsecs = 110 milhões de anos-luz.<b></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://www.slipperysnake.co.uk/educational-materials/science/space/observable-universe/</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif; font-weight: bold;">O mundo fantástico que se esconde </span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif; font-weight: bold;">por detrás do corpo da constelação virginal: </span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif; font-weight: bold;">o Aglomerado de Galáxias em Virgem</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Boa Leitura e Bons Estudos!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Visitando os Sites abaixo,<o:p></o:p></b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b> você conseguirá informações atualizadas e preciosas<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">sobre os Objetos Celestiais de seu interesse:</span></b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://ned.ipac.caltech.edu/<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)</span></span></div>
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<b><span lang="PT"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">REFERÊNCIAS BIBLIOGRÁFICAS:</span></span></b></div>
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<span lang="PT"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">COMPILAÇÃO (com todo o respeito)</span></span></div>
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<span lang="PT"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">E TRADUÇÃO literal (quando necessária)</span></span></div>
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<span lang="PT"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">de Janine Milward:</span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- </span><span lang="EN-US">Wil Tirion - Atlas of the Night Sky</span><span lang="EN-US"> - The Hamlyn Publishing Group Limited, <place w:st="on"><city w:st="on">London</city>, <country-region w:st="on">England</country-region></place></span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- </span><span lang="EN-US">Antonin Rükl - The Hamlyn Encyclopedia of Stars & Planets</span><span lang="EN-US"> - The Hamlyn Publishing Group Limited, <place w:st="on"><city w:st="on">London</city>, <country-region w:st="on">England</country-region></place></span></span></div>
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<span style="line-height: 18px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">The Virgo Cluster</span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18px;">[JLC] </span><a href="http://asterisk.apod.com/viewtopic.php?f=29&t=31295&start=125#p199678" rel="nofollow nofollow" style="cursor: pointer; line-height: 18px; text-decoration: none;" target="_blank">http://asterisk.apod.com/<wbr></wbr><span class="word_break" style="display: inline-block;"></span>viewtopic.php?f=29&t=31295&<wbr></wbr><span class="word_break" style="display: inline-block;"></span>start=125#p199678</a></span></div>
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<span style="line-height: 18px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Copyright: Stephen Mounioloux</span></span></div>
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<span lang="PT" style="line-height: 22px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://www.atlasoftheuniverse.com/galgrps/vir.html</span></span></div>
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<span style="color: #274e13;"><span lang="PT" style="line-height: 22px;"><span style="font-family: Arial, Helvetica, sans-serif;">http://www.atlasoftheuniverse.com/galgrps/vir.html. </span></span><span style="font-family: Arial, Helvetica, sans-serif;">This website belongs to </span><a href="http://www.atlasoftheuniverse.com/me.html" style="font-family: Arial, Helvetica, sans-serif; text-decoration: none;">Richard Powell</a><span style="font-family: Arial, Helvetica, sans-serif;">.</span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">- http://apod.nasa.gov/apod/ap070608.html</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">- <a href="http://annesastronomynews.com/photo-gallery-ii/galaxies-clusters/ngc-5257-and-ngc-5258-arp-240-are-two-interacting-spiral-galaxies-300-million-light-years-away-in-virgo-both-galaxies-are-distorted-by-the-gravitational-interaction-and-both-are-connected-by-a-t/" style="text-decoration: none;">http://annesastronomynews.com/photo-gallery-ii/galaxies-clusters/ngc-5257-and-ngc-5258-arp-240-are-two-interacting-spiral-galaxies-300-million-light-years-away-in-virgo-both-galaxies-are-distorted-by-the-gravitational-interaction-and-both-are-connected-by-a-t/</a></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">- <a href="http://pt.wikipedia.org/wiki/NGC_5258" style="text-decoration: none;">http://pt.wikipedia.org/wiki/NGC_5258</a></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">- <a href="http://pt.wikipedia.org/wiki/NGC_5257" style="text-decoration: none;">http://pt.wikipedia.org/wiki/NGC_5257</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas - AS </b><b>CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra..., bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>VISITE MINHA PÁGINA</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>DA TERRA AO CÉU E AO INFINITO</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><a href="http://daterraaoceueaoinfinito.blogspot.com.br/">http://daterraaoceueaoinfinito.blogspot.com.br/</a></b><o:p></o:p></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-83942211074056112102013-08-20T08:39:00.003-07:002014-04-27T13:20:31.840-07:00VELA, EM ARGO NAVIS, O NAVIO<div align="center" class="MsoNormal" style="text-align: center;">
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Da Terra ao Céu ....</span></a></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">.....<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="text-decoration: none;">e ao Infinito </a></span></h1>
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">- As 88 Constelações</span></a></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/">http://daterraaoceueaoinfinito.blogspot.com.br/</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">VELA, EM ARGO NAVIS, O NAVIO</span></h3>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Acessando o Link abaixo, o Leitor encontrará o Tema Vela,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">incluído na Página sobre Argo Navis, o Antigo Navio desmembrado em Carina, Puppis e Vela<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://sobreargonavis.blogspot.com.br/">http://sobreargonavis.blogspot.com.br/</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="A Glowing Pool of Light: Planetary Nebula NGC 3132" src="http://imgsrc.hubblesite.org/hu/db/images/hs-1998-39-a-1280_wallpaper.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">A Glowing Pool of Light: Planetary Nebula NGC 3132</span></h1>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><img alt="A Glowing Pool of Light: Planetary Nebula NGC 3132" src="http://imgsrc.hubblesite.org/hu/db/images/hs-1998-39-a-large_web.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></div>
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<span style="line-height: 11px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></span></div>
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<span style="line-height: 11px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; line-height: 14px;"> - excerto apresentando ALFABETO GREGO, CONVENÇÕES E USO DA CARTA CELESTE</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>ARGO NAVIS, O NAVIO</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação representa o navio no qual Jasão trouxe o Velocino de Ouro para Colquita - e dizem que foi o primeiro navio a ser construído.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação, o Navio, fazia parte do grupo de 48 constelações relacionado por Ptolomeu. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">La Caille, porém, dividiu o Navio em<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Carina, Vela e Puppis: Quilha, Vela e Popa<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">Argo Navis</b><span style="line-height: 19.1875px; text-align: start;"> era uma grande </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="line-height: 19.1875px; text-align: start;"> meridional, representava o navio utilizado pelos </span><a href="http://pt.wikipedia.org/wiki/Argonautas" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Argonautas">argonautas</a><span style="line-height: 19.1875px; text-align: start;"> em suas viagens. Foi dividida em </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Carina" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Carina">Carina</a><span style="line-height: 19.1875px; text-align: start;">(quilha), </span><a href="http://pt.wikipedia.org/wiki/Puppis" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Puppis">Puppis</a><span style="line-height: 19.1875px; text-align: start;"> (popa) e </span><a href="http://pt.wikipedia.org/wiki/Vela_(constela%C3%A7%C3%A3o)" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Vela (constelação)">Vela</a><span style="line-height: 19.1875px; text-align: start;"> (velame); as </span><a href="http://pt.wikipedia.org/wiki/Designa%C3%A7%C3%A3o_de_Bayer" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Designação de Bayer">designações de Bayer</a><span style="line-height: 19.1875px; text-align: start;">, entretanto, não foram mudadas, de modo que α e β estão em Carina, γ e δ em Vela, ε em Carina, ζ em Puppis e assim por diante. Por outro lado, </span><a href="http://pt.wikipedia.org/wiki/Pyxis" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Pyxis">Pyxis</a><span style="line-height: 19.1875px; text-align: start;">, a constelação da Bússola, embora ocupe uma área que havia sido considerada como os mastros do Argo, possui designações de Bayer próprias.</span></span></div>
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<a href="http://pt.wikipedia.org/wiki/Argo_Navis" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Argo_Navis</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Ficheiro:Argo Navis Hevelius.jpg" src="http://upload.wikimedia.org/wikipedia/commons/c/cc/Argo_Navis_Hevelius.jpg" height="519" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="640" /></span></div>
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<a href="http://pt.wikipedia.org/wiki/Ficheiro:Argo_Navis_Hevelius.jpg" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Ficheiro:Argo_Navis_Hevelius.jpg</span></a><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="external text" href="http://contentdm.lindahall.org/cdm4/document.php?CISOROOT=/star_atlas&CISOPTR=479" rel="nofollow" style="text-decoration: none;">Atlas Coelestis</a><span style="line-height: 19.1875px; text-align: start;">. Johannes Hevelius drew the constellation in Uranographia, his celestial catalogue in 1690.</span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 15.828125px; text-align: left;">Desenho de </span><b style="line-height: 15.828125px; text-align: left;">Argo Navis</b><span style="line-height: 15.828125px; text-align: left;"> por </span><a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-image: none; line-height: 15.828125px; text-align: left; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a><span style="line-height: 15.828125px; text-align: left;"> (</span><a href="http://pt.wikipedia.org/wiki/1690" style="background-image: none; line-height: 15.828125px; text-align: left; text-decoration: none;" title="1690">1690</a><span style="line-height: 15.828125px; text-align: left;">)</span></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US" style="line-height: 18px;">The image for the "Historical Essay" is taken from<span class="apple-converted-space"> </span></span><a href="http://www.lindahall.org/events_exhib/exhibit/exhibits/stars/cel.htm" style="text-decoration: none;"><span lang="EN-US" style="line-height: 18px;">Andreas Cellarius,</span><span class="apple-converted-space"><span lang="EN-US" style="line-height: 18px;"> </span></span><i><span lang="EN-US" style="line-height: 18px;">Harmonia macrocosmica,</span></i><span class="apple-converted-space"><span lang="EN-US" style="line-height: 18px;"> </span></span><span lang="EN-US" style="line-height: 18px;">1661</span></a><span lang="EN-US" style="line-height: 18px;">.</span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US" style="line-height: 18px;"><o:p></o:p></span><a href="http://www.lindahall.org/events_exhib/exhibit/exhibits/stars/images/cel4full.jpg" style="line-height: 14.25pt; text-decoration: none;">http://www.lindahall.org/events_exhib/exhibit/exhibits/stars/images/cel4full.jpg</a></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Julius Schiller, <i>Coelum stellatum Christianum</i>, 1627</span><br />
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<a href="http://www.lindahall.org/events_exhib/exhibit/exhibits/stars/cel_sch.htm" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.lindahall.org/events_exhib/exhibit/exhibits/stars/cel_sch.htm</span></a></div>
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<span style="line-height: 13px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESA /AOES Medialab</span></span></div>
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<a href="http://spaceinimages.esa.int/Images/2009/05/GOCE_in_orbit" style="text-decoration: none;"><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://spaceinimages.esa.int/Images/2009/05/GOCE_in_orbit</span></span></a></div>
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<span lang="EN-US" style="text-transform: uppercase;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">GOCE IN ORBIT<o:p></o:p></span></span></div>
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<span lang="EN-US" style="text-transform: uppercase;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O NAVIO NAVEGANDO NO ESPAÇO</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US" style="text-transform: uppercase;"><br /></span><span lang="EN-US" style="text-transform: uppercase;"><br /></span></span></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgM4pD8zwvkGVDZpGB1cx-MHIdua9wGHGaBaKxk84svyQzXhAhVZBwC935rRu8I35ec1d8ne9uwijnB2Slr9cxGp5bOXtkdPHCb3WCmkbaAzu-l_JJZMbiUzyCk6EZ5O0YjG4cz7N2HbDZ_/s640/navio+bel%C3%ADssimo.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /><b><br /></b>Imagem extraída do Facebook, sem créditos</span><br />
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b><b><span lang="PT">Da Terra ao Céu<o:p></o:p></span></b></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="PT"> e ao Infinito</span></b><o:p></o:p></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelações, Estrelas e Objetos Celestes<o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(sob o ponto de vista do Mundo Ocidental)<o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Suas histórias, seus mitos, seus significados e suas sintetizadas descrições<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">Reunião das Informações e Compilação,</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">Tradução para a língua portuguesa (em alguns momentos)</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">bem como Comentários Pessoais:</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><span lang="PT"><b>Janine Milward</b></span></i><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Alguns dados<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(tais como Ascensão Reta e Declinação, em muitos dos casos)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">são época/equinócio 1980<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e devem requerer do Caminhante do Céu<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NASA/IPAC</b><b> EXTRAGALACTIC DATABASE –</b><b><o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="text-decoration: none;"><b>http://ned.ipac.caltech.edu/</b></a><b><o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="text-decoration: none;"><b>http://ned.ipac.caltech.edu/forms/byname.html</b></a><b><o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<b><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><b><span lang="EN-US"><o:p></o:p></span></b></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="EN-US">The</span></b><span class="apple-converted-space"><b><span lang="EN-US"> </span></b></span><b><span lang="EN-US">Internet STELLAR DATABASE</span></b><b><span lang="EN-US"><o:p></o:p></span></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="text-decoration: none;"><b><span lang="EN-US">http://www.stellar-database.com/</span></b></a><b><span lang="EN-US"><o:p></o:p></span></b></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<o:p></o:p></span></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Mario Jaci Monteiro - As Constelações, Cartas Celestes</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span><br />
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<span style="line-height: 14px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></span></div>
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<span style="line-height: 14px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; line-height: 18px;"> - excerto apresentando ALFABETO GREGO, CONVENÇÕES E USO DA CARTA CELESTE</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>VELA</b><o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Posicionamento:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 8h2m / 11h24m Declinação -37<sup>o</sup>.0 / -57<sup>o</sup>.0<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Mito:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação representa o navio no qual Jasão trouxe o Velocino de Ouro para Colquita - e dizem que foi o primeiro navio a ser construído.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>História:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação, o Navio, fazia parte do grupo de 48 constelações relacionado por Ptolomeu. Porém, La Caille dividiu o Navio em<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Carina, Vela e Puppis: Quilha, Vela e Popa<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Algumas Informações Interessantes acerca esta Constelação:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Aglomerados abertos 2670 e 2391 e 2547<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As estrelas Kapa e Delta Velorum formam a <i>Falsa Cruz</i> juntamente com as estrelas Iota e Epsilon Carinae . <o:p></o:p></span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgHG2EDgA0dn30uB2HFZQqlFTWUSktMbz79tZgpzmyTwpQlKKxUdkTzQQezEKZHgHO7j3toUgRwXA3-SnCU7pLvX1BQeLZtIbOVCX9qMYeqVN6X0uu3Q4sqXGVXMmcTGv_XpX5GsLkOBDEj/s1600/FALSA+CRUZ+-+MARIO+JACI.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgHG2EDgA0dn30uB2HFZQqlFTWUSktMbz79tZgpzmyTwpQlKKxUdkTzQQezEKZHgHO7j3toUgRwXA3-SnCU7pLvX1BQeLZtIbOVCX9qMYeqVN6X0uu3Q4sqXGVXMmcTGv_XpX5GsLkOBDEj/s640/FALSA+CRUZ+-+MARIO+JACI.jpg" height="186" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes - parte da carta de Vela</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Fronteiras:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação faz vizinhança com Antlia, Pyxis, Puppis, Carina e Centaurus. <o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Carina Navis" src="http://www.lindahall.org/services/digital/ebooks/bayer/bigpix/040040bc.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<a href="http://www.lindahall.org/services/digital/ebooks/bayer/bayer92.shtml" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.lindahall.org/services/digital/ebooks/bayer/bayer92.shtml</span></a><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><br /><br /><br /><strong>Kornelii Reissig. <em>Sozviezdiia Predstavlennyia</em>... 1829.</strong><br />Map XXVII. Argo Navis, Monoceros, Columba, Officina Typographica, Canis Minor, and Canis Major.</span><br />
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<a href="http://www.lindahall.org/services/digital/ebooks/reissig/reissig84.shtml" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.lindahall.org/services/digital/ebooks/reissig/reissig84.shtml</span></a><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg1RE-6QHoCbY44So82CWdz9cHoj_P0jEnLLJjjN0SHJsqJwIW4DpbnfdWeeYf9QgrSzYAJwLAwqkEM_i6I_gKYHHtpKMOXkiZXWCY3WnI7am8Htsi18tngzvWShz2uMHzjaL56fHYasJjP/s1600/stellarium,+vela.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg1RE-6QHoCbY44So82CWdz9cHoj_P0jEnLLJjjN0SHJsqJwIW4DpbnfdWeeYf9QgrSzYAJwLAwqkEM_i6I_gKYHHtpKMOXkiZXWCY3WnI7am8Htsi18tngzvWShz2uMHzjaL56fHYasJjP/s1600/stellarium,+vela.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium trabalhado no Programa Corel</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="background-color: white; color: #073763;">Algumas Estrelas </span></b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>e alguns objetos interessantes, em Vela:</b><o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT"><b>Al Suhail</b></span><span lang="PT"><b> - Gamma Velorum - Sistema Múltiplo</b><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 09h 07,3m - Declinação - 43<sup>o</sup> 21’<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual 2,22 - Distância 750 anos-luz<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mastro, nome proveniente da expressão árabe Al Suhail al Muhlif, ou seja, o mastro do navio. Tal vocábulo também é empregado para designar as estrelas Zeta e Lambda Velorum.<o:p></o:p></span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjo99tDqiiaSuIaQqhcGVZq1qk8nwVw1nkP_qHalorvUZK00dlEojmivdJ2MwRkzaKBSAEVEYI6j1JPMBpW6IUo5WGyCR36brngX_w_RYOeUNo9mLs1Gf-RAJDOqVFau8W8uwElB4zva4I3/s1600/suhail.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjo99tDqiiaSuIaQqhcGVZq1qk8nwVw1nkP_qHalorvUZK00dlEojmivdJ2MwRkzaKBSAEVEYI6j1JPMBpW6IUo5WGyCR36brngX_w_RYOeUNo9mLs1Gf-RAJDOqVFau8W8uwElB4zva4I3/s1600/suhail.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Delta Velorum</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude 1.95, com uma companheira de magnitude 5.1. Existe uma terceira companheira que é uma binária expectroscópica e com magnitude 10.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Markeb - Kappa Velorum</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Navio, do antigo asterismo árabe situado na constelação da Vela.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium trabalhado no Programa Corel</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC I2391 - Aglomerado Aberto Vela</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 08h39m Declinação -52<sup>o</sup>.59<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 2,6 Magnitude fotográfica da mais brilhante estrela 3,5<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Distância kpc 0,15 Diâmetro 45’ Tipo Espectral B4<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b> I2395 - Aglomerado Aberto Vela</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 08h40m Declinação -48<sup>o</sup>.07<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 4,6 Magnitude fotográfica da mais brilhante estrela 10,1<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Distância kpc 0,90 Diâmetro 20’ Tipo Espectral B2<o:p></o:p></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="background-color: white; color: #073763;">NGC 3132 - Nebulosa planetária na fronteira entre a Vela e Antlia:</span></b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b> O ANEL DO SUL</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma nebulosa planetária com uma estrela central muito brilhante que, por sua vez, possui uma companheira anã,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> aquela que representa a fonte da radiação da nebulosa.<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 3132</b><span style="line-height: 19.1875px; text-align: start;"> é uma </span><a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Nebulosa planetária">nebulosa planetária</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Vela" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Vela">constelação de Vela</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="John Herschel">John Herschel</a><span style="line-height: 19.1875px; text-align: start;"> em 1835, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="line-height: 19.1875px; text-align: start;"> refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;"> (+9,2), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="line-height: 19.1875px; text-align: start;">amadores ou com equipamentos superiores.</span></span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 19.1875px; text-align: start;"><br /></span><a href="http://pt.wikipedia.org/wiki/NGC_3132" style="text-decoration: none;">http://pt.wikipedia.org/wiki/NGC_3132</a></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">NGC 3132 is a striking example of a planetary nebula. This expanding cloud of gas, surrounding a dying star, is known to amateur astronomers in the southern hemisphere as the 'Eight-Burst' or the 'Southern Ring' Nebula.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Hubble Heritage Team (STScI/AURA/<a href="http://www.nasa.gov/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">NASA</a>/<a href="http://www.esa.int/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">ESA</a><a href="http://www.spacetelescope.org/images/opo9839a/" style="text-align: start; text-decoration: none;">http://www.spacetelescope.org/images/opo9839a/</a></span></div>
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<tr><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">NGC 3132: Nebulosa do Anel Sul</b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Créditos e direitos autorais : </b><a href="http://hla.stsci.edu/" style="text-decoration: none;">Hubble Legacy Archive</a>, <a href="http://www.esa.int/" style="text-decoration: none;">ESA</a>, <a href="http://www.nasa.gov/" style="text-decoration: none;">NASA</a>; <i>Processamento </i>- <a href="http://www.waid-observatory.com/index.html" style="text-decoration: none;">Donald Waid</a></span></td></tr>
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<tr><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Explicação: </b>Não foi a estrela mais brilhante perto do centro de <a href="http://adsabs.harvard.edu/abs/1997AAS...191.1508S" style="text-decoration: none;">NGC 3132</a>, mas a estrela mais apagada que criou esta estranha e bela <a href="http://www.seds.org/messier/planetar.html" style="text-decoration: none;">nebulosa planetária</a>. Apelidada de <a href="http://en.wikipedia.org/wiki/NGC_3132" style="text-decoration: none;">Eight-Burst</a> em inglês e conhecida por nós como <a href="http://apod.astronomos.com.br/ap060625.html" style="text-decoration: none;">Nebulosa do Anel</a> do Sul, o gás brilhante se originou das <a href="http://apod.astronomos.com.br/ap010301.html" style="text-decoration: none;">camadas externas</a> de uma estrela como o nosso <a href="http://asterisk.apod.com/viewtopic.php?f=24&t=18012" style="text-decoration: none;">Sol</a>. Nesta <a href="http://heritage.stsci.edu/1998/39/supplemental.html" style="text-decoration: none;">imagem em cores representativas</a>, a quente piscina de luz azul vista em torno deste <a href="http://apod.astronomos.com.br/ap970219.html" style="text-decoration: none;">sistema binário</a> é energizada pela superfície quente da estrela mais apagada. Embora tenha sido <a href="http://hubblesite.org/newscenter/archive/releases/1998/39/image/a/" style="text-decoration: none;">fotografada para explorar</a> simetrias incomuns, são as assimetrias que tornam esta <a href="http://apod.astronomos.com.br/planetary_nebulae.html" style="text-decoration: none;">nebulosa planetária</a> tão intrigante. Nem a forma incomum da concha externa mais fria, nem a estrutura ou a disposição das frias <a href="http://apod.astronomos.com.br/ap020703.html" style="text-decoration: none;">faixas filamentárias de poeira</a> que atravessam <a href="http://www.youtube.com/watch?v=t6rWxIGEvxY" style="text-decoration: none;">NGC 3132</a> são bem compreendidas.<a href="http://www.seds.org/messier/planetar.html" style="text-decoration: none;"></a></span></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><a href="http://apod.astronomos.com.br/apod.php?lk=ap130409.html" style="text-decoration: none;">http://apod.astronomos.com.br/apod.php?lk=ap130409.html</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Crédito: Hubble Legacy Archive, ESA, NASA</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta é a <a href="http://apod.nasa.gov/apod/ap130409.html" style="text-decoration: none;">nebulosa planetária NGC 3132</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Foi gerada após a morte de uma estrela semelhante ao Sol.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mas a estrela que lhe deu origem não é a mais brilhante na imagem; a sua “mãe” é a anã branca menos brilhante que aparece na imagem próxima do centro da nebulosa.</span></div>
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<a href="http://astropt.org/blog/2013/09/05/ngc-3132-nebulosa-do-anel-do-sul/" style="text-align: start; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://astropt.org/blog/2013/09/05/ngc-3132-nebulosa-do-anel-do-sul/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="ALMA Takes Close Look at Drama of Starbirth" src="http://alma.mtk.nao.ac.jp/e/news/assets_c/2013/08/20130820_eso1336a-thumb-592xauto-3495.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; margin: 0px; max-width: 100%; outline: 0px; padding: 0px;" title="ALMA Takes Close Look at Drama of Starbirth" /></span></div>
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<em style="border: 0px; margin: 0px; outline: 0px; padding: 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">This unprecedented image of Herbig-Haro object HH 46-47 combines radio observations acquired with the Atacama Large Millimeter/submillimeter Array (ALMA) with much shorter wavelength visible light observations from ESO’s New Technology Telescope (NTT). The ALMA observations (orange and green, lower right) of the newborn star reveal a large energetic jet moving away from us, which in the visible is hidden by dust and gas. To the left (in pink and purple) the visible part of the jet is seen, streaming partly towards us.</span></em></div>
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<a href="http://annesastronomynews.com/a-close-look-at-drama-of-starbirth/" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://annesastronomynews.com/a-close-look-at-drama-of-starbirth/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Image Credit: <em style="border: 0px; margin: 0px; outline: 0px; padding: 0px;">ESO/ALMA (ESO/NAOJ/NRAO)/H. Arce.</em> Acknowledgements: <em style="border: 0px; margin: 0px; outline: 0px; padding: 0px;">Bo Reipurth</em></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Young stars are violent objects that eject material at speeds of as high as one million kilometers per hour. When this material crashes into the surrounding gas it glows, creating a Herbig-Haro object <strong style="border: 0px; margin: 0px; outline: 0px; padding: 0px;">[1]</strong>. A spectacular example is named Herbig Haro 46-47 and is situated about 1,400 light-years from Earth in the southern constellation of Vela (The Sails). This object was the target of a study using ALMA during the Early Science phase, whilst the telescope was still under construction and well before the array was completed.</span></div>
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<strong style="border: 0px; margin: 0px; outline: 0px; padding: 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 3256, a distorted spiral galaxy in Vela</span></strong></div>
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<a href="http://annesastronomynews.com/photo-gallery-ii/galaxies-clusters/ngc-3256/" rel="attachment wp-att-9063" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="NGC 3256, a distorted galaxy in Vela" class="aligncenter size-full wp-image-9063" src="http://annesastronomynews.com/wp-content/uploads/2012/02/NGC-3256.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; display: block; margin: 0px auto; max-width: 100%; outline: 0px; padding: 0px; position: relative;" width="1024" /></span></a></div>
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<a href="http://annesastronomynews.com/annes-picture-of-the-day-distorted-galaxy-ngc-3256/" style="text-align: center; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://annesastronomynews.com/annes-picture-of-the-day-distorted-galaxy-ngc-3256/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Image Credit: <em style="border: 0px; margin: 0px; outline: 0px; padding: 0px;">NASA, ESA, the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University)</em></span></div>
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<span style="border: 0px; margin: 0px; outline: 0px; padding: 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 3256 is a very bright, distorted spiral galaxy of more than 100,000 light-years across, located about 100 million light-years away from Earth in the southern constellation of Vela (Sails), while it is receding from us at approximately 2804 kilometers per second. It lies near, and is probably interacting with the barred spiral galaxies NGC 3256A, NGC 3256B en NGC 3256C, and belongs to the Hydra-Centaurus supercluster of galaxies.</span></span></div>
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<span style="border: 0px; margin: 0px; outline: 0px; padding: 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Herbig Haro object HH 47, a stellar jet in Vela</span></span></div>
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<a href="http://annesastronomynews.com/photo-gallery-ii/nebulae-clouds/herbig-haro-object-hh-47/" rel="attachment wp-att-6428" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="HH 47" class="aligncenter size-full wp-image-6428" src="http://annesastronomynews.com/wp-content/uploads/2012/02/Herbig-Haro-object-HH-47.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; display: block; margin: 0px auto; max-width: 100%; outline: 0px; padding: 0px; position: relative;" title="Herbig Haro object HH 47, a stellar jet in Vela" width="1024" /></span></a></div>
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<a href="http://annesastronomynews.com/annes-picture-of-the-day-herbig-haro-object-hh-47/" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://annesastronomynews.com/annes-picture-of-the-day-herbig-haro-object-hh-47/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Image Credit: <em style="border: 0px; margin: 0px; outline: 0px; padding: 0px;">J. Morse/STScI, and NASA/ESA</em></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 25.59375px;"><span style="background-color: white; border: 0px; color: #073763; margin: 0px; outline: 0px; padding: 0px;">Herbig Haro object HH 47 is a bipolar stellar jet of 4.83 trillion kilometers long and 10 times the width of our Solar System located at the edge of the Gum Nebula, about 1140 light-years away in the southern constellation of Vela.</span></span></div>
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<br /><br /><br /><span style="font-weight: bold; line-height: 20px; text-align: start;">Exposed Cranium Nebula</span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://www.spitzer.caltech.edu/uploaded_files/images/0009/7431/sig13-013_Sm.jpg" /></span><br />
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<a href="http://www.spitzer.caltech.edu/uploaded_files/images/0009/7431/sig13-013_Sm.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spitzer.caltech.edu/uploaded_files/images/0009/7431/sig13-013_Sm.jpg</span></a><br />
<span style="line-height: 18px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The brain-like orb called PMR 1 has been nicknamed the "Exposed Cranium" nebula by Spitzer scientists.</span></span><br />
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<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Credit</span></dt>
<dd property="photoshop:Credit" style="margin: 0px; padding: 2px 0px 0px 5px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NASA/JPL-Caltech/J. Hora (Harvard-Smithsonian CfA)</span></dd></dl>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">About the Object</span></h3>
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<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Name</span></dt>
<dd style="margin: 0px; padding: 2px 0px 0px 5px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span property="dc:subject">PMR1</span> • <span property="dc:subject">PN G272.8+01.0</span> • <span property="dc:subject">Exposed Cranium Nebula</span></span></dd>
<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Type</span></dt>
<dd property="avm:Subject.Category" style="margin: 0px; padding: 2px 0px 0px 5px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Nebula > Type > Planetary</span></dd>
<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distance</span></dt>
<dd property="avm:Distance" style="margin: 0px; padding: 2px 0px 0px 5px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">5,000 Light Years</span></dd></dl>
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<dt style="font-weight: bold; line-height: 12px; margin: 0px; padding: 3px 0px 0px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Position (undefined)</span></dt>
<dd property="avm:Spatial.ReferenceValue" style="line-height: 12px; margin: 0px; padding: 2px 0px 0px 5px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">RA = 9<sup>h</sup> 28<sup>m</sup> 40.9<sup>s</sup></span></dd><dd property="avm:Spatial.ReferenceValue" style="line-height: 12px; margin: 0px; padding: 2px 0px 0px 5px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dec = -49° 36' 26.6"</span></dd>
<dt style="font-weight: bold; line-height: 12px; margin: 0px; padding: 3px 0px 0px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Field of View</span></dt>
<dd property="avm:Spatial.ReferenceDimension" style="line-height: 12px; margin: 0px; padding: 2px 0px 0px 5px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">5.5 x 5.5 arcminutes</span></dd>
<dt style="font-weight: bold; line-height: 12px; margin: 0px; padding: 3px 0px 0px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Orientation</span></dt>
<dd property="avm:Spatial.Rotation" style="line-height: 12px; margin: 0px; padding: 2px 0px 0px 5px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">North is 62.4° right of vertical</span></dd>
<dt style="font-weight: bold; line-height: 12px; margin: 0px; padding: 3px 0px 0px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constellation</span></dt>
<dd style="line-height: 12px; margin: 0px; padding: 2px 0px 0px 5px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Vela</span></dd><a href="http://www.spitzer.caltech.edu/images/5687-sig13-013-Exposed-Cranium-Nebula"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spitzer.caltech.edu/images/5687-sig13-013-Exposed-Cranium-Nebula</span></a><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="The Night Sky Atlas logo image" src="http://www.nightskyatlas.com/logo.gif" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">The Night Sky Atlas</span></h1>
<a href="http://www.nightskyatlas.com/index.jsp?rightAscension=8.9&declination=-47.8" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.nightskyatlas.com/index.jsp?rightAscension=8.9&declination=-47.8</span></a></div>
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<tr><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Visible in September before dawn, to May after dusk, best in January.</span></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Skyatlas PNG Image" src="http://www.nightskyatlas.com/skyatlas.jsp?rightAscension=8.9&declination=-47.8&viewAngle=90.0&viewRotation=0.0&width=700&height=500" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<b><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Named Stars Index - The Night Sky Atlas<o:p></o:p></span></span></b></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Vela: Visible in October before dawn, to June after dusk, best in February.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=9.369&declination=-55.011&viewAngle=25" style="text-decoration: none;">Markab</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">κ<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Kappa<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">´ship´<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.astro.uiuc.edu/~jkaler/sow/markab.html" style="text-decoration: none;" target="starnotes" title="Jim Kaler´s star notes for Markab">Jim Kaler Notes</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=9.133&declination=-43.432&viewAngle=25" style="text-decoration: none;">Suhail</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">λ<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Lambda<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">?? (no translation)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.astro.uiuc.edu/~jkaler/sow/suhail.html" style="text-decoration: none;" target="starnotes" title="Jim Kaler´s star notes for Suhail">Jim Kaler Notes</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=8.159&declination=-47.337&viewAngle=25" style="text-decoration: none;">Suhail or Regor</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">γ2<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Gamma 2<o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">?? (no translation); ´Roger´ backwards [Roger Chaffee, Apollo 1]<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=9.948&declination=-54.568&viewAngle=25" style="text-decoration: none;">Tseen Ke</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">φ<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Phi<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">´heaven's record´<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/starnames.jsp" style="text-decoration: none;">http://www.nightskyatlas.com/starnames.jsp</a><o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">DSO Names - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Vela: Visible in October before dawn, to June after dusk, best in February.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=10.1167&declination=-40.4367&viewAngle=20.0" style="text-decoration: none;">Eight-burst Planetary</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC3132<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">10h 07.0m<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-40° 26.2´<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">also Southern Ring<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=8.5&declination=-45.0&viewAngle=20.0" style="text-decoration: none;">Gum Nebula</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">08h 30.0m<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-45° 00.0´<o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 225pt;" valign="top" width="300"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Gum 12. Also Vela SNR, 20x12 deg extended. Contains Vela pulsar (PSR 0833-45).<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=9.005&declination=-45.9483&viewAngle=20.0" style="text-decoration: none;">Herschel´s Ray</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC2736<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">09h 00.3m<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-45° 56.9´<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">also Pencil Nebula<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=8.6717&declination=-52.9167&viewAngle=20.0" style="text-decoration: none;">Omicron Velorum Cluster</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">IC2391<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">08h 40.3m<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-52° 55.0´<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=9.005&declination=-45.9483&viewAngle=20.0" style="text-decoration: none;">Pencil Nebula</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC2736<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">09h 00.3m<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-45° 56.9´<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">also Herschel´s Ray<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=10.1167&declination=-40.4367&viewAngle=20.0" style="text-decoration: none;">Southern Ring Nebula</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC3132<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">10h 07.0m<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-40° 26.2´<o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(John Caldwell´s list) also Eight-burst Planetary<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=8.5&declination=-45.0&viewAngle=20.0" style="text-decoration: none;">Vela SNR</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">08h 30.0m<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-45° 00.0´<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Gum 12, the Gum Nebula. 20x12 deg extended. Contains Vela pulsar (PSR 0833-45).<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/dsoNames.jsp" style="text-decoration: none;">http://www.nightskyatlas.com/dsoNames.jsp</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Asterisms - The Night Sky Atlas<o:p></o:p></span></h1>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Vela: Visible in September before dawn, to May after dusk, best in January.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=8.9667&declination=-56.4667" style="text-decoration: none;">False Cross</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">2<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">7d X 4d<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Kappa and Delta Velorum/ Iota and Epsilon Carina<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/asterisms.jsp" style="text-decoration: none;">http://www.nightskyatlas.com/asterisms.jsp</a><o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Principal Stars of Vela - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/stardata.jsp?id=VEL" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/stardata.jsp?id=VEL</span></a><o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Multiple Stars of Vela - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/multipleStars.jsp?id=VEL" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/multipleStars.jsp?id=VEL</span></a><o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">NGC Objects in Vela - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/ngcData.jsp?id=VEL" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/ngcData.jsp?id=VEL</span></a><o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">IC Objects Data - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/icData.jsp" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/icData.jsp</span></a><o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Galaxy Clusters of Vela - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/catAbell.jsp?id=VEL" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/catAbell.jsp?id=VEL</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgZZhxsivvQPjt7hhiHWf6Lh18bhwZOfWaTItfRQ61oN8_pAcgE1kOx4lqqoaai9p15ZG_zh6vFNNZiPb1pWn3-KN2RDjGZwim-fIvwVMTDfY-mBhJQztKAAFemvjggecIeKMefnEqHWPeK/s1600/sch4med.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgZZhxsivvQPjt7hhiHWf6Lh18bhwZOfWaTItfRQ61oN8_pAcgE1kOx4lqqoaai9p15ZG_zh6vFNNZiPb1pWn3-KN2RDjGZwim-fIvwVMTDfY-mBhJQztKAAFemvjggecIeKMefnEqHWPeK/s640/sch4med.jpg" height="437" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Julius Schiller, <i>Coelum stellatum Christianum</i>, 1627</span></div>
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<a href="http://www.lindahall.org/events_exhib/exhibit/exhibits/stars/cel_sch.htm" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.lindahall.org/events_exhib/exhibit/exhibits/stars/cel_sch.htm</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas – As Constelações - são como janelas que se abrem para a infinitude do universo e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e sendo por nossa mente conscientizado. </span><br />
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">COM UM ABRAÇO ESTRELADO,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>REFERÊNCIAS BIBLIOGRÁFICAS IMPRESSAS </b><b>:</b></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">COMPILAÇÃO E TRADUÇÃO literal (quando necessária) de Janine Milward:<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As Cartas Celestes foram realizadas por Mario Jaci Monteiro e escaneadas por Janine<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- </span><b>Mario Jaci Monteiro</b> , <b>As Constelações, Cartas Celestes</b> -<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- <b>Wil Tirion - Atlas of the Night Sky</b> - The Hamlyn Publishing Group Limited, London, England</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- <b>Antonin Rükl - The Hamlyn Encyclopedia of Stars & Planets</b> - The Hamlyn Publishng Group Limited, London, England</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- <b>Richard Hinckley Allen, Star Names, Their Lore and Meaning</b>, Dover Publications, Inc, New York, USA</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- <b>Bernard Pellequer - Pequeno Guia do Céu</b> - Editora Martins Fontes, São Paulo, Brasil</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- <b>Identificação do Céu</b> (Livro que foi sendo revisado e reeditado algumas vezes) de autoria de <b>Fernando Vieira</b>,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Secretaria Municipal de Cultura, Fundação Planetário da Cidade do Rio de Janeiro<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(com dedicatória do próprio autor para mim em Curso de Identificação do Céu,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em 30/07/1999))<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do <b>Atlas Celeste</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">de autoria de <b>Ronaldo Rogério de Freitas Mourão</b>,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(com dedicatória do próprio autor para mim<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em evento realizado no Museu de Astronomia do Rio de Janeiro,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As Cartas Celestes foram realizadas por Mario Jaci Monteiro e escaneadas por Janine</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- </span><b>Mario Jaci Monteiro</b> , <b>As Constelações, Cartas Celestes</b> -<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC - com dedicatória do autor para mim, em março de 2004 (quando Mário Jaci generosamente me presenteou com um instrumento de observação (kepleriano) artesanalmente construído por ele).<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Hemisphaerium Coeli Australe in quo Fixarum loca secundum Eclipticae ductum ad anum 1730 . .</span></h2>
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<a href="http://www.raremaps.com/gallery/detail/35290/Hemisphaerium_Coeli_Australe_in_quo_Fixarum_loca_secundum_Eclipticae_ductum/Doppelmayr.html" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Hemisphaerium Coeli Australe in quo Fixarum loca secundum Eclipticae ductum ad anum 1730 . ." src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEicMxVQEO9u4O0sVR33ZT0E6HH7Zs3a90ZceXwCU3Auix4ELYx57LaFn_2XBuq31UO000yC7nvlPstC5_gSACXakPHoOz3T-FdbYM_03dyGa1FiNEctB-emBFN-Cww2JYRcl7P2oZdBxxzw/s1260/MAPA+CELESTE+GRANDE.jpg" height="1061" id="Image2_img" style="border: none; position: relative; visibility: visible;" width="1260" /> </span></a><br />
<span class="caption" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Nice example of Johanne Doppelmayr's map of the Southern Skies, with the constellations shown and the various stars illustrated in gold. Dopplemayr's decorative celestial chart illustrates the southern sky form the south ecliptic pole to ecliptic. The constellations are delineated based upon the catalogue of Johannes Hevelius and include Orion, Scorpio, Taurus, Eridanus and the Southern Cross. The constellations include some unusal additions, including the Peacock, Toucan, and a lovely unicorn called Monoceros.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b><img alt="The Southern Ring Nebula (NGC 3132)" src="http://imgsrc.hubblesite.org/hu/db/images/hs-1998-39-a-1440x960_wallpaper.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span><br />
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<tr><td class="tr-caption" style="font-size: 13px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span><br />
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-20059596081658708622013-08-20T08:34:00.003-07:002014-07-28T04:42:11.931-07:00TUCANA, O TUCANO<div align="center" class="MsoNormal" style="text-align: center;">
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px; text-align: start;">Meu Projeto</span></div>
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="font-size: small;">Da Terra ao Céu ....</span></span></a></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="font-size: small;">.....<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;">e ao Infinito </a></span></span></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><span style="font-size: small;">- As 88 Constelações</span></a></span></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><b>http://daterraaoceueaoinfinito.blogspot.com.br/</b></a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo</span></div>
<div style="font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;">
<span style="font-family: Arial, Helvetica, sans-serif;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://apod.nasa.gov/apod/image/1105/vltsky_beletsky_3114.jpg">http://apod.nasa.gov/apod/image/1105/vltsky_beletsky_3114.jpg</a></span></span></div>
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<b>Wonder and Mystery above the Very Large Telescopes </b></div>
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<b>Credit: </b><a href="mailto:ybialets%20at%20eso.org">Yuri Beletsky</a> (<a href="http://www.eso.org/">ESO</a>)</div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Uma das grandes alegrias em morar na roça</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e buscando céus mais escuros e transparentes,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">é poder observar a olho nu</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">as Nuvens Pequena e Grande de Magalhães.</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Eu sempre me divirto (e até quase fico tonta)</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">quando me deparo ao norte</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">com a maravilhante visão da Galáxia de Andromeda</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">(que pode ser observada a olho nu e usando a vista enviesada)</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e, num giro corporal, volto-me para os céus do sul</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e me deparo com a belíssima visão das Nuvens Pequena e Grande de Magalhães!</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">(Talvez a tontura também fique por conta</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">do fato de que posso olhar à visão desarmada</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">para três Galáxias que,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">adjuntando com a Galáxia onde me encontro, a Via Lactea,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">formam os principais conjuntos estelares</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">do nossa família galáctica tão intimamente nomeada de Grupo Local!).</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Aqui na roça, um antigo caseiro meu</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">dizia que estas duas "Nuvens"</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">são as mulas do presépio do Menino Jesus...</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Não importa o que se pense sobre estas Nuvens</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">- que quase sempre nos engana, parecendo nuvens mesmo! -,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">porque o importante é que elas a nós se apresentam enfeitando os céus do sul...,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e fazem isso de maneira tão simples, quase humilde!</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Quer dizer,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">as nuvens que nomeamos de Nuvens e que sabemos serem Galáxias</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">parecem esconder (assim como as nuvens escondem)</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">um mundo de maravilhas.... , </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">porém apenas se apresentando</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"> enquanto nuvens, simples nuvens, simples quase-enganos.</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Com um abraço estrelado,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Janine Milward</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEirVGnewK9rLHKmVgrjdhEKwhy0rM9cNiiNTfRo_MoSFEqe14OqtKEZbeePSR4CPKjoVOloV4nxa12YFd3_Vqxd_AbMPOTUzK9FPz5SzVn529oNJ2Ct07ZRqkjnQNWCSRCYKua9o3J-gYg/s1600/vltsky_beletsky_2198_annotated.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEirVGnewK9rLHKmVgrjdhEKwhy0rM9cNiiNTfRo_MoSFEqe14OqtKEZbeePSR4CPKjoVOloV4nxa12YFd3_Vqxd_AbMPOTUzK9FPz5SzVn529oNJ2Ct07ZRqkjnQNWCSRCYKua9o3J-gYg/s1600/vltsky_beletsky_2198_annotated.jpg" /></a></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://apod.nasa.gov/apod/image/1105/vltsky_beletsky_3114.jpg</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Wonder and Mystery above the Very Large Telescopes </span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"></span></span><br /></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Credit: Yuri Beletsky (ESO) </span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>A CONSTELAÇÃO DO TUCANO, Tucana,</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>ACOLHE A PEQUENA NUVEM DE MAGALHÃES</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>(e compartilha um pedacinho dessa maravilhosa Nuvem</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>com a constelação da HIDRA MACHO, HYDRUS.</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiNGQ2WXH0qaaO87ATN9USz4dO6Rxse3QdPZ1_jFKTqpeTcv4riCA1f2ZQaHaSMFYGnWccTiA2GkmA8cR7Tbj4QlmlxCTKughLDzGWlpoxshWRu_DGhw2PXGEovH2cwz-7KFktDq632pJs/s1600/ticano.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiNGQ2WXH0qaaO87ATN9USz4dO6Rxse3QdPZ1_jFKTqpeTcv4riCA1f2ZQaHaSMFYGnWccTiA2GkmA8cR7Tbj4QlmlxCTKughLDzGWlpoxshWRu_DGhw2PXGEovH2cwz-7KFktDq632pJs/s1600/ticano.jpg" /></a></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiF8RptJ77yalJAHHo3otUltVMOGWdazHLxI1d1ybqwCdNk0_o5Im46MAs-hKtMrZTz_9dbdfLR8vbNhToazXPp4Q2YDdy6DGsm24iEWDbfZ9qx_DQVrCbsYmFZ9Usspb_vNml1TTeJbYA/s1600/Tucana,+Mario+Jaci.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiF8RptJ77yalJAHHo3otUltVMOGWdazHLxI1d1ybqwCdNk0_o5Im46MAs-hKtMrZTz_9dbdfLR8vbNhToazXPp4Q2YDdy6DGsm24iEWDbfZ9qx_DQVrCbsYmFZ9Usspb_vNml1TTeJbYA/s1600/Tucana,+Mario+Jaci.jpg" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes - CARJ</span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><span lang="EN-US"> </span>TUCANA, O TUCANO</b></span></div>
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<span style="line-height: 22px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 22h5m / 1h22m Declinação -56<sup>o</sup>.7 / -75<sup>o</sup>.7<o:p></o:p></span></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelação adicionada por Bayer em 1604.<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Em Tucano, podemos observar alguns objetos extremamente interessante</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">s e mesmo a olho nu nos chamam a atenção: </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> 47 Tucanae e a Pequena Nuvem de Magalhães.<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Alpha Tucanae</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Distância 62 anos-luz<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Beta Tucanae - Estrela Dupla</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 00h29m Declinação -63<sup>o</sup>.14 Magnitude 4,4 e 4,6<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ângulo de Posição 169<sup>o</sup>.,4 Distância entre estrelas 27”,13<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Kappa Tucanae - Estrela Dupla</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 01h14m Declinação -69<sup>o</sup>.08 Magnitude 5,1 e 7,5<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ângulo de Posição 349<sup>o</sup>.,5 Distância entre estrelas 5”,50</span><br />
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<span style="font-family: Arial, sans-serif;">- 6<sup>a</sup>. Edição do <b>Atlas Celeste</b></span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">de autoria de <b>Ronaldo Rogério de Freitas Mourão</b>,</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b>Tucana</b>, o Tucano, é uma <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> do <a href="http://pt.wikipedia.org/wiki/Hemisf%C3%A9rio_celestial_sul" style="background: none; color: #0b0080; text-decoration: none;" title="Hemisfério celestial sul">hemisfério celestial sul</a>. O genitivo, usado para formar nomes de estrelas, é <b>Tucanae</b>. Na sua extremidade sul está a <a href="http://pt.wikipedia.org/wiki/Pequena_Nuvem_de_Magalh%C3%A3es" style="background: none; color: #0b0080; text-decoration: none;" title="Pequena Nuvem de Magalhães">Pequena Nuvem de Magalhães</a>.</div>
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As constelações vizinhas, de acordo com as fronteiras modernas, são <a href="http://pt.wikipedia.org/wiki/Phoenix_(constela%C3%A7%C3%A3o)" style="background: none; color: #0b0080; text-decoration: none;" title="Phoenix (constelação)">Phoenix</a>, <a href="http://pt.wikipedia.org/wiki/Grus" style="background: none; color: #0b0080; text-decoration: none;" title="Grus">Grus</a>, <a href="http://pt.wikipedia.org/wiki/Indus" style="background: none; color: #0b0080; text-decoration: none;" title="Indus">Indus</a>, <a href="http://pt.wikipedia.org/wiki/Octans" style="background: none; color: #0b0080; text-decoration: none;" title="Octans">Octans</a> e <a href="http://pt.wikipedia.org/wiki/Hydrus" style="background: none; color: #0b0080; text-decoration: none;" title="Hydrus">Hydrus</a>.</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;"><a href="http://pt.wikipedia.org/wiki/Tucana">http://pt.wikipedia.org/wiki/Tucana</a></span></span></div>
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<b>Alpha Tucanae</b> (α Tuc, α Tucanae) é a <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a> mais brilhante da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Tucana" style="background: none; color: #0b0080; text-decoration: none;" title="Tucana">Tucana</a>, com uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 2,86.<span class="reference" id="cite_ref-clpl4_2-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Tucanae#cite_note-clpl4-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> Com base em medições de <a href="http://pt.wikipedia.org/wiki/Paralaxe" style="background: none; color: #0b0080; text-decoration: none;" title="Paralaxe">paralaxe</a>, está a aproximadamente 200 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (61 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">parsecs</a>) da Terra.</div>
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É uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Bin%C3%A1ria_espectrosc%C3%B3pica" style="background: none; color: #0b0080; text-decoration: none;" title="Binária espectroscópica">binária espectroscópica</a>, o que significa que as duas estrelas não foram vistas individualmente com um telescópio, mas a presença da segunda estrela foi inferida observando mudanças no espectro da primária. O <a href="http://pt.wikipedia.org/wiki/Per%C3%ADodo_orbital" style="background: none; color: #0b0080; text-decoration: none;" title="Período orbital">período orbital</a> do sistema é de 4197,7 dias (11,5 anos).<span class="reference" id="cite_ref-ncsbo_4-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Tucanae#cite_note-ncsbo-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> O componente primário tem uma <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">classificação estelar</a> de K3 III,<span class="reference" id="cite_ref-simbad_1-7" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Tucanae#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> o que indica que é uma <a href="http://pt.wikipedia.org/wiki/Estrela_gigante" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela gigante">estrela gigante</a> que consumiu todo o hidrogênio em seu núcleo e <a href="http://pt.wikipedia.org/wiki/Evolu%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Evolução estelar">evoluiu</a> da <a href="http://pt.wikipedia.org/wiki/Sequ%C3%AAncia_principal" style="background: none; color: #0b0080; text-decoration: none;" title="Sequência principal">sequência principal</a>. Tem coloração alaranjada, típica de estrelas de classe K.</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Alpha_Tucanae</span></span></div>
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<b>Beta Tucanae</b> (Tuc β / β Tucanae) é um <a href="http://pt.wikipedia.org/wiki/Sistema_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Sistema estelar">sistema estelar</a> composto por seis <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Tucana" style="background: none; color: #0b0080; text-decoration: none;" title="Tucana">Tucana</a>. Três dessas estrelas têm uma <a href="http://pt.wikipedia.org/wiki/Designa%C3%A7%C3%A3o_de_Bayer" style="background: none; color: #0b0080; text-decoration: none;" title="Designação de Bayer">designação de Bayer</a> própria.</div>
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A estrela mais brilhante, Beta<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">1</span> Tucanae (Beta Tucanae A), tem <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 4,36 e <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">tipo espectral</a> B9V. Ela tem uma companheira, Beta Tucanae B, que tem classe espectral M3V e magnitude aparente 13,5. A separação de Beta Tucanae A e Beta Tucanae B é de 110 <a href="http://pt.wikipedia.org/wiki/Unidade_astron%C3%B4mica" style="background: none; color: #0b0080; text-decoration: none;" title="Unidade astronômica">UA</a> e elas levam 700 <a href="http://pt.wikipedia.org/wiki/Ano" style="background: none; color: #0b0080; text-decoration: none;" title="Ano">anos</a> para completar uma órbita.</div>
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Beta<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">2</span> Tucanae (Beta Tucanae C), tem magnitude aparente 4,8 e classe espectral A2V. Sua compenheira, Beta Tucanae D, tem magnitude aparente 6,0 e classe espectral A7V e está a uma distância média de 16,5 UA de Beta Tucanae C, levando 43 anos para completar uma órbita.</div>
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Beta<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">1</span> Tucanae e Beta<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">2</span> Tucanae estão a 1 160 UA de distância.</div>
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Beta<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">3</span> Tucanae está a 23 000 UA do resto do sistema, e não se sabe se está vinculado com as outras estrelas. Essa estrela tem classe espectral A0V e magnitude aparente 5,8 e tem uma companheira que está a 4 UA de distância.</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Beta1_Tucanae</span></span></div>
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<b>Kappa Tucanae</b> (κ Tuc / κ Tucanae) é um <a href="http://pt.wikipedia.org/wiki/Sistema_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Sistema estelar">sistema estelar</a> quádruplo na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Tucana" style="background: none; color: #0b0080; text-decoration: none;" title="Tucana">Tucana</a> que está a aproximadamente 66 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> e que tem <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> em conjunto de 4,25.</div>
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O sistema consiste em dois pares de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a> separados por 5,3 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a>. A estrela mais brilhante, Kappa Tucanae A, é uma <a href="http://pt.wikipedia.org/wiki/Estrela_subgigante" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela subgigante">subgigante</a> de <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">classe F</a> de magnitude aparente 5,1. A outra estrela, Kappa Tucanae B, tem magnitude aparente 7,3 e está a 5 segundos de arco, ou 100 <a href="http://pt.wikipedia.org/wiki/Unidade_astron%C3%B4mica" style="background: none; color: #0b0080; text-decoration: none;" title="Unidade astronômica">UA</a>, da estrela A. Essas estrelas levam 1 222 <a href="http://pt.wikipedia.org/wiki/Ano" style="background: none; color: #0b0080; text-decoration: none;" title="Ano">anos</a> para completar uma órbita.</div>
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Kappa Tucanae C e Kappa Tucanae D, que formam o outro par de estrelas, têm magnitude aparente 7,8 e 8,2, respectivamente, e estão mais próximos entre si do que o outro par, com uma distância de 1,12 segundos de arco, ou 23 UA. Essas estrelas levam 86 anos para completar uma órbita.</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Kappa_Tucanae</span></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><br />PLANETAS EXTRA-SOLARES</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>NA CONSTELAÇÃO DE TUCANO:</b></span></div>
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">HD 4308 b</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Planeta_extrassolar" style="background-attachment: initial; background-clip: initial; background-color: white; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Planeta extrassolar">planeta extrassolar</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> que orbita a </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-color: white; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;" title="Estrela">estrela</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> </span><a href="http://pt.wikipedia.org/wiki/HD_4308" style="background-attachment: initial; background-clip: initial; background-color: white; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="HD 4308">HD 4308</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">.</span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><br />
<table class="toccolours" style="background-color: #f9f9f9; border: 1px solid rgb(170, 170, 170); clear: right; color: #252525; font-family: sans-serif; font-size: 12px; margin: 0px 0px 1em 1em; padding: 5px; width: 300pxpx;"><caption style="font-size: 16px; margin-left: inherit;"><b>HD 4308 b</b></caption><tbody>
<tr><th colspan="2" style="background-color: #a0b0ff;" width="140px"><small><a href="http://pt.wikipedia.org/wiki/Exoplaneta" style="background: none; color: #0b0080; text-decoration: none;" title="Exoplaneta">Exoplaneta</a></small></th><td align="center" width="160px"><small><a href="http://pt.wikipedia.org/wiki/Anexo:Lista_de_estrelas_com_exoplaneta" style="background: none; color: #0b0080; text-decoration: none;" title="Anexo:Lista de estrelas com exoplaneta">Lista de exoplanetas</a></small></td></tr>
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<tr><th colspan="3" style="background-color: #a0b0ff;">Estrela mãe</th></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">Estrela</a></b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/HD_4308" style="background: none; color: #0b0080; text-decoration: none;" title="HD 4308">HD 4308</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/Tucana" style="background: none; color: #0b0080; text-decoration: none;" title="Tucana">Tucana</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Ascensão reta</a></b></td><td align="left">00<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 44<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 39,3<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></b></td><td align="left">-65° 38′ 58,3″</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnitude aparente</a></b></td><td align="left">6,54</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Dist%C3%A2ncia" style="background: none; color: #0b0080; text-decoration: none;" title="Distância">Distância</a></b></td><td align="left">71,39 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (21,9 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</td></tr>
<tr><th colspan="3" style="background-color: #a0b0ff;"><a href="http://pt.wikipedia.org/wiki/Elementos_orbitais" style="background: none; color: #0b0080; text-decoration: none;" title="Elementos orbitais">Elementos orbitais</a></th></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Semieixo_maior" style="background: none; color: #0b0080; text-decoration: none;" title="Semieixo maior">Semieixo maior</a></b></td><td align="left">0,115 ± 0,096 <a href="http://pt.wikipedia.org/wiki/Unidade_astron%C3%B4mica" style="background: none; color: #0b0080; text-decoration: none;" title="Unidade astronômica">UA</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Periastro" style="background: none; color: #0b0080; text-decoration: none;" title="Periastro">Periastro</a></b></td><td align="left">0,115 <a href="http://pt.wikipedia.org/wiki/Unidade_astron%C3%B4mica" style="background: none; color: #0b0080; text-decoration: none;" title="Unidade astronômica">UA</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Apoastro" style="background: none; color: #0b0080; text-decoration: none;" title="Apoastro">Apoastro</a></b></td><td align="left">0,115 <a href="http://pt.wikipedia.org/wiki/Unidade_astron%C3%B4mica" style="background: none; color: #0b0080; text-decoration: none;" title="Unidade astronômica">UA</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Excentricidade_orbital" style="background: none; color: #0b0080; text-decoration: none;" title="Excentricidade orbital">Excentricidade</a></b></td><td align="left">0,00 ± 0,01</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Per%C3%ADodo_orbital" style="background: none; color: #0b0080; text-decoration: none;" title="Período orbital">Período orbital</a></b></td><td align="left">15,56 ± 0,02 <a href="http://pt.wikipedia.org/wiki/Dia" style="background: none; color: #0b0080; text-decoration: none;" title="Dia">dias</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Argumento_do_periastro" style="background: none; color: #0b0080; text-decoration: none;" title="Argumento do periastro">Argumento do periastro</a></b></td><td align="left">359 ± 47°</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Amplitude" style="background: none; color: #0b0080; text-decoration: none;" title="Amplitude">Semi-amplitude</a></b></td><td align="left">4,07 ± 0,2 <a href="http://pt.wikipedia.org/wiki/Metro_por_segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Metro por segundo">m/s</a> <a href="http://pt.wikipedia.org/wiki/Metro_por_segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Metro por segundo">m/s</a></td></tr>
<tr><th colspan="3" style="background-color: #a0b0ff;">Características físicas</th></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Massa" style="background: none; color: #0b0080; text-decoration: none;" title="Massa">Massa</a></b></td><td align="left">>0,0442 <a href="http://pt.wikipedia.org/wiki/Massa_de_J%C3%BApiter" style="background: none; color: #0b0080; text-decoration: none;" title="Massa de Júpiter"><i>M</i><span style="height: 0px; line-height: 1; position: relative; top: 0.5ex; vertical-align: baseline;">J</span></a><br />>14 <a href="http://pt.wikipedia.org/wiki/Massa_da_Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Massa da Terra"><i>M</i><span style="height: 0px; line-height: 1; position: relative; top: 0.5ex; vertical-align: baseline;">⊕</span></a></td></tr>
<tr><th colspan="3" style="background-color: #a0b0ff;">Descoberta</th></tr>
<tr><td align="left" colspan="2"><b>Data da descoberta</b></td><td align="left">22 de agosto de 2005</td></tr>
<tr><td align="left" colspan="2"><b>Descobridores</b></td><td align="left"><a class="new" href="http://pt.wikipedia.org/w/index.php?title=St%C3%A9phane_Udry&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Stéphane Udry (página não existe)">Udry</a> <i>et al</i>.</td></tr>
<tr><td align="left" colspan="2"><b>Método de detecção</b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/Espectroscopia_Doppler" style="background: none; color: #0b0080; text-decoration: none;" title="Espectroscopia Doppler">Espectroscopia Doppler</a></td></tr>
<tr><td align="left" colspan="2"><b>Estado da descoberta</b></td><td align="left">Publicada</td></tr>
</tbody></table>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 19px;">http://pt.wikipedia.org/wiki/HD_4308_b</span><br />
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<b style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;">HD 215497 b</b><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Planeta_extrassolar" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Planeta extrassolar">planeta extrassolar</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> que orbita a </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Estrela">estrela</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> </span><a href="http://pt.wikipedia.org/wiki/HD_215497" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="HD 215497">HD 215497</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;">, que está localizada a 142 </span><a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Ano-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> da </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/Tucana" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Tucana">Tucana</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;">. Esse planeta tem no mínimo 5,4 vezes a </span><a href="http://pt.wikipedia.org/wiki/Massa_da_Terra" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Massa da Terra">massa da Terra</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> e leva 3,93 </span><a href="http://pt.wikipedia.org/wiki/Dia" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Dia">dias</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> para orbitar a estrela. O papel da descoberta desse planeta ainda não foi publicado e nem todos os parâmetros orbitais estão disponíveis. HD 215497 b foi descoberto em 19 de outubro de 2009 pelo </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=High_Accuracy_Radial_Velocity_Planet_Searcher&action=edit&redlink=1" style="background: none rgb(255, 255, 255); color: #a55858; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="High Accuracy Radial Velocity Planet Searcher (página não existe)">HARPS</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;">, juntamente com outros 29 planetas, incluindo </span><a href="http://pt.wikipedia.org/wiki/HD_215497_c" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="HD 215497 c">HD 215497 c</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;">.</span><br />
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<table class="toccolours" style="background-color: #f9f9f9; border: 1px solid rgb(170, 170, 170); clear: right; color: #252525; font-family: sans-serif; font-size: 12px; margin: 0px 0px 1em 1em; padding: 5px; width: 300pxpx;"><caption style="font-size: 16px; margin-left: inherit;"><b>HD 215497 b</b></caption><tbody>
<tr><th colspan="2" style="background-color: #a0b0ff;" width="140px"><small><a href="http://pt.wikipedia.org/wiki/Exoplaneta" style="background: none; color: #0b0080; text-decoration: none;" title="Exoplaneta">Exoplaneta</a></small></th><td align="center" width="160px"><small><a href="http://pt.wikipedia.org/wiki/Anexo:Lista_de_estrelas_com_exoplaneta" style="background: none; color: #0b0080; text-decoration: none;" title="Anexo:Lista de estrelas com exoplaneta">Lista de exoplanetas</a></small></td></tr>
<tr><td colspan="3" style="text-align: center;"></td></tr>
<tr><th colspan="3" style="background-color: #a0b0ff;">Estrela mãe</th></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">Estrela</a></b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/HD_215497" style="background: none; color: #0b0080; text-decoration: none;" title="HD 215497">HD 215497</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/Tucana" style="background: none; color: #0b0080; text-decoration: none;" title="Tucana">Tucana</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Ascensão reta</a></b></td><td align="left">22<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 46<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 36,7<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></b></td><td align="left">-56° 35′ 58,3″</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnitude aparente</a></b></td><td align="left">8,97</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Dist%C3%A2ncia" style="background: none; color: #0b0080; text-decoration: none;" title="Distância">Distância</a></b></td><td align="left">142 ± 7,8 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a>(43,5 ± 2,4 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</td></tr>
<tr><th colspan="3" style="background-color: #a0b0ff;"><a href="http://pt.wikipedia.org/wiki/Elementos_orbitais" style="background: none; color: #0b0080; text-decoration: none;" title="Elementos orbitais">Elementos orbitais</a></th></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Semieixo_maior" style="background: none; color: #0b0080; text-decoration: none;" title="Semieixo maior">Semieixo maior</a></b></td><td align="left">0,044 <a href="http://pt.wikipedia.org/wiki/Unidade_astron%C3%B4mica" style="background: none; color: #0b0080; text-decoration: none;" title="Unidade astronômica">UA</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Per%C3%ADodo_orbital" style="background: none; color: #0b0080; text-decoration: none;" title="Período orbital">Período orbital</a></b></td><td align="left">3,93 <a href="http://pt.wikipedia.org/wiki/Dia" style="background: none; color: #0b0080; text-decoration: none;" title="Dia">dias</a> (0,0108 <a href="http://pt.wikipedia.org/wiki/Ano" style="background: none; color: #0b0080; text-decoration: none;" title="Ano">anos</a>)</td></tr>
<tr><th colspan="3" style="background-color: #a0b0ff;">Características físicas</th></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Massa" style="background: none; color: #0b0080; text-decoration: none;" title="Massa">Massa</a></b></td><td align="left">>0,017 <a href="http://pt.wikipedia.org/wiki/Massa_de_J%C3%BApiter" style="background: none; color: #0b0080; text-decoration: none;" title="Massa de Júpiter"><i>M</i><span style="height: 0px; line-height: 1; position: relative; top: 0.5ex; vertical-align: baseline;">J</span></a><br />>5,4 <a href="http://pt.wikipedia.org/wiki/Massa_da_Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Massa da Terra"><i>M</i><span style="height: 0px; line-height: 1; position: relative; top: 0.5ex; vertical-align: baseline;">⊕</span></a></td></tr>
<tr><th colspan="3" style="background-color: #a0b0ff;">Descoberta</th></tr>
<tr><td align="left" colspan="2"><b>Data da descoberta</b></td><td align="left">19 de outubro de 2009</td></tr>
<tr><td align="left" colspan="2"><b>Descobridores</b></td><td align="left">Lo Curto <i>et al</i>.</td></tr>
<tr><td align="left" colspan="2"><b>Método de detecção</b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/Velocidade_radial" style="background: none; color: #0b0080; text-decoration: none;" title="Velocidade radial">Velocidade radial</a> (<a class="new" href="http://pt.wikipedia.org/w/index.php?title=High_Accuracy_Radial_Velocity_Planet_Searcher&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="High Accuracy Radial Velocity Planet Searcher (página não existe)">HARPS</a>)</td></tr>
</tbody></table>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/HD_215497_b</span><br />
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<b style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;">HD 215497 c</b><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Planeta_extrassolar" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Planeta extrassolar">planeta extrassolar</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> que orbita a </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Estrela">estrela</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> </span><a href="http://pt.wikipedia.org/wiki/HD_215497" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="HD 215497">HD 215497</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;">, que está localizada a 140 </span><a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Ano-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> da </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/Tucana" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Tucana">Tucana</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;">. Esse planeta tem no mínimo um terço da </span><a href="http://pt.wikipedia.org/wiki/Massa_de_J%C3%BApiter" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Massa de Júpiter">massa de Júpiter</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> e leva 567 </span><a href="http://pt.wikipedia.org/wiki/Dia" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Dia">dias</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> para orbitar a estrela. Esse planeta foi descoberto pelo </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=High_Accuracy_Radial_Velocity_Planet_Searcher&action=edit&redlink=1" style="background: none rgb(255, 255, 255); color: #a55858; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="High Accuracy Radial Velocity Planet Searcher (página não existe)">HARPS</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> em 19 de outubro de 2009, juntamente com outros 29 planetas, incluindo </span><a href="http://pt.wikipedia.org/wiki/HD_215497_b" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="HD 215497 b">HD 215497 b</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;">.</span><br />
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<table class="toccolours" style="background-color: #f9f9f9; border: 1px solid rgb(170, 170, 170); clear: right; color: #252525; font-family: sans-serif; font-size: 12px; margin: 0px 0px 1em 1em; padding: 5px; width: 300pxpx;"><caption style="font-size: 16px; margin-left: inherit;"><b>HD 215497 c</b></caption><tbody>
<tr><th colspan="2" style="background-color: #a0b0ff;" width="140px"><small><a href="http://pt.wikipedia.org/wiki/Exoplaneta" style="background: none; color: #0b0080; text-decoration: none;" title="Exoplaneta">Exoplaneta</a></small></th><td align="center" width="160px"><small><a href="http://pt.wikipedia.org/wiki/Anexo:Lista_de_estrelas_com_exoplaneta" style="background: none; color: #0b0080; text-decoration: none;" title="Anexo:Lista de estrelas com exoplaneta">Lista de exoplanetas</a></small></td></tr>
<tr><td colspan="3" style="text-align: center;"></td></tr>
<tr><th colspan="3" style="background-color: #a0b0ff;">Estrela mãe</th></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">Estrela</a></b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/HD_215497" style="background: none; color: #0b0080; text-decoration: none;" title="HD 215497">HD 215497</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/Tucana" style="background: none; color: #0b0080; text-decoration: none;" title="Tucana">Tucana</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Ascensão reta</a></b></td><td align="left">22<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 46<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 36,7<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></b></td><td align="left">-56° 35′ 58,3″</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnitude aparente</a></b></td><td align="left">8,97</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Dist%C3%A2ncia" style="background: none; color: #0b0080; text-decoration: none;" title="Distância">Distância</a></b></td><td align="left">142 ± 7,8 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a>(43,5 ±2,4 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</td></tr>
<tr><th colspan="3" style="background-color: #a0b0ff;"><a href="http://pt.wikipedia.org/wiki/Elementos_orbitais" style="background: none; color: #0b0080; text-decoration: none;" title="Elementos orbitais">Elementos orbitais</a></th></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Semieixo_maior" style="background: none; color: #0b0080; text-decoration: none;" title="Semieixo maior">Semieixo maior</a></b></td><td align="left">1,282 <a href="http://pt.wikipedia.org/wiki/Unidade_astron%C3%B4mica" style="background: none; color: #0b0080; text-decoration: none;" title="Unidade astronômica">UA</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Excentricidade_orbital" style="background: none; color: #0b0080; text-decoration: none;" title="Excentricidade orbital">Excentricidade</a></b></td><td align="left">0,49 ± 0,04</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Per%C3%ADodo_orbital" style="background: none; color: #0b0080; text-decoration: none;" title="Período orbital">Período orbital</a></b></td><td align="left">569,94 <a href="http://pt.wikipedia.org/wiki/Dia" style="background: none; color: #0b0080; text-decoration: none;" title="Dia">dias</a> (1,56 <a href="http://pt.wikipedia.org/wiki/Ano" style="background: none; color: #0b0080; text-decoration: none;" title="Ano">anos</a>)</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Argumento_do_periastro" style="background: none; color: #0b0080; text-decoration: none;" title="Argumento do periastro">Argumento do periastro</a></b></td><td align="left">45 ± 4°</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Amplitude" style="background: none; color: #0b0080; text-decoration: none;" title="Amplitude">Semi-amplitude</a></b></td><td align="left">10,10 ± 0,65 <a href="http://pt.wikipedia.org/wiki/Metro_por_segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Metro por segundo">m/s</a> <a href="http://pt.wikipedia.org/wiki/Metro_por_segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Metro por segundo">m/s</a></td></tr>
<tr><th colspan="3" style="background-color: #a0b0ff;">Características físicas</th></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Massa" style="background: none; color: #0b0080; text-decoration: none;" title="Massa">Massa</a></b></td><td align="left">>0,33 <a href="http://pt.wikipedia.org/wiki/Massa_de_J%C3%BApiter" style="background: none; color: #0b0080; text-decoration: none;" title="Massa de Júpiter"><i>M</i><span style="height: 0px; line-height: 1; position: relative; top: 0.5ex; vertical-align: baseline;">J</span></a><br />>104,3 <a href="http://pt.wikipedia.org/wiki/Massa_da_Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Massa da Terra"><i>M</i><span style="height: 0px; line-height: 1; position: relative; top: 0.5ex; vertical-align: baseline;">⊕</span></a></td></tr>
<tr><th colspan="3" style="background-color: #a0b0ff;">Descoberta</th></tr>
<tr><td align="left" colspan="2"><b>Data da descoberta</b></td><td align="left">19 de outubro de 2009</td></tr>
<tr><td align="left" colspan="2"><b>Descobridores</b></td><td align="left">Lo Curto <i>et al</i>.</td></tr>
<tr><td align="left" colspan="2"><b>Método de detecção</b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/Velocidade_radial" style="background: none; color: #0b0080; text-decoration: none;" title="Velocidade radial">Velocidade radial</a> (<a class="new" href="http://pt.wikipedia.org/w/index.php?title=High_Accuracy_Radial_Velocity_Planet_Searcher&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="High Accuracy Radial Velocity Planet Searcher (página não existe)">HARPS</a>)</td></tr>
<tr><td align="left" colspan="2"><b>Estado da descoberta</b></td><td align="left">Publicada</td></tr>
</tbody></table>
<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/HD_215497_c</span><br />
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<b style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;">HD 221287 b</b><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Planeta_extrassolar" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Planeta extrassolar">planeta extrassolar</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> que orbita a </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Estrela">estrela</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> </span><a href="http://pt.wikipedia.org/wiki/HD_221287" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="HD 221287">HD 221287</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;">. Esse planeta tem massa mínima de 3,12 </span><a href="http://pt.wikipedia.org/wiki/Massa_de_J%C3%BApiter" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Massa de Júpiter"><i>M</i><span style="height: 0px; line-height: 1; position: relative; top: 0.5ex; vertical-align: baseline;">J</span></a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> e orbita a estrela a uma distância média de 1,25</span><a href="http://pt.wikipedia.org/wiki/Unidade_astron%C3%B4mica" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Unidade astronômica">UA</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;">, levando 456 </span><a href="http://pt.wikipedia.org/wiki/Dia" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Dia">dias</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> para completar uma órbita. </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Dominique_Naef&action=edit&redlink=1" style="background: none rgb(255, 255, 255); color: #a55858; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Dominique Naef (página não existe)">Dominique Naef</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"> o descobriu em 2007, usando o </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=High_Accuracy_Radial_Velocity_Planet_Searcher&action=edit&redlink=1" style="background: none rgb(255, 255, 255); color: #a55858; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;" title="High Accuracy Radial Velocity Planet Searcher (página não existe)">espectrógrafo HARPS</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;">, no </span><a href="http://pt.wikipedia.org/wiki/Chile" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Chile">Chile</a><span style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px; text-align: start;">.</span><br />
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<table class="toccolours" style="background-color: #f9f9f9; border: 1px solid rgb(170, 170, 170); clear: right; color: #252525; font-family: sans-serif; font-size: 12px; margin: 0px 0px 1em 1em; padding: 5px; width: 300pxpx;"><caption style="font-size: 16px; margin-left: inherit;"><b>HD 221287 b</b></caption><tbody>
<tr><th colspan="2" style="background-color: #a0b0ff;" width="140px"><small><a href="http://pt.wikipedia.org/wiki/Exoplaneta" style="background: none; color: #0b0080; text-decoration: none;" title="Exoplaneta">Exoplaneta</a></small></th><td align="center" width="160px"><small><a href="http://pt.wikipedia.org/wiki/Anexo:Lista_de_estrelas_com_exoplaneta" style="background: none; color: #0b0080; text-decoration: none;" title="Anexo:Lista de estrelas com exoplaneta">Lista de exoplanetas</a></small></td></tr>
<tr><td colspan="3" style="text-align: center;"></td></tr>
<tr><th colspan="3" style="background-color: #a0b0ff;">Estrela mãe</th></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">Estrela</a></b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/HD_221287" style="background: none; color: #0b0080; text-decoration: none;" title="HD 221287">HD 221287</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/Tucana" style="background: none; color: #0b0080; text-decoration: none;" title="Tucana">Tucana</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Ascensão reta</a></b></td><td align="left">23<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 31<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 20,3<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></b></td><td align="left">-58° 12′ 35,0″</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnitude aparente</a></b></td><td align="left">7,82</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Dist%C3%A2ncia" style="background: none; color: #0b0080; text-decoration: none;" title="Distância">Distância</a></b></td><td align="left">172,5 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (52,9 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</td></tr>
<tr><th colspan="3" style="background-color: #a0b0ff;"><a href="http://pt.wikipedia.org/wiki/Elementos_orbitais" style="background: none; color: #0b0080; text-decoration: none;" title="Elementos orbitais">Elementos orbitais</a></th></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Semieixo_maior" style="background: none; color: #0b0080; text-decoration: none;" title="Semieixo maior">Semieixo maior</a></b></td><td align="left">1,25 ± 0,04 <a href="http://pt.wikipedia.org/wiki/Unidade_astron%C3%B4mica" style="background: none; color: #0b0080; text-decoration: none;" title="Unidade astronômica">UA</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Periastro" style="background: none; color: #0b0080; text-decoration: none;" title="Periastro">Periastro</a></b></td><td align="left">1,15 <a href="http://pt.wikipedia.org/wiki/Unidade_astron%C3%B4mica" style="background: none; color: #0b0080; text-decoration: none;" title="Unidade astronômica">UA</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Apoastro" style="background: none; color: #0b0080; text-decoration: none;" title="Apoastro">Apoastro</a></b></td><td align="left">1,35 <a href="http://pt.wikipedia.org/wiki/Unidade_astron%C3%B4mica" style="background: none; color: #0b0080; text-decoration: none;" title="Unidade astronômica">UA</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Excentricidade_orbital" style="background: none; color: #0b0080; text-decoration: none;" title="Excentricidade orbital">Excentricidade</a></b></td><td align="left">0,08 ± 0,11</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Per%C3%ADodo_orbital" style="background: none; color: #0b0080; text-decoration: none;" title="Período orbital">Período orbital</a></b></td><td align="left">456,1 ± 6,5 <a href="http://pt.wikipedia.org/wiki/Dia" style="background: none; color: #0b0080; text-decoration: none;" title="Dia">dias</a>(1,2487 <a href="http://pt.wikipedia.org/wiki/Ano" style="background: none; color: #0b0080; text-decoration: none;" title="Ano">anos</a>)</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Argumento_do_periastro" style="background: none; color: #0b0080; text-decoration: none;" title="Argumento do periastro">Argumento do periastro</a></b></td><td align="left">98 ± 72°</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Amplitude" style="background: none; color: #0b0080; text-decoration: none;" title="Amplitude">Semi-amplitude</a></b></td><td align="left">71 ± 13 <a href="http://pt.wikipedia.org/wiki/Metro_por_segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Metro por segundo">m/s</a> <a href="http://pt.wikipedia.org/wiki/Metro_por_segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Metro por segundo">m/s</a></td></tr>
<tr><th colspan="3" style="background-color: #a0b0ff;">Características físicas</th></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Massa" style="background: none; color: #0b0080; text-decoration: none;" title="Massa">Massa</a></b></td><td align="left">>3,12 ± 0,78 <a href="http://pt.wikipedia.org/wiki/Massa_de_J%C3%BApiter" style="background: none; color: #0b0080; text-decoration: none;" title="Massa de Júpiter"><i>M</i><span style="height: 0px; line-height: 1; position: relative; top: 0.5ex; vertical-align: baseline;">J</span></a><br />>992 <a href="http://pt.wikipedia.org/wiki/Massa_da_Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Massa da Terra"><i>M</i><span style="height: 0px; line-height: 1; position: relative; top: 0.5ex; vertical-align: baseline;">⊕</span></a></td></tr>
<tr><th colspan="3" style="background-color: #a0b0ff;">Descoberta</th></tr>
<tr><td align="left" colspan="2"><b>Data da descoberta</b></td><td align="left">5 de março de 2007</td></tr>
<tr><td align="left" colspan="2"><b>Descobridores</b></td><td align="left">Naef <i>et al</i>.</td></tr>
<tr><td align="left" colspan="2"><b>Método de detecção</b></td><td align="left"><a class="new" href="http://pt.wikipedia.org/w/index.php?title=High_Accuracy_Radial_Velocity_Planet_Searcher&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="High Accuracy Radial Velocity Planet Searcher (página não existe)">Espectrógrafo HARPS</a></td></tr>
<tr><td align="left" colspan="2"><b>Estado da descoberta</b></td><td align="left">Publicada</td></tr>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/HD_221287_b</span><br />
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif; line-height: 14.25pt;"><b>AGLOMERADOS GLOBULARES,</b></span><br />
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>GALÁXIAS E QUASAR,</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>EM TUCANO</b></span></div>
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<b><span style="color: #660000; font-size: large;"><span style="background-color: white; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">The </span><span style="background-color: white; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">Tucana Dwarf Galaxy</span></span></b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> is a </span><a href="http://en.wikipedia.org/wiki/Dwarf_galaxy" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Dwarf galaxy">dwarf galaxy</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> in the </span><a href="http://en.wikipedia.org/wiki/Constellation" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Constellation">constellation</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> </span><a href="http://en.wikipedia.org/wiki/Tucana" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Tucana">Tucana</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. It was discovered in 1990 by R.J. Lavery of </span><a href="http://en.wikipedia.org/wiki/Mount_Stromlo_Observatory" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Mount Stromlo Observatory">Mount Stromlo Observatory</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. It is composed of very old stars and is very isolated from other galaxies. Its location on the opposite side of the Milky Way from other </span><a href="http://en.wikipedia.org/wiki/Local_Group" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Local Group">Local Group</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> galaxies makes it an important object for study.</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjkFHT0v9jvJ2LgJvdyshcLTYQlsAWsW1R5hj9TscZHOC5x4HY_RPdqCdiuUgZCr56zFInZvVdao-3-_rrqEk4x_rVrvgGXXU2MMAQRFuWiQjVUuyrsavjmwo4jCBdcza4Eg7OXomwnRqAZ/s1600/640px-Local_Group.svg.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjkFHT0v9jvJ2LgJvdyshcLTYQlsAWsW1R5hj9TscZHOC5x4HY_RPdqCdiuUgZCr56zFInZvVdao-3-_rrqEk4x_rVrvgGXXU2MMAQRFuWiQjVUuyrsavjmwo4jCBdcza4Eg7OXomwnRqAZ/s1600/640px-Local_Group.svg.png" /></a></div>
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<span style="background-color: white; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"><span style="color: #073763; font-family: sans-serif;">http://en.wikipedia.org/wiki/File:Local_Group.svg</span></span></div>
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<tr style="vertical-align: top;"><td class="description"><div class="description mw-content-ltr en" dir="ltr" lang="en" style="direction: ltr;">
<span style="background-color: white;"><span style="color: #073763;"><span class="language en" title=""><b>English:</b></span> The local group of galaxies surrounding the Milky Way</span></span></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_date" style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-weight: bold; padding-right: 0.4em; text-align: right; width: 191.6875px;"><span style="background-color: white;"><span style="color: #073763;">Date</span></span></td><td><span style="background-color: white; white-space: nowrap;"><span style="color: #073763;">21 September 2006</span></span></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-weight: bold; padding-right: 0.4em; text-align: right; width: 191.6875px;"><span style="background-color: white;"><span style="color: #073763;">Source</span></span></td><td><span style="background-color: white;"><span style="color: #073763;">Re-drawn from <a href="http://commons.wikimedia.org/wiki/File:Local_Group.JPG" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="File:Local Group.JPG">File:Local Group.JPG</a>, originally from <a class="external free" href="http://www.atlasoftheuniverse.com/" rel="nofollow" style="background-attachment: initial, initial; background-clip: initial, initial; background-image: linear-gradient(transparent, transparent), url(data:image/svg+xml; background-origin: initial, initial; background-position: 100% 50%, 100% 50%; background-repeat: no-repeat, initial no-repeat, initial; background-size: initial, initial; padding-right: 13px; text-decoration: none;">http://www.atlasoftheuniverse.com</a></span></span></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-weight: bold; padding-right: 0.4em; text-align: right; width: 191.6875px;"><span style="background-color: white;"><span style="color: #073763;">Author</span></span></td><td><span style="background-color: white;"><span style="color: #073763;">Richard Powell</span></span></td></tr>
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<b>A <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_An%C3%A3_de_Tucana" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia Anã de Tucana">Galáxia Anã de Tucana</a></b> que foi descoberta em <a href="http://pt.wikipedia.org/wiki/1990" style="background: none; color: #0b0080; text-decoration: none;" title="1990">1990</a> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_an%C3%A3_esferoidal" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia anã esferoidal">galáxia anã esferoidal</a> do tipo dE5 que é um membro isolado do nosso <a href="http://pt.wikipedia.org/wiki/Grupo_Local" style="background: none; color: #0b0080; text-decoration: none;" title="Grupo Local">Grupo Local</a><span class="reference" id="cite_ref-LaveryMighell1992_13-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Tucana#cite_note-LaveryMighell1992-13" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">13</a></span> . Ela está localizada a 870 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">kiloparsecs</a> (2.800 mil anos luz) do nosso <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Sistema_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Sistema solar">sistema solar</a>, por volta de 1.100 kiloparsecs (3.600 mil anos luz) do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Baricentro" style="background: none; color: #0b0080; text-decoration: none;" title="Baricentro">baricentro</a> do Grupo Local, a segunda galáxia mais remota de todos os membros do grupo perdendo apenas para a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_An%C3%A3_Irregular_de_Sagit%C3%A1rio" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia Anã Irregular de Sagitário">Galáxia Anã Irregular de Sagitário</a><span class="reference" id="cite_ref-vandenbergh2000_14-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Tucana#cite_note-vandenbergh2000-14" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">14</a></span> .</div>
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<a href="http://pt.wikipedia.org/wiki/Tucana">http://pt.wikipedia.org/wiki/Tucana</a><br />
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A <b>galáxia Anã de Tucana</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_an%C3%A3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia anã">galáxia anã</a> na direção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Tucana" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Tucana">Tucana</a>. Ela foi descoberta por R. J. Lavrey em <a href="http://pt.wikipedia.org/wiki/1990" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1990">1990</a> no Observatório Monte Stromlo.</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Gal%C3%A1xia_An%C3%A3_de_Tucana</span></span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhf2lv7xtWNbVN2AN3RWhsUYnWxhWfgUSQewG9SlwWWIWj3s2qCV6pLhbnv4pszPIscEcvX9G5M40waA6KXGm4o28LIfhTqc4ltpbWERB8eWbgzMFdgkL6eJc8D5SkG7_88vqX-iCAgVQhx/s1600/800px-Tucana_Dwarf_Hubble_WikiSky.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhf2lv7xtWNbVN2AN3RWhsUYnWxhWfgUSQewG9SlwWWIWj3s2qCV6pLhbnv4pszPIscEcvX9G5M40waA6KXGm4o28LIfhTqc4ltpbWERB8eWbgzMFdgkL6eJc8D5SkG7_88vqX-iCAgVQhx/s1600/800px-Tucana_Dwarf_Hubble_WikiSky.jpg" /></a></div>
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<span style="font-family: sans-serif; font-size: 14px; line-height: 22.399999618530273px;"><span style="background-color: white; color: #252525;">http://en.wikipedia.org/wiki/Tucana_Dwarf#med</span><span style="color: #073763;"><span style="background-color: white;">iaviewer/File:Tucana_Dwarf_Hubble_WikiSky.jpg</span></span></span></div>
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<span style="background-color: white; color: #073763;"><span class="mw-mmv-title" original-title="File name" style="font-size: 1.2em; max-width: 60%;">Tucana Dwarf Hubble WikiSky</span><a class="mw-mmv-license" href="http://commons.wikimedia.org/wiki/File:Tucana_Dwarf_Hubble_WikiSky.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-size: 0.9em; padding: 0px 10px; text-align: right; text-decoration: none;" target="">Public Domain</a></span></div>
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<span class="mw-mmv-source-author" original-title="Author and source information" style="background-color: white;"><span style="color: #073763;"><span class="mw-mmv-author"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="en:NASA">en:NASA</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/STScI" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="en:STScI">en:STScI</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span> - <span class="mw-mmv-source"><a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="en:WikiSky">en:WikiSky</a>'s snapshot tool - <a class="external autonumber" href="http://wikisky.org/snapshot?img_size=&img_res=&ra=22.69687685317207&de=-64.42135429295065&angle=0.05501760563380282&projection=tan&rotation=-38.85255240682787&survey=astrophoto&img_id=905828&width=4000&height=4000&img_borders=0&interpolation=bicubic2&jpeg_quality=0.85" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;">[1]</a></span></span></span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiUBwmyrqd7W4m6tVtJsZF1iIFAZ1nGTMZPof1d0pbKIXSVyXN0NfA7w8LF2vDkh_cOcwlEjRbWMNZ30xNUa9O6jwmUITpXz_TpdSXDTgZqa8L__Ogrs975lZzqDX1wPG4tGZbZVQfU8Qo6/s1600/800px-5_Local_Galactic_Group_(ELitU).png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiUBwmyrqd7W4m6tVtJsZF1iIFAZ1nGTMZPof1d0pbKIXSVyXN0NfA7w8LF2vDkh_cOcwlEjRbWMNZ30xNUa9O6jwmUITpXz_TpdSXDTgZqa8L__Ogrs975lZzqDX1wPG4tGZbZVQfU8Qo6/s1600/800px-5_Local_Galactic_Group_(ELitU).png" /></a></div>
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<span class="mw-mmv-source-author" original-title="Author and source information" style="background-color: white; color: #073763; font-family: sans-serif; line-height: 24px; white-space: nowrap;">http://en.wikipedia.org/wiki/Milky_Way#mediaviewer/File:5_Local_Galactic_Group_(ELitU).png</span></div>
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<span style="background-color: white;"><span class="mw-mmv-title" original-title="File name" style="font-size: 1.2em; max-width: 60%;">5 Local Galactic Group (ELitU)</span><a class="mw-mmv-license cc-license" href="http://creativecommons.org/licenses/by-sa/3.0" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-size: 0.9em; padding: 0px 10px; text-align: right; text-decoration: none;" target="_blank">CC BY-SA 3.0</a></span></div>
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<span class="mw-mmv-source-author" original-title="Author and source information" style="background-color: white;"><span class="mw-mmv-author"><a href="http://commons.wikimedia.org/wiki/User:Azcolvin429" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="User:Azcolvin429">Andrew Z. Colvin</a></span> - <span class="mw-mmv-source"><span class="int-own-work">Own work</span></span></span></div>
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<b>A <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral_barrada" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia espiral barrada">galáxia espiral barrada</a> <a href="http://pt.wikipedia.org/wiki/NGC_7408" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 7408">NGC 7408</a></b> está localizada a três graus a noroeste de Delta Tucanae e foi confundida inicialmente com uma <a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa planetária">nebulosa planetária</a><span class="reference" id="cite_ref-striecher_2005_11-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Tucana#cite_note-striecher_2005-11" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">11</a></span> .</div>
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<a href="http://pt.wikipedia.org/wiki/Tucana">http://pt.wikipedia.org/wiki/Tucana</a></div>
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<b>NGC 7408</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral_barrada" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia espiral barrada">espiral barrada</a> (SBc) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Tucana" style="background: none; color: #0b0080; text-decoration: none;" title="Tucana">Tucana</a>. Possui uma declinação de -63° 41' 43" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 22<a href="http://pt.wikipedia.org/wiki/Hora" style="background: none; color: #0b0080; text-decoration: none;" title="Hora">horas</a>, 55 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto">minutos</a> e 56,7 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a>.</div>
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A galáxia <b>NGC 7408</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/1_de_Novembro" style="background: none; color: #0b0080; text-decoration: none;" title="1 de Novembro">1 de Novembro</a> de <a href="http://pt.wikipedia.org/wiki/1834" style="background: none; color: #0b0080; text-decoration: none;" title="1834">1834</a> por <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background: none; color: #0b0080; text-decoration: none;" title="John Herschel">John Herschel</a>.</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/NGC_7408</span></span></div>
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Parte da constelação foi alvo de um programa de observação de duas semanas do <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_espacial_Hubble" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio espacial Hubble">telescópio espacial Hubble</a> em <a href="http://pt.wikipedia.org/wiki/1998" style="background: none; color: #0b0080; text-decoration: none;" title="1998">1998</a> que resultou no <a href="http://pt.wikipedia.org/wiki/Campo_Profundo_Sul_do_Hubble" style="background: none; color: #0b0080; text-decoration: none;" title="Campo Profundo Sul do Hubble">Campo Profundo Sul do Hubble</a><span class="reference" id="cite_ref-aj120_4_1648_15-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Tucana#cite_note-aj120_4_1648-15" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">15</a></span> . A área que deveria ser coberta precisava estar nos polos da órbita do telescópio para permitir observação contínua e teve como resultado a descoberta de <b>um <a href="http://pt.wikipedia.org/wiki/Quasar" style="background: none; color: #0b0080; text-decoration: none;" title="Quasar">quasar</a> neste campo: QSO J2233-606</b><span class="reference" id="cite_ref-16" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Tucana#cite_note-16" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">16</a></span> .</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;"><a href="http://pt.wikipedia.org/wiki/Tucana">http://pt.wikipedia.org/wiki/Tucana</a></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">NGC 362 - Tucanae - Aglomerado Globular</b><span style="background-color: white;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 01h01m - Declinação -71<sup>o</sup>.57 - Magnitude fotográfica global 8,0 - Diâmetro aparente em minuto de arco 17’,7</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Tipo Espectral G5 Distância kpc 12,8<o:p></o:p></span><br />
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">NGC 362</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Tucana" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Tucana">constelação de Tucana</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/James_Dunlop" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="James Dunlop">James Dunlop</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> em 1826, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> refletor com abertura de 9 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> (+6,8), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> amadores ou com equipamentos superiores.</span><br />
<span style="background-color: white; line-height: 22.399999618530273px; text-align: start;"><span style="color: #252525; font-family: sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_362">http://pt.wikipedia.org/wiki/NGC_362</a></span></span><br />
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<a href="http://pt.wikipedia.org/wiki/NGC_362" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="NGC 362"><b>NGC 362</b></a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é um outro aglomerado globular em Tucana com magnitude aparente de 6,4 a 27.700 anos-luz da Terra. Como o vizinho 47 Tucanae, NGC 362 é um aglomerado Shapley classe III e está entre os mais brilhantes do céu. Sua órbita o leva para muito próximo do centro da </span><a href="http://pt.wikipedia.org/wiki/Via_L%C3%A1ctea" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Via Láctea">Via Láctea</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> a aproximadamente 3 mil anos-luz, o que não é usual. Foi descoberto por volta de 1820 por </span><a href="http://pt.wikipedia.org/wiki/James_Dunlop" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="James Dunlop">James Dunlop</a><span class="reference" id="cite_ref-FOOTNOTELevy2005165_10-0" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Tucana#cite_note-FOOTNOTELevy2005165-10" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">10</a></span><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> . Suas estrelas se tornam visíveis com uma magnificação de 180x no telescópio</span><span class="reference" id="cite_ref-striecher_2005_11-0" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Tucana#cite_note-striecher_2005-11" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">11</a></span><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> .</span><br />
<span style="background-color: white; line-height: 22.399999618530273px; text-align: start;"><span style="color: #252525; font-family: sans-serif;"><a href="http://pt.wikipedia.org/wiki/Tucana">http://pt.wikipedia.org/wiki/Tucana</a></span></span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgTlnfgfhxs1j_-MRryyq9pBWrFcd3-CMqyTOMMYb2Mb0wSH8MNRiEuyjaT8EEXM2lYwPnjoxYcDOkOL7Yai-TcnM-iL_x6j45GUs1F5NGLT4lApvm00HkTQXIbtedZcs-59TnHzykyoaU/s1600/GALEX_image_of_NGC_362.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgTlnfgfhxs1j_-MRryyq9pBWrFcd3-CMqyTOMMYb2Mb0wSH8MNRiEuyjaT8EEXM2lYwPnjoxYcDOkOL7Yai-TcnM-iL_x6j45GUs1F5NGLT4lApvm00HkTQXIbtedZcs-59TnHzykyoaU/s1600/GALEX_image_of_NGC_362.jpg" /></a></div>
<span style="background-color: white; font-size: 14px; line-height: 22.399999618530273px; text-align: start;"><span style="color: #252525; font-family: sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_362#mediaviewer/Ficheiro:GALEX_image_of_NGC_362.jpg">http://pt.wikipedia.org/wiki/NGC_362#mediaviewer/Ficheiro:GALEX_image_of_NGC_362.jpg</a></span></span><br />
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<span style="background-color: white;"><span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%; overflow: hidden; text-overflow: ellipsis;">GALEX image of NGC 362</span><a class="mw-mmv-license" href="http://commons.wikimedia.org/wiki/File:GALEX_image_of_NGC_362.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-size: 0.9em; padding: 0px 10px; text-align: right; text-decoration: none;" target="">Domínio público</a></span></div>
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<span style="background-color: white;"><span class="mw-mmv-author" original-title="Autor">NASA/JPL-Caltech/University of Virginia/R. Schiavon (Univ. of Virginia)</span> - <span class="mw-mmv-source" original-title="Fonte"><a class="external free" href="http://www.galex.caltech.edu/media/glx2007-03f_img01.html" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://www.galex.caltech.edu/media/glx2007-03f_img01.html</a></span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEivqKGexchoZt19gm_GNw7n7X-zOorCV04rcJ9nxH9IbTRRuso7Ddfz0OLS9qXjyLxG3p2lpIaLqc-Wunir4uxNDUKAjXi05y2NUuwye8rLGmd6zTz8iIO8laYofnjlHLq2QPFk-ldPX70/s1600/47+Tucanae.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEivqKGexchoZt19gm_GNw7n7X-zOorCV04rcJ9nxH9IbTRRuso7Ddfz0OLS9qXjyLxG3p2lpIaLqc-Wunir4uxNDUKAjXi05y2NUuwye8rLGmd6zTz8iIO8laYofnjlHLq2QPFk-ldPX70/s1600/47+Tucanae.jpg" /></a></div>
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Globular cluster 47 Tucanae and the Small Magellanic Cloud (ground-based image)</h1>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgIkocu6NJ2WRL8LDMxvBLZrJV5p2xQ7juDVVlnmWe_5knOvSYVOBxnES3AnBblMbO3xu20IKqNqjgSyCmXjTzwVA_uHSspPoaQ359sgUwZ6Z6FkZa0jbX8waZdROPZaL_CByRwhee6Hr4/s1600/heic0616e.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgIkocu6NJ2WRL8LDMxvBLZrJV5p2xQ7juDVVlnmWe_5knOvSYVOBxnES3AnBblMbO3xu20IKqNqjgSyCmXjTzwVA_uHSspPoaQ359sgUwZ6Z6FkZa0jbX8waZdROPZaL_CByRwhee6Hr4/s1600/heic0616e.jpg" /></a></div>
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<a href="http://www.spacetelescope.org/images/heic0616e/">http://www.spacetelescope.org/images/heic0616e/</a></div>
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This photo was taken by the Japanese astrophotographer Akira Fujii and shows a wide-angle view of the globular cluster 47 Tucanae and the Small Magellanic Cloud.</div>
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<strong style="border: 0px; margin: 0px 0px 15px; outline: 0px; padding: 0px; vertical-align: baseline;">Credit: </strong>Akira Fujii</div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 104 = 47 Tucanae - Aglomerado Globular</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">AR 00h23m Declinação - 72<sup>o</sup>.11 Magnitude média das 25 estrelas mais brilhantes 13,54 Magnitude fotográfica global 4,4 Diâmetro aparente em minuto de arco 44’,0</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Número conhecido de Variáveis 11 Distância kpc 5,0<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Imenso Aglomerado Globular na constelação de Tucano. É o segundo aglomerado em tamanho, depois de Omega Centauri. Visível a olho nú em noites escuras e transparentes, a cerca de 2<sup>o</sup>. a sudoeste de Theta Tucanae. Com um bom par de binóculos, observamos uma forte condensação central (onde as estrelas parecem estar amontoadas umas sobre as outras) e com um telescópio podemos vislumbrar um dos objetos mais belos do céu.</span></div>
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<span style="font-family: Arial, sans-serif;">- 6<sup>a</sup>. Edição do <b>Atlas Celeste</b></span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">de autoria de <b>Ronaldo Rogério de Freitas Mourão</b>,</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<a href="http://www.spacetelescope.org/images/heic0616c/">http://www.spacetelescope.org/images/heic0616c/</a></div>
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A photo of the globular star cluster 47 Tucanae taken with the Very Large Telescope, in Chile. It is one of the densest globular clusters in the Southern hemisphere. The cluster contains one million stars.</div>
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<strong style="border: 0px; margin: 0px 0px 15px; outline: 0px; padding: 0px; vertical-align: baseline;">Credit:</strong></div>
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Very Large Telescope/European Southern Observatory, R. Kotak and H. Boffin (ESO)</div>
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<b>47 Tucanae</b> (<b>NGC 104</b>) ou apenas <b>47 Tuc</b> é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> situado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Tucana" style="background: none; color: #0b0080; text-decoration: none;" title="Tucana">Tucana</a>. Está a de cerca de 16 700 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> de distância da <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>, e tem 120 anos-luz de diâmetro. Pode ser visto a <a href="http://pt.wikipedia.org/wiki/Olho_nu" style="background: none; color: #0b0080; text-decoration: none;" title="Olho nu">olho nu</a>, e é brilhante o suficiente para ganhar uma <a href="http://pt.wikipedia.org/wiki/Designa%C3%A7%C3%A3o_de_Flamsteed" style="background: none; color: #0b0080; text-decoration: none;" title="Designação de Flamsteed">designação de Flamsteed</a> com uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Magnitude_visual" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude visual">magnitude visual</a> de 4,0. É apenas uma de um pequeno número de características com essa designação do céu do sul.</div>
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47 Tucanae foi descoberto por <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background: none; color: #0b0080; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a> em <a href="http://pt.wikipedia.org/wiki/1751" style="background: none; color: #0b0080; text-decoration: none;" title="1751">1751</a>; a sua localização muito ao sul tem escondido de observadores europeus até então. O aglomerado aparece aproximadamente com o tamanho da <a href="http://pt.wikipedia.org/wiki/Lua" style="background: none; color: #0b0080; text-decoration: none;" title="Lua">lua</a> cheia no céu em condições ideais.</div>
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É o segundo aglomerado globular mais brilhante no céu (depois de <a href="http://pt.wikipedia.org/wiki/Omega_Centauri" style="background: none; color: #0b0080; text-decoration: none;" title="Omega Centauri">Omega Centauri</a>), e é conhecido por ter um núcleo muito brilhante e denso. Ele tem de 22 pulsares milisegundos conhecidos, e pelo menos 21 estrelas retardatárias azuis (blue stragglers) perto do centro.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/47_Tucanae#cite_note-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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47 Tucanae está incluído no Catálogo Caldwell de Sir Patrick Moore como C106.</div>
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NGC 104 concorre com <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/NGC_5139" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 5139">NGC 5139</a> (Omega Centauri) para o título: O mais esplêndido Aglomerado Globular no céu. NGC 104 tem duas características em seu favor. Ele é arredondado e tem um centro mais compacto. No entanto, devido à localização, mais observadores vão para NGC 5139.</div>
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/47_Tucanae">http://pt.wikipedia.org/wiki/47_Tucanae</a></span></span><br />
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spacetelescope.org/news/heic0616/</span></span><br />
<span style="background-color: white; color: #515151; font-family: Arial, Helvetica, san-serif; font-size: 12px; line-height: 15px; text-align: start;">Image credit: NASA, ESA, and G. Meylan (?cole Polytechnique Federale de Lausanne)</span><br />
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A seven year study with the NASA/ESA Hubble Space Telescope has provided astronomers with the best observational evidence yet that globular clusters sort out stars according to their mass, governed by a gravitational billiard ball game between stars. Heavier stars slow down and sink to the cluster's core, while lighter stars pick up speed and move across the cluster to its periphery. This process, called "mass segregation", has long been suspected for globular star clusters, but has never before been directly seen in action.</div>
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LEIA MAIS em</div>
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<span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">O segundo </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> mais brilhante do céu depois de </span><a href="http://pt.wikipedia.org/wiki/Omega_Centauri" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Omega Centauri">Omega Centauri</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é </span><a href="http://pt.wikipedia.org/wiki/47_Tucanae" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="47 Tucanae"><b>47 Tucanae</b></a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"><b> (NGC 104)</b> que está um pouco a oeste da </span><a href="http://pt.wikipedia.org/wiki/Pequena_Nuvem_de_Magalh%C3%A3es" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Pequena Nuvem de Magalhães">Pequena Nuvem de Magalhães</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. Dista apenas 14.700 </span><a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Ano-luz">anos-luz</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> da Terra com idade aproximada de 12 bilhões de anos</span><span class="reference" id="cite_ref-o.27meara_7-0" style="bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Tucana#cite_note-o.27meara-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> . É predominantemente composto de estrelhas amarelas apesar de possuir um contingente de </span><a href="http://pt.wikipedia.org/wiki/Estrela_retardat%C3%A1ria_azul" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Estrela retardatária azul">estrelas retardatárias azuis</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">, estrelas quentes que hipoteticamente se formaram da união de </span><a href="http://pt.wikipedia.org/wiki/Estrela_bin%C3%A1ria" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Estrela binária">estrelas binárias</a><span class="reference" id="cite_ref-objects_8-0" style="bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Tucana#cite_note-objects-8" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">8</a></span><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> . 47 Tucanae tem uma magnitude aparente de 3,9, o que significa que é visível a </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Olho_n%C3%BA&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Olho nú (página não existe)">olho nú</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. É um aglomerado Shapley classe III, o que significa que tem um núcleo bem definido. Os aglomerados próximos são o pequeno </span><a href="http://pt.wikipedia.org/wiki/NGC_121" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="NGC 121">NGC 121</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">, 10 arcominutos distante da borda do grande aglomerado</span><span class="reference" id="cite_ref-FOOTNOTELevy2005163.E2.80.93164_9-0" style="bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Tucana#cite_note-FOOTNOTELevy2005163.E2.80.93164-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> .</span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://en.wikipedia.org/wiki/Magellanic_Clouds#mediaviewer/File:Magellanic_Clouds_%E2%80%95_Irregular_Dwarf_Galaxies.jpg</span></span><br />
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<span class="mw-mmv-title" original-title="File name" style="background-color: white; font-size: 1.2em; max-width: 60%; overflow: hidden; text-overflow: ellipsis;">Magellanic Clouds ― Irregular Dwarf Galaxies</span></div>
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<span style="background-color: white;"><span class="mw-mmv-author" original-title="Author">ESO/<a class="extiw" href="http://en.wikipedia.org/wiki/Serge_Brunier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:Serge Brunier">S. Brunier</a></span> - <span class="mw-mmv-source" original-title="Source"><a class="external text" href="http://www.eso.org/gallery/v/ESOPIA/Galaxies/B01.tif.html" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">ESO</a></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">As Nuvens de Magalhães</span></b><span style="color: #073763;"><o:p></o:p></span></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Existem duas pequenas nuvens esfumaçadas que pareciam ser fragmentos da Via Láctea e que formam um quase triangulo com o pólo sul celestial. Estas nuvens foram primeiramente descritas pelo navegante português Fernando de Magalhães, no começo do século dezesseis. Porém, somente nos anos de 1920, os astrônomos determinaram que as Nuvens de Magalhães são galáxias, irregulares, pequena e próximas.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As Nuvens de Magalhães são ligadas entre si e à nossa Galáxia não somente pela força de gravidade mas também pela ponte gigantesca de hidrogênio neutro e frio. O brilho azulado das Nuvens de Magalhães revelam a presença de um imenso número de estrelas jovens, quentes e gigantes muito luminosas.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Se pudéssemos olhar para nossa Galáxia de um ponto externo à mesma, veríamos três pequenos e próximos satélites (galáxias-satélites), as Nuvens de Magalhães. Um sistema similar acontece com a Galáxia de ndrômeda, onde podemos observar várias pequenas galáxias satélites.<o:p></o:p></span><br />
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<span style="font-family: Arial, sans-serif;">- 6<sup>a</sup>. Edição do <b>Atlas Celeste</b></span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">de autoria de <b>Ronaldo Rogério de Freitas Mourão</b>,</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b>The Magellanic Clouds</b> have been known since the first millennium in <a href="http://en.wikipedia.org/wiki/Western_Asia" style="background: none; color: #0b0080; text-decoration: none;" title="Western Asia">Western Asia</a>. The first preserved mention of the <a href="http://en.wikipedia.org/wiki/Large_Magellanic_Cloud" style="background: none; color: #0b0080; text-decoration: none;" title="Large Magellanic Cloud">Large Magellanic Cloud</a> is by the <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Persia" style="background: none; color: #0b0080; text-decoration: none;" title="Persia">Persian</a> astronomer <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Al_Sufi" style="background: none; color: #0b0080; text-decoration: none;" title="Al Sufi">Al Sufi</a>.<sup class="reference" id="cite_ref-4" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Magellanic_Clouds#cite_note-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[4]</a></sup><sup class="reference" id="cite_ref-5" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Magellanic_Clouds#cite_note-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[5]</a></sup> In 964, in his <i><a href="http://en.wikipedia.org/wiki/Book_of_Fixed_Stars" style="background: none; color: #0b0080; text-decoration: none;" title="Book of Fixed Stars">Book of Fixed Stars</a></i>, he called it <i>al-Bakr</i> ("the Sheep") "of the southern Arabs"; he noted that the Cloud is not visible from northern <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Arabia" style="background: none; color: #0b0080; text-decoration: none;" title="Arabia">Arabia</a> and <a href="http://en.wikipedia.org/wiki/Baghdad" style="background: none; color: #0b0080; text-decoration: none;" title="Baghdad">Baghdad</a>, but can be seen at the strait of <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Bab_el_Mandeb" style="background: none; color: #0b0080; text-decoration: none;" title="Bab el Mandeb">Bab el Mandeb</a> (12°15' N), which is the southernmost point of Arabia.<sup class="reference" id="cite_ref-allen_2-1" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Magellanic_Clouds#cite_note-allen-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup></div>
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In <a href="http://en.wikipedia.org/wiki/Europe" style="background: none; color: #0b0080; text-decoration: none;" title="Europe">Europe</a>, the Clouds were first observed by Italian explorers <a href="http://en.wikipedia.org/wiki/Peter_Martyr_d%27Anghiera" style="background: none; color: #0b0080; text-decoration: none;" title="Peter Martyr d'Anghiera">Peter Martyr d'Anghiera</a> and <a href="http://en.wikipedia.org/wiki/Andrea_Corsali" style="background: none; color: #0b0080; text-decoration: none;" title="Andrea Corsali">Andrea Corsali</a> at the end of the 15th century. Subsequently, they were reported by<a href="http://en.wikipedia.org/wiki/Antonio_Pigafetta" style="background: none; color: #0b0080; text-decoration: none;" title="Antonio Pigafetta">Antonio Pigafetta</a>, who accompanied the expedition of <a href="http://en.wikipedia.org/wiki/Ferdinand_Magellan" style="background: none; color: #0b0080; text-decoration: none;" title="Ferdinand Magellan">Ferdinand Magellan</a> on its circumnavigation of the world in 1519-1522.<sup class="reference" id="cite_ref-allen_2-2" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Magellanic_Clouds#cite_note-allen-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup> However, naming the clouds after Magellan did not become widespread until much later. In Bayer's <i><a href="http://en.wikipedia.org/wiki/Uranometria" style="background: none; color: #0b0080; text-decoration: none;" title="Uranometria">Uranometria</a></i> they are designated as <i>nubecula major</i> and <i>nubecula minor</i>.<sup class="reference" id="cite_ref-6" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Magellanic_Clouds#cite_note-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[6]</a></sup> In the 1756 star map of the French astronomer <a href="http://en.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background: none; color: #0b0080; text-decoration: none;" title="Nicolas Louis de Lacaille">Lacaille</a>, they are designated as <i>le Grand Nuage</i> and <i>le Petit Nuage</i> ("the Large Cloud" and "the Small Cloud").<sup class="reference" id="cite_ref-7" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Magellanic_Clouds#cite_note-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[7]</a></sup></div>
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In <a href="http://en.wikipedia.org/wiki/Sri_Lanka" style="background: none; color: #0b0080; text-decoration: none;" title="Sri Lanka">Sri Lanka</a>, from ancient times, these clouds have been referred to as the 'Maha Mera Paruwathaya' meaning "the great mountain", as they look like the peaks of a distant mountain range.</div>
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In the southern hemisphere,<b> the Magellanic clouds</b> have long been included in the lore of native inhabitants, including <a href="http://en.wikipedia.org/wiki/Pacific_Ocean" style="background: none; color: #0b0080; text-decoration: none;" title="Pacific Ocean">south sea</a> islanders and <a href="http://en.wikipedia.org/wiki/Indigenous_Australians" style="background: none; color: #0b0080; text-decoration: none;" title="Indigenous Australians">indigenous Australians</a>. <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Persia" style="background: none; color: #0b0080; text-decoration: none;" title="Persia">Persian</a> astronomer <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Abd_Al-Rahman_Al_Sufi" style="background: none; color: #0b0080; text-decoration: none;" title="Abd Al-Rahman Al Sufi">Al Sufi</a> labelled the larger of the two clouds as Al Bakr, the White Ox. <a href="http://en.wikipedia.org/wiki/Europe" style="background: none; color: #0b0080; text-decoration: none;" title="Europe">European</a> sailors may have first noticed the clouds during the <a href="http://en.wikipedia.org/wiki/Middle_Ages" style="background: none; color: #0b0080; text-decoration: none;" title="Middle Ages">Middle Ages</a> when they were used for navigation.<a href="http://en.wikipedia.org/wiki/Kingdom_of_Portugal" style="background: none; color: #0b0080; text-decoration: none;" title="Kingdom of Portugal">Portuguese</a> and <a href="http://en.wikipedia.org/wiki/Dutch_Republic" style="background: none; color: #0b0080; text-decoration: none;" title="Dutch Republic">Dutch</a> sailors called them the Cape Clouds, a name that was retained for several centuries. During the circumnavigation of the Earth by <a href="http://en.wikipedia.org/wiki/Ferdinand_Magellan" style="background: none; color: #0b0080; text-decoration: none;" title="Ferdinand Magellan">Ferdinand Magellan</a> in 1519–22, they were described by <a href="http://en.wikipedia.org/wiki/Antonio_Pigafetta" style="background: none; color: #0b0080; text-decoration: none;" title="Antonio Pigafetta">Antonio Pigafetta</a> as dim clusters of stars.<sup class="reference" id="cite_ref-8" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Small_Magellanic_Cloud#cite_note-8" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[8]</a></sup> In <a href="http://en.wikipedia.org/wiki/Johann_Bayer" style="background: none; color: #0b0080; text-decoration: none;" title="Johann Bayer">Johann Bayer</a>'s celestial atlas <a href="http://en.wikipedia.org/wiki/Uranometria" style="background: none; color: #0b0080; text-decoration: none;" title="Uranometria">Uranometria</a>, published in 1603, he named the smaller cloud, Nubecula Minor.<sup class="reference" id="cite_ref-9" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Small_Magellanic_Cloud#cite_note-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[9]</a></sup>In <a href="http://en.wikipedia.org/wiki/Latin" style="background: none; color: #0b0080; text-decoration: none;" title="Latin">Latin</a>, Nubecula means a little cloud.<sup class="reference" id="cite_ref-10" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Small_Magellanic_Cloud#cite_note-10" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[10]</a></sup></div>
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Between 1834 and 1838, <a class="mw-redirect" href="http://en.wikipedia.org/wiki/John_Frederick_William_Herschel" style="background: none; color: #0b0080; text-decoration: none;" title="John Frederick William Herschel">John Frederick William Herschel</a> made observations of the southern skies with his 14-inch (36 cm) reflector from the <a class="new" href="http://en.wikipedia.org/w/index.php?title=Royal_Observatory_(Cape_of_Good_Hope)&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Royal Observatory (Cape of Good Hope) (page does not exist)">Royal Observatory</a> at the <a href="http://en.wikipedia.org/wiki/Cape_of_Good_Hope" style="background: none; color: #0b0080; text-decoration: none;" title="Cape of Good Hope">Cape of Good Hope</a>. While observing the Nubecula Minor, he described it as a cloudy mass of light with an oval shape and a bright center. Within the area of this cloud he catalogued a concentration of 37 nebulae and clusters.<sup class="reference" id="cite_ref-11" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Small_Magellanic_Cloud#cite_note-11" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[11]</a></sup></div>
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In 1891, <a href="http://en.wikipedia.org/wiki/Harvard_College_Observatory" style="background: none; color: #0b0080; text-decoration: none;" title="Harvard College Observatory">Harvard College Observatory</a> opened an observing station at <a href="http://en.wikipedia.org/wiki/Arequipa_Region" style="background: none; color: #0b0080; text-decoration: none;" title="Arequipa Region">Arequipa</a> in <a href="http://en.wikipedia.org/wiki/Peru" style="background: none; color: #0b0080; text-decoration: none;" title="Peru">Peru</a>. Between 1893 and 1906, under the direction of <a href="http://en.wikipedia.org/wiki/Solon_Irving_Bailey" style="background: none; color: #0b0080; text-decoration: none;" title="Solon Irving Bailey">Solon Bailey</a>, the 24-inch (610 mm) telescope at this site was used to survey photographically both the Large and Small Magellanic Clouds.<sup class="reference" id="cite_ref-12" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Small_Magellanic_Cloud#cite_note-12" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[12]</a></sup> <a href="http://en.wikipedia.org/wiki/Henrietta_Swan_Leavitt" style="background: none; color: #0b0080; text-decoration: none;" title="Henrietta Swan Leavitt">Henrietta Swan Leavitt</a>, an astronomer at the <a href="http://en.wikipedia.org/wiki/Harvard_College_Observatory" style="background: none; color: #0b0080; text-decoration: none;" title="Harvard College Observatory">Harvard College Observatory</a>, used the plates from Arequipa to study the variations in relative luminosity of stars in the SMC. In 1908, the results of her study were published, which showed that a type of <a href="http://en.wikipedia.org/wiki/Variable_star" style="background: none; color: #0b0080; text-decoration: none;" title="Variable star">variable star</a> called a "cluster variable", later called a <a href="http://en.wikipedia.org/wiki/Cepheid_variable" style="background: none; color: #0b0080; text-decoration: none;" title="Cepheid variable">Cepheid variable</a> after the prototype star <a href="http://en.wikipedia.org/wiki/Delta_Cephei" style="background: none; color: #0b0080; text-decoration: none;" title="Delta Cephei">Delta Cephei</a>, showed a definite relationship between the variability period and the star's luminosity.<sup class="reference" id="cite_ref-13" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Small_Magellanic_Cloud#cite_note-13" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[13]</a></sup> This important period-luminosity relation allowed the distance to any other cepheid variable to be estimated in terms of the distance to the SMC. Hence, once the distance to the SMC was known with greater accuracy, Cepheid variables could be used as a <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Standard_candle" style="background: none; color: #0b0080; text-decoration: none;" title="Standard candle">standard candle</a> for measuring the distances to other galaxies.<sup class="reference" id="cite_ref-14" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Small_Magellanic_Cloud#cite_note-14" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[14]</a></sup></div>
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Using this period-luminosity relation, in 1913 the distance to the SMC was first estimated by <a href="http://en.wikipedia.org/wiki/Ejnar_Hertzsprung" style="background: none; color: #0b0080; text-decoration: none;" title="Ejnar Hertzsprung">Ejnar Hertzsprung</a>. First he measured thirteen nearby cepheid variables to find the <a href="http://en.wikipedia.org/wiki/Absolute_magnitude" style="background: none; color: #0b0080; text-decoration: none;" title="Absolute magnitude">absolute magnitude</a> of a variable with a period of one day. By comparing this to the periodicity of the variables as measured by Leavitt, he was able to estimate a distance of 10,000 parsecs (30,000 light years) between the Sun and the SMC.<sup class="reference" id="cite_ref-15" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Small_Magellanic_Cloud#cite_note-15" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[15]</a></sup> This later proved to be a gross underestimate of the true distance, but it did demonstrate the potential usefulness of this technique.<sup class="reference" id="cite_ref-16" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Small_Magellanic_Cloud#cite_note-16" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[16]</a></sup></div>
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Announced in 2006, measurements with the Hubble Space Telescope suggest the Large and Small Magellanic Clouds may be moving too fast to be orbiting the <a href="http://en.wikipedia.org/wiki/Milky_Way" style="background: none; color: #0b0080; text-decoration: none;" title="Milky Way">Milky Way</a>.<sup class="reference" id="cite_ref-17" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Small_Magellanic_Cloud#cite_note-17" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[17</a></sup></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhsmEqZefv6SI2bF1yx3CSt8aO3yDkQFCxpn1cMKHEB2CoEWi4PzXnoue0bd9zY51U27KT3hOhrPCfX4Tbu6XTxg3MumNG96jEf1zxv0xKoO5wG5_Zsr8EN943VFf_4yHifVLpr2BJ8f9g/s1600/Satellite_Galaxies.JPG" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhsmEqZefv6SI2bF1yx3CSt8aO3yDkQFCxpn1cMKHEB2CoEWi4PzXnoue0bd9zY51U27KT3hOhrPCfX4Tbu6XTxg3MumNG96jEf1zxv0xKoO5wG5_Zsr8EN943VFf_4yHifVLpr2BJ8f9g/s1600/Satellite_Galaxies.JPG" /></a></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;"><span style="font-size: 15px;">http://en.wikipedia.org/wiki/Large_Magellanic_Cloud#mediaviewer/File:Satellite_Galaxies.JPG</span></span></div>
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<tr><th colspan="2" style="vertical-align: middle;"><span style="background-color: white;"><span style="color: #073763;">Large Magellanic Cloud</span></span></th></tr>
<tr><td style="vertical-align: middle;"><span style="background-color: white;"><span style="color: #073763;"><img alt="The Large Magellanic Cloud" src="http://www.atlasoftheuniverse.com/localgrp/s_lmc.jpg" height="80" width="100" /></span></span></td><td style="vertical-align: middle;"><span style="background-color: white;"><span style="color: #073763;">The largest of the satellite galaxies and also the fourth largest galaxy in the Local Group. This galaxy is a large bright object in southern hemisphere skies and it is the brightest galaxy in the sky. It contains several billion stars and many stars are still forming in it, most notably in the Tarantula nebula, a huge concentration of gas and dust over 2000 light years in diameter. A supernova exploded in the Large Magellanic Cloud in 1987 and observations of the expanding supernova remnant provided accurate distance measurements to the galaxy.</span></span></td></tr>
<tr><th colspan="2" style="vertical-align: middle;"><span style="background-color: white;"><span style="color: #073763;">Small Magellanic Cloud</span></span></th></tr>
<tr><td style="vertical-align: middle;"><span style="background-color: white;"><span style="color: #073763;"><img alt="The Small Magellanic Cloud" src="http://www.atlasoftheuniverse.com/localgrp/s_smc.jpg" height="80" width="100" /></span></span></td><td style="vertical-align: middle;"><span style="background-color: white;"><span style="color: #073763;">Despite its name, this galaxy is fairly large for a dwarf galaxy. It contains at least several hundred million stars and is easily visible with the naked eye from the southern hemisphere. Like the Large Magellanic Cloud, there is still a lot star formation taking place within it.</span></span></td></tr>
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<span class="mw-mmv-title" original-title="File name" style="background-color: white; font-size: 1.2em; max-width: 60%; overflow: hidden; text-overflow: ellipsis;"><span style="color: #073763;">Satellite Galaxies</span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span class="mw-mmv-author" original-title="Author">Richard Powell</span> - <span class="mw-mmv-source" original-title="Source"><a class="external free" href="http://www.atlasoftheuniverse.com/" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;">http://www.atlasoftheuniverse.com</a></span></span></span></div>
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<span class="mw-mmv-title" original-title="File name" style="background-color: white; font-size: 1.2em; max-width: 60%; overflow: hidden; text-overflow: ellipsis;">Panoramic Large and Small Magellanic Clouds</span></div>
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<span style="background-color: white;"><span class="mw-mmv-author" original-title="Author">ESO/Y. Beletsky</span> - <span class="mw-mmv-source" original-title="Source"><a class="external free" href="http://www.eso.org/public/images/potw1114a/" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080;">http://www.eso.org/public/images/potw1114a/</a></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Galáxia Tucano - Pequena Nuvem de Magalhães</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 00h52m Declinação -72<sup>o</sup>.56<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Magnitude fotográfica aparente 2,86<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dimensões Angulares 216 X 216 Distância (milhões de anos-luz) 0,2<o:p></o:p></span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>A Pequena Nuvem de Magalhães</b><o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta é uma galáxia irregular e próxima e que, juntamente com a Grande Nuvem de Magalhães, órbita nossa Galáxia como se ambas fossem nossos satélites. <o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A maior parte da massa da Pequena Nuvem de Magalhães consiste de nuvens interestelares de hidrogênio, o material básico de formação das estrelas - que nesta galáxia acontecem em larga escala. Prova disso é o grande numero de estrelas jovens e quentes - gigantes azuis - que trazem à Nuvem esta sua coloração azulada.<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Em 1984, radio-astronomos australianos descobriram que a Pequena Nuvem de Magalhães consiste, na verdade, de duas galáxias separadas, uma atrás da outra, uma sendo ocultada de forma que vemos apenas um único objeto no céu. Estas duas galáxias estão se separando uma da outra e foi exatamente a diferença de velocidade entre ambas que revelou o fato de a Pequena Nuvem ser, na verdade, duas galáxias separadas.<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">- 6<sup>a</sup>. Edição do <b>Atlas Celeste</b></span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">de autoria de <b>Ronaldo Rogério de Freitas Mourão</b>,</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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Localizada ao sul de Tucana, a <a href="http://pt.wikipedia.org/wiki/Pequena_Nuvem_de_Magalh%C3%A3es" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pequena Nuvem de Magalhães">Pequena Nuvem de Magalhães</a> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_an%C3%A3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia anã">galáxia anã</a> que é uma das vizinhas mais próximas da <a href="http://pt.wikipedia.org/wiki/Via_L%C3%A1ctea" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Via Láctea">Via Láctea</a> a uma distância de 210 mil anos-luz. Embora provavelmente tenha tido o formato de disco, as <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/For%C3%A7as_de_mar%C3%A9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080;" title="Forças de maré">forças de maré</a> da Via Láctea a distorceram. Juntamente com a <a href="http://pt.wikipedia.org/wiki/Grande_Nuvem_de_Magalh%C3%A3es" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Grande Nuvem de Magalhães">Grande Nuvem de Magalhães</a>, ela está na<a class="new" href="http://pt.wikipedia.org/w/index.php?title=Corrente_de_Magalh%C3%A3es&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Corrente de Magalhães (página não existe)">corrente de Magalhães</a>, uma nuvem de gás que conecta as duas galáxias<span class="reference" id="cite_ref-objects_8-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Tucana#cite_note-objects-8" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">8</a></span> . <a href="http://pt.wikipedia.org/wiki/NGC_346" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 346">NGC 346</a> é uma região de formação de estrelas na Pequena Nuvem de Magalhães. Ela tem magnitude aparente de 10,3<span class="reference" id="cite_ref-striecher_2005_11-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Tucana#cite_note-striecher_2005-11" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">11</a></span> . Dentro dela está o sistema estelar triplo <a class="new" href="http://pt.wikipedia.org/w/index.php?title=HD_5980&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="HD 5980 (página não existe)">HD 5980</a>, sendo cada um de seus membros as estrelas mais luminosas conhecidas<span class="reference" id="cite_ref-triple_12-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Tucana#cite_note-triple-12" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">12</a></span> .</div>
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<span style="font-size: small;">Hubble finds source of Magellanic Stream</span></h1>
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<span style="font-size: small;">Astronomers explore origin of gas ribbon wrapped around our galaxy</span></h3>
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<span style="background-color: white; color: #515151; font-family: Arial, Helvetica, san-serif; line-height: 15px; text-align: start;">Image credit: David L. Nidever, et al., NRAO/AUI/NSF and Mellinger, LAB Survey, Parkes Observatory, Westerbork Observatory, and Arecibo Observatory.</span></div>
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Astronomers using the NASA/ESA Hubble Space Telescope have solved the 40-year-old mystery of the origin of the Magellanic Stream, a long ribbon of gas stretching nearly halfway around the Milky Way. New Hubble observations reveal that most of this stream was stripped from the Small Magellanic Cloud some two billion years ago, with a smaller portion originating more recently from its larger neighbour.</div>
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The Magellanic Clouds, two dwarf galaxies orbiting our galaxy, are at the head of a huge gaseous filament known as the Magellanic Stream. Since the Stream's discovery in the early 1970s, astronomers have wondered whether this gas comes from one or both of the satellite galaxies. Now, new Hubble observations show that most of the gas was stripped from the Small Magellanic Cloud about two billion years ago — but surprisingly, a second region of the stream was formed more recently from the Large Magellanic Cloud.</div>
<span style="font-family: Arial, Helvetica, sans-serif;">LEIA MAIS EM</span><br />
<span style="text-align: center;"><span style="font-family: Arial, Helvetica, sans-serif;">http://www.spacetelescope.org/news/heic1314/</span></span><br />
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">AGLOMERADOS LOCALIZADOS</span></b></div>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">NA PEQUENA NUVEM DE MAGALHÃES</span></b><br />
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<b style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"><span style="font-size: large;">NGC 121</span></b><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Tucana" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Tucana">constelação de Tucana</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="John Herschel">John Herschel</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> em 1835, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Telescópio">telescópio</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> refletor com abertura de 18,6 polegadas.</span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;"><a href="http://pt.wikipedia.org/wiki/NGC_121">http://pt.wikipedia.org/wiki/NGC_121</a></span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhxCljm_z0pZM65z2FHTJ_Pb4RCOD8IlTw_m14EtBifdxMMsYpSC9W9sOyL4TpsE2l1GYfI2oIJZeZQuyPgevb0bPWi0xxgqAvrvYmBef1a9If1YnXH9ft4Wy89aB9AEERgCQ4aTHUq_mbL/s1600/800px-NGC_121_Hubble_WikiSky.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhxCljm_z0pZM65z2FHTJ_Pb4RCOD8IlTw_m14EtBifdxMMsYpSC9W9sOyL4TpsE2l1GYfI2oIJZeZQuyPgevb0bPWi0xxgqAvrvYmBef1a9If1YnXH9ft4Wy89aB9AEERgCQ4aTHUq_mbL/s1600/800px-NGC_121_Hubble_WikiSky.jpg" /></a></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="background-color: white; font-size: 14px; line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/NGC_121#mediaviewer/Ficheiro:NGC_121_Hubble_WikiSky.jpg</span></span></div>
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<span style="background-color: white;"><span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%; overflow: hidden; text-overflow: ellipsis;">NGC 121 Hubble WikiSky</span><a class="mw-mmv-license" href="http://commons.wikimedia.org/wiki/File:NGC_121_Hubble_WikiSky.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-size: 0.9em; padding: 0px 10px; text-align: right; text-decoration: none;" target="">Domínio público</a></span></div>
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<span style="background-color: white;"><span class="mw-mmv-author" original-title="Autor"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:NASA">en:NASA</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/STScI" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:STScI">en:STScI</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span> - <span class="mw-mmv-source" original-title="Fonte"><a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a>'s snapshot tool - <a class="external autonumber" href="http://wikisky.org/snapshot?img_size=&img_res=&ra=0.4454782953531459&de=-71.53526077222936&angle=0.05188157166574433&projection=tan&rotation=21.255246469946197&survey=astrophoto&img_id=60563&width=4000&height=4000&img_borders=0&interpolation=bicubic&jpeg_quality=0.8" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">[1]</a></span></span></div>
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<strong style="border: 0px; margin: 0px 0px 15px; outline: 0px; padding: 0px; vertical-align: baseline;">Credit:</strong></div>
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<a href="http://www.spacetelescope.org/" style="border: 0px; color: #1596c1; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">ESA/Hubble</a> & <a href="http://www.nasa.gov/" style="border: 0px; color: #1596c1; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">NASA</a><br />
Acknowlegement: Stefano Campani</div>
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This image shows NGC 121, a <a href="http://en.wikipedia.org/wiki/Globular_cluster" style="border: 0px; color: #1596c1; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">globular cluster</a> in the constellation of Tucana (The Toucan). Globular clusters are big balls of old stars that orbit the centres of their galaxies like satellites — the Milky Way, for example, has around 150.</div>
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NGC 121 belongs to one of our neighbouring galaxies, the Small Magellanic Cloud (SMC). It was discovered in 1835 by English astronomer John Herschel, and in recent years it has been studied in detail by astronomers wishing to learn more about how stars form and evolve.</div>
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Stars do not live forever — they develop differently depending on their original mass. In many clusters, all the stars seem to have formed at the same time, although in others we see distinct populations of stars that are different ages. By studying old stellar populations in globular clusters, astronomers can effectively use them as tracers for the stellar population of their host galaxies. With an object like NGC 121, which lies close to the Milky Way, Hubble is able to resolve individual stars and get a very detailed insight.</div>
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LEIA MAIS EM</div>
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<span style="color: #515151; font-family: Arial, Helvetica, san-serif;"><span style="line-height: 15px;"><a href="http://www.spacetelescope.org/images/potw1428a/">http://www.spacetelescope.org/images/potw1428a/</a></span></span></div>
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<b><span style="font-size: large;">NGC 602</span></b> is a young, bright <a href="http://en.wikipedia.org/wiki/Open_cluster" style="background: none; color: #0b0080; text-decoration: none;" title="Open cluster">open cluster</a> of <a href="http://en.wikipedia.org/wiki/Star" style="background: none; color: #0b0080; text-decoration: none;" title="Star">stars</a> located in the <a href="http://en.wikipedia.org/wiki/Small_Magellanic_Cloud" style="background: none; color: #0b0080; text-decoration: none;" title="Small Magellanic Cloud">Small Magellanic Cloud</a> (SMC), a <a href="http://en.wikipedia.org/wiki/Satellite_galaxy" style="background: none; color: #0b0080; text-decoration: none;" title="Satellite galaxy">satellite galaxy</a> to the <a href="http://en.wikipedia.org/wiki/Milky_Way" style="background: none; color: #0b0080; text-decoration: none;" title="Milky Way">Milky Way</a>. <a href="http://en.wikipedia.org/wiki/Radiation" style="background: none; color: #0b0080; text-decoration: none;" title="Radiation">Radiation</a> and <a href="http://en.wikipedia.org/wiki/Shock_wave" style="background: none; color: #0b0080; text-decoration: none;" title="Shock wave">shock waves</a> from the stars have pushed away much of the lighter surrounding <a href="http://en.wikipedia.org/wiki/Interstellar_medium" style="background: none; color: #0b0080; text-decoration: none;" title="Interstellar medium">gas and dust</a> that compose the <a href="http://en.wikipedia.org/wiki/Nebula" style="background: none; color: #0b0080; text-decoration: none;" title="Nebula">nebula</a> known as N90, and this in turn has triggered new <a href="http://en.wikipedia.org/wiki/Star_formation" style="background: none; color: #0b0080; text-decoration: none;" title="Star formation">star formation</a>in the ridges (or "<a href="http://en.wikipedia.org/wiki/Elephant_trunks" style="background: none; color: #0b0080; text-decoration: none;" title="Elephant trunks">elephant trunks</a>") of the nebula. These even younger, pre-<a href="http://en.wikipedia.org/wiki/Main_sequence" style="background: none; color: #0b0080; text-decoration: none;" title="Main sequence">main sequence</a> stars are still enshrouded in dust but are visible to the <a href="http://en.wikipedia.org/wiki/Spitzer_Space_Telescope" style="background: none; color: #0b0080; text-decoration: none;" title="Spitzer Space Telescope">Spitzer Space Telescope</a> at <a href="http://en.wikipedia.org/wiki/Infrared" style="background: none; color: #0b0080; text-decoration: none;" title="Infrared">infrared</a> wavelengths.<sup class="reference" id="cite_ref-5" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/NGC_602#cite_note-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[5]</a></sup> The cluster is of particular interest because it is located in the wing of the SMC leading to the <a href="http://en.wikipedia.org/wiki/Magellanic_Bridge" style="background: none; color: #0b0080; text-decoration: none;" title="Magellanic Bridge">Magellanic Bridge</a>. Hence, while its chemical properties should be similar to those of the rest of the <a href="http://en.wikipedia.org/wiki/Galaxy" style="background: none; color: #0b0080; text-decoration: none;" title="Galaxy">galaxy</a>, it is relatively isolated and so easier to study.<sup class="reference" id="cite_ref-6" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/NGC_602#cite_note-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[6]</a></sup></div>
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A number of other, more distant galaxies also appear in the background of the <a href="http://en.wikipedia.org/wiki/Hubble_Space_Telescope" style="background: none; color: #0b0080; text-decoration: none;" title="Hubble Space Telescope">Hubble</a> images of NGC 602, making for a "tantalizing"<sup class="reference" id="cite_ref-APOD_4-1" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/NGC_602#cite_note-APOD-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[4]</a></sup> and "grand"<sup class="reference" id="cite_ref-7" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/NGC_602#cite_note-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[7]</a></sup> view</div>
<a href="http://en.wikipedia.org/wiki/NGC_602">http://en.wikipedia.org/wiki/NGC_602</a><br />
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<span style="background-color: white;"><span style="color: #073763; font-size: small;">Image: Hubble Observes Infant Stars in Nearby Galaxy</span></span></h2>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjn_nBX9PyvdrQ76BJ2Fg6E7Z915xDa86kGfFImxfz44ZvP2mRKfnmlcKv4E7vcKftmWBjYr__vFNpdQMONMjnFTtXc4aSIxTz7HrxdTqz0SBqF6BagUjga5kQnB8g2niMvyJLI3ATOgII/s1600/hs-2007-04-a-web_print.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjn_nBX9PyvdrQ76BJ2Fg6E7Z915xDa86kGfFImxfz44ZvP2mRKfnmlcKv4E7vcKftmWBjYr__vFNpdQMONMjnFTtXc4aSIxTz7HrxdTqz0SBqF6BagUjga5kQnB8g2niMvyJLI3ATOgII/s1600/hs-2007-04-a-web_print.jpg" /></a></div>
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<a href="http://hubblesite.org/newscenter/archive/releases/2007/04/image/a/format/web_print/">http://hubblesite.org/newscenter/archive/releases/2007/04/image/a/format/web_print/</a></div>
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Zooming on NGC 602</h1>
<a href="http://www.spacetelescope.org/videos/heic0702a/">http://www.spacetelescope.org/videos/heic0702a/</a><br />
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<strong style="border: 0px; margin: 0px 0px 15px; outline: 0px; padding: 0px; vertical-align: baseline;">Credit:</strong></div>
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Akira Fujii, Digitized Sky Survey 2 and <a href="http://www.esa.int/" style="border: 0px; color: #1596c1; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">ESA</a>/<a href="http://www.spacetelescope.org/" style="border: 0px; color: #1596c1; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">Hubble</a></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgDa6uJILIWD-mzB4nqB0eRMBhdGakPoDiZh3m7h_6KVMOarLFaS7Q5BZsGd7TKiaZPC3JFvzuKF19hAYLcqbfopOM1tW1S84A4i7MUQiMZm8WW-Rwz-8gBT4qoyhzqAvB-xJD5kS-3KqA/s1600/NGC602_AAS209_lg.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgDa6uJILIWD-mzB4nqB0eRMBhdGakPoDiZh3m7h_6KVMOarLFaS7Q5BZsGd7TKiaZPC3JFvzuKF19hAYLcqbfopOM1tW1S84A4i7MUQiMZm8WW-Rwz-8gBT4qoyhzqAvB-xJD5kS-3KqA/s1600/NGC602_AAS209_lg.jpg" /></a></div>
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<a href="http://heritage.stsci.edu/2007/04/images/NGC602_AAS209_lg.jpg">http://heritage.stsci.edu/2007/04/images/NGC602_AAS209_lg.jpg</a></div>
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<span class="style8" style="font-family: Arial, Helvetica, sans-serif;"><b>NGC 602</b>: Ongoing Star Formation in a Young SMC Cluster</span></div>
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<span class="style7"><br /><span class="style2">Lynn Redding Carlson (JHU), Antonella Nota (STScI/ESA), Elena Sabbi (STScI), Marco Sirianni (STScI/ESA), Joseph L. Hora (Harvard/CfA), Margaret Meixner (STScI), M. Clampin (NASA/Goddard), J. Gallagher (U. Wisconsin), M. S. Oey (U. Michigan), A. Pasquali (Inst. Of Astron., ETH), L. J. Smith (UCL), M. Tosi (Bologna Obs.), R. Walterbos (U. New Mexico)<br /><br /><em>(The following is a poster presentation made at the American<br />Astronomical Society conference in January 2007 in Seattle, Washington.)</em></span></span></div>
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<span class="style7" style="font-family: Arial, Helvetica, sans-serif;"><br />The young stellar cluster NGC 602 is located in the wing of the SMC, Z~0.004, a low density region far from the main body of the galaxy with low gas and stellar content. From deep optical imaging with the Advanced Camera for Surveys (ACS) aboard the Hubble Space Telescope (HST), we have discovered the existence of an extensive pre-Main Sequence (PMS) population, with stellar masses in the range 0.6–3 Mo. This pre-Main Sequence population formed coevally with the central cluster about 5 Myr ago. Spitzer Space Telescope (SST) images of the region in all four Infrared Array Camera (IRAC) bands reveal a second population of Young Stellar Objects (YSOs), which formed after the stars seen with HST/ACS imaging. Some of these very young objects are still embedded in nebular material. We infer that star formation started in this region ~5 Myr ago with the formation of the central cluster and gradually propagated towards the outskirts where we find evidence of on going star formation (~1 Myr).</span></div>
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<a href="http://heritage.stsci.edu/2007/04/supplemental.html">http://heritage.stsci.edu/2007/04/supplemental.html</a><br />
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"><span style="font-size: large;">NGC 265</span></b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> is an </span><a href="http://en.wikipedia.org/wiki/Open_cluster" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Open cluster">open cluster</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> in the </span><a href="http://en.wikipedia.org/wiki/Small_Magellanic_Cloud" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Small Magellanic Cloud">Small Magellanic Cloud</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">,</span><sup class="reference" id="cite_ref-APOD_3-0" style="background-color: white; color: #252525; font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/NGC_265#cite_note-APOD-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[3]</a></sup><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> which is located in the </span><a href="http://en.wikipedia.org/wiki/Constellation" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Constellation">constellation</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Tucana_(constellation)" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;" title="Tucana (constellation)">Tucana</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">.</span><br />
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<a href="http://en.wikipedia.org/wiki/NGC_265">http://en.wikipedia.org/wiki/NGC_265</a><br />
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"><span style="font-size: large;">NGC 290</span></b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> is an </span><a href="http://en.wikipedia.org/wiki/Open_cluster" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Open cluster">open cluster</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. It lies some 200,000 </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Light_years" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Light years">light years</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> away in the </span><a href="http://en.wikipedia.org/wiki/Small_Magellanic_Cloud" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Small Magellanic Cloud">Small Magellanic Cloud</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">,</span><sup class="reference" id="cite_ref-APOD_2-0" style="background-color: white; color: #252525; font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/NGC_290#cite_note-APOD-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> which is located in the </span><a href="http://en.wikipedia.org/wiki/Constellation" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Constellation">constellation</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> </span><a href="http://en.wikipedia.org/wiki/Tucana" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Tucana">Tucana</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. It spans 65 light years across.</span><sup class="reference" id="cite_ref-3" style="background-color: white; color: #252525; font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/NGC_290#cite_note-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[3]</a></sup><br />
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<a href="http://en.wikipedia.org/wiki/NGC_290">http://en.wikipedia.org/wiki/NGC_290</a><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhY7X_tFFTXadh-jbIQkauKVSZwYbbBk2mucHsmtU6yyxq7OFnylfZiAmrJhkmWf4x3zWu6I5VEzUkU6aPTvp1EFY-mIL4zoIA5IIZsTQvWn2km6d1eLPTiYRmyINWTfwASsq7CNVNjzWk/s1600/heic0603a.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhY7X_tFFTXadh-jbIQkauKVSZwYbbBk2mucHsmtU6yyxq7OFnylfZiAmrJhkmWf4x3zWu6I5VEzUkU6aPTvp1EFY-mIL4zoIA5IIZsTQvWn2km6d1eLPTiYRmyINWTfwASsq7CNVNjzWk/s1600/heic0603a.jpg" /></a></div>
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<a href="http://www.spacetelescope.org/images/heic0603a/">http://www.spacetelescope.org/images/heic0603a/</a></div>
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Hubble has captured the most detailed images to date of the open star clusters<b> NGC 265 and NGC 290 in the Small Magellanic Cloud</b> - two sparkling sets of gemstones in the southern sky.</div>
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Two new composite images taken with the <a href="http://www.spacetelescope.org/about/general/instruments/acs.html" style="border: 0px; color: #1596c1; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">Advanced Camera for Surveys</a> onboard the <a href="http://www.nasa.gov/" style="border: 0px; color: #1596c1; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">NASA</a>/<a href="http://www.esa.int/" style="border: 0px; color: #1596c1; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">ESA</a> Hubble Space Telescope show a myriad of stars in crystal clear detail. The brilliant open star clusters, NGC 265 and NGC 290, are located about 200,000 light-years away and are roughly 65 light-years across.</div>
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<strong style="border: 0px; margin: 0px 0px 15px; outline: 0px; padding: 0px; vertical-align: baseline;">Credit:</strong></div>
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European Space Agency & <a href="http://www.nasa.gov/" style="border: 0px; color: #1596c1; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">NASA</a></div>
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Acknowledgements:</div>
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Davide De Martin (<a href="http://www.esa.org/" style="border: 0px; color: #1596c1; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">ESA</a>/<a href="http://www.spacetelescope.org/" style="border: 0px; color: #1596c1; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">Hubble</a>) and Edward W. Olszewski (University of Arizona, USA)</div>
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<b style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"><span style="font-size: large;">NGC 346</span></b><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> is an </span><a href="http://en.wikipedia.org/wiki/Open_cluster" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px;" title="Open cluster">open cluster</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> with associated </span><a href="http://en.wikipedia.org/wiki/Nebula" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Nebula">nebula</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> located in the </span><a href="http://en.wikipedia.org/wiki/Small_Magellanic_Cloud" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Small Magellanic Cloud">Small Magellanic Cloud</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> that appears in the </span><a href="http://en.wikipedia.org/wiki/Constellation" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Constellation">constellation</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Tucana_(constellation)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Tucana (constellation)">Tucana</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">. It contains </span><a href="http://en.wikipedia.org/wiki/HD_5980" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="HD 5980">HD 5980</a><span style="color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">, the brightest star in the SMC.</span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://en.wikipedia.org/wiki/NGC_346</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEi0BLo_27GFEcNCDCrOZu3LPvjkqS-PEDiPCqY3NqJnJVo80DBgNL8JK5WqHSAppSu-bmF-KLsmkZP9O_RtDgJ6-Q-Ga_pjTAj6wME1e-cMTNFsLoLBfLhIcxVd0I74Or_QQjBt3ui-Zno/s1600/Ngc346.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEi0BLo_27GFEcNCDCrOZu3LPvjkqS-PEDiPCqY3NqJnJVo80DBgNL8JK5WqHSAppSu-bmF-KLsmkZP9O_RtDgJ6-Q-Ga_pjTAj6wME1e-cMTNFsLoLBfLhIcxVd0I74Or_QQjBt3ui-Zno/s1600/Ngc346.jpg" /></a></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="background-color: white; font-size: 14px; line-height: 22.399999618530273px;"><a href="http://en.wikipedia.org/wiki/NGC_346#mediaviewer/File:Ngc346.jpg">http://en.wikipedia.org/wiki/NGC_346#mediaviewer/File:Ngc346.jpg</a></span></span></div>
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<span style="background-color: white;"><span class="mw-mmv-title" original-title="File name" style="font-size: 1.2em; max-width: 60%; overflow: hidden; text-overflow: ellipsis;">Ngc346</span><a class="mw-mmv-license" href="http://commons.wikimedia.org/wiki/File:Ngc346.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-size: 0.9em; padding: 0px 10px; text-align: right; text-decoration: none;" target="">Public Domain</a></span></div>
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<span style="background-color: white;"><span class="mw-mmv-author" original-title="Author">NASA, ESA and A. Nota (ESA/STScI, STScI/AURA)</span> - <span class="mw-mmv-source" original-title="Source"><a class="external free" href="http://www.spacetelescope.org/images/html/heic0514a.html" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://www.spacetelescope.org/images/html/heic0514a.html</a> (<a class="external text" href="http://www.spacetelescope.org/images/large/heic0514a.jpg" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">direct link</a>)</span></span></div>
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<b>Wonder and Mystery above the Very Large Telescopes </b><br /><b>Credit: </b><a href="mailto:ybialets%20at%20eso.org">Yuri Beletsky</a> (<a href="http://www.eso.org/">ESO</a>)</center>
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<b>Explanation: </b>What's that bright orange dot above the large telescope on the right? Even seasoned sky enthusiasts might <a href="http://apod.nasa.gov/apod/ap101213.html">ponder</a> the origin of the orange orb seen by <a href="http://blogs.families.com/media/catncompuermouse.jpg">scrolling</a> across <a href="http://www.eso.org/public/images/potw1119a/">this panoramic image</a>, taken last December. Perhaps identifying known objects will help. To start, on the far left is a diagonal band of light known as <a href="http://en.wikipedia.org/wiki/Zodiacal_light">zodiacal light</a>, sunlight reflected off of dust orbiting in the inner Solar System. The bright white spot on the left, just above the horizon, is <a href="http://apod.nasa.gov/apod/ap101020.html">Venus</a>, which also glows by reflected sunlight. Rising diagonally from the ground to the right of Venus is the band of our <a href="http://casswww.ucsd.edu/archive/public/tutorial/MW.html">Milky Way Galaxy</a>. In the image, the band, which usually <a href="http://www.youtube.com/watch?v=Wj8n_95_yNc">stretches dramatically</a> overhead, appears to arch above the elevated <a href="http://en.wikipedia.org/wiki/Chile">Chile</a>an landscape. Under the Milky Way arch, toward the left, lie both the <a href="http://coolcosmos.ipac.caltech.edu/cosmic_classroom/multiwavelength_astronomy/multiwavelength_museum/lmc.html">Large</a> and Small <a href="http://en.wikipedia.org/wiki/Magellanic_Clouds">Magellanic Cloud</a> galaxies, while toward the right lies the constellation of Orion surrounded by the red ring of <a href="http://apod.nasa.gov/apod/ap101023.html">Barnard's Loop</a>. On the ground, each of the four <a href="http://www.eso.org/public/teles-instr/vlt.html">Very Large Telescopes</a> is busy keeping an eye on the distant universe. The orange spot -- it's the Moon. The image was taken during a <a href="http://www.universetoday.com/81716/total-lunar-eclipse-december-21-2010/">total lunar eclipse</a> when the normally bright full moon turned into a faint <a href="http://science.nasa.gov/science-news/science-at-nasa/2008/13feb_lunareclipse/">orb tinted orange</a> by the intervening Earth's atmosphere. </div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas – As Constelações - são como janelas que se abrem para a infinitude do universo e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e sendo por nossa mente conscientizado. Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>COM UM ABRAÇO ESTRELADO,<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span></div>
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<span style="color: #073763;"><span style="font-family: Arial, sans-serif;">- 6<sup>a</sup>. Edição do <b>Atlas Celeste</b></span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="color: #073763;"><span style="font-family: Arial, sans-serif;">de autoria de <b>Ronaldo Rogério de Freitas Mourão</b>,</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="color: #073763;"><span style="font-family: Arial, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="color: #073763;"><span style="font-family: Arial, sans-serif;">(com dedicatória do próprio autor para mim</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="color: #073763;"><span style="font-family: Arial, sans-serif;">em evento realizado no Museu de Astronomia do Rio de Janeiro,</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="color: #073763;"><span style="font-family: Arial, sans-serif;">em 16/06/1989)</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="color: #073763;"><span lang="PT" style="font-family: Arial, sans-serif;">- </span><b><span style="font-family: Arial, sans-serif;">Mario Jaci Monteiro</span></b><span style="font-family: Arial, sans-serif;"> , <b>As Constelações, Cartas Celestes</b> -</span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="color: #073763;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC - com dedicatória do autor para mim, em março de 2004 (quando Mário Jaci generosamente me presenteou com um instrumento de observação (kepleriano) artesanalmente construído por ele).</span></span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US"><b>O CÉU DO SUL</b></span></span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgueo6uiaUbtGYn_oi4B4Dx9FsFCFtCThd7PlsMplJmYA0sheTK0gEc8YSIIGiO5aimUDXWf4ZPUwlaSp5a77eoHW5FVHGVHjTKzeqOS3NOWKvuKnSFsRkuXCqisfqAbLT29rJnkRgyLX_Z/s1600/c%C3%A9ud+o+sul.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgueo6uiaUbtGYn_oi4B4Dx9FsFCFtCThd7PlsMplJmYA0sheTK0gEc8YSIIGiO5aimUDXWf4ZPUwlaSp5a77eoHW5FVHGVHjTKzeqOS3NOWKvuKnSFsRkuXCqisfqAbLT29rJnkRgyLX_Z/s1600/c%C3%A9ud+o+sul.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
http://www.stellarium.org/pt/</div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="PT">Da Terra ao Céu<o:p></o:p></span></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="PT"> e ao Infinito</span></b><o:p></o:p></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelações, Estrelas e Objetos Celestes<o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(sob o ponto de vista do Mundo Ocidental)<o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Suas histórias, seus mitos, seus significados e suas sintetizadas descrições<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">Reunião das Informações e Compilação,</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">Tradução para a língua portuguesa (em alguns momentos)</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">bem como Comentários Pessoais:</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><span lang="PT">Janine Milward</span></i><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<o:p></o:p></span></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-40257207935844228052013-08-20T08:33:00.002-07:002015-06-09T05:59:09.137-07:00TRIANGULUM AUSTRALIS, O TRIÂNGULO DO SUL<div align="center" class="MsoNormal" style="text-align: center;">
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ao observarmos os céus mais ao sul,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">nestes tempos de céus mais escuros e transparentes</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e de ausência de Lua ao começo da noite,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">podemos nos deixar embevecer pela faixa esbranquiçada</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- a Via Lactea -</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que visualmente parece começar a partir da cauda do Escorpião,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">no horizonte mais a sudeste, </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">dirigindo-se para o Centauro acolhendo o Cruzeiro do Sul,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">esfuziantemente fusionando o Centauro à Quilha do Navio, Carina,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e ainda perseguindo o Cão Maior...., até desaparecer na linha do horizonte oeste.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">No Centauro, certamente duas estrelas sempre nos atraem a atenção:</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">são as estrelas Alpha e Beta Centauri, também conhecidas como Rigel Kent e Hadar.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Nesse lugar e um tantinho ainda mais ao sul,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">existe uma constelação que é absolutamente perfeita</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">de ser bem divisada em suas três estrelas ponteadoras</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">de seu formato estelar em Triângulo:</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">são as estrelas Alpha, Beta e Gamma Trianguli Australis.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A estrela-alpha Trianguli Australis é denominada enquanto Atria, </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">quer dizer, Alpha de Triangulum e é uma estrela-guia, certamente,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">brilhando como um farol, um farol austral!</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Triangulum Australis, o Triângulo do Sul ou Austral, </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é uma constelação neste formato estelar bem mais nítida</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">do que sua irmã bem mais ao norte, simplesmente conhecida por Triangulum</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e que se insere entre as constelações Perseus, Andromeda, Aries e Pisces.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(Aliás, é sempre bom recordarmos que as Galáxias Andromeda e Triangulum,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">M31 e M33, respectivamente, </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">moram nas direções das constelações </span></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Andromeda e Triangulum! </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">M31 e M33 fazem parte do nosso chamado Grupo Local de Galáxias.)</span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">É certo que nosso Triângulo do Sul não acolhe tanta importância...,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">mas, por outro lado, é bem mais perfeitamente desenhado estelarmente,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é bem mais visível do que seu irmão Triângulo do Norte!</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A bem da verdade, eu penso que a partir de nossa visualização do Triângulo Austral,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">outras constelações não tão nítidas em seu entorno podem vir a ser mais bem divisadas,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">como Ara, o Altar, Circinus, o Compasso, Musca, a Mosca, Apus, o Pássaro-do-Paraíso,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Pavo, o Pavão, Chamaleon, o Camaleão, Octans, o Oitante..... Enfim, todo uma côrte</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">de estrelinhas tímidas agrupadas em constelações fazendo suas vezes de girarem</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">conjuntamente em redor do ponto denominado como Polo Sul.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ah, os céus do sul são emocionantes</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e mais emocionados ficamos ao nos depararmos</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">com o farol iluminado e piscante</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que Atria realiza!</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celetes - CARJ</span></div>
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<span style="background-color: white; color: #073763;"><b><span lang="EN-US" style="font-family: Arial, sans-serif;"> </span><span style="font-family: Arial, sans-serif; font-size: 11pt; text-align: center;">TRIANGULUM AUSTRALIS, O TRIÂNGULO DO SUL</span></b></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Ascensão Reta 14h50m / 17h9m Declinação -60<sup>o</sup>.3 / -70<sup>o</sup>.3<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">História:<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Constelação atribuída a Pieter Theodor, no século 16. <o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Algumas Informações Interessantes acerca esta Constelação:<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">As estrelas Alpha, Beta e Gamma </span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">formam as três partes distintas que formam o Triangulo.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif; font-size: 11pt;">Atria</span><span style="font-family: Arial, sans-serif; font-size: 11pt;"> - Alpha Trianguli Australis<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Magnitude 1.93 Distância 82 anos-luz<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Vocábulo formado pela associação da letra A</span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;"> e a abreviatura do nome da constelação.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Beta Trianguli Australis<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Magnitude 2.87 Distância 42 anos-luz<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Gamma Trianguli Australis<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">Magnitude 2.94 Distância 113 anos-luz<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">- 6<sup>a</sup>. Edição do <b>Atlas Celeste</b></span><span style="font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">de autoria de <b>Ronaldo Rogério de Freitas Mourão</b>,</span><span style="font-family: "Arial","sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></div>
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<span style="background-position: initial initial; background-repeat: initial initial; color: #073763; font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><strong>Title: </strong>[Celestial Map of the Southern Hemisphere] <strong>Map<span style="color: #274e13;"> Maker: </span></strong><a href="https://www.raremaps.com/gallery/browse/creator_id/3418" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; text-decoration: none;">Ignace Gaston Pardies</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #274e13;"><span style="font-size: xx-small;">Fine fully colored example of this rare 17th Century map of the Southern Celestial Hemisphere, originally issued in 1674 by Ignace Gastone Pardies in Paris and revised in 1690, based in part on the work of the French Jesuit mathematician and astronomer Thomas Gouye (1650-1725).</span></span></span></div>
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<a href="https://www.blogger.com/null" id="p417"></a><span class="noindex pagenum" style="color: rgb(255, 51, 0) !important; font-size: x-small; font-weight: normal; position: absolute; right: 1.5em; text-align: right; top: auto; width: 70px;"><br />p417</span><div class="halfstart center" style="background-color: #ccffff; color: black; font-size: 12.8000001907349px; font-weight: normal; margin-left: 10px; margin-right: 10px; margin-top: 1.5em;">
<a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/home.html" style="color: rgb(204, 0, 0) !important; text-decoration: none;" target="index"><b><span class="larger" style="font-size: 17.9200000762939px;">Star Names<br /><span class="small" style="font-size: 15.2319993972778px;">Their Lore and Meaning </span></span><br />by<br /><span class="larger" style="font-size: 17.9200000762939px;">Richard Hinckley Allen </span></b></a><br />as reprinted<br />in the Dover edition, 1963</div>
<span style="background-color: #ccffff; color: black; font-size: 12.8000001907349px; font-weight: normal;">The text is in the public domain.</span></h2>
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<span style="background-color: white; font-size: 12.8000001907349px;"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Triangulum_Australe*.html">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Triangulum_Australe*.html</a></span></div>
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Triangulum Australe, the Southern Triangle</h2>
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much more noticeable than its northern original, first appeared in print in Bayer's <i>Uranometria</i> of 1603, although its formation is attributed to Pieter Theodor of nearly a century previous.</div>
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Caesius cited names for it drawn from the older constellation, among them <b>Almutabet algenubi</b> <span class="Latin" style="color: rgb(153, 0, 0) !important;">Arabicē neotericis</span>, which would show that either the Arabians had anticipated Bayer, or were very prompt to learn of his work. But he also called it the <b>Three Patriarchs</b>, doubtless Abraham, Isaac, and Jacob, from its three prominent stars; and Julius Schiller had recourse to their descendants for his alphabetical title <b>Signum Tau</b>. Proctor catalogued it as plain <b>Triangulum</b>, the Northern Triangle being one of his <b>Triangula</b>. The French, Germans, and Italians exactly translate the Latin words. The Chinese equivalent is <b><span class="Chinese" style="color: rgb(218, 83, 0) !important;">San Kiō Hung</span></b>.</div>
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The constellation lies south of Ara, between the tail of Pavo and the fore feet of the Centaur, Gould assigning to it 46 components down to the 7th magnitude. The <i>lucida</i> <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">α</span> comes to the meridian on the 14th of July.</div>
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<span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">α</span>, 2.2, <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">β</span> and <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 14.3999996185303px; font-style: italic;">γ</span>, 3.1 each, were — perhaps are now — the seamen's <b>Triangle Stars</b>.</div>
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Ideler said that La Caille substituted for it Norma et Regula, but in maps of the present day both constellations appear side by side.</div>
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<span style="color: #000066; font-family: Palatino Linotype, Palatino, Gentium Plus, serif;"><span style="line-height: 24px;">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Triangulum_Australe*.html</span></span></div>
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<img alt="Triangulum Australe constellation map.png" height="640" src="http://upload.wikimedia.org/wikipedia/commons/thumb/a/ab/Triangulum_Australe_constellation_map.png/240px-Triangulum_Australe_constellation_map.png" width="640" /><br />
http://pt.wikipedia.org/wiki/Triangulum_Australe#/media/File:Triangulum_Australe_constellation_map.png</div>
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<b>Triangulum Australe</b> (TrA) é uma pequena <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> no <a href="http://pt.wikipedia.org/wiki/Hemisf%C3%A9rio_celestial_sul" style="background: none; color: #0b0080; text-decoration: none;" title="Hemisfério celestial sul">hemisfério celestial sul</a>. Seu nome vem do <a href="http://pt.wikipedia.org/wiki/Latim" style="background: none; color: #0b0080; text-decoration: none;" title="Latim">Latim</a> e significa "triângulo do sul", distinguindo-a da constelação<a href="http://pt.wikipedia.org/wiki/Triangulum" style="background: none; color: #0b0080; text-decoration: none;" title="Triangulum">Triangulum</a> no hemisfério celestial norte. Esse nome é derivado do triângulo quase <a href="http://pt.wikipedia.org/wiki/Tri%C3%A2ngulo_equil%C3%A1tero" style="background: none; color: #0b0080; text-decoration: none;" title="Triângulo equilátero">equilátero</a> que suas três estrelas mais brilhantes formam. Apareceu pela primeira vez num globo celestial de <a href="http://pt.wikipedia.org/wiki/Petrus_Plancius" style="background: none; color: #0b0080; text-decoration: none;" title="Petrus Plancius">Petrus Plancius</a> em 1589, como Triangulus Antarcticus, e mais tarde com mais detalhes e seu nome atual por <a href="http://pt.wikipedia.org/wiki/Johann_Bayer" style="background: none; color: #0b0080; text-decoration: none;" title="Johann Bayer">Johann Bayer</a> em 1603 na obra<i><a href="http://pt.wikipedia.org/wiki/Uranometria" style="background: none; color: #0b0080; text-decoration: none;" title="Uranometria">Uranometria</a></i>. Em 1756, o explorador e astrônomo francês <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background: none; color: #0b0080; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a> catalogou as estrelas mais brilhantes e deu suas <a href="http://pt.wikipedia.org/wiki/Designa%C3%A7%C3%A3o_de_Bayer" style="background: none; color: #0b0080; text-decoration: none;" title="Designação de Bayer">designações de Bayer</a>.</div>
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A estrela mais brilhante da constelação, <a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli_Australis" style="background: none; color: #0b0080; text-decoration: none;" title="Alpha Trianguli Australis">Alpha Trianguli Australis</a>, conhecida como Atria, é uma <a href="http://pt.wikipedia.org/wiki/Estrela_gigante" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela gigante">gigante</a> laranja de segunda <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude</a>. As <a href="http://pt.wikipedia.org/wiki/Estrela_branca_da_sequ%C3%AAncia_principal" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela branca da sequência principal">estrelas brancas da sequência principal</a> <a href="http://pt.wikipedia.org/wiki/Beta_Trianguli_Australis" style="background: none; color: #0b0080; text-decoration: none;" title="Beta Trianguli Australis">Beta</a> e <a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli_Australis" style="background: none; color: #0b0080; text-decoration: none;" title="Gamma Trianguli Australis">Gamma Trianguli Australis</a> completam o triângulo. Apesar da constelação estar situada na <a href="http://pt.wikipedia.org/wiki/Via_L%C3%A1ctea" style="background: none; color: #0b0080; text-decoration: none;" title="Via Láctea">Via Láctea</a> e conter muitas estrelas, há poucos <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background: none; color: #0b0080; text-decoration: none;" title="Céu profundo">objetos de céu profundo</a> proeminentes, como o <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> <a href="http://pt.wikipedia.org/wiki/NGC_6025" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 6025">NGC 6025</a> e a <a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa planetária">nebulosa planetária</a> <a href="http://pt.wikipedia.org/wiki/NGC_5979" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 5979">NGC 5979</a>.</div>
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<span class="mw-headline" id="Hist.C3.B3ria"><span style="font-size: small;">História</span></span></h2>
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O navegador italiano <a href="http://pt.wikipedia.org/wiki/Am%C3%A9rico_Vesp%C3%BAcio" style="background: none; color: #0b0080; text-decoration: none;" title="Américo Vespúcio">Américo Vespúcio</a> explorou o <a href="http://pt.wikipedia.org/wiki/Novo_Mundo" style="background: none; color: #0b0080; text-decoration: none;" title="Novo Mundo">Novo Mundo</a> no início do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/S%C3%A9culo_16" style="background: none; color: #0b0080; text-decoration: none;" title="Século 16">século 16</a>. Ele observou e catalogou as estrelas do <a href="http://pt.wikipedia.org/wiki/Hemisf%C3%A9rio_celestial_sul" style="background: none; color: #0b0080; text-decoration: none;" title="Hemisfério celestial sul">hemisfério sul</a> para o rei <a href="http://pt.wikipedia.org/wiki/Manuel_I_de_Portugal" style="background: none; color: #0b0080; text-decoration: none;" title="Manuel I de Portugal">Manuel I de Portugal</a>. Além disso, também descreveu as estrelas do hemisfério sul, incluindo um triângulo que pode ser Triangulum Australe ou <a href="http://pt.wikipedia.org/wiki/Apus" style="background: none; color: #0b0080; text-decoration: none;" title="Apus">Apus</a>. Essas observações foram publicadas por <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Lorenzo_di_Pierfrancesco_de%27_Medici" style="background: none; color: #0b0080; text-decoration: none;" title="Lorenzo di Pierfrancesco de' Medici">Lorenzo di Pierfrancesco de' Medici</a> em 1504 como <i>Mundus Novus</i>.<span class="reference" id="cite_ref-Kanas2007_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-Kanas2007-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> A primeira representação da constelação foi feita em 1589 pelo astrônomo holandês<a href="http://pt.wikipedia.org/wiki/Petrus_Plancius" style="background: none; color: #0b0080; text-decoration: none;" title="Petrus Plancius">Petrus Plancius</a> em um <a href="http://pt.wikipedia.org/wiki/Globo_terrestre" style="background: none; color: #0b0080; text-decoration: none;" title="Globo terrestre">globo</a> celestial de 32,5 <a href="http://pt.wikipedia.org/wiki/Cent%C3%ADmetro" style="background: none; color: #0b0080; text-decoration: none;" title="Centímetro">cm</a> de diâmetro publicado em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Amsterd%C3%A3" style="background: none; color: #0b0080; text-decoration: none;" title="Amsterdã">Amsterdã</a> pelo cartógrafo <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Jacob_Floris_van_Langren&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Jacob Floris van Langren (página não existe)">Jacob Floris van Langren</a>,<span class="reference" id="cite_ref-StarTalesTrA_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-StarTalesTrA-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> no qual foi representada incorretamente a sul de <a href="http://pt.wikipedia.org/wiki/Argo_Navis" style="background: none; color: #0b0080; text-decoration: none;" title="Argo Navis">Argo Navis</a>, com o nome Triangulus Antarcticus. Seu estudante, junto com o explorador holandês <a href="http://pt.wikipedia.org/wiki/Frederick_de_Houtman" style="background: none; color: #0b0080; text-decoration: none;" title="Frederick de Houtman">Frederick de Houtman</a>, criou o nome Den Zuyden Trianghel.<span class="reference" id="cite_ref-Wagman2003_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-Wagman2003-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span>Triangulum Australe foi representada com mais precisão por <a href="http://pt.wikipedia.org/wiki/Johann_Bayer" style="background: none; color: #0b0080; text-decoration: none;" title="Johann Bayer">Johann Bayer</a> em seu atlas celestial <i><a href="http://pt.wikipedia.org/wiki/Uranometria" style="background: none; color: #0b0080; text-decoration: none;" title="Uranometria">Uranometria</a></i> em 1603, onde também recebeu seu nome atual.<span class="reference" id="cite_ref-Moore1997_4-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-Moore1997-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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Em um mapa de estrelas meridionais de 1756, <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background: none; color: #0b0080; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a> retratou as constelações <a href="http://pt.wikipedia.org/wiki/Norma_(constela%C3%A7%C3%A3o)" style="background: none; color: #0b0080; text-decoration: none;" title="Norma (constelação)">Norma</a>, <a href="http://pt.wikipedia.org/wiki/Circinus" style="background: none; color: #0b0080; text-decoration: none;" title="Circinus">Circinus</a> e Triangulum Australe como um <a href="http://pt.wikipedia.org/wiki/Esquadro" style="background: none; color: #0b0080; text-decoration: none;" title="Esquadro">esquadro</a> e régua, um<a href="http://pt.wikipedia.org/wiki/Compasso_(geometria)" style="background: none; color: #0b0080; text-decoration: none;" title="Compasso (geometria)">compasso</a>, e um <a href="http://pt.wikipedia.org/wiki/N%C3%ADvel" style="background: none; color: #0b0080; text-decoration: none;" title="Nível">nível</a> respectivamente como um conjunto de instrumentos de desenhista.<span class="reference" id="cite_ref-StarTalesLacaille_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-StarTalesLacaille-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> Também representando-a como um nível, o astrônomo alemão <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Johann_Bode" style="background: none; color: #0b0080; text-decoration: none;" title="Johann Bode">Johann Bode</a>deu à constelação o nome alternativo de Libella em <i>Uranographia</i>.<span class="reference" id="cite_ref-StarTalesTrA_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-StarTalesTrA-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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O autor e poeta alemão <a href="http://pt.wikipedia.org/wiki/Philipp_von_Zesen" style="background: none; color: #0b0080; text-decoration: none;" title="Philipp von Zesen">Philippus Caesius</a> visualizou as estrelas como os <a href="http://pt.wikipedia.org/wiki/Patriarcas_b%C3%ADblicos" style="background: none; color: #0b0080; text-decoration: none;" title="Patriarcas bíblicos">três patriarcas bíblicos</a>, Abraão, Isaque e Jacó (com Atria sendo Abraão).<span class="reference" id="cite_ref-Motz1991_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-Motz1991-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span> Uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Abor%C3%ADgene_australiano" style="background: none; color: #0b0080; text-decoration: none;" title="Aborígene australiano">tribo indígena</a> do norte da Austrália representou as estrelas de Triangulum Australe como a cauda da divindade <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Serpente_Arco-%C3%8Dris&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Serpente Arco-Íris (página não existe)">Serpente Arco-Íris</a>, que se estendia desde <a href="http://pt.wikipedia.org/wiki/Crux" style="background: none; color: #0b0080; text-decoration: none;" title="Crux">Crux</a> até <a href="http://pt.wikipedia.org/wiki/Scorpius" style="background: none; color: #0b0080; text-decoration: none;" title="Scorpius">Scorpius</a>.<span class="reference" id="cite_ref-Harney2004_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-Harney2004-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span></div>
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<span class="mw-headline" id="Caracter.C3.ADsticas"><span style="font-size: small;">Características</span></span></h2>
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Triangulum Australe é uma pequena constelação limitada por <a href="http://pt.wikipedia.org/wiki/Norma_(constela%C3%A7%C3%A3o)" style="background: none; color: #0b0080; text-decoration: none;" title="Norma (constelação)">Norma</a> a norte, <a href="http://pt.wikipedia.org/wiki/Circinus" style="background: none; color: #0b0080; text-decoration: none;" title="Circinus">Circinus</a> a oeste, <a href="http://pt.wikipedia.org/wiki/Apus" style="background: none; color: #0b0080; text-decoration: none;" title="Apus">Apus</a> a sul e <a href="http://pt.wikipedia.org/wiki/Ara" style="background: none; color: #0b0080; text-decoration: none;" title="Ara">Ara</a> a leste. Está próxima de <a href="http://pt.wikipedia.org/wiki/Alpha_Centauri" style="background: none; color: #0b0080; text-decoration: none;" title="Alpha Centauri">Alpha</a> e <a href="http://pt.wikipedia.org/wiki/Beta_Centauri" style="background: none; color: #0b0080; text-decoration: none;" title="Beta Centauri">Beta Centauri</a>, com somente Circinus no meio.<span class="reference" id="cite_ref-Moore2005_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-Moore2005-8" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">8</a></span> A constelação está localizada dentro da <a href="http://pt.wikipedia.org/wiki/Via_L%C3%A1ctea" style="background: none; color: #0b0080; text-decoration: none;" title="Via Láctea">Via Láctea</a>, portanto possui muitas estrelas.<span class="reference" id="cite_ref-Inglis2004_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-Inglis2004-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span> Pode ser facilmente identificada no céu como um triângulo quase <a href="http://pt.wikipedia.org/wiki/Tri%C3%A2ngulo_equil%C3%A1tero" style="background: none; color: #0b0080; text-decoration: none;" title="Triângulo equilátero">equilátero</a>. Triangulum Australe está muito ao sul para ser visível dos Estados Unidos ou Europa,<span class="reference" id="cite_ref-Moore2005_8-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-Moore2005-8" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">8</a></span> mas pode ser observada de todo o hemisfério sul e é<a href="http://pt.wikipedia.org/wiki/Estrela_circumpolar" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela circumpolar">circumpolar</a> em boa parte dele.<span class="reference" id="cite_ref-Inglis2004_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-Inglis2004-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span> A abreviação de três letras da constelação, conforme definida pela <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Uni%C3%A3o_Astron%C3%B4mica_Internacional" style="background: none; color: #0b0080; text-decoration: none;" title="União Astronômica Internacional">União Astronômica Internacional</a> em 1922, é "TrA".<span class="reference" id="cite_ref-Russell1922_10-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-Russell1922-10" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">10</a></span> As bordas oficiais da constelação, definidas por <a href="http://pt.wikipedia.org/wiki/Eug%C3%A8ne_Joseph_Delporte" style="background: none; color: #0b0080; text-decoration: none;" title="Eugène Joseph Delporte">Eugène Delporte</a> em 1930, consistem de um polígono de 18 segmentos, com <a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">ascensão reta</a> variando entre 14<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 56,4<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> e 17<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 13,5<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> e<a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Declinação">declinação</a> entre −60,26° e −70,51°.<span class="reference" id="cite_ref-IAUboundary_11-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-IAUboundary-11" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">11</a></span></div>
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<span class="mw-headline" id="Objetos_not.C3.A1veis"><span style="font-size: small;">Objetos notáveis</span></span></h2>
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<span class="mw-headline" id="Estrelas"><span style="font-size: small;">Estrelas</span></span></h3>
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Triangulum Australe possui dez estrelas com <a href="http://pt.wikipedia.org/wiki/Designa%C3%A7%C3%A3o_de_Bayer" style="background: none; color: #0b0080; text-decoration: none;" title="Designação de Bayer">designação de Bayer</a>. Essas designações foram dadas por <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background: none; color: #0b0080; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, que nomeou doze estrelas, sendo que duas delas (Eta<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">2</span> e Lambda) não são mais conhecidas pela designação.<span class="reference" id="cite_ref-Wagman2003_3-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-Wagman2003-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> As três estrelas mais brilhantes, Alpha, Beta e Gamma, formam o triângulo. <a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli_Australis" style="background: none; color: #0b0080; text-decoration: none;" title="Alpha Trianguli Australis">Alpha Trianguli Australis</a> (conhecida como Atria), a mais brilhante, é uma <a href="http://pt.wikipedia.org/wiki/Estrela_gigante_luminosa" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela gigante luminosa">gigante luminosa</a> de <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar#classe_K" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">classe K</a> a uma distância de 415 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> da Terra, com uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 1,92.<span class="reference" id="cite_ref-stars-alpha_12-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-stars-alpha-12" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">12</a></span> <a href="http://pt.wikipedia.org/wiki/Beta_Trianguli_Australis" style="background: none; color: #0b0080; text-decoration: none;" title="Beta Trianguli Australis">Beta Trianguli Australis</a> é uma <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Estrela_de_classe_F_da_sequ%C3%AAncia_principal&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Estrela de classe F da sequência principal (página não existe)">estrela de classe F da sequência principal</a> a 40 anos-luz de distância, com magnitude de 2,85.<span class="reference" id="cite_ref-stars-beta_13-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-stars-beta-13" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">13</a></span>Completando o triângulo, <a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli_Australis" style="background: none; color: #0b0080; text-decoration: none;" title="Gamma Trianguli Australis">Gamma Trianguli Australis</a> é uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Estrela_de_classe_A_da_sequ%C3%AAncia_principal" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela de classe A da sequência principal">estrela de classe A da sequência principal</a> a 183 anos-luz de distância e magnitude de 2,89.<span class="reference" id="cite_ref-stars-gamma_14-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-stars-gamma-14" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">14</a></span></div>
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<span class="mw-headline" id="Objetos_de_c.C3.A9u_profundo"><span style="font-size: small;">Objetos de céu profundo</span></span></h3>
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<br />Triangulum Australe tem poucos objetos de <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background: none; color: #0b0080; text-decoration: none;" title="Céu profundo">céu profundo</a>, que incluem um aglomerado aberto e algumas nebulosas e galáxias.<span class="reference" id="cite_ref-Inglis2004_9-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-Inglis2004-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span> <a href="http://pt.wikipedia.org/wiki/NGC_6025" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 6025">NGC 6025</a> é um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> com cerca de 30 estrelas de magnitude 7 a 9.<span class="reference" id="cite_ref-Inglis2004_9-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-Inglis2004-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span> Localizado aproximadamente 3 graus a nordeste de Beta Trianguli Australis, está a cerca de 2 500 anos-luz (770 parsecs) da Terra e tem um diâmetro de 11 anos-luz (3,4 parsecs). Sua estrela mais brilhante é MQ Trianguli Australis, com uma magnitude aparente de 7,1.<span class="reference" id="cite_ref-Mobberley2009_15-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-Mobberley2009-15" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">15</a></span> <a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa planetária">Nebulosas planetárias</a> na constelação incluem <a href="http://pt.wikipedia.org/wiki/NGC_5979" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 5979">NGC 5979</a>, de magnitude 12,3, e Henize 2-138, de magnitude 11,0.<span class="reference" id="cite_ref-Griffiths2012_16-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-Griffiths2012-16" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">16</a></span> <a href="http://pt.wikipedia.org/wiki/NGC_5938" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 5938">NGC 5938</a> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a> a 300 milhões de anos-luz (90 megaparsecs) de distância. Está localizada 5 graus a sul de Epsilon Trianguli Australis.<span class="reference" id="cite_ref-Polakis2001_17-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-Polakis2001-17" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">17</a></span> <a class="new" href="http://pt.wikipedia.org/w/index.php?title=ESO_69-6&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="ESO 69-6 (página não existe)">ESO 69-6</a> é um par de galáxias em fusão a 600 milhões de anos-luz (185 megaparsecs). A interação entre elas arrastou para fora seu material, formando longas caudas de gás e estrelas.<span class="reference" id="cite_ref-ESO69-6_18-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-ESO69-6-18" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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<span class="reference" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-ESO69-6-18" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">8</a></span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe">http://pt.wikipedia.org/wiki/Triangulum_Australe</a></span></span></div>
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Stellarium</div>
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<b>Alpha Trianguli Australis</b> (α TrA, α Trianguli Australis) é a <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a> mais brilhante da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Triangulum_Australe" style="background: none; color: #0b0080; text-decoration: none;" title="Triangulum Australe">Triangulum Australe</a>, com uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 1,92.<span class="reference" id="cite_ref-stars_5-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli_Australis#cite_note-stars-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> É uma das três estrelas que formam o triângulo representado na constelação. Tem o nome tradicional <b>Atria</b>, que é uma mera contração de sua <a href="http://pt.wikipedia.org/wiki/Designa%C3%A7%C3%A3o_de_Bayer" style="background: none; color: #0b0080; text-decoration: none;" title="Designação de Bayer">designação de Bayer</a>.<span class="reference" id="cite_ref-ridpath1989_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli_Australis#cite_note-ridpath1989-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span>Aparece na <a href="http://pt.wikipedia.org/wiki/Bandeira_do_Brasil" style="background: none; color: #0b0080; text-decoration: none;" title="Bandeira do Brasil">bandeira do Brasil</a>, simbolizando o estado do <a href="http://pt.wikipedia.org/wiki/Rio_Grande_do_Sul" style="background: none; color: #0b0080; text-decoration: none;" title="Rio Grande do Sul">Rio Grande do Sul</a>.<span class="reference" id="cite_ref-brazil_flag_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli_Australis#cite_note-brazil_flag-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span> Com base em medições de <a href="http://pt.wikipedia.org/wiki/Paralaxe" style="background: none; color: #0b0080; text-decoration: none;" title="Paralaxe">paralaxe</a>, está localizada a aproximadamente 391 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a>(120 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">parsecs</a>) da Terra.<span class="reference" id="cite_ref-simbad_1-8" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli_Australis#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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Alpha Trianguli Australis é uma estrela massiva com uma <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">classificação estelar</a> de K2 IIb-IIIa,<span class="reference" id="cite_ref-aaa120_1_21_2-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli_Australis#cite_note-aaa120_1_21-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> o que indica que, a uma idade de 48 milhões de anos,<span class="reference" id="cite_ref-aaa120_1_21_2-7" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli_Australis#cite_note-aaa120_1_21-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> já passou pela<a href="http://pt.wikipedia.org/wiki/Sequ%C3%AAncia_principal" style="background: none; color: #0b0080; text-decoration: none;" title="Sequência principal">sequência principal</a> e apresenta características de uma estrela <a href="http://pt.wikipedia.org/wiki/Estrela_gigante" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela gigante">gigante</a> e <a href="http://pt.wikipedia.org/wiki/Estrela_gigante_luminosa" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela gigante luminosa">gigante luminosa</a>. Tem uma massa de cerca de sete vezes a <a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Massa solar">massa do Sol</a><span class="reference" id="cite_ref-aaa120_1_21_2-8" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli_Australis#cite_note-aaa120_1_21-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> e um raio de 130 vezes o do Sol, equivalente a 60% do raio orbital da Terra.<span class="reference" id="cite_ref-stars_5-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli_Australis#cite_note-stars-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> Sua <a href="http://pt.wikipedia.org/wiki/Atmosfera_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Atmosfera estelar">atmosfera externa</a> emite 5 500 vezes mais luminosidade que o Sol, a uma <a href="http://pt.wikipedia.org/wiki/Temperatura_efetiva" style="background: none; color: #0b0080; text-decoration: none;" title="Temperatura efetiva">temperatura efetiva</a> de 4 150 <a href="http://pt.wikipedia.org/wiki/Kelvin" style="background: none; color: #0b0080; text-decoration: none;" title="Kelvin">K</a>,<span class="reference" id="cite_ref-aaa120_1_21_2-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli_Australis#cite_note-aaa120_1_21-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> o que lhe dá o brilho alaranjado típico de estrelas de classe K.<span class="reference" id="cite_ref-csiro_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli_Australis#cite_note-csiro-8" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Há indícios de que Alpha Trianguli Australis seja uma <a href="http://pt.wikipedia.org/wiki/Estrela_bin%C3%A1ria" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela binária">estrela binária</a>. Ela apresenta características incomuns para uma estrela de sua classe, como <a href="http://pt.wikipedia.org/wiki/Erup%C3%A7%C3%A3o_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Erupção solar">erupções</a> e uma alta emissão de <a href="http://pt.wikipedia.org/wiki/Raios_X" style="background: none; color: #0b0080; text-decoration: none;" title="Raios X">raios X</a>, as quais podem ser explicadas pela presença de uma estrela companheira <a href="http://pt.wikipedia.org/wiki/Campo_magn%C3%A9tico_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Campo magnético estelar">magneticamente ativa</a> com uma classificação estelar próxima a G0 V. Estrelas jovens de <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar#classe_G" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">classe G</a> têm uma alta temperatura na <a href="http://pt.wikipedia.org/wiki/Coroa_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Coroa solar">coroa</a> e frequentemente sofrem erupções, causando um aumento breve na luminosidade. Tal estrela teria uma massa parecida à do Sol e um <a href="http://pt.wikipedia.org/wiki/Per%C3%ADodo_orbital" style="background: none; color: #0b0080; text-decoration: none;" title="Período orbital">período orbital</a> de pelo menos 130 anos, estando separada da estrela primária por 50 <a href="http://pt.wikipedia.org/wiki/Unidade_astron%C3%B4mica" style="background: none; color: #0b0080; text-decoration: none;" title="Unidade astronômica">UA</a>.<span class="reference" id="cite_ref-apj658_2_L107_4-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli_Australis#cite_note-apj658_2_L107-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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<b>Beta Trianguli Australis</b> (β TrA, β Trianguli Australis) é a segunda <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a> mais brilhante da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Triangulum_Australe" style="background: none; color: #0b0080; text-decoration: none;" title="Triangulum Australe">Triangulum Australe</a>, com uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 2,85.<span class="reference" id="cite_ref-stars_3-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli_Australis#cite_note-stars-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> Com base em medições de <a href="http://pt.wikipedia.org/wiki/Paralaxe" style="background: none; color: #0b0080; text-decoration: none;" title="Paralaxe">paralaxe</a>, está localizada a aproximadamente 40,37 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (12,38 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">parsecs</a>) da Terra.<span class="reference" id="cite_ref-simbad_1-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli_Australis#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> Tem um <a href="http://pt.wikipedia.org/wiki/Estrela_de_movimento_pr%C3%B3prio" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela de movimento próprio">movimento próprio</a>particularmente rápido pela <a href="http://pt.wikipedia.org/wiki/Esfera_celeste" style="background: none; color: #0b0080; text-decoration: none;" title="Esfera celeste">esfera celeste</a>, de quase meio <a href="http://pt.wikipedia.org/wiki/Segundo_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Segundo de arco">segundo de arco</a> por ano.<span class="reference" id="cite_ref-stars_3-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli_Australis#cite_note-stars-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></div>
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O espectro de Beta Trianguli Australis corresponde a uma <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">classificação estelar</a> de F1 V,<span class="reference" id="cite_ref-simbad_1-10" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli_Australis#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> o que indica que é uma <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Estrela_de_classe_F_da_sequ%C3%AAncia_principal&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Estrela de classe F da sequência principal (página não existe)">estrela de classe F da sequência principal</a>. Tem uma massa de 1,65 vezes a <a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Massa solar">massa do Sol</a> e um raio de 1,9 vezes o <a href="http://pt.wikipedia.org/wiki/Raio_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Raio solar">raio solar</a>.<span class="reference" id="cite_ref-stars_3-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli_Australis#cite_note-stars-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> Emite uma luminosidade 8,5 vezes maior que a do Sol<span class="reference" id="cite_ref-stars_3-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli_Australis#cite_note-stars-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> a uma <a href="http://pt.wikipedia.org/wiki/Temperatura_efetiva" style="background: none; color: #0b0080; text-decoration: none;" title="Temperatura efetiva">temperatura efetiva</a> de cerca de 7 400 <a href="http://pt.wikipedia.org/wiki/Kelvin" style="background: none; color: #0b0080; text-decoration: none;" title="Kelvin">K</a>,<span class="reference" id="cite_ref-aaa420_183_4-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli_Australis#cite_note-aaa420_183-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> o que lhe dá a coloração branco-amarela típica de estrelas de classe F.<span class="reference" id="cite_ref-csiro_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli_Australis#cite_note-csiro-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span> Beta Trianguli Australis forma uma <a href="http://pt.wikipedia.org/wiki/Estrela_dupla" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela dupla">estrela dupla</a> com uma <a href="http://pt.wikipedia.org/wiki/An%C3%A3_laranja" style="background: none; color: #0b0080; text-decoration: none;" title="Anã laranja">anã laranja</a> ou <a href="http://pt.wikipedia.org/wiki/An%C3%A3_branca" style="background: none; color: #0b0080; text-decoration: none;" title="Anã branca">anã branca</a> de magnitude 13 a uma separação de quase três <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a> na esfera celeste, o que é provavelmente apenas uma coincidência na linha de visão.<span class="reference" id="cite_ref-stars_3-7" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli_Australis#cite_note-stars-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></div>
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Observações com o <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Spitzer" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Spitzer">Telescópio Espacial Spitzer</a> revelam que Beta Trianguli Australis emite <a href="http://pt.wikipedia.org/wiki/Radia%C3%A7%C3%A3o_infravermelha" style="background: none; color: #0b0080; text-decoration: none;" title="Radiação infravermelha">radiação infravermelha</a> em excesso. Isso sugere a presença de material circunstelar no sistema, que pode ser um <a href="http://pt.wikipedia.org/wiki/Disco_circunstelar" style="background: none; color: #0b0080; text-decoration: none;" title="Disco circunstelar">disco de detritos</a>.<span class="reference" id="cite_ref-apjl710_1_L26_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli_Australis#cite_note-apjl710_1_L26-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span> A estrela pode ser um membro do <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Grupo_Beta_Pictoris&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Grupo Beta Pictoris (página não existe)">grupo Beta Pictoris</a>, uma <a href="http://pt.wikipedia.org/wiki/Cinem%C3%A1tica_estelar#associa.C3.A7.C3.B5es_estelares" style="background: none; color: #0b0080; text-decoration: none;" title="Cinemática estelar">associação</a> de cerca de 17 estrelas que compatilham origem e movimento pelo espaço. Se for um membro do grupo, Beta Trianguli Australis tem uma idade de cerca de 12 milhões de anos, que é a idade do grupo em si.<span class="reference" id="cite_ref-aj140_3_713_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli_Australis#cite_note-aj140_3_713-8" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Beta Trianguli Australis é uma das estrelas que aparecem na <a href="http://pt.wikipedia.org/wiki/Bandeira_do_Brasil" style="background: none; color: #0b0080; text-decoration: none;" title="Bandeira do Brasil">bandeira do Brasil</a>. Ela simboliza o estado de <a href="http://pt.wikipedia.org/wiki/Santa_Catarina" style="background: none; color: #0b0080; text-decoration: none;" title="Santa Catarina">Santa Catarina</a>.<span class="reference" id="cite_ref-bandeira_do_brasil_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli_Australis#cite_note-bandeira_do_brasil-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span></div>
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<b>Gamma Trianguli Australis</b> (γ TrA, γ Trianguli Australis) é a terceira <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a> mais brilhante da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Triangulum_Australe" style="background: none; color: #0b0080; text-decoration: none;" title="Triangulum Australe">Triangulum Australe</a>, com uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 2,88.<span class="reference" id="cite_ref-simbad_1-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli_Australis#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> É a estrela mais a sudoeste do <a href="http://pt.wikipedia.org/wiki/Asterismo_(astronomia)" style="background: none; color: #0b0080; text-decoration: none;" title="Asterismo (astronomia)">asterismo</a> tringular que dá nome à constelação.<span class="reference" id="cite_ref-stars_3-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli_Australis#cite_note-stars-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> Com base em medições de <a href="http://pt.wikipedia.org/wiki/Paralaxe" style="background: none; color: #0b0080; text-decoration: none;" title="Paralaxe">paralaxe</a>, está localizada a aproximadamente 184 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (56,4 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">parsecs</a>) da Terra.<span class="reference" id="cite_ref-simbad_1-10" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli_Australis#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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O espectro de Gamma Trianguli Australis corresponde a uma <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">classificação estelar</a> de A1 V,<span class="reference" id="cite_ref-simbad_1-11" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli_Australis#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> indicando que é uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Estrela_de_classe_A_da_sequ%C3%AAncia_principal" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela de classe A da sequência principal">estrela de classe A da sequência principal</a>, a qual gera energia pela <a href="http://pt.wikipedia.org/wiki/Fus%C3%A3o_nuclear" style="background: none; color: #0b0080; text-decoration: none;" title="Fusão nuclear">fusão nuclear</a> de hidrogênio em seu núcleo. No entanto, a uma idade de 260 milhões de anos,<span class="reference" id="cite_ref-apj620_2_1010_6-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli_Australis#cite_note-apj620_2_1010-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span> está perto do fim da fase de sequência principal e, portanto, é maior e mais brilhante que outras estrelas da mesma classe espectral (como <a href="http://pt.wikipedia.org/wiki/Sirius" style="background: none; color: #0b0080; text-decoration: none;" title="Sirius">Sirius</a>).<span class="reference" id="cite_ref-stars_3-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli_Australis#cite_note-stars-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> Gamma Trianguli Australis tem uma massa de aproximadamente 3,3 vezes a <a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Massa solar">massa solar</a><span class="reference" id="cite_ref-stars_3-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli_Australis#cite_note-stars-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> e um raio de 5,86 vezes o <a href="http://pt.wikipedia.org/wiki/Raio_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Raio solar">raio solar</a>.<span class="reference" id="cite_ref-apj660_2_1556_4-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli_Australis#cite_note-apj660_2_1556-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> Emite 220 vezes mais luminosidade que o Sol,<span class="reference" id="cite_ref-stars_3-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli_Australis#cite_note-stars-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> a uma <a href="http://pt.wikipedia.org/wiki/Temperatura_efetiva" style="background: none; color: #0b0080; text-decoration: none;" title="Temperatura efetiva">temperatura efetiva</a> de 9 400 <a href="http://pt.wikipedia.org/wiki/Kelvin" style="background: none; color: #0b0080; text-decoration: none;" title="Kelvin">K</a>,<span class="reference" id="cite_ref-apj660_2_1556_4-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli_Australis#cite_note-apj660_2_1556-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> o que lhe dá a coloração branca típica de estrelas de classe A.<span class="reference" id="cite_ref-csiro_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli_Australis#cite_note-csiro-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span></div>
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Gamma Trianguli Australis possui uma abundância anormal do elemento <a href="http://pt.wikipedia.org/wiki/Eur%C3%B3pio" style="background: none; color: #0b0080; text-decoration: none;" title="Európio">európio</a>, o que indica que é uma <a href="http://pt.wikipedia.org/wiki/Estrela_peculiar" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela peculiar">estrela peculiar</a> do tipo <a href="http://pt.wikipedia.org/wiki/Estrela_Ap_e_Bp" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela Ap e Bp">Ap</a>.<span class="reference" id="cite_ref-aas130_215_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli_Australis#cite_note-aas130_215-8" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">8</a></span> A maioria dessas estrelas têm<a href="http://pt.wikipedia.org/wiki/Rota%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Rotação estelar">rotação</a> lenta,<span class="reference" id="cite_ref-apjs99_135_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli_Australis#cite_note-apjs99_135-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span> mas Gamma Trianguli Australis apresenta uma alta <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Velocidade_de_rota%C3%A7%C3%A3o_projetada" style="background: none; color: #0b0080; text-decoration: none;" title="Velocidade de rotação projetada">velocidade de rotação projetada</a> de 199 km/s.<span class="reference" id="cite_ref-aaa463_2_671_5-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli_Australis#cite_note-aaa463_2_671-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> Esta estrela emite excesso de <a href="http://pt.wikipedia.org/wiki/Radia%C3%A7%C3%A3o_infravermelha" style="background: none; color: #0b0080; text-decoration: none;" title="Radiação infravermelha">radiação infravermelha</a>, sugerindo a existência de um <a href="http://pt.wikipedia.org/wiki/Disco_circunstelar" style="background: none; color: #0b0080; text-decoration: none;" title="Disco circunstelar">disco circunstelar</a> orbitando-a. A temperatura média dessa emissão é de 50 K, correspondendo a uma separação de 481 <a href="http://pt.wikipedia.org/wiki/Unidade_astron%C3%B4mica" style="background: none; color: #0b0080; text-decoration: none;" title="Unidade astronômica">UA</a> da estrela.<span class="reference" id="cite_ref-apj660_2_1556_4-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli_Australis#cite_note-apj660_2_1556-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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Gamma Trianguli Australis é uma das estrelas que aparecem na <a href="http://pt.wikipedia.org/wiki/Bandeira_do_Brasil" style="background: none; color: #0b0080; text-decoration: none;" title="Bandeira do Brasil">bandeira do Brasil</a>. Ela simboliza o estado do <a href="http://pt.wikipedia.org/wiki/Paran%C3%A1" style="background: none; color: #0b0080; text-decoration: none;" title="Paraná">Paraná</a>.<span class="reference" id="cite_ref-bandeira_do_brasil_10-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli_Australis#cite_note-bandeira_do_brasil-10" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">10</a></span></div>
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<b>Delta Trianguli Australis</b> (δ TrA, δ Trianguli Australis) é a quarta <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a> mais brilhante da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Triangulum_Australe" style="background: none; color: #0b0080; text-decoration: none;" title="Triangulum Australe">Triangulum Australe</a>, com uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 3,86.<span class="reference" id="cite_ref-simbad_1-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Delta_Trianguli_Australis#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> De acordo com sua <a href="http://pt.wikipedia.org/wiki/Paralaxe" style="background: none; color: #0b0080; text-decoration: none;" title="Paralaxe">paralaxe</a> de 5,37 <a href="http://pt.wikipedia.org/wiki/Segundo_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Segundo de arco">milissegundos de arco</a>, está a uma distância de aproximadamente 610 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (186 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">parsecs</a>) da Terra.<span class="reference" id="cite_ref-simbad_1-10" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Delta_Trianguli_Australis#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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O espectro de Delta Trianguli Australis corresponde a uma <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">classificação estelar</a> de G2Ib-II,<span class="reference" id="cite_ref-simbad_1-11" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Delta_Trianguli_Australis#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> o que significa que é uma estrela de <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar#classe_G" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">classe G</a> (amarela) <a href="http://pt.wikipedia.org/wiki/Evolu%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Evolução estelar">evoluída</a> que apresenta características de uma <a href="http://pt.wikipedia.org/wiki/Estrela_supergigante" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela supergigante">supergigante</a> e <a href="http://pt.wikipedia.org/wiki/Estrela_gigante_luminosa" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela gigante luminosa">gigante luminosa</a>. De fato, é uma estrela enorme, com um raio de cerca de 50 vezes o <a href="http://pt.wikipedia.org/wiki/Raio_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Raio solar">raio solar</a>, valor calculado a partir do seu <a href="http://pt.wikipedia.org/wiki/Di%C3%A2metro_angular" style="background: none; color: #0b0080; text-decoration: none;" title="Diâmetro angular">diâmetro angular</a> de 2,5 milissegundos de arco e distância.<span class="reference" id="cite_ref-lang2006_3-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Delta_Trianguli_Australis#cite_note-lang2006-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> <span class="reference" id="cite_ref-aaa367_521_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Delta_Trianguli_Australis#cite_note-aaa367_521-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> Sua <a href="http://pt.wikipedia.org/wiki/Temperatura_efetiva" style="background: none; color: #0b0080; text-decoration: none;" title="Temperatura efetiva">temperatura efetiva</a> é de 4 990 <a href="http://pt.wikipedia.org/wiki/Kelvin" style="background: none; color: #0b0080; text-decoration: none;" title="Kelvin">K</a> e sua <a href="http://pt.wikipedia.org/wiki/Metalicidade" style="background: none; color: #0b0080; text-decoration: none;" title="Metalicidade">metalicidade</a>, a abundância de elementos além de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Hidrog%C3%AAnio" style="background: none; color: #0b0080; text-decoration: none;" title="Hidrogênio">hidrogênio</a> e <a href="http://pt.wikipedia.org/wiki/H%C3%A9lio" style="background: none; color: #0b0080; text-decoration: none;" title="Hélio">hélio</a>, equivale a 125% da solar.<span class="reference" id="cite_ref-aaa515_A11_4-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Delta_Trianguli_Australis#cite_note-aaa515_A11-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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Delta Trianguli Australis forma uma <a href="http://pt.wikipedia.org/wiki/Estrela_dupla" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela dupla">estrela dupla</a> com uma estrela de magnitude 12 separada no céu por 30 segundos de arco.<span class="reference" id="cite_ref-simbad_1-12" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Delta_Trianguli_Australis#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> <span class="reference" id="cite_ref-simbad2_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Delta_Trianguli_Australis#cite_note-simbad2-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span> <span class="reference" id="cite_ref-simbad3_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Delta_Trianguli_Australis#cite_note-simbad3-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span></div>
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<b>Epsilon Trianguli Australis</b> (ε TrA, ε Trianguli Australis) é a quinta <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a> mais brilhante da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Triangulum_Australe" style="background: none; color: #0b0080; text-decoration: none;" title="Triangulum Australe">Triangulum Australe</a>, com uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 4,11.<span class="reference" id="cite_ref-simbad_1-8" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Trianguli_Australis#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> Com base em medições de <a href="http://pt.wikipedia.org/wiki/Paralaxe" style="background: none; color: #0b0080; text-decoration: none;" title="Paralaxe">paralaxe</a>, está localizada a aproximadamente 202 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (61,8 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">parsecs</a>) da Terra.<span class="reference" id="cite_ref-simbad_1-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Trianguli_Australis#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> É uma <a href="http://pt.wikipedia.org/wiki/Estrela_gigante" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela gigante">gigante</a> laranja com uma <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">classificação estelar</a> de K1.5 III<span class="reference" id="cite_ref-simbad_1-10" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Trianguli_Australis#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> e uma <a href="http://pt.wikipedia.org/wiki/Temperatura_efetiva" style="background: none; color: #0b0080; text-decoration: none;" title="Temperatura efetiva">temperatura efetiva</a> de 4 444 <a href="http://pt.wikipedia.org/wiki/Kelvin" style="background: none; color: #0b0080; text-decoration: none;" title="Kelvin">K</a>.<span class="reference" id="cite_ref-Borde2002_5-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Trianguli_Australis#cite_note-Borde2002-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> Seu <a href="http://pt.wikipedia.org/wiki/Di%C3%A2metro_angular" style="background: none; color: #0b0080; text-decoration: none;" title="Diâmetro angular">diâmetro angular</a>, após correções de <a href="http://pt.wikipedia.org/wiki/Escurecimento_de_bordo" style="background: none; color: #0b0080; text-decoration: none;" title="Escurecimento de bordo">escurecimento de bordo</a>, é de 2,56 <a href="http://pt.wikipedia.org/wiki/Segundo_de_arco" style="background: none; color: #0b0080;" title="Segundo de arco">milissegundos de arco</a>,<span class="reference" id="cite_ref-aaa431_773_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Trianguli_Australis#cite_note-aaa431_773-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span> o que corresponde a um raio de 17 vezes o <a href="http://pt.wikipedia.org/wiki/Raio_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Raio solar">raio solar</a>.<span class="reference" id="cite_ref-lang2006_4-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Trianguli_Australis#cite_note-lang2006-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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Epsilon Trianguli Australis forma um <a href="http://pt.wikipedia.org/wiki/Estrela_bin%C3%A1ria" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela binária">sistema estelar binário</a> com uma estrela de <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar#classe_A" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">classe A</a> a uma distância angular de 83,2 segundos de arco na <a href="http://pt.wikipedia.org/wiki/Esfera_celeste" style="background: none; color: #0b0080; text-decoration: none;" title="Esfera celeste">esfera celeste</a>.<span class="reference" id="cite_ref-mnras389_2_869_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Trianguli_Australis#cite_note-mnras389_2_869-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span></div>
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<b style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">NGC 6025</b><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Triangulum Australe">constelação de Triangulum Australe</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. O objeto foi descoberto pelo astrônomo </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Nicolas_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Nicolas Lacaille">Nicolas Lacaille</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> em 1751, usando um</span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Telescópio">telescópio</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> refrator com abertura de 0,5 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> (+5,1), é fracamente visível a </span><a class="mw-disambig" href="http://pt.wikipedia.org/wiki/Olho_nu" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Olho nu">olho nu</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, mesmo em regiões distantes de cidades.</span></div>
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<img alt="NGC 5979, NASA" height="627" src="http://upload.wikimedia.org/wikipedia/commons/thumb/2/21/Ngc5979.jpg/250px-Ngc5979.jpg" width="640" /></div>
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http://pt.wikipedia.org/wiki/NGC_5979#/media/File:Ngc5979.jpg</div>
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<b style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">NGC 5979</b><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> é uma </span><a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Nebulosa planetária">nebulosa planetária</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Triangulum Australe">constelação de Triangulum Australe</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="John Herschel">John Herschel</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> em 1835, usando um</span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Telescópio">telescópio</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> (+11,5), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Telescópio">telescópios</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> amadores ou com equipamentos superiores.</span></div>
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<b>NGC 5938</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral_barrada" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia espiral barrada">espiral barrada</a> (SBbc) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Triangulum_Australe" style="background: none; color: #0b0080; text-decoration: none;" title="Triangulum Australe">Triangulum Australe</a>. Possui uma declinação de -66° 51' 33" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 15 <a href="http://pt.wikipedia.org/wiki/Hora" style="background: none; color: #0b0080; text-decoration: none;" title="Hora">horas</a>, 36 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto">minutos</a> e 26,1 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a>.</div>
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A galáxia <b>NGC 5938</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/9_de_Junho" style="background: none; color: #0b0080; text-decoration: none;" title="9 de Junho">9 de Junho</a> de <a href="http://pt.wikipedia.org/wiki/1836" style="background: none; color: #0b0080; text-decoration: none;" title="1836">1836</a> por <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background: none; color: #0b0080; text-decoration: none;" title="John Herschel">John Herschel</a>.</div>
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"Hubble Interacting Galaxy ESO 69-6 (2008-04-24)" por NASA, ESA, the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration, and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University) - http://hubblesite.org/newscenter/archive/releases/2008/16/image/as/ (direct link). Licenciado sob Domínio público, via Wikimedia Commons - http://commons.wikimedia.org/wiki/File:Hubble_Interacting_Galaxy_ESO_69-6_(2008-04-24).jpg#/media/File:Hubble_Interacting_Galaxy_ESO_69-6_(2008-04-24).jpg</div>
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NASA, ESA, the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration, and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University) -<a href="http://hubblesite.org/newscenter/archive/releases/2008/16/image/as/">http://hubblesite.org/newscenter/archive/releases/2008/16/image/as/</a> (<a href="http://imgsrc.hubblesite.org/hu/db/2008/16/images/as/formats/full_jpg.jpg">direct link</a>)</div>
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<b>The galaxies of this beautiful interacting pair bear some resemblance to musical notes on a stave. Long tidal tails sweep out from the two galaxies: gas and stars were stripped out and torn away from the outer regions of the galaxies. The presence of these tails is the unique signature of an interaction. ESO 69-6 is located in the constellation of Triangulum Australe, the Southern Triangle, about 650 million light-years away from Earth.</b> This image is part of a large collection of 59 images of merging galaxies taken by the Hubble Space Telescope and released on the occasion of its 18th anniversary on 24th April 2008. About the object Object name ESO 69-6, ESO 069-IG006, AM 1633-682 Object description Interacting Galaxies Position (J2000) 16 38 12.69 -68 26 25.4 Constellation Triangulum Australe Distance 600 million light-years (200 million parsecs) About the data Data description The Hubble image was created using HST data from proposal 10592: A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University) Instrument ACS/WFC Exposure date(s) April 8, 2002 Exposure time 39 minutes Filters F435W (B) and F814W (I)</div>
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<b><span style="font-family: sans-serif; line-height: 22.3999996185303px;"> </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=ESO_69-6&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="ESO 69-6 (página não existe)">ESO 69-6</a></b><span style="font-family: sans-serif; line-height: 22.3999996185303px;"> é um par de galáxias em fusão a 600 milhões de anos-luz (185 megaparsecs). A interação entre elas arrastou para fora seu material, formando longas caudas de gás e estrelas.</span><span class="reference" id="cite_ref-ESO69-6_18-0" style="bottom: 1ex; font-family: sans-serif; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Triangulum_Australe#cite_note-ESO69-6-18" style="background: none; text-decoration: none; white-space: nowrap;">18</a></span></div>
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http://pt.wikipedia.org/wiki/Triangulum_Australe</div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas </b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b>– As Constelações - </b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo</b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b> e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra...; </b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b> vai se tornando Cosmos</b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b> e sendo por nossa mente conscientizado. </b></span><br />
<b><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Quer dizer, </span></b><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>COM UM ABRAÇO ESTRELADO,<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b><o:p></o:p></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgyn7LtmGHfhMt_xhRYFzw38ogk9Hl9bs09tNFppwMrRnkxpWldwh3E23Y6r_8vODrpKEpSaIgztAc_rU25st5e7xUnEkLm2Juuyhkp672GISNSmGNSRCdoaHYVtSC-knHydT5ohnCbI6aB/s1600/constela%C3%A7%C3%B5es+junto+ao+polo+sul.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgyn7LtmGHfhMt_xhRYFzw38ogk9Hl9bs09tNFppwMrRnkxpWldwh3E23Y6r_8vODrpKEpSaIgztAc_rU25st5e7xUnEkLm2Juuyhkp672GISNSmGNSRCdoaHYVtSC-knHydT5ohnCbI6aB/s1600/constela%C3%A7%C3%B5es+junto+ao+polo+sul.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
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<a href="http://www.raremaps.com/gallery/detail/28535/The_Consellations_Southern_Hemisphere/Burritt.html" style="color: #274e13; text-decoration: none;"><span style="color: #073763;">http://www.raremaps.com/gallery/detail/28535/The_Consellations_Southern_Hemisphere/Burritt.html</span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">The Consellations (Southern Hemisphere)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/808" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; text-decoration: none;">Elijah J. Burritt</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Decorative chart of the southern skies, with a chart at the bottom left, identifying the magnitude of the various stars.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">The constellations and major stars are named within the image. From Burritt's <em>Atlas Designed to Illustrate the Geography of the Heavens.</em></span></div>
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<span style="background-color: white; color: #073763;"><b><span style="font-family: Arial, sans-serif;"><span style="line-height: 19px;"><br /></span></span></b><b style="line-height: 14.25pt;"><span lang="PT" style="font-family: Arial, sans-serif; font-size: 12pt;">Da Terra ao Céu<o:p></o:p></span></b></span></div>
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<span style="background-color: white; color: #073763;"><b><span lang="PT" style="font-family: Arial, sans-serif; font-size: 12pt;"> e ao Infinito</span></b><span style="font-family: Arial, sans-serif; font-size: 12pt;"><o:p></o:p></span></span></div>
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<span lang="PT" style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Constelações, Estrelas e Objetos Celestes<o:p></o:p></span></span></div>
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<span lang="PT" style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">(sob o ponto de vista do Mundo Ocidental)<o:p></o:p></span></span></div>
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<span lang="PT" style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Suas histórias, seus mitos, seus significados e suas sintetizadas descrições<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="PT" style="font-family: Arial, sans-serif;">Reunião das Informações e Compilação,</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="PT" style="font-family: Arial, sans-serif;">Tradução para a língua portuguesa (em alguns momentos)</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="PT" style="font-family: Arial, sans-serif;">bem como Comentários Pessoais:</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><i><span lang="PT" style="font-family: Arial, sans-serif;">Janine Milward</span></i><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif; font-size: 10.5pt;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado. Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Alguns dados<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">(tais como Ascensão Reta e Declinação, em muitos dos casos)<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">são época/equinócio 1980<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">e devem requerer do Caminhante do Céu<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">alguma pequena retificação.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Obrigada por sua compreensão.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;">Visitando os Sites abaixo,</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;"> você conseguirá informações atualizadas e preciosas</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;">sobre os Objetos Celestiais de seu interesse:</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><b><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">NASA/IPAC</span></b><b><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"> EXTRAGALACTIC DATABASE –</span></b><b><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></b></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://ned.ipac.caltech.edu/"><b><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">http://ned.ipac.caltech.edu/</span></b></a><b><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></b></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://ned.ipac.caltech.edu/forms/byname.html"><b><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">http://ned.ipac.caltech.edu/forms/byname.html</span></b></a><b><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></b></span></div>
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<span style="background-color: white; color: #073763;"><em><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">NASA/IPAC Extragalactic Database (NED) -</span></b></em><span class="apple-converted-space"><b><i><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"> </span></i></b></span><em><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></b></em><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></b></span></div>
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<b><span lang="EN-US" style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></b></div>
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<span style="background-color: white; color: #073763;"><a href="http://www.nightskyatlas.com/index.jsp"><span lang="EN-US" style="font-family: Arial, sans-serif;">http://www.nightskyatlas.com/index.jsp</span></a><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></b></span></div>
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<b><span lang="EN-US" style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></b></div>
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<span style="background-color: white; color: #073763;"><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">The</span></b><span class="apple-converted-space"><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"> </span></b></span><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">Internet STELLAR DATABASE</span></b><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></b></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://www.stellar-database.com/"><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">http://www.stellar-database.com/</span></b></a><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></b></span></div>
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<b><span lang="EN-US" style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<o:p></o:p></span></span></b></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-25728164120642121382013-08-20T08:32:00.001-07:002014-11-13T10:09:01.852-08:00TRIANGULUM, O TRIÂNGULO<div align="center" class="MsoNormal" style="text-align: center;">
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px; text-align: start;">Olá!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;"><div style="text-align: center;">
Caro Leitor, ao comentarmos um tantinhosobre a constelação Triangulum,</div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">estaremos também trazendo algumas palavras</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">sobre o fato de que M33, a Galáxia Triangulum,</span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">é nossa galáxia-irmã,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;"> quer dizer, pertencente ao chamado Grupo Local...</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;"><div style="text-align: center;">
Existe o chamado Grupo Local</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">formado por mais de 54 galáxias (incluindo as galáxias anãs)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e onde reinam a Via Lactea e Andromeda, M31, e ainda a Galáxia Triangulum, M33.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Neste nosso Grupo, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">o centro gravitacional repousa em algum lugar entre Via Lactea e Andromeda</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(e, em algum dia do futuro bem distante, estaremos nos abraçando).</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;"><div style="text-align: center;">
No entanto, vamos encontrar alguns alfarrábios</div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">comentando sobre o fato da possibilidade</span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">da Galáxia Triangulum ser </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">(ou não ser)</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">uma galáxia satélite de Andromeda.</span></div>
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(A galáxia-anã Pisces, satélite de Triangulum,</div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">posiciona-se em equidistância entre Triangulum e Andromeda</span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">e,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;"> portanto, podendo ser considerada como pertencente a ambas</span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;"> </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">e atuando enquanto laço de união entre ambas).</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Afirmam os alfarrábios,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">que a magnitude visual de Andromeda, M31, é 3.4</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(quer dizer, pode ser observada a olho nu</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">em céus escuros e transparentes e em noites de ausência de Lua</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- eu mesma já morei num Sítio de onde podia</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">observar Andromeda em visão enviesada, ou seja,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">através o rápido rasgo de visão).</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Afirmam os alfarrábios,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">que a magnitude visual de Triangulum, M33, é 5.7</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(quer dizer, dificilmente pode ser observada a olho nu...</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">porém é sempre aconselhável poder se tentar - por que não? -</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e também recorrer a um bom par de binóculos</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">ou mesmo a um simpático telescópio).</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">De quaquer forma,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">é bom que saibamos que,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">ao visualizarmos </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(seja a olho nu ou seja através alguma lente óptica)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">a Galáxia Andromeda, M31,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">estaremos também muito próximos </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">da boa visualização da Galáxia Triangulum, M33!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">E, após visualizarmos ou bem nos apercebermos</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">dos posicionamentos dessas nossas Galáxias-Irmãs,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">ao norte - Andromeda e Triangulum -,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">sempre poderemos girar nossa cabeça</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e voltarmos nosso corpo para o sul, bem ao sul,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e observarmos, felizes e contentes e a olho nu</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(em lugares de céus escuros e transparentes e em noites sem Lua)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">as Galáxias também nossas Irmãs,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">as Nuvens Pequena e Grande de Magalhães</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- as constelações Hydrus e Tucana acolhendo a Pequena Nuvem</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e as constelações Dorado e Mons Mensa acolhendo a Grande Nuvem!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Sem dúvida alguma,</span></div>
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estaremos diante de</div>
</span><span style="font-family: Arial, Helvetica, sans-serif;"><div style="text-align: center;">
uma longa jornada</div>
</span><span style="font-family: Arial, Helvetica, sans-serif;"><div style="text-align: center;">
da Terra ao Céu e ao Infinito!</div>
</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 18px; text-align: center;">
<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">The <b>Local Group</b> is the <a href="http://en.wikipedia.org/wiki/Galaxy_group" style="background-image: none; color: #274e13; text-decoration: none;" title="Galaxy group">group</a> of <a href="http://en.wikipedia.org/wiki/Galaxy" style="background-image: none; color: #274e13; text-decoration: none;" title="Galaxy">galaxies</a> that includes the <a href="http://en.wikipedia.org/wiki/Milky_Way" style="background-image: none; color: #274e13; text-decoration: none;" title="Milky Way">Milky Way</a> among others. It comprises more than 54 galaxies, counting <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Dwarf_galaxies" style="background-image: none; color: #274e13; text-decoration: none;" title="Dwarf galaxies">dwarf galaxies</a>. Its gravitational center is located somewhere between Milky Way and <a href="http://en.wikipedia.org/wiki/Andromeda_Galaxy" style="background-image: none; color: #274e13; text-decoration: none;" title="Andromeda Galaxy">Andromeda Galaxy</a>. The Local Group covers a diameter of 10 <a href="http://en.wikipedia.org/wiki/Light-year#Distances_in_light-years" style="background-image: none; color: #274e13; text-decoration: none;" title="Light-year">megalight-years</a>(3.1 <a href="http://en.wikipedia.org/wiki/Parsec#Megaparsecs_and_gigaparsecs" style="background-image: none; color: #274e13; text-decoration: none;" title="Parsec">megaparsecs</a>) (see <a class="mw-redirect" href="http://en.wikipedia.org/wiki/1_E%2B23_m" style="background-image: none; color: #274e13; text-decoration: none;" title="1 E+23 m">1 E+23 m</a> for distance comparisons) and has a binary (dumbbell)<sup class="reference" id="cite_ref-Karachentsevetal2006_1-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Local_Group#cite_note-Karachentsevetal2006-1" style="background-image: none; color: #274e13; text-decoration: none; white-space: nowrap;">[1]</a></sup> distribution. The group is estimated to have a total mass of 1.29±0.14 <span style="margin: 0px 0.15em 0px 0.25em;">×</span>10<sup style="line-height: 1em;">12</sup> <a href="http://en.wikipedia.org/wiki/Solar_mass" style="background-image: none; color: #274e13; text-decoration: none;" title="Solar mass">M<sub style="line-height: 1em;">☉</sub></a><sup class="reference" id="cite_ref-Karachentsevetal2006_1-1" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Local_Group#cite_note-Karachentsevetal2006-1" style="background-image: none; color: #274e13; text-decoration: none; white-space: nowrap;">[1]</a></sup> and has a <a href="http://en.wikipedia.org/wiki/Velocity_dispersion" style="background-image: none; color: #274e13; text-decoration: none;" title="Velocity dispersion">velocity dispersion</a> of 61±8 km/s.<sup class="reference" id="cite_ref-van_den_Bergh_1999_2-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Local_Group#cite_note-van_den_Bergh_1999-2" style="background-image: none; color: #274e13; text-decoration: none; white-space: nowrap;">[2]</a></sup> The group itself is part of the <a href="http://en.wikipedia.org/wiki/Virgo_Supercluster" style="background-image: none; color: #274e13; text-decoration: none;" title="Virgo Supercluster">Virgo Supercluster</a> (i.e. the Local Supercluster).<sup class="reference" id="cite_ref-tully1982_3-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Local_Group#cite_note-tully1982-3" style="background-image: none; color: #274e13; text-decoration: none; white-space: nowrap;">[3]</a></sup></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">The two most massive members of the group are Milky Way and Andromeda Galaxy. These two <a href="http://en.wikipedia.org/wiki/Spiral_galaxy" style="background-image: none; color: #274e13; text-decoration: none;" title="Spiral galaxy">spiral galaxies</a> each have a system of satellite galaxies.</span></div>
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<li style="border: none; margin: 0px 0px 0.1em; padding: 0.25em 0px; text-align: center;"><span style="font-family: Arial, Helvetica, sans-serif;">Milky Way's <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Milky_Way%27s_satellite_galaxies" style="background-image: none; color: #274e13; text-decoration: none;" title="Milky Way's satellite galaxies">satellite system</a> consists of <a href="http://en.wikipedia.org/wiki/Sagittarius_Dwarf_Elliptical_Galaxy" style="background-image: none; color: #274e13; text-decoration: none;" title="Sagittarius Dwarf Elliptical Galaxy">Sagittarius Dwarf Galaxy</a>, <a href="http://en.wikipedia.org/wiki/Large_Magellanic_Cloud" style="background-image: none; color: #274e13; text-decoration: none;" title="Large Magellanic Cloud">Large Magellanic Cloud</a>, <a href="http://en.wikipedia.org/wiki/Small_Magellanic_Cloud" style="background-image: none; color: #274e13; text-decoration: none;" title="Small Magellanic Cloud">Small Magellanic Cloud</a>, <a href="http://en.wikipedia.org/wiki/Canis_Major_Dwarf_Galaxy" style="background-image: none; color: #274e13; text-decoration: none;" title="Canis Major Dwarf Galaxy">Canis Major Dwarf</a>, <a href="http://en.wikipedia.org/wiki/Ursa_Minor_Dwarf" style="background-image: none; color: #274e13; text-decoration: none;" title="Ursa Minor Dwarf">Ursa Minor Dwarf</a>, <a href="http://en.wikipedia.org/wiki/Draco_Dwarf" style="background-image: none; color: #274e13; text-decoration: none;" title="Draco Dwarf">Draco Dwarf</a>, <a href="http://en.wikipedia.org/wiki/Carina_Dwarf" style="background-image: none; color: #274e13; text-decoration: none;" title="Carina Dwarf">Carina Dwarf</a>, <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Sextans_Dwarf" style="background-image: none; color: #274e13; text-decoration: none;" title="Sextans Dwarf">Sextans Dwarf</a>, <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Sculptor_Dwarf" style="background-image: none; color: #274e13; text-decoration: none;" title="Sculptor Dwarf">Sculptor Dwarf</a>, <a href="http://en.wikipedia.org/wiki/Fornax_Dwarf" style="background-image: none; color: #274e13; text-decoration: none;" title="Fornax Dwarf">Fornax Dwarf</a>, <a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)" style="background-image: none; color: #274e13; text-decoration: none;" title="Leo I (dwarf galaxy)">Leo I</a>, <a href="http://en.wikipedia.org/wiki/Leo_II_(dwarf_galaxy)" style="background-image: none; color: #274e13; text-decoration: none;" title="Leo II (dwarf galaxy)">Leo II</a>, and <a href="http://en.wikipedia.org/wiki/Ursa_Major_I_Dwarf" style="background-image: none; color: #274e13; text-decoration: none;" title="Ursa Major I Dwarf">Ursa Major I Dwarf</a> and <a href="http://en.wikipedia.org/wiki/Ursa_Major_II_Dwarf" style="background-image: none; color: #274e13; text-decoration: none;" title="Ursa Major II Dwarf">Ursa Major II Dwarf</a>.</span></li>
<li style="border: none; margin: 0px 0px 0.1em; padding: 0.25em 0px; text-align: center;"><span style="font-family: Arial, Helvetica, sans-serif;">Andromeda's <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Andromeda%27s_satellite_galaxies" style="background-image: none; color: #274e13; text-decoration: none;" title="Andromeda's satellite galaxies">satellite system</a> consists of <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Elliptical_Galaxy_M32" style="background-image: none; color: #274e13; text-decoration: none;" title="Elliptical Galaxy M32">M32</a>, <a href="http://en.wikipedia.org/wiki/Messier_110" style="background-image: none; color: #274e13; text-decoration: none;" title="Messier 110">M110</a>, <a href="http://en.wikipedia.org/wiki/NGC_147" style="background-image: none; color: #274e13; text-decoration: none;" title="NGC 147">NGC 147</a>, <a href="http://en.wikipedia.org/wiki/NGC_185" style="background-image: none; color: #274e13; text-decoration: none;" title="NGC 185">NGC 185</a>, <a href="http://en.wikipedia.org/wiki/Andromeda_I" style="background-image: none; color: #274e13; text-decoration: none;" title="Andromeda I">And I</a>, <a href="http://en.wikipedia.org/wiki/Andromeda_II" style="background-image: none; color: #274e13; text-decoration: none;" title="Andromeda II">And II</a>, <a href="http://en.wikipedia.org/wiki/Andromeda_III" style="background-image: none; color: #274e13; text-decoration: none;" title="Andromeda III">And III</a>, <a href="http://en.wikipedia.org/wiki/Andromeda_IV" style="background-image: none; color: #274e13; text-decoration: none;" title="Andromeda IV">And IV</a>, <a href="http://en.wikipedia.org/wiki/Andromeda_V" style="background-image: none; color: #274e13; text-decoration: none;" title="Andromeda V">And V</a>, <a href="http://en.wikipedia.org/wiki/Pegasus_Dwarf_Spheroidal_Galaxy" style="background-image: none; color: #274e13; text-decoration: none;" title="Pegasus Dwarf Spheroidal Galaxy">Pegasus dSph (aka And VI)</a>,<a href="http://en.wikipedia.org/wiki/Cassiopeia_Dwarf" style="background-image: none; color: #274e13; text-decoration: none;" title="Cassiopeia Dwarf">Cassiopeia Dwarf (aka And VII)</a>, <a href="http://en.wikipedia.org/wiki/Andromeda_VIII" style="background-image: none; color: #274e13; text-decoration: none;" title="Andromeda VIII">And VIII</a>, <a href="http://en.wikipedia.org/wiki/Andromeda_IX" style="background-image: none; color: #274e13; text-decoration: none;" title="Andromeda IX">And IX</a>, <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Dwarf_Spheroidal_Galaxy_Andromeda_X" style="background-image: none; color: #274e13; text-decoration: none;" title="Dwarf Spheroidal Galaxy Andromeda X">And X</a>, And XI, And XII, And XIII, And XIV, And XV, And XVI, And XVII, And XVIII, And XIX, and And XX.</span></li>
<li style="border: none; margin: 0px 0px 0.1em; padding: 0.25em 0px; text-align: center;"><span style="font-family: Arial, Helvetica, sans-serif;">The <a href="http://en.wikipedia.org/wiki/Triangulum_Galaxy" style="background-image: none; color: #274e13; text-decoration: none;" title="Triangulum Galaxy">Triangulum Galaxy</a>, the third largest and only unbarred <a href="http://en.wikipedia.org/wiki/Spiral_galaxy" style="background-image: none; color: #274e13; text-decoration: none;" title="Spiral galaxy">spiral galaxy</a> in the Local Group, may or may not be a companion to the Andromeda Galaxy. <a href="http://en.wikipedia.org/wiki/Pisces_Dwarf" style="background-image: none; color: #274e13; text-decoration: none;" title="Pisces Dwarf">Pisces Dwarf</a> is equidistant from the Andromeda Galaxy and the Triangulum Galaxy, so it may be a satellite of either.<sup class="reference" id="cite_ref-apj562_2_4-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Local_Group#cite_note-apj562_2-4" style="background-image: none; color: #274e13; text-decoration: none; white-space: nowrap;">[4]</a></sup></span></li>
<li style="border: none; margin: 0px 0px 0.1em; padding: 0.25em 0px; text-align: center;"><span style="font-family: Arial, Helvetica, sans-serif;">The membership of <a href="http://en.wikipedia.org/wiki/NGC_3109" style="background-image: none; color: #274e13; text-decoration: none;" title="NGC 3109">NGC 3109</a>, with its companions <a href="http://en.wikipedia.org/wiki/Sextans_A" style="background-image: none; color: #274e13; text-decoration: none;" title="Sextans A">Sextans A</a> and the <a href="http://en.wikipedia.org/wiki/Antlia_Dwarf" style="background-image: none; color: #274e13; text-decoration: none;" title="Antlia Dwarf">Antlia Dwarf</a>, is uncertain due to extreme distances from the center of the Local Group.</span></li>
<li style="border: none; margin: 0px 0px 0.1em; padding: 0.25em 0px; text-align: center;"><span style="font-family: Arial, Helvetica, sans-serif;">The other members of the group are gravitationally secluded from these large subgroups: <a href="http://en.wikipedia.org/wiki/IC_10" style="background-image: none; color: #274e13; text-decoration: none;" title="IC 10">IC 10</a>, <a href="http://en.wikipedia.org/wiki/IC_1613" style="background-image: none; color: #274e13; text-decoration: none;" title="IC 1613">IC 1613</a>, <a href="http://en.wikipedia.org/wiki/Phoenix_Dwarf" style="background-image: none; color: #274e13; text-decoration: none;" title="Phoenix Dwarf">Phoenix Dwarf</a>, <a href="http://en.wikipedia.org/wiki/Leo_A" style="background-image: none; color: #274e13; text-decoration: none;" title="Leo A">Leo A</a>, <a href="http://en.wikipedia.org/wiki/Tucana_Dwarf" style="background-image: none; color: #274e13; text-decoration: none;" title="Tucana Dwarf">Tucana Dwarf</a>,<a href="http://en.wikipedia.org/wiki/Cetus_Dwarf" style="background-image: none; color: #274e13; text-decoration: none;" title="Cetus Dwarf">Cetus Dwarf</a>, <a class="mw-redirect" href="http://en.wikipedia.org/wiki/PegDIG" style="background-image: none; color: #274e13; text-decoration: none;" title="PegDIG">Pegasus Dwarf Irregular</a>, <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Wolf-Lundmark-Melotte" style="background-image: none; color: #274e13; text-decoration: none;" title="Wolf-Lundmark-Melotte">Wolf-Lundmark-Melotte</a>, <a href="http://en.wikipedia.org/wiki/Aquarius_Dwarf" style="background-image: none; color: #274e13; text-decoration: none;" title="Aquarius Dwarf">Aquarius Dwarf</a>, and <a class="mw-redirect" href="http://en.wikipedia.org/wiki/SagDIG" style="background-image: none; color: #274e13; text-decoration: none;" title="SagDIG">Sagittarius Dwarf Irregular</a>.</span></li>
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<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Edwin_Hubble" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Edwin Hubble">Edwin Hubble</a> foi o primeiro a identificar o Grupo Local, no capítulo VI do seu livro <i>The Realm of Nebulae</i> (Hubble 1936, págs. 124-151). Ele descreve "<i>um típico e pequeno grupo de nebulosas o qual está isolado no campo geral</i>". No livro, ele descreve <b>por luminosidade decrescente, e os membros são <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M31" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="M31">M31</a>, a <a href="http://pt.wikipedia.org/wiki/Via_L%C3%A1ctea" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Via Láctea">Via Láctea</a>, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M33" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="M33">M33</a>, a <a href="http://pt.wikipedia.org/wiki/Grande_Nuvem_de_Magalh%C3%A3es" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Grande Nuvem de Magalhães">Grande Nuvem de Magalhães</a>, a<a href="http://pt.wikipedia.org/wiki/Pequena_Nuvem_de_Magalh%C3%A3es" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pequena Nuvem de Magalhães">Pequena Nuvem de Magalhães</a></b>, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M32" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="M32">M32</a>, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/NGC_205" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 205">NGC 205</a>, <a href="http://pt.wikipedia.org/wiki/NGC_6822" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 6822">NGC 6822</a>, <a href="http://pt.wikipedia.org/wiki/NGC_185" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 185">NGC 185</a>, <a href="http://pt.wikipedia.org/wiki/IC_1613" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="IC 1613">IC 1613</a> e <a href="http://pt.wikipedia.org/wiki/NGC_147" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 147">NGC 147</a>. Ele também identifica <a href="http://pt.wikipedia.org/wiki/IC_10" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="IC 10">IC 10</a> como um possível membro do Grupo Local. No anos 70, desde o trabalho dele, o número de membros conhecidos no Grupo Local tem aumentado de 12 para 36, em 2003. Este foi de modo, quase duas dúzias de galáxias de baixa luminosidade.<span class="reference" id="cite_ref-Bergh2003_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_Local#cite_note-Bergh2003-3" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></div>
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<span class="mw-headline" id="Gal.C3.A1xias_componentes"><span style="font-size: small;">Galáxias componentes</span></span></h2>
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<span class="mw-headline" id="Mapa">Mapa</span></h4>
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<map id="ImageMap_1_848498325" name="ImageMap_1_848498325" style="margin-left: auto; margin-right: auto;"></map><img alt="" class="thumbimage" data-file-height="480" data-file-width="640" height="480" src="http://upload.wikimedia.org/wikipedia/commons/thumb/f/fe/Local_Group.svg/640px-Local_Group.svg.png" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(242, 238, 228); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(204, 204, 204); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; margin-left: auto; margin-right: auto; padding: 8px; vertical-align: middle;" usemap="#ImageMap_1_848498325" width="640" /><br /><div style="margin-left: 0px; margin-right: auto; margin-top: -20px; text-align: left;">
<a href="http://pt.wikipedia.org/wiki/Ficheiro:Local_Group.svg" style="background: none; color: #0b0080; margin-left: auto; margin-right: auto; text-decoration: none;" title="Sobre esta imagem"><img alt="Sobre esta imagem" src="http://bits.wikimedia.org/static-1.25wmf2/extensions/ImageMap/desc-20.png" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(242, 238, 228); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; margin-left: auto; margin-right: auto; padding: 8px; position: relative; vertical-align: middle;" /></a></div>
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Grupo Local (mapa clicável)</div>
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<span class="mw-headline" id="Gal.C3.A1xias_membros">Galáxias membros</span></h4>
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<tr><th colspan="4" style="background-color: #f2f2f2; border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia espiral">Galáxias Espirais</a></th></tr>
<tr><th style="background-color: #f2f2f2; border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;">nome</th><th style="background-color: #f2f2f2; border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;">tipo</th><th style="background-color: #f2f2f2; border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;">constelação</th><th style="background-color: #f2f2f2; border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;">notas</th></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia de Andrômeda">Galáxia de Andrômeda</a> (M31, NGC 224)</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">SA(s)b</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="mw-disambig" href="http://pt.wikipedia.org/wiki/Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Andrômeda">Andrômeda</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">Maior membro do grupo, recentemente (2006) descobriu-se que também é uma espiral barrada. Pode ser menos massiva que a Via Láctea.</td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://pt.wikipedia.org/wiki/Via_L%C3%A1ctea" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Via Láctea">Via Láctea</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">SBbc</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">nenhuma</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">Segunda maior, contudo, a possível galáxia mais massiva do Grupo Local.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_Local#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/NGC_598" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 598">Galáxia do Triângulo</a> (M33, NGC 598)</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">SAc</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://pt.wikipedia.org/wiki/Triangulum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Triangulum">Triangulum</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">a única galáxia espiral não barrada e possível satélite da galáxia de Andrômeda.</td></tr>
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<span style="font-family: Arial, Helvetica, sans-serif;">A listagem continua</span></div>
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LEIA MAIS</div>
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em</div>
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<a href="http://pt.wikipedia.org/wiki/Grupo_Local">http://pt.wikipedia.org/wiki/Grupo_Local</a></div>
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<span style="font-size: 14px;">............................................</span><span style="font-family: Arial, Helvetica, sans-serif;"> M33, A Galáxia Triangulum</span></div>
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<span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">É uma das únicas três </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia espiral">galáxias espirais</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> do </span><a href="http://pt.wikipedia.org/wiki/Grupo_Local" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Grupo Local">Grupo Local</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> de galáxias, as outras sendo </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia de Andrômeda">Andrômeda</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> e a </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Via-Láctea">Via-Láctea</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. Contudo, é significativamente menor comparada as suas companheiras espirais, embora seja maior do que a média das galáxias espirais do </span><a href="http://pt.wikipedia.org/wiki/Universo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Universo">Universo</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. É provável que tenha uma</span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_sat%C3%A9lite" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia satélite">galáxia satélite</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, a </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_an%C3%A3_Pisces" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia anã Pisces">galáxia anã Pisces</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, embora também seja provável que a própria galáxia de Triângulo esteja ligada </span><a href="http://pt.wikipedia.org/wiki/Gravidade" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Gravidade">gravitacionalmente</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> a Andrômeda.</span><span class="reference" id="cite_ref-seds_6-2" style="bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-seds-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span></div>
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http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo</div>
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NASA's Galaxy Evolution Explorer Mission celebrates its sixth anniversary studying galaxies beyond our Milky Way through its sensitive ultraviolet telescope, the only such far-ultraviolet detector in space.</div>
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The mission studies the shape, brightness, size and distance of distant galaxies across 10 billion years of cosmic history, giving scientists a wealth of data to help us better understand the origins of the universe. One such object is pictured here, the galaxy NGC598, more commonly known as M33.</div>
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The image shows a map of the recent star formation history of M33. The bright blue and white areas are where star formation has been extremely active over the past few million years. The patches of yellow and gold are regions where star formation was more active 100 million years ago.</div>
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In addition, the ultraviolet image shows the most massive young stars in M33. These stars burn their large supply of hydrogen fuel quickly, burning hot and bright while emitting most of their energy at ultraviolet wavelengths. Compared with low-mass stars like our sun, which live for billions of years, these massive stars never reach old age, having a lifespan as short as a few million years.</div>
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Credit: NASA/JPL-Caltech</div>
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<span style="font-family: Arial, Helvetica, Verdana, sans-serif;"><i><a href="http://www.galex.caltech.edu/media/glx2009-01f_img02.html">http://www.galex.caltech.edu/media/glx2009-01f_img02.html</a></i></span></div>
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Mario Jaci Monteiro - As Constelações, Cartas Celestes</div>
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<span style="color: #660000;"><b><span lang="EN-US" style="font-family: Arial, sans-serif;"> </span><span style="font-family: Arial, sans-serif;">TRIANGULUM, O TRIÂNGULO</span></b></span></div>
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<span style="font-family: Arial, sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; line-height: 22px;">Ascensão Reta 1h29m / 2h48m Declinação +25<sup>o</sup>.4 / +37<sup>o</sup>.0<o:p></o:p></span><br /><span style="font-family: Arial, sans-serif; line-height: 22px;"><br /></span></div>
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<span style="font-family: Arial, sans-serif;"><b>Mito:</b><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">O Triângulo foi colocado no céu por Júpiter, </span></div>
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<span style="font-family: Arial, sans-serif;">a pedido de Ceres que gostaria de ver o formato da Ilha da Sicília</span></div>
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<span style="font-family: Arial, sans-serif;"> representado entre as estrelas.<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Algumas Informações Interessantes acerca esta Constelação:<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Esta constelação pode ser bem identificada</span></div>
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<span style="font-family: Arial, sans-serif;"> situando-se entre as estrelas Gamma Andromedae, Alamak, e Alpha Arietis, Hamal.<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Fronteiras:</span></div>
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<span style="font-family: Arial, sans-serif;">A constelação do Triangulum faz fronteira com Andrômeda, Pisces, Áries e Perseus.<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<img src="http://www.iau.org/static/public/constellations/gif/TRI.gif" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(242, 238, 228); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(102, 0, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></div>
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http://www.iau.org/static/public/constellations/gif/TRI.gif</div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">Estrelas e objetos interessantes, em Triangulum:</span></b><o:p></o:p></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Rasalmothallah - Alpha Trianguli</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude 3.45<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">O Triângulo, oriundo do árabe Ral al Muthallath.<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Beta Trianguli</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude 3<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>R Trianguli - Estrela Variável</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 02h34m Declinação +34<sup>o</sup>.03<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitudes: Max 5,3 Min 12,0 Período 265,6<o:p></o:p></span><br />
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;"> 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b>Alpha Trianguli</b> (α Tri, α Trianguli) é uma <a href="http://pt.wikipedia.org/wiki/Estrela_bin%C3%A1ria" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela binária">estrela binária</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Triangulum" style="background: none; color: #0b0080; text-decoration: none;" title="Triangulum">Triangulum</a>. É também conhecida pelos nomes tradicionais <b>Ras al Muthallah</b>, <b>Mothallah</b>e <b>Caput Trianguli</b>.<span class="reference" id="cite_ref-allen1962_7-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli#cite_note-allen1962-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span></div>
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Estimativas da <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">classificação estelar</a> combinada do sistema variam entre F5III<span class="reference" id="cite_ref-apjs180_1_117_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli#cite_note-apjs180_1_117-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> e F6IV.<span class="reference" id="cite_ref-aj125_4_2196_3-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli#cite_note-aj125_4_2196-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> A classe de luminosidade 'IV' ou 'III' indica se o componente primário é uma<a href="http://pt.wikipedia.org/wiki/Estrela_subgigante" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela subgigante">estrela subgigante</a> ou <a href="http://pt.wikipedia.org/wiki/Estrela_gigante" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela gigante">gigante</a>, respectivamente. Alpha Trianguli é uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Bin%C3%A1ria_espectrosc%C3%B3pica" style="background: none; color: #0b0080; text-decoration: none;" title="Binária espectroscópica">binária espectroscópica</a>, cujos componentes completam uma órbita ao redor do centro de massa a cada 1,736 dias. Como a estrela primária possui um rápido período de rotação, sua forma provavelmente é de um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Esferoide_oblato" style="background: none; color: #0b0080; text-decoration: none;" title="Esferoide oblato">esferoide oblato</a> (achatada nos polos). A visão <a href="http://pt.wikipedia.org/wiki/Elipsoide" style="background: none; color: #0b0080; text-decoration: none;" title="Elipsoide">elipsoidal</a> da estrela, vista de Terra, varia ao longo de uma órbita causando a luminosidade variar durante o mesmo período.<span class="reference" id="cite_ref-aj125_4_2196_3-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli#cite_note-aj125_4_2196-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> Estrelas assim são chamadas de<a class="new" href="http://pt.wikipedia.org/w/index.php?title=Vari%C3%A1vel_elipsoidal_rotativa&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Variável elipsoidal rotativa (página não existe)">variáveis elipsoidais</a>.</div>
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A <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> média de +3,41<span class="reference" id="cite_ref-simbad_1-10" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> de Alpha Trianguli é brilhante o suficiente para a estrela poder ser vista a olho nu. Ela é a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anexo:Lista_de_estrelas_da_constela%C3%A7%C3%A3o_de_Triangulum" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anexo:Lista de estrelas da constelação de Triangulum">segunda estrela mais brilhante</a>dessa fraca constelação, depois de <a href="http://pt.wikipedia.org/wiki/Beta_Trianguli" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Beta Trianguli">Beta Trianguli</a>. Medições de <a href="http://pt.wikipedia.org/wiki/Paralaxe" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Paralaxe">paralaxe</a> colocam o sistema a uma distância de 63,3 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (19,4 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Parsec">parsecs</a>) da Terra. A <a href="http://pt.wikipedia.org/wiki/Temperatura_efetiva" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Temperatura efetiva">temperatura efetiva</a> das camadas externas da estrela primária é de 6 288 K,<span class="reference" id="cite_ref-apj1_354_310_5-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli#cite_note-apj1_354_310-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> dando a ela um tom branco-amarelado típico de estrela de classe F. Seu raio média é cerca de três vezes o <a href="http://pt.wikipedia.org/wiki/Raio_solar" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Raio solar">raio solar</a>.<span class="reference" id="cite_ref-aj125_4_2196_3-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli#cite_note-aj125_4_2196-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> Estima-se que o sistema tenha uma idade de 1,6 bilhões de anos.<span class="reference" id="cite_ref-aaa418_989_4-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli#cite_note-aaa418_989-4" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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<b>Beta Trianguli</b> (β Trianguli, β Tri) é uma <a href="http://pt.wikipedia.org/wiki/Estrela_bin%C3%A1ria" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela binária">estrela binária</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Triangulum" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Triangulum">Triangulum</a>, localizada a cerca de 127 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>.<span class="reference" id="cite_ref-simbad_1-8" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> Embora tenha uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de apenas 3,0,<span class="reference" id="cite_ref-clpl4_99_2-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli#cite_note-clpl4_99-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> é a estrela mais brilhante dessa constelação.<span class="reference" id="cite_ref-garfinckle1997_4-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli#cite_note-garfinckle1997-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> Juntamente com <a href="http://pt.wikipedia.org/wiki/Alpha_Trianguli" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Alpha Trianguli">Alpha Trianguli</a>, essas estrelas eram chamadas de Al Mīzān em <a href="http://pt.wikipedia.org/wiki/L%C3%ADngua_%C3%A1rabe" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Língua árabe">árabe</a>.<span class="reference" id="cite_ref-garfinckle1997_4-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli#cite_note-garfinckle1997-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> Na astronomia tradicional chinesa, era a nona estrela de <i><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Tien_Ta_Tseang&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Tien Ta Tseang (página não existe)">Tien Ta Tseang</a></i> (<span lang="zh" xml:lang="zh">天大將軍九</span>).<span class="reference" id="cite_ref-AEEA_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli#cite_note-AEEA-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span></div>
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Beta Trianguli tem um <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">tipo espectral</a> de A5III, indicando que já passou pela <a href="http://pt.wikipedia.org/wiki/Sequ%C3%AAncia_principal" style="background: none; color: #0b0080; text-decoration: none;" title="Sequência principal">sequência principal</a> e é agora uma <a href="http://pt.wikipedia.org/wiki/Estrela_gigante" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela gigante">estrela gigante</a>. Está entre as estrelas menos <a href="http://pt.wikipedia.org/wiki/Estrela_vari%C3%A1vel" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela variável">variáveis</a>observadas pela sonda <a href="http://pt.wikipedia.org/wiki/Hipparcos" style="background: none; color: #0b0080; text-decoration: none;" title="Hipparcos">Hipparcos</a>, com a mangitude variando apenas 0,0005.<span class="reference" id="cite_ref-aaa367_297_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli#cite_note-aaa367_297-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span> É provavelmente uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Bin%C3%A1ria_espectrosc%C3%B3pica" style="background: none; color: #0b0080; text-decoration: none;" title="Binária espectroscópica">binária espectroscópica</a> com um período orbital de 31,39 dias e uma <a href="http://pt.wikipedia.org/wiki/Excentricidade_orbital" style="background: none; color: #0b0080; text-decoration: none;" title="Excentricidade orbital">excentricidade</a> de 0,43.<span class="reference" id="cite_ref-mnras389_2_869_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli#cite_note-mnras389_2_869-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span> As estrelas estão separadas por uma distância de menos de 5 <a href="http://pt.wikipedia.org/wiki/Unidade_astron%C3%B4mica" style="background: none; color: #0b0080; text-decoration: none;" title="Unidade astronômica">UA</a>.<span class="reference" id="cite_ref-pap5_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli#cite_note-pap5-8" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com base em observações feitas pelo <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Spitzer" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Spitzer">Telescópio Espacial Spitzer</a>, o sistema está emitindo um excesso de <a href="http://pt.wikipedia.org/wiki/Radia%C3%A7%C3%A3o_infravermelha" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Radiação infravermelha">radiação infravermelha</a>. Essa emissão pode ser explicada por um <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Disco_de_poeira&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Disco de poeira (página não existe)">disco de poeira</a> circumbinário orbitando a uma distância de cerca de 10–20 UA das estrelas. O disco está emitindo radiação infravermelha a uma temperatura de 100 K.<span class="reference" id="cite_ref-pap5_8-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Beta_Trianguli#cite_note-pap5-8" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">8</a></span></div>
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<b>Gamma Trianguli</b> (γ Tri, γ Trianguli) é a terceira <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a> mais brilhante da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Triangulum" style="background: none; color: #0b0080; text-decoration: none;" title="Triangulum">Triangulum</a>. Está localizada a aproximadamente 112 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>. Tem uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de +4,01 e forma uma estrela tripla óptica (coincidência na linha de visão) com <a href="http://pt.wikipedia.org/wiki/Delta_Trianguli" style="background: none; color: #0b0080; text-decoration: none;" title="Delta Trianguli">Delta Trianguli</a> e <a class="new" href="http://pt.wikipedia.org/w/index.php?title=7_Trianguli&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="7 Trianguli (página não existe)">7 Trianguli</a>.<span class="reference" id="cite_ref-kaler_stars_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli#cite_note-kaler_stars-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span></div>
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Gamma Trianguli tem um <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">tipo espectral</a> de A1Vnn,<span class="reference" id="cite_ref-aj74_375_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli#cite_note-aj74_375-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span> o que indica que é uma <a href="http://pt.wikipedia.org/wiki/Estrela_branca_da_sequ%C3%AAncia_principal" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela branca da sequência principal">estrela branca da sequência principal</a>. A <a href="http://pt.wikipedia.org/wiki/Temperatura_efetiva" style="background: none; color: #0b0080; text-decoration: none;" title="Temperatura efetiva">temperatura efetiva</a> na sua <a href="http://pt.wikipedia.org/wiki/Fotosfera" style="background: none; color: #0b0080; text-decoration: none;" title="Fotosfera">fotosfera</a> é de 9,440 K.<span class="reference" id="cite_ref-aaa501_1_297_4-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli#cite_note-aaa501_1_297-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> Possui uma <a href="http://pt.wikipedia.org/wiki/Rota%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Rotação estelar">rotação</a> rápida, com uma velocidade de 254 km/s no equador,<span class="reference" id="cite_ref-aaa462_2_671_5-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli#cite_note-aaa462_2_671-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> o que faz a estrelas obter a forma de um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Esferoide_oblato" style="background: none; color: #0b0080; text-decoration: none;" title="Esferoide oblato">esferoide oblato</a> como <a href="http://pt.wikipedia.org/wiki/Altair_(estrela)" style="background: none; color: #0b0080; text-decoration: none;" title="Altair (estrela)">Altair</a>.<span class="reference" id="cite_ref-kaler_stars_6-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli#cite_note-kaler_stars-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span> Como a<a href="http://pt.wikipedia.org/wiki/Inclina%C3%A7%C3%A3o_axial" style="background: none; color: #0b0080; text-decoration: none;" title="Inclinação axial">inclinação axial</a> da estrela é desconhecida, sua velocidade equatorial é no mínimo esse valor e possivelmente maior.<span class="reference" id="cite_ref-aaa462_2_671_5-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli#cite_note-aaa462_2_671-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> Por comparação, o <a href="http://pt.wikipedia.org/wiki/Sol" style="background: none; color: #0b0080; text-decoration: none;" title="Sol">Sol</a> possui uma rotação lenta com uma velocidade equatorial de 2 km/s.<span class="reference" id="cite_ref-stix2004_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli#cite_note-stix2004-8" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">8</a></span> O <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Efeito_doppler" style="background: none; color: #0b0080; text-decoration: none;" title="Efeito doppler">efeito doppler</a> da rápida rotação resulta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Linha_espectral" style="background: none; color: #0b0080;" title="Linha espectral">linhas de absorção</a> difusas no espectro, como indicado pelo 'nn' na classificação.<span class="reference" id="cite_ref-kaler2011_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli#cite_note-kaler2011-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span></div>
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Existe um <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Disco_de_poeira&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Disco de poeira (página não existe)">disco de poeira</a> orbitando a estrela, com uma massa combinada de cerca de <span style="white-space: nowrap;">2,9 × 10<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">–2</span></span> vezes a <a href="http://pt.wikipedia.org/wiki/Massa_da_Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Massa da Terra">massa da Terra</a>. Esse disco pode ser detectado porque ele é aquecido a uma temperatura de cerca de 75 K por Gamma Trianguli e está radiando isso como energia infravermelha. Ele está separado da estrela por 2,24 <a href="http://pt.wikipedia.org/wiki/Segundo_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Segundo de arco">segundos de arco</a>, correspondendo a 80 <a href="http://pt.wikipedia.org/wiki/Unidade_astron%C3%B4mica" style="background: none; color: #0b0080; text-decoration: none;" title="Unidade astronômica">UA</a>, ou 80 vezes a distância entre a Terra e o Sol.<span class="reference" id="cite_ref-apj660_2_1556_3-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gamma_Trianguli#cite_note-apj660_2_1556-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></div>
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m33atlas.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(242, 238, 228); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(102, 0, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></div>
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<span style="font-size: x-small;">http://www.ipac.caltech.edu/2mass/gallery/m33atlas.jpg</span></h1>
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<a href="https://www.blogger.com/null" name="m81" style="color: #274e13; text-decoration: none;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation." </a></div>
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Messier 33</h1>
<i><a href="http://messier.obspm.fr/galaxy.html" style="color: #274e13; text-decoration: none;">Spiral Galaxy</a> M33 (NGC 598)</i>, type Sc, in <a href="http://messier.obspm.fr/map/Tri.html" style="color: #274e13; text-decoration: none;">Triangulum</a><b><span style="font-size: medium;">Triangulum Galaxy</span></b><br /><b><br /></b><b><br /></b></center>
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<a href="http://messier.obspm.fr/Jpg/m33.jpg" style="color: #274e13; text-decoration: none;"><img align="right" alt="[m33.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m33.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(242, 238, 228); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(102, 0, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">01 : 33.9 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+30 : 39 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">3000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">5.7 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">73x45 (arc min)</td></tr>
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Probably discovered by Hodierna before 1654.</div>
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Independently discovered by Charles Messier 1764.</div>
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The Triangulum Galaxy Messier 33 (M33, NGC 598) is another prominent member of the <a href="http://messier.obspm.fr/more/local.html" style="color: #274e13; text-decoration: none;">Local Group</a> of galaxies. This galaxy is small compared to its big apparent neighbor, the <a href="http://messier.obspm.fr/m/m031.html" style="color: #274e13; text-decoration: none;">Andromeda galaxy M31</a>, and to our <a href="http://messier.obspm.fr/more/mw.html" style="color: #274e13; text-decoration: none;">Milky Way galaxy</a>, but by this more of average size for spiral galaxies in the universe. One of the small Local Group member galaxies, LGS 3, is possibly a satellite of M33, which itself may be a remote but gravitationally bound companion of the <a href="http://messier.obspm.fr/m/m031.html" style="color: #274e13; text-decoration: none;">Andromeda galaxy M31</a>.</div>
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M33 is approaching us (our Solar System) at 182 km/s according to R. Brent Tully, or at 179 +/-3 km/s according to <a href="http://messier.obspm.fr/xtra/supp/m_NED.html#m33" style="color: #274e13; text-decoration: none;">NED</a>. Corrected for our motion around the Milky Way's Galactic Center, it is approaching our Galaxy at 24 km/sec.</div>
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M33 was probably first found by <a href="http://messier.obspm.fr/xtra/similar/hodierna.html" style="color: #274e13; text-decoration: none;">Hodierna</a> before 1654 (perhaps together with open cluster <a href="http://messier.obspm.fr/xtra/ngc/n0752.html" style="color: #274e13; text-decoration: none;">NGC 752</a>). It was independently rediscovered by <a href="http://messier.obspm.fr/xtra/history/biograph.html" style="color: #274e13; text-decoration: none;">Charles Messier</a>, and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M33" style="color: #274e13; text-decoration: none;">cataloged by him</a> on August 25, 1764. Nevertheless, <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html" style="color: #274e13; text-decoration: none;">William Herschel</a>, who otherwise carefully avoided to number Messier's objects in his survey, <a href="http://messier.obspm.fr/xtra/similar/herschel.html" style="color: #274e13; text-decoration: none;">assigned it</a> the number H V.17, on the ground of an observation dated September 11, 1784. Also because of the cataloging of Herschel, the brightest and largest HII region (diffuse emission nebula containing ionized hydrogen) has obtained a NGC number of its own: <a href="http://messier.obspm.fr/more/m033_n604.html" style="color: #274e13; text-decoration: none;">NGC 604</a> (William Herschel's H III.150); it is situated in the northeastern part of the galaxy; apparently the bright knot near the top of our image. This is one of the largest H II regions known at all: it has a diameter of nearly 1500 light-years, and a spectrum similar to the Orion nebula <a href="http://messier.obspm.fr/m/m042.html" style="color: #274e13; text-decoration: none;">M42</a>. Hui Yang (University of Illinois) and Jeff J. Hester (Arizona State University) have taken a <a href="http://messier.obspm.fr/more/m033_n604.html" style="color: #274e13; text-decoration: none;">photograph of NGC 604 with the Hubble Space Tepescope</a>, resolving over 200 young hot massive stars (of 15 to 60 solar masses) which have recently formed here.</div>
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LEIA MAIS</div>
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em</div>
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<a href="http://messier.obspm.fr/m/m033.html">http://messier.obspm.fr/m/m033.html</a></div>
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<img alt="Click here for poster version of PIA12000" height="547" src="http://photojournal.jpl.nasa.gov/figures/PIA12000_fig1_thumb.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(242, 238, 228); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(102, 0, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="640" /></div>
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http://www.nasa.gov/mission_pages/galex/galexC-20090428.html</div>
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<span style="font-family: Arial, Helvetica, sans-serif; font-size: 12px; line-height: 18px; text-align: left;">In these side-by-side images of M33, the ultraviolet image on the left was taken by the Galaxy Evolution Explorer, while the ultraviolet and infrared image on the right is a blend of the mission's M33 image and another taken by NASA's Spitzer Space Telescope. M33, one of our closest galactic neighbors, is about 2.9 million light-years away in the constellation Triangulum, part of what's known as our Local Group of galaxies. </span><br style="font-family: Arial, Helvetica, sans-serif; font-size: 12px; line-height: 18px; text-align: left;" /><br style="font-family: Arial, Helvetica, sans-serif; font-size: 12px; line-height: 18px; text-align: left;" /><span style="font-family: Arial, Helvetica, sans-serif; font-size: 12px; line-height: 18px; text-align: left;">Image credit: NASA/JPL-Caltech </span></div>
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<span lang="EN-US" style="font-family: Arial, sans-serif;"><b><span style="color: #660000;">NGC 598 = M33 Galáxia Pinwheel</span></b><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Ascensão Reta 01h32m Declinação +30<sup>o</sup>.33<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Tipo S - Galáxia Espiral Magnitude fotográfica aparente 6,19 <o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Dimensões Angulares 61 X 42 Distância (milhões de anos-luz) 2,4<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Pinwheel Galaxy, com um diâmetro igual ao da Lua. </span></div>
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<span style="font-family: Arial, sans-serif;"> Não é fácil de ser observada devido ao seu brilho pouco intenso. </span></div>
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<span style="font-family: Arial, sans-serif;">A partir do núcleo brilhante e pequeno, </span></div>
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<span style="font-family: Arial, sans-serif;">dois grandes e principais braços espiralados </span></div>
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<span style="font-family: Arial, sans-serif;">e alguns outros braços auxiliares são observados. </span></div>
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<span style="font-family: Arial, sans-serif;">Através grandes telescópios, podemos observar </span></div>
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<span style="font-family: Arial, sans-serif;">que os braços consistem de nuvens de estrelas</span></div>
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<span style="font-family: Arial, sans-serif;">e outros objetos como estrelas variáveis, aglomerados abertos e globulares, </span></div>
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<span style="font-family: Arial, sans-serif;">nebulosas, etc. </span></div>
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<span style="font-family: Arial, sans-serif;">A distância é de 2.4 milhões de anos-luz </span></div>
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<span style="font-family: Arial, sans-serif;">e o diâmetro é de cerca de 60 mil anos-luz </span></div>
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<span style="font-family: Arial, sans-serif;">e sua luminosidade total é igual a 300 milhões de nosso Sol. </span></div>
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<span style="font-family: Arial, sans-serif;"> Como o Triângulo é vizinho à Andrômeda, </span></div>
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<span style="font-family: Arial, sans-serif;">M33 situa-se próximo às estrelas Alpha do Triangulo e Beta de Andrômeda </span></div>
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<span style="font-family: Arial, sans-serif;">e esta Galáxia distancia-se da Galáxia de Andrômeda cerca de 570 mil anos-luz.<span style="background-color: #073763; color: black;"><o:p></o:p></span></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b style="color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif;">PIA11970: M33: A Close Neighbor Reveals its True Size and Splendor</b><span style="color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif;"> </span></div>
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<dd style="background-color: white; color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif; font-size: 14px; line-height: 19.6000003814697px; text-align: start;"><div style="margin-bottom: 1em; margin-top: 1em; padding: 0px;">
One of our closest galactic neighbors shows its awesome beauty in this new image from NASA's Spitzer Space Telescope. M33, also known as the Triangulum Galaxy, is a member of what's known as our Local Group of galaxies. Along with our own Milky Way, this group travels together in the universe, as they are gravitationally bound. In fact, M33 is one of the few galaxies that is moving toward the Milky Way despite the fact that space itself is expanding, causing most galaxies in the universe to grow farther and farther apart.</div>
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M33 is located about 2.9 million light-years away in the constellation Triangulum. This composite image was taken by Spitzer's infrared array camera. The color blue indicates infrared light of 3.6 microns, green shows 4.5-micron light, and red 8.0 microns.</div>
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<dt style="background-color: white; color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif; font-size: 14px; font-weight: bold; line-height: 19.6000003814697px; text-align: start;"><b>Image Credit:</b></dt>
<dd style="background-color: white; color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif; font-size: 14px; line-height: 19.6000003814697px; text-align: start;">NASA/JPL-Caltech</dd><dd style="background-color: white; color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif; font-size: 14px; line-height: 19.6000003814697px; text-align: start;"><br /></dd><dd style="background-color: white; color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif; font-size: 14px; line-height: 19.6000003814697px; text-align: start;">LEIA MAIS</dd><dd style="background-color: white; color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif; font-size: 14px; line-height: 19.6000003814697px; text-align: start;">em</dd><dd style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 14px; line-height: 19.6000003814697px; text-align: start;"><span style="color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif;"><a href="http://photojournal.jpl.nasa.gov/catalog/PIA11970">http://photojournal.jpl.nasa.gov/catalog/PIA11970</a></span></dd><dd style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 14px; line-height: 19.6000003814697px; text-align: start;"><span style="color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif;"><br /></span></dd><dd style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 14px; line-height: 19.6000003814697px; text-align: start;"><span style="color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif;"><br /></span></dd><dd style="background-color: white; color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif; font-size: 14px; line-height: 19.6000003814697px; text-align: start;"><div style="text-align: center;">
<img height="416" src="http://photojournal.jpl.nasa.gov/jpeg/PIA11969.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(242, 238, 228); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(102, 0, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="640" /></div>
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<span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">A </span><b style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">galáxia do Triângulo</b><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> (Messier 33, </span><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="New General Catalogue">NGC 598</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">) é uma </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> localizada a cerca de três milhões de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> na direção da </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o_do_Tri%C3%A2ngulo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Constelação do Triângulo">constelação do Triângulo</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">. Possui entre 40 a 60 mil anos-luz de </span><a href="http://pt.wikipedia.org/wiki/Di%C3%A2metro" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Diâmetro">diâmetro</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> e uma </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> de 5,5. Foi descoberta antes de 1654 por </span><a href="http://pt.wikipedia.org/wiki/Giovanni_Battista_Hodierna" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Giovanni Battista Hodierna">Giovanni Battista Hodierna</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">.</span></div>
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A <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a> foi descoberta por <a href="http://pt.wikipedia.org/wiki/Giovanni_Battista_Hodierna" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Giovanni Battista Hodierna">Giovanni Battista Hodierna</a> antes de 1654, juntamente com o <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> <a href="http://pt.wikipedia.org/wiki/NGC_752" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 752">NGC 752</a>. Foi redescoberta independentemente pelo astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a>, que o <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catalogou</a> em 25 de agosto de 1764.<a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="William Herschel">William Herschel</a>, descobridor de <a href="http://pt.wikipedia.org/wiki/Urano_(planeta)" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Urano (planeta)">Urano</a>, que usualmente não catalogava objetos já catalogados por Messier, catalogou a galáxia como a entrada H V.17 de seu catálogo durante uma observação em 11 de setembro de 1784. <span class="reference" id="cite_ref-seds_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-seds-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span></div>
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Pode ser vista a <a class="mw-disambig" href="http://pt.wikipedia.org/wiki/Olho_nu" style="background: none; color: #0b0080; text-decoration: none;" title="Olho nu">olho nu</a> em um <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background: none; color: #0b0080; text-decoration: none;" title="Céu noturno">céu noturno</a> sob excelentes condições: é o <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objeto_do_c%C3%A9u_profundo" style="background: none; color: #0b0080; text-decoration: none;" title="Objeto do céu profundo">objeto do céu profundo</a> mais distante a ser visto sem o auxílio de instrumentos ópticos. É razoavelmente observado em <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background: none; color: #0b0080; text-decoration: none;" title="Binóculo">binóculos</a>, embora todo o seu brilho esteja distribuído em uma área quatro vezes maior do que a <a href="http://pt.wikipedia.org/wiki/Lua_cheia" style="background: none; color: #0b0080; text-decoration: none;" title="Lua cheia">lua cheia</a>, deixando sua superfície extremamente pouco brilhante. Portanto, é praticamente impossível visualizar a galáxia em <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a> que não permitam baixa magnificação. É um dos alvos preferidos para a<a href="http://pt.wikipedia.org/wiki/Astronomia_amadora" style="background: none; color: #0b0080; text-decoration: none;" title="Astronomia amadora">astronomia amadora</a> e para os <a href="http://pt.wikipedia.org/wiki/Astrofotografia" style="background: none; color: #0b0080; text-decoration: none;" title="Astrofotografia">astrofotógrafos</a> amadores, pois é possível visualizar seus braços espirais e nebulosas brilhantes sem a utilização de equipamentos caros.<span class="reference" id="cite_ref-seds_6-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-seds-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span></div>
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É uma das únicas três <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia espiral">galáxias espirais</a> do <a href="http://pt.wikipedia.org/wiki/Grupo_Local" style="background: none; color: #0b0080; text-decoration: none;" title="Grupo Local">Grupo Local</a> de galáxias, as outras sendo <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia de Andrômeda">Andrômeda</a> e a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea" style="background: none; color: #0b0080; text-decoration: none;" title="Via-Láctea">Via-Láctea</a>. Contudo, é significativamente menor comparada as suas companheiras espirais, embora seja maior do que a média das galáxias espirais do <a href="http://pt.wikipedia.org/wiki/Universo" style="background: none; color: #0b0080; text-decoration: none;" title="Universo">Universo</a>. É provável que tenha uma<a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_sat%C3%A9lite" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia satélite">galáxia satélite</a>, a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_an%C3%A3_Pisces" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia anã Pisces">galáxia anã Pisces</a>, embora também seja provável que a própria galáxia de Triângulo esteja ligada <a href="http://pt.wikipedia.org/wiki/Gravidade" style="background: none; color: #0b0080; text-decoration: none;" title="Gravidade">gravitacionalmente</a> a Andrômeda.<span class="reference" id="cite_ref-seds_6-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-seds-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span></div>
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Está se aproximando radialmente do <a href="http://pt.wikipedia.org/wiki/Sistema_Solar" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sistema Solar">Sistema Solar</a> a uma velocidade de 182 km/s. Descontando a velocidade orbital do <a href="http://pt.wikipedia.org/wiki/Sol" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sol">Sol</a> em torno da Via-Láctea, Triângulo está se aproximando de nossa galáxia a 24 km/s.<br /></div>
<table border="0" cellpadding="3" class="infobox_v2" style="background-attachment: initial; background-clip: initial; background-color: #f9f9f9; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border: 1px solid rgb(170, 170, 170); clear: right; color: black; font-family: sans-serif; font-size: 12px; line-height: 1.1em; margin: 0px 0px 0.5em 1em; padding: 2px; width: 20em;"><tbody>
<tr><th class="" colspan="2" style="background-color: #99c9e6; font-size: 16px; text-align: center; vertical-align: top;"><span class="" style="font-weight: normal;"><span style="font-family: 'Times New Roman'; font-size: x-small;">Galáxia do Triângulo</span></span></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:M33HunterWilson09.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; margin-left: auto; margin-right: auto; text-decoration: none;"><span style="color: black; font-family: 'Times New Roman'; font-size: x-small;"></span></a></div>
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<small><span style="font-family: 'Times New Roman'; font-size: x-small;">Galáxia do Triângulo</span></small></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><span style="font-family: 'Times New Roman'; font-size: x-small;"><span style="font-weight: normal;">Dados observacionais (J2000)</span></span></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Constelação"><span style="color: black; font-family: 'Times New Roman'; font-size: x-small;">Constelação</span></a></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Triangulum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Triangulum"><span style="color: black; font-family: 'Times New Roman'; font-size: x-small;">Triangulum</span></a></td></tr>
<tr><td scope="row" valign="top"><span style="font-family: 'Times New Roman'; font-size: x-small;">Tipo</span></td><td valign="top"><span style="font-family: 'Times New Roman'; font-size: x-small;">SA(s)cd<span class="reference" id="cite_ref-ned_1-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;">1</a></span></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Ascensão reta"><span style="color: black; font-family: 'Times New Roman'; font-size: x-small;">Asc. reta</span></a></td><td valign="top"><span style="font-family: 'Times New Roman'; font-size: x-small;">01<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">h</span> 33<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">m</span> 50,02<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-SIMBAD-M33_2-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-SIMBAD-M33-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;">2</a></span></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Declinação"><span style="color: black; font-family: 'Times New Roman'; font-size: x-small;">Declinação</span></a></td><td valign="top"><span style="font-family: 'Times New Roman'; font-size: x-small;">+30° 39′ 36,7″<span class="reference" id="cite_ref-SIMBAD-M33_2-1" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-SIMBAD-M33-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;">2</a></span></span></td></tr>
<tr><td scope="row" valign="top"><span style="font-family: 'Times New Roman'; font-size: x-small;">Distância</span></td><td valign="top"><span style="font-family: 'Times New Roman'; font-size: x-small;">2,38-3,07 milhões de <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Ano-luz">anos-luz</a><br />(730-940 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Parsec">kpc</a>)<span class="reference" id="cite_ref-aass06_3-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-aass06-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;">3</a></span> <span class="reference" id="cite_ref-apj696_4-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-apj696-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;">4</a></span></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Desvio_para_o_vermelho" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Desvio para o vermelho"><span style="color: black; font-family: 'Times New Roman'; font-size: x-small;">Redshift</span></a></td><td valign="top"><span style="font-family: 'Times New Roman'; font-size: x-small;">-0,000607 ± 0,000010<span class="reference" id="cite_ref-SIMBAD-M33_2-2" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-SIMBAD-M33-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;">2</a></span></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Magnitude aparente"><span style="color: black; font-family: 'Times New Roman'; font-size: x-small;">Magnit. apar.</span></a></td><td valign="top"><span style="font-family: 'Times New Roman'; font-size: x-small;">5,72<span class="reference" id="cite_ref-SIMBAD-M33_2-3" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-SIMBAD-M33-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;">2</a></span></span></td></tr>
<tr><td scope="row" valign="top"><span style="font-family: 'Times New Roman'; font-size: x-small;">Dimensões</span></td><td valign="top"><span style="font-family: 'Times New Roman'; font-size: x-small;">70,8 × 41,7 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Minuto de arco">minutos de arco</a><span class="reference" id="cite_ref-SIMBAD-M33_2-4" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-SIMBAD-M33-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;">2</a></span></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><span style="font-family: 'Times New Roman'; font-size: x-small;"><span style="font-weight: normal;">Características físicas</span></span></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Massa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Massa"><span style="color: black; font-family: 'Times New Roman'; font-size: x-small;">Massa</span></a></td><td valign="top"><span style="font-family: 'Times New Roman'; font-size: x-small;">5 × 10<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">10</span><span class="reference" id="cite_ref-mnras342_1_5-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-mnras342_1-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;">5</a></span></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><span style="font-family: 'Times New Roman'; font-size: x-small;"><span style="font-weight: normal;">Outras denominações</span></span></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top"><span style="font-family: 'Times New Roman'; font-size: x-small;">Messier 33, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">NGC</a> 0598, MCG +05-04-069, 1ES 0131+303, RX J0133.8+3039, PGC 005818.<span class="reference" id="cite_ref-ned_1-1" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;">1</a></span></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><span style="font-family: 'Times New Roman'; font-size: x-small;"><span style="font-weight: normal;">Mapa</span></span></th></tr>
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<a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo">http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo</a></div>
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<br /><br /><span style="font-size: 14px;">...................................................... </span><span style="font-family: Arial, Helvetica, sans-serif; font-size: 14px;"> M33, A Galáxia Triangulum</span><br /><div style="font-size: 14px;">
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<span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">Foi umas das primeiras galáxias espirais a ser identificada como tal, segundo </span><a href="http://pt.wikipedia.org/wiki/William_Parsons" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="William Parsons">William Parsons</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. Também foi umas das primeiras galáxias, por definição, reconhecidas; </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Edwin_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Edwin Hubble">Edwin Hubble</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, com base na distância estimada com o auxílio de variáveis </span><a href="http://pt.wikipedia.org/wiki/Cefeida" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Cefeida">cefeidas</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, concluiu que Triângulo era um sistema estelar extragaláctico, publicando seus resultados em 1926. <b>Vários outros objetos brilhantes da galáxia ganharam suas próprias entradas no catálogo NGC: NGC 588, 592, 595 e 603, bem como no </b></span><i style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/Index_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="Index Catalogue"><b>Index Catalogue</b></a></i><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"><b>, IC 131, 132, 133, 134, 135, 136, 137, 139, 140, 142 e 143</b>, todas visíveis em </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Telescópio">telescópios</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> amadores com aberturas de 12,5 polegadas ou mais.</span><span class="reference" id="cite_ref-seds_6-4" style="bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-seds-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span><br /><br /><span style="font-size: 14px;">...........................................................</span></div>
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<a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo">http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo</a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">................................. <b> M33, A Galáxia Triangulum</b></span></div>
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<br /><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">Está se aproximando radialmente do </span><a href="http://pt.wikipedia.org/wiki/Sistema_Solar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Sistema Solar">Sistema Solar</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> a uma velocidade de 182 km/s. Descontando a velocidade orbital do </span><a href="http://pt.wikipedia.org/wiki/Sol" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Sol">Sol</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> em torno da Via-Láctea, Triângulo está se aproximando de nossa galáxia a 24 km/s.<b> Sua maior e mais brilhante </b></span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Regi%C3%A3o_HII" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Região HII">região HII</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> (uma </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Nebulosa_difusa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Nebulosa difusa">nebulosa difusa</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> contendo </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Hidrog%C3%AAnio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Hidrogênio">hidrogênio</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> ionizado) obteve seu próprio número </span><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="New General Catalogue">NGC</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">,</span><a href="http://pt.wikipedia.org/wiki/NGC_604" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="NGC 604">NGC 604</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. É uma das maiores regiões HII conhecidas, tendo um diâmetro de 1 500 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> e apresenta </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Linha_espectral" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Linha espectral">linhas espectrais</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> semelhantes às encontradas na </span><a href="http://pt.wikipedia.org/wiki/Nebulosa_de_%C3%93rion" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Nebulosa de Órion">nebulosa de Órion</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> (M42).</span><span class="reference" id="cite_ref-seds_6-3" style="bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-seds-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span><br /><br /><br /><div style="font-size: 14px;">
<a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo">http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo</a></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Nursery of New Stars - GPN-2000-000972</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte"><span class="mw-mmv-author">NASA, Hui Yang University of Illinois ODNursery of New Stars</span> - <span class="mw-mmv-source"><a class="external text" href="http://dayton.hq.nasa.gov/IMAGES/LARGE/GPN-2000-000972.jpg" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">Great Images in NASA</a> <a class="external text" href="http://grin.hq.nasa.gov/ABSTRACTS/GPN-2000-000972.html" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">Description</a></span></span></div>
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<span style="background-color: #fbfbfb; color: #555555; font-size: 16px; line-height: 24px;">This is a Hubble Space Telescope image (right) of a vast nebula called NGC 604, which lies in the neighboring spiral galaxy M33, located 2.7 million light-years away in the constellation Triangulum. This is a site where new stars are being born in a spiral arm of the galaxy. Though such nebulae are common in galaxies, this one is particularly large, nearly 1,500 light-years across. The nebula is so vast it is easily seen in ground-based telescopic images (left). At the heart of NGC 604 are over 200 hot stars, much more massive than our Sun (15 to 60 solar masses). They heat the gaseous walls of the nebula making the gas fluoresce. Their light also highlights the nebula's three-dimensional shape, like a lantern in a cavern. By studying the physical structure of a giant nebula, astronomers may determine how clusters of massive stars affect the evolution of the interstellar medium of the galaxy. The nebula also yields clues to its star formation history and will improve understanding of the starburst process when a galaxy undergoes a "firestorm" of star formation. The image was taken on January 17, 1995 with Hubble's Wide Field and Planetary Camera 2. Separate exposures were taken in different colors of light to study the physical properties of the hot gas (17,000 degrees Fahrenheit, 10,000 degrees Kelvin</span></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Interstellar.cloud.arp.750pix</span></div>
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<span class="mw-mmv-source-author mw-mmv-reduce-toolong" original-title="Autor e informação sobre a fonte" style="font-size: 0.8em;"><span class="mw-mmv-author">Hui Yang (University of Illinois) and NASA/ESA</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.spacetelescope.org/images/html/opo9627a.html" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">http://www.spacetelescope.org/images/html/opo9627a.html</a> (<a class="external text" href="http://www.spacetelescope.org/images/original/opo9627a.jpg" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">direct link</a>) <a class="external free" href="http://hubblesite.org/newscenter/archive/releases/1996/27/image/a/" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">http://hubblesite.org/newscenter/archive/releases/1996/27/image/a/</a></span></span></div>
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Uma das maiores <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Regi%C3%A3o_HII" style="background: none; color: #0b0080; text-decoration: none;" title="Região HII">regiões HII</a> (imagem obtida do <a href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_Palomar" style="background: none; color: #0b0080; text-decoration: none;" title="Observatório Palomar">Observatório Palomar</a>) encontra-se em Triângulo</div>
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The nebula cataloged as <a class="extiw" href="http://en.wikipedia.org/wiki/NGC_604" style="background: none; color: #0b0080; text-decoration: none;" title="en:NGC 604">NGC 604</a> is a giant star forming region, 1500 light years across, in the nearby spiral galaxy, <a class="extiw" href="http://en.wikipedia.org/wiki/Triangulum_Galaxy" style="background: none; color: #0b0080; text-decoration: none;" title="en:Triangulum Galaxy">M33</a>. Over 200 newly formed, hot, massive, stars are scattered within a cavern-like, gaseous, interstellar cloud. The stars irradiate the gas with energetic ultraviolet light stripping electrons from atoms and exciting them — producing a characteristic nebular glow.</div>
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<b>NGC 604</b> é uma <a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa">nebulosa</a> de grandes dimensões, com uma extensão de aproximadamente 1500 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a>. Essa nebulosa se encontra a cerca de 3 milhões de anos-luz da<a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> na direção da <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o_do_Tri%C3%A2ngulo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação do Triângulo">constelação do Triângulo</a>, próxima à borda da <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a> <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M33" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="M33">M33</a>.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/NGC_604#cite_note-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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A nebulosa NGC 604 apresenta belas cores e intensa atividade de <a href="http://pt.wikipedia.org/wiki/Forma%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Formação estelar">formação estelar</a>, sendo que muitos detalhes importantes da estrutura da nebulosa foram obtidos pelo<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a> em Agosto de <a href="http://pt.wikipedia.org/wiki/1996" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1996">1996</a> e ajudaram a esclarecer muitos pontos referentes à formação de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a> e à evolução do <a href="http://pt.wikipedia.org/wiki/Meio_interestelar" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Meio interestelar">meio interestelar</a>.</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/NGC_604</span></span></div>
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<span style="font-size: 14px;">......................................</span> <b><span style="font-family: Arial, Helvetica, sans-serif;">M33, A Galáxia Triangulum</span></b></div>
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<span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">É uma das únicas três </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia espiral">galáxias espirais</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> do </span><a href="http://pt.wikipedia.org/wiki/Grupo_Local" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Grupo Local">Grupo Local</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> de galáxias, as outras sendo </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia de Andrômeda">Andrômeda</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> e a </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Via-Láctea">Via-Láctea</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. Contudo, é significativamente menor comparada as suas companheiras espirais, embora seja maior do que a média das galáxias espirais do </span><a href="http://pt.wikipedia.org/wiki/Universo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Universo">Universo</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. <b>É provável que tenha uma</b></span><b><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_sat%C3%A9lite" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia satélite">galáxia satélite</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, a </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_an%C3%A3_Pisces" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia anã Pisces">galáxia anã Pisces</a></b><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, embora também seja provável que a própria galáxia de Triângulo esteja ligada </span><a href="http://pt.wikipedia.org/wiki/Gravidade" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Gravidade">gravitacionalmente</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> a Andrômeda.</span><span class="reference" id="cite_ref-seds_6-2" style="bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-seds-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a>................................</span></div>
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<span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">A galáxia anã </span><b style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">Pisces</b><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> é um pequena </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_irregular" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia irregular">galáxia irregular</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> e parte do </span><a href="http://pt.wikipedia.org/wiki/Grupo_Local" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Grupo Local">Grupo Local</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. <b>É a possível </b></span><b><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_sat%C3%A9lite" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia satélite">galáxia satélite</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> da </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia do Triângulo">Galáxia do Triângulo</a></b><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"><b> (M33)</b>. Na direção da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Constelação">constelação</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> de</span><a href="http://pt.wikipedia.org/wiki/Pisces" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Pisces">Pisces</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, a </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia">galáxia</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> é chamada de </span><i style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">Pisces</i><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> ou, para diferenciá-la de outros objetos astronômicos de nome similar, </span><i style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">Pisces anã</i><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. De acordo com os o deslocamento de suas linhas espectrais, calcula-se que esta galáxia esteja se aproximando da </span><a href="http://pt.wikipedia.org/wiki/Via_L%C3%A1ctea" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Via Láctea">Via Láctea</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> com uma velocidade de 287 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Km/s" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Km/s">km/s</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. Seu tipo morfológico está classificado alternativamente entre </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_an%C3%A3_esferoidal" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia anã esferoidal">esferoidal anã</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> e </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_irregular_an%C3%A3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia irregular anã">irregular anã</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, e isto é muito raro, só há duas galáxias conhecidas desse tipo.</span></div>
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<tr><th class="" colspan="2" style="background-color: #99c9e6; font-size: 16px; text-align: center; vertical-align: top;"><span class="">Pisces</span></th></tr>
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<small>Uma imagem da galáxia anã Pisces.</small></td></tr>
<tr><td scope="row" valign="top">Descoberto por</td><td valign="top">Karachentseva</td></tr>
<tr><td scope="row" valign="top">Data de descoberta</td><td valign="top">de <a href="http://pt.wikipedia.org/wiki/1976" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1976">1976</a></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Dados observacionais (J2000)</b></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Pisces" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pisces">Pisces</a></td></tr>
<tr><td scope="row" valign="top">Tipo</td><td valign="top">dIrr/dSph</td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td valign="top">01<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 03<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 55.0<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td valign="top">+21° 53′ 06″</td></tr>
<tr><td scope="row" valign="top">Distância</td><td valign="top">2.51 ± 0.08 milhões de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a>(769 ± 25 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>)</td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Desvio_para_o_vermelho" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Desvio para o vermelho">Redshift</a></td><td valign="top">-287 ± 0 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Km/s" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Km/s">km/s</a></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td valign="top">14.2</td></tr>
<tr><td scope="row" valign="top">Dimensões</td><td valign="top">2' × 2'</td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Outras denominações</b></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top">LGS 3, PGC 3792.</td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Mapa</b></th></tr>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas </span></b></div>
<div style="text-align: center;">
<b><span style="font-family: Arial, Helvetica, sans-serif;">são como janelas que se abrem para a infinitude do universo </span></b><br /><b><span style="font-family: Arial, Helvetica, sans-serif;">e que possibilitam nossa mente </span></b></div>
<div style="text-align: center;">
<b><span style="font-family: Arial, Helvetica, sans-serif;">a ir percebendo que existe mais, bem mais, </span></b><br /><b><span style="font-family: Arial, Helvetica, sans-serif;">entre o céu e a terra...; </span></b><br /><b><span style="font-family: Arial, Helvetica, sans-serif;">bem como percebendo que o caos, vagarosamente, </span></b><br /><b><span style="font-family: Arial, Helvetica, sans-serif;">vai se tornando Cosmos </span></b></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">e sendo por nossa mente conscientizado. </span></b></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">Quer dizer, </span></b></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></b></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">COM UM ABRAÇO ESTRELADO,</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span></div>
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</dd><dd><span style="color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif;"><br /></span></dd><dd style="color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif;"><img src="http://photojournal.jpl.nasa.gov/jpeg/PIA11969.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(242, 238, 228); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(102, 0, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></dd><br /><div class="separator" style="clear: both; text-align: center;">
<span style="line-height: 22.3999996185303px; text-align: start;"><span style="color: #252525; font-family: sans-serif;">http://photojournal.jpl.nasa.gov/jpeg/PIA11969.jpg</span></span></div>
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<img src="http://www.galex.caltech.edu/media/images/glx2009-01f_img02.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(242, 238, 228); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(102, 0, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br />
</b><b><span lang="PT">Da Terra ao Céu <o:p></o:p></span></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="PT"> e ao Infinito </span></b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelações, Estrelas e Objetos Celestes<o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(sob o ponto de vista do Mundo Ocidental)<o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Suas histórias, seus mitos, seus significados e suas sintetizadas
descrições<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">Reunião das
Informações e Compilação,</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">Tradução para a
língua portuguesa (em alguns momentos)</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">bem como
Comentários Pessoais:</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><span lang="PT">Janine Milward</span></i><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif; font-size: 10.5pt;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são
como janelas que se abrem para a infinitude do universo e que possibilitam
nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra
bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este
por nossa mente sendo conscientizado. Quer dizer, nossa mente é tão infinita
quanto infinito é o Cosmos.</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Alguns dados<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(tais como Ascensão Reta e Declinação, em muitos dos casos)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">são época/equinócio 1980<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e devem requerer do Caminhante do Céu<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações
atualizadas e preciosas<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de
seu interesse:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">NASA/IPAC</span><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"> EXTRAGALACTIC DATABASE
–</span><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/"><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">http://ned.ipac.caltech.edu/</span></a><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html"><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">http://ned.ipac.caltech.edu/forms/byname.html</span></a><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"> </span></i></span><em><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"> operated by the Jet Propulsion Laboratory,
California Institute of Technology, under contract with the National
Aeronautics and Space Administration.</span></em><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY
ATLAS<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky,
allowing easy location of any object. Detailed chart images show all stars
visible to the naked eye, the constellations, Messier objects, and names of the
brightest stars.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">The</span><span class="apple-converted-space"><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"> </span></span><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">Internet STELLAR DATABASE</span><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/"><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">http://www.stellar-database.com/</span></a><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- stars within 75
light-years. (Plus some of the more well-known "name brand"
stars farther away.)</span><span style="background-color: #073763; color: #fff2cc; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-58289791422340940212013-08-20T08:30:00.000-07:002015-05-27T06:48:34.260-07:00TELESCOPIUM, O TELESCÓPIO<div align="center" class="MsoNormal" style="text-align: center;">
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px; text-align: start;">Meu Projeto</span></div>
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="font-size: medium;">Da Terra ao Céu ....</span></span></a></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="font-size: medium;">.....<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;">e ao Infinito </a></span></span></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><span style="font-size: medium;">- As 88 Constelações</span></a></span></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;">http://daterraaoceueaoinfinito.blogspot.com.br/</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Stellarium</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Olá!</span></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Existe uma constelação bem interessante</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e que somente pode ser observada</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">em lugares de céus escuros e em noites límpidas</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e com Lua ausente:</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">é a constelação do Telescópio</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">que repousa sob a Coroa Austral</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">(outra constelação maravilhosa porém acolhendo estrelas bem tímidas!)</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e ambas essas constelações acontecem</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">bem próximasao lugar mais ao sul das entre as constelações do Escorpião e do Sagitário.</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Quer dizer, viemos conhecendo bem nitidamente tanto o Escorpião quanto o Sagitário</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">- que podem ser observados em noites com Lua ou sem Lua </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">(principalmente a figura impressionante do Escorpião, não é verdade?)...,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">no entanto, a Coroa Austral e, fundamentalmente, o Telescópio</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">são constelações bem pouco visíveis nos centros muito iluminados artificialmente</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">ou mesmo em noites de Lua trazendo muita iluminação</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">aos céus estrelados.</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Nesta Postagem, Caro Leitor,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">veja algumas informações</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">sobre a tímida e quase imperceptível</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">constelação do Telescópio</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">(constelação bem recente, formada por La Caille, em 1752)..</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Tímida e quase imperceptível - sim -,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">porém representando uma imensa homenagem</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">ao fantástico instrumento óptico</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">que nos revelou um novo mundo!</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Com um abraço estrelado,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Janine Milward</span></span><br />
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<span lang="EN-US" style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> </span><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>TELESCOPIUM, O TELESCÓPIO</b></span><br />
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<tr><td class="tr-caption" style="font-size: 13px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></td></tr>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000; line-height: 18.3999996185303px;"><span style="font-size: medium;">Galileo's telescope</span><span class="apple-converted-space"> </span></span></b><span lang="EN-US" style="color: #073763; line-height: 13.033332824707px;"><o:p></o:p></span></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US" style="line-height: 13.033332824707px;">© 2010<span class="apple-converted-space"> </span></span><span style="line-height: 16.8666667938232px;"><a href="http://www.museogalileo.it/en" style="color: #274e13; text-decoration: none;"><span lang="EN-US" style="line-height: 13.033332824707px;">Museo Galileo - Institute and Museum of the History of Science<span class="apple-converted-space"> </span></span></a></span><span lang="EN-US" style="line-height: 13.033332824707px;">· Piazza dei Giudici 1 · 50122 Florence · ITALY</span></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.astronomy2009.org/static/archives/images/screen/galileo_05.jpg" style="color: #274e13; text-decoration: none;">http://www.astronomy2009.org/static/archives/images/screen/galileo_05.jpg</a> <span style="line-height: 11.5px;"><br /></span>- Istituto e Museo di Storia della Scienza, Florence<o:p></o:p></span></div>
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<a href="http://catalogue.museogalileo.it/gallery/GalileosTelescope_n01.html" style="color: #274e13; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">http://catalogue.museogalileo.it/gallery/GalileosTelescope_n01.html</span></a></div>
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<a href="http://catalogue.museogalileo.it/gallery/GalileosTelescope_n03.html" style="color: #274e13; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">http://catalogue.museogalileo.it/gallery/GalileosTelescope_n03.html</span></a></div>
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<tr><td class="tr-caption" style="font-size: 13px;"><a href="http://catalogue.museogalileo.it/gallery/GalileoGalilei.html" style="color: #274e13; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">http://catalogue.museogalileo.it/gallery/GalileoGalilei.html</span></a></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>SAIBA MAIS SOBRE GALILEO GALILEI: </b> <a href="http://catalogue.museogalileo.it/object/GalileosTelescope_n01.html" style="color: #274e13; text-decoration: none;">http://catalogue.museogalileo.it/object/GalileosTelescop<u>http://catalogue.museogalileo.it/biography/GalileoGalilei.html</u>e_n01.html</a></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><br /><br /><br /><br /><br /><br /><br /><b><span style="color: #660000;">UMA REPRODUÇÃO DO TELESCÓPIO</span></b></span><br />
<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>USADO PARA DESCOBRIR URANO</b></span><br />
<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>- Na casa de WILLIAM HERSCHEL</b></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A reproduction of the telescope used to discover Uranus, Herschel House, Bath, England, // <em>Credit: David J. Eicher</em></span></div>
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<b><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">English Astronomers: Stonehenge and Bath, England<o:p></o:p></span></span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><span lang="EN-US"> </span><a href="http://cs.astronomy.com/members/David-Eicher/default.aspx" style="color: #274e13; text-decoration: none;"><span lang="EN-US">David Eicher </span></a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><b><span lang="EN-US"> </span></b><b><span lang="EN-US"><a href="http://cs.astronomy.com/asy/b/daves-universe/archive/2013/08/13/english-astronomers-stonehenge-and-bath-england.aspx" style="color: #274e13; text-decoration: none;">http://cs.astronomy.com/asy/b/daves-universe/archive/2013/08/13/english-astronomers-stonehenge-and-bath-england.aspx</a></span></b></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh_hRgoawDP9_R9o2P-KWSiHqi0f0trYAdEIY5zlk1qPa8nf5nUdRtPh1ZSPCNFCECol38QTZscg9hLsabeQPovvJQJFZlde9Fdfq0dWJzYv6HQh4ovQnBDRiRJIxaDr84k8l0qI6NmC23s/s1600/9275-Garden-at-Herschel-House.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" height="426" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh_hRgoawDP9_R9o2P-KWSiHqi0f0trYAdEIY5zlk1qPa8nf5nUdRtPh1ZSPCNFCECol38QTZscg9hLsabeQPovvJQJFZlde9Fdfq0dWJzYv6HQh4ovQnBDRiRJIxaDr84k8l0qI6NmC23s/s640/9275-Garden-at-Herschel-House.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The garden in which William Herschel discovered Uranus, Herschel House, Bath, England, August 12, 2013.<o:p></o:p></span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiJ1xdrpfumC75cWTv-XVeDB0pdH9V8IXcMuqOmsVoNAn_6ykx0lcY9f7Ek8kZHeYwBseMTyQ9WVYWwQW3WcRXB8nP02qDTwYji1puGovR8srEQLfayvMmTSlIIoPRX4F2zzX11QFUAxXZK/s1600/9237-Music-room-Herschel-House.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" height="426" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiJ1xdrpfumC75cWTv-XVeDB0pdH9V8IXcMuqOmsVoNAn_6ykx0lcY9f7Ek8kZHeYwBseMTyQ9WVYWwQW3WcRXB8nP02qDTwYji1puGovR8srEQLfayvMmTSlIIoPRX4F2zzX11QFUAxXZK/s640/9237-Music-room-Herschel-House.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US"> The music room, Herschel House, Bath, England, August 12, 2013.</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US"><a href="http://pt.wikipedia.org/wiki/Sir" style="color: #274e13; text-decoration: none;" title="Sir">Sir</a> <b>William Herschel</b></span><o:p></o:p></span></div>
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<tr><td class="tr-caption" style="font-size: 13px;"><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="color: #274e13; text-decoration: none;"><span lang="PT-BR"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">http://pt.wikipedia.org/wiki/William_Herschel</span></span></a></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><a href="http://en.wikipedia.org/wiki/Lemuel_Francis_Abbott" style="color: #274e13; text-decoration: none;">Lemuel Francis Abbott</a> (1760–1802) </b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><a href="http://en.wikipedia.org/wiki/William_Herschel" style="color: #274e13; text-decoration: none;"><span lang="EN-US">William Herschel</span></a></i><i><span lang="EN-US">, German-British astronomer.</span></i><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1785<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Óleo sobre tela<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">76.2 × 63.5 cm<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><a href="http://pt.wikipedia.org/wiki/National_Portrait_Gallery" style="color: #274e13; text-decoration: none;">National Portrait Gallery</a> </b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US"><a href="http://pt.wikipedia.org/wiki/Sir" style="color: #274e13; text-decoration: none;" title="Sir"><span lang="PT-BR">Sir</span></a></span> <b>William Herschel</b> (<span lang="EN-US"><a href="http://pt.wikipedia.org/wiki/Han%C3%B4ver" style="color: #274e13; text-decoration: none;" title="Hanôver"><span lang="PT-BR">Hanôver</span></a></span>, <span lang="EN-US"><a href="http://pt.wikipedia.org/wiki/15_de_Novembro" style="color: #274e13; text-decoration: none;" title="15 de Novembro"><span lang="PT-BR">15 de Novembro</span></a></span> de <span lang="EN-US"><a href="http://pt.wikipedia.org/wiki/1738" style="color: #274e13; text-decoration: none;" title="1738"><span lang="PT-BR">1738</span></a></span> — <span lang="EN-US"><a href="http://pt.wikipedia.org/wiki/Slough" style="color: #274e13; text-decoration: none;" title="Slough"><span lang="PT-BR">Slough</span></a></span>, <span lang="EN-US"><a href="http://pt.wikipedia.org/wiki/25_de_Agosto" style="color: #274e13; text-decoration: none;" title="25 de Agosto"><span lang="PT-BR">25 de Agosto</span></a></span> de <span lang="EN-US"><a href="http://pt.wikipedia.org/wiki/1822" style="color: #274e13; text-decoration: none;" title="1822"><span lang="PT-BR">1822</span></a></span>) foi um <span lang="EN-US"><a href="http://pt.wikipedia.org/wiki/Astr%C3%B4nomo" style="color: #274e13; text-decoration: none;" title="Astrônomo"><span lang="PT-BR">astrônomo</span></a></span> e <span lang="EN-US"><a href="http://pt.wikipedia.org/wiki/Compositor" style="color: #274e13; text-decoration: none;" title="Compositor"><span lang="PT-BR">compositor</span></a></span> <span lang="EN-US"><a href="http://pt.wikipedia.org/wiki/Alemanha" style="color: #274e13; text-decoration: none;" title="Alemanha"><span lang="PT-BR">alemão</span></a></span> naturalizado inglês nascido na <span lang="EN-US"><a href="http://pt.wikipedia.org/wiki/Alemanha" style="color: #274e13; text-decoration: none;" title="Alemanha"><span lang="PT-BR">Alemanha</span></a></span>. Aos 19 anos mudou-se para a <span lang="EN-US"><a href="http://pt.wikipedia.org/wiki/Inglaterra" style="color: #274e13; text-decoration: none;" title="Inglaterra"><span lang="PT-BR">Inglaterra</span></a></span> onde passou a ensinar música, antes de se tornar um organista. Com o tempo passou a estudar astronomia e ficou famoso por sua descoberta do planeta <span lang="EN-US"><a href="http://pt.wikipedia.org/wiki/Urano_(planeta)" style="color: #274e13; text-decoration: none;" title="Urano (planeta)"><span lang="PT-BR">Urano</span></a></span>, assim como de duas de suas luas (<span lang="EN-US"><a href="http://pt.wikipedia.org/wiki/Titania" style="color: #274e13; text-decoration: none;" title="Titania"><span lang="PT-BR">Titania</span></a></span> e <span lang="EN-US"><a href="http://pt.wikipedia.org/wiki/Oberon" style="color: #274e13; text-decoration: none;" title="Oberon"><span lang="PT-BR">Oberon</span></a></span>), ele também descobriu duas luas de <span lang="EN-US"><a href="http://pt.wikipedia.org/wiki/Saturno_(planeta)" style="color: #274e13; text-decoration: none;" title="Saturno (planeta)"><span lang="PT-BR">Saturno</span></a></span> e a existência da <span lang="EN-US"><a href="http://pt.wikipedia.org/wiki/Radia%C3%A7%C3%A3o_infravermelha" style="color: #274e13; text-decoration: none;" title="Radiação infravermelha"><span lang="PT-BR">radiação infravermelha</span></a></span>. Ele é também conhecido pelas vinte e quatro <span lang="EN-US"><a href="http://pt.wikipedia.org/wiki/Sinfonias" style="color: #274e13; text-decoration: none;" title="Sinfonias"><span lang="PT-BR">sinfonias</span></a></span> que compôs.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sua casa em Bath, onde ele fez inúmeros telescópios e observou Urano pela primeira vez, abriga atualmente o <a href="http://pt.wikipedia.org/w/index.php?title=Museu_de_Astronomia_Herschel&action=edit&redlink=1" style="color: #274e13; text-decoration: none;" title="Museu de Astronomia Herschel (página não existe)">Museu de Astronomia Herschel</a>.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LEIA MAIS SOBRE SIR WILLIAM HERSCHEL:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US"><span lang="PT-BR"><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/William_Herschel</a></span></span><o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US"><br /></span></span><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Em Tempo e sobre a imagem acima</b>: </span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">Minha citação sobre Sir William Herschel se deve ao fato de sua importância na Astronomia </span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">e no uso eficaz de um telescópio. </span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">No entanto, no passado e depois considerada obsoleta, </span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">houve a Constelação em sua honra:</span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US"> </span><span style="line-height: 18px;">Telescopium Herschell, o Telescópio de Herschell</span></span><br />
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">Constelação formada pelo Abade Hell em 1781,</span></span><br />
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"> em honra a Sir William Herschell (o descobridor de Urano).</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal;">http://www.stellarium.org/pt/</span></div>
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<span lang="EN-US" style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> </span><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>TELESCOPIUM, O TELESCÓPIO</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 18h6m / 20h26m Declinação -45<sup>o</sup>.4 / -56<sup>o</sup>.9<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelação formada por La Caille, em 1752.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É uma constelação rodeada pela Corona Australis, por Ara, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Pavo (sua estrela Alpha, Peacock, faz fronteira com o Telescópio, realmente),</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Indus e Sagittarius. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As três estrelas mais proeminentes aparecem bem próximas à fronteira com a Coroa Austral.<o:p></o:p></span></div>
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<b style="color: rgb(204, 0, 0) !important; text-decoration: none;"><b style="font-size: 12.8000001907349px;"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/home.html" style="color: rgb(204, 0, 0) !important; text-decoration: none;" target="index">by </a></b></b></div>
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<b style="color: rgb(204, 0, 0) !important; text-decoration: none;"><b style="font-size: 12.8000001907349px;"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/home.html" style="color: rgb(204, 0, 0) !important; text-decoration: none;" target="index"><span class="larger" style="font-size: 17.9200000762939px;">Richard Hinckley Allen </span></a></b></b></div>
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<span style="font-size: 12.8000001907349px;">as reprinted</span><span style="font-size: 12.8000001907349px;"> </span></div>
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<span style="font-size: 12.8000001907349px;">in the Dover edition, 1963</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Telescopium, or Tubus Astronomicus,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">was formed by La Caille between Ara and Sagittarius on the edge of the Milky Way, but in such irregular form that it encroached upon four of the old constellations; η Sagittarii having been taken as β to mark the Telescope's stand; d Ophiuchi for its θ; σ was in Corona Australis; and γ was the υ of Scorpio. Bode had it in his Gestirne of 1805 as the Astronomische Fernrohr, crowding it in between Sagittarius and Scorpio; but Baily and Gould restricted it to the south of Scorpio, Sagittarius, and Corona Australis.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Gould assigned to it 87 naked-eye stars, the brightest a 3½‑magnitude.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Small as these are, two bore individual title s in Chinese astronomy; α being known as We, Danger; and γ as the mythological Chuen Shwo.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">The constellation culminates on the 13th of August, at the same time as Wega of the Lyre.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Telescopium</b> (Tel), o <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio">Telescópio</a>, é uma <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> do <a href="http://pt.wikipedia.org/wiki/Hemisf%C3%A9rio_celestial_sul" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hemisfério celestial sul">hemisfério celestial sul</a>. O genitivo, usado para formar nomes de estrelas, é <b>Telescopii</b>. É uma das 14 constelações criadas pelo <a href="http://pt.wikipedia.org/wiki/Astr%C3%B4nomo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Astrônomo">astrônomo</a> <a class="mw-disambig" href="http://pt.wikipedia.org/wiki/Franc%C3%AAs" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Francês">francês</a> <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a> no século XVIII.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">As constelações vizinhas são <a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagittarius</a>, <a href="http://pt.wikipedia.org/wiki/Corona_Australis" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Corona Australis">Corona Australis</a>, <a href="http://pt.wikipedia.org/wiki/Ara" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ara">Ara</a>, <a href="http://pt.wikipedia.org/wiki/Pavo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pavo">Pavo</a> e <a href="http://pt.wikipedia.org/wiki/Indus" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Indus">Indus</a>.</span></div>
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A constelação Telescopium foi apresentada por volta de <a href="http://pt.wikipedia.org/wiki/1751" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1751">1751</a> por <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a> com o nome em <a href="http://pt.wikipedia.org/wiki/L%C3%ADngua_francesa" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Língua francesa">francês</a> <i>le telescope</i>, representando um <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_a%C3%A9reo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio aéreo">telescópio aéreo</a>. Ela se alonga na direção norte entre <a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagittarius</a> e <a href="http://pt.wikipedia.org/wiki/Scorpius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Scorpius">Scorpius</a><span class="reference" id="cite_ref-FOOTNOTERidpath.2C_.27.27Star_Tales.27.27_Telescopium_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Telescopium#cite_note-FOOTNOTERidpath.2C_.27.27Star_Tales.27.27_Telescopium-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> . <a href="http://pt.wikipedia.org/wiki/Johann_Elert_Bode" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Johann Elert Bode">Johann Bode</a> a denominou <i>Astronomische Fernrohr</i> em <a href="http://pt.wikipedia.org/wiki/1805" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1805">1805</a> em sua obra <i>Gestirne</i> e manteve seu tamanho, mas Baily e Gould reduziram seus limiares<span class="reference" id="cite_ref-FOOTNOTEAllen1963414_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Telescopium#cite_note-FOOTNOTEAllen1963414-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> . A constelação já reduzida perdeu outras estrelas brilhantes para as constelações vizinhas: Beta telescopii se tornou<a href="http://pt.wikipedia.org/wiki/Eta_Sagittarii" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Eta Sagittarii">Eta Sagittarii</a><span class="reference" id="cite_ref-FOOTNOTEStaal1988233_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Telescopium#cite_note-FOOTNOTEStaal1988233-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> , onde já estava antes de Lacaille colocá-la na constelação<span class="reference" id="cite_ref-FOOTNOTEWagman2003300_4-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Telescopium#cite_note-FOOTNOTEWagman2003300-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> . Gamma telescopii retornou ao seu antigo nome de<a href="http://pt.wikipedia.org/wiki/45_Ophiuchi" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="45 Ophiuchi">45 Ophiuchi</a><span class="reference" id="cite_ref-FOOTNOTEWagman2003300_4-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Telescopium#cite_note-FOOTNOTEWagman2003300-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> , e sigma telescopii foi colocado na constelação <a href="http://pt.wikipedia.org/wiki/Corona_Australis" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Corona Australis">Corona Australis</a>. Anteriormente esta estrela não possuía nome, mas agora é conhecida como HR 6875<span class="reference" id="cite_ref-FOOTNOTEWagman2003300_4-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Telescopium#cite_note-FOOTNOTEWagman2003300-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> .</div>
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Telescopium foi constantemente chamada "Tubus Astronomicus", entretanto este nome agora é obsoleto<span class="reference" id="cite_ref-FOOTNOTEStaal1988233_3-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Telescopium#cite_note-FOOTNOTEStaal1988233-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> .</div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg6aQFK7PSE55emTm2brPWBX7MKiZ-Hk9J3oTU7urG4mGbn6dqJ3c2Ry9FawNbWTr_usZy_-chFkAiHgAnvRBu21bUeB5KJIJkewR1bwiPZrgk9IDjU4plQadDS-M0CO_Zr_t5F0CBYzJE/s1600/a+tel.png" imageanchor="1" style="clear: left; float: left; margin-bottom: 1em; margin-right: 1em; text-align: center;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg6aQFK7PSE55emTm2brPWBX7MKiZ-Hk9J3oTU7urG4mGbn6dqJ3c2Ry9FawNbWTr_usZy_-chFkAiHgAnvRBu21bUeB5KJIJkewR1bwiPZrgk9IDjU4plQadDS-M0CO_Zr_t5F0CBYzJE/s1600/a+tel.png" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Stellarium</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Alpha Telescopii</b> (α Tel, α Telescopii) é a <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a> mais brilhante na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Telescopium" style="background: none; color: #0b0080; text-decoration: none;" title="Telescopium">Telescopium</a>, com uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 3,48.<span class="reference" id="cite_ref-simbad_1-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Telescopii#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ptolomeu" style="background: none; color: #0b0080; text-decoration: none;" title="Ptolomeu">Ptolomeu</a> originalmente a incluiu na constelação de <a href="http://pt.wikipedia.org/wiki/Corona_Australis" style="background: none; color: #0b0080; text-decoration: none;" title="Corona Australis">Corona Australis</a>, mas ela foi movida para Telescopium quando a constelação foi criada por <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background: none; color: #0b0080; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a> no <a href="http://pt.wikipedia.org/wiki/S%C3%A9culo_XVIII" style="background: none; color: #0b0080; text-decoration: none;" title="Século XVIII">século XVIII</a>.<span class="reference" id="cite_ref-ridpath_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Telescopii#cite_note-ridpath-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> Com base em medições de <a href="http://pt.wikipedia.org/wiki/Paralaxe" style="background: none; color: #0b0080; text-decoration: none;" title="Paralaxe">paralaxe</a>, está localizada a aproximadamente 278 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (85 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">parsecs</a>) da Terra.<span class="reference" id="cite_ref-simbad_1-10" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Telescopii#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Alpha Telescopii é bem maior que o <a href="http://pt.wikipedia.org/wiki/Sol" style="background: none; color: #0b0080; text-decoration: none;" title="Sol">Sol</a>, com cerca de cinco vezes a <a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Massa solar">massa</a> e três vezes o <a href="http://pt.wikipedia.org/wiki/Raio_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Raio solar">raio solar</a>.<span class="reference" id="cite_ref-an330_4_317_3-7" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Telescopii#cite_note-an330_4_317-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> Seu espectro corresponde a uma <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">classificação estelar</a> de B3 IV,<span class="reference" id="cite_ref-simbad_1-11" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Telescopii#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> onde a classe de luminosidade 'IV' indica que é uma <a href="http://pt.wikipedia.org/wiki/Estrela_subgigante" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela subgigante">estrela subgigante</a> que consumiu praticamente todo o hidrogênio de seu núcleo e está saindo da<a href="http://pt.wikipedia.org/wiki/Sequ%C3%AAncia_principal" style="background: none; color: #0b0080; text-decoration: none;" title="Sequência principal">sequência principal</a>. É uma estrela brilhante, com 800 vezes a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Luminosidade_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Luminosidade solar">luminosidade solar</a>. Essa energia está sendo irradiada da atmosfera externa a uma <a href="http://pt.wikipedia.org/wiki/Temperatura_efetiva" style="background: none; color: #0b0080; text-decoration: none;" title="Temperatura efetiva">temperatura efetiva</a>de 16 700 <a href="http://pt.wikipedia.org/wiki/Kelvin" style="background: none; color: #0b0080; text-decoration: none;" title="Kelvin">K</a>,<span class="reference" id="cite_ref-an330_4_317_3-8" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Telescopii#cite_note-an330_4_317-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> o que lhe dá o brilho azul-branco típico de estrelas de classe B.<span class="reference" id="cite_ref-csiro_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Telescopii#cite_note-csiro-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span> É também uma <a href="http://pt.wikipedia.org/wiki/Estrela_peculiar" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela peculiar">estrela quimicamente peculiar</a> que apresenta altas quantidades de<a href="http://pt.wikipedia.org/wiki/H%C3%A9lio" style="background: none; color: #0b0080; text-decoration: none;" title="Hélio">hélio</a>.<span class="reference" id="cite_ref-stars_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Telescopii#cite_note-stars-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Alpha Telescopii pertence a uma classe de <a href="http://pt.wikipedia.org/wiki/Estrela_vari%C3%A1vel" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela variável">estrelas variáveis</a> conhecida como estrelas B pulsantes lentas. Tem um <a href="http://pt.wikipedia.org/wiki/Campo_magn%C3%A9tico_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Campo magnético estelar">campo magnético</a> longitudinal com uma força média de <span style="white-space: nowrap;">–233 ± 43 <a href="http://pt.wikipedia.org/wiki/Gauss_(unidade)" style="background: none; color: #0b0080; text-decoration: none;" title="Gauss (unidade)">G</a></span> e uma <a href="http://pt.wikipedia.org/wiki/Rota%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Rotação estelar">velocidade de rotação projetada</a> de cerca de 14 km/s,<span class="reference" id="cite_ref-an330_4_317_3-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Telescopii#cite_note-an330_4_317-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> considerada baixa para uma estrela desse tipo, o que sugere que a estrela está com o polo virado para a Terra.<span class="reference" id="cite_ref-stars_7-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Alpha_Telescopii#cite_note-stars-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span></span></div>
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Stellarium</div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Zeta Telescopii</b> (ζ Tel / ζ Telescopii) é a segunda <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a> mais brilhante da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Telescopium" style="background: none; color: #0b0080; text-decoration: none;" title="Telescopium">Telescopium</a>.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Zeta Telescopii é uma <a href="http://pt.wikipedia.org/wiki/Estrela_gigante" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela gigante">estrela gigante</a> de <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">classe</a> K com <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 4,13. Está a cerca de 127 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>.</span></div>
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<span style="color: #252525; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Zeta_Telescopii</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhn2s0pafKdk4FW-yhdVRc6bqGWFSwyreWP79MerK1aMJa95J6ou9AJx50YsYPnOANSnjdyU_iEbzlqBAoYkcCiVyJmuAp7IGu2qriOZ0pdZMVgqYw2R_pJBOyzYoS8yGlij4bZvDcNdJI/s1600/2+w+1+tel.png" imageanchor="1" style="clear: left; float: left; margin-bottom: 1em; margin-right: 1em; text-align: center;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhn2s0pafKdk4FW-yhdVRc6bqGWFSwyreWP79MerK1aMJa95J6ou9AJx50YsYPnOANSnjdyU_iEbzlqBAoYkcCiVyJmuAp7IGu2qriOZ0pdZMVgqYw2R_pJBOyzYoS8yGlij4bZvDcNdJI/s1600/2+w+1+tel.png" /></a></div>
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Stellarium</div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Delta<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">1</span> Telescopii</b> (δ<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">1</span> Tel / δ<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">1</span> Telescopii) é uma <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a> <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Bin%C3%A1ria_espectrosc%C3%B3pica" style="background: none; color: #0b0080; text-decoration: none;" title="Binária espectroscópica">binária espectroscópica</a> localizada na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Telescopium" style="background: none; color: #0b0080; text-decoration: none;" title="Telescopium">Telescopium</a>.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Delta<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">1</span> Telescopii é uma <a href="http://pt.wikipedia.org/wiki/Estrela_subgigante" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela subgigante">subgigante</a> de <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">classe</a> B com <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 4,916. Está a cerca de 800 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>.</span></div>
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<span style="color: #252525; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Delta1_Telescopii</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b style="color: #252525; line-height: 22.3999996185303px;">Delta<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">2</span> Telescopii</b><span style="color: #252525; line-height: 22.3999996185303px;"> (17 Telescopii) é uma </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Estrela">estrela</a><span style="color: #252525; line-height: 22.3999996185303px;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Constelação">constelação</a><span style="color: #252525; line-height: 22.3999996185303px;"> de </span><a href="http://pt.wikipedia.org/wiki/Telescopium" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Telescopium">Telescopium</a><span style="color: #252525; line-height: 22.3999996185303px;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="color: #252525; line-height: 22.3999996185303px;"> de 18h 32m 01.94s e uma </span><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Declinação">declinação</a><span style="color: #252525; line-height: 22.3999996185303px;"> de −45° 45′ 26.5″. Sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525; line-height: 22.3999996185303px;"> é igual a 5.07. Considerando sua distância de 1116 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="color: #252525; line-height: 22.3999996185303px;"> em relação à </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Terra">Terra</a><span style="color: #252525; line-height: 22.3999996185303px;">, sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a><span style="color: #252525; line-height: 22.3999996185303px;"> é igual a −2.60. Pertence à </span><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Classificação estelar">classe espectral</a><span style="color: #252525; line-height: 22.3999996185303px;"> B3III.</span></span></div>
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<span style="color: #252525; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Delta2_Telescopii</span></span></div>
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<img alt="Telescopium constellation map.png" src="http://upload.wikimedia.org/wikipedia/commons/thumb/2/21/Telescopium_constellation_map.png/800px-Telescopium_constellation_map.png" height="557" width="640" /></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">"Telescopium constellation map". Licenciado sob CC BY-SA 3.0, via Wikimedia Commons - http://commons.wikimedia.org/wiki/File:Telescopium_constellation_map.png#/media/File:Telescopium_constellation_map.png</span></span></div>
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">NGC 6584</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Telescopium" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Telescopium">constelação de Telescopium</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/James_Dunlop" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="James Dunlop">James Dunlop</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> em 1826, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">refletor com abertura de 9 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> (+7,9), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> amadores ou com equipamentos superiores.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_6584</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">http://archive.stsci.edu/cgi-bin/dss_search?e=J2000&c=none&h=10&w=10&f=GIF&r=274.65705937847736&d=-52.21501896898023&v=all</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">http://www.messier45.com/index.html#s/NGC_6584</span><br />
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<b>NGC 6868</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_el%C3%ADptica" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia elíptica">elíptica</a> (E2) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Telescopium" style="background: none; color: #0b0080; text-decoration: none;" title="Telescopium">Telescopium</a>. Possui uma declinação de -48° 22' 48" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 20 <a href="http://pt.wikipedia.org/wiki/Hora" style="background: none; color: #0b0080; text-decoration: none;" title="Hora">horas</a>, 09<a href="http://pt.wikipedia.org/wiki/Minuto" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto">minutos</a> e 54,0 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a>.</div>
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A galáxia <b>NGC 6868</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/7_de_Julho" style="background: none; color: #0b0080; text-decoration: none;" title="7 de Julho">7 de Julho</a> de <a href="http://pt.wikipedia.org/wiki/1834" style="background: none; color: #0b0080; text-decoration: none;" title="1834">1834</a> por <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background: none; color: #0b0080; text-decoration: none;" title="John Herschel">John Herschel</a>.</div>
<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_6868</span><br />
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://archive.stsci.edu/cgi-bin/dss_search?e=J2000&c=none&h=5&w=5&f=GIF&r=302.47587920546425&d=-48.37975407993353&v=all</span><br />
<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.messier45.com/index.html#s/_NGC_6868</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>IC 4699</b> est une <a href="http://fr.wikipedia.org/wiki/N%C3%A9buleuse_plan%C3%A9taire" style="background: none; color: #0b0080; text-decoration: none;" title="Nébuleuse planétaire">nébuleuse planétaire</a> dans la constellation du <a href="http://fr.wikipedia.org/wiki/T%C3%A9lescope_(constellation)" style="background: none; color: #0b0080; text-decoration: none;" title="Télescope (constellation)">Télescope</a>.</span></div>
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<li style="margin-bottom: 0.1em; text-align: left;"><span style="font-family: Arial, Helvetica, sans-serif;">Ascension droite 18h 14' 55"</span></li>
<li style="margin-bottom: 0.1em; text-align: left;"><span style="font-family: Arial, Helvetica, sans-serif;">Déclinaison - 46° 1'</span></li>
<li style="margin-bottom: 0.1em; text-align: left;"><span style="font-family: Arial, Helvetica, sans-serif;">Taille ?</span></li>
<li style="margin-bottom: 0.1em; text-align: left;"><span style="font-family: Arial, Helvetica, sans-serif;">Magnitude 11,9</span></li>
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<span style="font-family: Arial, Helvetica, sans-serif;">Nébuleuse planétaire visible dans l'hémisphère sud.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">La nébuleuse est située près de l'étoile alpha du Télescope, près de la limite avec les constellations Autel/Couronne Australe. Un télescope de 200 mm permet de voir cette nébuleuse. Attention toutefois à la proximité de l'étoile.</span></div>
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<span style="color: #252525; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;">http://fr.wikipedia.org/wiki/IC_4699</span></span></div>
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<tr><td class="tr-caption" style="font-size: 13px;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=19.2&declination=-50.1" style="color: #274e13; text-decoration: none;"><span style="background-color: white; color: #073763;">http://www.nightskyatlas.com/viewer.jsp?rightAscension=19.2&declination=-50.1</span></a></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Bath e Stonehenge, </span></h2>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Fátima e Janine</span></h2>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"> em gelado domingo do outono inglês, </span></h2>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">em 1986</span></h2>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Perdoem-me pelas fotos arranhadas pelo scanner -</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> fotos envelhecidas trabalhadas em scanner envelhecido... </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Eu sou a moçoila (aos meus 36 anos de idade) da direita,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> feliz e contente por estar em Stonehenge ao final de um domingo outonal,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> quando saímos cedinho de Londres </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">para tomar chá no campo, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">nos arredores de Bath.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="EN-US"> </span><span lang="EN-US"><o:p></o:p></span></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas – As Constelações - são como janelas que se abrem para a infinitude do universo e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e sendo por nossa mente conscientizado. Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>COM UM ABRAÇO ESTRELADO,<o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward<o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">REFERÊNCIAS BIBLIOGRÁFICAS:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">www.stellarium.org<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quase sempre, para as Constelações comentadas, em Ilustrações para a Latitude 21s52 e Longitude 43w00.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">English Astronomers: Stonehenge and Bath, England</span></h3>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="user-name"><a class="internal-link view-user-profile" href="http://cs.astronomy.com/members/David-Eicher/default.aspx" style="color: #274e13; outline: none; text-decoration: none;">David Eicher </a></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tue, Aug 13 2013</span></div>
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<a href="http://cs.astronomy.com/asy/b/daves-universe/archive/2013/08/13/english-astronomers-stonehenge-and-bath-england.aspx" style="color: #274e13; text-decoration: none;"></a><a href="http://cs.astronomy.com/asy/b/daves-universe/archive/2013/08/13/english-astronomers-stonehenge-and-bath-england.aspx" style="color: #274e13; text-decoration: none;">http://cs.astronomy.com/asy/b/daves-universe/archive/2013/08/13/english-astronomers-stonehenge-and-bath-england.aspx</a></div>
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<a href="http://pt.wikipedia.org/wiki/William_Herschel" style="color: #274e13; text-align: center; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/William_Herschel</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do <b>Atlas Celeste</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">de autoria de <b>Ronaldo Rogério de Freitas Mourão</b>,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(com dedicatória do próprio autor para mim<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em 16/06/1989)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- </span><b>Mario Jaci Monteiro</b> , <b>As Constelações, Cartas Celestes</b> -<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC - com dedicatória do autor para mim, em março de 2004 (quando Mário Jaci generosamente me presenteou com um instrumento de observação (kepleriano) artesanalmente construído por ele).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas – As Constelações - são como janelas que se abrem para a infinitude do universo e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e sendo por nossa mente conscientizado. Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>COM UM ABRAÇO ESTRELADO,<o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward<o:p></o:p></b></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-61451372247906801782013-08-20T08:23:00.002-07:002014-12-04T07:52:46.271-08:00TAURUS, O TOURO<div align="center" class="MsoNormal" style="text-align: center;">
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px; text-align: start;">Meu Projeto</span></div>
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="font-size: large;">Da Terra ao Céu ....</span></span></a></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="font-size: large;">.....<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;">e ao Infinito </a></span></span></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><span style="font-size: large;">- As 88 Constelações</span></a></span></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;">http://daterraaoceueaoinfinito.blogspot.com.br/</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A constelação do Touro é imensa</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- mesmo que seja figurado somente a partir de sua metade dianteira,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">incluindo peito e coração, patas dianteiras e cabeça e chifres.</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A Lua demora cerca de três dias para bem realizar seu passeio através o Touro,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">começando por seu abraço às Pleiades, as irmãs que choram,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">depois mergulhando nas Hyades e cumprimentando a belíssima Aldebaran, estrela-alpha Tauri,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">finalizando ao roçar um dos chifres do Touro,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">de um lado a maravilhosa M 1, a Nebulosa do Caranguejo,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e, de outro lado, El Nath, estrela-beta Tauri.</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Estaremos também nós nos sentindo como se a Lua fôssemos</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e visitando o Touro em três partes acima comentadas.</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,<br />Janine Milward</span><br />
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/enlarge/37703</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.raremaps.com/gallery/detail/37703/The_January_February_and_March_S" style="color: #274e13; text-decoration: none;">http://www.raremaps.com/gallery/detail/37703/The_January_February_and_March_S</a>ky_Cancer_Perseus_Gemini_Taurus/Burritt.html</span></div>
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<span style="color: white; font-family: verdana, arial, georgia, sans-serif; text-align: start;">Map Maker: </span><span style="color: white; font-family: verdana, arial, georgia, sans-serif; text-align: start;"></span><a href="https://www.raremaps.com/gallery/browse/creator_id/808" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: white; font-family: verdana, arial, georgia, sans-serif; text-align: start; text-decoration: none;">Elijah J. Burritt</a></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"> Mario Jaci Monteiro - Cartas Celestes, As Constelações - CARJ</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">TAURUS, O TOURO</span></b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 3h20m / 5h58m Declinação +0<sup>o</sup>.1 / +30<sup>o</sup>.9<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">Mito:</span></b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Júpiter ansiava por encontrar-se com Europa. </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">Certa vez, disfarçou-se em touro e fez parte de uma manada </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">até encontrar-se com a moça, numa praia. </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">Europa sentiu-se encorajada com a placidez do touro</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> e montou-o </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">e foi quando Júpiter correu para o mar </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">e levou a moça até a ilha de Creta. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">De acordo com outro mito, </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">o touro representa Io </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">a quem Júpiter transformou em vaca, </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">para despistar o ciúme e a vigilância de Juno, sua mulher.<o:p></o:p></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://www.theoi.com/Gallery/K1.8.html</span></div>
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<span style="color: #274e13;">K1.8 EUROPA & THE BULL</span></div>
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<span style="color: #274e13;"><span class="details">Museum Collection:</span> Kunst-historiches Museum, Vienna, Austria </span></div>
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<span style="color: #274e13;"><span class="details">Museum Catalogue No.:</span> TBA </span><span class="details" style="color: #274e13;">Beazley Archive No.:</span><span style="color: #274e13;"> N/A </span></div>
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<span style="color: #274e13;"><span class="details">Ware:</span> Apulian Red Figure </span><span class="details" style="color: #274e13;">Shape:</span><span style="color: #274e13;"> Kylix </span></div>
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<span style="color: #274e13;"><span class="details">Painter:</span> -- </span><span class="details" style="color: #274e13;">Date:</span><span style="color: #274e13;"> ca 330 - 320 BC </span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span class="details">Period:</span> Late Classical</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">Algumas Informações Interessantes acerca esta Constelação:</span></b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A mais antiga de todas as constelações e talvez a primeira a ser delimitada pelos babilônios, que a utilizaram para marcar o início do ano, pois o equinócio da primavera, há 4000 AC, localizava-se neste asterismo. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> Aliás, o estudo de todos os antigos zodíacos mostram o seu início no Touro: o ano começava com o aparecer matinal das Pleiades na primavera, e o inverno, com o seu aparecimento vespertino no outono. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">O aparecimento das Pleiades em novembro era saudado como a festa dos mortos, que comemoramos até hoje. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Povos da antiguidade, como os caldeus e hebreus, davam ao mês de novembro o nome de Pleiades.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">No mais antigo de todos os zodíacos egípcios - o de Denderah -, a constelação do Touro está associada a Osíris, que era o deus especial do Nilo.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">O nascer helíaco das Hyades, principal aglomerado do Touro, era associado à estação da chuva - donde a origem do seu nome, que significava ‘chover’.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Fronteiras:</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Taurus situa-se entre as constelações de Gemini, Auriga, Perseus, Áries, Cetus, Eridanus e Orion<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://upload.wikimedia.org/wikipedia/commons/4/4e/Pleiades_large.jpg</span></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Origem</span></td><td><a class="external free" href="http://hubblesite.org/newscenter/archive/releases/2004/20/image/a/" rel="nofollow" style="color: #274e13; text-decoration: none;"><span style="font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/2004/20/image/a/</span></a></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Autor</span></td><td><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">NASA, ESA, AURA/Caltech, Palomar Observatory<br /><span style="height: 0px; line-height: 1; position: relative; top: 0.5ex; vertical-align: baseline;">The science team consists of: D. Soderblom and E. Nelan (STScI), F. Benedict and B. Arthur (U. Texas), and B. Jones (Lick Obs.)</span></span></td></tr>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">AS PLEIADES</span></b></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">As Pleiades sempre me parecem figurar um tercinho, algo assim,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">composto de estrelinhas bem delicadas, sutis, quase inefáveis,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e que somente se apresentam em lugares de céus mais escuros e transparentes.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando em noites de ausência de Lua</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e em lugares de céus escuros e transparentes,</span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">as Pleiades ganham luminosidade, </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">surgem de onde estiveram escondidas</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e se apresentam magnificamente</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e sempre nos emocionam muitíssimo,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">nos trazendo o desejo de podermos rezar em suas continhas de terço celeste!</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 22.399999618530273px;">As Pleiades formam um aglomerado, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 22.399999618530273px;">com Alcyone como estrela principal, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 22.399999618530273px;">estrela situada no ombro do Touro.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> http://www.stellarium.org/pt/</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> http://www.stellarium.org/pt/</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> Mario Jaci Monteiro - Cartas Celestes, As Constelações (excerto) - CARJ</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif; font-size: small;"><b>Pleiades - M45</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Distância: cerca de 350 anos-luz.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Aglomerado de mais de 400 estrelas</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> em uma área de um grau de diâmetro</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> e facilmente visível a olho nu.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>As Pleiades ou Atlântidas eram as sete filhas de Atlas e Pleione, </b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b>seis das quais podem ser vistas a olho nu e uma invisível ou “perdida”. </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Elas eram as companheiras virgens de Diana </b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b>e foram levadas para o céu </b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b>para escaparem do Gigante Orion que as importunava. </b></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiT7ARlRqzmX4pEZThmf5Rcn8Hty9NkanxYvTbpacQKVSTIEcHLTKVuxo2HXk0CJxh1LjvdJIFPQxKpZVfXSpILL69Bz_FDTdrSPJyNdkz9XKzh0ygy5I3WzKvWMgqzx8EY02YlRNYtZ8I/s1600/%D0%94%D1%80%D0%B5%D0%B2%D0%BD%D0%B8%D0%B5_%D1%81%D0%BE%D0%B7%D0%B2%D0%B5%D0%B7%D0%B4%D0%B8%D1%8F_%D0%BD%D0%B0%D0%B4_%D1%82%D0%B5%D0%BB%D0%B5%D1%81%D0%BA%D0%BE%D0%BF%D0%BE%D0%BC_ALMA.jpg" imageanchor="1" style="clear: left; color: #274e13; float: left; margin-bottom: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiT7ARlRqzmX4pEZThmf5Rcn8Hty9NkanxYvTbpacQKVSTIEcHLTKVuxo2HXk0CJxh1LjvdJIFPQxKpZVfXSpILL69Bz_FDTdrSPJyNdkz9XKzh0ygy5I3WzKvWMgqzx8EY02YlRNYtZ8I/s1600/%D0%94%D1%80%D0%B5%D0%B2%D0%BD%D0%B8%D0%B5_%D1%81%D0%BE%D0%B7%D0%B2%D0%B5%D0%B7%D0%B4%D0%B8%D1%8F_%D0%BD%D0%B0%D0%B4_%D1%82%D0%B5%D0%BB%D0%B5%D1%81%D0%BA%D0%BE%D0%BF%D0%BE%D0%BC_ALMA.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<span style="font-size: 12px; line-height: 16.799999237060547px; margin: 0px; padding: 0px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://www.eso.org/public/images/potw1347a/</span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><strong style="margin: 0px; padding: 0px;">Credit: </strong><span style="line-height: 1.4em;">ESO/B. Tafreshi (</span><a href="http://www.twanight.org/tafreshi" style="background-image: url(http://www.eso.org/public/archives/app/i/ext_link2.e3e6349c34f8.gif); background-position: 0% 50%; background-repeat: no-repeat; color: #274e13; line-height: 1.4em; margin: 0px; padding-bottom: 0px; padding-left: 12px !important; padding-right: 0px; padding-top: 0px; text-decoration: none;">twanight.org</a><span style="line-height: 1.4em;">)</span></span></div>
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<span style="line-height: 19.200000762939453px; text-align: start;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Babak Tafreshi, one of the ESO Photo Ambassadors, has captured the antennas of the Atacama Large Millimeter/submillimeter Array (ALMA) in an enthralling image combining the beauty of the southern sky with the amazing dimensions of the biggest astronomical project in the world.</span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Thousands of stars are revealed to the naked eye in the clear skies over the Chajnantor Plateau. Its dry and transparent night sky is one of the reasons ALMA has been built here. Surprisingly bright in the upper left corner of the picture, there is a tightly packed bunch of young stars, the Pleiades Cluster, which was already known to most ancient civilisations. The constellation of Orion (The Hunter) is clearly visible over the closest of the antennas — the hunter’s belt is formed by the three blue stars just to the left of the red light. According to classic mythology, Orion was a hunter who chased the Pleiades, the beautiful daughters of Atlas. When seen through the thin atmosphere over the Atacama, it almost seems that this epic hunt is really happening.</span></div>
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<b style="color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: 12px; line-height: 16.799999237060547px;">http://www.eso.org/public/images/potw1347a/</b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(Minha humilde tradução literal para o texto explicativo acima acerca esta belíssima imagem realizada por Babak Tafreshi)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Milhares de estrelas nos são apresentadas a olho nu nos céus límpidos do Plateau Chajnantor. O céu noturno seco e transparente é uma das razões pelas quais ALMA foi ali construído. Surpreendentemente iluminado no canto esquerdo ao alto da foto encontra-se um aglomerado de estrelas jovens bem compactadas, o Aglomerado das Pleiades (que também era conhecido nas antigas civilizações). A constelação de Orion (O Caçador) é claramente visível e bem próximo às antenas - o Cinturão do Caçador sendo formado peles três estrelas azuladas bem à esquerda da luz vermelha. De acordo com a mitologia clássica, Orion era um caçador que buscava alcançar as Pleiades, as belas filhas de Atlas. Quando visto através a atmosfera delicada do Atacama, nos parece que esse épico de caçada está realmente acontecendo.</span><br />
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif; text-align: -webkit-left;">Atlas holding the sky. 7201: Atlante sostiene la volta celeste 2C AD. Collezione Farnese. National Archaeological Museum, Naples. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>De acordo com outro mito, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>as Pleiades foram para o céu por causa de suas tristezas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> com o destino de seu pai, Atlas, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>que carregava o mundo nas costas.</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;"><img src="http://www.observatorio.ufmg.br/pleiades.JPG" height="528" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="640" /></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #274e13;">http://www.observatorio.ufmg.br/dicas10.htm</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os nomes das Irmãs que Choram e de seus pais são:<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Alcyone, Maia, Electra, Merope, Taygette, Celaeno e Sterope,<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>com a adição dos pais, Atlas e Pleione.</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A Plêiade que se perdeu parece ser Merope, que casou-se com um mortal, Sisyplus, </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">e por isso escondeu-se</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> por ser a única filha que não foi casada com um deus. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Outro mito diz que foi Electra quem desapareceu</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> em função de sua dor pela destruição de Ilium, </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">que foi fundada por seu filho Dardanos.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>As Pleiades formam um aglomerado, com Alcyone como estrela principal, situado no ombro do Touro.</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span class="mw-headline" id="Estrelas_mais_brilhantes"><span style="font-size: large;">Estrelas mais brilhantes</span></span></h2>
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As nove estrelas mais brilhantes nas Plêiades tem os nomes das <a href="http://pt.wikipedia.org/wiki/Pl%C3%AAiades_(mitologia)" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Plêiades (mitologia)">Sete Irmãs</a> da <a href="http://pt.wikipedia.org/wiki/Mitologia_grega" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Mitologia grega">mitologia grega</a>: <a href="http://pt.wikipedia.org/wiki/Asterope" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Asterope">Asterope</a>, <a href="http://pt.wikipedia.org/wiki/M%C3%A9rope" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Mérope">Mérope</a>, <a href="http://pt.wikipedia.org/wiki/Electra_(filha_de_Atlas)" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Electra (filha de Atlas)">Electra</a>, <a href="http://pt.wikipedia.org/wiki/Celeno" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Celeno">Celeno</a>, <a href="http://pt.wikipedia.org/wiki/Taigete" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Taigete">Taigete</a>, <a href="http://pt.wikipedia.org/wiki/Maia_(mitologia)" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Maia (mitologia)">Maia</a> e <a href="http://pt.wikipedia.org/wiki/Dr%C3%ADope" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Dríope">Dríope</a>, junto com seus pais, <a href="http://pt.wikipedia.org/wiki/Atlas_(mitologia)" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Atlas (mitologia)">Atlas</a> e <a href="http://pt.wikipedia.org/wiki/Pleione" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pleione">Pleione</a>. Como filhas de Atlas, as <a href="http://pt.wikipedia.org/wiki/H%C3%ADades" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Híades">híades</a> eram irmãs das Plêiades. O nome do aglomerado é em si de origem <a href="http://pt.wikipedia.org/wiki/Gr%C3%A9cia" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Grécia">grega</a>, apesar da etimologia não estar clara. Algumas derivações incluem: de πλεîν <i>plein</i>, navegar, fazendo das Plêiades "as navegantes"; de <i>pleos</i>, cheio ou muitos; ou então de <i>peleiades</i>, bando de pombas. A seguinte tabela dá detalhes das estrelas mais brilhantes no aglomerado:</div>
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<tr><td>Estrela</td><td>Designação</td><td>longitude em 2000</td><td>classe espectral</td></tr>
<tr><td><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Electra_(estrela)&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Electra (estrela) (página não existe)">Electra</a></td><td>17 Tauri</td><td>29TAU25</td><td>B5</td></tr>
<tr><td><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Celeno_(estrela)&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Celeno (estrela) (página não existe)">Celaeno</a></td><td>16 Tauri</td><td>29TAU26</td><td>B7</td></tr>
<tr><td><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Taigete_(estrela)&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Taigete (estrela) (página não existe)">Taygeta</a></td><td>19 Tauri</td><td>29TAU34</td><td>B7</td></tr>
<tr><td><a href="http://pt.wikipedia.org/wiki/Maia_(estrela)" style="background: none; color: #0b0080; text-decoration: none;" title="Maia (estrela)">Maia</a></td><td>20 Tauri</td><td>29TAU41</td><td>B9</td></tr>
<tr><td><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Merope_(estrela)&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Merope (estrela) (página não existe)">Merope</a></td><td>23 Tauri</td><td>29TAU42</td><td>B5</td></tr>
<tr><td><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Asterope_(estrela)&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Asterope (estrela) (página não existe)">Asterope</a></td><td>21 Tauri</td><td>29TAU44</td><td>B9</td></tr>
<tr><td><a href="http://pt.wikipedia.org/wiki/Alcyone_(estrela)" style="background: none; color: #0b0080; text-decoration: none;" title="Alcyone (estrela)">Alcyone</a></td><td>Eta (25) Tauri</td><td>00GEM00</td><td>B7</td></tr>
<tr><td align="center" colspan="4">Pais das Plêiades</td></tr>
<tr><td><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Atlas_(estrela)&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Atlas (estrela) (página não existe)">Atlas</a></td><td>27 Tauri</td><td>00GEM21</td><td>B9</td></tr>
<tr><td><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Pleione_(estrela)&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Pleione (estrela) (página não existe)">Pleione</a></td><td>28 (BU) Tauri</td><td>00GEM23</td><td>B8</td></tr>
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<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="line-height: 22.399999618530273px;"><br /></span></span><span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Pl%C3%AAiades</span></span><br />
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<img src="http://www.naic.edu/~gibson/pleiades/vedder/vedder_crop_light.jpg" height="395" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="640" /></div>
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F. E. Fillebrown engraving of <i>The Dance of the Pleiades</i> by Elihu Vedder</div>
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As <b>Plêiades</b> (<a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo Messier">Messier 45</a>) são um grupo de estrelas na constelação do <a href="http://pt.wikipedia.org/wiki/Taurus" style="background: none; color: #0b0080; text-decoration: none;" title="Taurus">Touro</a>. As Plêiades, também chamadas de <i>aglomerado estelar</i> (ou <i>aglomerado aberto</i>) <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo Messier">M45</a> são facilmente visíveis a olho nu nos dois hemisférios e consistem de várias <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a> brilhantes e quentes, de <a href="http://pt.wikipedia.org/wiki/Espectro" style="background: none; color: #0b0080; text-decoration: none;" title="Espectro">espectro</a> predominantemente azul. As Plêiades tem vários<a href="http://pt.wikipedia.org/wiki/Pl%C3%AAiades_no_folclore_e_literatura" style="background: none; color: #0b0080; text-decoration: none;" title="Plêiades no folclore e literatura">significados em diferentes culturas e tradições</a>.</div>
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O cluster é dominado por <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">estrelas azuis</a> quentes, que se formaram nos últimos 100 milhões de anos. Há uma <a href="http://pt.wikipedia.org/wiki/Nebulosa_de_reflex%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa de reflexão">nebulosa de reflexão</a> formada por poeira em torno das estrelas mais brilhantes que acreditava-se a princípio ter sido formado pelos restos da formação do cluster (por isto receberam o nome alternativo de <b>Nebulosa Maia</b>, da estrela<a href="http://pt.wikipedia.org/wiki/Maia_(estrela)" style="background: none; color: #0b0080; text-decoration: none;" title="Maia (estrela)">Maia</a>), mas hoje sabe-se que se trata de uma nuvem de poeira não relacionada ao aglomerado, no <a href="http://pt.wikipedia.org/wiki/Meio_interestelar" style="background: none; color: #0b0080; text-decoration: none;" title="Meio interestelar">meio interestelar</a> que as estrelas estão atravessando atualmente. Os astrônomos estimam que o cluster irá sobreviver por mais 250 milhões de anos, depois dos quais será dispersado devido a interações gravitacionais com a vizinhança galática.</div>
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<span class="mw-headline" id="Visualiza.C3.A7.C3.A3o">Visualização</span></h2>
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É um excelente objeto para a visualização, desde os mais simples <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Binóculo">binóculos</a> até os maiores <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a>, mostrando mais de 100 estrelas em um diâmetro aparente de cerca de 72 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto de arco">minuto de arco</a>. Contém inúmeras estrelas duplas ou múltiplas. A <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Nebulosa_de_M%C3%A9rope" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa de Mérope">nebulosa de Mérope</a>, em torno da estrela <a class="new" href="http://pt.wikipedia.org/w/index.php?title=M%C3%A9rope_(estrela)&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Mérope (estrela) (página não existe)">Mérope</a>, pode ser vista com <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a> amadores de 4 polegadas de abertura em um <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Céu noturno">céu noturno</a> de excelente qualidade.</div>
<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;">LEIA MAIS</span><br />
<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;">em</span><br />
<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="line-height: 22.399999618530273px;"><a href="http://pt.wikipedia.org/wiki/Pl%C3%AAiades" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Pl%C3%AAiades</a></span></span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgykBYcehc-U9ei65zyruX9wQqHx2ElwLTbmKjMq0qnzMc9unqRjMtW8p6o6Sc9PxkVebtiWLfIA5SprexR9oIDIsAzZmpoAjrB1ygkVAypc9BRBMUPj7y5a0lEpoNSLYgtHDYF_4zUIXM/s1600/pleiades.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgykBYcehc-U9ei65zyruX9wQqHx2ElwLTbmKjMq0qnzMc9unqRjMtW8p6o6Sc9PxkVebtiWLfIA5SprexR9oIDIsAzZmpoAjrB1ygkVAypc9BRBMUPj7y5a0lEpoNSLYgtHDYF_4zUIXM/s1600/pleiades.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium - As Pleiades aproximadas</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Quem não conhece As Pleiades?</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Mesmo em lugares de céus extremamente iluminados </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- assim como acontece nas cidades -,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">mesmo que esses moradores possam tão somente observar</span><span style="font-family: Arial, Helvetica, sans-serif;"> a olho nu </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Aldebaran, a estrela-alpha Tauri,</span><span style="font-family: Arial, Helvetica, sans-serif;">o Olho Iluminado do Touro; </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">mesmo que esses moradores jamais tenham visualizado As Pleiades....,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">mesmo assim e mesmo por tudo isso e com tudo isso, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">moradores das urbes e das roças e das florestas,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">todos já ouviram falar nas Pleiades!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Sempre o nome "Pleiades" nos faz lembrar da constelação do Touro, não é verdade?</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">No entanto, existe um outro conjunto estelar também denominado de Pleiades, você sabia?</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A bem da verdade, essa denominação acontece como Pleiades do Sul ou Pleiades Austrais.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">As Pleiades do Sul ou Austrais são um aglomerado aberto </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> conhecido como IC 2602</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e que vêm encantando de tal maneira a visão de quem as observa</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> (mesmo a olho nú e em lugares de céus escuros e transparentes!)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">que também recebeu o nome de "Diamantes Celestes"!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">As Pleiades do Sul moram bem pertinho (visualmente falando)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">da Grande Nebulosa em Carina, </span><span style="font-family: Arial, Helvetica, sans-serif;">a Quilha do Navio. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(Veja nossa Postagem acessando</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://oceudomes.blogspot.com/2014/05/a-grande-nebulosa-em-carina.html" style="color: #274e13; text-decoration: none;">http://oceudomes.blogspot.com/2014/05/a-grande-nebulosa-em-carina.html</a>)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Vemos, portanto,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">que existe </span><span style="font-family: Arial, Helvetica, sans-serif;">um lugar de maravilhas que podem ser visualizadas a olho nú,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">sempre em lugares de céus escuros e transparentes, é claro,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> um lugar fronteiriço entre as patas traseiras do Centauro</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- não nos esquecendo que o Cruzeiro do Sul situa-se entre as patas traseiras e dianteiras -</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e as partes que sobraram da Quilha e da Proa do Navio Argo</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(no mito, pedras desabaram sobre estas partes e as destruíram</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">e o Navio foi levado ao céu estrelado do sul carente de Proa -</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e isso será tema para outra conversa nossa!).</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><cite style="font-style: normal; line-height: 17px; text-align: start;" title="apod.nasa.gov"><br /></cite></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><cite style="font-style: normal; line-height: 17px; text-align: start;" title="apod.nasa.gov"><br /></cite></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><cite style="font-style: normal; line-height: 17px; text-align: start;" title="apod.nasa.gov">apod.nasa.gov</cite><br style="line-height: 17px; text-align: start;" /><span style="line-height: 17px; text-align: start;">Astronomy</span><span style="line-height: 17px; text-align: start;"> Picture of the </span><span style="line-height: 17px; text-align: start;">Day</span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">M45: The Pleiades Star Cluster </span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Credit & Copyright: <a href="mailto:%20roberto.colombari%20at%20techedgegroup%20dot%20com" style="color: #274e13; text-decoration: none;">Roberto Colombari</a></span></div>
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<span style="line-height: 17px; text-align: start;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://apod.nasa.gov/apod/ap130918.html</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">É sempre um imenso prazer visitarmos</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> a belíssima estrela-alpha Tauri, Aldebaran,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que <i>parece</i> fazer parte das Hyades, aglomerado em movimento do Touro</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- mas não faz. </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">É um pertencimento apenas aparente.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">De qualquer forma, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">eu penso que as Hyades parecem formar um triângulo</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- quase como se fosse uma árvore conífera -,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e Aldebaran vem enfeitar, em tons alaranjados,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> esse Aglomerado de estrelas como se uma brilhante gema fosse. </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">E é.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Aldebaran formava uma das quatro estrelas reais ou guardiãs dos céus </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">entre os persas cerca de 3.000 anos a.C, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">quando, enquanto Guardiã do leste, marcava o Equinócio Vernal </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- as outras estrelas eram Regulus, Antares e Fomalhaut.<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">As Hyades são o Aglomerado Aberto mais próximo ao nosso Sol </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e todas suas estrelas encontram-se em movimento em conjunto.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Aldebaran situa-se em cerca da metade do caminho entre o centro das Hyades e nosso Sol.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">No entanto, a olho nu, todo esse conjunto estelar que forma a cabeça do Touro</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é de uma beleza rara</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e sempre nos emociona</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- principalmente quando visitado pela Lua ou por algum Planeta.</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18.200000762939453px;"><b>O AGLOMERADO DAS HYADES </b></span></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18.200000762939453px;"><b>E </b></span></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18.200000762939453px;"><b>ALDEBARAN, GIGANTE VERMELHA, O OLHO ILUMINADO DO TOURO:</b></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="ES-TRAD"><b><span style="color: #660000;">Aldebaran</span></b></span><span lang="ES-TRAD"><b><span style="color: #660000;">. Alpha Tauri. </span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span lang="PT"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 04h34,8m - Declinação +16<sup>o</sup> 28’<o:p></o:p></span></span></div>
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<span lang="PT"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual 1,06 - Distância 68 anos-luz<o:p></o:p></span></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela gigante alaranjada marcando o olho esquerdo e sul do Touro. <o:p></o:p></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Seu nome advém de Al Dabaran, Aquela que Segue. Aquela que vem antes da Estrela da Água, isto é, das Pleiades. </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Formava uma das quatro estrelas reais ou guardiãs dos céus entre os persas cerca de 3.000 anos a.C, quando, enquanto Guardiã do leste, marcava o Equinócio Vernal - as outras estrelas eram Regulus, Antares e Fomalhaut.<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<span style="color: #660000;"><b>Alpha Tauri</b> (α Tau) conhecida como <b>Aldebarã</b> ou <b>Aldebaran</b></span><span style="color: #252525;"> é uma </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Estrela_de_primeira_magnitude&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Estrela de primeira magnitude (página não existe)">estrela de primeira magnitude</a><span style="color: #252525;">, e a </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a><span style="color: #252525;"> mais </span><a href="http://pt.wikipedia.org/wiki/Brilhante" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Brilhante">brilhante</a><span style="color: #252525;"> da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a><span style="color: #252525;"> </span><a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Taurus">Taurus</a><span style="color: #252525;">.</span><span class="reference" id="cite_ref-thomas.pavitt.2_1-0" style="bottom: 1ex; color: #252525; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Aldebar%C3%A3#cite_note-thomas.pavitt.2-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span><span style="color: #252525;"> É também designada pelos </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Nomes" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nomes">nomes</a><span style="color: #252525;"> de </span><b style="color: #252525;">Cor Tauri</b><span style="color: #252525;">; </span><b style="color: #252525;">Parilicium</b><span style="color: #252525;"> ou ainda, pelos códigos </span><b style="color: #252525;">HR 1457</b><span style="color: #252525;"> e </span><b style="color: #252525;">HD 29139</b><span style="color: #252525;">.</span></div>
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Na <a href="http://pt.wikipedia.org/wiki/Gr%C3%A9cia" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Grécia">Grécia</a> antiga era conhecida como "tocha" ou "facho".</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Aldebar%C3%A3</span></span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/4/48/Aldebaran_e_sol.JPG" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></div>
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<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Aldebar%C3%A3#mediaviewer/Ficheiro:Aldebaran_e_sol.JPG</span></span></div>
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<span style="background-color: white; font-family: sans-serif; line-height: 17.318561553955078px; text-align: left;"><span style="color: #073763;"><b>Comparação do tamanho relativo de Aldebaran e do Sol</b></span></span></div>
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<span class="mw-headline" id="Descri.C3.A7.C3.A3o_e_localiza.C3.A7.C3.A3o"><span style="font-size: x-small;">Descrição </span></span></h2>
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Se imaginarmos a imagem sugerida para a constelação, a estrela ocupará sensivelmente a posição do olho esquerdo do Touro mítico.</div>
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O seu nome provém da palavra <a href="http://pt.wikipedia.org/wiki/L%C3%ADngua_%C3%A1rabe" style="background: none; color: #0b0080; text-decoration: none;" title="Língua árabe">árabe</a> <b>الدبران</b> <i>al-dabarān</i> que significa "aquela que segue" ou "olho do Touro" – referência à forma como a estrela parece seguir o <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado estelar">aglomerado estelar</a> das <a href="http://pt.wikipedia.org/wiki/Pl%C3%AAiades" style="background: none; color: #0b0080; text-decoration: none;" title="Plêiades">Plêiades</a> durante o seu movimento aparente ao longo do céu nocturno.</div>
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Quase parece que Aldebarã pertence ao mais disperso dos enxames estelares (as <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/H%C3%ADades_(astronomia)" style="background: none; color: #0b0080; text-decoration: none;" title="Híades (astronomia)">Híades</a>) que constitui, também, o aglomerado mais próximo da <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>. Contudo, a maior parte dos autores crê que, na verdade, está apenas localizada na mesma direcção da linha de visão entre a Terra e as Híades – sendo, portanto, uma estrela independente.</div>
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Actualmente, a sua <a href="http://pt.wikipedia.org/wiki/Energia" style="background: none; color: #0b0080; text-decoration: none;" title="Energia">energia</a> provém apenas da fusão de <a href="http://pt.wikipedia.org/wiki/H%C3%A9lio" style="background: none; color: #0b0080; text-decoration: none;" title="Hélio">hélio</a>, da qual resultam cinzas de <a href="http://pt.wikipedia.org/wiki/Carbono" style="background: none; color: #0b0080; text-decoration: none;" title="Carbono">Carbono</a> e <a href="http://pt.wikipedia.org/wiki/Oxig%C3%A9nio" style="background: none; color: #0b0080; text-decoration: none;" title="Oxigénio">Oxigénio</a>.Aldebarã é uma estrela de tipo espectral K5 III (é uma <a href="http://pt.wikipedia.org/wiki/Gigante_vermelha" style="background: none; color: #0b0080; text-decoration: none;" title="Gigante vermelha">gigante vermelha</a>), o que significa que tem cor alaranjada; tem grandes dimensões, e saiu da <a href="http://pt.wikipedia.org/wiki/Sequ%C3%AAncia_principal" style="background: none; color: #0b0080; text-decoration: none;" title="Sequência principal">sequência principal</a> do<a href="http://pt.wikipedia.org/wiki/Diagrama_de_Hertzsprung-Russell" style="background: none; color: #0b0080; text-decoration: none;" title="Diagrama de Hertzsprung-Russell">Diagrama de Hertzsprung-Russell</a> depois de ter gasto todo o <a href="http://pt.wikipedia.org/wiki/Hidrog%C3%A9nio" style="background: none; color: #0b0080; text-decoration: none;" title="Hidrogénio">hidrogénio</a> que constituía o seu “combustível”. Tem uma companheira menor (uma estrela mais pálida, tipo M2 anã que orbita a várias centenas de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Unidades_astron%C3%B3micas" style="background: none; color: #0b0080; text-decoration: none;" title="Unidades astronómicas">UA</a>).</div>
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O corpo principal desta estrela expandiu-se para um diâmetro de aproximadamente 5,3 <a href="http://pt.wikipedia.org/wiki/Nota%C3%A7%C3%A3o_cient%C3%ADfica" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Notação científica">×</a> 10<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">7</span> <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Quil%C3%B3metro" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Quilómetro">km</a>, ou seja, cerca de 38 vezes maior que o <a href="http://pt.wikipedia.org/wiki/Sol" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sol">Sol</a> (outras fontes referem que é 50 vezes maior). As medições efectuadas pelo satélite <i><a href="http://pt.wikipedia.org/wiki/Hipparcos" style="background: none; color: #0b0080; text-decoration: none;" title="Hipparcos">Hipparcos</a></i> localizam a estrela a 65,1 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> da Terra, e permitem saber que a sua luminosidade é 150 vezes superior à do<a href="http://pt.wikipedia.org/wiki/Sol" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sol">Sol</a>, o que a torna a décima terceira estrela mais brilhante do céu (0,9 de magnitude). É ligeiramente <a href="http://pt.wikipedia.org/wiki/Estrela_vari%C3%A1vel" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela variável">variável</a>, do tipo <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Vari%C3%A1vel_pulsante&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Variável pulsante (página não existe)">variável pulsante</a>, apresentando uma variação de cerca de 0.2 de magnitude.</div>
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<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Aldebar%C3%A3</span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>Hyades for the Holidays </b><br /><b>Image Credit & <a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply" style="color: #274e13; text-decoration: none;">Copyright</a>: </b>Jerry Lodriguss (<a href="http://www.astropix.com/INDEX.HTM" style="color: #274e13; text-decoration: none;">Catching the Light</a>)</span></center>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>Explanation: </b>Recognized since antiquity and depicted on the <a href="http://faculty.goucher.edu/eng240/shield_of_achilles.htm" style="color: #274e13; text-decoration: none;">shield of Achilles</a> according to Homer, stars of the <a href="http://www.nightskyinfo.com/archive/hyades/" style="color: #274e13; text-decoration: none;">Hyades cluster</a> form the head of the constellation Taurus the Bull. Their general V-shape is anchored by <a href="http://stars.astro.illinois.edu/sow/aldebaran.html" style="color: #274e13; text-decoration: none;">Aldebaran</a>, the eye of the Bull and by far the constellation's brightest star. Yellowish in appearance, red giant Aldebaran is not a Hyades cluster member, though. Modern astronomy puts <a href="http://messier.seds.org/xtra/ngc/hyades.html" style="color: #274e13; text-decoration: none;">the Hyades cluster</a> 151 light-years away making it the nearest established open star cluster, while Aldebaran lies at less than half that distance, along the same line-of-sight. <a href="http://www.astropix.com/HTML/SHOW_DIG/Hyades.HTM" style="color: #274e13; text-decoration: none;">Along with colorful Hyades stars</a>, this stellar holiday portrait locates Aldebaran just below center, as well as another <a href="http://stars.astro.illinois.edu/sow/cluster.html" style="color: #274e13; text-decoration: none;">open star cluster</a> in Taurus, NGC 1647 at the left, some 2,000 light-years or more in the background. Just slide your cursor over the image to identify the stars. The central Hyades stars are spread out over about 15 light-years. Formed some 800 million years ago, the Hyades star cluster may share a common origin <a href="http://messier.seds.org/m/m044.html" style="color: #274e13; text-decoration: none;">with M44</a> (Praesepe), a naked-eye open star cluster in Cancer, based on M44's <a href="http://en.wikipedia.org/wiki/Hyades_%28star_cluster%29#Proper_motion" style="color: #274e13; text-decoration: none;">motion through space</a> and remarkably similar age.</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18.200000762939453px;"><b><a href="http://apod.nasa.gov/apod/ap121224.html" style="color: #274e13; text-decoration: none;">http://apod.nasa.gov/apod/ap121224.html</a></b></span></span></div>
<span style="background-color: #073763;"><span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 22.399999618530273px;"><b>Hyades for the Holidays </b><br /><b>Image Credit & <a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply" style="color: #274e13; text-decoration: none;">Copyright</a>: </b>Jerry Lodriguss (<a href="http://www.astropix.com/INDEX.HTM" style="color: #274e13; text-decoration: none;">Catching the Light</a>)</span><br /><span style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px;"><span style="font-family: Arial, Helvetica, sans-serif;">(foto com marcação)</span></span><span style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px;"> </span><span style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></span><span style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px;"></span></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">Hyades - Aglomerado em movimento</span></b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Grupo de mais de 200 estrelas que circundam Aldebarã e que se deslocam todas para um mesmo ponto do céu, próximo a Betelgeuse, a estrela-alpha de Órion. Estas estrelas são um aglomerado aberto e seu desenho forma a cabeça do Touro. Todas as estrelas encontram-se em movimento em conjunto e por esta razão as Hyades são chamadas de Aglomerado em Movimento do Touro. A estrela Alpha Tauri, Aldebarã, gigante alaranjada, adorna as Hyades como se fosse uma gema brilhante porém não é membro desse aglomerado por se situar cerca da metade do caminho entre o centro das Hyades e nosso Sol.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Prima Hyadum</b><b>. Gama Taurus. </b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A estrela-chefe das Hiades, o aglomerado. As Híades consistem de seis estrelas situadas na testa do Touro e marcando o olho ao norte.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">As Híades eram as sete filhas de Atlas e Aethra, meia-irmãs das Pleiades (que eram filhas de Atlas e de Pleione) e foram encarregadas por Júpiter de cuidar de Baco, quando criança. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Elas foram colocadas no céu como prêmio por seu amor fraternal e pela tristeza pela morte de seu irmão Hyas, que foi morto por um animal feroz, na Líbia.<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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The <b>Hyades</b> (<span class="nowrap" style="white-space: nowrap;"><span class="IPA" title="Representation in the International Phonetic Alphabet (IPA)"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English" style="background: none; color: #0b0080; text-decoration: none !important;" title="Help:IPA for English">/</a></span><span class="IPA nopopups"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English#Key" style="background: none; color: #0b0080; text-decoration: none !important;" title="Help:IPA for English"><span style="border-bottom-style: dotted; border-bottom-width: 1px;" title="/ˈ/ primary stress follows">ˈ</span></a></span><span class="IPA nopopups"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English#Key" style="background: none; color: #0b0080; text-decoration: none !important;" title="Help:IPA for English"><span style="border-bottom-style: dotted; border-bottom-width: 1px;" title="'h' in 'hi'">h</span></a></span><span class="IPA nopopups"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English#Key" style="background: none; color: #0b0080; text-decoration: none !important;" title="Help:IPA for English"><span style="border-bottom-style: dotted; border-bottom-width: 1px;" title="/aɪ/ long 'i' in 'bide'">aɪ</span></a></span><span class="IPA nopopups"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English#Key" style="background: none; color: #0b0080; text-decoration: none !important;" title="Help:IPA for English"><span style="border-bottom-style: dotted; border-bottom-width: 1px;" title="/./ syllable break">.</span></a></span><span class="IPA nopopups"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English#Key" style="background: none; color: #0b0080; text-decoration: none !important;" title="Help:IPA for English"><span style="border-bottom-style: dotted; border-bottom-width: 1px;" title="/ə/ 'u' in 'syrup'">ə</span></a></span><span class="IPA nopopups"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English#Key" style="background: none; color: #0b0080; text-decoration: none !important;" title="Help:IPA for English"><span style="border-bottom-style: dotted; border-bottom-width: 1px;" title="'d' in 'dye'">d</span></a></span><span class="IPA nopopups"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English#Key" style="background: none; color: #0b0080; text-decoration: none !important;" title="Help:IPA for English"><span style="border-bottom-style: dotted; border-bottom-width: 1px;" title="/iː/ long 'e' in 'seed'">iː</span></a></span><span class="IPA nopopups"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English#Key" style="background: none; color: #0b0080; text-decoration: none !important;" title="Help:IPA for English"><span style="border-bottom-style: dotted; border-bottom-width: 1px;" title="'z' in 'zebra'">z</span></a></span><span class="IPA" title="Representation in the International Phonetic Alphabet (IPA)"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English" style="background: none; color: #0b0080; text-decoration: none !important;" title="Help:IPA for English">/</a></span></span>; <a href="http://en.wikipedia.org/wiki/Greek_language" style="background: none; color: #0b0080; text-decoration: none;" title="Greek language">Greek</a> Ὑάδες, also known as <a href="http://en.wikipedia.org/wiki/Philibert_Jacques_Melotte" style="background: none; color: #0b0080; text-decoration: none;" title="Philibert Jacques Melotte">Melotte</a> 25 or <a href="http://en.wikipedia.org/wiki/Collinder_catalog" style="background: none; color: #0b0080; text-decoration: none;" title="Collinder catalog">Collinder</a> 50), is the nearest <a href="http://en.wikipedia.org/wiki/Open_cluster" style="background: none; color: #0b0080; text-decoration: none;" title="Open cluster">open cluster</a> to the <a href="http://en.wikipedia.org/wiki/Solar_System" style="background: none; color: #0b0080; text-decoration: none;" title="Solar System">Solar System</a> and one of the best-studied of all <a href="http://en.wikipedia.org/wiki/Star_cluster" style="background: none; color: #0b0080; text-decoration: none;" title="Star cluster">star clusters</a>. The <a href="http://en.wikipedia.org/wiki/Hipparcos" style="background: none; color: #0b0080; text-decoration: none;" title="Hipparcos">Hipparcos</a> satellite, the <a href="http://en.wikipedia.org/wiki/Hubble_Space_Telescope" style="background: none; color: #0b0080; text-decoration: none;" title="Hubble Space Telescope">Hubble Space Telescope</a>, and infrared <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Color-magnitude_diagram" style="background: none; color: #0b0080; text-decoration: none;" title="Color-magnitude diagram">color-magnitude diagram</a> fitting have been used to establish a distance of ~153 ly (47 pc) to the cluster center.<sup class="reference" id="cite_ref-Perryman_1-1" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)#cite_note-Perryman-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup><sup class="reference" id="cite_ref-vanleeuwen09_2-1" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)#cite_note-vanleeuwen09-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup><sup class="reference" id="cite_ref-majaess11_3-1" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)#cite_note-majaess11-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[3]</a></sup><sup class="reference" id="cite_ref-mcarthur11_4-1" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)#cite_note-mcarthur11-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[4]</a></sup> The distances established by these three independent methods agree, thereby making the Hyades an important rung on the<a href="http://en.wikipedia.org/wiki/Cosmic_distance_ladder" style="background: none; color: #0b0080; text-decoration: none;" title="Cosmic distance ladder">cosmic distance ladder</a>. The cluster consists of a roughly spherical group of hundreds of stars sharing the same age, place of origin, chemical content, and motion through space.<sup class="reference" id="cite_ref-Perryman_1-2" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)#cite_note-Perryman-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup><sup class="reference" id="cite_ref-Bouvier_5-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)#cite_note-Bouvier-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[5]</a></sup> From the perspective of observers on <a href="http://en.wikipedia.org/wiki/Earth" style="background: none; color: #0b0080; text-decoration: none;" title="Earth">Earth</a>, the Hyades Cluster appears in the <a href="http://en.wikipedia.org/wiki/Constellation" style="background: none; color: #0b0080; text-decoration: none;" title="Constellation">constellation</a> <a href="http://en.wikipedia.org/wiki/Taurus_(constellation)" style="background: none; color: #0b0080; text-decoration: none;" title="Taurus (constellation)">Taurus</a>, where its brightest stars form a "V" shape along with the still brighter <a href="http://en.wikipedia.org/wiki/Red_giant" style="background: none; color: #0b0080; text-decoration: none;" title="Red giant">red giant</a> <a href="http://en.wikipedia.org/wiki/Aldebaran" style="background: none; color: #0b0080; text-decoration: none;" title="Aldebaran">Aldebaran</a>. However, Aldebaran is unrelated to the Hyades, as it is located much closer to Earth (hence its apparent brightness) and merely happens to lie along the same line of sight.</div>
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The five brightest member stars of the Hyades have all evolved away from the <a href="http://en.wikipedia.org/wiki/Main_sequence" style="background: none; color: #0b0080; text-decoration: none;" title="Main sequence">Main Sequence</a> and now lie at the bottom of the giant branch.<sup class="reference" id="cite_ref-Hyadum1_6-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)#cite_note-Hyadum1-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[6]</a></sup> Four of these stars, with <a href="http://en.wikipedia.org/wiki/Bayer_designation" style="background: none; color: #0b0080; text-decoration: none;" title="Bayer designation">Bayer designations</a> <a href="http://en.wikipedia.org/wiki/Gamma_Tauri" style="background: none; color: #0b0080; text-decoration: none;" title="Gamma Tauri">Gamma</a>, <a href="http://en.wikipedia.org/wiki/Delta_Tauri" style="background: none; color: #0b0080; text-decoration: none;" title="Delta Tauri">Delta 1</a>, <a href="http://en.wikipedia.org/wiki/Epsilon_Tauri" style="background: none; color: #0b0080; text-decoration: none;" title="Epsilon Tauri">Epsilon</a>, and <a href="http://en.wikipedia.org/wiki/Theta_Tauri" style="background: none; color: #0b0080; text-decoration: none;" title="Theta Tauri">Theta Tauri</a>, form an <a href="http://en.wikipedia.org/wiki/Asterism_(astronomy)" style="background: none; color: #0b0080; text-decoration: none;" title="Asterism (astronomy)">asterism</a> that is traditionally identified as the head of Taurus the Bull.<sup class="reference" id="cite_ref-Hyadum1_6-1" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)#cite_note-Hyadum1-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[6]</a></sup> The other is<a href="http://en.wikipedia.org/wiki/Zeta_Tauri" style="background: none; color: #0b0080; text-decoration: none;" title="Zeta Tauri">Zeta 1 Tauri</a>, which lies 2° further south. Epsilon Tauri, known as <i>Ain</i> (the "Bull's Eye"), has a <a href="http://en.wikipedia.org/wiki/Gas_giant" style="background: none; color: #0b0080; text-decoration: none;" title="Gas giant">gas giant</a> exoplanet candidate,<sup class="reference" id="cite_ref-Sato_7-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)#cite_note-Sato-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[7]</a></sup> the first planet to be found in any open cluster.</div>
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The age of the Hyades is estimated to be about 625 million years.<sup class="reference" id="cite_ref-Perryman_1-3" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)#cite_note-Perryman-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup> The cluster core, where stars are most densely packed, has a radius of 2.7 parsecs (corresponding to a diameter of 17.6 light years), and the cluster's <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Tidal_radius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Tidal radius">tidal radius</a> is 10 parsecs (corresponding to a diameter of 65 light years).<sup class="reference" id="cite_ref-Perryman_1-4" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)#cite_note-Perryman-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup> However, about one-third of confirmed member stars have been observed well outside this boundary, in the cluster's extended halo; these stars are probably in the process of escaping from its gravitational influence.<sup class="reference" id="cite_ref-Perryman_1-5" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)#cite_note-Perryman-1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)" style="color: #274e13; text-decoration: none;">http://en.wikipedia.org/wiki/Hyades_(star_cluster)</a></span></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_desc" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Description</span></td><td class="description"><div class="description mw-content-ltr en" dir="ltr" lang="en" style="direction: ltr;">
<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span class="language en" title=""><b>English:</b></span> This map represents prominent stars in the core of the Hyades Cluster. Filled red circles refer to red giant stars. Filled blue circles refer to A, F, and G-type stars. The four Hyades giants are labeled with their Bayer designations (e.g., Epsilon Tauri). Arabic numerals provide Flamsteed designations (e.g., 68 Tauri). Small italics provide designations from the <a href="http://commons.wikimedia.org/wiki/Henry_Draper" style="background-image: none; color: #274e13; text-decoration: none;" title="Henry Draper">Henry Draper</a> catalog (e.g., HD 28406). The vertical scale indicates declination; the horizontal scale indicates right ascension, measured in hours and minutes. Not all stars in the field of view belong to the Hyades Cluster. Membership determinations were made on the basis of Table 2 in Perryman et al., "The Hyades Cluster: distance, structure, dynamics, and age" (Astronomy and Astrophysics 331, 81-120, 1998). On this map, the only non-member star that carries a label is the most prominent one, Aldebaran. All other non-member stars are left unmarked.</span></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_date" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Date</span></td><td><time class="dtstart" datetime="2008-10-13" style="display: inline;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">13 October 2008</span></time></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Source</span></td><td><span class="int-own-work"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Own work</span></span></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Author</span></td><td><a href="http://commons.wikimedia.org/wiki/User:Thuvan_Dihn" style="background-image: none; color: #274e13; text-decoration: none;" title="User:Thuvan Dihn"><span style="font-family: Arial, Helvetica, sans-serif;">Thuvan Dihn</span></a></td></tr>
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<span class="mw-headline" id="History"><span style="font-size: x-small;">History</span></span></h2>
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As a naked-eye object, the Hyades cluster has been known since prehistoric times. It is mentioned by numerous Classical authors from <a href="http://en.wikipedia.org/wiki/Homer" style="background: none; color: #0b0080; text-decoration: none;" title="Homer">Homer</a> to <a href="http://en.wikipedia.org/wiki/Ovid" style="background: none; color: #0b0080; text-decoration: none;" title="Ovid">Ovid</a>.<sup class="reference" id="cite_ref-seds_13-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)#cite_note-seds-13" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[13]</a></sup> In Book 18 of the <i><a href="http://en.wikipedia.org/wiki/Iliad" style="background: none; color: #0b0080; text-decoration: none;" title="Iliad">Iliad</a></i> the stars of the Hyades appear along with the <a href="http://en.wikipedia.org/wiki/Pleiades" style="background: none; color: #0b0080; text-decoration: none;" title="Pleiades">Pleiades</a>, <a href="http://en.wikipedia.org/wiki/Ursa_Major" style="background: none; color: #0b0080; text-decoration: none;" title="Ursa Major">Ursa Major</a>, and <a href="http://en.wikipedia.org/wiki/Orion_(constellation)" style="background: none; color: #0b0080; text-decoration: none;" title="Orion (constellation)">Orion</a> on the shield that the god <a href="http://en.wikipedia.org/wiki/Hephaestus" style="background: none; color: #0b0080; text-decoration: none;" title="Hephaestus">Hephaistos</a> made for <a href="http://en.wikipedia.org/wiki/Achilles" style="background: none; color: #0b0080; text-decoration: none;" title="Achilles">Achilles</a>.<sup class="reference" id="cite_ref-Lattimore_14-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)#cite_note-Lattimore-14" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[14]</a></sup>In Greek mythology, the <a href="http://en.wikipedia.org/wiki/Hyades_(mythology)" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hyades (mythology)">Hyades</a> were the five daughters of <a href="http://en.wikipedia.org/wiki/Atlas_(mythology)" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Atlas (mythology)">Atlas</a> and half-sisters to the <a href="http://en.wikipedia.org/wiki/Pleiades_(Greek_mythology)" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pleiades (Greek mythology)">Pleiades</a>. After the death of their brother, Hyas, the weeping sisters were transformed into a cluster of stars that was afterwards associated with rain.</div>
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In England the cluster was known as the "April Rainers" from an association with April showers, as recorded in the folk song "<a href="http://en.wikipedia.org/wiki/Green_Grow_the_Rushes,_O" style="background: none; color: #0b0080; text-decoration: none;" title="Green Grow the Rushes, O">Green Grow the Rushes, O</a>".</div>
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The cluster was probably first catalogued by <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Giovanni_Batista_Hodierna" style="background: none; color: #0b0080; text-decoration: none;" title="Giovanni Batista Hodierna">Giovanni Batista Hodierna</a> in 1654, and it subsequently appeared in many star atlases of the 17th and 18th centuries.<sup class="reference" id="cite_ref-seds_13-1" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)#cite_note-seds-13" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[13]</a></sup> However, <a href="http://en.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> did not include the Hyades in his 1781 catalog of deep sky objects.<sup class="reference" id="cite_ref-seds_13-2" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)#cite_note-seds-13" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[13]</a></sup> It therefore lacks a Messier number, unlike many other, more distant open clusters – e.g., <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Messier_44" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 44">M44</a> (Praesepe), <a href="http://en.wikipedia.org/wiki/Pleiades" style="background: none; color: #0b0080; text-decoration: none;" title="Pleiades">M45</a> (Pleiades), and <a href="http://en.wikipedia.org/wiki/Messier_67" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 67">M67</a>.</div>
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In 1869, the astronomer R.A. Proctor observed that numerous stars at large distances from the Hyades share a similar motion through space.<sup class="reference" id="cite_ref-Zuckerman_15-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)#cite_note-Zuckerman-15" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[15]</a></sup> In 1908, <a href="http://en.wikipedia.org/wiki/Lewis_Boss" style="background: none; color: #0b0080; text-decoration: none;" title="Lewis Boss">Lewis Boss</a> reported almost 25 years of observations to support this premise, arguing for the existence of a co-moving group of stars that he called the Taurus Stream (now generally known as the Hyades Stream or Hyades Supercluster). Boss published a chart that traced the scattered stars' movements back to a common point of convergence.<sup class="reference" id="cite_ref-Boss_16-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)#cite_note-Boss-16" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[16]</a></sup></div>
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By the 1920s, the notion that the Hyades shared a common origin with the Praesepe Cluster was widespread,<sup class="reference" id="cite_ref-Hertzprung_17-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)#cite_note-Hertzprung-17" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[17]</a></sup> with Rudolf Klein-Wassink noting in 1927 that the two clusters are "probably cosmically related."<sup class="reference" id="cite_ref-Klein-Wassink_18-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Hyades_(star_cluster)#cite_note-Klein-Wassink-18" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[18]</a></sup> For much of the twentieth century, scientific study of the Hyades focused on determining its distance; modeling its evolution; confirming or rejecting candidate members; and characterizing individual stars.</div>
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LEIA MAIS em</div>
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the highest resolution version available." src="http://apod.nasa.gov/apod/image/0009/sepsky_stanrichard.jpg" height="640" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="440" /></div>
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<b style="background-color: white;">http://apod.nasa.gov/apod/ap000929.html</b></div>
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<span style="background-color: white;"><b style="color: black; font-family: 'Times New Roman'; line-height: normal;">Credit & Copyright: </b><span style="color: black; font-family: 'Times New Roman'; line-height: normal;"></span><a href="mailto:snkrichard@msn.com" style="color: #274e13; font-family: 'Times New Roman'; line-height: normal; text-decoration: none;">Stan Richard</a></span></div>
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<span style="background-color: white;"><b style="color: black; font-family: 'Times New Roman'; line-height: normal; text-align: start;">Explanation: </b><span style="color: black; font-family: 'Times New Roman'; line-height: normal; text-align: start;">Star clusters, planets, and a red giant posed for this portrait of the </span><a href="http://apod.nasa.gov/apod/ap000708.html" style="color: #274e13; font-family: 'Times New Roman'; line-height: normal; text-align: start; text-decoration: none;">night</a><span style="color: black; font-family: 'Times New Roman'; line-height: normal; text-align: start;"> sky from rural Jasper County, Iowa, USA. </span><a href="http://geocities.com/stanzman_2001/" style="color: #274e13; font-family: 'Times New Roman'; line-height: normal; text-align: start; text-decoration: none;">Astrophotographer</a><span style="color: black; font-family: 'Times New Roman'; line-height: normal; text-align: start;"> Stan Richard recorded the four minute time exposure looking east around midnight on September 3rd at Ashton-Wildwood Park. To avoid </span><a href="http://pages.prodigy.net/pam.orman/JoeTrails.html" style="color: #274e13; font-family: 'Times New Roman'; line-height: normal; text-align: start; text-decoration: none;">star trails</a><span style="color: black; font-family: 'Times New Roman'; line-height: normal; text-align: start;">, his camera was mounted on a </span><a href="http://casa.colorado.edu/~rachford/widefield/barndoor.html" style="color: #274e13; font-family: 'Times New Roman'; line-height: normal; text-align: start; text-decoration: none;">barndoor-style</a><span style="color: black; font-family: 'Times New Roman'; line-height: normal; text-align: start;"> tracker to compensate for the Earth's </span><a href="http://apod.nasa.gov/apod/ap000715.html" style="color: #274e13; font-family: 'Times New Roman'; line-height: normal; text-align: start; text-decoration: none;">rotation</a><span style="color: black; font-family: 'Times New Roman'; line-height: normal; text-align: start;">. Can you identify his celestial subjects? (Click on the image for a labeled version.) The </span><a href="http://www.pantheon.org/mythica/articles/p/pleiades.html" style="color: #274e13; font-family: 'Times New Roman'; line-height: normal; text-align: start; text-decoration: none;">Pleiades</a><span style="color: black; font-family: 'Times New Roman'; line-height: normal; text-align: start;"> and </span><a href="http://www.pantheon.org/mythica/articles/h/hyades.html" style="color: #274e13; font-family: 'Times New Roman'; line-height: normal; text-align: start; text-decoration: none;">Hyades</a><span style="color: black; font-family: 'Times New Roman'; line-height: normal; text-align: start;">, the closest open or galactic </span><a href="http://www.seds.org/messier/open.html" style="color: #274e13; font-family: 'Times New Roman'; line-height: normal; text-align: start; text-decoration: none;">star clusters</a><span style="color: black; font-family: 'Times New Roman'; line-height: normal; text-align: start;">to the Sun, should be recognizable to beginning </span><a href="http://starchild.gsfc.nasa.gov/" style="color: #274e13; font-family: 'Times New Roman'; line-height: normal; text-align: start; text-decoration: none;">stargazers</a><span style="color: black; font-family: 'Times New Roman'; line-height: normal; text-align: start;">. Of course gas giant </span><a href="http://galileo.jpl.nasa.gov/jupiter/jupiter.html" style="color: #274e13; font-family: 'Times New Roman'; line-height: normal; text-align: start; text-decoration: none;">Jupiter</a><span style="color: black; font-family: 'Times New Roman'; line-height: normal; text-align: start;"> rules as the brightest object in the picture and the largest planet in the Solar System, but second largest planet </span><a href="http://www.jpl.nasa.gov/cassini/Kids/stories/" style="color: #274e13; font-family: 'Times New Roman'; line-height: normal; text-align: start; text-decoration: none;">Saturn</a><span style="color: black; font-family: 'Times New Roman'; line-height: normal; text-align: start;"> is also visible nearby. For sheer size cool </span><a href="http://www.astro.uiuc.edu/~kaler/sow/aldebaran.html" style="color: #274e13; font-family: 'Times New Roman'; line-height: normal; text-align: start; text-decoration: none;">red giant star Aldebaran</a><span style="color: black; font-family: 'Times New Roman'; line-height: normal; text-align: start;"> is more impressive though, spanning about forty times the diameter of the Sun. Sixty light-years away and yellowish in this picture, Aldebaran is known as Alpha Tauri, the brightest star </span><a href="http://aibn47.astro.uni-bonn.de/~gallery/constellations/taurus/" style="color: #274e13; font-family: 'Times New Roman'; line-height: normal; text-align: start; text-decoration: none;">in Taurus</a><span style="color: black; font-family: 'Times New Roman'; line-height: normal; text-align: start;">, the Bull.</span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.atlasoftheuniverse.com/250lys.html" style="color: #274e13; text-decoration: none;">http://www.atlasoftheuniverse.com/250lys.html</a></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">The Hyades Star Cluster</span></h3>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">The Hyades cluster is the nearest major star cluster and the only one close enough to be mapped in three dimensions. The Hyades cluster is a bright object in Taurus, but the view is partially ruined by Aldebaran - a brilliant orange giant star that lies in front of the cluster at less than half the distance. The cluster itself is 151 light years from us. It was formed about 660 million years ago and the cluster has probably travelled around the Galaxy three times since then. Like most open star clusters, the stars in the cluster are slowly moving apart.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Minha (Janine) tradução simples literal para o texto acima:</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>O Aglomerado das Hyades</b> é o maior aglomerado estelar mais próximo de nós e o único suficientemente próximo para ser mapeado em três dimensões. O alglomerado das Hyades é um brilhante objeto em Touro, porém sua visão fica parcialmente arruinada pela presença de Aldebaran - uma estrela gigante alaranjada brilhante e que encontra-se em frente ao aglomerado e pelo menos na metade da distância do mesmo. O aglomerado está a 151 anos-luz de nós e foi formado cerca de 660 milhões de anos atrás e teria provavelmente viajado em torno da Galáxia por três vezes, desde então. Assim como a maioria dos aglomerados estelares abertos, as estrelas no aglomerado estão vagarosamente se separando.</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjkfFwxcyagcIrW6FGjY-pEMifHMw_jv5qff8xMie4FNty2JHDwPw5gGBDlVCXTa_iNgmUVCaAb4IuBIBsK8iEAsQkCKO_sspvJXpGzejO3Bwedeg9-rdVB5KaZf38Xul_l7DZqOpDd9bg/s1600/hyades.gif" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjkfFwxcyagcIrW6FGjY-pEMifHMw_jv5qff8xMie4FNty2JHDwPw5gGBDlVCXTa_iNgmUVCaAb4IuBIBsK8iEAsQkCKO_sspvJXpGzejO3Bwedeg9-rdVB5KaZf38Xul_l7DZqOpDd9bg/s1600/hyades.gif" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
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<span style="color: #274e13;"><span style="font-size: small;">The Universe within 250 Light Years<br />The Solar Neighbourhood</span></span></h1>
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<span style="letter-spacing: 0.2em;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><span style="font-size: small;">O Universo contido em 250 anos-luz</span></span></span></h3>
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<span style="letter-spacing: 0.2em;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><span style="font-size: small;">A VIZINHANÇA SOLAR</span></span></span></h3>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgF1xjlwO1dQyh4okmMUWDUvhoDnluoEPP9Qq5RDxn9kIV4V0LOunL43YfDWYISc3rHhmeOXunTIyWU5jBaXrPCgWbrDaIO_hneE54uipvapc9FCSaO-f1_U7YvhyrZWGU70PaWl9IGcKc/s1600/250lys.gif" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgF1xjlwO1dQyh4okmMUWDUvhoDnluoEPP9Qq5RDxn9kIV4V0LOunL43YfDWYISc3rHhmeOXunTIyWU5jBaXrPCgWbrDaIO_hneE54uipvapc9FCSaO-f1_U7YvhyrZWGU70PaWl9IGcKc/s1600/250lys.gif" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<span style="text-align: start;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">This map is a plot of the 1500 most luminous stars within 250 light years. All of these stars are much more luminous than the Sun and most of them can be seen with the naked eye. About one third of the stars visible with the naked eye lie within 250 light years, even though this is only a tiny part of our galaxy.</span></span></div>
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<b><b><span lang="EN-US"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">ATLAS DO UNIVERSO</span></span></b></b></div>
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<a href="http://www.atlasoftheuniverse.com/index.html" style="color: #274e13; text-decoration: none;"><span style="font-family: Arial, Helvetica, sans-serif;">http://www.atlasoftheuniverse.com/index.html</span></a></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">This website belongs to <a href="http://www.atlasoftheuniverse.com/me.html" style="color: #274e13; text-decoration: none;">Richard Powell</a>.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Minha (Janine) tradução simples e literal para o texto acima:</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Este mapa apresenta as 1.500 estrelas mais luminosas contidas em 250 anos-luz. Todas estas estrelas são bem mais luminosas do que o Sol e muitas delas podem ser vistas a olho nu. Cerca de um terço das estrelas visíveis a olho nu encontram-se dentre 250 anos-luz, mesmo que isso signifique apenas uma pequena parte de nossa galáxia.</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18px;"><a href="http://www.deepskycolors.com/archive/2010/09/26/hyades-in-the-Dust.html" style="color: #274e13; text-decoration: none;">http://www.deepskycolors.com/archive/2010/09/26/hyades-in-the-Dust.html</a></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Entre no Link acima e leia o texto (em inglês) comentando sobre como o autor - Rogélio Bernal Andreo - realizou esta belíssima foto.</span></div>
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<span lang="EN-US"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj6fNztn0buc6gBCz4XcgC1mgmMFzORCQGRgLy0WwhAGY-xIH_S0Y1MmFR35f7rUeQ1j_n03nJus0lW5_R-JkvhcwAtuJIzL7aAVlCFVWsCXPhr8SaxDkEEA95MCmpTeLiSygSfMEb_IdE/s1600/urania17.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj6fNztn0buc6gBCz4XcgC1mgmMFzORCQGRgLy0WwhAGY-xIH_S0Y1MmFR35f7rUeQ1j_n03nJus0lW5_R-JkvhcwAtuJIzL7aAVlCFVWsCXPhr8SaxDkEEA95MCmpTeLiSygSfMEb_IdE/s1600/urania17.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://apod.nasa.gov/apod/ap111225.html</span></div>
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<a href="https://www.blogger.com/blogger.g?blogID=2442159895732486967" imageanchor="1" style="clear: right; color: #274e13; float: right; line-height: 22.399999618530273px; margin-bottom: 1em; margin-left: 1em; text-decoration: none;"></a><a href="https://www.blogger.com/blogger.g?blogID=2442159895732486967" imageanchor="1" style="clear: right; color: #274e13; float: right; line-height: 22.399999618530273px; margin-bottom: 1em; margin-left: 1em; text-decoration: none;"></a><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>M1: The Crab Nebula from Hubble </b><br /><b>Image Credit: </b><a href="http://www.nasa.gov/" style="color: #274e13; text-decoration: none;">NASA</a>, <a href="http://hubble.esa.int/" style="color: #274e13; text-decoration: none;">ESA</a>, J. Hester, A. Loll (<a href="http://sese.asu.edu/" style="color: #274e13; text-decoration: none;">ASU</a>); Acknowledgement: Davide De Martin (<a href="http://www.skyfactory.org/" style="color: #274e13; text-decoration: none;">Skyfactory</a>)</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">Concluindo nossa visita à constelação do Touro</span><span style="font-family: Arial, Helvetica, sans-serif;">,</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><b>vamos observar que </b></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>o Chifre mais ao norte acolhe a estrela-beta Tauri, El Nath:</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="ES-TRAD">El Nath</span><span lang="ES-TRAD">. Beta Tauri. <o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 05h25,0m - Declinação +28<sup>o</sup> 36<o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual 1,78 - Distância 300 anos-luz<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela dupla, de um branco brilhante e de um pálido cinza, situada na ponta do chifre ao norte do Touro e comumente conhecida como o Chifre ao Norte do Touro. <span lang="ES-TRAD">De Al Natih. </span><span lang="PT">O Pastor. Em outra versão, é a Viagem, nome árabe que indica a viagem empreendida pela constelação do Cocheiro.<o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>E vamos observar que</b></span></div>
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<b><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">nas vizinhanças do Chifre do Sul do Touro </span><br /><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">mora a belíssima</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">NEBULOSA DO CARANGUEJO, M1, NGC 1952!</span></b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">........................... Uma estrela que certa dia explodiu, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">tornando-se uma chamada supernova,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e que, com o passar do tempo, tornou-se uma nuvem...;</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">nuvem penetrada por lentes ópticas </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">comandadas por olhares penetrantes e estudiosos...; </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">nuvem que foi revelando, descobrindo, não mais cobrindo,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">seus segredos de vida (quase) infinita, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">vida que sempre encontra </span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">uma nova maneira de ser, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">vida que se transforma em nova vida,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">através um novo coração, um pulsar, uma estrela de nêutrons, uma nova estrela<b>!</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Tempo e Espaço atuando através a eterna continuidade da Vida.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">.........................................</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><i>Houve um tempo num passado não muito distante em que aquele pedaço do céu deu lugar a uma "estrela visitante" que surgiu com sua imensa luz mesmo durante o tempo da luz do Sol ao longo de 23 dias, maravilhando os povos que a observaram atentamente. Isso aconteceu em 04 de julho de 1054.... e por ainda mais dois anos, puderam os maravilhados Terrestres ainda observarem sua luz inebriante no céu noturno.... até que finalmente, seu brilho foi esmaecendo, esmaecendo, esmaecendo, até que desapareceu por completo, tão subitamente assim como havia chegado! E foi somente recentemente (com a ajuda de bons telescópios) que os Terrestres puderam voltar a ver aquela estrela - ou a memória do que ela havia sido no passado - através da nuvem de gases firulantes e coloridos que foram soprados, largados para trás, como um lenço de seda solto ao vento da escuridão da noite do universo sem fim....</i></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><i>............... A verdade é que a explosão dessa estrela aconteceu cerca de 5500 anos antes de cristo...</i></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">.........................................................</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Encontre</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(ao final desta Postagem) </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">este Conto Surreal</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">escrito por mim, Janine, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">quando do encontro entre Saturno e a Nebulosa do Caranguejo,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">em 04 de janeiro de 2003.</span></div>
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<h3 class="post-title entry-title" itemprop="name" style="color: #073763; font-size: 22px; line-height: normal; margin: 0px; position: relative;">
<span style="color: #660000; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">O Tempo e o Sonho da Luz do Passado</span></h3>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">(Uma conversa entre Saturno e a Nebulosa do Caranguejo,</span><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"> ouvida da Terra</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"> - um conto surreal...)</span></div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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<h1>
Messier 1</h1>
<i><a href="http://messier.obspm.fr/nebula.html">Supernova Remnant</a> M1 (NGC 1952)</i> in <a href="http://messier.obspm.fr/map/Tau.html">Taurus</a></center>
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<br /><b><span style="font-size: large;">Crab Nebula</span></b><br /><b><br /></b></center>
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<a href="http://messier.obspm.fr/Jpg/m1.jpg"><img align="right" alt="[m1.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m1.jpg" /></a></div>
<table border="2" cellpadding="5" cellspacing="0" style="font-family: 'Times New Roman'; font-size: 16px;"><tbody>
<tr><th align="left">Right Ascension</th><td align="center">05 : 34.5 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+22 : 01 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">6.3 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">8.4 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">6x4 (arc min)</td></tr>
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Discovered 1731 by British amateur astronomer John Bevis.</div>
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The Crab Nebula, Messier 1 (M1, NGC 1952), is the most famous and conspicuous known supernova remnant, the expanding cloud of gas created in the explosion of a star as supernova which was observed in the year 1054 AD. It shines as a nebula of magnitude 8.4 near the southern "horn" of Taurus, the Bull.</div>
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<a href="http://messier.obspm.fr/more/m001_sn.html">The supernova</a> was noted on July 4, 1054 A.D. by Chinese astronomers as a new or "guest star," and was about four times brighter than Venus, or about mag -6. According to the records, it was visible in daylight for 23 days, and 653 days to the naked eye in the night sky. It was probably also recorded by Anasazi Indian artists (in present-day Arizona and New Mexico), as findings in Navaho Canyon and White Mesa (both Arizona) as well as in the Chaco Canyon National Park (New Mexico) indicate; there's a review of the research on the <a href="http://www.astronomy.pomona.edu/archeo/outside/chaco/nebula.html">Chaco Canyon Anasazi art online</a>. In addition, Ralph R. Robbins of the University of Texas has found Mimbres Indian art from New Mexico, possibly depicting the supernova.</div>
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The Supernova 1054 was also assigned the variable star designation CM Tauri. It is one of few <a href="http://messier.obspm.fr/more/mw_sn.html">historically observed supernovae</a> in our <a href="http://messier.obspm.fr/more/mw.html">Milky Way Galaxy</a>.</div>
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The nebulous remnant was discovered by <a href="http://messier.obspm.fr/xtra/Bios/bevis.html">John Bevis</a> in 1731, who <a href="http://messier.obspm.fr/more/m001_bevis.html">added it</a> to his sky atlas, <i>Uranographia Britannica</i>. <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> independently <a href="http://messier.obspm.fr/xtra/history/m-m001.html">found it</a> on August 28, 1758, when he was looking for comet Halley on its first predicted return, and first thought it was a comet. Of course, he soon recognized that it had no apparent proper motion, and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M1">cataloged it</a> on September 12, 1758. It was the discovery of this object which caused Charles Messier to begin with the compilation of <a href="http://messier.obspm.fr/xtra/history/m-cat.html">his catalog</a>. It was also the discovery of this object, which closely resembled a comet (1758 De la Nux, C/1758 K1) in his small refracting telescope, which brought him to the idea to search for comets with telescopes (see his<a href="http://messier.obspm.fr/xtra/history/notes-c.html#1801note">note</a>). Messier acknowledged the prior, original discovery by Bevis when he learned of it in a letter of June 10, 1771.</div>
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Although Messier's catalog was primarily compiled for preventing confusion of these objects with comets, M1 was again confused with comet Halley on the occasion of that comet's second predicted return in 1835.</div>
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This nebula was christened the "Crab Nebula" on the ground of a <a href="http://messier.obspm.fr/more/m001_rosse.html">drawing made by Lord Rosse</a> about 1844. Of the early observers, Messier, Bode and William Herschel correctly remarked that this nebula is not resolvable into stars, but William Herschel thought that it was a stellar system which should be resolvable by larger telescopes. John Herschel and Lord Rosse erroneously thought it is "barely resolvable" into stars. </div>
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LEIA MAIS</div>
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em</div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEghGz_KRCgBElWPAZduQ74fLpl3c7RJlgmmM9u8eScVyiXxMFzmB1Dzgw0TMNZ_LzO2rIYzP-_w0Lyo1ebfHpxvATCVd8te7nEt03VjK5-_7c3UT59YTDQaMF3_l9az-ihM3WjCcsCUOuI/s1600/m1_hst_900.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEghGz_KRCgBElWPAZduQ74fLpl3c7RJlgmmM9u8eScVyiXxMFzmB1Dzgw0TMNZ_LzO2rIYzP-_w0Lyo1ebfHpxvATCVd8te7nEt03VjK5-_7c3UT59YTDQaMF3_l9az-ihM3WjCcsCUOuI/s1600/m1_hst_900.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-color: #faf2d9; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></span></div>
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<a href="https://www.blogger.com/blogger.g?blogID=2442159895732486967" imageanchor="1" style="clear: right; color: #274e13; float: right; line-height: 22.3999996185303px; margin-bottom: 1em; margin-left: 1em; text-decoration: none;"></a><a href="https://www.blogger.com/blogger.g?blogID=2442159895732486967" imageanchor="1" style="clear: right; color: #274e13; float: right; line-height: 22.3999996185303px; margin-bottom: 1em; margin-left: 1em; text-decoration: none;"></a><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>M1: The Crab Nebula from Hubble </b><br /><b>Image Credit: </b><a href="http://www.nasa.gov/" style="color: #274e13; text-decoration: none;">NASA</a>, <a href="http://hubble.esa.int/" style="color: #274e13; text-decoration: none;">ESA</a>, J. Hester, A. Loll (<a href="http://sese.asu.edu/" style="color: #274e13; text-decoration: none;">ASU</a>); Acknowledgement: Davide De Martin (<a href="http://www.skyfactory.org/" style="color: #274e13; text-decoration: none;">Skyfactory</a>)</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>NEBULOSA DO CARANGUEJO, M1, NGC 1952!</b></span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC 1952 - M 1 - Taurus - Nebulosa Resto de Supernova - Caranguejo<o:p></o:p></span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 05h33m Declinação +22<sup>o</sup>.05<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo Nebulosa Planetária SN Dimensão 5,0 Magnitude 19<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude da Estrela associada 16V Distância em anos-luz 4,0<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Por volta do ano 5500 antes de cristo, uma imensa estrela explodiu como Supernova... seis mil e quinhentos anos mais tarde, em 4 de julho de 1054, astrônomos japoneses e chineses puderam observar a aparição de uma 'estrela convidada" no céu na constelação que hoje denominamos de Touro. Essa nova estrela, tão brilhante quanto Vênus, pôde ser vista durante o dia por cerca de 23 dias e durante dois anos pôde ser observada e estudada no céu noturno.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Quando a supernova esmaeceu, passaram-se mais 700 anos até que uma pequena nuvem de gás verde luminoso surgiu no lugar onde ela aparecera anteriormente, um grau ao norte e oeste de Zeta Tauri, já em um dos chifres do Touro quase aos pés dos Gêmeos.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Por volta do ano 5500 antes de cristo, uma imensa estrela explodiu como Supernova... seis mil e quinhentos anos mais tarde, em 4 de julho de 1054, astrônomos japoneses e chineses puderam observar a aparição de uma 'estrela convidada" no céu na constelação que hoje denominamos de Touro. Essa nova estrela, tão brilhante quanto Vênus, pôde ser vista durante o dia por cerca de 23 dias e durante dois anos pôde ser observada e estudada no céu noturno.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Quando a supernova esmaeceu, passaram-se mais 700 anos até que uma pequena nuvem de gás verde luminoso surgiu no lugar aonde ela aparecera anteriormente, um grau ao norte e oeste de Zeta Tauri, já em um dos chifres do Touro quase aos pés dos Gêmeos.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Charles Messier (1730-1817) era um caçador de cometas e sempre vasculhava o céu em busca dos mesmos. Em 12 de setembro de 1758 (ou em 28 de Agosto, segundo outro documento - Nota da Tradutora), Messier apontou para esse ponto de luz difusa no céu e o descreveu a nebulosa como contendo nenhuma estrela, esbranquiçada em sua cor e alongada como a chama de uma vela. Mais tarde, Messier veio a saber que tal nebulosa já havia sido avistada por um astrônomo inglês, John Bevis, em 1731.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Messier continuou sua busca por cometas (naquele mesmo houve o retorno, já previsto, do Cometa Halley durante o mês de dezembro) - e passou então, a elaborar uma lista de objetos no céu que não eram cometas. Finalmente, uma versão final dessa lista foi publicada em 1784 contendo 109 ou 110 objetos, sendo que o primeiro objeto mencionado foi a Nebulosa que ora é visitada por Saturno. Essa lista é hoje conhecida como A Lista de Messier e seus objetos são denominados M1, M2, M3.... A Nebulosa do Caranguejo é M1.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">No entanto, esse nome, Nebulosa do Caranguejo foi dado por Earl of Rosse, em 1840 que publicou um desenho da mesma com filamentos que sugeriam o formato de um caranguejo. Mais tarde, ele observou a nebulosa já com outra aparelhagem mais potente e rejeitou sua descrição anterior da mesma.... tarde demais: a Nebulosa do Caranguejo já era assim conhecida!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A Nebulosa do Caranguejo não é difícil de ser localizada com um telescópio mais simples e do quintal de sua casa - afinal foi assim que Messier a encontrou! Porém, em céus mais transparentes, longe das luzes da cidade, sua visão se torna bem mais enriquecida e se você tiver um telescópio possante, será fantástico poder observar um estrela que ainda permanece em seu centro, um pulsar que gira cerca de 30 vezes por segundo!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #274e13;">"<b>A Nebulosa do Caranguejo</b>" é uma re-leitura, síntese e tradução de Janine Milward de artigo extraído da Revista Astronomy em sua edição de novembro na seção "Southern Sky Show" - "The Starry Sky".</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhLtRUYHugjcUeUcMKrHk2qgQ8DWWzTH1QXXz4un9MxUJ7Vds2X-ioImbzE6q02MxL9OS16zSf7rfhPS9HmINLmmDNhQQZvOlxdPHY812W8MitSeF1XFv1iJMhSQFjATAF-mYk4TUCZl4M/s1600/m1_hst_900.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhLtRUYHugjcUeUcMKrHk2qgQ8DWWzTH1QXXz4un9MxUJ7Vds2X-ioImbzE6q02MxL9OS16zSf7rfhPS9HmINLmmDNhQQZvOlxdPHY812W8MitSeF1XFv1iJMhSQFjATAF-mYk4TUCZl4M/s1600/m1_hst_900.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://apod.nasa.gov/apod/ap111225.html</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>M1: The Crab Nebula from Hubble </b><br /><b>Image Credit: </b><a href="http://www.nasa.gov/" style="color: #274e13; text-decoration: none;">NASA</a>, <a href="http://hubble.esa.int/" style="color: #274e13; text-decoration: none;">ESA</a>, J. Hester, A. Loll (<a href="http://sese.asu.edu/" style="color: #274e13; text-decoration: none;">ASU</a>); Acknowledgement: Davide De Martin (<a href="http://www.skyfactory.org/" style="color: #274e13; text-decoration: none;">Skyfactory</a>)</span></div>
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<b><span style="color: #660000; font-size: medium;">A Nebulosa do Caranguejo (também catalogado como <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Catálogo Messier">Messier</a> 1, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">NGC</a> 1952, Taurus A)</span></b><span style="color: #252525;"> é um <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Remanescente de supernova">remanescente de supernova</a> e uma <a href="http://pt.wikipedia.org/wiki/Nebulosa_de_vento_de_pulsar" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa de vento de pulsar">nebulosa de vento de pulsar</a> na<a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> do <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Taurus">Touro</a>. A nebulosa foi primeiramente observada por <a href="http://pt.wikipedia.org/wiki/John_Bevis" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="John Bevis">John Bevis</a> em 1731 e corresponde a uma brilhante <a href="http://pt.wikipedia.org/wiki/Supernova" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Supernova">supernova</a> (<a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="SN 1054">SN 1054</a>) registrada por astrônomos chineses e árabes em 1054. A nebulosa é a mais intensa fonte de <a href="http://pt.wikipedia.org/wiki/Raios_X" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Raios X">raios X</a> e <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Raios_gama" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Raios gama">gama</a> para energias acima de 30 <a href="http://pt.wikipedia.org/wiki/El%C3%A9tron-volt" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Elétron-volt">KeV</a>, com fluxo de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Energia_luminosa" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Energia luminosa">energia luminosa</a> acima de 10<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">12</span> eV. Dista a cerca de 6 500 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (2 quilo<a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Parsec">parsecs</a>) da Terra e tem um diâmetro de 11 anos-luz (3,4 parsecs), expandindo-se a uma taxa de aproximadamente 1 500 quilômetros por segundo.</span></div>
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No centro da nebulosa há o <a href="http://pt.wikipedia.org/wiki/Pulsar_do_Caranguejo" style="background: none; color: #0b0080; text-decoration: none;" title="Pulsar do Caranguejo">Pulsar do Caranguejo</a>, uma <a href="http://pt.wikipedia.org/wiki/Estrela_de_n%C3%AAutrons" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela de nêutrons">estrela de nêutrons</a> com 28 a 30 quilômetros de diâmetro,<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#cite_note-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> que emite pulsos periódicos de radiação que abrange quase todo o <a href="http://pt.wikipedia.org/wiki/Espectro_eletromagn%C3%A9tico" style="background: none; color: #0b0080; text-decoration: none;" title="Espectro eletromagnético">espectro eletromagnético</a>, com uma <a href="http://pt.wikipedia.org/wiki/Frequ%C3%AAncia" style="background: none; color: #0b0080; text-decoration: none;" title="Frequência">frequência</a> de 30,2 vezes por segundo, evidenciando uma rotação com período de apenas 33 milissegundos. Foi o primeiro objeto astronômico associado a uma explosão de supernova.</div>
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Age como uma fonte de radiação para o estudo de <a href="http://pt.wikipedia.org/wiki/Corpo_celeste" style="background: none; color: #0b0080; text-decoration: none;" title="Corpo celeste">corpos celestes</a> que por vezes a <a href="http://pt.wikipedia.org/wiki/Oculta%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Ocultação">ocultam</a>. Na década de 1950 e 1960, a <a href="http://pt.wikipedia.org/wiki/Coroa_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Coroa solar">coroa solar</a> foi mapeada a partir de observações das ondas de rádio da nebulosa que passaram através dela. Em 2003, a espessura da atmosfera de <a href="http://pt.wikipedia.org/wiki/Tit%C3%A3_(sat%C3%A9lite)" style="background: none; color: #0b0080; text-decoration: none;" title="Titã (satélite)">Titã</a>, satélite de <a href="http://pt.wikipedia.org/wiki/Saturno_(planeta)" style="background: none; color: #0b0080; text-decoration: none;" title="Saturno (planeta)">Saturno</a>, foi medida através do bloqueio de raios-X provenientes da nebulosa pela atmosfera do satélite.</div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.399999618530273px;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo</a></span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.399999618530273px;"><br /></span></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.399999618530273px;"><br /></span></span><img src="http://upload.wikimedia.org/wikipedia/commons/thumb/c/c9/Chandra-crab.jpg/800px-Chandra-crab.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br />http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#mediaviewer/Ficheiro:Chandra-crab.jpg</span></div>
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<span style="background-color: white;"><span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Chandra-crab</span><a class="mw-mmv-license" href="http://commons.wikimedia.org/wiki/File:Chandra-crab.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-size: 0.9em; padding: 0px 10px; text-align: right; text-decoration: none;" target="">Domínio público</a></span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span class="mw-mmv-author">Optical: NASA/HST/ASU/J. Hester et al. X-Ray: NASA/CXC/ASU/J. Hester et al.</span> - <span class="mw-mmv-source"><a class="external free" href="http://hubblesite.org/newscenter/newsdesk/archive/releases/2002/24/image/a" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://hubblesite.org/newscenter/newsdesk/archive/releases/2002/24/image/a</a></span></span></div>
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<span style="background-color: white;">O Pulsar do Caranguejo. Esta imagem combina informações ópticas do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Hubble</a> (em vermelho) e imagens de <a href="http://pt.wikipedia.org/wiki/Astronomia_de_raios-X" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Astronomia de raios-X">raios-X</a> do <a href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_de_raios-X_Chandra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Observatório de raios-X Chandra">Observatório de raios-X Chandra</a> (em azul).</span></div>
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<span style="background-color: white;">A composite image of the Crab Nebula showing the X-ray (blue), and optical (red) images superimposed. The size of the X-ray image is smaller because the higher energy X-ray emitting electrons radiate away their energy more quickly than the lower energy optically emitting electrons as they move</span></div>
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<span class="mw-headline" id="Condi.C3.A7.C3.B5es_f.C3.ADsicas" style="font-size: x-small;">Condições físicas</span></h2>
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Os filamentos observados são restos da <a href="http://pt.wikipedia.org/wiki/Atmosfera" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Atmosfera">atmosfera</a> da estrela progenitora e consistem basicamente de <a href="http://pt.wikipedia.org/wiki/H%C3%A9lio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hélio">hélio</a> e <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Hidrog%C3%AAnio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hidrogênio">hidrogênio</a> <a href="http://pt.wikipedia.org/wiki/Ioniza%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ionização">ionizado</a>, juntamente com <a href="http://pt.wikipedia.org/wiki/Carbono" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Carbono">carbono</a>, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Oxig%C3%AAnio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Oxigênio">oxigênio</a>,<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Nitrog%C3%AAnio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nitrogênio">nitrogênio</a>, <a href="http://pt.wikipedia.org/wiki/Ferro" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ferro">ferro</a>, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ne%C3%B4nio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Neônio">neônio</a> e <a href="http://pt.wikipedia.org/wiki/Enxofre" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Enxofre">enxofre</a>. A temperatura dos gases nesses filamentos é de 11 000 a 18 000 <a href="http://pt.wikipedia.org/wiki/Kelvin" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Kelvin">kelvin</a> e sua <a href="http://pt.wikipedia.org/wiki/Densidade" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Densidade">densidade</a> é de 1 300 partículas por <a href="http://pt.wikipedia.org/wiki/Cent%C3%ADmetro_c%C3%BAbico" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Centímetro cúbico">centímetro cúbico</a>.<span class="reference" id="cite_ref-Fesenetal1982_17-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#cite_note-Fesenetal1982-17" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">17</a></span>Considerando-se a <a href="http://pt.wikipedia.org/wiki/Luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Luz">luz visível</a>, a Nebulosa do Caranguejo é composta de uma massa <a href="http://pt.wikipedia.org/wiki/Oval" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Oval">oval</a> de filamentos, com diâmetro angular de aproximadamente 6x4 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a> em torno de uma região central azul difusa. Como comparação, a <a href="http://pt.wikipedia.org/wiki/Lua_cheia" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Lua cheia">lua cheia</a> tem 30 minutos de arco de diâmetro. Em três dimensões, especula-se que a nebulosa tenha a forma de um <a href="http://pt.wikipedia.org/wiki/Esferoide_prolato" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Esferoide prolato">esferoide prolato</a>.<span class="reference" id="cite_ref-Trimble1973_3-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#cite_note-Trimble1973-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> Ao longo de sua maior dimensão visível, a nebulosa mede cerca de (13 ± 3) anos-luz.</div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/5/59/Filaments_in_the_Crab_Nebula.jpg/640px-Filaments_in_the_Crab_Nebula.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#mediaviewer/Ficheiro:Filaments_in_the_Crab_Nebula.jpg</span></span></div>
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<span style="background-color: white;">Imagem do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a> de uma pequena região da Nebulosa do Caranguejo, mostrando sua intricada estrutura filamentar. Crédito:<a href="http://pt.wikipedia.org/wiki/NASA" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NASA">NASA</a>/<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/ESA" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="ESA">ESA</a>.</span></div>
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<span style="background-color: white;">Hubble Space Telescope image of filaments in the Crab Nebula (M1, NGC 1952).</span></div>
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Em 1953, o russo <a href="http://pt.wikipedia.org/wiki/Iosif_Shklovsky" style="background: none; color: #0b0080; text-decoration: none;" title="Iosif Shklovsky">Iosif Shklovsky</a> propôs que a região azul difusa fosse produzida por <a href="http://pt.wikipedia.org/wiki/Radia%C3%A7%C3%A3o_s%C3%ADncrotron" style="background: none; color: #0b0080; text-decoration: none;" title="Radiação síncrotron">radiação síncrotron</a>, que é a radiação emitida pelo movimento curvilíneo de <a href="http://pt.wikipedia.org/wiki/El%C3%A9tron" style="background: none; color: #0b0080; text-decoration: none;" title="Elétron">elétrons</a> em velocidades próximas à <a href="http://pt.wikipedia.org/wiki/Velocidade_da_luz" style="background: none; color: #0b0080; text-decoration: none;" title="Velocidade da luz">velocidade da luz</a>.<span class="reference" id="cite_ref-18" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#cite_note-18" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">18</a></span> Três anos depois, a hipótese foi confirmada a partir das observações. Na década de 1960, verificou-se que a origem das trajetórias curvas dos elétrons era devida ao forte <a href="http://pt.wikipedia.org/wiki/Campo_magn%C3%A9tico" style="background: none; color: #0b0080; text-decoration: none;" title="Campo magnético">campo magnético</a> produzido por uma <a href="http://pt.wikipedia.org/wiki/Estrela_de_n%C3%AAutrons" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela de nêutrons">estrela de nêutrons</a> no centro da nebulosa.</div>
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A Nebulosa do Caranguejo é foco de muita atenção dos astrônomos, mas a sua distância à Terra permanece uma questão em aberto devido às grandes incertezas em cada método utilizado para calcular sua distância. Fotografias tomadas ao longo de vários anos revelam a lenta expansão da nebulosa,<span class="reference" id="cite_ref-19" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#cite_note-19" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">19</a></span> e comparando esta expansão angular observada no céu com a sua velocidade de expansão determinada através da <a href="http://pt.wikipedia.org/wiki/Espectroscopia" style="background: none; color: #0b0080; text-decoration: none;" title="Espectroscopia">análise espectroscópica</a>, a distância da nebulosa em relação à Terra pode ser estimada com mais precisão. Em 1973, uma análise a partir dos diversos métodos utilizados para calcular a distância à nebulosa alcançou a conclusão de 6 300 anos-luz.<span class="reference" id="cite_ref-Trimble1973_3-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#cite_note-Trimble1973-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> As estimativas mais recentes dão conta que sua distância em relação à Terra é de (6,5 ± 1,8) x 10³ anos-luz, o que equivale a (2,0 ± 0,5) <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>, e que está se expandindo a uma taxa de aproximadamente 1 500 quilômetros por segundo.<span class="reference" id="cite_ref-Bietneholz_20-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#cite_note-Bietneholz-20" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">20</a></span></div>
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Seguindo cronologicamente de forma retrógrada e uniforme sua expansão, alcança-se uma data várias décadas após 1054, o que implica que a sua velocidade de expansão tem acelerado desde a explosão da supernova.<span class="reference" id="cite_ref-Trimble1968_21-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#cite_note-Trimble1968-21" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">21</a></span> Acredita-se que esta aceleração seja causada pela energia do <a href="http://pt.wikipedia.org/wiki/Pulsar" style="background: none; color: #0b0080; text-decoration: none;" title="Pulsar">pulsar</a>, que de alguma forma interfere com o <a href="http://pt.wikipedia.org/wiki/Campo_magn%C3%A9tico" style="background: none; color: #0b0080; text-decoration: none;" title="Campo magnético">campo magnético</a> da nebulosa, que se expande e força seus filamentos em direção ao espaço vazio.<span class="reference" id="cite_ref-Bejgeretal2003_22-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#cite_note-Bejgeretal2003-22" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">22</a></span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">Acredita-se que o pulsar do Caranguejo tenha cerca de 28 a 30 km de diâmetro.30 Emite pulsos de radiação a cada 33 milissegundos,31 e são emitidos em comprimentos de onda que abrangem praticamente todo o espectro eletromagnético, desde as ondas de rádio aos raios gama. Como todos os pulsares, o seu período de rotação está diminuindo gradualmente. Ocasionalmente, o seu período de rotação passa mudanças bruscas, conhecidas como "falhas", que se acredita serem causadas por um realinhamento repentino da massa da estrela de nêutrons, mudando seu momento de inércia e sua velocidade angular para que seu momento angular seja conservado. A energia liberada quando o pulsar desacelera é enorme e causa uma maior emissão da radiação síncrotron, que tem uma luminosidade total aproximadamente 75 000 vezes maior que a do Sol.32</span></span></div>
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<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="line-height: 22.399999618530273px;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo</a></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>SAIBA MUITO, MUITO MAIS</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>SOBRE A NEBULOSA DO CARANGUEJO</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://chandra.harvard.edu/xray_sources/crab/crab.htm" style="color: #274e13; text-decoration: none;">http://chandra.harvard.edu/xray_sources/crab/crab.htm</a></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">PÁGINA DA CHANDRA SOBRE A NEBULOSA</span></div>
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<span style="background-color: white;"><span style="color: #073763; font-size: medium;">Hubble Astronomers Unveil "Crab Nebula - The Movie"</span></span></h1>
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<span class="text-holder" style="float: right; width: 248px;"><a href="http://hubblesite.org/newscenter/archive/releases/1996/22/video/a/" style="color: #993333; text-decoration: none;">Crab Nebula -- The Movie</a><span class="running-time" style="color: #666666; display: block; font-style: oblique;"><strong>Running Time: </strong>10 seconds</span></span><a href="http://hubblesite.org/newscenter/archive/releases/1996/22/video/a/" style="color: #993333; text-decoration: none;"><img alt="Crab Nebula -- The Movie" class="icon" src="http://imgsrc.hubblesite.org/hu/db/1996/22/videos/a/thumb.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(103, 32, 29); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<span class="text-holder" style="float: right; width: 248px;"><a href="http://hubblesite.org/newscenter/archive/releases/1996/22/video/b/" style="color: #993333; text-decoration: none;">Animation Depicting the Environment Around the Pulsar</a><span class="running-time" style="color: #666666; display: block; font-style: oblique;"><strong>Running Time: </strong>18 seconds</span></span><a href="http://hubblesite.org/newscenter/archive/releases/1996/22/video/b/" style="color: #993333; text-decoration: none;"><img alt="Animation Depicting the Environment Around the Pulsar" class="icon" src="http://imgsrc.hubblesite.org/hu/db/1996/22/videos/b/thumb.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(103, 32, 29); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a><span class="artists-concept" style="color: #666666; display: block; font-size: 9px; font-style: oblique; line-height: 12.600000381469727px; text-align: center; width: 82px;">Artist's Concept</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj6UOWbS_ej6PdgPIyv-xbt5x8MK6QTCddQKeJ5qIOKdTSBgPMOgVHFjaQFq-wLPYfT8QGvdwub2lMjEGW129NuN2qCGiYVEc8O1N8Mz9IK6-PL25AaMZQWF0mQlL49qEUl04HVaMNaBuo/s1600/m1animation_block_bw.gif" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj6UOWbS_ej6PdgPIyv-xbt5x8MK6QTCddQKeJ5qIOKdTSBgPMOgVHFjaQFq-wLPYfT8QGvdwub2lMjEGW129NuN2qCGiYVEc8O1N8Mz9IK6-PL25AaMZQWF0mQlL49qEUl04HVaMNaBuo/s1600/m1animation_block_bw.gif" height="522" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.399999618530273px;"><a href="http://apod.nasa.gov/apod/ap011227.html" style="color: #274e13; text-decoration: none;">http://apod.nasa.gov/apod/ap011227.html</a></span></span></div>
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<b>The Incredible Expanding Crab </b><br /><b>Credit: </b>Courtesy <a href="mailto:ablock@noao.edu" style="color: #274e13; text-decoration: none;">Adam Block</a> (<a href="http://www.noao.edu/outreach/nop/pop.html" style="color: #274e13; text-decoration: none;">KPNO Visitor Program</a>), <a href="http://www.noao.edu/" style="color: #274e13; text-decoration: none;">NOAO</a>, <a href="http://www.nsf.gov/" style="color: #274e13; text-decoration: none;">NSF</a></center>
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<b>Explanation: </b>The Crab Nebula is cataloged as M1, the first on <a href="http://apod.nasa.gov/apod/ap960626.html" style="color: #274e13; text-decoration: none;">Charles Messier's</a> famous list of things which are not comets. In fact, <a href="http://apod.nasa.gov/apod/ap010602.html" style="color: #274e13; text-decoration: none;">the Crab is</a> now known to be a supernova remnant, an expanding cloud of debris from the explosion of a massive star. The violent birth of the Crab was <a href="http://www.seds.org/messier/more/m001_sn.html" style="color: #274e13; text-decoration: none;">witnessed by astronomers</a> in the year 1054. Roughly 10 light-years across today, the nebula is still expanding at a rate of over 1,000 kilometers per second. Flipping between two images made nearly 30 years apart, this animation clearly demonstrates the expansion. The smaller Crab was recorded as a <a href="http://www.noao.edu/image_gallery/html/im0345.html" style="color: #274e13; text-decoration: none;">photographic image</a> made in 1973 using the <a href="http://www.noao.edu/kpno/" style="color: #274e13; text-decoration: none;">Kitt Peak</a> National Observatory 4-meter telescope in 1973. <a href="http://www.noao.edu/outreach/aop/observers/m1.html" style="color: #274e13; text-decoration: none;">The expanded Crab</a> was made this year with the Kitt Peak <a href="http://www.noao.edu/outreach/nop/pop.html" style="color: #274e13; text-decoration: none;">Visitor Center's</a> 0.4-meter telescope and digital camera. Background stars were used to register the two images.</div>
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<b><span style="color: #660000; font-size: medium;">Supernova</span></b><span style="color: #252525;"><span style="font-size: 14px;"> </span>é o nome dado aos corpos celestes surgidos após as explosões de </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a><span style="color: #252525;"> (estimativa) com mais de 10 </span><a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Massa solar">massas solares</a><span style="color: #252525;">, que produzem objetos extremamente brilhantes, os quais declinam até se tornarem invisíveis, passadas algumas semanas ou meses. Em apenas alguns dias o seu brilho pode intensificar-se em 1 bilhão de vezes a partir de seu estado original, tornando a estrela tão brilhante quanto uma galáxia, mas, com o passar do tempo, sua temperatura e brilho diminuem até chegarem a um grau inferior aos primeiros.</span></div>
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A explosão de uma supernova pode expulsar para o espaço até 90% da <a href="http://pt.wikipedia.org/wiki/Mat%C3%A9ria" style="background: none; color: #0b0080; text-decoration: none;" title="Matéria">matéria</a> de uma <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a>. O núcleo remanescente tem massa superior a 1,5 massas solares, a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Press%C3%A3o_de_Degeneresc%C3%AAncia" style="background: none; color: #0b0080; text-decoration: none;" title="Pressão de Degenerescência">Pressão de Degenerescência</a> dos <a href="http://pt.wikipedia.org/wiki/El%C3%A9tron" style="background: none; color: #0b0080; text-decoration: none;" title="Elétron">elétrons</a> não é mais suficiente para manter o núcleo estável; então os <a href="http://pt.wikipedia.org/wiki/El%C3%A9tron" style="background: none; color: #0b0080; text-decoration: none;" title="Elétron">elétrons</a> colapsam com o núcleo, chocando-se com os <a href="http://pt.wikipedia.org/wiki/Pr%C3%B3ton" style="background: none; color: #0b0080; text-decoration: none;" title="Próton">prótons</a>, originando<a href="http://pt.wikipedia.org/wiki/N%C3%AAutron" style="background: none; color: #0b0080; text-decoration: none;" title="Nêutron">nêutrons</a>: o resultado é uma estrela composta de <a href="http://pt.wikipedia.org/wiki/N%C3%AAutron" style="background: none; color: #0b0080; text-decoration: none;" title="Nêutron">nêutrons</a>, com aproximadamente 15 km de diametro e extremamente densa, conhecida como <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Estrela_de_n%C3%AAutron" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela de nêutron">estrela de nêutrons</a> ou <a href="http://pt.wikipedia.org/wiki/Pulsar" style="background: none; color: #0b0080; text-decoration: none;" title="Pulsar">pulsar</a>. Mas, quando a massa desse núcleo ultrapassa 3 massas solares, nem mesmo a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Press%C3%A3o_de_Degeneresc%C3%AAncia" style="background: none; color: #0b0080; text-decoration: none;" title="Pressão de Degenerescência">Pressão de Degenerescência</a> dos <a href="http://pt.wikipedia.org/wiki/N%C3%AAutron" style="background: none; color: #0b0080; text-decoration: none;" title="Nêutron">nêutrons</a> consegue manter o núcleo; então a estrela continua a se colapsar, dando origem a uma <a href="http://pt.wikipedia.org/wiki/Singularidade_gravitacional" style="background: none; color: #0b0080; text-decoration: none;" title="Singularidade gravitacional">singularidade</a> no espaço-tempo, conhecida como <a href="http://pt.wikipedia.org/wiki/Buraco_negro" style="background: none; color: #0b0080; text-decoration: none;" title="Buraco negro">buraco negro</a>, cuja <a href="http://pt.wikipedia.org/wiki/Velocidade_de_escape" style="background: none; color: #0b0080; text-decoration: none;" title="Velocidade de escape">velocidade de escape</a> é maior do que a velocidade da luz.</div>
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Atualmente, são utilizadas como velas-padrão para estudos da expansão do universo, técnica similar à utilizada por <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Edwin_Hubble" style="background: none; color: #0b0080; text-decoration: none;" title="Edwin Hubble">Edwin Hubble</a> com <a href="http://pt.wikipedia.org/wiki/Cefeida" style="background: none; color: #0b0080; text-decoration: none;" title="Cefeida">cefeidas</a>, mas, com eficiência muito maior, pois o brilho das Supernovas é bem maior.</div>
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LEIA MAIS em</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Supernova</span></span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/4/40/Crab_Nebula_NGC_1952_%28composite_from_Chandra%2C_Hubble_and_Spitzer%29.jpg/800px-Crab_Nebula_NGC_1952_%28composite_from_Chandra%2C_Hubble_and_Spitzer%29.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px; padding: 8px; text-align: -webkit-center;" /></div>
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<span style="background-color: white;"><span class="mw-mmv-title" original-title="File name" style="font-size: 1.2em; max-width: 60%;">Crab Nebula NGC 1952 (composite from Chandra, Hubble and Spitzer)</span></span></div>
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<span class="mw-mmv-source-author mw-mmv-reduce-toolong mw-mmv-truncate-toolong" original-title="Author and source information" style="background-color: white; cursor: pointer; font-size: 0.8em;"><span class="mw-mmv-author">X-Ray: NASA/CXC/J.Hester (ASU); Optical: NASA/ESA/J.Hester & A.Loll (ASU); Infrared: NASA/JPL-Caltech/R.Gehrz (Univ. Minn.)</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.spitzer.caltech.edu/images/2857-sig09-009-NASA-s-Great-Observatories-View-of-the-Crab-Nebula" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://www.spitzer.caltech.edu/images/2857-sig09-009-NASA-s-Great-Observatories-View-of-the-Crab-Nebula</a> (<a class="external text" href="http://www.spitzer.caltech.edu/uploaded_files/images/0005/7591/sig09-009.jpg" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">direct link</a>)</span></span><br />
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<span style="line-height: normal;"><b><span style="font-family: Arial, Helvetica, sans-serif;">EM 04 de janeiro de 2003, SATURNO VISITOU </span></b></span></div>
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<span style="line-height: normal;"><b><span style="font-family: Arial, Helvetica, sans-serif;">M1, A NEBULOSA DO CARANGUEJO!</span></b></span></div>
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<span style="line-height: normal;"><span style="font-family: Arial, Helvetica, sans-serif;">Eu me senti tão emocionada com aquele encontro que escrevi um conto surreal .</span></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif; font-size: medium;">O Tempo e o Sonho da Luz do Passado</span></h3>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">(Uma conversa entre Saturno e a Nebulosa do Caranguejo, </span><br />
<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">ouvida da Terra</span><br />
<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"> - um conto surreal...)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Saturno - Nasa</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEghGz_KRCgBElWPAZduQ74fLpl3c7RJlgmmM9u8eScVyiXxMFzmB1Dzgw0TMNZ_LzO2rIYzP-_w0Lyo1ebfHpxvATCVd8te7nEt03VjK5-_7c3UT59YTDQaMF3_l9az-ihM3WjCcsCUOuI/s1600/m1_hst_900.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEghGz_KRCgBElWPAZduQ74fLpl3c7RJlgmmM9u8eScVyiXxMFzmB1Dzgw0TMNZ_LzO2rIYzP-_w0Lyo1ebfHpxvATCVd8te7nEt03VjK5-_7c3UT59YTDQaMF3_l9az-ihM3WjCcsCUOuI/s1600/m1_hst_900.jpg" height="347" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="400" /></a></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://apod.nasa.gov/apod/ap111225.html</span></div>
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<a href="https://www.blogger.com/blogger.g?blogID=2442159895732486967" imageanchor="1" style="clear: right; color: #274e13; float: right; line-height: 22.399999618530273px; margin-bottom: 1em; margin-left: 1em; text-decoration: none;"></a><a href="https://www.blogger.com/blogger.g?blogID=2442159895732486967" imageanchor="1" style="clear: right; color: #274e13; float: right; line-height: 22.399999618530273px; margin-bottom: 1em; margin-left: 1em; text-decoration: none;"></a><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>M1: The Crab Nebula from Hubble </b><br /><b>Image Credit: </b><a href="http://www.nasa.gov/" style="color: #274e13; text-decoration: none;">NASA</a>, <a href="http://hubble.esa.int/" style="color: #274e13; text-decoration: none;">ESA</a>, J. Hester, A. Loll (<a href="http://sese.asu.edu/" style="color: #274e13; text-decoration: none;">ASU</a>); Acknowledgement: Davide De Martin (<a href="http://www.skyfactory.org/" style="color: #274e13; text-decoration: none;">Skyfactory</a>)</span></div>
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<span style="line-height: normal;"><span style="color: #274e13;">2003 January 10 </span></span></div>
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<span style="color: #274e13;"><b>The Crab that Played with the Planet </b><br /><b>Credit & Copyright: </b><a href="http://www.newastro.com/newastro/default.asp" style="color: #274e13; text-decoration: none;">Ron Wodaski</a>, <a href="http://www.newastro.com/remote/" style="color: #274e13; text-decoration: none;">Newastro Remote Telescope</a> at <a href="http://www.nmskies.com/" style="color: #274e13; text-decoration: none;">New Mexico Skies</a></span></center>
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<span style="color: #274e13;"><b>Explanation: </b><a href="http://es.rice.edu/ES/humsoc/Galileo/Things/saturn.html" style="color: #274e13; text-decoration: none;">Wandering</a> through the constellation Taurus, <a href="http://science.nasa.gov/headlines/y2002/13dec_saturn.htm" style="color: #274e13; text-decoration: none;">Saturn made</a> its closest approach to planet Earth last month, tilting its lovely rings toward appreciative skygazers while rising high in midnight skies. On January 4th and 5th, Saturn also crossed in front of the <a href="http://www.boop.org/jan/justso/crab.htm" style="color: #274e13; text-decoration: none;">high and far-off</a> Crab Nebula (M1), a cosmic cloud of debris from a stellar explosion and first on the list of astronomer <a href="http://apod.nasa.gov/apod/ap960626.html" style="color: #274e13; text-decoration: none;">Charles Messier's</a> celestial sights. But <a href="http://www.marcush.net/astronomy/m1.html" style="color: #274e13; text-decoration: none;">Saturn and the Crab</a> made poor playmates, as light from the bright planet overwhelmed the the diffuse nebula, all but hiding the Crab <a href="http://www.surveyor.in-berlin.de/himmel/indexe.html#saturn" style="color: #274e13; text-decoration: none;">during the transit</a>. Taken on January 2nd, a few days before their closest encounter, this composite digital image illustrates the problem. The <a href="http://www.seds.org/messier/m/m001.html" style="color: #274e13; text-decoration: none;">subtle nebula</a> is just visible at the right, while on the left, light from a drastically over-exposed Saturn overflows its pixels. Composited into the image is a correctly exposed picture of <a href="http://apod.nasa.gov/apod/ap021104.html" style="color: #274e13; text-decoration: none;">ringed Saturn</a> with the Saturnian moons labeled. The well-exposed Saturn image was also taken on January 2nd, but captured with an exposure lasting only a fraction of a second, in contrast with the tens of seconds of exposure time required to reveal the Crab.</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium trabalhado no Programa Corel - para a data de 04 de janeiro de 2003</span></div>
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<span class="mw-mmv-source-author mw-mmv-reduce-toolong mw-mmv-truncate-toolong" original-title="Author and source information" style="background-color: white; cursor: pointer;"><span class="mw-mmv-source" style="color: #660000; font-size: medium;"><b style="font-family: Arial, Helvetica, sans-serif; line-height: 22.399999618530273px;">NEBULOSA DO CARANGUEJO, M1, NGC 1952!</b></span></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">........................... Uma estrela que certa dia explodiu, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">tornando-se uma chamada supernova,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e que, com o passar do tempo, tornou-se uma nuvem...;</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">nuvem penetrada por lentes ópticas </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">comandadas por olhares penetrantes e estudiosos...; </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">nuvem que foi revelando, descobrindo, não mais cobrindo,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">seus segredos de vida (quase) infinita, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">vida que sempre encontra </span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">uma nova maneira de ser, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">vida que se transforma em nova vida,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">através um novo coração, um pulsar, uma estrela de nêutrons, uma nova estrela<b>!</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Tempo e Espaço atuando através a eterna continuidade da Vida.</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif; font-size: medium;">O Tempo e o Sonho da Luz do Passado</span></h3>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">(Uma conversa entre Saturno e a Nebulosa do Caranguejo,</span><br />
<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"> ouvida da Terra</span><br />
<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"> - um conto surreal...)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Saturno andava pelos lados do Touro, cumprindo sua jornada em torno de sua estrela, nosso Sol. Do ponto de vista da Terra, Saturno se encontrava em movimento retrógrado, ainda cumprimentando uma vez mais e se despedindo das estrelas que compõem os chifres daquela constelação pertencente ao Zodíaco, a Roda dos Animais.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Certa noite, de 4 para 5 de janeiro de 2003, Saturno ia passando através da Nebulosa do Caranguejo (do ponto de vista da Terra) e pôde-se escutar essa conversa:</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - Tempo! Ó Tempo! Ó Ceifador de vidas!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Saturno olhou de um lado para o outro e apenas podia ver uma nuvem difusa, com o centro azul esmeralda e as bordas amareladas, alaranjadas e avermelhadas ainda com riscos desencontrados e firulados esbranquiçados, desenhando sua visão... que bela visão!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Sim, quem me chama?</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - Sou eu, M1, a Nebulosa do Caranguejo como sou conhecida na Terra, sua irmã de seu sistema solar.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Olá, Nebulosa, eu já havia passado bem perto de você quando estava em meu movimento direto, já ansioso para deixar o Touro e me deixar enroscar pelos pés dos Gêmeos... mas a Terra me deu mais um movimento retrógrado... e eis-me aqui, voltando uns poucos graus Touro adentro até retomar meu movimento direto no final do mês de fevereiro... Mas, que bom revê-la, Nebulosa, assim tão difusa e maravilhante como um sonho de uma noite de verão... ou de inverno.... pois que não é verdade que você se situa bem próximo do ponto do Solstício de Junho, que traz o verão para o hemisfério norte e o inverno para o hemisfério sul?</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - É bem verdade. Obviamente, esse será sempre seu ponto de vista de acordo com o lugar do espaço que você e seu sistema solar ocupam, meu caro Khronos. Nada no universo possui um lugar próprio, você bem sabe disso. Esse lugar aparentemente próprio será sempre designado por aquele que o observa e do ponto de vista de quem observa, naturalmente! Assim, para os Terrestres meu posicionamento é Ascensão Reta 05h 34m 30s e Declinação. +21 graus e 01 min.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - O Tempo contado a partir do ponto de vista da Terra é apenas uma objetividade dentro da total subjetividade do espaço e do tempo do universo - nisso você tem razão. Assim, para nós nesse sistema solar, o resto do universo parece quase não se mover.... por isso os antigos denominavam que tudo aquilo no universo para além de mim, Saturno, O Deus do Tempo, eram "estrelas fixas". Hoje, sabemos que não apenas nada é fixo no universo, como tudo se movimenta sempre, além da infinita expansão a qual, aparentemente, estamos destinados, nos separando cada vez mais uns dos outros, cada vez mais.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - Diga-me, Deus do Tempo, por que seu também sou chamada de M1?</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Charles Messier foi um caçador de cometas e de tal maneira estava interessado em descobrir novos cometas nos céus que fez uma lista dos objetos celestes que não eram cometas - assim ele poderia continuar em suas buscas já deixando de lado aqueles objetos eliminados! Então, ironicamente, foi exatamente esta lista que o colocou na história da astronomia - apesar de ele ter sido o descobridor ou co-descobridor de cerca de 13 cometas ao longo de sua vida.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">O ano de 1758 foi um ano de expectativa de retorno do Cometa Halley, que na verdade, foi primeiramente encontrado por Palitzsch em 25 de dezembro e mais tarde, no ano seguinte, visto novamente por Messier em 21 de janeiro. Porém, ainda em 28 de Agosto de 1758, enquanto esquadrinhava os céus procurando pelo cometa, Messier encontrou uma nebulosa que acabou imortalizando seu nome e assim ele a descreveu em seus alfarrábios: ".... 28 de Agosto... ela se encontra acima do chifre mais ao sul do Taurus, sem conter qualquer estrela, tendo um névoa esbranquiçada, alongada e contornada como a luz de uma vela...." Era M1, a Nebulosa do Caranguejo, você!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Houve um tempo num passado não muito distante em que aquele pedaço do céu deu lugar a uma "estrela visitante" que surgiu com sua imensa luz mesmo durante o tempo da luz do Sol ao longo de 23 dias, maravilhando os povos que a observaram atentamente. Isso aconteceu em 04 de julho de 1054.... e por ainda mais dois anos, puderam os maravilhados Terrestres ainda observarem sua luz inebriante no céu noturno.... até que finalmente, seu brilho foi esmaecendo, esmaecendo, esmaecendo, até que desapareceu por completo, tão subitamente assim como havia chegado! E foi somente recentemente (com a ajuda de bons telescópios) que os Terrestres puderam voltar a ver aquela estrela - ou a memória do que ela havia sido no passado - através da nuvem de gases firulantes e coloridos que foram soprados, largados para trás, como um lenço de seda solto ao vento da escuridão da noite do universo sem fim....</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">............... A verdade é que a explosão dessa estrela aconteceu cerca de 5500 anos antes de cristo...</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - Os Terrestres amantes do céu estão com seus telescópios voltados para nós, não é mesmo? Todos querem se deliciar com a bela visão que formamos num mesmo enquadramento de imagem mostrando você, Tempo, passeando contra o pano de fundo de meus restos de Luz do passado, de meu tapête bordado de sonho e de lembranças da bela e imensa estrela que já fui...</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Não chore, meu sonho, minha ilusão, restos da estrela do passado, luz que se extinguiu mas que aqueceu o espaço em torno e seus planetas e sua vida durante tanto, tanto tempo! Não chore, não chore, você ainda é tão bela, tão cantada, tão encantada, tão sublime! Não é sublime morrer e ainda se deixar viver como um lenço de seda solto ao vento na noite escura, buscada por telescópios que escondem olhares ansiosos e perscrutadores...</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - Mas... eu já fui um sol, um imenso sol, bem maior do que o seu Sol, Tempo.... e no entanto, um dia, comecei a inchar, inchar, inchar, até que finalmente Buummm! explodi! E quando explodi pude ser vista e admirada por tantos outros sóis que de mim compadeceram e por tantos outros planetas e seres que por mim se encantaram! Mas a verdade é que eu deixei de ser um sol para me tornar apenas poeira de estrela e uma nuvem difusa e silenciosa, esvoaçante e inefável como um sonho quase intraduzível....</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Mas você, meu sonho, você não morreu! Você não morreu! Você apenas se transmutou, você viveu a vida que a natureza lhe deu e viveu essa vida desde o seu princípio até o seu final.... e seu final foi apenas um "turning point" ou ponto de mutação, um ponto de transição.... porque nada no universo ou pluriverso realmente morre, apenas transmuta, muda, transforma, re-inicia sua vida através de uma outra forma, outra qualidade, outro modo de ser.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - Mas eu era um sol! Eu aquecia planetas e seres, eu doava vida, eu era a vida.... e hoje, o que sou eu? Sou apenas sonho ou lembrança etérea do meu passado de glória!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Hoje você é uma Nebulosa em uma das suas formas... mas pense bem, o que terá acontecido com todo aquele material e gases ejetados no espaço intergalático depois de sua estonteante explosão?</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">nebulosa: - Bem, eu penso que tudo se dispersou céu a fóra, noite adentro ou a fóra.... tudo o que era vida em mim apenas se tornou lixo, solto, vagando por aí....</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Quando você explodiu, numa galáxia muito distante aonde você morava, minha galáxia, meu país, a Via Láctea, já estava bem formada bem como minha casa, minha família, meu sistema solar. Eu mesmo pude observar você em sua explosão, em seu esmaecimento e quando você deixou sua casca de halo de sonhos sair de seu sol anterior e tornar-se uma nuvem vagante noite escura adentro... Mas também posso saber que seus outros restos têm formado, ao longo do Tempo - eu, Saturno, sendo o Tempo, bem sei disso - outros sóis, outros planetas, outros seres.... Você não pensa nisso? Você percebe que já hoje e certamente no futuro você estará vivendo, partes de você estarão vivendo em outras estrelas, outros planetas, outros seres, outras vidas?</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - É verdade! O Tempo existe não apenas para mim hoje, que sou uma Nebulosa dos sonhos da Luz de outrora, mas também existe para todos os outros restos de mim mesma que vêm vagando universo adentro e afóra, agregando-se e fusionando-se também a outros restos de outras estrelas de outrora que também explodiram!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Assim, você, Nebulosa dos meus sonhos, você é passado, presente e futuro!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Passado porque ainda outras estrelas, planetas e seres do universo mais jovens e distantes que nós ainda não conheceram a luz advinda de sua explosão.... portanto, para eles, você ainda é uma estrela! Você ainda existe enquanto estrela!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Presente, porque para algumas estrelas, planetas e seres você está explodindo nesse exato momento: Buum! - assim, você nesse momento não é apenas uma estrela como também é uma estupenda e estonteante e maravilhante Supernova!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Futuro, porque ainda outras estrelas, planetas e seres em outros cantos ainda mais longínquos e jovens do universo não apenas sequer sonham ou têm a expectativa de ver sua luz nem como estrela nem como supernova e talvez nem como nebulosa mas que certamente serão confeccionados a partir de seus restos deixados vagando pelo universo.... Dessa forma, cara Nebulosa, você nunca deixará de ser uma estrela! Sua Luz será sempre Luz, não importa o tempo - mesmo porque o tempo é eterno e essa eternidade dará sempre berço à sua possibilidade de Luz acontecer!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - Um dia também você não mais me verá, Tempo, nem mesmo como Nebulosa dos seus sonhos... Chegará um dia em que eu desvanecei por completo e em meu lugar apenas restará a escuridão dos céus.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Minha doce Nebulosa, mesmo que você hoje já seja um tanto apagada a olho nú, brilhando numa magnitude de oitava classe, quero revelar a você um segredo... você sabia que em seu centro, lá no lugar do seu coração, existe uma pulsar que gira 30 vezes por segundo, brilhando numa magnitude de décima sexta classe? Você tem coração! Seu coração bate aceleradamente e pode ser admirado somente por Terrestres munidos por telescópios poderosos!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - Verdade? Sim, eu tenho um coração, assim como tudo no universo possui um coração, objetivo ou subjetivo.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Sim. E seu coração, seu pulsar, é uma estrela de nêutrons, portanto, você ainda é uma estrela!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - O que é uma estrela de nêutrons?</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Bem, quando ultrapassada a fase de gigante vermelha de sua estrela enorme e maciça original, a camada externa foi perdida, dando origem a você, cara Nebulosa do Caranguejo. No entanto, as porções internas dessa estrela em sua explosão, sofreu um colapso tão violento, com sua massa atraída para o interior com tal força, que a massa da porção aniquilada, se compactou ainda para além do estágio de anã branca.... Assim, os elétrons foram forçados a se combinar com os prótons nos núcleos livres, formando nêutrons. Criou-se , então, uma estrela totalmente de nêutrons, sem carga elétrica, os quais se aproximam até se tocar.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - Mas por que então as estrelas de nêutrons também são chamadas de pulsares?</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - As estrelas de nêutrons são pequenas o suficiente para dar um giro numa fração de segundo, sem se desintegrar no processo, graças à intensa gravidade em sua superfície. Elas apresentam um campo magnético fortíssimo, cujos pólos magnéticos não se localizam necessariamente nos pólos de rotação. Os elétrons, extremamente aglutinados pela atração gravitacional, conseguem escapar apenas junto aos pólos magnéticos e ao serem expulsos, perdem energia na forma de micro ondas. Quando a estrela de nêutrons lança as microondas em nossa direção, captamos uma ou duas explosões a cada rotação!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - Então... você quer dizer que meu coração é como um Farol no mar escuro dos céu profundo!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - E você mesma, Nebulosa, é como a chama de uma vela.... assim como Charles Messier bem descreveu você...</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - No entanto, também meu coração vai parando, parando, vagarosamente, e desaparecendo por completo....</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Isso também é uma verdade.... seu coração, seu pulsar, sua estrela de nêutrons, cara Nebulosa, vai perdendo sua energia rotatória à medida que emite microondas, aumentando o período de rotação bem vagarosamente, Na verdade, seu período fica 36,48 bilionésimos de segundo mais longo a cada dia...... Mas, veja por outro lado, é bem possível que este processo ainda dure por bilhões de anos a frente.... tempo suficiente para que você mesma, Nebulosa dos Sonhos, vá se dissipando, apagando - por não possuir mais tanta luz irradiada por sua estrela coronária - anuviando, esfumaçando, desaparecendo.... assim como a imagem do sonho que sai do consciente e retorna ao inconsciente, deixando apenas uma vaga lembrança, doce lembrança.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">.............. Nebulosa e Saturno, o Sonho de hoje e a Luz do Passado juntamente com O Tempo, explodiram em um radioso sorriso de alegria! O Tempo em sua viagem através do Sonho Desmanchado mal havia percebido que o tempo havia passado e os telescópios Terrestres já não mais apontavam para ambos.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tudo não passou de um evento astronômico que ficou no passado.....</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">COM UM ABRAÇO ESTRELADO,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">111 questões sobre a Terra e o Espaço - Isaac Asimov - Editora Best Seller</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Revista Astronomy Now, edição de Março de 1998 - seção Focus - Tema do mês: The Messier Objects: The Messier Marathon por Owen Brazell e The Messier Catalogue - páginas 41 a 52 - Tonbridge, Kent, England</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">"A Nebulosa do Caranguejo" é uma re-leitura, síntese e tradução de Janine de artigo extraído da Revista Astronomy em sua edição de novembro na seção "Southern Sky Show" - "The Starry Sky".</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">Sobre A Nebulosa do Caranguejo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Nos dias 4 e 5 de janeiro de 2003, vimos Saturno, o Deus do Tempo, passeando através de M1,a Nebulosa do Caranguejo.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Por volta do ano 5500 antes de cristo, uma imensa estrela explodiu como Supernova... seis mil e quinhentos anos mais tarde, em 4 de julho de 1054, astrônomos japoneses e chineses puderam observar a aparição de uma 'estrela convidada" no céu na constelação que hoje denominamos de Touro. Essa nova estrela, tão brilhante quanto Vênus, pôde ser vista durante o dia por cerca de 23 dias e durante dois anos pôde ser observada e estudada no céu noturno.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Quando a supernova esmaeceu, passaram-se mais 700 anos até que uma pequena nuvem de gás verde luminoso surgiu no lugar aonde ela aparecera anteriormente, um grau ao norte e oeste de Zeta Tauri, já em um dos chifres do Touro quase aos pés dos Gêmeos.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Charles Messier (1730-1817) era um caçador de cometas e sempre vasculhava o céu em busca dos mesmos. Em 12 de setembro de 1758 (ou em 28 de Agosto, segundo outro documento - Nota da Tradutora), Messier apontou para esse ponto de luz difusa no céu e o descreveu a nebulosa como contendo nenhuma estrela, esbranquiçada em sua cor e alongada como a chama de uma vela. Mais tarde, Messier veio a saber que tal nebulosa já havia sido avistada por um astrônomo inglês, John Bevis, em 1731.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Messier continuou sua busca por cometas (naquele mesmo houve o retorno, já previsto, do Cometa Halley durante o mês de dezembro) - e passou então, a elaborar uma lista de objetos no céu que não eram cometas. Finalmente, uma versão final dessa lista foi publicada em 1784 contendo 109 ou 110 objetos, sendo que o primeiro objeto mencionado foi a Nebulosa que ora é visitada por Saturno. Essa lista é hoje conhecida como A Lista de Messier e seus objetos são denominados M1, M2, M3.... A Nebulosa do Caranguejo é M1.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">No entanto, esse nome, Nebulosa do Caranguejo foi dado por Earl of Rosse, em 1840 que publicou um desenho da mesma com filamentos que sugeriam o formato de um caranguejo. Mais tarde, ele observou a nebulosa já com outra aparelhagem mais potente e rejeitou sua descrição anterior da mesma.... tarde demais: a Nebulosa do Caranguejo já era assim conhecida!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A Nebulosa do Caranguejo não é difícil de ser localizada com um telescópio mais simples e do quintal de sua casa - afinal foi assim que Messier a encontrou! Porém, em céus mais transparentes, longe das luzes da cidade, sua visão se torna bem mais enriquecida e se você tiver um telescópio possante, será fantástico poder observar um estrela que ainda permanece em seu centro, um pulsar que gira cerca de 30 vezes por segundo!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Sítio das Estrelas - parada de um caminho a Caminho do Céu</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh_l_nYUIOk7EVLVZf1siicPYrvsgLU8ZI_Pw5qgKBH-O0utAG8gOh3BUtb1Eyk07_RYfkOJTiYORrM4cETtEFVFsCOkW0SV1CPQQSTQRcrNbW2ZSXRklTglYS8IBlGLZoNci9xETtSU4w/s1600/crabshrug_rox_big.jpg" imageanchor="1" style="clear: left; color: #274e13; float: left; margin-bottom: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh_l_nYUIOk7EVLVZf1siicPYrvsgLU8ZI_Pw5qgKBH-O0utAG8gOh3BUtb1Eyk07_RYfkOJTiYORrM4cETtEFVFsCOkW0SV1CPQQSTQRcrNbW2ZSXRklTglYS8IBlGLZoNci9xETtSU4w/s1600/crabshrug_rox_big.jpg" height="505" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></a></div>
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<span style="color: #274e13;">http://apod.nasa.gov/apod/ap020920.html<span style="margin-left: 1em; margin-right: 1em;"></span></span></div>
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<span style="color: #274e13;"><b style="line-height: normal; text-align: -webkit-center;">The Crab Nebula Pulsar Shrugs </b></span></div>
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<span style="color: #274e13;"><span style="line-height: normal; text-align: -webkit-center;"></span><b><br style="line-height: normal; text-align: -webkit-center;" /></b><span style="line-height: normal; text-align: -webkit-center;">Credit: </span><span style="line-height: normal; text-align: -webkit-center;"></span><a href="http://eagle.la.asu.edu/hester/" style="color: #274e13; line-height: normal; text-align: -webkit-center; text-decoration: none;">J. Hester</a><span style="line-height: normal; text-align: -webkit-center;"> (</span><a href="http://phyastweb.la.asu.edu/" style="color: #274e13; line-height: normal; text-align: -webkit-center; text-decoration: none;">ASU</a><span style="line-height: normal; text-align: -webkit-center;">), </span><a href="http://chandra.harvard.edu/" style="color: #274e13; line-height: normal; text-align: -webkit-center; text-decoration: none;">CXC</a><span style="line-height: normal; text-align: -webkit-center;">, </span><a href="http://www.stsci.edu/hst/" style="color: #274e13; line-height: normal; text-align: -webkit-center; text-decoration: none;">HST</a><span style="line-height: normal; text-align: -webkit-center;">, </span><a href="http://www.nrao.edu/" style="color: #274e13; line-height: normal; text-align: -webkit-center; text-decoration: none;">NRAO</a><span style="line-height: normal; text-align: -webkit-center;">, </span><a href="http://www.nsf.gov/" style="color: #274e13; line-height: normal; text-align: -webkit-center; text-decoration: none;">NSF</a><span style="line-height: normal; text-align: -webkit-center;">, </span><a href="http://www.nasa.gov/" style="color: #274e13; line-height: normal; text-align: -webkit-center; text-decoration: none;">NASA</a></span></div>
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<span style="color: #073763; font-family: Arial, sans-serif; font-size: 13.5pt;">Os desenhos formados pelas estrelas</span><br />
<span style="color: #073763; font-family: Arial, sans-serif; font-size: 13.5pt;"> - AS CONSTELAÇÕES -</span><br />
<span style="color: #073763; font-family: Arial, sans-serif; font-size: 13.5pt;"> são como janelas que se abrem para a infinitude do universo </span><br />
<span style="color: #073763; font-family: Arial, sans-serif; font-size: 13.5pt;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, </span><br />
<span style="color: #073763; font-family: Arial, sans-serif; font-size: 13.5pt;">entre o céu e a terra...,</span><br />
<span style="color: #073763; font-family: Arial, sans-serif; font-size: 13.5pt;"> bem como percebendo que o caos,</span><br />
<span style="color: #073763; font-family: Arial, sans-serif; font-size: 13.5pt;"> vagarosamente,</span><br />
<span style="color: #073763; font-family: Arial, sans-serif; font-size: 13.5pt;">vai se tornando Cosmos </span><br />
<span style="color: #073763; font-family: Arial, sans-serif; font-size: 13.5pt;">e este por nossa mente sendo conscientizado.</span><span style="font-size: 13.5pt;"><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, sans-serif; font-size: 13.5pt;">Quer dizer, nossa mente é tão infinita </span><br />
<span style="color: #073763; font-family: Arial, sans-serif; font-size: 13.5pt;">quanto infinito é o Cosmos.</span><span style="font-size: 13.5pt;"><o:p></o:p></span></div>
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<b><span style="color: #660000; font-family: Arial, sans-serif; font-size: 13.5pt;">Com um abraço estrelado,</span></b><span style="font-size: 13.5pt;"><o:p></o:p></span></div>
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<b><span style="color: #660000; font-family: Arial, sans-serif; font-size: 13.5pt;">Janine Milward</span></b><span style="font-size: 13.5pt;"><o:p></o:p></span></div>
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</span><span lang="PT" style="font-family: Arial, sans-serif; font-size: 12pt;">Da Terra ao Céu <o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="PT" style="font-family: Arial, sans-serif; font-size: 12pt;"> e ao Infinito </span><span style="font-family: Arial, sans-serif; font-size: 12pt;"><o:p></o:p></span></span></div>
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<span lang="PT" style="background-color: white; color: #073763; font-family: Arial, sans-serif;">Constelações, Estrelas e Objetos Celestes<o:p></o:p></span></div>
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<span lang="PT" style="background-color: white; color: #073763; font-family: Arial, sans-serif;">(sob o ponto de vista do Mundo Ocidental)<o:p></o:p></span></div>
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<span lang="PT" style="background-color: white; color: #073763; font-family: Arial, sans-serif;">Suas histórias, seus mitos, seus significados e suas sintetizadas
descrições<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763;"><span lang="PT" style="font-family: Arial, sans-serif;">Reunião das
Informações e Compilação,</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="PT" style="font-family: Arial, sans-serif;">Tradução para a
língua portuguesa (em alguns momentos)</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="PT" style="font-family: Arial, sans-serif;">bem como
Comentários Pessoais:</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><i><span lang="PT" style="font-family: Arial, sans-serif;">Janine Milward</span></i></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, sans-serif;">Alguns dados<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, sans-serif;">(tais como Ascensão Reta e Declinação, em muitos dos casos)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, sans-serif;">são época/equinócio 1980<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, sans-serif;">e devem requerer do Caminhante do Céu<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;">Visitando os Sites abaixo,</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;"> você conseguirá informações
atualizadas e preciosas</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;">sobre os Objetos Celestiais de
seu interesse:</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">NASA/IPAC</span><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"> EXTRAGALACTIC DATABASE
–</span><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://ned.ipac.caltech.edu/"><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">http://ned.ipac.caltech.edu/</span></a><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://ned.ipac.caltech.edu/forms/byname.html"><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">http://ned.ipac.caltech.edu/forms/byname.html</span></a><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><em><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"> </span></i></span><em><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"> operated by the Jet Propulsion Laboratory,
California Institute of Technology, under contract with the National
Aeronautics and Space Administration.</span></em><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, sans-serif;">THE NIGHT SKY
ATLAS<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://www.nightskyatlas.com/index.jsp"><span lang="EN-US" style="font-family: Arial, sans-serif;">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, sans-serif;">The night sky atlas creates images of any part of the night sky,
allowing easy location of any object. Detailed chart images show all stars
visible to the naked eye, the constellations, Messier objects, and names of the
brightest stars.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763;"><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">The</span><span class="apple-converted-space"><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"> </span></span><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">Internet STELLAR DATABASE</span><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://www.stellar-database.com/"><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">http://www.stellar-database.com/</span></a><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, sans-serif;">- stars within 75
light-years. (Plus some of the more well-known "name brand"
stars farther away.)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; font-weight: normal; line-height: 18px;">Meu Projeto</span></h3>
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Da Terra ao Céu ....</span></a></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">.....<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="text-decoration: none;">e ao Infinito </a></span></h1>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="background-color: white; text-decoration: none;">- As 88 Constelações</a></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/">http://daterraaoceueaoinfinito.blogspot.com.br/</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; font-weight: normal;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; font-weight: normal;">Com um abraço estrelado,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Janine Milward</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">Conheça </b></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">Ophiucus, O Serpentário,</b></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">acessando</b></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><a href="http://sobreophiucuseserpens.blogspot.com.br/2013/11/ophiucus-o-serpentario.html" style="background-color: white;">http://sobreophiucuseserpens.blogspot.com.br/2013/11/ophiucus-o-serpentario.html</a></b></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">SERPENS, A SERPENTE</span></h3>
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<span style="line-height: 23px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Acessando o Link abaixo, o Leitor encontrará uma Página própria acolhendo </span></span><br />
<span style="line-height: 23px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ophiucus e a Serpente:</span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 23px;"><a href="http://sobreophiucuseserpens.blogspot.com.br/" style="text-decoration: none;">http://sobreophiucuseserpens.blogspot.com.br/</a></span><span style="font-size: small;"><br /></span><a href="http://sobreophiucuseserpens.blogspot.com.br/2013/11/serpens-caput-e-serpens-cauda-serpente.html">http://sobreophiucuseserpens.blogspot.com.br/2013/11/serpens-caput-e-serpens-cauda-serpente.html</a></span></div>
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<tr><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_011.jpg" /></span><br />
<a href="http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_011.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_011.jpg</span></a><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiZrc4w8mfG1WH7r_i7i1U-9G5Rav3CgMs74OwXNeUfvJOFjMZPX2zH2I1G2rkp6PdnIqNAm-_BsKf0R_eJBuBed_wMYApSjDe2QfO3WMwPglEcHOjQaQSciCT5a-bnVCsvYoGrvjxCwIqD/s1600/pillars6_hst_960.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiZrc4w8mfG1WH7r_i7i1U-9G5Rav3CgMs74OwXNeUfvJOFjMZPX2zH2I1G2rkp6PdnIqNAm-_BsKf0R_eJBuBed_wMYApSjDe2QfO3WMwPglEcHOjQaQSciCT5a-bnVCsvYoGrvjxCwIqD/s1600/pillars6_hst_960.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://apod.nasa.gov/apod/ap120722.html<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="EN-US">M16: Pillars of Creation </span></b><span lang="EN-US"><br /><b>Image Credit: </b>J. Hester, P. Scowen (</span><a href="http://sese.asu.edu/" style="text-decoration: none;"><span lang="EN-US">ASU</span></a><span lang="EN-US">), </span><a href="http://www.stsci.edu/hst/HST_overview/" style="text-decoration: none;"><span lang="EN-US">HST</span></a><span lang="EN-US">, </span><a href="http://www.nasa.gov/" style="text-decoration: none;"><span lang="EN-US">NASA</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><img src="http://www.raremaps.com/maps/medium/34422ac.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /><br /><a href="http://www.raremaps.com/gallery/detail/34422ac/Serpens_and_Serpentarius/Hevelius.html" style="text-decoration: none;">http://www.raremaps.com/gallery/detail/34422ac/Serpens_and_Serpentarius/Hevelius.html</a></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/2813" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">Johannes Hevelius</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Fine example of Johannes Hevelius's chart of the constellations Serpens and Serpentarius (also called Ophiucus) and surrounding environs, from his highly influential work, <em>Firmamentum Sobiescianum sive Uranographia</em>. </span></div>
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<tr><td class="tr-caption"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></td></tr>
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<tr><td class="tr-caption"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a class="external free" href="http://www.hubblesite.org/newscenter/archive/2002/22/image/a" rel="nofollow" style="text-decoration: none;">http://www.hubblesite.org/newscenter/archive/2002/22/image/a</a><br /><a href="http://pt.wikipedia.org/wiki/Sexteto_de_Seyfert" style="text-decoration: none;">http://pt.wikipedia.org/wiki/Sexteto_de_Seyfert</a><br />Sexteto de Seyfert</span></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"> - excerto apresentando ALFABETO GREGO, CONVENÇÕES E USO DA CARTA CELESTE</span></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b><b><span lang="PT">Da Terra ao Céu<o:p></o:p></span></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="PT"> e ao Infinito</span></b><o:p></o:p></span></div>
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<span lang="PT" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelações, Estrelas e Objetos Celestes<o:p></o:p></span></div>
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<span lang="PT" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(sob o ponto de vista do Mundo Ocidental)<o:p></o:p></span></div>
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<span lang="PT" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Suas histórias, seus mitos, seus significados e suas sintetizadas descrições<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">Reunião das Informações e Compilação,</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">Tradução para a língua portuguesa (em alguns momentos)</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">bem como Comentários Pessoais:</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><span lang="PT">Janine Milward</span></i><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; text-align: start;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; text-align: start;"> bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; text-align: start;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Alguns dados<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(tais como Ascensão Reta e Declinação, em muitos dos casos)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">são época/equinócio 1980<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e devem requerer do Caminhante do Céu<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NASA/IPAC</b><b> EXTRAGALACTIC DATABASE –</b><b><o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="text-decoration: none;"><b>http://ned.ipac.caltech.edu/</b></a><b><o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="text-decoration: none;"><b>http://ned.ipac.caltech.edu/forms/byname.html</b></a><b><o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<b><span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><b><span lang="EN-US"><o:p></o:p></span></b></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>T</b>he night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="EN-US">The</span></b><span class="apple-converted-space"><b><span lang="EN-US"> </span></b></span><b><span lang="EN-US">Internet STELLAR DATABASE</span></b><b><span lang="EN-US"><o:p></o:p></span></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="text-decoration: none;"><b><span lang="EN-US">http://www.stellar-database.com/</span></b></a><b><span lang="EN-US"><o:p></o:p></span></b></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<o:p></o:p></span></div>
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<tr><td><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgROHTaXItoaVo9j__K9rNtpFjL1p_WBDU_ELmRy6k4xAgpOHPRUpL9Rl2ct5sd0IURc9KeG9L_iEck-TZr4XlP2ezhAxhyVBsysGea5FFYZjpkbkP0ZcW72XFBxrcGe2HNxj8q72OePlh6/s1600/urania12.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgROHTaXItoaVo9j__K9rNtpFjL1p_WBDU_ELmRy6k4xAgpOHPRUpL9Rl2ct5sd0IURc9KeG9L_iEck-TZr4XlP2ezhAxhyVBsysGea5FFYZjpkbkP0ZcW72XFBxrcGe2HNxj8q72OePlh6/s640/urania12.jpg" height="446" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><b><a href="http://www.ianridpath.com/atlases/urania/urania12.jpg" style="text-decoration: none;" target="_blank">Card 12</a> </b><a href="http://www.ianridpath.com/atlases/urania/urania12.jpg" style="line-height: 13px; text-decoration: none;" target="_blank">Taurus Poniatowski, Serpentarius (i.e. Ophiuchus), Scutum Sobiesky, and Serpens</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><i><span lang="EN-US" style="line-height: 16px;">Urania’s Mirror</span></i><span lang="EN-US" style="line-height: 16px;"> is a boxed set of 32 constellation cards</span></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; line-height: 16px;"> © Ian Ridpath</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://www.ianridpath.com/atlases/urania.htm" style="text-decoration: none;"><span lang="EN-US">http://www.ianridpath.com/atlases/urania.htm</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">Serpens Cauda et Serpens Caput </b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b> a Cauda e a Cabeça da Serpente</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><img src="http://www.raremaps.com/maps/medium/33412op.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
<a href="http://www.raremaps.com/gallery/detail/33412op/_Serpens/Bayer.html" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/33412op/_Serpens/Bayer.html</span></a><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/247" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">Johann Bayer</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Fine example of Bayer's map of the Constellation Serpens, one of the 48 constellations listed by the 2nd century astronomer Ptolemy, which remains one of the 88 modern constellations defined by the International Astronomical Union. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Posicionamento:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 15h8m / 18h56m Declinação +25<sup>o</sup>.7 / -16<sup>o</sup>.0<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Mito:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando Glaucus, filho de Minos, Rei de Creta, foi afogado em uma colméia, Esculapius foi trazido para restaurar a vida ao menino. Enquanto Esculapius pensava o que iria fazer, uma serpente entrou no quarto e ele matou-a. Então, entrou outra serpente trazendo uma erva que foi colocada na cabeça da serpente morta, trazendo-a à vida. Usando a mesma erva, Esculapius trouxe a vida de volta ao menino. A serpente foi colocada nos céus e é por esta razão que muitos escritores confundem Ophiucus com Esculapius. De acordo com outro mito, a serpente seria uma das que deveriam matar Hercules em seu berço, quando ainda era uma criança.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Fronteiras:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Serpens (Cauda e Caput) acabam fazendo parte da constelação Ophiucus - porque este é Aquele que Segura a Serpente - e todas três acabam formando um conjunto imenso de situações entrelaçadas. E também estaremos encontrando as constelações Scorpius, Sagittarius, Scutum, Aquila, Hercules Corona Borealis, Libra<o:p></o:p></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><br /><img src="http://www.raremaps.com/maps/medium/34480.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span><br />
<a href="http://www.raremaps.com/gallery/detail/34480/Ophiuchus_and_Serpent/Jamieson.html" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/34480/Ophiuchus_and_Serpent/Jamieson.html</span></a><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1372" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">Alexander Jamieson</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Striking star chart, marvelously engraved and delicately colored. Shows the featured constellations in color with neighboring stars and constellations without color.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Jamieson's work is one of the finest of it's kind in the early 19th century.</span></div>
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<tr><td class="tr-caption"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">The Hamlyn Enciclopedia of Stars and Planets - Antonin Rukl</span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><b style="background-color: white;">Meus (Janine) Comentários </b></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><b style="background-color: white;">sobre a Cabeça da Serpente </b></span><br />
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<tr><td class="tr-caption"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Ilustração realizada em Programa Stellarium e trabalhada em Programa Corel<br />Veja que Vênus e Saturno podem ser vistas ainda em Virgo enquanto a Lua trilha por Balança!</span><br />
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<tr><td class="tr-caption"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Celestial Charts - Antique Maps of the Heavens - Carole Stott - Crescent Books, NY, USA</span></td></tr>
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<i><span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; line-height: 16px;">EXTRACTED FROM</span></i><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><i><span lang="EN-US" style="line-height: 16px;">Urania’s Mirror</span></i><span lang="EN-US" style="line-height: 16px;"> is a boxed set of 32 constellation cards</span></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; line-height: 16px;"> © Ian Ridpath</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span lang="EN-US"><a href="http://www.ianridpath.com/atlases/urania.htm" style="text-decoration: none;">http://www.ianridpath.com/atlases/urania.htm</a></span><span lang="EN-US"><o:p></o:p></span></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Eu moro num lugar de céus escuros e transparentes - volta e meia, nem sempre, infelizmente -, e em noites sem Lua, certamente eu aprecio imensamente observar a região entre Escorpião e Sagitário, sendo que o Serpentário, Ophicus, vem ocupando seu espaço um tantinho mais ao norte e sendo enlaçado, digamos assim, pela Cauda da Serpente e pela Cabeça da Serpente (a Cauda mais grudada a Escorpião e a Sagitário enquanto que a Cabeça se situa mais voltada para o Boieiro, Bootes, sempre apresentando sua belíssima estrela-alpha Arcturus, a mais bela do norte, e desafiando Hercules e... pasme!: protegendo a Coroa Boreal!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Confesso que tenho uma certa dificuldade em divisar exatamente o Serpentário, Ophiucus (ainda não estudei bem esse posicionamento de estrelinhas tímidas). No entanto, a Cauda da Serpente bem como sua Cabeça são bem delineadas.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">A Cabeça propriamente dita da Serpente é de uma beleza extremamente rara, com suas cinco estrelas (pelo menos, é bem assim que as vejo e conto) fazendo acontecer um Asterismo quase realizando uma imagem de um papagaio, uma pandorga, um <i>kite</i>, uma pipa...</span></div>
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<tr><td class="tr-caption"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">The Hamlyn Enciclopedia of Stars and Planets - Antonin Ruk</span></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">É uma visão magnífica e ao mesmo tempo, aterrorizante! Quer dizer, a Coroa Boreal é uma constelação de delicadeza ímpar em suas estrelinhas tímidas... Mais tímidas ainda são as estrelinhas que compõem a Cabeça propriamente dita da Serpente... e é exatamente este fato que torna este conjunto de situações - Coroa Boreal e Cabeça da Serpente - como algo que realmente vale a pena ser observado...., sempre em lugares de céus escuros e transparentes e em noites sem Lua, de preferência.</span></div>
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<tr><td class="tr-caption"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">The Hamlyn Enciclopedia of Stars and Planets - Antonin Ruk</span></td></tr>
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<a href="http://www.raremaps.com/gallery/detail/34896/Hercules_La_Couronne_Hercules_and_The_Crown/Flamsteed-Fortin.html" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">http://www.raremaps.com/gallery/detail/34896/Hercules_La_Couronne_Hercules_and_The_Crown/Flamsteed-Fortin.html</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1260" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">John Flamsteed</a> / <a href="https://www.raremaps.com/gallery/browse/creator_id/1454" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">MJ Fortin</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Detailed star chart of the constellations Hercules and neighboring constellations, from Fortin's <em>Atlas Celeste de Flamsteed </em>. . , published in Paris. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">John Flamsteed was the first Astronomer Royal at the London Observatory, winning out over Edmund Halley and Isaac Newton</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Com um abraço estrelado,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Janine</span></div>
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<tr><td class="tr-caption"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Ilustração realizada em Programa Stellarium e trabalhada em Programa Corel</span></td></tr>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">Estrelas e Objetos interessantes, em Serpens:<o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Unukalhal. Alpha Serpentis. </b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela amarelo pálido situada no pescoço da Serpente. De Unk Al Hayyah, o Pescoço da Serpente, e também chamada de Coração da Serpente.<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT"><b>Alya</b></span><span lang="PT"><b> - Theta Serpentis - Estrela Dupla</b><o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">AR 18h53m Dec. + 04<sup>o</sup>.08<o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual 4,5 e 4,5 Distância entre estrelas 22”,23<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É a estrela finalizando a Cauda da Serpente. A Lúcida, denominação árabe.</span><br />
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<span style="background-color: white; color: #073763; line-height: 18px;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></span><span style="line-height: 18px;"><img src="http://upload.wikimedia.org/wikipedia/commons/thumb/9/91/Serpens_constellation_map.png/800px-Serpens_constellation_map.png" /></span><span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /><span style="line-height: 18px;">http://pt.wikipedia.org/wiki/NGC_6535#mediaviewer/File:Serpens_constellation_map.png</span></span></span><br />
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18px;"><br /></span></span></span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">NGC 6535</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: white; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Serpens" style="background-attachment: initial; background-clip: initial; background-color: white; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Serpens">constelação de Serpens</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/John_Hind" style="background-attachment: initial; background-clip: initial; background-color: white; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="John Hind">John Hind</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> em 1852, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-color: white; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> refrator com abertura de 7 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: white; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> (+9,3), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-color: white; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> amadores ou com equipamentos superiores.</span><br />
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/NGC_6535</span></span></div>
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This image captures the stunning NGC 6535, a globular cluster 22,000 light-years away in the constellation of Serpens (The Serpent) that measures one light-year across.</div>
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Globular clusters are tightly bound groups of stars which orbit galaxies. The large mass in the rich stellar centre of the globular cluster pulls the stars inward to form a ball of stars. The word <em style="border: 0px; font-stretch: inherit; font-variant: inherit; font-weight: inherit; letter-spacing: 0px; line-height: inherit; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;">globulus</em>, from which these clusters take their name, is Latin for <em style="border: 0px; font-stretch: inherit; font-variant: inherit; font-weight: inherit; letter-spacing: 0px; line-height: inherit; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;">small sphere</em>.</div>
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Globular clusters are generally very ancient objects formed around the same time as their host galaxy. To date, no new star formation has been observed within a globular cluster, which explains the abundance of aging yellow stars in this image, most of them containing very few heavy elements.</div>
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NGC 6535 was first discovered in 1852 by English astronomer John Russell Hind. The cluster would have appeared to Hind as a small, faint smudge through his telescope. Now, over 160 years later, instruments like the <a href="http://www.spacetelescope.org/about/general/instruments/acs/" style="-webkit-font-smoothing: antialiased !important; border: 0px; color: rgb(39, 61, 162) !important; font-stretch: inherit; font-style: inherit; font-variant: inherit; font-weight: inherit; letter-spacing: 0px; line-height: inherit; margin: 0px; outline: 0px; padding: 0px; text-decoration: none !important; vertical-align: baseline;">Advanced Camera for Surveys</a> (ACS) and <a href="http://www.spacetelescope.org/about/general/instruments/wfc3/" style="-webkit-font-smoothing: antialiased !important; border: 0px; color: rgb(39, 61, 162) !important; font-stretch: inherit; font-style: inherit; font-variant: inherit; font-weight: inherit; letter-spacing: 0px; line-height: inherit; margin: 0px; outline: 0px; padding: 0px; text-decoration: none !important; vertical-align: baseline;">Wide Field Camera 3</a> (WFC3) on the NASA/ European Space Agency (ESA) Hubble Space Telescope allow us to marvel at the cluster and its contents in greater detail.</div>
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<strong style="border: 0px; font-stretch: inherit; font-style: inherit; font-variant: inherit; letter-spacing: 0px; line-height: inherit; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><em style="border: 0px; font-stretch: inherit; font-variant: inherit; font-weight: inherit; letter-spacing: 0px; line-height: inherit; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;">European Space Agency</em></strong></div>
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<strong style="border: 0px; font-stretch: inherit; font-style: inherit; font-variant: inherit; letter-spacing: 0px; line-height: inherit; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><strong style="border: 0px; font-stretch: inherit; font-style: inherit; font-variant: inherit; letter-spacing: 0px; line-height: inherit; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><em style="border: 0px; font-stretch: inherit; font-variant: inherit; font-weight: inherit; letter-spacing: 0px; line-height: inherit; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;">Credit: <a href="http://www.spacetelescope.org/" style="-webkit-font-smoothing: antialiased !important; border: 0px; color: rgb(39, 61, 162) !important; font-stretch: inherit; font-style: inherit; font-variant: inherit; font-weight: inherit; letter-spacing: 0px; line-height: inherit; margin: 0px; outline: 0px; padding: 0px; text-decoration: none !important; vertical-align: baseline;">ESA/Hubble</a> & <a href="http://www.nasa.gov/" style="-webkit-font-smoothing: antialiased !important; border: 0px; color: rgb(39, 61, 162) !important; font-stretch: inherit; font-style: inherit; font-variant: inherit; font-weight: inherit; letter-spacing: 0px; line-height: inherit; margin: 0px; outline: 0px; padding: 0px; text-decoration: none !important; vertical-align: baseline;">NASA</a>, Acknowledgement: Gilles Chapdelaine </em></strong><span style="line-height: 22.3999996185303px;"> </span></strong></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">http://www.nasa.gov/content/goddard/hubble-sees-an-ancient-globular-cluster/#.VKVB-dLF9mY<br /><br /><br /><br /><br /></span><span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px;"><br /></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 6027 -</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Um grupo pouco comum de galáxias bem próximo à Cabeça propriamente dita da Serpente.<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 6027</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_lenticular" style="background-image: none; text-decoration: none;" title="Galáxia lenticular">galáxia lenticular</a>, a aproximadamente 190 milhões de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; text-decoration: none;" title="Anos-luz">anos-luz</a>, na direção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Serpens" style="background-image: none; text-decoration: none;" title="Serpens">Serpens Caput</a>. A <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> é o membro mais brilhante do <a href="http://pt.wikipedia.org/wiki/Sexteto_de_Seyfert" style="background-image: none; text-decoration: none;" title="Sexteto de Seyfert">Sexteto de Seyfert</a>, um grupo compacto de galáxias.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> <b>NGC 6027</b> foi descoberta por <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/%C3%89douard_Stephan" style="background-image: none; text-decoration: none;" title="Édouard Stephan">Édouard Stephan</a>, em <a href="http://pt.wikipedia.org/wiki/1882" style="background-image: none; text-decoration: none;" title="1882">1882</a>.</span></div>
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<tr><th class="" colspan="2" style="vertical-align: top;"><span class=""><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 6027</span></span></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Ngc_6027.jpg" style="background-image: none; margin-left: auto; margin-right: auto; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="" src="http://upload.wikimedia.org/wikipedia/commons/thumb/d/d0/Ngc_6027.jpg/280px-Ngc_6027.jpg" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/d/d0/Ngc_6027.jpg/420px-Ngc_6027.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/d/d0/Ngc_6027.jpg/560px-Ngc_6027.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; margin-left: auto; margin-right: auto; padding: 8px; position: relative; vertical-align: middle;" /></span></a></div>
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<small><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Uma imagem da <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> NGC 6027, pelo <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-image: none; text-decoration: none;" title="Telescópio Espacial Hubble">HST</a>.<br />Crédito: HST/<a href="http://pt.wikipedia.org/wiki/NASA" style="background-image: none; text-decoration: none;" title="NASA">NASA</a>/<a href="http://pt.wikipedia.org/wiki/ESA" style="background-image: none; text-decoration: none;" title="ESA">ESA</a>.</span></small></td></tr>
<tr><td scope="row" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Descoberto por</span></td><td valign="top"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/%C3%89douard_Stephan" style="background-image: none; text-decoration: none;" title="Édouard Stephan"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Édouard Stephan</span></a></td></tr>
<tr><td scope="row" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Data de descoberta</span></td><td valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">de <a href="http://pt.wikipedia.org/wiki/1882" style="background-image: none; text-decoration: none;" title="1882">1882</a></span></td></tr>
<tr><th colspan="2" style="vertical-align: top;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dados observacionais (J2000)</span></b></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelação</span></a></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Serpens" style="background-image: none; text-decoration: none;" title="Serpens"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Serpens Caput</span></a></td></tr>
<tr><td scope="row" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo</span></td><td valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0 pec. <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_lenticular" style="background-image: none; text-decoration: none;" title="Galáxia lenticular">Lenticular</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-image: none; text-decoration: none;" title="Ascensão reta"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Asc. reta</span></a></td><td valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 59<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 12.5<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Declinação"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Declinação</span></a></td><td valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">+20° 45′ 48″</span></td></tr>
<tr><td scope="row" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distância</span></td><td valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">aprox. 190 milhões de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; text-decoration: none;" title="Anos-luz">anos-luz</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Desvio_para_o_vermelho" style="background-image: none; text-decoration: none;" title="Desvio para o vermelho"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Redshift</span></a></td><td valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">4447±11 <a href="http://pt.wikipedia.org/wiki/Quil%C3%B4metro" style="background-image: none; text-decoration: none;" title="Quilômetro">km</a>/<a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; text-decoration: none;" title="Segundo">s</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; text-decoration: none;" title="Magnitude aparente"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnit. apar.</span></a></td><td valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">14.7</span></td></tr>
<tr><td scope="row" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dimensões</span></td><td valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">0.4′ × 0.2′</span></td></tr>
<tr><th colspan="2" style="vertical-align: top;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Características físicas</span></b></th></tr>
<tr><td scope="row" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Raio</span></td><td valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">17.500 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; text-decoration: none;" title="Anos-luz">anos-luz</a></span></td></tr>
<tr><th colspan="2" style="vertical-align: top;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Outras denominações</span></b></th></tr>
<tr><td colspan="2" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Uppsala_General_Catalogue" style="background-image: none; text-decoration: none;" title="Uppsala General Catalogue">UGC</a> 10116, <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Principal_Galaxies_Catalogue&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="Principal Galaxies Catalogue (página não existe)">PGC</a> 56575, HCG 79b.</span></td></tr>
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<a href="http://pt.wikipedia.org/wiki/NGC_6027" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_6027</span></a></div>
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<h1 style="border: 0px; line-height: 28px; margin: 0px 0px 13px; outline: 0px; padding: 0px; vertical-align: baseline;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Cosmic Dance of Destruction</span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://www.spacetelescope.org/static/archives/images/screen/opo0222a.jpg" /></span></div>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.spacetelescope.org/images/opo0222a/" style="background-color: white;">http://www.spacetelescope.org/images/opo0222a/</a></span><br />
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<strong style="border: 0px; margin: 0px 0px 15px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Credit:</span></strong></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nasa.gov/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">NASA</a>/<a href="http://www.esa.int/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">ESA</a>, J. English (U. Manitoba), S. Hunsberger, S. Zonak, J. Charlton, S. Gallagher (PSU), and L. Frattare (<a href="http://www.stsci.edu/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">STScI</a>)</span></div>
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<tr style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><strong style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Name:</span></strong></td><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><a href="http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Seyfert%27s+Sextet" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Seyfert's Sextet</span></a></td></tr>
<tr style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><strong style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Type:</span></strong></td><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">• Local Universe : Galaxy : Type : Interacting<br />• X - Galaxies Images/Videos</span></td></tr>
<tr style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><strong style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distance:</span></strong></td><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">200 million <a href="http://en.wikipedia.org/wiki/Light-year" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">light years</a></span></td></tr>
<tr style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><strong style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constellation:</span></strong></td><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Serpens Caput</span></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The <a href="http://www.nasa.gov/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">NASA</a>/<a href="http://www.esa.int/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">ESA</a> Hubble Space Telescope is witnessing a grouping of galaxies engaging in a slow dance of destruction that will last for billions of years. The galaxies are so tightly packed together that gravitational forces are beginning to rip stars from them and distort their shapes. Those same gravitational forces eventually could bring the galaxies together to form one large galaxy.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The name of this grouping, Seyfert's Sextet, implies that six galaxies are participating in the action. But only four galaxies are on the dance card. The small face-on spiral with the prominent arms [center] of gas and stars is a background galaxy almost five times farther away than the other four. Only a chance alignment makes it appear as if it is part of the group. The sixth member of the sextet isn't a galaxy at all but a long 'tidal tail' of stars [below, right] torn from one of the galaxies.</span></div>
<a href="http://www.spacetelescope.org/images/opo0222a/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spacetelescope.org/images/opo0222a/</span></a><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 19.1875px; text-align: start;">O </span><b style="line-height: 19.1875px; text-align: start;">Sexteto de Seyfert</b><span style="line-height: 19.1875px; text-align: start;"> é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_de_gal%C3%A1xias" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Aglomerado de galáxias">grupo de galáxias</a><span style="line-height: 19.1875px; text-align: start;"> a aproximadamente 190 milhões de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="line-height: 19.1875px; text-align: start;"> de distância </span><a class="external autonumber" href="http://www.laughtergenealogy.com/bin/hubble/html/seyfert.html" rel="nofollow" style="text-decoration: none;">[1]</a><span style="line-height: 19.1875px; text-align: start;">, na direção da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="line-height: 19.1875px; text-align: start;"> de</span><a href="http://pt.wikipedia.org/wiki/Serpens" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Serpens">Serpens Caput</a><span style="line-height: 19.1875px; text-align: start;">. O grupo parece conter seis membros, mas uma das galáxias está em plano de fundo e a outra "galáxia" é uma parte de gás e</span><a href="http://pt.wikipedia.org/wiki/Poeira_interestelar" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Poeira interestelar">poeira interestelar</a><span style="line-height: 19.1875px; text-align: start;"> que pertence a uma das galáxias. A </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Intera%C3%A7%C3%A3o_gravitacional&action=edit&redlink=1" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Interação gravitacional (página não existe)">interação gravitacional</a><span style="line-height: 19.1875px; text-align: start;"> entre estas galáxias continuará por centenas de milhões de anos. E em última instância, estas </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Galáxia">galáxias</a><span style="line-height: 19.1875px; text-align: start;"> irão se fundir para formar uma única e gigante </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_el%C3%ADptica" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Galáxia elíptica">galáxia elíptica</a><span style="line-height: 19.1875px; text-align: start;">.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; line-height: 18px;"><span style="line-height: 19.1875px; text-align: start;">O grupo foi descoberto por </span><a href="http://pt.wikipedia.org/wiki/Carl_Keenan_Seyfert" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Carl Keenan Seyfert">Carl Keenan Seyfert</a><span style="line-height: 19.1875px; text-align: start;">, usando chapas fotográficas do </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Observat%C3%B3rio_Barnard&action=edit&redlink=1" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Observatório Barnard (página não existe)">Observatório Barnard</a><span style="line-height: 19.1875px; text-align: start;">, da Universidade Vanderbilt. Quando os primeiros resultados foram publicados, em </span><a href="http://pt.wikipedia.org/wiki/1951" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="1951">1951</a><span style="line-height: 19.1875px; text-align: start;">, este grupo foi o mais compacto grupo já identificado.</span></span></div>
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<tr style="vertical-align: top;"><td colspan="2"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sexteto de Seyfert</span></b></td></tr>
<tr style="vertical-align: top;"><td colspan="2"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Seyfert_Sextet_full.jpg" style="background-image: none; text-decoration: none;" title="O Sexteto de Seyfert, fotografado pelo HST.Crédito: NASA/ESA."><img alt="O Sexteto de Seyfert, fotografado pelo HST.Crédito: NASA/ESA." src="http://upload.wikimedia.org/wikipedia/commons/thumb/2/20/Seyfert_Sextet_full.jpg/250px-Seyfert_Sextet_full.jpg" height="599" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/20/Seyfert_Sextet_full.jpg/375px-Seyfert_Sextet_full.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/20/Seyfert_Sextet_full.jpg/500px-Seyfert_Sextet_full.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="640" /></a><br />O Sexteto de Seyfert, fotografado pelo <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-image: none; text-decoration: none;" title="Telescópio Espacial Hubble">HST</a>.<br />Crédito: <a href="http://pt.wikipedia.org/wiki/NASA" style="background-image: none; text-decoration: none;" title="NASA">NASA</a>/<a href="http://pt.wikipedia.org/wiki/ESA" style="background-image: none; text-decoration: none;" title="ESA">ESA</a>.</span></td></tr>
<tr style="vertical-align: top;"><td colspan="2"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dados observacionais (J2000)</span></b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelação</span></a></td><td><a href="http://pt.wikipedia.org/wiki/Serpens" style="background-image: none; text-decoration: none;" title="Serpens"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Serpens Caput</span></a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-image: none; text-decoration: none;" title="Ascensão reta"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Asc. reta</span></a></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 59<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 11.9<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-ned_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Sexteto_de_Seyfert#cite_note-ned-1" style="background-image: none; text-decoration: none;">1</a></span></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Declinação"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Declinação</span></a></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">+20° 45′ 31″<span class="reference" id="cite_ref-ned_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Sexteto_de_Seyfert#cite_note-ned-1" style="background-image: none; text-decoration: none;">1</a></span></span></td></tr>
<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Número de Membros</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">4<span class="reference" id="cite_ref-ned_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Sexteto_de_Seyfert#cite_note-ned-1" style="background-image: none; text-decoration: none;">1</a></span></span></td></tr>
<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Membro Brilhante</span></td><td><a href="http://pt.wikipedia.org/wiki/NGC_6027" style="background-image: none; text-decoration: none;" title="NGC 6027"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 6027</span></a></td></tr>
<tr style="vertical-align: top;"><td colspan="2"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Outras denominações</span></b></td></tr>
<tr style="vertical-align: top;"><td colspan="2"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sexteto Serpens, HCG 79, <a href="http://pt.wikipedia.org/wiki/Uppsala_General_Catalogue" style="background-image: none; text-decoration: none;" title="Uppsala General Catalogue">UGC</a> 10116,<br />.VV 115, VII Zw 631<span class="reference" id="cite_ref-ned_1-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Sexteto_de_Seyfert#cite_note-ned-1" style="background-image: none; text-decoration: none;">1</a></span></span></td></tr>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Membros do Sexteto de Seyfert</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Nome<a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_de_Hubble" style="background-image: none; text-decoration: none;" title="Classificação de Hubble">Tipo</a>Distância do <a href="http://pt.wikipedia.org/wiki/Sol" style="background-image: none; text-decoration: none;" title="Sol">Sol</a>(milhões de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; text-decoration: none;" title="Anos-luz">anos-luz</a>)<a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; text-decoration: none;" title="Magnitude aparente">Magnitude</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_6027" style="background-image: none; text-decoration: none;" title="NGC 6027">NGC 6027</a>S0 pec.~190+14.7</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_6027a" style="background-image: none; text-decoration: none;" title="NGC 6027a">NGC 6027a</a>S0 pec.~190+15.4</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_6027b" style="background-image: none; text-decoration: none;" title="NGC 6027b">NGC 6027b</a>SAa pec.~190+15.4</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_6027c" style="background-image: none; text-decoration: none;" title="NGC 6027c">NGC 6027c</a>SB(S)c~190+16</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_6027d" style="background-image: none; text-decoration: none;" title="NGC 6027d">NGC 6027d</a>SB(S)bc pec.~190+15.6</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_6027e" style="background-image: none; text-decoration: none;" title="NGC 6027e">NGC 6027e</a>SB0 pec.~190+16.5</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><br /><br /><a href="http://pt.wikipedia.org/wiki/Sexteto_de_Seyfert" style="text-decoration: none;">http://pt.wikipedia.org/wiki/Sexteto_de_Seyfert</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M5 - NGC 5904 - Aglomerado Globular</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Na parte da Cabeça da Serpente, um brilhante aglomerado globular distante cerca de 27 mil anos-luz e contendo cerca de meio milhão de estrelas.<o:p></o:p></span></div>
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<tr><td><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgdpciTMLl7Ognx3shN1r8ZM9M9Jn7honPhyCuD3APnBs0oCRXHjYMXVaoXy8wwtw_ZuRZ6x2fUo0KRXDJRB-zSLy-j9HEYEQ_YvCYRWiByPhLkIKFIsj94mv6f6BgleRRsm8ieZHVRELT9/s1600/Messier5_Hubble_WikiSky.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgdpciTMLl7Ognx3shN1r8ZM9M9Jn7honPhyCuD3APnBs0oCRXHjYMXVaoXy8wwtw_ZuRZ6x2fUo0KRXDJRB-zSLy-j9HEYEQ_YvCYRWiByPhLkIKFIsj94mv6f6BgleRRsm8ieZHVRELT9/s640/Messier5_Hubble_WikiSky.jpg" height="640" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></td></tr>
<tr><td class="tr-caption"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a class="extiw" href="http://en.wikipedia.org/wiki/Messier_5" style="background-image: none; line-height: 18.234375px; text-align: start; text-decoration: none;" title="en:Messier 5">en:Messier 5</a><span style="line-height: 18.234375px; text-align: start;"> - </span><a class="extiw" href="http://en.wikipedia.org/wiki/globular_cluster" style="background-image: none; line-height: 18.234375px; text-align: start; text-decoration: none;" title="en:globular cluster">en:globular cluster</a><span style="line-height: 18.234375px; text-align: start;"> by </span><a class="extiw" href="http://en.wikipedia.org/wiki/Hubble_Space_Telescope" style="background-image: none; line-height: 18.234375px; text-align: start; text-decoration: none;" title="en:Hubble Space Telescope">en:Hubble Space Telescope</a><span style="line-height: 18.234375px; text-align: start;">. </span><i style="line-height: 18.234375px; text-align: start;">2.4′ view</i><span style="line-height: 18.234375px; text-align: start;">. The image created using </span><a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-image: none; line-height: 18.234375px; text-align: start; text-decoration: none;" title="en:WikiSky">en:WikiSky</a><span style="line-height: 18.234375px; text-align: start;">'s image cutout tool out of </span><a class="extiw" href="http://en.wikipedia.org/wiki/Hubble_Space_Telescope" style="background-image: none; line-height: 18.234375px; text-align: start; text-decoration: none;" title="en:Hubble Space Telescope">en:Hubble Space Telescope</a><span style="line-height: 18.234375px; text-align: start;">data. Source url: </span><a class="external autonumber" href="http://server1.wikisky.org/snapshot?survey=ASTROPHOTO&img_id=60142&angle=0.040&ra=15.3093&de=2.084&x_shift=0&y_shift=0&width=2800&height=2800&projection=tan&rotation=0&reverse=0&interpolation=bicubic&jpeg_quality=.95" rel="nofollow" style="text-decoration: none;">[1]</a><span style="line-height: 18.234375px; text-align: start;"> Hubble source data: </span><a class="external autonumber" href="http://archive.stsci.edu/cgi-bin/mastpreview?mission=hst&dataid=J9DX02080" rel="nofollow" style="text-decoration: none;">[2]</a><span style="line-height: 18.234375px; text-align: start;">. Related images: </span><a class="extiw" href="http://en.wikipedia.org/wiki/Image:m5--LRGB2_898x688.jpg" style="background-image: none; line-height: 18.234375px; text-align: start; text-decoration: none;" title="en:Image:m5--LRGB2 898x688.jpg">en::Image:m5--LRGB2 898x688.jpg</a><span style="line-height: 18.234375px; text-align: start;">.</span><a href="http://pt.wikipedia.org/wiki/Messier_5" style="text-decoration: none;">http://pt.wikipedia.org/wiki/Messier_5</a></span></td></tr>
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<span lang="PT" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M10 - NGC 6254 - Aglomerado Globular</b><o:p></o:p></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Na parte ao sul do Ophiúco existem, entre partes adoráveis da Via Láctea, Nuvens de Estrelas e Nebulosas Escuras. Próximo à estrela Alya, Theta Serpentis, é possível se observar a olho nú uma imensa nuvem escura no formato de um Cachimbo, é a Nebulosa do Cachimbo. Quando observamos esta região e sua vizinhança fazendo parte da Via Láctea em Sagitário, estamos olhando em direção ao centro de nossa Galáxia.<o:p></o:p></span></span></div>
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<tr><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Ficheiro:Messier 10 Hubble WikiSky.jpg" src="http://upload.wikimedia.org/wikipedia/commons/thumb/6/67/Messier_10_Hubble_WikiSky.jpg/600px-Messier_10_Hubble_WikiSky.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; margin-left: auto; margin-right: auto; padding: 8px;" /></span></td></tr>
<tr><td class="tr-caption"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="en:NASA">en:NASA</a><span style="line-height: 19.1875px; text-align: start;">, </span><a class="extiw" href="http://en.wikipedia.org/wiki/STScI" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="en:STScI">en:STScI</a><span style="line-height: 19.1875px; text-align: start;">, </span><a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M16 - NGC 6611 - Aglomerado Aberto</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Fazendo parte da Cauda da Serpente, encontramos um grande aglomerado aberto rodeado por uma nebulosa difusa, um dos mais interessantes objetos de sua espécie, denominado de <b>A Nebulosa da Águia ou a Nebulosa da Estrela da Rainha</b> (em função da silhueta escura no meio da nebulosa, parecendo uma rainha sentada no trono). A nebulosa luminosa encontra-se numa região de hidrogênio ionizado e ao fundo existem regiões de material interestelar frios e escuros - tudo isso formando um modelo bizarro. M16 cobre uma área igual à de uma Lua cheia, no entanto sua luminosidade é pálida e difícil de ser observada mesmo em grandes telescópios.<o:p></o:p></span></div>
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<tr><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Ficheiro:Eagle Nebula from ESO.jpg" src="http://upload.wikimedia.org/wikipedia/commons/thumb/2/2b/Eagle_Nebula_from_ESO.jpg/600px-Eagle_Nebula_from_ESO.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; margin-left: auto; margin-right: auto; padding: 8px;" /></span></td></tr>
<tr><td class="tr-caption"><a href="http://pt.wikipedia.org/wiki/Ficheiro:Eagle_Nebula_from_ESO.jpg" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">http://pt.wikipedia.org/wiki/Ficheiro:Eagle_Nebula_from_ESO.jpg</span></a><br />
<a class="external free" href="http://www.eso.org/public/images/eso0926a/" rel="nofollow" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">http://www.eso.org/public/images/eso0926a/</span></a><br />
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Hubble Goes High-Definition to Revisit Iconic 'Pillars of Creation'</div>
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<span class="date-display-single" content="2015-01-05T00:00:00-05:00" datatype="xsd:dateTime" property="dc:date" style="border: 0px; font-stretch: inherit; font-style: inherit; font-variant: inherit; letter-spacing: 0px; line-height: inherit; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;">January 5, 2015</span></div>
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<span style="line-height: 18px;">http://www.nasa.gov/content/goddard/hubble-goes-high-definition-to-revisit-iconic-pillars-of-creation/index.html#.VKwWjdLF9mZ</span></div>
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<tr><td><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgbYNc-mHwIc90_07NJl6WJe15D4W6rB8LwwuY-GRH8FeJwtZzXUQS1kHn-VdmQrAqm7PwHdWUaMqhgyQvk1yt3sPz5Abv99fS1IvA3fF4ihjbXu78JtNsenclssGYdvi2UYqiqlBNzAy06/s1600/Eagle_nebula_pillars.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgbYNc-mHwIc90_07NJl6WJe15D4W6rB8LwwuY-GRH8FeJwtZzXUQS1kHn-VdmQrAqm7PwHdWUaMqhgyQvk1yt3sPz5Abv99fS1IvA3fF4ihjbXu78JtNsenclssGYdvi2UYqiqlBNzAy06/s1600/Eagle_nebula_pillars.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></td></tr>
<tr><td class="tr-caption"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 15.828125px; text-align: left;"><span style="color: #073763; font-size: small;"><b style="background-color: white;">Os "Pilares da Criação" </b></span></span></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; font-size: small; line-height: 15.828125px; text-align: left;"><b>no interior da Nebulosa da Águia</b>.</span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 15.828125px; text-align: left;"> </span><small style="line-height: 15.828125px; text-align: left;">Cortesia <a href="http://pt.wikipedia.org/wiki/NASA" style="background-image: none; text-decoration: none;" title="NASA">NASA</a>/<a href="http://pt.wikipedia.org/wiki/ESA" style="background-image: none; text-decoration: none;" title="ESA">ESA</a><br /><a href="http://pt.wikipedia.org/wiki/Ficheiro:Eagle_nebula_pillars.jpg" style="text-decoration: none;">http://pt.wikipedia.org/wiki/Ficheiro:Eagle_nebula_pillars.jpg</a><br /><span style="line-height: 19.1875px;">Credit: NASA, Jeff Hester, and Paul Scowen (Arizona State University)</span></small></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 19.1875px; text-align: start;">"</span><b style="line-height: 19.1875px; text-align: start;">Os pilares da criação</b><span style="line-height: 19.1875px; text-align: start;">" é um aglomerado de poeira e gás com tamanho interestelar na nebulosa de Aguia situado à aproximadamente 7,000 anos luz da terra, No nome, "Pilares" é sugestivo ao formato do lugar, e a parte "Criação" originou-se devido o local ser um enorme berço de estrelas. Sua primeira imagem datada em 1/04/1995, foi tirada pelo telescópio espacial Hubble.</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Pilares_da_Cria%C3%A7%C3%A3o" style="background-color: white; text-decoration: none;">http://pt.wikipedia.org/wiki/Pilares_da_Cria%C3%A7%C3%A3o</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">The Eagle has risen: Stellar spire in the Eagle Nebula</span></h1>
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<a href="http://www.spacetelescope.org/images/heic0506b/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spacetelescope.org/images/heic0506b/</span></a><br />
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<strong style="border: 0px; margin: 0px 0px 15px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Credit:</span></strong></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nasa.gov/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">NASA</a>, <a href="http://www.esa.int/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">ESA</a>, and The Hubble Heritage Team <a href="http://www.stsci.edu/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">STScI</a>/<a href="http://www.aura-astronomy.org/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">AURA</a>)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Appearing like a winged fairy-tale creature poised on a pedestal, this object is actually a billowing tower of cold gas and dust rising from a stellar nursery called the Eagle Nebula. The soaring tower is 9.5 light-years or about 90 trillion kilometres high, about twice the distance from our Sun to the next nearest star.</span></div>
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<span style="line-height: 16px; text-align: left;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">Hubble peers deeply into the Eagle Nebula</b></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong style="border: 0px; margin: 0px 0px 15px; outline: 0px; padding: 0px; vertical-align: baseline;">Credit: </strong>ESA/Hubble & NASA</span></div>
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<a href="http://www.spacetelescope.org/images/potw1033a/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spacetelescope.org/images/potw1033a/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The NASA/ESA Hubble Space Telescope has once more turned its attention towards the magnificent Eagle Nebula (Messier 16). This picture shows the northwestern part of the region, well away from the centre, and features some very bright young stars that formed from the same cloud of material. These energetic toddlers are part of an open cluster and emit ultraviolet radiation that causes the surrounding nebula to glow.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The star cluster is very bright and was discovered in the mid-eighteenth century. The nebula, however, is much more elusive and it took almost a further two decades for it to be first noted by Charles Messier in 1764. Although it is commonly known as the Eagle Nebula, its official designation is Messier 16 and the cluster is also named NGC 6611. One spectacular area of the nebula (outside the field of view) has been nicknamed “The Pillars of Creation” ever since the Hubble Space Telescope captured an iconic image of dramatic pillars of star-forming gas and dust.</span></div>
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<span class="watch-title yt-uix-expander-head" dir="ltr" id="eow-title" style="-webkit-user-select: auto; border: 0px; cursor: auto; margin: 0px; padding: 0px;" title="Pillars Of Creation"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Pillars Of Creation - VÍDEO</span></span></h1>
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<a href="https://www.youtube.com/watch?v=9D9q-7lqZdc" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">https://www.youtube.com/watch?v=9D9q-7lqZdc</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><a href="http://annesastronomynews.com/annes-image-of-the-day-the-flaming-skull-nebula/">http://annesastronomynews.com/annes-image-of-the-day-the-flaming-skull-nebula/</a></span><br />
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<strong style="border: 0px; margin: 0px; outline: 0px; padding: 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The Flaming Skull Nebula, a planetary nebula in Serpens Cauda</span></strong></div>
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<a href="http://annesastronomynews.com/photo-gallery-ii/nebulae-clouds/the-flaming-skull-nebula-sh2-68/" rel="attachment wp-att-9906" style="border: 0px; margin: 0px; outline: 0px; padding: 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Sharpless 68, Sh2-68" class="aligncenter size-full wp-image-9906" src="http://annesastronomynews.com/wp-content/uploads/2012/02/The-Flaming-Skull-Nebula-Sh2-68.jpg" style="border: none; display: block; margin: 0px auto; max-width: 100%; outline: 0px; padding: 0px;" width="1024" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Image Credit: <em style="border: 0px; margin: 0px; outline: 0px; padding: 0px;">T.A. Rector (University of Alaska Anchorage) and H. Schweiker (WIYN and NOAO/AURA/NSF)</em></span></div>
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<span style="background-color: white; border: 0px; color: #073763; margin: 0px; outline: 0px; padding: 0px;"><span style="font-family: Arial, Helvetica, sans-serif;"><b>The Flaming Skull Nebula (Sharpless 68 or Sh2-68) </b></span><span style="font-family: Arial, Helvetica, sans-serif;">is a large planetary nebula located in the northern part of the constellation of Serpens Cauda, the Serpent’s Tail. (The Serpens constellation is unique among the constellations in being split into two non-contiguous parts, Serpens Caput, the Serpent’s Head to the west and Serpens Cauda to the east. Between these two halves lies the constellation of Ophiuchus, the Serpent-Bearer.)</span></span></div>
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<span style="border: 0px; margin: 0px; outline: 0px; padding: 0px;"><a href="http://annesastronomynews.com/annes-image-of-the-day-the-flaming-skull-nebula/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://annesastronomynews.com/annes-image-of-the-day-the-flaming-skull-nebula/</span></a></span></div>
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<a href="http://annesastronomynews.com/annes-image-of-the-day-merging-galaxies-arp-220/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://annesastronomynews.com/annes-image-of-the-day-merging-galaxies-arp-220/</span></a><br />
<strong style="border: 0px; line-height: 25.59375px; margin: 0px; outline: 0px; padding: 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Arp 220, merging galaxies in Serpens</span></strong><br />
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<a href="http://annesastronomynews.com/annes-image-of-the-day-merging-galaxies-arp-220/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://annesastronomynews.com/annes-image-of-the-day-merging-galaxies-arp-220/</span></a><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Image Credit: <em style="border: 0px; margin: 0px; outline: 0px; padding: 0px;">ESA/NASA and WikiSky</em></span></div>
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<strong style="border: 0px; margin: 0px; outline: 0px; padding: 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Arp 220 is the result of a collision between two galaxies which are now in the process of merging, situated some 250 million light-years away from Earth in the northern constellation of Serpens (the Serpent). It is receding from us at about 5434 kilometers per second.</span></strong></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Arp 220</span></h1>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://www.spacetelescope.org/static/archives/images/screen/heic0810bf.jpg" /></span><br />
<a href="http://www.spacetelescope.org/images/heic0810bf/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spacetelescope.org/images/heic0810bf/</span></a><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NASA, ESA, the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Arp 220 appears to be a single, odd-looking galaxy, but is in fact a nearby example of the aftermath of a collision between two spiral galaxies. It is the brightest of the three galactic mergers closest to Earth, about 250 million light-years away in the constellation of Serpens, the Serpent. The collision, which began about 700 million years ago, has sparked a cracking burst of star formation, resulting in about 200 huge star clusters in a packed, dusty region about 5,000 light-years across (about 5 percent of the Milky Way's diameter).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Super Star Clusters in Dust-Enshrouded Galaxy</span></h1>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><img src="http://www.spacetelescope.org/static/archives/images/screen/opo0626a.jpg" /></span><br />
<a href="http://www.spacetelescope.org/images/opo0626a/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spacetelescope.org/images/opo0626a/</span></a><br />
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<tr style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><strong style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Name:</span></strong></td><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Arp+220" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">Arp 220</a>, <a href="http://simbad.u-strasbg.fr/simbad/sim-id?Ident=IC+4553" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">IC 4553</a></span></td></tr>
<tr style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><strong style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Type:</span></strong></td><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">• Local Universe : Galaxy : Activity : AGN : Seyfert<br />• X - Galaxies Images/Videos</span></td></tr>
<tr style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><strong style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Distance:</span></strong></td><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">250 million <a href="http://en.wikipedia.org/wiki/Light-year" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">light years</a></span></td></tr>
<tr style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><strong style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Constellation:</span></strong></td><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Serpens Caput</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">The sharp eye of the Hubble Space Telescope's <a href="http://www.spacetelescope.org/about/general/instruments/acs.html" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">Advanced Camera for Surveys</a> has uncovered more than 200 mammoth star clusters in the heart of the galaxy Arp 220.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">The clusters are the bluish-white dots scattered throughout the image. The heftiest Arp 220 cluster - about 10 million solar masses - is twice as massive as any comparable star cluster in the Milky Way Galaxy. Arp 220 collided with another galaxy about 700 million years ago, fueling the frenzy of star birth in a small region about 5,000 light-years across. The galaxy is a nearby example of the aftermath of two colliding galaxies.</span></div>
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<strong style="border: 0px; margin: 0px 0px 15px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Credit:</span></strong></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://www.nasa.gov/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">NASA</a>, <a href="http://www.esa.int/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">ESA</a>, and The Hubble Heritage Team <a href="http://www.stsci.edu/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">STScI</a>/<a href="http://www.aura-astronomy.org/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">AURA</a>)</span></div>
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<a href="http://www.spacetelescope.org/images/opo0626a/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">http://www.spacetelescope.org/images/opo0626a/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">A Wheel within a Wheel</span></h1>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://www.spacetelescope.org/static/archives/images/screen/opo0221a.jpg" /></span><br />
<a href="http://www.spacetelescope.org/images/opo0221a/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spacetelescope.org/images/opo0221a/</span></a><br />
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<strong style="border: 0px; margin: 0px 0px 15px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Credit:</span></strong></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nasa.gov/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">NASA</a>/<a href="http://www.esa.int/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">ESA</a> and The Hubble Heritage Team <a href="http://www.stsci.edu/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">STScI</a>/<a href="http://www.aura-astronomy.org/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">AURA</a>)</span></div>
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<tr style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><strong style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Name:</span></strong></td><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><a href="http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Hoag%27s+Object" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Hoag's Object</span></a></td></tr>
<tr style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><strong style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Type:</span></strong></td><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">• Local Universe : Galaxy : Type : Ring<br />• X - Galaxies Images/Videos</span></td></tr>
<tr style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><strong style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distance:</span></strong></td><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">550 million <a href="http://en.wikipedia.org/wiki/Light-year" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">light years</a></span></td></tr>
<tr style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><strong style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constellation:</span></strong></td><td style="border: 2px !important; margin: 0px; outline: 0px; padding: 2px !important; vertical-align: baseline;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Serpens Caput</span></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A nearly perfect ring of hot, blue stars pinwheels about the yellow nucleus of an unusual galaxy known as Hoag's Object. This image from the NASA/ESA Hubble Space Telescope captures a face-on view of the galaxy's ring of stars, revealing more detail than any existing photo of this object.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A nearly perfect ring of hot, blue stars pinwheels about the yellow nucleus of an unusual galaxy known as Hoag's Object. This image from the <a href="http://www.nasa.gov/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">NASA</a>/<a href="http://www.esa.int/" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">ESA</a> Hubble Space Telescope captures a face-on view of the galaxy's ring of stars, revealing more detail than any existing photo of this object.</span></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><br /><br /><br /><a href="http://annesastronomynews.com/annes-picture-of-the-day-spiral-galaxy-ngc-6118/">http://annesastronomynews.com/annes-picture-of-the-day-spiral-galaxy-ngc-6118/</a></span><br />
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<strong style="border: 0px; margin: 0px; outline: 0px; padding: 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 6118, a grand design spiral galaxy in Serpens</span></strong></div>
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<a href="http://annesastronomynews.com/photo-gallery-ii/galaxies-clusters/ngc-6118-with-sn-2004dk/" rel="attachment wp-att-8945" style="border: 0px; margin: 0px; outline: 0px; padding: 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="The Blinking Galaxy" class="aligncenter size-full wp-image-8945" src="http://annesastronomynews.com/wp-content/uploads/2012/02/NGC-6118-with-SN-2004dk.jpg" style="border: none; display: block; margin: 0px auto; max-width: 100%; outline: 0px; padding: 0px;" width="1021" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Image Credit: <em style="border: 0px; margin: 0px; outline: 0px; padding: 0px;">ESO</em></span></div>
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<strong style="border: 0px; margin: 0px; outline: 0px; padding: 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 6118 (also known as the Blinking Galaxy) is a “grand design” spiral galaxy of roughly 110,000 light-years across (more or less the same size as our own Milky Way galaxy), located about 82.9 million light-years away from Earth in the southern constellation of Serpens (the Snake). It is receding from us at approximately 1573 kilometers per second.</span></strong></div>
<a href="http://annesastronomynews.com/annes-picture-of-the-day-spiral-galaxy-ngc-6118/"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://annesastronomynews.com/annes-picture-of-the-day-spiral-galaxy-ngc-6118/</span></a><br />
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<a href="http://en.wikipedia.org/wiki/Serpens_south"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://en.wikipedia.org/wiki/Serpens_south</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>The Serpens South star cluster</b> is a relatively dense group of 50 young stars, 35 of which are protostars just beginning to form. The <a href="http://en.wikipedia.org/wiki/Star_cluster" style="background-image: none; text-decoration: none;" title="Star cluster">cluster</a> is situated in the southern portion of the <a href="http://en.wikipedia.org/wiki/Serpens" style="background-image: none; text-decoration: none;" title="Serpens">Serpens</a> cloud, located approximately 848 <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Light_year" style="background-image: none; text-decoration: none;" title="Light year">light-years</a> away from Earth.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The cluster was uncovered by NASA's <a href="http://en.wikipedia.org/wiki/Spitzer_Space_Telescope" style="background-image: none; text-decoration: none;" title="Spitzer Space Telescope">Spitzer Space Telescope</a> in the southern portion of the Serpens cloud. The discovery was possible due to the<a href="http://en.wikipedia.org/wiki/Infrared" style="background-image: none; text-decoration: none;" title="Infrared">infrared</a> observation capabilities of the SST because at visible <a href="http://en.wikipedia.org/wiki/Wavelength" style="background-image: none; text-decoration: none;" title="Wavelength">wavelengths</a> the stars are completely obscured by <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Interstellar_dust" style="background-image: none; text-decoration: none;" title="Interstellar dust">interstellar dust</a> in the Serpens cloud.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The stars of the cluster were dubbed "siblings" by the team of astronomers led by Dr. Robert Gutermuth, of the <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Harvard-Smithsonian_Center_for_Astrophysics" style="background-image: none; text-decoration: none;" title="Harvard-Smithsonian Center for Astrophysics">Harvard-Smithsonian Center for Astrophysics</a>, because they were able to determine that the newly discovered stars belonged to the Serpens star-forming cloud,<sup class="reference" id="cite_ref-1" style="line-height: 1em;"><a href="http://en.wikipedia.org/wiki/Serpens_south#cite_note-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup> which also hosts the previously known Serpens embedded cluster, three degrees to the north.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The discovery of Serpens South is a direct result of the <a href="http://en.wikipedia.org/wiki/Gould_Belt_Survey" style="background-image: none; text-decoration: none;" title="Gould Belt Survey">Gould's Belt Legacy</a> project, which aims to study all prominent star-forming regions within about 1,600 light-years of Earth. These regions together form a ring of molecular clouds and associated young stars known as the <a href="http://en.wikipedia.org/wiki/Gould_Belt" style="background-image: none; text-decoration: none;" title="Gould Belt">Gould’s Belt</a> and was first described by astronomer <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Benjamin_Gould" style="background-image: none; text-decoration: none;" title="Benjamin Gould">Benjamin Gould</a> in 1879. Astronomers working on the project are trying to determine how members of large stellar families are related.<sup class="reference" id="cite_ref-2" style="line-height: 1em;"><a href="http://en.wikipedia.org/wiki/Serpens_south#cite_note-2" style="background-image: none; text-decoration: none; white-space: nowrap;">[2]</a></sup><sup class="reference" id="cite_ref-3" style="line-height: 1em;"><a href="http://en.wikipedia.org/wiki/Serpens_south#cite_note-3" style="background-image: none; text-decoration: none; white-space: nowrap;">[3]</a></sup></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://upload.wikimedia.org/wikipedia/commons/6/67/Serpens_south.jpg" /></span><br />
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><a href="http://upload.wikimedia.org/wikipedia/commons/6/67/Serpens_south.jpg"><span style="font-family: Arial, Helvetica, sans-serif;">http://upload.wikimedia.org/wikipedia/commons/6/67/Serpens_south.jpg</span></a></span><br />
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="padding-right: 0.4em; text-align: right; width: 156.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Source</span></td><td><a class="external free" href="http://ipac.jpl.nasa.gov/media_images/sig07-014.jpg" rel="nofollow"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://ipac.jpl.nasa.gov/media_images/sig07-014.jpg</span></a></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="padding-right: 0.4em; text-align: right; width: 156.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Author</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Image creadit: NASA/JPL-Caltech/L. Allen (Harvard-Smithsonian CfA) & Gould's Belt Legacy Team</span></td></tr>
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<span style="font-weight: bold; line-height: 20px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Stellar Families: Young Stars in Serpens</span></span></div>
<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Credit</span></dt>
<dd property="photoshop:Credit" style="margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NASA/JPL-Caltech/L. Allen (Harvard-Smithsonian CfA) & Gould's Belt Legacy Team</span></dd></dl>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">About the Object</span></h3>
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<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Name</span></dt>
<dd style="margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span property="dc:subject">Serpens South</span> • <span property="dc:subject">W40</span></span></dd>
<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Type</span></dt>
<dd property="avm:Subject.Category" style="margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Star > Grouping > Cluster</span></dd><dd property="avm:Subject.Category" style="margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Star > Evolutionary Stage > Protostar</span></dd><dd property="avm:Subject.Category" style="margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Nebula > Appearance > Dark > Molecular Cloud</span></dd>
<dt style="font-weight: bold; margin: 0px; padding: 3px 0px 0px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distance</span></dt>
<dd property="avm:Distance" style="margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">848 Light Years</span></dd></dl>
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<span class="watch-title yt-uix-expander-head" dir="ltr" id="eow-title" title="The Largest Galaxy in the Universe: IC 1101"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">The Largest Galaxy in the Universe: IC 1101</span></span></h1>
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<span class="watch-title yt-uix-expander-head" dir="ltr" title="The Largest Galaxy in the Universe: IC 1101"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">https://www.youtube.com/watch?v=UE8yHySiJ4A</span></b></span></div>
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<span class="watch-title yt-uix-expander-head" dir="ltr" title="The Largest Galaxy in the Universe: IC 1101"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><br /></span></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">IC 1101</b><span style="line-height: 19.1875px; text-align: start;"> é um </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_lenticular" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Galáxia lenticular">galáxia lenticular</a><span style="line-height: 19.1875px; text-align: start;"> gigante no centro do </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_de_gal%C3%A1xias" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Aglomerado de galáxias">aglomerado de galáxias</a><span style="line-height: 19.1875px; text-align: start;"> </span><a href="http://pt.wikipedia.org/wiki/Abell_2029" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Abell 2029">Abell 2029</a><span style="line-height: 19.1875px; text-align: start;">. Ela é classificada como uma galáxia cD. Está a 1 bilhão de </span><a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Ano-luz">anos-luz</a><span style="line-height: 19.1875px; text-align: start;"> de distância, na constelação de </span><a href="http://pt.wikipedia.org/wiki/Serpens" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Serpens">Serpens</a><span style="line-height: 19.1875px; text-align: start;">. Esta galáxia tem um diâmetro de aproximadamente 6 milhões de anos-luz, e é atualmente (desde 2011) a maior galáxia conhecida em termos de largura.</span><span class="reference" id="cite_ref-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/IC_1101#cite_note-2" style="background-image: none; text-decoration: none;">2</a></span><span style="line-height: 19.1875px; text-align: start;"> Acredita-se que contenha até 100 trilhões de estrelas, em comparação com</span><a href="http://pt.wikipedia.org/wiki/Via_L%C3%A1ctea" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Via Láctea">nossa galáxia</a><span style="line-height: 19.1875px; text-align: start;"> estimada em 200 bilhões de estrelas, ou a </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Galáxia de Andrômeda">Andrômeda</a><span style="line-height: 19.1875px; text-align: start;"> estimada em 400 bilhões. Se estivesse no lugar da nossa galáxia, engoliria a </span><a href="http://pt.wikipedia.org/wiki/Grande_Nuvem_de_Magalh%C3%A3es" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Grande Nuvem de Magalhães">Grande Nuvem de Magalhães</a><span style="line-height: 19.1875px; text-align: start;">, a </span><a href="http://pt.wikipedia.org/wiki/Pequena_Nuvem_de_Magalh%C3%A3es" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Pequena Nuvem de Magalhães">Pequena Nuvem de Magalhães</a><span style="line-height: 19.1875px; text-align: start;">, a </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Galáxia de Andrômeda">Galáxia de Andrômeda</a><span style="line-height: 19.1875px; text-align: start;"> e a </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Galáxia do Triângulo">Galáxia do Triângulo</a><span style="line-height: 19.1875px; text-align: start;">.</span></span></div>
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<tr><th class="" colspan="2" style="vertical-align: top;"><span class=""><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">IC 1101</span></span></th></tr>
<tr><th colspan="2" style="vertical-align: top;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dados observacionais (J2000)</span></b></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelação</span></a></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Serpens" style="background-image: none; text-decoration: none;" title="Serpens"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Serpens</span></a></td></tr>
<tr><td scope="row" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo</span></td><td valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S0<span class="reference" id="cite_ref-ned_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/IC_1101#cite_note-ned-1" style="background-image: none; text-decoration: none;">1</a></span></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-image: none; text-decoration: none;" title="Ascensão reta"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Asc. reta</span></a></td><td valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 10<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 56,1<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-ned_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/IC_1101#cite_note-ned-1" style="background-image: none; text-decoration: none;">1</a></span></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Declinação"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Declinação</span></a></td><td valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">+05° 44′ 41″<span class="reference" id="cite_ref-ned_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/IC_1101#cite_note-ned-1" style="background-image: none; text-decoration: none;">1</a></span></span></td></tr>
<tr><td scope="row" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distância</span></td><td valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1,07 bilhões de <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-image: none; text-decoration: none;" title="Ano-luz">anos-luz</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Desvio_para_o_vermelho" style="background-image: none; text-decoration: none;" title="Desvio para o vermelho"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Redshift</span></a></td><td valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">23370 ± 30<span class="reference" id="cite_ref-ned_1-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/IC_1101#cite_note-ned-1" style="background-image: none; text-decoration: none;">1</a></span></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; text-decoration: none;" title="Magnitude aparente"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnit. apar.</span></a></td><td valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">+14.7<span class="reference" id="cite_ref-ned_1-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/IC_1101#cite_note-ned-1" style="background-image: none; text-decoration: none;">1</a></span></span></td></tr>
<tr><td scope="row" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dimensões</span></td><td valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1',2 × 0',6<span class="reference" id="cite_ref-ned_1-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/IC_1101#cite_note-ned-1" style="background-image: none; text-decoration: none;">1</a></span></span></td></tr>
<tr><th colspan="2" style="vertical-align: top;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Outras denominações</span></b></th></tr>
<tr><td colspan="2" valign="top"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">UGC 9752<span class="reference" id="cite_ref-ned_1-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/IC_1101#cite_note-ned-1" style="background-image: none; text-decoration: none;">1</a></span> ; PGC 54167<span class="reference" id="cite_ref-ned_1-7" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/IC_1101#cite_note-ned-1" style="background-image: none; text-decoration: none;">1</a></span></span></td></tr>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;"><a href="http://pt.wikipedia.org/wiki/IC_1101" style="background-color: white; text-decoration: none;">http://pt.wikipedia.org/wiki/IC_1101</a></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><br /><b>CONFIRA EM:</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://scaleofuniverse.com/" style="background-color: white; text-decoration: none;">http://scaleofuniverse.com/</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><br /><img alt="The Night Sky Atlas logo image" src="http://www.nightskyatlas.com/logo.gif" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
<div style="line-height: 18px;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br />ENCONTRE MAIORES INFORMAÇÕES SOBRE SERPENS</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">acessando </span></div>
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<a href="http://www.nightskyatlas.com/index.jsp" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.nightskyatlas.com/index.jsp</span></a></div>
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<tr><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Skyatlas PNG Image" src="http://www.nightskyatlas.com/skyatlas.jsp?rightAscension=18.1&declination=-3.6&viewAngle=90.0&viewRotation=0.0&width=700&height=500" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; margin-left: auto; margin-right: auto; padding: 8px;" /></span></td></tr>
<tr><td class="tr-caption"><a href="http://www.nightskyatlas.com/index.jsp?rightAscension=18.1&declination=-3.6" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">http://www.nightskyatlas.com/index.jsp?rightAscension=18.1&declination=-3.6</span></a></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<tr><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Skyatlas PNG Image" src="http://www.nightskyatlas.com/skyatlas.jsp?rightAscension=15.8&declination=10.7&viewAngle=90.0&viewRotation=0.0&width=700&height=500" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; margin-left: auto; margin-right: auto; padding: 8px;" /></span></td></tr>
<tr><td class="tr-caption"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://www.nightskyatlas.com/index.jsp?rightAscension=15.8&declination=10.7" style="background-color: white; text-decoration: none;">http://www.nightskyatlas.com/index.jsp?rightAscension=15.8&declination=10.7</a></span><br />
<div class="MsoNormal">
<a href="http://www.nightskyatlas.com/starnames.jsp" style="text-decoration: none;"><span class="Ttulo1Char"><span style="line-height: 11px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">http://www.nightskyatlas.com/starnames.jsp</span></span></span></a></div>
<h1 style="margin: 0px; position: relative;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Named Stars Index - The Night Sky Atlas</span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span lang="EN-US"></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Star Name<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Bayer<br />Designation<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Description<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Offsite Links<o:p></o:p></span></div>
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<span style="background-color: white;"><span lang="EN-US" style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span lang="EN-US"></span><br />
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<tr style="height: 27pt;"><td colspan="4" style="height: 27pt; padding: 0cm;" valign="bottom"><div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Serpens: </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=18.937&declination=4.202&viewAngle=25" style="text-decoration: none;">Alya</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">θ2<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Theta 2<o:p></o:p></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">´the fatty tail´ (of a breed of Oriental sheep)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=15.770&declination=15.422&viewAngle=25" style="text-decoration: none;">Chow</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">β<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Beta<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">´imperial dynasty´<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=15.738&declination=6.426&viewAngle=25" style="text-decoration: none;"><span lang="EN-US">Unuk Al Hay or Unukalhai</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">α<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Alpha<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">´neck of the snake´<o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><br /></span></span></div>
<span style="background-color: white;"><span lang="EN-US" style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span lang="EN-US"><br /></span><span lang="EN-US"><br /></span><span lang="EN-US"><br /></span></span></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><br />
</span><br />
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<span class="Ttulo1Char"><span style="line-height: 11px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://www.nightskyatlas.com/dsoNames.jsp" style="background-color: white; text-decoration: none;">http://www.nightskyatlas.com/dsoNames.jsp</a></span></span></span><br />
<span class="Ttulo1Char"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; line-height: 11px;"><br /></span></span></div>
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<b><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">DSO Names - The Night Sky Atlas<o:p></o:p></span></span></b></div>
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<b><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Popular Deep Space Objects<o:p></o:p></span></span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Common Name<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Catalog Numbers<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">RA<br />hours<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">DEC<br />degrees<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Notes<o:p></o:p></span></div>
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<tr><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"></td><td style="padding: 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"></td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"></td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"></td><td style="padding: 0cm 3.75pt; width: 225pt;" valign="top" width="300"></td></tr>
<tr><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"></td><td style="padding: 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"></td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"></td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"></td><td style="padding: 0cm 3.75pt; width: 225pt;" valign="top" width="300"></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">Serpens: </span><span lang="EN-US">Visible in February before dawn, to October after dusk, best in June.</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<tr><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=18.3133&declination=-13.8067&viewAngle=20.0" style="text-decoration: none;">Eagle Nebula</a><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"><div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">M16<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">18h 18.8m<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-13° 48.4´<o:p></o:p></span></div>
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<tr><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=18.6483&declination=5.45&viewAngle=20.0" style="text-decoration: none;">Graff´s Cluster</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">IC4756<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">18h 38.9m<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">+05° 27.0´<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=15.2867&declination=21.5833&viewAngle=20.0" style="text-decoration: none;">Hoag´s Object</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15h 17.2m<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">+21° 35.0´<o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 225pt;" valign="top" width="300"><div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">PGC 54559, PRC D-51; Polar Ring Galaxy in Serpens<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=15.2683&declination=-0.1283&viewAngle=20.0" style="text-decoration: none;">Serpens Dwarf</a><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"></td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15h 16.1m<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-00° 07.7´<o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 225pt;" valign="top" width="300"><div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">UGC 9792, A 1513; Globular Cluster Palomar 5 (former Local Group galaxy suspect)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=15.9867&declination=20.75&viewAngle=20.0" style="text-decoration: none;">Seyfert´s Sextet</a><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"><div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC6027 NGC6027A to NGC6027E<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">15h 59.2m<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">+20° 45.0´<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=18.3&declination=-13.8333&viewAngle=20.0" style="text-decoration: none;">Star Queen Nebula</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">associated with M16<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">18h 18.0m<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-13° 50.0´<o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">also Eagle Nebula, associated with the star cluster M16=NGC 6611<o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Asterisms - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://www.nightskyatlas.com/asterisms.jsp" style="text-decoration: none;"><span class="Ttulo1Char"><span lang="EN-US" style="line-height: 14px;">http://www.nightskyatlas.com/asterisms.jsp</span></span></a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=18.0833&declination=-3" style="text-decoration: none;">Bull of Poniatowski</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">4<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">3.5 deg<o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A ´V´ shaped group of stars consisting of 66;67;68;70 and 73 Ophiuchi; similar to Hyades ´V´; also Mel 186</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span lang="EN-US">Principal Stars of Serpens - The Night Sky Atlas</span> </span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://www.nightskyatlas.com/stardata.jsp?id=SER" style="text-decoration: none;"><span class="Ttulo1Char"><span lang="EN-US" style="font-weight: normal;">http://www.nightskyatlas.com/stardata.jsp?id=SER</span></span></a><span lang="EN-US"><o:p></o:p></span></span></h1>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Galaxy Clusters of Serpens - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/catAbell.jsp?id=SER" style="text-decoration: none;"><span class="Ttulo1Char"><span lang="EN-US" style="line-height: 14px;">http://www.nightskyatlas.com/catAbell.jsp?id=SER</span></span></a><o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">IC Objects in Serpens - The Night Sky Atl<o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://www.nightskyatlas.com/icData.jsp?id=SER" style="text-decoration: none;"><span class="Ttulo1Char"><span lang="EN-US" style="font-weight: normal;">http://www.nightskyatlas.com/icData.jsp?id=SER</span></span></a><o:p></o:p></span></h1>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">NGC Objects in Serpens - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Multiple Stars of Serpens - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span class="Ttulo1Char"><span lang="EN-US" style="font-weight: normal;"><a href="http://www.nightskyatlas.com/multipleStars.jsp?id=SER" style="text-decoration: none;">http://www.nightskyatlas.com/multipleStars.jsp?id=SER</a></span></span><o:p></o:p></span></h1>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Principal Stars of Serpens - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://www.nightskyatlas.com/stardata.jsp?id=SER" style="text-decoration: none;"><span class="Ttulo1Char"><span lang="EN-US" style="font-weight: normal;">http://www.nightskyatlas.com/stardata.jsp?id=SER</span></span></a><span lang="EN-US"><o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_011.jpg" /></span></div>
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<a href="http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_011.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_011.jpg</span></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">Conheça </b></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">Ophiucus, O Serpentário,</b></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">acessando</b></span><br />
<a href="http://sobreophiucuseserpens.blogspot.com.br/2013/11/ophiucus-o-serpentario.html"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">http://sobreophiucuseserpens.blogspot.com.br/2013/11/ophiucus-o-serpentario.html</b></span></a></div>
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<span style="font-size: small;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas são como janelas que se abrem para a infinitude do universo e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e sendo por nossa mente conscientizado. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">COM UM ABRAÇO ESTRELADO,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>REFERÊNCIAS BIBLIOGRÁFICAS IMPRESSAS para Serpens Caput e Serpens Cauda:</b><o:p></o:p></span></div>
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<span lang="PT" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">COMPILAÇÃO E TRADUÇÃO literal (quando necessária) de Janine Milward:</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As Cartas Celestes foram realizadas por Mario Jaci Monteiro e escaneadas por Janine<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- </span><b>Mario Jaci Monteiro</b> , <b>As Constelações, Cartas Celestes</b> -<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- <b>Wil Tirion - Atlas of the Night Sky</b> - The Hamlyn Publishing Group Limited, London, England</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- <b>Antonin Rükl - The Hamlyn Encyclopedia of Stars & Planets</b> - The Hamlyn Publishng Group Limited, London, England</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- <b>Richard Hinckley Allen, Star Names, Their Lore and Meaning</b>, Dover Publications, Inc, New York, USA</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- <b>Bernard Pellequer - Pequeno Guia do Céu</b> - Editora Martins Fontes, São Paulo, Brasil</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- <b>Identificação do Céu</b> (Livro que foi sendo revisado e reeditado algumas vezes) de autoria de <b>Fernando Vieira</b>,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Secretaria Municipal de Cultura, Fundação Planetário da Cidade do Rio de Janeiro<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(com dedicatória do próprio autor para mim em Curso de Identificação do Céu,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em 30/07/1999))<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do <b>Atlas Celeste</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">de autoria de <b>Ronaldo Rogério de Freitas Mourão</b>,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(com dedicatória do próprio autor para mim<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em evento realizado no Museu de Astronomia do Rio de Janeiro,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em 16/06/1989)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- </span><b>Mario Jaci Monteiro</b> , <b>As Constelações, Cartas Celestes</b> -<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC - com dedicatória do autor para mim, em março de 2004 (quando Mário Jaci generosamente me presenteou com um instrumento de observação (kepleriano) artesanalmente construído por ele).<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://apod.nasa.gov/apod/ap120722.html</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M16: Pillars of Creation </b><br /><b>Image Credit: </b>J. Hester, P. Scowen (<a href="http://sese.asu.edu/">ASU</a>), <a href="http://www.stsci.edu/hst/HST_overview/">HST</a>, <a href="http://www.nasa.gov/">NASA</a></span></center>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Explanation: </b>It was one of the most <a href="http://pus.sagepub.com/content/13/1/83.full.pdf">famous image</a>s of the 1990s. <a href="http://hubblesite.org/newscenter/archive/releases/1995/44/">This image</a>, taken with the <a href="http://apod.nasa.gov/apod/ap021124.html">Hubble Space Telescope</a> in 1995, shows <a href="http://hubblesite.org/newscenter/archive/releases/1995/44/text/">evaporating gaseous globules</a> (EGGs) emerging from pillars of molecular <a href="http://apod.nasa.gov/apod/ap010113.html">hydrogen gas</a> and <a href="http://apod.nasa.gov/apod/ap030706.html">dust</a>. The <a href="http://apod.nasa.gov/apod/ap970730.html">giant pillars</a> are <a href="http://chandra.harvard.edu/photo/cosmic_distance.html">light years</a> in length and are so dense that interior gas <a href="http://hyperphysics.phy-astr.gsu.edu/hbase/astro/gravc.html">contracts gravitationally</a> to form stars. At each <a href="http://apod.nasa.gov/apod/ap061022.html">pillars' end</a>, the intense radiation of bright young stars causes low density material to boil away, leaving <a href="http://apod.nasa.gov/apod/stellar_nurseries.html">stellar nurseries</a> of dense <a href="http://en.wikipedia.org/wiki/Egg_%28biology%29">EGGs</a> exposed. The <a href="http://messier.seds.org/m/m016.html">Eagle Nebula</a>, associated with the <a href="http://apod.nasa.gov/apod/open_clusters.html">open star cluster</a> <a href="http://apod.nasa.gov/apod/ap030921.html">M16</a>, lies about 7000 <a href="http://chandra.harvard.edu/photo/cosmic_distance.html">light years</a> away. The <a href="http://en.wikipedia.org/wiki/Eagle_Nebula#.27Pillars_of_Creation.27_region">pillars of creation</a> were <a href="http://apod.nasa.gov/apod/ap070111.html">imaged</a> again in 2007 by the orbiting <a href="http://chandra.harvard.edu/about/axaf_mission.html">Spitzer Space Telescope</a> in infrared light, leading to the conjecture that the pillars <a href="http://www.nasa.gov/mission_pages/spitzer/multimedia/ssc2007-01b.html">may already have been destroyed</a> by a local supernova, but light from that event has yet to reach the Earth.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Authors & editors: </b><a href="http://www.phy.mtu.edu/faculty/Nemiroff.html">Robert Nemiroff</a> (<a href="http://www.phy.mtu.edu/">MTU</a>) & <a href="http://antwrp.gsfc.nasa.gov/htmltest/jbonnell/www/bonnell.html">Jerry Bonnell</a> (<a href="http://www.astro.umd.edu/">UMCP</a>)<br /><b>NASA Official: </b>Phillip Newman <a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply">Specific rights apply</a>.<br /><a href="http://www.nasa.gov/about/highlights/HP_Privacy.html">NASA Web Privacy Policy and Important Notices</a><br /><b>A service of:</b> <a href="http://astrophysics.gsfc.nasa.gov/">ASD</a> at <a href="http://www.nasa.gov/">NASA</a> / <a href="http://www.nasa.gov/centers/goddard/">GSFC</a><br /><b>&</b> <a href="http://www.mtu.edu/">Michigan Tech. U.</a></span></center>
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<span style="font-weight: bold; line-height: 20px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Cosmic Epic Unfolds in Infrared: The Eagle Nebula</span></span></div>
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<dd property="photoshop:Credit" style="line-height: 12px; margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NASA/JPL-Caltech/N. Flagey (IAS/SSC & A. Noriega-Crespo (SSC/Caltech)</span></dd>
<dt style="font-weight: bold; line-height: 12px; margin: 0px; padding: 3px 0px 0px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Observers</span></dt>
<dd style="line-height: 12px; margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">S. Carey (SSC/Caltech) A. Noriega-Crespo (SSC/Caltech) F. Boulanger (IAS, France) S. Price (AFRL) R. Indebetouw (U. Virginia) N. Flagey (IAS/SSC) R. Paladini (SSC/Caltech) S. Shenoy (SSC/Caltech) F. Marleau (SSC/Caltech) K. Kraemer (AFRL) D. Mizuno (Boston College) D. Padgett (SSC/Caltech) T. Kuchar (Boston College)</span></dd><dd style="line-height: 12px; margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></dd><dd style="line-height: 12px; margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></dd><dd style="line-height: 12px; margin: 0px; padding: 2px 0px 0px 5px; text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br />
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<a href="http://www.raremaps.com/gallery/detail/35567/Le_Globe_Celeste/De%20La%20Croix.html"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/35567/Le_Globe_Celeste/De%20La%20Croix.html</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Title: </strong>Le Globe Celeste</span></div>
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Da Terra ao Céu ....</span></a></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">.....<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="text-decoration: none;">e ao Infinito </a></span></h1>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="background-color: white; text-decoration: none;">- As 88 Constelações</a></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; font-weight: normal; line-height: normal;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; font-weight: normal; line-height: normal;">Com um abraço estrelado,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Janine Milward</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;"><b style="background-color: white;">Serpens Caput e Serpens Cauda, a Serpente</b></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Acessando o Link abaixo, o Leitor encontrará uma Página própria</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">acolhendo Ophiucus e Serpens:</span></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><b style="line-height: 23px;"><a href="http://sobreophiucuseserpens.blogspot.com.br/" style="text-decoration: none;">http://sobreophiucuseserpens.blogspot.com.br/</a></b></span><br />
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<a href="http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_011.jpg" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_011.jpg</span></a></div>
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<tr><td><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEglgM1sJ3bT9VPxDMtqZU0hiOXPzrmkGABBFte2C6qJ3UhItDUIRgcEAM18IfIb1ns4rSWJGri1GKtcPx8upUE6XZeXvUbxmptVOTt8sNfZbpeJm8jGIcFQEdMeRxv_bFGzA5NDzuJOE59V/s1600/OPHIUCUS.gif" imageanchor="1" style="margin-left: auto; margin-right: auto; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEglgM1sJ3bT9VPxDMtqZU0hiOXPzrmkGABBFte2C6qJ3UhItDUIRgcEAM18IfIb1ns4rSWJGri1GKtcPx8upUE6XZeXvUbxmptVOTt8sNfZbpeJm8jGIcFQEdMeRxv_bFGzA5NDzuJOE59V/s1600/OPHIUCUS.gif" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></td></tr>
<tr><td class="tr-caption"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></td></tr>
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<tr><td><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhaiJTfsFLgHNQFwJMvi51SznKOTTRyyV3puG_yNSxkqtvYBeQG0VvjsTBhDMuiHcoK5CZElwKIhSAIKu-sUbsKNBy9xy6S0tGhO02XR_3dr2zv3opEzuEU3oe72LJqlQ4Mz0wbM7IfzDNw/s1600/alfabeto+grego%252C+conven%25C3%25A7%25C3%25B5es+e+uso+da+carta+celeste.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhaiJTfsFLgHNQFwJMvi51SznKOTTRyyV3puG_yNSxkqtvYBeQG0VvjsTBhDMuiHcoK5CZElwKIhSAIKu-sUbsKNBy9xy6S0tGhO02XR_3dr2zv3opEzuEU3oe72LJqlQ4Mz0wbM7IfzDNw/s640/alfabeto+grego%252C+conven%25C3%25A7%25C3%25B5es+e+uso+da+carta+celeste.jpg" height="420" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></td></tr>
<tr><td class="tr-caption"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; line-height: 14px;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; line-height: 14px;"> - excerto apresentando ALFABETO GREGO, CONVENÇÕES E USO DA CARTA CELESTE</span></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b><b><span lang="PT">Da Terra ao Céu<o:p></o:p></span></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="PT"> e ao Infinito</span></b><o:p></o:p></span></div>
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<span lang="PT" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelações, Estrelas e Objetos Celestes<o:p></o:p></span></div>
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<span lang="PT" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(sob o ponto de vista do Mundo Ocidental)<o:p></o:p></span></div>
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<span lang="PT" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Suas histórias, seus mitos, seus significados e suas sintetizadas descrições<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">Reunião das Informações e Compilação,</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">Tradução para a língua portuguesa (em alguns momentos)</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">bem como Comentários Pessoais:</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><span lang="PT">Janine Milward</span></i><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...; bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.</span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Alguns dados<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(tais como Ascensão Reta e Declinação, em muitos dos casos)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">são época/equinócio 1980<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e devem requerer do Caminhante do Céu<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NASA/IPAC</b><b> EXTRAGALACTIC DATABASE –</b><b><o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="text-decoration: none;"><b>http://ned.ipac.caltech.edu/</b></a><b><o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="text-decoration: none;"><b>http://ned.ipac.caltech.edu/forms/byname.html</b></a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<b><span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="EN-US">The</span></b><span class="apple-converted-space"><b><span lang="EN-US"> </span></b></span><b><span lang="EN-US">Internet STELLAR DATABASE</span></b><b><span lang="EN-US"><o:p></o:p></span></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="text-decoration: none;"><b><span lang="EN-US">http://www.stellar-database.com/</span></b></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<o:p></o:p></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhjqa6chiuE4kTp6PGZKfZ1mcvwxecN8JOFWXQiuvsBtmzUadGrqKqhYtnUvghroxu2fULSc908kO8xdZY0JKXSkJSm36D_G_WHeTl9SxqPT7yo7wSRqdOkLqVCorh1ew-7xpQQQzGaHUY/s1600/La_Hire_Philippe_de_1705_Planisphere_Celeste_Septentrional.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhjqa6chiuE4kTp6PGZKfZ1mcvwxecN8JOFWXQiuvsBtmzUadGrqKqhYtnUvghroxu2fULSc908kO8xdZY0JKXSkJSm36D_G_WHeTl9SxqPT7yo7wSRqdOkLqVCorh1ew-7xpQQQzGaHUY/s640/La_Hire_Philippe_de_1705_Planisphere_Celeste_Septentrional.jpg" height="640" width="637" /></span></a></div>
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<a href="http://lhldigital.lindahall.org/cdm/singleitem/collection/test/id/1145"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://lhldigital.lindahall.org/cdm/singleitem/collection/test/id/1145</span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; font-weight: bold; line-height: normal; text-align: start;">La Hire, Philippe de, 1705, Planisphere Celeste Septentrional.</span></span></div>
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<tr><td class="description_col1" id="metadata_nickname_title" style="font-weight: bold; padding: 3px 2px 8px; vertical-align: top; width: 100px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></td><td class="description_col2" id="metadata_title" style="padding: 3px 2px 10px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></td></tr>
<tr><td class="description_col1" id="metadata_nickname_rights" style="font-weight: bold; padding: 3px 2px 8px; vertical-align: top; width: 100px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Rights</span></td><td class="description_col2" id="metadata_rights" style="padding: 3px 2px 10px;"><a class="body_link_11" href="http://www.lindahall.org/imagerepro/index.shtml" style="text-decoration: none;" target="_blank"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="font-size: small;">http://www.lindahall.org/imagerepro/index.shtml</span><span class="icon_11 ui-icon-extlink" style="background-image: url(http://lhldigital.lindahall.org/ui/cdm/default/collection/default/css/images/smoothness-ui-icons_888888_256x240.png); background-position: -35px -83px; display: inline-block; height: 11px; margin: 2px; vertical-align: bottom; width: 12px;"></span></span></a></td></tr>
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<tr><td><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh_dPCdDHMicNadgw8VV_WdsMwRYUAAsjIrZxk50nmSxHnD0lz8MV5nvR-j1ttpEFNLwXffAktvv9fMeFEqELHgwRt4-j6rDZLdmg1JUUXgyTG2VwNNrUbULlQ0U_4Bw3wEHcmiwA-RWVvN/s1600/urania12.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh_dPCdDHMicNadgw8VV_WdsMwRYUAAsjIrZxk50nmSxHnD0lz8MV5nvR-j1ttpEFNLwXffAktvv9fMeFEqELHgwRt4-j6rDZLdmg1JUUXgyTG2VwNNrUbULlQ0U_4Bw3wEHcmiwA-RWVvN/s640/urania12.jpg" height="446" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><b><a href="http://www.ianridpath.com/atlases/urania/urania12.jpg" style="text-decoration: none;" target="_blank">Card 12</a> </b><a href="http://www.ianridpath.com/atlases/urania/urania12.jpg" style="line-height: 13px; text-decoration: none;" target="_blank">Taurus Poniatowski, Serpentarius (i.e. Ophiuchus), Scutum Sobiesky, and Serpens</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><i><span lang="EN-US" style="line-height: 16px;">Urania’s Mirror</span></i><span lang="EN-US" style="line-height: 16px;"> is a boxed set of 32 constellation cards</span></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; line-height: 16px;"> © Ian Ridpath</span></div>
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<a href="http://www.ianridpath.com/atlases/urania.htm" style="text-decoration: none;"><span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">http://www.ianridpath.com/atlases/urania.htm</span></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">OPHIUCUS, OFIÚCO<o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>ou Serpentarius, aquele que Segura a Serpente</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 15h58m / 18h42m Declinação +14<sup>o</sup>.3 / -30<sup>o</sup>.1<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Mito:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Hercules, quando criança, estrangulou duas serpentes enviadas por Juno para matá-lo enquanto dormia em seu berço. Esta constelação também foi chamada de Esculapius, o pai da medicina.<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Ophiuchus" src="http://www.lindahall.org/services/digital/ebooks/bayer/bigpix/040013bc.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.lindahall.org/services/digital/ebooks/bayer/bayer38.shtml" style="background-color: white; text-decoration: none;">http://www.lindahall.org/services/digital/ebooks/bayer/bayer38.shtml</a></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><br /><br /><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Ophiuchus*.html" style="text-decoration: none;">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Ophiuchus*.html</a></span><br />
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.amazon.com/dp/0486210790/ref=rdr_ext_tmb" style="text-decoration: none;">http://www.amazon.com/dp/0486210790/ref=rdr_ext_tmb</a></span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiUq7sfdAtvkDDL99fRvS-8RvUCPtlRGx27VIFLO8kxgO9kl0Cxx6ZzcuzoOE2GlCLqtLT8fyBEJFhPVyC5CbXlngA60afgIoIXH7T8PvmBe6FjWG66Tc3TtTPsYq1S4iiTuNaqqUe1VnZd/s1600/logo+allen+allen.jpg" imageanchor="1" style="clear: left; float: left; margin-bottom: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiUq7sfdAtvkDDL99fRvS-8RvUCPtlRGx27VIFLO8kxgO9kl0Cxx6ZzcuzoOE2GlCLqtLT8fyBEJFhPVyC5CbXlngA60afgIoIXH7T8PvmBe6FjWG66Tc3TtTPsYq1S4iiTuNaqqUe1VnZd/s200/logo+allen+allen.jpg" height="200" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="126" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- </span><b><span lang="EN-US">Richard Hinckley Allen, Star Names, Their Lore and Meaning</span></b><span lang="EN-US">, Dover Publications, Inc, New York, USA <o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Segundo Allen, em seu livro Star Names, Their Lore and Meaning – fantástico livro e já em domínio público – e traduzindo literalmente, de forma simples e sintética, por mim, Janine:<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">Ophiucus vel Serpentarius, o Serpentário</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> – não Ophiucus Serpentarius, é Ofiuco em italiano, Schlangentrager em alemão e Serpentaire em francês.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">…. (Porém) o Serpentário foi normalmente identificado com Asclepios ou Aesculapius, a quem o Rei James I descreveu como “um curador que mais tarde foi feito deus”, com cujas adoradas serpentes eram sempre associados como símbolos de prudência, renovação, sabedoria e o poder de descobrir ervas curadoras. Educado por seu pai Apollo – ou pelo Centauro Quíron -, Aesculapius foi o primeiro em sua profissão e o cirurgião do navio Argo. Quando a famosa viagem terminou, ele estava tão treinado em sua prática que ele pôde até trazer mortos à vida – entre esses, Hippolytus.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sucessivas operações e inúmeras e notáveis curas – e especialmente a tentativa de reviver Órion morto -, levaram Plutão (que temia pela continuidade de seu reino) induzir Júpiter a atingir Aesculapius com um raio e colocá-lo dentre as constelações.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ophiucus também foi associado a Caecius, o Cego, assassinado por Hercules e celebrado por Dante no Inferno. Na verdade, diz-se que o Herói foi atribuído a estas estrelas por Hyginus e nomeou-as com seu nome: uma confusão que pode ter vindo à tona em função das fronteiras entre essas duas constelações – por serem mal-definidas, primeiramente, ou pela similaridade de seus mitos originais em relação a Izhdubar e o dragão Tiamat.<o:p></o:p></span></div>
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<a href="http://www.lindahall.org/services/digital/ebooks/reissig/reissig66.shtml" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.lindahall.org/services/digital/ebooks/reissig/reissig66.shtml</span></a><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Algumas Informações Interessantes acerca esta Constelação:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><b>A 13a. Constelação do Zodíaco</b></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando o Zodíaco foi originalmente nomeado, a Eclíptica não passava pelo Ofiúco, de forma que esta constelação não foi incluída. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Hoje em dia, sim, em função da precessão, Ofiúco recebe a passagem da linha da Eclíptica e o Sol passa um bom tempo aqui depois de ter adentrado a Cabeça do Escorpião e passado ao largo de sua estrela Alpha, Antares.<o:p></o:p></span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgdtd_5NmskKFbG3k-iCoyerJ47wfyKQQIt1VeXrFU0Q0ahe6UGh45iLb0LE_i42MDDQYnw_4Ovn9OsPv6PpWdZR9eehia8cAHaOzYAy10i-z0BSwUA7ps3uGO5QH0_3U0EEe4MDlzn5K0/s1600/stellaiurm+-+sol+e+antares.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgdtd_5NmskKFbG3k-iCoyerJ47wfyKQQIt1VeXrFU0Q0ahe6UGh45iLb0LE_i42MDDQYnw_4Ovn9OsPv6PpWdZR9eehia8cAHaOzYAy10i-z0BSwUA7ps3uGO5QH0_3U0EEe4MDlzn5K0/s640/stellaiurm+-+sol+e+antares.jpg" height="550" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium trabalhado em Programa Corel</span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiFlq1soty0XD5zc6g0D3lCzd-FMHk12ahHKLXPyAbJ9KSAF9f6Z8kJFQgmDM_3KXfQhvxEzRoiet2ivUwWuabrvBoHmYVpwRroIj8uUvIOCnOUV0_oqtnP6xWDYzwnwU1LvXgnqrFQLOg/s1600/stellarium+-+sol+em+ophiucus.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiFlq1soty0XD5zc6g0D3lCzd-FMHk12ahHKLXPyAbJ9KSAF9f6Z8kJFQgmDM_3KXfQhvxEzRoiet2ivUwWuabrvBoHmYVpwRroIj8uUvIOCnOUV0_oqtnP6xWDYzwnwU1LvXgnqrFQLOg/s640/stellarium+-+sol+em+ophiucus.jpg" height="310" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium trabalhado em Programa Corel</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://www.heavens-above.com/wholeskychart.ashx?&size=800&SL=1&SN=1&BW=0&time=56638.57708&ecl=1&cb=1" id="ctl00_ContentPlaceHolder1_imgSkyChart" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; height: 800px; padding: 8px; width: 800px;" /></span></div>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">http://www.heavens-above.com/skychart.aspx</b></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">Movimentos: tudo sempre se move</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Estarei repetindo aquilo que recebi em Fórum na Internet, parte da Aula 2 sobre Movimentos do Céu, by dario.rostirolla@londrina.pr.gov.br:</span></div>
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<i><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">“Como é sabido, a Terra apresenta dois movimentos básicos (e outros): rotação (em torno do próprio eixo, com período de 1 dia) e translação (movimento orbital ao redor do sol, com período de 1 ano). Enquanto gira ao redor do Sol, a Terra percorre em sua órbita cerca de um grau por dia - logo, as estrelas se adiantam um pouco com relação ao Sol (como um carro que se aproxima de uma esquina e obtém melhor visibilidade), cerca de 4 minutos. É esta a causa da pequena diferença entre o dia solar e o dia sideral.</span></i></div>
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<i><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">No decorrer de um ano a Terra percorre 360 graus ao redor do Sol, de modo que as estrelas que se encontravam ocultadas pelo Sol, dentro de algum tempo se tornarão visíveis em função do deslocamento da Terra sobre sua órbita. Ao longo do ano, diferentes partes do céu vão se tornando visíveis em determinado horário fixo (digamos, logo após o pôr do Sol), de modo que toda a esfera celeste vai sendo avistada ao longo do ano, setor por setor. A cada ano, esse movimento se repete de modo que as constelações visíveis numa determinada data serão visíveis na mesma data dos anos subseqüentes.”</span></i></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A precessão dos Equinócios é o movimento que estaria aglutinando, digamos assim, ambos os movimentos anteriores: o de rotação e o de translação. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Não podemos nos esquecer que a Terra gira em torno de seu eixo sim, porém com uma inclinação de 23 graus.... Ao mesmo tempo, a Terra perfaz um passeio de 360 graus em sua órbita em torno ao Sol. Ao mesmo tempo, também o Sol vai realizando seu próprio andamento e o faz em direção a um ponto próximo à constelação Hercules. Tudo no universo se movimenta... por que deixaria nosso Sol de fazer o mesmo?</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ao longo do período de 26 mil anos, esse eixo da Terra em movimento de rotação e de translação e atrelado ainda ao movimento próprio do Sol, vai imantando os direcionamentos norte e sul e deslocando, apontando então para diferentes pontos dessa região da esfera celeste! Esse grande círculo imaginário que se forma é o Grande Ano das Eras! Uma maneira simples de entender esse movimento é soltarmos um pião e o deixarmos girar, girar, girar..... é bem assim. A estrela que denominamos de Polar, vem atuando como imantação Norte desde há muito tempo e ainda estará fazendo isso por bom tempo adiante. Porém, um dia no futuro, teremos que renomeá-la... pois não estará mais reinante na posição de Estrela Polar.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É realmente interessante que possamos perceber as questões relativas às mudanças de Eras em termos de onde caem os Pontos de Equinócios e de Solstícios:</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A Era de Gêmeos trouxe o Ponto Vernal a acontecer dentro desta constelação ocupando o lugar de Primavera, Virgem ocupando o lugar do Solstício do Verão, Sagitário ocupando o lugar do Equinócio do Outono e Peixes ocupando o lugar do Solstício de Inverno.</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quadro sobre a Precessão dos Equinócios durante 4 Eras, mostrando o Caminho do Sol contra o pano de fundo das constelações do Zodíaco. As cores originais foram invertidas.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Inserido no Artigo “When the Zodiac Climbed into the Sky” por Alexander Gurshtein para a Revista Sky & Telescope edição de outubro de 1995, página 30, publicada por Sky Publishing Corporation, Cambridge, MA, USA.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A Era de Touro trouxe o Ponto Vernal a acontecer dentro desta constelação ocupando o lugar de Equinócio da Primavera; Leão ocupando o lugar do Solstício do Verão; Sagitário ocupando o lugar do Equinócio do Outono e Peixes ocupando o lugar do Solstício de Inverno.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Permita-me lhes dizer, caro Amigo das Estrelas, que foi naquela Era que surgiu o conceito das Quatro Estrelas Reais, Guardiãs das Quatro Estações do Ano e da Vida: em Touro, Aldebarã, o olho iluminado, guardiã do Leste; em Leão, Regulus, sua pata dianteira, guardiã do Sul; em Escorpião, Antares, a rival de Marte, Anti-Ars, gigante vermelha maravilhosa, guardiã do Oeste; e finalmente, Fomalhaut, em Pisces Austrinus, guardiã do Norte.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A Era de Áries trouxe o Ponto Vernal a acontecer dentro desta constelação ocupando o lugar de Equinócio da Primavera; Câncer ocupando o lugar de Solstício do Verão; Balança ocupando o lugar do Equinócio do Outono e Capricórnio ocupando o lugar do Solstício de Inverno.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Vega,a estrela Alpha Lyrae, atuou como a estrela polar (há mais de 12 milênios atrás). Vega estará novamente ocupando o lugar de estrela polar mais uns tantos milênios à frente (14.000 anos DC, ou seja mais 12.000 anos à frente) - sempre a estrela polar mais brilhante!</span></div>
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<i><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A Precessão acontece porque as forças gravitacionais do sol e da lua atuam por sobre a Terra (que não é esférica) enquanto esta gira, vagarosamente mudando a orientação do eixo da Terra. Este eixo, inclinado num ângulo de 23<sup>o</sup>., traça um caminho em torno da eclíptica ao longo de 25.800 mil anos terrestres na realização de todo seu círculo. Isso significa que Polaris - a estrela que viemos considerando nossa estrela polar celestial do norte -, vagarosamente irá transmitir sua posição à Vega, a brilhante estrela da constelação da Lira. </span></i></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Extraído da revista Astronomy, edição de junho de 2002, página 73. Parte do texto foi traduzido literalmente por Janine e também a ilustração sobre o caminho do pólo norte celestial foi invertida, para melhor visualização.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">Pequeno Glossário:</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><i>Apex</i></b> <b>- </b>um ponto central para onde outro objeto orbita e se move em direção a.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><i>Apex</i></b><b> do Caminho do Sol</b> - o ponto na esfera celeste em direção ao qual nosso Sol viaja numa velocidade de cerca de 20 quilômetros por segundo. A posição correta do apex do Sol pode variar entre os cientistas porém é quase acordado que seja em Hércules ou Lyra, Ascensão Reta de 18 horas ou 270 graus e Declinação 34 Norte. (3)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Eclíptica (plano da)</b> - Plano da órbita terrestre. Podemos definir também como o grande círculo de interseção deste plano com a esfera celeste. O plano da eclíptica é inclinado de 23<sup>o</sup>27’ em relação ao Equador.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Ponto vernal</b> - ponto da esfera celeste, situado na interseção da eclíptica com o equador, na qual o Sol, em seu movimento aparente anual, passa do hemisfério sul para o norte.(....) O ponto vernal é habitualmente designado pela letra <i>y</i>; equinócio da primavera, equinócio vernal, primeiro ponto de Áries. (1)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Equinócio </b> - Ponto da esfera celeste, interseção da eclíptica com o Equador. O equinócio da primavera corresponde à passagem do Sol do hemisfério austral ao hemisfério boreal. O equinócio do outono é o caso inverso. Tais termos se aplicam também aos momentos em que estes fenômenos ocorrem. Podemos dizer, também, que o equinócio é a data do ano na qual o dia é igual à noite (20-21 de março - 22-23 de setembro) (2)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Precessão dos Equinócios</b> - o movimento do equinócio consiste em uma retrogradação (ou <i>precessão</i>) sobre a <i>eclíptica, </i>da ordem de 50.256 por ano, ou seja, de uma volta completa do equilíbrio em 26.000 anos (2)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Solstício </b> - é o instante no qual o Sol está mais afastado do Equador (22 ou 23 de junho e 22 ou 23 de dezembro) (2) - Nessas datas, acontecem os solstícios de inverno e de verão.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(1) - Atlas Celeste<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ronaldo Rogério de Freitas Mourão<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">6<sup>ª</sup> edição - Editora Vozes, Petrópolis, RJ, Brasil – 1986<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(2) - Explicando o Cosmos<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Editora Tecnoprint S.A., Rio, Brasil, 1984<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">(3)<span style="line-height: normal;"> </span></span><span lang="EN-US">Norton’s Star Atlas<o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Arthur P Norton and J. Gall Inglis<o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sky Publishing Co.<o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Cambridge, MA, USA<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ophiucus situa-se entre as constelações Serpens Cauda e Serpens Caput (e todas três acabam formando um conjunto imenso de situações entrelaçadas), e também Scorpius, Sagittarius, Scutum, Aquila, Hercules Corona Borealis, Libra<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><img src="http://www.nightskyatlas.com/skyatlas.jsp?wpCalendar=1&rightAscension=17.3&declination=-5.0&viewAngle=90.0&viewRotation=0.0&width=1366&height=768" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<a href="http://www.nightskyatlas.com/skyatlas.jsp?wpCalendar=1&rightAscension=17.3&declination=-5.0&viewAngle=90.0&viewRotation=0.0&width=1366&height=768" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.nightskyatlas.com/skyatlas.jsp?wpCalendar=1&rightAscension=17.3&declination=-5.0&viewAngle=90.0&viewRotation=0.0&width=1366&height=768</span></a><br />
<a href="http://www.nightskyatlas.com/index.jsp?rightAscension=17.3&declination=-5.0" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.nightskyatlas.com/index.jsp?rightAscension=17.3&declination=-5.0</span></a><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Algumas Estrelas e alguns objetos interessantes, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em Ofiúco<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Existe um Asterismo interessante denominado de O Touro de Poniatowkski, composto pelas estrelas 66, 67, 68 e 70 Ophiuchi. Este Asterismo já constou como uma Constelação mas foi considerada obsoleta, posteriormente.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Rasalhague. Alpha Ophiuchi. </b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude 2.09 Distância 58 anos-luz<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela safira situada na cabeça do Ofiúco. De Rãs Al Hawwa, a Cabeça daquele que Segura a Serpente, a Cabeça do Serpentário. <o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta estrela se situa ao norte do equador celestial e já quase na fronteira de Ofiúco com a constelação de Hercules.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Cebalrai ou Cheleb - Beta Ophiuci</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude 2.77 Distância 124 anos-luz<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Cão do Pastor, vocábulo oriundo da expressão árabe Kalb al Rai.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="ES-TRAD"><b>Yed Prior</b></span><span lang="ES-TRAD"><b>. Delta Ophiuchi. </b><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">Magnitude 2.72 Distância 140 anos-luz</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela amarelada situada a mão esquerda do Ofiúco. De Yad, a Mão. A Mão Anterior.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US"><b>Yed Posterior</b></span><span lang="EN-US"><b> - Epsilon Ophiuchi</b><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mão Posterior, denominação moderna de oriegem latino-árabe usada por Bayer. A palavra Yed significa mão.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Han. Zeta Ophiuchi. </b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude 2.57 Distância de mais de 500 anos-luz<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela pequena situada próxima ao joelho esquerdo do Ofiuco. Han é um nome de origem chinesa que denominava um velho Estado feudal da China.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Sabik. Eta Ophiuchi. Estrela Dupla</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h09,3m - Declinação -15<sup>o</sup> 42’<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual 2,43 - Distância 69 anos-luz<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela amarelo pálido situada no joelho esquerdo do Ofiúco. De Sabik, Aquela que Precede. O Condutor, do vocábulo árabe Sabik.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="ES-TRAD">Sinistra</span><span lang="ES-TRAD">. Mu Ophiuchi</span></b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela pequena situada na mão esquerda do Ofiúco.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>U Ophiuchii - Estrela Variável do tipo Algol</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h14m Declinação +01<sup>o</sup>.16<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitudes: Max 5,7 Min 6,4 Período 1,7<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo ALG Espectro B8<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Y Ophiuchii - Estrela Variável Cefeida</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h50m Declinação -06<sup>o</sup>.08<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitudes: Max 6,1 Min 6,5 Período 17,1<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo CEF Espectro G0<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Ophiucus - Nebulosa Complexa - Ro Ophiuchi</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 16h24m Declinação -23<sup>o</sup>.24<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo Nebulosa Planetária COM Dimensão 4,0 Distância em anos-luz 0,5<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Ophiucus - Nebulosa Complexa - Theta Ophiuchi</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h20m Declinação -24<sup>o</sup>.59<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo Nebulosa Planetária COM Dimensão 5,0 Magnitude<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude da Estrela associada Distância em anos-luz 0,5<o:p></o:p></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><br /><br /><br /><b>A FAMOSA ESTRELA BARNARD</b></span></div>
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<tr><td><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjL6VUtCrR09EStKIeOm9WKyom6zjJbRGx6kGs9ONPF8IU6wDt3IruqriMYZnTg_eaC6EUkysTRwKIl6IcSA_unwEgVdzI5M7UT6q6fVEn1Fegq0kzwfl-P9mzfLPdIcHAldORm1h0emZ9j/s1600/BARNARD.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjL6VUtCrR09EStKIeOm9WKyom6zjJbRGx6kGs9ONPF8IU6wDt3IruqriMYZnTg_eaC6EUkysTRwKIl6IcSA_unwEgVdzI5M7UT6q6fVEn1Fegq0kzwfl-P9mzfLPdIcHAldORm1h0emZ9j/s640/BARNARD.jpg" height="218" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></td></tr>
<tr><td class="tr-caption"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">EXCERTO de Ophiucus - As Constelações, Cartas Celestes, Mario Jaci Monteiro</span></td></tr>
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<span class="mw-headline" id="Map_of_nearby_stars"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Map of nearby stars</span></span></h2>
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<span class="mw-headline"><a href="http://en.wikipedia.org/wiki/List_of_nearest_stars" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://en.wikipedia.org/wiki/List_of_nearest_stars</span></a></span></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><br /><img alt="Nearby Stars (14ly Radius).svg" src="http://upload.wikimedia.org/wikipedia/commons/thumb/f/ff/Nearby_Stars_%2814ly_Radius%29.svg/600px-Nearby_Stars_%2814ly_Radius%29.svg.png" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">Barnard's Star</b><span style="line-height: 19.1875px; text-align: start;"> </span><span class="nowrap" style="line-height: 19.1875px; text-align: start; white-space: nowrap;"><span class="IPA" title="Representation in the International Phonetic Alphabet (IPA)"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English" style="background-image: none; text-decoration: none !important;" title="Help:IPA for English">/</a></span><span class="IPA nopopups"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English#Key" style="background-image: none; text-decoration: none !important;" title="Help:IPA for English"><span style="border-bottom-style: dotted; border-bottom-width: 1px;" title="/ˈ/ primary stress follows">ˈ</span></a></span><span class="IPA nopopups"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English#Key" style="background-image: none; text-decoration: none !important;" title="Help:IPA for English"><span style="border-bottom-style: dotted; border-bottom-width: 1px;" title="'b' in 'buy'">b</span></a></span><span class="IPA nopopups"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English#Key" style="background-image: none; text-decoration: none !important;" title="Help:IPA for English"><span style="border-bottom-style: dotted; border-bottom-width: 1px;" title="/ɑr/ 'ar' in 'bard'">ɑr</span></a></span><span class="IPA nopopups"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English#Key" style="background-image: none; text-decoration: none !important;" title="Help:IPA for English"><span style="border-bottom-style: dotted; border-bottom-width: 1px;" title="'n' in 'nigh'">n</span></a></span><span class="IPA nopopups"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English#Key" style="background-image: none; text-decoration: none !important;" title="Help:IPA for English"><span style="border-bottom-style: dotted; border-bottom-width: 1px;" title="/ər/ 'er' in 'finger'">ər</span></a></span><span class="IPA nopopups"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English#Key" style="background-image: none; text-decoration: none !important;" title="Help:IPA for English"><span style="border-bottom-style: dotted; border-bottom-width: 1px;" title="'d' in 'dye'">d</span></a></span><span class="IPA" title="Representation in the International Phonetic Alphabet (IPA)"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English" style="background-image: none; text-decoration: none !important;" title="Help:IPA for English">/</a></span></span><span style="line-height: 19.1875px; text-align: start;"> is a very low-mass </span><a href="http://en.wikipedia.org/wiki/Red_dwarf" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Red dwarf">red dwarf</a><span style="line-height: 19.1875px; text-align: start;"> </span><a href="http://en.wikipedia.org/wiki/Star" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Star">star</a><span style="line-height: 19.1875px; text-align: start;"> about six </span><a href="http://en.wikipedia.org/wiki/Light-year" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Light-year">light-years</a><span style="line-height: 19.1875px; text-align: start;"> away from Earth in the </span><a href="http://en.wikipedia.org/wiki/Constellation" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Constellation">constellation</a><span style="line-height: 19.1875px; text-align: start;"> of </span><a href="http://en.wikipedia.org/wiki/Ophiuchus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Ophiuchus">Ophiuchus</a><span style="line-height: 19.1875px; text-align: start;">, the Snake-holder. Barnard's Star is the </span><a href="http://en.wikipedia.org/wiki/List_of_nearest_stars" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="List of nearest stars">fourth-closest</a><span style="line-height: 19.1875px; text-align: start;"> known individual star to the Sun, after the three components of the </span><a href="http://en.wikipedia.org/wiki/Alpha_Centauri" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Alpha Centauri">Alpha Centauri</a><span style="line-height: 19.1875px; text-align: start;"> system, and the closest star in the Northern Hemisphere.</span><sup class="reference" id="cite_ref-14" style="line-height: 1em; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Barnard's_Star#cite_note-14" style="background-image: none; text-decoration: none; white-space: nowrap;">[14]</a></sup><span style="line-height: 19.1875px; text-align: start;"> Despite its proximity, Barnard's Star, at a dim </span><a href="http://en.wikipedia.org/wiki/Apparent_magnitude" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Apparent magnitude">apparent magnitude</a><span style="line-height: 19.1875px; text-align: start;"> of about nine, is not visible with the unaided eye; however, it is much brighter in the </span><a href="http://en.wikipedia.org/wiki/Infrared" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Infrared">infrared</a><span style="line-height: 19.1875px; text-align: start;"> than it is in </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Visible_light" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Visible light">visible light</a><span style="line-height: 19.1875px; text-align: start;">. The star is named for American </span><a href="http://en.wikipedia.org/wiki/Astronomer" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Astronomer">astronomer</a><span style="line-height: 19.1875px; text-align: start;"> </span><a href="http://en.wikipedia.org/wiki/Edward_Emerson_Barnard" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Edward Emerson Barnard">E.E. Barnard</a><span style="line-height: 19.1875px; text-align: start;">. He was not the first to observe the star (it appeared on Harvard College University plates in 1888 and 1890), but in 1916 he measured its </span><a href="http://en.wikipedia.org/wiki/Proper_motion" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Proper motion">proper motion</a><span style="line-height: 19.1875px; text-align: start;"> as 10.3 </span><a href="http://en.wikipedia.org/wiki/Minute_of_arc" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Minute of arc">arcseconds</a><span style="line-height: 19.1875px; text-align: start;"> (20,000 inverse </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Radians" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Radians">radians</a><span style="line-height: 19.1875px; text-align: start;">) per year, which remains the largest-known proper motion of any star relative to the </span><a href="http://en.wikipedia.org/wiki/Solar_System" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Solar System">Solar System</a><span style="line-height: 19.1875px; text-align: start;">.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgvtymjodJKaj4B2YcSQaUUuSpxp7xDyPyvGFTa2FPrNkHnBeVtqxlAsAgQQMAD61W5dyakGKfAgDxgKiqMT1LuJihKha905Edn220whkMlMJtBTWHrHSc9kkbGpW68skz4hrfpYhkRNkpP/s1600/estrelas-mais-proximas-da-terra_kwnh4r.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span><br />
<a href="http://astronomy-universo.blogspot.com.br/2013/11/conheca-as-10-estrelas-mais-proximas-da.html?spref=fb" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://astronomy-universo.blogspot.com.br/2013/11/conheca-as-10-estrelas-mais-proximas-da.html?spref=fb</span></a><br />
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<strong><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Estrela de Barnard</span></strong></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Distância: 5,96 anos-luz</strong> </span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjbN-89Ua7PDQcjm8s16A3x5AV4UjyhqqHfNQkDSsgvMvZlmpXeC4fJXMDO-InXn4hvrTK6mCoEykCN3z89wECeZRmzBL2SKa90Ix9x912AGukuBn-2Uz5lM2zTJU03kT9hOk2cQIuEhFca/s1600/estrela+de+barnard.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjbN-89Ua7PDQcjm8s16A3x5AV4UjyhqqHfNQkDSsgvMvZlmpXeC4fJXMDO-InXn4hvrTK6mCoEykCN3z89wECeZRmzBL2SKa90Ix9x912AGukuBn-2Uz5lM2zTJU03kT9hOk2cQIuEhFca/s640/estrela+de+barnard.jpg" height="326" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(102, 0, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta é uma anã vermelha ténue que fica a cerca de 5,96 anos-luz da Terra. No passado os cientistas acreditavam que a <strong>estrela de Barnard</strong> podia conter planetas ao seu redor, mas as tentativas de detectar tais objetos não resultaram em nenhuma observação. A estrela de Barnard fica situada se na constelação Ophiuchus.</span></div>
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<a href="http://astronomy-universo.blogspot.com.br/2013/11/conheca-as-10-estrelas-mais-proximas-da.html?spref=fb" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://astronomy-universo.blogspot.com.br/2013/11/conheca-as-10-estrelas-mais-proximas-da.html?spref=fb</span></a></div>
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<strong style="text-align: justify;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Fonte: ciencia-online.net</span></strong></div>
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<table class="infobox" style="border: 1px solid rgb(170, 170, 170); clear: right; line-height: 1.5em; margin: 0.5em 0px 0.5em 1em; padding: 0.2em; text-align: center; width: 22em;"><caption style="font-weight: bold;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Barnard's Star</span></caption><tbody>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="image" href="http://en.wikipedia.org/wiki/File:Barnardstar2006.jpg" style="background-image: none; text-decoration: none;"><img alt="Barnardstar2006.jpg" src="http://upload.wikimedia.org/wikipedia/commons/thumb/1/18/Barnardstar2006.jpg/250px-Barnardstar2006.jpg" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/18/Barnardstar2006.jpg/375px-Barnardstar2006.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/1/18/Barnardstar2006.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" /></a><br />The location of Barnard's Star</span></div>
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<tr><th colspan="2" style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Observation data<br /><small><a href="http://en.wikipedia.org/wiki/Epoch_(astronomy)" style="background-image: none; text-decoration: none;" title="Epoch (astronomy)">Epoch</a> <a class="mw-redirect" href="http://en.wikipedia.org/wiki/J2000.0" style="background-image: none; text-decoration: none;" title="J2000.0">J2000.0</a> <a href="http://en.wikipedia.org/wiki/Equinox_(celestial_coordinates)" style="background-image: none; text-decoration: none;" title="Equinox (celestial coordinates)">Equinox</a> <a class="mw-redirect" href="http://en.wikipedia.org/wiki/J2000.0" style="background-image: none; text-decoration: none;" title="J2000.0">J2000.0</a></small></span></th></tr>
<tr><td style="vertical-align: top;"><b><a href="http://en.wikipedia.org/wiki/Constellation" style="background-image: none; text-decoration: none;" title="Constellation"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constellation</span></a></b></td><td style="vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Ophiuchus" style="background-image: none; text-decoration: none;" title="Ophiuchus"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ophiuchus</span></a></td></tr>
<tr valign="top"><td style="vertical-align: top;"><b><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Wikipedia:IPA_for_English" style="background-image: none; text-decoration: none;" title="Wikipedia:IPA for English"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Pronunciation</span></a></b></td><td style="vertical-align: top;"><span class="nowrap" style="white-space: nowrap;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="IPA" title="Representation in the International Phonetic Alphabet (IPA)"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English" style="background-image: none; text-decoration: none !important;" title="Help:IPA for English">/</a></span><span class="IPA nopopups"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English#Key" style="background-image: none; text-decoration: none !important;" title="Help:IPA for English"><span style="border-bottom-style: dotted; border-bottom-width: 1px;" title="/ˈ/ primary stress follows">ˈ</span></a></span><span class="IPA nopopups"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English#Key" style="background-image: none; text-decoration: none !important;" title="Help:IPA for English"><span style="border-bottom-style: dotted; border-bottom-width: 1px;" title="'b' in 'buy'">b</span></a></span><span class="IPA nopopups"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English#Key" style="background-image: none; text-decoration: none !important;" title="Help:IPA for English"><span style="border-bottom-style: dotted; border-bottom-width: 1px;" title="/ɑr/ 'ar' in 'bard'">ɑr</span></a></span><span class="IPA nopopups"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English#Key" style="background-image: none; text-decoration: none !important;" title="Help:IPA for English"><span style="border-bottom-style: dotted; border-bottom-width: 1px;" title="'n' in 'nigh'">n</span></a></span><span class="IPA nopopups"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English#Key" style="background-image: none; text-decoration: none !important;" title="Help:IPA for English"><span style="border-bottom-style: dotted; border-bottom-width: 1px;" title="/ər/ 'er' in 'finger'">ər</span></a></span><span class="IPA nopopups"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English#Key" style="background-image: none; text-decoration: none !important;" title="Help:IPA for English"><span style="border-bottom-style: dotted; border-bottom-width: 1px;" title="'d' in 'dye'">d</span></a></span><span class="IPA" title="Representation in the International Phonetic Alphabet (IPA)"><a href="http://en.wikipedia.org/wiki/Help:IPA_for_English" style="background-image: none; text-decoration: none !important;" title="Help:IPA for English">/</a></span></span></span></td></tr>
<tr><td style="vertical-align: top;"><b><a href="http://en.wikipedia.org/wiki/Right_ascension" style="background-image: none; text-decoration: none;" title="Right ascension"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Right ascension</span></a></b></td><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">17<sup style="line-height: 1em;">h</sup> 57<sup style="line-height: 1em;">m</sup> 48.49803<sup style="line-height: 1em;">s</sup><sup class="reference" id="cite_ref-simbad_1-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Barnard's_Star#cite_note-simbad-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></td></tr>
<tr><td style="vertical-align: top;"><b><a href="http://en.wikipedia.org/wiki/Declination" style="background-image: none; text-decoration: none;" title="Declination"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Declination</span></a></b></td><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">+04° 41′ 36.2072″<sup class="reference" id="cite_ref-simbad_1-1" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Barnard's_Star#cite_note-simbad-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></td></tr>
<tr valign="top"><td style="vertical-align: top;"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Apparent_magnitude" style="background-image: none; text-decoration: none;" title="Apparent magnitude">Apparent magnitude</a> <small>(V)</small></span></b></td><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">9.54<sup class="reference" id="cite_ref-simbad_1-2" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Barnard's_Star#cite_note-simbad-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></td></tr>
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<a href="http://en.wikipedia.org/wiki/Barnard's_Star" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://en.wikipedia.org/wiki/Barnard's_Star</span></a><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual integral 7,6 Tipo A7<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">Messier 9</b><span style="line-height: 19.1875px; text-align: start;"> (</span><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="New General Catalogue">NGC 6333</a><span style="line-height: 19.1875px; text-align: start;">) é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="line-height: 19.1875px; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Estrela">estrelas</a><span style="line-height: 19.1875px; text-align: start;"> na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="line-height: 19.1875px; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Ophiuchus">Ofiúco</a><span style="line-height: 19.1875px; text-align: start;">. Foi descoberto pelo francês </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="line-height: 19.1875px; text-align: start;"> em 1764 e é um dos aglomerados globulares próximos ao centro da </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Via-Láctea">Via-Láctea</a><span style="line-height: 19.1875px; text-align: start;">, a uma distância de 5 500 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="line-height: 19.1875px; text-align: start;">. Está a uma distância de cerca de 25 800 anos-luz em relação à </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="line-height: 19.1875px; text-align: start;">.</span></span></div>
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<table cellpadding="0" cellspacing="2" class="infobox" style="border-collapse: collapse; border: 1px solid rgb(170, 170, 170); clear: right; line-height: 19.1875px; margin: 0px 0px 1em 1em; padding: 0.2em; text-align: center; width: 250px;"><tbody>
<tr style="vertical-align: top;"><td colspan="2"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Messier 9</span></b></td></tr>
<tr style="vertical-align: top;"><td colspan="2"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_9_Hubble_WikiSky_wfpc2_patched.jpg" style="background-image: none; text-decoration: none;" title="Messier 9 visto pelo Telescópio Espacial Hubble."><img alt="Messier 9 visto pelo Telescópio Espacial Hubble." src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/0e/Messier_9_Hubble_WikiSky_wfpc2_patched.jpg/250px-Messier_9_Hubble_WikiSky_wfpc2_patched.jpg" height="640" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/0e/Messier_9_Hubble_WikiSky_wfpc2_patched.jpg/375px-Messier_9_Hubble_WikiSky_wfpc2_patched.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/0e/Messier_9_Hubble_WikiSky_wfpc2_patched.jpg/500px-Messier_9_Hubble_WikiSky_wfpc2_patched.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="640" /></a><br />Messier 9 visto pelo Telescópio Espacial Hubble.</span></td></tr>
<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Descoberto por</span></td><td><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-image: none; text-decoration: none;" title="Charles Messier"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Charles Messier</span></a></td></tr>
<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Data</span></td><td><a href="http://pt.wikipedia.org/wiki/1764" style="background-image: none; text-decoration: none;" title="1764"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1764</span></a></td></tr>
<tr style="vertical-align: top;"><td colspan="2"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dados observacionais (J2000)</span></b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelação</span></a></td><td><a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background-image: none; text-decoration: none;" title="Ophiuchus"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ophiuchus</span></a></td></tr>
<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">VII</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-image: none; text-decoration: none;" title="Ascensão reta"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Asc. reta</span></a></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">17<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 19<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 11,78<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_9#cite_note-simbad-1" style="background-image: none; text-decoration: none;">1</a></span></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Declinação"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Declinação</span></a></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18° 30′ 58,5″<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_9#cite_note-simbad-1" style="background-image: none; text-decoration: none;">1</a></span></span></td></tr>
<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distância</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">25 800 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-image: none; text-decoration: none;" title="Ano-luz">anos-luz</a> (7,9 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-image: none; text-decoration: none;" title="Parsec">kpc</a>)</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; text-decoration: none;" title="Magnitude aparente"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnit. apar.</span></a></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">8,42<span class="reference" id="cite_ref-simbad_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_9#cite_note-simbad-1" style="background-image: none; text-decoration: none;">1</a></span></span></td></tr>
<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dimensões</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">12',0</span></td></tr>
<tr style="vertical-align: top;"><td colspan="2"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Características físicas</span></b></td></tr>
<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Raio</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">45 anos-luz</span></td></tr>
<tr style="vertical-align: top;"><td colspan="2"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Outras denominações</span></b></td></tr>
<tr style="vertical-align: top;"><td colspan="2"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-image: none; text-decoration: none;" title="New General Catalogue">NGC</a> 6333</span></td></tr>
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<a href="http://pt.wikipedia.org/wiki/Messier_9" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Messier_9</span></a><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M 14 - NGC 6402 - Ophiucus - Aglomerado Estelar Globular</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h36m Declinação -03<sup>o</sup>.14<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual integral 7,8 Tipo AG<o:p></o:p></span></div>
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<table cellpadding="0" cellspacing="2" class="infobox" style="border-collapse: collapse; border: 1px solid rgb(170, 170, 170); clear: right; line-height: 19.1875px; margin: 0px 0px 1em 1em; padding: 0.2em; text-align: center; width: 250px;"><tbody>
<tr style="vertical-align: top;"><td colspan="2"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Messier 14</span></b></td></tr>
<tr style="vertical-align: top;"><td colspan="2"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:M14HunterWilson.jpg" style="background-image: none; text-decoration: none;" title="Messier 14 por um telescópio amador"><img alt="Messier 14 por um telescópio amador" src="http://upload.wikimedia.org/wikipedia/commons/thumb/3/30/M14HunterWilson.jpg/250px-M14HunterWilson.jpg" height="527" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/3/30/M14HunterWilson.jpg/375px-M14HunterWilson.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/3/30/M14HunterWilson.jpg/500px-M14HunterWilson.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="640" /></a><br />Messier 14 por um telescópio amador</span></td></tr>
<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Descoberto por</span></td><td><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-image: none; text-decoration: none;" title="Charles Messier"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Charles Messier</span></a></td></tr>
<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Data</span></td><td><a href="http://pt.wikipedia.org/wiki/1764" style="background-image: none; text-decoration: none;" title="1764"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1764</span></a></td></tr>
<tr style="vertical-align: top;"><td colspan="2"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dados observacionais (J2000)</span></b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelação</span></a></td><td><a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background-image: none; text-decoration: none;" title="Ophiuchus"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ophiuchus</span></a></td></tr>
<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">VIII</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-image: none; text-decoration: none;" title="Ascensão reta"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Asc. reta</span></a></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">17<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 37<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 36,15<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_14#cite_note-simbad-1" style="background-image: none; text-decoration: none;">1</a></span></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Declinação"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Declinação</span></a></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-03° 14′ 45,3″<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_14#cite_note-simbad-1" style="background-image: none; text-decoration: none;">1</a></span></span></td></tr>
<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distância</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">30 300 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-image: none; text-decoration: none;" title="Ano-luz">anos-luz</a> (9,3 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-image: none; text-decoration: none;" title="Parsec">kpc</a>)</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; text-decoration: none;" title="Magnitude aparente"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnit. apar.</span></a></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">8,32<span class="reference" id="cite_ref-simbad_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_14#cite_note-simbad-1" style="background-image: none; text-decoration: none;">1</a></span></span></td></tr>
<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dimensões</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">11',0</span></td></tr>
<tr style="vertical-align: top;"><td colspan="2"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Características físicas</span></b></td></tr>
<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Raio</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">50 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; text-decoration: none;" title="Anos-luz">anos-luz</a></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Outras denominações</span></b></td></tr>
<tr style="vertical-align: top;"><td colspan="2"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-image: none; text-decoration: none;" title="New General Catalogue">NGC</a> 6402</span></td></tr>
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<a href="http://pt.wikipedia.org/wiki/Messier_14" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Messier_14</span></a><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M 10 - NGC 6254 - Ophiucus - Aglomerado Estelar Globular</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 16h56 Declinação -04<sup>o</sup>.05<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual integral 6,5 Tipo AG</span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Na parte ao sul do Ophiúco existem, entre partes adoráveis da Via Láctea, Nuvens de Estrelas e Nebulosas Escuras. Próximo à estrela Alya, Theta Serpentis, é possível se observar a olho nú uma imensa nuvem escura no formato de um Cachimbo, é a Nebulosa do Cachimbo. Quando observamos esta região e sua vizinhança fazendo parte da Via Láctea em Sagitário, estamos olhando em direção ao centro de nossa Galáxia.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 16h56m Declinação -04<sup>o</sup>.05<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 7,3 Diâmetro aparente 16’,2 Tipo Espectral G1<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude média das 25 mais brilhantes estrelas (excluindo as 5 mais brilhantes) 14,17<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Número conhecido de Variáveis 3 Distância kpc 6,2<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Velocidade Radial (km/s) + 71<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;">M 12 - NGC 6218 - Ophiucus - Aglomerado Estelar Globular</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual integral 6,7 Tipo AG</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 16h46m Declinação -01<sup>o</sup> 55<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 7,6 Diâmetro aparente 21’,5 Tipo Espectral F8<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude média das 25 mais brilhantes estrelas (excluindo as 5 mais brilhantes) 14,07<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Velocidade Radial (km/s) -16<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b> I 4665 - Aglomerado Aberto Ophiucus</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h45m Declinação +5<sup>o</sup>.44<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 5,4 Magnitude fotográfica da mais brilhante estrela 8,3<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Distância kpc 0,33 Diâmetro 50’ Tipo Espectral B8<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M107</b><o:p></o:p></span><br />
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<tr><td><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEifJKYzqV4dYKBKODCo-5THLrVLL211hsB0Pqs7p1kKLeQzqi-P-sIAkA3944lzmjb1dLXo0fVzIGRy-OHnqZc9NX0gSChbV4Q4SbMprIoVvwZN6_ggt_6YPqHUGyJHiOZqKkBz0wKliFCt/s1600/600px-Messier_107_Hubble_WikiSky.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEifJKYzqV4dYKBKODCo-5THLrVLL211hsB0Pqs7p1kKLeQzqi-P-sIAkA3944lzmjb1dLXo0fVzIGRy-OHnqZc9NX0gSChbV4Q4SbMprIoVvwZN6_ggt_6YPqHUGyJHiOZqKkBz0wKliFCt/s1600/600px-Messier_107_Hubble_WikiSky.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></td></tr>
<tr><td class="tr-caption"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 17px;"><a href="http://en.wikipedia.org/wiki/NASA" style="text-decoration: none;" title="en:NASA"><span lang="EN-US" style="line-height: 13px;">en:NASA</span></a></span><span lang="EN-US" style="line-height: 13px;">,</span><span lang="EN-US" style="line-height: 13px;"> </span><span style="line-height: 13px;"><a href="http://en.wikipedia.org/wiki/STScI" style="text-decoration: none;" title="en:STScI"><span lang="EN-US">en:STScI</span></a></span><span lang="EN-US" style="line-height: 13px;">,</span><span lang="EN-US" style="line-height: 13px;"> </span><span style="line-height: 13px;"><span lang="EN-US"><a href="http://en.wikipedia.org/wiki/WikiSky" style="text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span></span></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Messier_107" style="text-decoration: none;">http://pt.wikipedia.org/wiki/Messier_107</a> </span><br />
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<tr><td><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjube5Ho15pxxi99ROTg6mCQTnKaFFI-9gbvjLi-2qx-0FtXH-Dp1Ksfg5PUA9IcFTp-FLqCJp8uTqky1km4xYuFN5P-yN8D9w3A9AiYVaOSJzUS9Te0A-jEMC4MrxIP4_Aj2eDJeRznzhb/s1600/eso1048a+m107.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjube5Ho15pxxi99ROTg6mCQTnKaFFI-9gbvjLi-2qx-0FtXH-Dp1Ksfg5PUA9IcFTp-FLqCJp8uTqky1km4xYuFN5P-yN8D9w3A9AiYVaOSJzUS9Te0A-jEMC4MrxIP4_Aj2eDJeRznzhb/s640/eso1048a+m107.jpg" height="584" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></td></tr>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">The globular cluster Messier 107, also known as NGC 6171, is located about 21 000 light-years away in the constellation of Ophiuchus. Messier 107 is about 13 arcminutes across, which corresponds to about 80 light-years at its distance. As is typical of globular clusters, a population of thousands of old stars in Messier 107 is densely concentrated into a volume that is only about twenty times the distance between our Sun and its nearest stellar neighbour, Alpha Centauri, across. This image was created from exposures taken through blue, green and near-infrared filters, using the Wide Field Imager (WFI) on the MPG/ESO 2.2-metre telescope at La Silla Observatory, Chile.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><strong><span lang="EN-US">Credit:</span></strong><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">ESO/ESO Imaging Survey<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M62</b><o:p></o:p></span></div>
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<tr><td><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjqvYQ8UWY4Vmk9-rEx99O4xNxoi8BVxT3gSGo9dPmvj9op2qRGgbrolZaKZfZ-XdxVtiztsZDhXZnmDcw-H512kOvJaNK5cnBESZIDMpaXAA9avs-23LywgfTMzESNBwalyoc7t8PxA8Uv/s1600/M62_3.6_5.8_8.0_microns_spitzer.png" imageanchor="1" style="margin-left: auto; margin-right: auto; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjqvYQ8UWY4Vmk9-rEx99O4xNxoi8BVxT3gSGo9dPmvj9op2qRGgbrolZaKZfZ-XdxVtiztsZDhXZnmDcw-H512kOvJaNK5cnBESZIDMpaXAA9avs-23LywgfTMzESNBwalyoc7t8PxA8Uv/s640/M62_3.6_5.8_8.0_microns_spitzer.png" height="625" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></td></tr>
<tr><td class="tr-caption"><span style="line-height: 19.1875px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Image of the M62 star cluster in infrared at 3.6 (blue), 4.5 (green) and 8.0 µm. The image has been made by myself (Médéric Boquien) from the public image archive of the Spitzer Space Telescope (courtesy NASA/JPL-Caltech).</span></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">O <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-image: none; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> foi descoberto pelo astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-image: none; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 7 de junho de 1771, embora ele tenha tomado sua posição na <a href="http://pt.wikipedia.org/wiki/Esfera_celeste" style="background-image: none; text-decoration: none;" title="Esfera celeste">esfera celeste</a> apenas em 4 de junho de 1779, quando listou em seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-image: none; text-decoration: none;" title="Catálogo Messier">catálogo</a>. <a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-image: none; text-decoration: none;" title="William Herschel">William Herschel</a>, descobridor de <a href="http://pt.wikipedia.org/wiki/Urano_(planeta)" style="background-image: none; text-decoration: none;" title="Urano (planeta)">Urano</a>, foi o primeiro a resolver suas estrelas mais brilhantes.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">É um dos <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-image: none; text-decoration: none;" title="Aglomerado globular">aglomerados globulares</a> mais irregulares que se conhece. Sua deformação, relatada primeiramente por Herschel, é o resultado das <a href="http://pt.wikipedia.org/wiki/For%C3%A7a_de_mar%C3%A9" style="background-image: none; text-decoration: none;" title="Força de maré">forças de maré</a> do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea#N.C3.BAcleo" style="background-image: none; text-decoration: none;" title="Via-Láctea">núcleo da Via-Láctea</a>; o aglomerado está apenas 6 100 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; text-decoration: none;" title="Anos-luz">anos-luz</a> do centro galáctico, um dos aglomerados globulares do <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-image: none; text-decoration: none;" title="Catálogo Messier">catálogo Messier</a>mais próximos da região central da Via-Láctea.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Está a uma distância de 22 500 anos-luz em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background-image: none; text-decoration: none;" title="Terra">Terra</a>, e seu diâmetro aparente de 15 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-image: none; text-decoration: none;" title="Minuto de arco">minutos de grau</a>, metade do diâmetro aparente da <a href="http://pt.wikipedia.org/wiki/Fases_da_Lua" style="background-image: none; text-decoration: none;" title="Fases da Lua">Lua Cheia</a>, corresponde a um diâmetro real de 100 anos-luz.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Contém 89 <a href="http://pt.wikipedia.org/wiki/Estrela_vari%C3%A1vel" style="background-image: none; text-decoration: none;" title="Estrela variável">estrelas variáveis</a> conhecidas, a maior parte variáveis <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/RR_Lyrae" style="background-image: none; text-decoration: none;" title="RR Lyrae">RR Lyrae</a>. Seu núcleo é extremamente denso;possívelmente o núcleo sofreu no passado um colapso de núcleo, de modo semelhante ao encontrado nos aglomerados <a href="http://pt.wikipedia.org/wiki/Messier_15" style="background-image: none; text-decoration: none;" title="Messier 15">Messier 15</a>, <a href="http://pt.wikipedia.org/wiki/Messier_30" style="background-image: none; text-decoration: none;" title="Messier 30">Messier 30</a> e <a href="http://pt.wikipedia.org/wiki/Messier_70" style="background-image: none; text-decoration: none;" title="Messier 70">Messier 70</a>. Contém vários <a href="http://pt.wikipedia.org/wiki/Bin%C3%A1rio_de_raio_X" style="background-image: none; text-decoration: none;" title="Binário de raio X">binários de raios X</a>, consequência da alta <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Densidade_estelar&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="Densidade estelar (página não existe)">densidade estelar</a> de seu núcleo; tais binários de raios-X são consequência de quase-colisões entre estrelas</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Messier_62" style="text-decoration: none;"><span style="background-color: white; color: #073763;">http://pt.wikipedia.org/wiki/Messier_62</span></a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 6273 - M 19 - Aglomerado Globular Ophiucus</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h01m Declinação -26<sup>o</sup>.14<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 8,3 Diâmetro aparente 5’,3 Tipo Espectral F2<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distância kpc 6,9 Velocidade Radial (km/s) + 102</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h10m Declinação -26<sup>o</sup>.14<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual integral 6,9 Tipo AG<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /><span style="line-height: 18px;"><br /></span></span><a href="http://pt.wikipedia.org/wiki/Messier_19" style="text-decoration: none;"><span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Messier_19</span></a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Messier 19</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-image: none; text-decoration: none;" title="New General Catalogue">NGC 6273</a>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-image: none; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-image: none; text-decoration: none;" title="Estrela">estrelas</a> localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background-image: none; text-decoration: none;" title="Ophiuchus">Ofiúco</a>. Foi descoberto pelo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-image: none; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 1764, que o adicionou ao seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-image: none; text-decoration: none;" title="Catálogo Messier">catálogo de objetos</a> de aparência semelhante a <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-image: none; text-decoration: none;" title="Cometa">cometas</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Messier 19 é o mais oblato dos aglomerados globulares conhecidos. Está a uma distância de cerca de 28 000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; text-decoration: none;" title="Anos-luz">anos-luz</a> do <a href="http://pt.wikipedia.org/wiki/Sistema_Solar" style="background-image: none; text-decoration: none;" title="Sistema Solar">Sistema Solar</a>, e está bastante próximo ao Centro Galáctico, com apenas cerca de 5.200 anos-luz de distância.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É um dos aglomerados globulares mais <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Esferoide_oblato" style="background-image: none; text-decoration: none;" title="Esferoide oblato">oblatos</a> (achatados) conhecidos. Essa deformidade pode estar relacionado à proximidade do aglomerado ao <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea#N.C3.BAcleo" style="background-image: none; text-decoration: none;" title="Via-Láctea">centro galáctico</a>: embora esteja a cerca de 28 000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; text-decoration: none;" title="Anos-luz">anos-luz</a>da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-image: none; text-decoration: none;" title="Terra">Terra</a>, está apenas a 5 200 do núcleo da Via-Láctea, ou cerca de 9° acima do núcleo galáctico na<a href="http://pt.wikipedia.org/wiki/Esfera_celeste" style="background-image: none; text-decoration: none;" title="Esfera celeste">esfera celeste</a>. Afasta-se radialmente do <a href="http://pt.wikipedia.org/wiki/Sistema_Solar" style="background-image: none; text-decoration: none;" title="Sistema Solar">Sistema Solar</a> a uma velocidade aproximada de 146 km/s.<span class="reference" id="cite_ref-seds_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_19#cite_note-seds-2" style="background-image: none; text-decoration: none;">2</a></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Ficheiro:M19HunterWilson.jpg" src="http://upload.wikimedia.org/wikipedia/commons/thumb/3/38/M19HunterWilson.jpg/600px-M19HunterWilson.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
<table cellpadding="4" class="toccolours vevent mw-content-ltr" style="border: 1px solid rgb(170, 170, 170); direction: ltr; line-height: 19.1875px; padding: 5px; text-align: center; width: 1112px;"><tbody>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 156.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Autor</span></td><td><a href="http://commons.wikimedia.org/wiki/User:Hewholooks" style="background-image: none; text-decoration: none;" title="User:Hewholooks"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Hewholooks</span></a><br />
<h1 class="firstHeading" id="firstHeading" lang="pt" style="background-image: none; border-bottom-color: rgb(170, 170, 170); border-bottom-style: solid; border-bottom-width: 1px; font-weight: normal; line-height: 1.2em; margin: 0px 0px 0.1em; overflow: hidden; padding-bottom: 0px; padding-top: 0px; position: relative;">
<span dir="auto"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">M19HunterWilson.</span></span></h1>
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<span style="background-color: white; color: #073763;"><a href="http://pt.wikipedia.org/wiki/Messier_19" style="text-decoration: none;"><span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Messier_19</span></a><span style="font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18px;"><br /></span></span><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_6572" style="text-decoration: none;">http://pt.wikipedia.org/wiki/NGC_6572</a><span style="line-height: 18px;"><br /></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; line-height: 18px;"><b style="line-height: 19.1875px; text-align: start;">NGC 6572</b><span style="line-height: 19.1875px; text-align: start;"> é uma </span><a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Nebulosa planetária">nebulosa planetária</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Ophiuchus">constelação de Ophiuchus</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Wilhelm_Struve" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Wilhelm Struve">Wilhelm Struve</a><span style="line-height: 19.1875px; text-align: start;"> em 1825, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="line-height: 19.1875px; text-align: start;"> refrator com abertura de 9,5 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;"> (+8,1), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="line-height: 19.1875px; text-align: start;">amadores ou com equipamentos superiores.</span></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 1.4;"><a href="http://pt.wikipedia.org/wiki/NGC_6572" style="background-color: white; text-decoration: none;">http://pt.wikipedia.org/wiki/NGC_6572</a></span><br />
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<h1 style="border: 0px; line-height: 28px; margin: 0px 0px 13px; outline: 0px; padding: 0px; position: relative; vertical-align: baseline;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">A dazzling planetary nebula</span></h1>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://www.spacetelescope.org/static/archives/images/screen/potw1034a.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /><br /><a href="http://www.spacetelescope.org/images/potw1034a/" style="text-decoration: none;">http://www.spacetelescope.org/images/potw1034a/</a></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong style="border: 0px; margin: 0px 0px 15px; outline: 0px; padding: 0px; vertical-align: baseline;">Credit: </strong>ESA/Hubble & NASA</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 15px; text-align: start;">This picture of NGC 6572 shows the intricate shapes that can develop as stars exhale their last breaths. Hubble has even imaged the central white dwarf star, the origin of the dazzling nebula, but now a faint, but hot, vestige of its former glory</span><span style="line-height: 15px; text-align: start;">.</span></span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_6304" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_6304</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 6304</b><span style="line-height: 19.1875px; text-align: start;"> é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Ophiuchus">constelação de Ophiuchus</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="William Herschel">William Herschel</a><span style="line-height: 19.1875px; text-align: start;"> em 1786, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="line-height: 19.1875px; text-align: start;"> refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;"> (+8,3), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="line-height: 19.1875px; text-align: start;">amadores ou com equipamentos superiores.</span></span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_6304" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_6304</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 6293</b><span style="line-height: 19.1875px; text-align: start;"> é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Ophiuchus">constelação de Ophiuchus</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="William Herschel">William Herschel</a><span style="line-height: 19.1875px; text-align: start;"> em 1784, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="line-height: 19.1875px; text-align: start;"> refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;"> (+8,3), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="line-height: 19.1875px; text-align: start;">amadores ou com equipamentos superiores.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Ficheiro:NGC 6293 Hubble WikiSky.jpg" src="http://upload.wikimedia.org/wikipedia/commons/thumb/b/b9/NGC_6293_Hubble_WikiSky.jpg/600px-NGC_6293_Hubble_WikiSky.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_6293" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_6293</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="en:NASA">en:NASA</a><span style="line-height: 19.1875px; text-align: start;">, </span><a class="extiw" href="http://en.wikipedia.org/wiki/STScI" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="en:STScI">en:STScI</a><span style="line-height: 19.1875px; text-align: start;">, </span><a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_6355" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_6355</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 6355</b><span style="line-height: 19.1875px; text-align: start;"> é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Ophiuchus">constelação de Ophiuchus</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="William Herschel">William Herschel</a><span style="line-height: 19.1875px; text-align: start;"> em 1784, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="line-height: 19.1875px; text-align: start;"> refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;"> (+8,6), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="line-height: 19.1875px; text-align: start;">amadores ou com equipamentos superiores</span></span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_6342" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_6342</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 6342</b><span style="line-height: 19.1875px; text-align: start;"> é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Ophiuchus">constelação de Ophiuchus</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="William Herschel">William Herschel</a><span style="line-height: 19.1875px; text-align: start;"> em 1786, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="line-height: 19.1875px; text-align: start;"> refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;"> (+9,5), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="line-height: 19.1875px; text-align: start;">amadores ou com equipamentos superiores.</span></span></div>
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<a href="http://en.wikipedia.org/wiki/IC_4665" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://en.wikipedia.org/wiki/IC_4665</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">IC 4665</b><span style="line-height: 19.1875px; text-align: start;"> is an </span><a href="http://en.wikipedia.org/wiki/Open_cluster" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Open cluster">open cluster</a><span style="line-height: 19.1875px; text-align: start;"> in the </span><a href="http://en.wikipedia.org/wiki/Constellation" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Constellation">constellation</a><span style="line-height: 19.1875px; text-align: start;"> </span><a href="http://en.wikipedia.org/wiki/Ophiuchus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Ophiuchus">Ophiuchus</a><span style="line-height: 19.1875px; text-align: start;">. It was discovered by </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Philippe_Loys_de_Ch%C3%A9seaux" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Philippe Loys de Chéseaux">Philippe Loys de Chéseaux</a><span style="line-height: 19.1875px; text-align: start;"> in 1745. The cluster began to develop less than 40 million years ago, and lies about 1,400 </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Light_year" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Light year">light years</a><span style="line-height: 19.1875px; text-align: start;"> away from </span><a href="http://en.wikipedia.org/wiki/Earth" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Earth">Earth</a><span style="line-height: 19.1875px; text-align: start;">. It is easily visible in the smallest of </span><a href="http://en.wikipedia.org/wiki/Telescope" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescope">telescopes</a><span style="line-height: 19.1875px; text-align: start;"> and also with </span><a href="http://en.wikipedia.org/wiki/Binoculars" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Binoculars">binoculars</a><span style="line-height: 19.1875px; text-align: start;">. From a sufficiently dark place it is also visible to the </span><a href="http://en.wikipedia.org/wiki/Naked_eye" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Naked eye">naked eye</a><span style="line-height: 19.1875px; text-align: start;">.</span></span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_6633" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_6633</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 6633</b><span style="line-height: 19.1875px; text-align: start;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Ophiuchus">constelação de Ophiuchus</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Philippe_de_Cheseaux" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Philippe de Cheseaux">Philippe de Cheseaux</a><span style="line-height: 19.1875px; text-align: start;"> em 1745, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="line-height: 19.1875px; text-align: start;"> refrator com abertura de 0 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;"> (+4,6), é visível a </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Olho_nu" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Olho nu">olho nu</a><span style="line-height: 19.1875px; text-align: start;">, porém em regiões distantes de cidades</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://astrobob.areavoices.com/astrobob/images/NWA_6633_DSS2_Wikisky.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<span style="line-height: 24px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The smallest of the four featured star clusters, NGC 6633. Credit: DSS2 Survey/Wikisky - See more at: http://astrobob.areavoices.com/2009/07/16/steeped-in-summer-star-clusters/#sthash.gwKe4wBl.dpuf</span></span></div>
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<a href="http://astrobob.areavoices.com/2009/07/16/steeped-in-summer-star-clusters/" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://astrobob.areavoices.com/2009/07/16/steeped-in-summer-star-clusters/</span></a></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_6235" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_6235</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 6235</b><span style="line-height: 19.1875px; text-align: start;"> é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Ophiuchus">constelação de Ophiuchus</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="William Herschel">William Herschel</a><span style="line-height: 19.1875px; text-align: start;"> em 1786, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="line-height: 19.1875px; text-align: start;"> refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;"> (+8,9), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="line-height: 19.1875px; text-align: start;">amadores ou com equipamentos superiores.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://gclusters.altervista.org/ima/dss_ngc6235.gif" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><i><span style="font-family: Arial, Helvetica, sans-serif;">Image of the cluster from the <a href="http://en.wikipedia.org/wiki/Digitized_Sky_Survey" style="text-decoration: none;">Digital Sky Survey</a></span></i></span><br />
<a href="http://gclusters.altervista.org/cluster_4.php?ggc=NGC+6235" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://gclusters.altervista.org/cluster_4.php?ggc=NGC+6235</span></a><br />
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><a href="http://pt.wikipedia.org/wiki/NGC_6284" style="text-decoration: none;"><span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_6284</span></a></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 6284</b><span style="line-height: 19.1875px; text-align: start;"> é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Ophiuchus">constelação de Ophiuchus</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="William Herschel">William Herschel</a><span style="line-height: 19.1875px; text-align: start;"> em 1784, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="line-height: 19.1875px; text-align: start;"> refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;"> (+8,9), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="line-height: 19.1875px; text-align: start;">amadores ou com equipamentos superiores.</span></span></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://rti.lcogt.net/observations/2005/06/04/process-8216-1.jpg" height="637" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="640" /></span><br />
<a href="http://lcogt.net/observations/ogg/2m0a/7023" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://lcogt.net/observations/ogg/2m0a/7023</span></a><br />
<table class="avm" style="border-collapse: collapse; border: 0px !important; margin: 0px !important; text-align: center;"><tbody style="border-top-style: none;">
<tr><td class="first" style="border-collapse: separate; border: 0px !important; font-weight: bold; line-height: 24px; padding: 0px; text-align: right; vertical-align: top; width: 80px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Credit:</span></td><td style="border-collapse: separate; border: 0px !important; line-height: 24px; padding: 0px 8px; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Provided to Las Cumbres Observatory under license from the Dill Faulkes Educational Trust</span></td></tr>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-color: white; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; color: #073763; line-height: 18px;"><img alt="The Night Sky Atlas logo image" src="http://www.nightskyatlas.com/logo.gif" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;"><br />ENCONTRE MAIORES INFORMAÇÕES SOBRE OPHIUCUS</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">acessando </span></div>
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<h1 style="line-height: 1.4; margin: 0px; position: relative;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">The Night Sky Atlas</span></h1>
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<a href="http://www.nightskyatlas.com/index.jsp?rightAscension=17.3&declination=-5.0" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.nightskyatlas.com/index.jsp?rightAscension=17.3&declination=-5.0</span></a></div>
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<b><span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Named Stars Index - The Night Sky Atlas<o:p></o:p></span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/starnames.jsp" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/starnames.jsp</span></a><b><span lang="EN-US"><o:p></o:p></span></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Star <span class="SpellE">Name</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Bayer<br /><span class="SpellE">Designation</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE">Description</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE">Offsite</span> Links<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE"><span lang="EN-US">Ophiucus</span></span><span lang="EN-US">: Visible in February before dawn, to October after dusk, best in June.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=17.725&declination=4.567&viewAngle=25" style="text-decoration: none;"><span class="SpellE">Cheleb</span> <span class="SpellE">or</span> <span class="SpellE">Celbalrai</span></a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">β<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Beta<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE"><span class="GramE">´dog</span></span> <span class="SpellE">of</span> <span class="SpellE">the</span> <span class="SpellE">shepherd´</span><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt;"></td></tr>
<tr><td colspan="2" nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=17.582&declination=12.560&viewAngle=25" style="text-decoration: none;"><span class="SpellE">Ras</span> <span class="SpellE">Alhague</span></a><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">α<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE">Alpha</span><o:p></o:p></span></div>
</td><td style="padding: 0cm 0cm 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE"><span class="GramE">´head</span></span> <span class="SpellE">of</span> <span class="SpellE">the</span> <span class="SpellE">snake´</span><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt;"></td></tr>
<tr><td colspan="2" nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=17.173&declination=-15.725&viewAngle=25" style="text-decoration: none;"><span class="SpellE">Sabik</span></a><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">η<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE"><span class="GramE">Eta</span></span><o:p></o:p></span></div>
</td><td style="padding: 0cm 0cm 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE"><span class="GramE">´the</span></span> <span class="SpellE">preceding´</span><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt;"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.astro.uiuc.edu/~jkaler/sow/sabik.html" style="text-decoration: none;" target="starnotes" title="Jim Kaler´s star notes for Sabik">Jim <span class="SpellE">Kaler</span> Notes</a><o:p></o:p></span></div>
</td></tr>
<tr><td colspan="2" nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=16.305&declination=-4.692&viewAngle=25" style="text-decoration: none;"><span class="SpellE">Yed</span> Posterior</a><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ε<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE">Epsilon</span><o:p></o:p></span></div>
</td><td style="padding: 0cm 0cm 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE"><span class="GramE">´hand</span></span>´ (<span class="SpellE">after</span>; <span class="SpellE">eastern</span>)<o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt;"></td></tr>
<tr><td colspan="2" nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=16.239&declination=-3.694&viewAngle=25" style="text-decoration: none;"><span class="SpellE">Yed</span> Prior</a><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">δ<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Delta<o:p></o:p></span></div>
</td><td style="padding: 0cm 0cm 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE"><span class="GramE">´hand</span></span>´ (<span class="SpellE">before</span>; western)<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</td><td style="padding: 0cm 3.75pt;"></td></tr>
</tbody></table>
</div>
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="text-align: center;">
<b><span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">DSO Names - The Night Sky Atlas<o:p></o:p></span></b></div>
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/dsoNames.jsp" style="text-decoration: none;">http://www.nightskyatlas.com/dsoNames.jsp</a><b><o:p></o:p></b></span></div>
<div style="text-align: center;">
<table border="0" cellpadding="0" cellspacing="0" class="MsoNormalTable" style="text-align: center;"><tbody>
<tr><td style="padding: 0cm 3.75pt;"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE">Common</span> <span class="SpellE">Name</span><o:p></o:p></span></div>
</td><td colspan="2" style="padding: 0cm 3.75pt;"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE">Catalog</span> <span class="SpellE">Numbers</span><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt;"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">RA<br /><span class="SpellE">hours</span><o:p></o:p></span></div>
</td><td colspan="2" style="padding: 0cm 3.75pt;"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">DEC<br /><span class="SpellE">degrees</span><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt;"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Notes<o:p></o:p></span></div>
</td><td colspan="2" style="border: medium none; padding: 0cm;" width="247"><div class="MsoNormal">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</td></tr>
<tr style="height: 27pt;"><td colspan="9" style="height: 27pt; padding: 0cm;" valign="bottom"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE"><span lang="EN-US">Ophiucus</span></span><span lang="EN-US">: Visible in February before dawn, to October after dusk, best in June.<o:p></o:p></span></span></div>
</td></tr>
<tr><td colspan="2" nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=17.235&declination=-12.91&viewAngle=20.0" style="text-decoration: none;">Box <span class="SpellE">Nebula</span></a><o:p></o:p></span></div>
</td><td colspan="3" style="padding: 0cm 3.75pt; width: 69.8pt;" valign="top" width="93"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC6309<o:p></o:p></span></div>
</td><td colspan="2" nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">17h 14.1m<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-12° 54.6´<o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 125.15pt;" valign="top" width="167"></td></tr>
<tr><td colspan="2" nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=17.0933&declination=-10.1333&viewAngle=20.0" style="text-decoration: none;"><span class="SpellE">Butterfly</span> <span class="SpellE">Nebula</span></a><o:p></o:p></span></div>
</td><td colspan="3" style="padding: 0cm 3.75pt; width: 69.8pt;" valign="top" width="93"></td><td colspan="2" nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">17h 05.6m<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-10° 08.0´<o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 125.15pt;" valign="top" width="167"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">PK 10+18.2 <span class="SpellE">planetary</span> <span class="SpellE">nebula</span><o:p></o:p></span></div>
</td></tr>
<tr><td colspan="2" nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=16.8533&declination=4.9833&viewAngle=20.0" style="text-decoration: none;">Hercules A</a><o:p></o:p></span></div>
</td><td colspan="3" style="padding: 0cm 3.75pt; width: 69.8pt;" valign="top" width="93"></td><td colspan="2" nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">16h 51.2m<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">+04° 59.0´<o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 125.15pt;" valign="top" width="167"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="GramE">3C</span> 348, MCG+01-43-006<o:p></o:p></span></div>
</td></tr>
<tr><td colspan="2" nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=17.51&declination=-21.4833&viewAngle=20.0" style="text-decoration: none;"><span class="SpellE"><span class="GramE">Kepler´</span></span>s <span class="SpellE">supernova</span>/SNR</a><o:p></o:p></span></div>
</td><td colspan="3" style="padding: 0cm 3.75pt; width: 69.8pt;" valign="top" width="93"></td><td colspan="2" nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">17h 30.6m<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-21° 29.0´<o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 125.15pt;" valign="top" width="167"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="GramE">3C</span> 358<o:p></o:p></span></div>
</td></tr>
<tr><td colspan="2" nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=17.4883&declination=-23.76&viewAngle=20.0" style="text-decoration: none;"><span class="SpellE">Little</span> <span class="SpellE">Ghost</span> <span class="SpellE">Nebula</span></a><o:p></o:p></span></div>
</td><td colspan="3" style="padding: 0cm 3.75pt; width: 69.8pt;" valign="top" width="93"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC6369<o:p></o:p></span></div>
</td><td colspan="2" nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">17h 29.3m<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-23° 45.6´<o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 125.15pt;" valign="top" width="167"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(Steve <span class="SpellE">Gottlieb</span>)<o:p></o:p></span></div>
</td></tr>
<tr><td style="border: medium none;" width="98"></td><td style="border: medium none;" width="53"></td><td style="border: medium none;" width="53"></td><td style="border: medium none;" width="40"></td><td style="border: medium none;" width="25"></td><td style="border: medium none;" width="26"></td><td style="border: medium none;" width="43"></td><td style="border: medium none;" width="67"></td><td style="border: medium none;" width="167"></td></tr>
</tbody></table>
</div>
<div class="MsoNormal">
<div style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</div>
<div style="text-align: center;">
<table border="0" cellpadding="0" cellspacing="0" class="MsoNormalTable" style="text-align: center;"><tbody>
<tr><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=17.55&declination=-26.0&viewAngle=20.0" style="text-decoration: none;"><span class="SpellE">Pipe</span> <span class="SpellE">Nebula</span></a><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"></td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">17h 33.0m<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-26° 00.0´<o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 225pt;" valign="top" width="300"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE">Barnard</span> 59, 56-7, 65; <span class="SpellE">dark</span> <span class="SpellE">nebula</span><o:p></o:p></span></div>
</td></tr>
<tr><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=17.3517&declination=-26.7833&viewAngle=20.0" style="text-decoration: none;"><span class="SpellE">Pipe</span> <span class="SpellE">Nebula</span> <span class="SpellE">Stem</span></a><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"></td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">17h 21.1m<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-26° 47.0´<o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 225pt;" valign="top" width="300"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LDN 1773, also Stem of the Pipe Nebula<o:p></o:p></span></div>
</td></tr>
<tr><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=16.4233&declination=-24.4667&viewAngle=20.0" style="text-decoration: none;"><span class="SpellE">Rho</span> <span class="SpellE">Ophiuchi</span> <span class="SpellE">Complex</span></a><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">IC4603 IC4604<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">16h 25.4m<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-24° 28.0´<o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 225pt;" valign="top" width="300"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">+ <span class="SpellE">dark</span> <span class="SpellE">nebulae</span>; <span class="SpellE">interstellar</span> <span class="SpellE">cloud</span><o:p></o:p></span></div>
</td></tr>
<tr><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=16.6333&declination=-24.1&viewAngle=20.0" style="text-decoration: none;"><span class="SpellE">Rho</span> <span class="SpellE">Ophiuchi</span> <span class="SpellE">Dark</span> <span class="SpellE">Cloud</span></a><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"></td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">16h 38.0m<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-24° 06.0´<o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 225pt;" valign="top" width="300"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">dark lanes in Rho <span class="SpellE">Oph</span> complex<o:p></o:p></span></div>
</td></tr>
<tr><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=16.425&declination=-23.4433&viewAngle=20.0" style="text-decoration: none;"><span class="SpellE">Rho</span> <span class="SpellE">Ophiuchi</span> <span class="SpellE">Nebula</span></a><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">IC4604<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">16h 25.5m<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-23° 26.6´<o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 225pt;" valign="top" width="300"></td></tr>
<tr><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=17.3917&declination=-23.6333&viewAngle=20.0" style="text-decoration: none;">S <span class="SpellE">Nebula</span></a><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"></td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">17h 23.5m<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-23° 38.0´<o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 225pt;" valign="top" width="300"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE">Barnard</span> 72 <span class="SpellE">dark</span> <span class="SpellE">nebula</span>; <span class="SpellE">also</span> <span class="SpellE">Snake</span> <span class="SpellE">Nebula</span><o:p></o:p></span></div>
</td></tr>
<tr><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=17.0933&declination=-10.145&viewAngle=20.0" style="text-decoration: none;"><span class="SpellE">Siamese</span> <span class="SpellE">Squid</span> <span class="SpellE">Nebula</span></a><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"></td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">17h 05.6m<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-10° 08.7´<o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 225pt;" valign="top" width="300"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">M2-<span class="GramE">9 bipolar</span> <span class="SpellE">nebula</span>, <span class="SpellE">also</span> <span class="SpellE">Twinjet</span> <span class="SpellE">Nebula</span>, <span class="SpellE">Butterfly</span><span class="SpellE">Nebula</span><o:p></o:p></span></div>
</td></tr>
</tbody></table>
</div>
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div style="text-align: center;">
<table border="0" cellpadding="0" cellspacing="0" class="MsoNormalTable" style="text-align: center; width: 800px;"><tbody>
<tr><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=17.3917&declination=-23.6333&viewAngle=20.0" style="text-decoration: none;"><span class="SpellE">Snake</span> <span class="SpellE">Nebula</span></a><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 72.75pt;" valign="top" width="97"></td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">17h 23.5m<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-23° 38.0´<o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 156.15pt;" valign="top" width="208"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE">Barnard</span> 72 <span class="SpellE">dark</span> <span class="SpellE">nebula</span>; <span class="SpellE">also</span> S <span class="SpellE">Nebula</span><o:p></o:p></span></div>
</td></tr>
<tr><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=17.3517&declination=-26.7833&viewAngle=20.0" style="text-decoration: none;"><span lang="EN-US">Stem of the Pipe Nebula</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
</td><td style="padding: 0cm 3.75pt; width: 72.75pt;" valign="top" width="97"></td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">17h 21.1m<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-26° 47.0´<o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 156.15pt;" valign="top" width="208"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">LDN 1773, <span class="SpellE">also</span> <span class="SpellE">Pipe</span> <span class="SpellE">Nebula</span><o:p></o:p></span></div>
</td></tr>
<tr><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=17.0933&declination=-10.145&viewAngle=20.0" style="text-decoration: none;"><span class="SpellE">Twinjet</span> <span class="SpellE">Nebula</span></a><o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal">
<b><span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Asterisms - The Night Sky Atlas<o:p></o:p></span></b></div>
<div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/asterisms.jsp" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/asterisms.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</td><td style="padding: 0cm 3.75pt; width: 72.75pt;" valign="top" width="97"></td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">17h 05.6m<o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-10° 08.7´<o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt; width: 156.15pt;" valign="top" width="208"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">M2-<span class="GramE">9 bipolar</span> <span class="SpellE">nebula</span>, <span class="SpellE">also</span> <span class="SpellE">Siamese</span><span class="SpellE">Squid</span> <span class="SpellE">Nebula</span>, <span class="SpellE">Butterfly</span> <span class="SpellE">Nebula</span><o:p></o:p></span></div>
</td></tr>
<tr><td style="padding: 0cm 3.75pt;"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE">Name</span><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt;"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE">Mag</span><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt;"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE">Size</span><o:p></o:p></span></div>
</td><td colspan="2" style="padding: 0cm 3.75pt;"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE">Description</span><o:p></o:p></span></div>
</td></tr>
</tbody></table>
</div>
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div style="text-align: center;">
<table border="0" cellpadding="0" cellspacing="0" class="MsoNormalTable" style="text-align: center; width: 800px;"><tbody>
<tr style="height: 27pt;"><td colspan="4" style="height: 27pt; padding: 0cm;" valign="bottom"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="SpellE"><span lang="EN-US">Ophiucus</span></span><span lang="EN-US">: Visible in February before dawn, to October after dusk, best in June.<o:p></o:p></span></span></div>
</td></tr>
<tr><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=17&declination=0" style="text-decoration: none;"><span class="SpellE">Coffin</span></a><o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="GramE">3</span><o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="GramE">30d</span> X 24d<o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The outline of Delta; Zeta; Eta; Gamma; Alpha; Kappa and Lambda <span class="SpellE">Ophiuchi</span> create the shape of a box for burial; he is a Snake Handler <span class="SpellE">ya´know</span><o:p></o:p></span></div>
</td></tr>
<tr><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=18.5&declination=10" style="text-decoration: none;"><span class="SpellE">Offramp</span></a><o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="GramE">4</span><o:p></o:p></span></div>
</td><td nowrap="" style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">21 <span class="SpellE">deg</span><o:p></o:p></span></div>
</td><td style="padding: 0cm 3.75pt;" valign="top"><div class="MsoNormal" style="margin-bottom: 0pt;">
<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">An elongated section of Milky Way from Epsilon <span class="SpellE">Aquilae</span> to Beta <span class="SpellE">Ophiuchi</span>; also ´The Thumb´ of the Milky Way<o:p></o:p></span></div>
</td></tr>
</tbody></table>
</div>
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="text-align: center;">
<b><span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Principal Stars of <span class="SpellE">Ophiucus</span> - The Night Sky Atlas<o:p></o:p></span></b></div>
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/stardata.jsp?id=OPH" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/stardata.jsp?id=OPH</span></a><o:p></o:p></span></div>
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<h1 style="margin: 0px; position: relative; text-align: center;">
<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Multiple Stars of <span class="SpellE">Ophiucus</span> - The Night Sky Atlas<o:p></o:p></span></h1>
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/multipleStars.jsp?id=OPH" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/multipleStars.jsp?id=OPH</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="text-align: center;">
<b><span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC Objects in <span class="SpellE">Ophiucus</span> - The Night Sky Atlas<o:p></o:p></span></b></div>
<div class="MsoNormal" style="margin-bottom: 0pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="margin-bottom: 0pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/ngcData.jsp?id=OPH" style="text-decoration: none;">http://www.nightskyatlas.com/ngcData.jsp?id=OPH</a><o:p></o:p></span></div>
<h1 style="margin: 0px; position: relative; text-align: center;">
<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">IC Objects in <span class="SpellE">Ophiucus</span> - The Night Sky Atlas<o:p></o:p></span></h1>
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/icData.jsp?id=OPH" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/icData.jsp?id=OPH</span></a><o:p></o:p></span></div>
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<h1 style="margin: 0px; position: relative; text-align: center;">
<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Galaxy Clusters of <span class="SpellE">Ophiucus</span> - The Night Sky Atlas<o:p></o:p></span></h1>
<div class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/catAbell.jsp?id=OPH" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/catAbell.jsp?id=OPH</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
</div>
<div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div style="text-align: center;">
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas – As Constelações - são como janelas que se abrem para a infinitude do universo e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra ...; bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e sendo por nossa mente conscientizado. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">COM UM ABRAÇO ESTRELADO,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>REFERÊNCIAS BIBLIOGRÁFICAS IMPRESSAS para Ophiucus, o Serpentário:</b><o:p></o:p></span></div>
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<span lang="PT" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">COMPILAÇÃO E TRADUÇÃO literal (quando necessária) de Janine Milward:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As Cartas Celestes foram realizadas por Mario Jaci Monteiro e escaneadas por Janine<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- </span><b>Mario Jaci Monteiro</b> , <b>As Constelações, Cartas Celestes</b> -<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Quadro sobre a Precessão dos Equinócios durante 4 Eras</b>, mostrando o Caminho do Sol contra o pano de fundo das constelações do Zodíaco. As cores originais foram invertidas.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Inserido no Artigo “When the Zodiac Climbed into the Sky” por Alexander Gurshtein para a Revista Sky & Telescope edição de outubro de 1995, página 30, publicada por Sky Publishing Corporation, Cambridge, MA, USA.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><b>A Precessão acontece porque</b> as forças gravitacionais do sol e da lua atuam por sobre a Terra (que não é esférica) enquanto esta gira, vagarosamente mudando a orientação do eixo da Terra. Este eixo, inclinado num ângulo de 23<sup>o</sup>., traça um caminho em torno da eclíptica ao longo de 25.800 mil anos terrestres na realização de todo seu círculo. Isso significa que Polaris - a estrela que viemos considerando nossa estrela polar celestial do norte -, vagarosamente irá transmitir sua posição à Vega, a brilhante estrela da constelação da Lira. </i><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Extraído da revista Astronomy, edição de junho de 2002, página 73. Parte do texto foi traduzido literalmente por Janine e também a ilustração sobre o caminho do pólo norte celestial foi invertida, para melhor visualização.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Pequeno Glossário:<o:p></o:p></span></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(1) - Atlas Celeste</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ronaldo Rogério de Freitas Mourão<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">6<sup>ª</sup> edição - Editora Vozes, Petrópolis, RJ, Brasil – 1986<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(2) - Explicando o Cosmos<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ronaldo Rogério de Freitas Mourão<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Editora Tecnoprint S.A., Rio, Brasil, 1984<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">(3)</span><span lang="EN-US"> </span><span lang="EN-US">Norton’s Star Atlas</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">Arthur P Norton and J. Gall Inglis</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">Sky Publishing Co.</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- <b>Wil Tirion - Atlas of the Night Sky</b> - The Hamlyn Publishing Group Limited, London, England</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- <b>Antonin Rükl - The Hamlyn Encyclopedia of Stars & Planets</b> - The Hamlyn Publishng Group Limited, London, England</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- <b>Richard Hinckley Allen, Star Names, Their Lore and Meaning</b>, Dover Publications, Inc, New York, USA</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- <b>Bernard Pellequer - Pequeno Guia do Céu</b> - Editora Martins Fontes, São Paulo, Brasil</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- <b>Identificação do Céu</b> (Livro que foi sendo revisado e reeditado algumas vezes) de autoria de <b>Fernando Vieira</b>,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Secretaria Municipal de Cultura, Fundação Planetário da Cidade do Rio de Janeiro<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(com dedicatória do próprio autor para mim em Curso de Identificação do Céu,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em 30/07/1999))<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do <b>Atlas Celeste</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">de autoria de <b>Ronaldo Rogério de Freitas Mourão</b>,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(com dedicatória do próprio autor para mim<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em evento realizado no Museu de Astronomia do Rio de Janeiro,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em 16/06/1989)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As Cartas Celestes foram realizadas por Mario Jaci Monteiro e escaneadas por Janine<span lang="PT"><br /></span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- </span><b>Mario Jaci Monteiro</b> , <b>As Constelações, Cartas Celestes</b> -<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC - com dedicatória do autor para mim, em março de 2004 (quando Mário Jaci generosamente me presenteou com um instrumento de observação (kepleriano) artesanalmente construído por ele).<o:p></o:p></span></div>
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<a href="http://www.raremaps.com/gallery/detail/35567/Le_Globe_Celeste/De%20La%20Croix.html" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/35567/Le_Globe_Celeste/De%20La%20Croix.html</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Title: </strong>Le Globe Celeste</span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-1350561943900750222013-08-20T08:17:00.002-07:002014-08-28T10:45:44.582-07:00SCORPIUS, O ESCORPIÃO<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif; line-height: 22.399999618530273px;"><span style="line-height: 18px;">Meu Projeto</span></span></span></span><br />
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="text-decoration: none;"><span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763; font-size: small;">Da Terra ao Céu ....</span></span></a></h1>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763; font-size: small;">.....<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="text-decoration: none;">e ao Infinito </a></span></span></h1>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="text-decoration: none;"><span style="color: #073763; font-size: small;">- As 88 Constelações</span></a></span></h1>
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<span style="font-family: Arial, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="text-decoration: none;"><span style="background-color: white;"><span style="color: #073763; font-size: small;">http://daterraaoceueaoinfinito.blogspot.com.br/</span></span></a></span></h1>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo<br />e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;<br />bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.<br /><br />Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<br /><br />Com um abraço estrelado,<br />Janine Milward</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Nesta Página, Caro Leitor,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">vamos conhecer um tantinho</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre o Coração do Escorpião,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre sua Cabeça ou suas Garras</span></div>
<div style="font-family: 'Times New Roman'; text-align: center;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e sobre sua longa Cauda sinuosa e insinuante!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://media.skysurvey.org/interactive360/index.html</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">O Coração, como todos sabemos,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é a estrela-alpha Scorpii, Antares,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">maravilhosamente avermelhada/alaranjada</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e sempre rivalizando com Marte, o Planeta Vermelho -</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">daí ser chamada de anti-ars, ou Antares </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(Ares é o nome grego para Marte).</span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj4W42HFdx-mmlwVJ6negYcXSECfp9piV3r-V9M4p7GeynNVdbHOYJlPu-SqQxwEu2JubwK4IY9vbMG9jvpXGDI_ghmH1XHOVehyoyyywzfAFxHPZNwShQTWE_Krrs8aZELkJz9-0NURWc/s1600/o+cora%C3%A7%C3%A3o.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj4W42HFdx-mmlwVJ6negYcXSECfp9piV3r-V9M4p7GeynNVdbHOYJlPu-SqQxwEu2JubwK4IY9vbMG9jvpXGDI_ghmH1XHOVehyoyyywzfAFxHPZNwShQTWE_Krrs8aZELkJz9-0NURWc/s1600/o+cora%C3%A7%C3%A3o.jpg" height="456" width="640" /></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://media.skysurvey.org/interactive360/index.html</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">As Garras ou a Cabeça</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">são as estrelas que delineiam o começo da constelação do Escorpião</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e por onde a Linha da Eclíptica passa.</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhKvbZZnQqD6QHNka9Jqf460doht7ObL0MZ3lxtEs4-ztGL2jPqgVB66WM2Qr4tc97RqlQG-ZdYMnJRxfwCJQSeY1WkjLNG-Mw0B6p7HJQc-i3tRrSeL_N5t8_vWwcTx1FTObdhbvgyn8k/s1600/a+cabe%C3%A7a.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhKvbZZnQqD6QHNka9Jqf460doht7ObL0MZ3lxtEs4-ztGL2jPqgVB66WM2Qr4tc97RqlQG-ZdYMnJRxfwCJQSeY1WkjLNG-Mw0B6p7HJQc-i3tRrSeL_N5t8_vWwcTx1FTObdhbvgyn8k/s1600/a+cabe%C3%A7a.jpg" height="370" width="640" /></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://media.skysurvey.org/interactive360/index.html</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(Antigamente, muito antigamente, as duas estrelas ponteadoras da Balança</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">era consideradas como As Garras do Escorpião - e isso faz sentido,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">quando as vemos no céu estrelado!).</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjZ4ZWKadTi_EWCKdxSdq58vsK6r0haIREUIT4l1X_XWQrRBcKw53nYB23IzW-0yO127eVuRlh3CJ828OBE8igP8TWw5SzykR1NhcXfKbqNyUwn2ldH3WWWh0gAdVR71JpNVevO56FgSmE/s1600/libra+e+escorpi%C3%A3o.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjZ4ZWKadTi_EWCKdxSdq58vsK6r0haIREUIT4l1X_XWQrRBcKw53nYB23IzW-0yO127eVuRlh3CJ828OBE8igP8TWw5SzykR1NhcXfKbqNyUwn2ldH3WWWh0gAdVR71JpNVevO56FgSmE/s1600/libra+e+escorpi%C3%A3o.jpg" height="640" width="358" /></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://media.skysurvey.org/interactive360/index.html</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A longa Cauda, sinuosa e insinuante,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é uma visão quase fantástica, aterradora, aterrorizante!</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEinWfM8w2eFA-IrcO4G7vV5Lawt13KrH4A0ubs4z92Tl6jYgeOmlV-q0TOTi9Rb4OJZJjWuhvsvQuI-eBr9NodrW37siEH1vNkB-Zs90b3KUhaR0uEKihDZffVzZNVLiDUuYdgU7IUQdxQ/s1600/a+cauda.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEinWfM8w2eFA-IrcO4G7vV5Lawt13KrH4A0ubs4z92Tl6jYgeOmlV-q0TOTi9Rb4OJZJjWuhvsvQuI-eBr9NodrW37siEH1vNkB-Zs90b3KUhaR0uEKihDZffVzZNVLiDUuYdgU7IUQdxQ/s1600/a+cauda.jpg" height="390" width="640" /></a></div>
<div style="text-align: center;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://media.skysurvey.org/interactive360/index.html</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">As duas estrelas que finalizam a Cauda e escondem o veneno do animal rastejante</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- Schaula e Lesath - </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">são duas joias, dois tesouros, duas ameaças!</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Finalmente,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">para testar a boa visão dos Caminhantes,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">lhes digo que muito antigamente, muito antigamente,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">serviam os dois objetos maravilhosos</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que se apresentam quase na fronteira entre o Escorpião e o Sagitário</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e bem direcionados para a região que nos leva ao centro da Galáxia:</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Messier 6 e Messier 7,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Aglomerados Abertos Borboleta e Ptolomeu, respectivamente.</span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg04W0uX3lIaNHl7-k0sQXYpV7xXq3zvXRZoGjtpUnek3MZrWkKyVr9x_hnVSrZiBhy2jN3TIMq17y_nS6BpQlJP8fmueoJpmgKVT8rUhdYmz9VSTcADf52Kn91sk20fqktbRQLdMCGBtY/s1600/schuala+e+lesath+e+m6+e+m7.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg04W0uX3lIaNHl7-k0sQXYpV7xXq3zvXRZoGjtpUnek3MZrWkKyVr9x_hnVSrZiBhy2jN3TIMq17y_nS6BpQlJP8fmueoJpmgKVT8rUhdYmz9VSTcADf52Kn91sk20fqktbRQLdMCGBtY/s1600/schuala+e+lesath+e+m6+e+m7.jpg" height="354" width="640" /></a></div>
<div style="text-align: center;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://media.skysurvey.org/interactive360/index.html</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Last but not least,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é na direção da constelação do Escorpião</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que encontra-se </span><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Scorpius X-1 </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- considerada a mais forte fonte de emissão de raio-x no céu</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(depois de nosso Sol, é claro).</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Boa Observação e Bons Estudos!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span></div>
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<span style="color: #274e13; font-family: Arial, sans-serif;"><span style="font-size: 15px;"><b>Mario Jaci Monteiro - As Constelações, Cartas Celestes</b></span></span><br />
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<span style="color: #274e13; font-family: Arial, sans-serif;"><span style="font-size: 15px;"><b>http://apod.nasa.gov/apod/ap140504.html</b></span></span></div>
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<span style="color: #274e13; font-family: Arial, sans-serif;"><span style="font-size: 15px;"><b><a href="http://apod.nasa.gov/apod/ap140504.html" style="color: #274e13; text-decoration: none;">http://apod.nasa.gov/apod/ap140504.html</a></b></span></span></div>
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<span style="color: #274e13;"><b><span style="font-family: Arial, Helvetica, sans-serif;">A Scorpius Sky Spectacular </span></b><br /><span style="font-size: medium;"><b>Image Credit & Copyright: </b><a href="http://sguisard.astrosurf.com/" style="color: #274e13; text-decoration: none;">Stéphane Guisard</a>, <a href="http://www.twanight.org/newTWAN/index.asp" style="color: #274e13; text-decoration: none;">TWAN</a></span></span></center>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>Explanation: </b>If Scorpius looked this good to the unaided eye, humans might remember it better. <a href="http://www.allthesky.com/constellations/scorpius/" style="color: #274e13; text-decoration: none;">Scorpius</a> more typically appears as a few bright stars in a well-known but rarely pointed out <a href="http://en.wikipedia.org/wiki/Zodiac" style="color: #274e13; text-decoration: none;">zodiacal</a> <a href="http://modernconstellations.com/constellationhistory.html" style="color: #274e13; text-decoration: none;">constellation</a>. To get a spectacular image like <a href="http://astrosurf.com/sguisard/Pagim/Scorpius_constellation-LHRVB-50mm.html" style="color: #274e13; text-decoration: none;">this</a>, though, one needs a good <a href="http://electronics.howstuffworks.com/digital-camera.htm" style="color: #274e13; text-decoration: none;">camera</a>, color <a href="http://en.wikipedia.org/wiki/Filter_%28optics%29" style="color: #274e13; text-decoration: none;">filters</a>, and a digital image processor. To bring out detail, the <a href="http://astrosurf.com/sguisard/Pagim/Scorpius_constellation-LHRVB-50mm.html" style="color: #274e13; text-decoration: none;">above image</a> not only involved long duration exposures taken in several colors, but one exposure in a <a href="http://apod.nasa.gov/apod/ap050930.html" style="color: #274e13; text-decoration: none;">very specific red color</a> emitted by <a href="http://periodic.lanl.gov/1.shtml" style="color: #274e13; text-decoration: none;">hydrogen</a>. The <a href="http://astrosurf.com/sguisard/Pagim/Scorpius_constellation-LHRVB-50mm.html" style="color: #274e13; text-decoration: none;">resulting image</a> shows many breathtaking features. Vertically across the image left is part of the <a href="http://apod.nasa.gov/apod/ap050605.html" style="color: #274e13; text-decoration: none;">plane</a> of our <a href="http://en.wikipedia.org/wiki/Milky_Way" style="color: #274e13; text-decoration: none;">Milky Way Galaxy</a>. Visible there are vast clouds of bright stars and long filaments of dark <a href="http://apod.nasa.gov/apod/ap030706.html" style="color: #274e13; text-decoration: none;">dust</a>. Jutting out diagonally from the <a href="http://apod.nasa.gov/apod/ap070123.html" style="color: #274e13; text-decoration: none;">Milky Way</a> in the image center are dark dust bands known as the <a href="http://apod.nasa.gov/apod/ap090708.html" style="color: #274e13; text-decoration: none;">Dark River</a>. This river connects to several bright stars on the right that are part of <a href="http://www.ianridpath.com/startales/scorpius.htm" style="color: #274e13; text-decoration: none;">Scorpius' head and claws</a>, and include the bright star <a href="http://stars.astro.illinois.edu/sow/antares.html" style="color: #274e13; text-decoration: none;">Antares</a>. Above and right of Antares is an even brighter planet Jupiter. Numerous red <a href="http://apod.nasa.gov/apod/emission_nebulae.html" style="color: #274e13; text-decoration: none;">emission nebulas</a> and blue <a href="http://en.wikipedia.org/wiki/Reflection_nebula" style="color: #274e13; text-decoration: none;">reflection nebulas</a> are visible throughout the image.<a href="http://en.wikipedia.org/wiki/Scorpion" style="color: #274e13; text-decoration: none;">Scorpius</a> appears prominently in southern skies after sunset during the middle of the year.</span></div>
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<span style="font-family: Arial, sans-serif;"><b><span style="color: #660000;"><span style="font-size: large;">SCORPIUS, O ESCORPIÃO</span></span><span style="color: #0f243e; font-size: 11pt;"><o:p></o:p></span></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Mito:</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Esta constelação representa o escorpião morto por Orion.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Os poetas gregos nos ensinavam que Scorpius foi o animal enviado por Diana para matar Orion, que intervinha nas atividades da caçadora, mas ele nunca conseguia atingir a sua meta: realmente, as estrelas de Orion desaparecem no ocidente justamente quando o Escorpião nasce no oriente.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Algumas Informações Interessantes acerca esta Constelação:</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Segundo alguns autores, sua origem deve associar-se às secas e às pragas que assolavam o Egito quando o Sol se encontrava naquela região do céu.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Desde a mais remota antiguidade, esta constelação foi representada pelos gregos, latinos, árabes e persas pela figura de um escorpião.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">O equinócio de outono, há 3000 aC, localizava-se aí, quando este asterismo foi instituído. Na Pérsia, Antares, a estrela mais brilhante do Escorpião, era uma das quatro “Estrelas Reais”, uma das guardiãs do céu e, naquela época, indicava o outono.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Fronteiras:</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Scorpius situa-se entre Libra, Lupus, Norma, Ara, Corona Australis, Sagittarius, Ophiucus, Serpens<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;"> 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<span style="color: #274e13;">The Mythology of the Night Sky: An Amateur Astronomer's Guide to the Ancient ...</span></h1>
<span style="color: #274e13;"><span style="font-family: Arial, sans-serif; font-size: 13px; line-height: normal; text-align: start;"> </span><span class="addmd" style="font-family: Arial, sans-serif; font-size: 11px; left: -5px; line-height: normal; margin-left: 2px; position: relative; text-align: start;">Por David E. Falkner</span></span></div>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">O CORAÇÃO DO ESCORPIÃO</span></b></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a href="http://nexusnow.info/forum/showthread.php?13982-Star-of-the-week-Antares-is-Heart-of-the-Scorpion" style="color: #274e13; text-decoration: none;">http://nexusnow.info/forum/showthread.php?13982-Star-of-the-week-Antares-is-Heart-of-the-Scorpion</a></span></div>
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<a href="mailto:stargazerbob@aol.com" style="color: #274e13; text-align: left;"><span style="font-family: Arial, Helvetica, sans-serif;">stargazerbob@aol.com</span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;"><b>Antares.</b><b> Alpha Scorpii. Estrela Dupla e Variável</b></span><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 16h28,2m - Declinação -26<sup>o</sup> 23’<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude visual 1,22 - Distância 520 anos-luz<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude visual 1,1 e 6,5 Distância entre estrelas 2”,90<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Uma estrela binária, intensamente avermelhada e verde-esmeralda, situada no corpo do Escorpião. De Anti-Ares, similar ou Rival de Ares, Marte. Foi uma das quatro estrelas reais da Pérsia, cerca de 3.000 anos a.c., e atuava como a Guardiã do Oeste pois marcava o Equinócio de Outono. Muitas vezes chamada de Coração do Escorpião, Cor Scorpio.<span style="color: #0f243e;"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;"> 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<span style="color: #252525; font-family: sans-serif; text-align: start;">Antares é uma </span><a href="http://pt.wikipedia.org/wiki/Estrela_supergigante" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Estrela supergigante">estrela supergigante</a><span style="color: #252525; font-family: sans-serif; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Classificação estelar">classe M</a><span style="color: #252525; font-family: sans-serif; text-align: start;">, com um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Raio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Raio">raio</a><span style="color: #252525; font-family: sans-serif; text-align: start;"> de aproximadamente 800 vezes o </span><a href="http://pt.wikipedia.org/wiki/Raio_solar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Raio solar">raio do Sol</a><span style="color: #252525; font-family: sans-serif; text-align: start;">; se fosse colocada no centro do </span><a href="http://pt.wikipedia.org/wiki/Sistema_Solar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Sistema Solar">Sistema Solar</a><span style="color: #252525; font-family: sans-serif; text-align: start;">, sua parte mais externa se encontraria entre a órbita de </span><a href="http://pt.wikipedia.org/wiki/Marte_(planeta)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Marte (planeta)">Marte</a><span style="color: #252525; font-family: sans-serif; text-align: start;"> e </span><a href="http://pt.wikipedia.org/wiki/J%C3%BApiter_(planeta)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Júpiter (planeta)">Júpiter</a><span style="color: #252525; font-family: sans-serif; text-align: start;">. Antares está a aproximadamente 600 </span><a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Ano-luz">anos-luz</a><span style="color: #252525; font-family: sans-serif; text-align: start;"> (180 </span><a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Parsec">pc</a><span style="color: #252525; font-family: sans-serif; text-align: start;">) da </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="color: #252525; font-family: sans-serif; text-align: start;">. Sua </span><a href="http://pt.wikipedia.org/wiki/Luminosidade" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Luminosidade">luminosidade</a><span style="color: #252525; font-family: sans-serif; text-align: start;"> visual é de cerca de 10 000 vezes a do Sol, mas como a estrela irradia uma parte considerável de sua energia na parte </span><a href="http://pt.wikipedia.org/wiki/Radia%C3%A7%C3%A3o_infravermelha" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Radiação infravermelha">infravermelha</a><span style="color: #252525; font-family: sans-serif; text-align: start;"> do </span><a href="http://pt.wikipedia.org/wiki/Espectro_(f%C3%ADsica)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Espectro (física)">espectro</a><span style="color: #252525; font-family: sans-serif; text-align: start;">, sua luminosidade bolométrica é de 65 000 vezes a solar. A </span><a href="http://pt.wikipedia.org/wiki/Massa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Massa">massa</a><span style="color: #252525; font-family: sans-serif; text-align: start;"> de Antares é de 15 a 18 </span><a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Massa solar">massas solares</a><span style="color: #252525; font-family: sans-serif; text-align: start;">.</span><span class="reference" id="cite_ref-kaler_3-0" style="bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Antares#cite_note-kaler-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span><span style="color: #252525; font-family: sans-serif; text-align: start;"> Esse tamanho grande e relativamente pouca massa dão a Antares uma </span><a href="http://pt.wikipedia.org/wiki/Densidade" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Densidade">densidade</a><span style="color: #252525; font-family: sans-serif; text-align: start;"> muito pequena.</span></div>
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<span style="text-align: start;"><span style="color: #252525; font-family: sans-serif;"><a href="http://pt.wikipedia.org/wiki/Antares" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Antares</a></span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhWN48R69I3wjnxJNmmP1UkLPaBZc6gwGoOwmJ6661G8Zb8VNhU9BNGX7dCalDcw76XO0MRm7I57BKTqrKHyEGgsZUBBJTGZOn4RTxIsXV7b7ut5iiUFL0mEI4AMVt4Qeuwx0bgE0yqYK0/s1600/GiganteVermelha.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhWN48R69I3wjnxJNmmP1UkLPaBZc6gwGoOwmJ6661G8Zb8VNhU9BNGX7dCalDcw76XO0MRm7I57BKTqrKHyEGgsZUBBJTGZOn4RTxIsXV7b7ut5iiUFL0mEI4AMVt4Qeuwx0bgE0yqYK0/s1600/GiganteVermelha.jpg" height="640" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></a></div>
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<span style="color: #274e13; font-family: Arial, sans-serif;"><span style="font-size: 15px;"><a href="http://pt.wikipedia.org/wiki/Antares#mediaviewer/Ficheiro:GiganteVermelha.jpg" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Antares#mediaviewer/Ficheiro:GiganteVermelha.jpg</a></span></span></div>
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<span style="color: #274e13;"><span class="mw-mmv-title" style="font-size: 1.2em; max-width: 60%; overflow: hidden; text-overflow: ellipsis;">GiganteVermelha</span></span></div>
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<span style="color: #274e13;"><span class="mw-mmv-author">By Sebastiao Rocha (?)</span> </span></div>
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<span style="color: #274e13;">Comparação entre Antares e o <a href="http://pt.wikipedia.org/wiki/Sol" style="background: none; color: #274e13; text-decoration: none;" title="Sol">Sol</a>, que é mostrado como um pequeno ponto no canto superior direito da imagem. O círculo preto é do tamanho da órbita de <a href="http://pt.wikipedia.org/wiki/Marte_(planeta)" style="background: none; color: #274e13; text-decoration: none;" title="Marte (planeta)">Marte</a>. A outra estrela é <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Arcturus" style="background: none; color: #274e13; text-decoration: none;" title="Arcturus">Arcturus</a>.</span></div>
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<span style="color: #274e13;">Uma gigante vermelha comparada com o Sol e outras estrelas</span></div>
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<span style="color: #274e13;">Detalhes da licença</span></h3>
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<span style="color: #274e13;">Released into the public domain (by the author)</span></div>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">Ainda próximo a Antares, </span></b></div>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">vamos encontrar uma outra estrela </span></b></div>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">que também se alcunha de Coração:</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US"><b>Al Nyiat</b></span><span lang="EN-US"><b> - Tau Scorpii</b><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A Aorta, denominação árabe que designa o coração do Escorpião - usada também para Alpha e Sigma Scorpii.</span></div>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">Visualmente próximo a Antares, ao Coração do Escorpião,</span></b></div>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">encontraremos um belíssimo Aglomerado Globular:</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>M 4 - NGC 6121 - Scorpius - Aglomerado Estelar Globular</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 16h22m Declinação -26<sup>o</sup>.27<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude visual integral 6,1 Tipo AG</span><span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;"><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;"> 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgh_k8tHs9CtMXndgSYG-K8ipKJJLi2nktch1S2_OrJtF3ZDVAh4ozV83SWcJQyky5S0c3Eb4pS4dYkXP95ewv2nG0uL5T3iHCFbVGTL_dixfoAEjL1W0xrwwq_BUT75WVdqYlpZQ3AM-g/s1600/800px-Messier_4_Hubble_WikiSky.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgh_k8tHs9CtMXndgSYG-K8ipKJJLi2nktch1S2_OrJtF3ZDVAh4ozV83SWcJQyky5S0c3Eb4pS4dYkXP95ewv2nG0uL5T3iHCFbVGTL_dixfoAEjL1W0xrwwq_BUT75WVdqYlpZQ3AM-g/s1600/800px-Messier_4_Hubble_WikiSky.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<span style="color: #274e13; font-family: Arial, sans-serif;"><span style="font-size: 15px;"><a href="http://pt.wikipedia.org/wiki/Messier_4#mediaviewer/Ficheiro:Messier_4_Hubble_WikiSky.jpg" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Messier_4#mediaviewer/Ficheiro:Messier_4_Hubble_WikiSky.jpg</a></span></span></div>
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<span class="mw-mmv-title" style="font-size: 1.2em; max-width: 60%; overflow: hidden; text-overflow: ellipsis;"><span style="color: #274e13;">Messier 4 Hubble WikiSky</span></span></div>
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<span class="mw-mmv-author"><span style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13;"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="en:NASA">en:NASA</a></span></span></div>
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<span style="color: #274e13;"><b>Messier 4</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">NGC 6121</a>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Estrela">estrelas</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Constelação">constela</a><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Constelação">ção</a> de <a href="http://pt.wikipedia.org/wiki/Scorpius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Scorpius">Escorpião</a>, descoberto pelo astrônomo suíço <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Foi catalogado pelo astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 1764, que foi o primeiro a reconhecer o <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objeto_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Objeto astronômico">objeto astronômico</a> como um aglomerado globular, o primeiro descoberto da história.</span></div>
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<span style="color: #274e13;">Tem <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #274e13; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 7,1, não sendo possível observá-lo a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Olho_nu" style="background: none; color: #274e13; text-decoration: none;" title="Olho nu">olho nu</a>, mas com o uso de <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background: none; color: #274e13; text-decoration: none;" title="Binóculo">binóculos</a> e pequenos <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none; color: #274e13; text-decoration: none;" title="Telescópio">telescópios</a> é possível identificá-lo como uma pequena mancha nebulosa e difusa. Suas estrelas mais brilhantes são vistas apenas com o uso de telescópios maiores. Está a uma distância de cerca de 33 900 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #274e13; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #274e13; text-decoration: none;" title="Terra">Terra</a> e sua idade foi estimada em 12,2 bilhões de anos. Localiza-se a apenas 1,3° a leste de <a href="http://pt.wikipedia.org/wiki/Antares" style="background: none; color: #274e13; text-decoration: none;" title="Antares">Antares</a>, a estrela amarelada e a mais brilhante da constelação de<a href="http://pt.wikipedia.org/wiki/Scorpius" style="background: none; color: #274e13; text-decoration: none;" title="Scorpius">Escorpião</a>.</span></div>
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<span style="color: #274e13; font-family: sans-serif;"><a href="http://pt.wikipedia.org/wiki/Messier_4" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Messier_4</a></span></div>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">AS GARRAS</span></b></div>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">OU</span></b></div>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">A CABEÇA DO ESCORPIÃO</span></b></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Stellarium</span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Stellarium</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Graffias ou Acrab</b><b>. Beta Scorpii. Estrela Dupla</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">AR 16h02m Dec. - 19<sup>o</sup>.40<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude visual 2,9 e 5,1 Distância entre estrelas 13”,63<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Uma estrela tripla, branco pálido e lilás, situada na cabeça do Escorpião. Esta estrela é também conhecida por Acrab, nome árabe que deu origem à constelação do Escorpião.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Isidis ou Dschubba ou Jabbah.</b><b> Delta Scorpii. </b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude 2.34 Distância 520 anos-luz<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Situada próxima da garra direita do Escorpião. Nome árabe que designa A Fronte.<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="color: #073763;"><b>NGC 6093 - M 80 - Aglomerado Globular</b><o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="color: #073763;">Ascensão Reta 16h15 Declinação -22<sup>o</sup>.56<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="color: #073763;">Magnitude fotográfica global 8,4 Diâmetro aparente 5’,1 Tipo Espectral F4<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="color: #073763;">Distância kpc 11,0 Velocidade Radial (km/s) + 18</span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;"> 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<span style="color: #274e13;"><b style="font-family: sans-serif; text-align: start;">Messier 80</b><span style="font-family: sans-serif; text-align: start;"> (também conhecido como </span><b style="font-family: sans-serif; text-align: start;">M80</b><span style="font-family: sans-serif; text-align: start;"> ou </span><b style="font-family: sans-serif; text-align: start;">NGC 6093</b><span style="font-family: sans-serif; text-align: start;">) é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="font-family: sans-serif; text-align: start;"> localizado na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="font-family: sans-serif; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/Scorpius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Scorpius">Scorpius</a><span style="font-family: sans-serif; text-align: start;"> a 32 600 </span><a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Ano-luz">anos-luz</a><span style="font-family: sans-serif; text-align: start;"> da </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="font-family: sans-serif; text-align: start;">. Foi descoberto por</span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="font-family: sans-serif; text-align: start;"> em </span><a href="http://pt.wikipedia.org/wiki/1781" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="1781">1781</a><span style="font-family: sans-serif; text-align: start;">. Possui um raio de 47,5 anos-luz e uma dimensão aparente de 10,0 </span><a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Minuto de arco">minutos de arco</a><span style="font-family: sans-serif; text-align: start;">.</span><span class="reference" id="cite_ref-seds_2-4" style="bottom: 1ex; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_80#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none; white-space: nowrap;">2</a></span></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>A SINUOSA CAUDA DO ESCORPIÃO</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="FR"><b>Wei - </b></span><span lang="FR"><b>Epsilon Scorpii</b><o:p></o:p></span></span></div>
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<span lang="FR"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A Cauda, nome de origem chinesa para designar a cauda do Escorpião.</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Lesath. Upsilon Scorpii. </b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma pequena estrela situada na cauda venenosa do Escorpião, o Ferrão. </span></div>
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<span lang="ES-TRAD"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">De Al Las’ah, o Ferrão.<o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="FR"><b>Schaula</b></span><span lang="FR"><b> - Lambda Scorpii</b><o:p></o:p></span></span></div>
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<span lang="FR"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h32,mm - Declinação -37o.05<o:p></o:p></span></span></div>
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<span lang="FR"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual 1,71 - Distância 310 anos-luz<o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A Cauda do Escorpião<o:p></o:p></span></div>
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<span lang="FR"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A Cauda, nome árabe que designa o grupo de estrelas formado por Lambda e Nu Scorpii.<o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Nu Scorpii - Estrela Dupla</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">AR 16h09m Dec. - 19<sup>o</sup>.20<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual 4,3 e 6,5 Distância entre estrelas 41’,25</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Sargas - Teta Scorpii</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Cavalo Teimoso, nome de origem persa.<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Girtab - Kappa Scorpii</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Mordedor, designação de origem árabe </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">utilizada também para as estrelas Iota, Lambda e Epsilon</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> da constelação do Escorpião.</span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;"> 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<span style="color: #274e13;"><b style="font-family: sans-serif; text-align: start;">Kappa Scorpii</b><span style="font-family: sans-serif; text-align: start;"> (κ Sco, κ Scorpii) is a </span><a href="http://en.wikipedia.org/wiki/Binary_star" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Binary star">binary star</a><span style="font-family: sans-serif; text-align: start;"> system in the southern </span><a href="http://en.wikipedia.org/wiki/Constellation" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Constellation">constellation</a><span style="font-family: sans-serif; text-align: start;"> of </span><a href="http://en.wikipedia.org/wiki/Scorpius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Scorpius">Scorpius</a><span style="font-family: sans-serif; text-align: start;">. It has the traditional name </span><b style="font-family: sans-serif; text-align: start;">Girtab</b><span style="font-family: sans-serif; text-align: start;">,</span><sup class="reference" id="cite_ref-falkner2011_8-0" style="font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Kappa_Scorpii#cite_note-falkner2011-8" style="background: none; text-decoration: none; white-space: nowrap;">[8]</a></sup><span style="font-family: sans-serif; text-align: start;"> which is the Sumerian word for 'scorpion' and has survived through the </span><a href="http://en.wikipedia.org/wiki/Babylonian_star_catalogues" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Babylonian star catalogues">Babylonian star catalogues</a><span style="font-family: sans-serif; text-align: start;">.</span><sup class="reference" id="cite_ref-ridpath1989_9-0" style="font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Kappa_Scorpii#cite_note-ridpath1989-9" style="background: none; text-decoration: none; white-space: nowrap;">[9]</a></sup><span style="font-family: sans-serif; text-align: start;"> The name </span><b style="font-family: sans-serif; text-align: start;">Girtab</b><span style="font-family: sans-serif; text-align: start;"> is actually (or perhaps originally) applied to an </span><a href="http://en.wikipedia.org/wiki/Asterism_(astronomy)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Asterism (astronomy)">asterism</a><span style="font-family: sans-serif; text-align: start;"> comprising this star,</span><a href="http://en.wikipedia.org/wiki/Lambda_Scorpii" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Lambda Scorpii">Lambda Scorpii</a><span style="font-family: sans-serif; text-align: start;">, </span><a href="http://en.wikipedia.org/wiki/Upsilon_Scorpii" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Upsilon Scorpii">Upsilon Scorpii</a><span style="font-family: sans-serif; text-align: start;">, and </span><a href="http://en.wikipedia.org/wiki/Iota_Scorpii" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Iota Scorpii">Iota Scorpii</a><span style="font-family: sans-serif; text-align: start;">.</span><sup class="reference" id="cite_ref-falkner2011_8-1" style="font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Kappa_Scorpii#cite_note-falkner2011-8" style="background: none; text-decoration: none; white-space: nowrap;">[8]</a></sup><span style="font-family: sans-serif; text-align: start;"> With an </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Apparent_visual_magnitude" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start;" title="Apparent visual magnitude">apparent visual magnitude</a><span style="font-family: sans-serif; text-align: start;"> of 2.4,</span><sup class="reference" id="cite_ref-scfs_2-2" style="font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Kappa_Scorpii#cite_note-scfs-2" style="background: none; text-decoration: none; white-space: nowrap;">[2]</a></sup><span style="font-family: sans-serif; text-align: start;"> this star system is readily visible to the naked eye. </span><a href="http://en.wikipedia.org/wiki/Parallax" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Parallax">Parallax</a><span style="font-family: sans-serif; text-align: start;"> measurements place it at an estimated distance of roughly 480 </span><a href="http://en.wikipedia.org/wiki/Light-year" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Light-year">light-years</a><span style="font-family: sans-serif; text-align: start;"> (150 </span><a href="http://en.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Parsec">parsecs</a><span style="font-family: sans-serif; text-align: start;">) from the </span><a href="http://en.wikipedia.org/wiki/Earth" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Earth">Earth</a><span style="font-family: sans-serif; text-align: start;">.</span><sup class="reference" id="cite_ref-aaa474_2_653_1-5" style="font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Kappa_Scorpii#cite_note-aaa474_2_653-1" style="background: none; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgQ2OB5Hd-XDbrXzLcgXNeBCdyk2QX4m-4nziWV63q3RhYcQlK6_r3ysER6YfI-kPDD3x71CnIJgfBzYepSahp2CjTaYdxUOUYTu7_LCgr7HRHQGAqJQAPsl9n2APF79B4mMqjCj63eyj8/s1600/NGC+6231.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgQ2OB5Hd-XDbrXzLcgXNeBCdyk2QX4m-4nziWV63q3RhYcQlK6_r3ysER6YfI-kPDD3x71CnIJgfBzYepSahp2CjTaYdxUOUYTu7_LCgr7HRHQGAqJQAPsl9n2APF79B4mMqjCj63eyj8/s1600/NGC+6231.jpg" /></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 6231 - Aglomerado Aberto Scorpius</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 16h52m Declinação 41<sup>o</sup>.56<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 8,5 Magnitude fotográfica da mais brilhante estrela 7,5<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> Distância kpc 1,77 Diâmetro 16’ Tipo Espectral O7<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Situado ao norte do par formado por Zeta Scorpii, possui um diâmetro de 10’. Junto a este encontra-se um outro aglomerado, o H12. A observação de ambos estes aglomerados acontece mesmo a olho nú porém podendo ser mais bem observados através um bom par de binóculos ou uma luneta. NGC 6231 é mais concentrado em suas 120 estrelas enquanto H12 é bem mais disperso e maior acolhendo cerca de 200 estrelas num círculo de 40’ de diâmetro.<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;"> 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="color: #274e13;"><b style="background-color: white; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">NGC 6231</b><span style="background-color: white; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background: none rgb(255, 255, 255); font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="background-color: white; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Scorpius" style="background: none rgb(255, 255, 255); font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Scorpius">constelação de Scorpius</a><span style="background-color: white; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Giovanni_Hodierna" style="background: none rgb(255, 255, 255); font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Giovanni Hodierna">Giovanni Hodierna</a><span style="background-color: white; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> em 1654, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none rgb(255, 255, 255); font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="background-color: white; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">refrator. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none rgb(255, 255, 255); font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="background-color: white; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> (+2,6), é visível mesmo a </span><a href="http://pt.wikipedia.org/wiki/Olho_nu" style="background: none rgb(255, 255, 255); font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Olho nu">olho nu</a><span style="background-color: white; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">.</span></span></div>
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<img alt="Scorpius constellation map.png" src="http://upload.wikimedia.org/wikipedia/commons/thumb/5/52/Scorpius_constellation_map.png/250px-Scorpius_constellation_map.png" height="640" width="640" /></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_6231">http://pt.wikipedia.org/wiki/NGC_6231</a></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Dois Aglomerados Abertos bem próximos um ao outro<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">e facilmente encontrados ao final da cauda do Escorpião:</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M6 - NGC 6405 - Aglomerado Aberto - Aculeus</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Um belo aglomerado aberto bem visível a olho nú ou através pequenos telescópios.<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M7 - NGC 6475 - Aglomerado Aberto - Acumen</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Um belo aglomerado aberto bem visível a olho nú ou através pequenos telescópios.<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 6405 - M 6 - Aglomerado Aberto Scorpius</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h38m Declinação -32<sup>o</sup>.12<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 4,6 Magnitude fotográfica da mais brilhante estrela 8,3<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> Distância kpc 0,45 Diâmetro 26’ Tipo Espectral B4<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 6475 - M 7 - Aglomerado Aberto Scorpius</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h52m Declinação -34<sup>o</sup>.48<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 3,3 Magnitude fotográfica da mais brilhante estrela 7,4<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> Distância kpc 0,23 Diâmetro 50’ Tipo Espectral B5</span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;"> 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg8o82zssRavhetZeDy1n1DE1phEkybWBq4D5SWuZB_fIrWp4ulWIlgiiG4YsWgOxhvagPq3eRD0BXEnbKdsgxJcN2Gi-kV7imkInxdj4_YWbGNuZBgmMwQr7rcySAIN5cI_2JzZWeGO4k/s1600/borboleta+-+m+6.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg8o82zssRavhetZeDy1n1DE1phEkybWBq4D5SWuZB_fIrWp4ulWIlgiiG4YsWgOxhvagPq3eRD0BXEnbKdsgxJcN2Gi-kV7imkInxdj4_YWbGNuZBgmMwQr7rcySAIN5cI_2JzZWeGO4k/s1600/borboleta+-+m+6.jpg" /></span></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M 6 - NGC 6405 - Scorpius - Aglomerado Estelar Aberto - A Borboleta</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h38m Declinação -32<sup>o</sup>.11<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual integral 6,0 Tipo AA<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Para alguns, o desenho do aglomerado aberto M6, também conhecido como NGc 5405, se parece com uma borboleta. M5 espalha-se ao longo de cerca de 20 anos-luz e dista cerca de 2 mil anos-luz de nós. M6 pode bem ser visualizado a olho nú, sempre em lugares de céus escuros e transparentes, porém também um par de binóculos nos apresenta uma bela visão, como se fosse uma lua cheia de estrelas. Como acontece em outros aglomerados abertos, M6 é composto predominantemente de estrelas jovens e azuis, apesar de que a estrela mais brilhante é quase alaranjada. M6 é estimado em ter cerca de 100 milhões de idade. A determinação de aglomerados tais como M6 ajuda os astronomos a calibrarem a escala de distâncias do universo.<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;"> 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<span style="color: #274e13;">O <b>Aglomerado da Borboleta</b> (Messier 6, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="New General Catalogue">NGC 6405</a>) é um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Estrela">estrelas</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Scorpius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Scorpius">Escorpião</a>. O primeiro astrônomo a registrar a existência do aglomerado foi o italiano <a href="http://pt.wikipedia.org/wiki/Giovanni_Battista_Hodierna" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Giovanni Battista Hodierna">Giovanni Battista Hodierna</a> em 1654. Entretanto, o astronômo americano <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Robert_Burnham,_Jr.&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Robert Burnham, Jr. (página não existe)">Robert Burnham, Jr.</a> argumenta que o astrônomo <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ptolomeu" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Ptolomeu">Ptolomeu</a>, no <a href="http://pt.wikipedia.org/wiki/S%C3%A9culo_I" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Século I">século I</a>, observou o aglomerado enquanto observava outro objeto vizinho, o <a href="http://pt.wikipedia.org/wiki/Aglomerado_de_Ptolomeu" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Aglomerado de Ptolomeu">Aglomerado de Ptolomeu</a>. O astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Charles Messier">Charles Messier</a> catalogou o aglomerado como Messier 6 em 1764.</span></div>
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<span style="color: #274e13;">Tem <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 4,2, sendo possível observá-lo a <a href="http://pt.wikipedia.org/wiki/Olho_nu" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Olho nu">olho nu</a> sob boas condições de visualização. Suas estrelas mais brilhantes podem ser visualizadas com o auxílio de <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Binóculo">binóculos</a> ou pequenos <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Telescópio">telescópios</a>. Situa-se a apenas 6 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Terra">Terra</a> e sua idade foi estimada em 100 milhões de anos. Na <a href="http://pt.wikipedia.org/wiki/Esfera_celeste" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Esfera celeste">esfera celeste</a>, situa-se logo a norte da ponta da "cauda" da constelação de <a href="http://pt.wikipedia.org/wiki/Scorpius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Scorpius">Escorpião</a>.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Aglomerado_da_Borboleta</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgM1gROTAdTdv9JbknDJVrNAkn3aJowr4FG5yGGXQtGqYjZfqYNrbI8eftDh9ns-Wdi5JBi4NbFOAbiXhs_-9x2Vz0O1jvVwtfVIeximGkGj2WRjoKLg7Tba5Qxy53HivzvD1U1hyphenhyphen2wCNw/s1600/m+7.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgM1gROTAdTdv9JbknDJVrNAkn3aJowr4FG5yGGXQtGqYjZfqYNrbI8eftDh9ns-Wdi5JBi4NbFOAbiXhs_-9x2Vz0O1jvVwtfVIeximGkGj2WRjoKLg7Tba5Qxy53HivzvD1U1hyphenhyphen2wCNw/s1600/m+7.jpg" /></span></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M 7 - NGC 6475 - Scorpius - Aglomerado Estelar Aberto</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h52m Declinação -34<sup>o</sup>.48<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual integral 5,0 Tipo AA<o:p></o:p></span></div>
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<span style="color: #274e13;">O <b>Aglomerado de Ptolomeu</b> (Messier 7, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; text-decoration: none;" title="New General Catalogue">NGC 6475</a>) é um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background: none; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; text-decoration: none;" title="Estrela">estrelas</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Scorpius" style="background: none; text-decoration: none;" title="Scorpius">Escorpião</a>. O primeiro observador a registrar a existência do aglomerado foi <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ptolomeu" style="background: none; text-decoration: none;" title="Ptolomeu">Ptolomeu</a> ainda no <a href="http://pt.wikipedia.org/wiki/S%C3%A9culo_II" style="background: none; text-decoration: none;" title="Século II">século II</a>. O astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; text-decoration: none;" title="Charles Messier">Charles Messier</a> catalogou o aglomerado como Messier 7 em 1764.</span></div>
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<span style="color: #274e13;">Tem <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 3,3, sendo possível observá-lo a <a href="http://pt.wikipedia.org/wiki/Olho_nu" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Olho nu">olho nu</a> sob boas condições de visualização. Suas estrelas mais brilhantes podem ser visualizadas com o auxílio de <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Binóculo">binóculos</a> ou pequenos <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Telescópio">telescópios</a>. Situa-se 800 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Terra">Terra</a> e sua idade foi estimada em 220 milhões de anos. Na <a href="http://pt.wikipedia.org/wiki/Esfera_celeste" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Esfera celeste">esfera celeste</a>, situa-se logo a norte da ponta da "cauda" da constelação de <a href="http://pt.wikipedia.org/wiki/Scorpius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Scorpius">Escorpião</a>.</span></div>
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<img alt="Scorpius constellation map.png" src="http://upload.wikimedia.org/wikipedia/commons/thumb/5/52/Scorpius_constellation_map.png/250px-Scorpius_constellation_map.png" height="640" width="640" /></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Aglomerado_de_Ptolomeu#mediaviewer/Ficheiro:Open-cluster-Messier-7.jpeg</span></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%; overflow: hidden; text-overflow: ellipsis;"><span style="color: #274e13;">Open-cluster-Messier-7</span></span></div>
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<span style="color: #274e13;"><span class="mw-mmv-author" original-title="Autor">Oliver Stein</span> - <span class="mw-mmv-source" original-title="Fonte"><a class="external text" href="http://www.estelar.de/" rel="nofollow" style="background: none; text-decoration: none;">Homepage of Oliver Stein</a> <a class="external free" href="http://www.estelar.de/deepsky/kb_300_800mm/m7.htm" rel="nofollow" style="background: none;">http://www.estelar.de/deepsky/kb_300_800mm/m7.htm</a></span></span></div>
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<span style="background-color: white; font-family: Helvetica, sans-serif; font-size: 18px; font-weight: bold; line-height: 20px; text-align: start;"><span style="color: #073763;">In the Blackest Night, a Green Ring Nebula</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjaeUfGCGnsc0Dq22xD9ffNgF_nisr5yx1ctokkRso7NbyCFtjPbU7jXcdaVBBMt6p_2FPo4JWDfXZZ3AbVj-JxwRj0HJ3mg0eTb5XnwuB3DVRgEpUR9IhaQ6SdYAIlX14e8QpDgeUuYTo/s1600/green+ring.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjaeUfGCGnsc0Dq22xD9ffNgF_nisr5yx1ctokkRso7NbyCFtjPbU7jXcdaVBBMt6p_2FPo4JWDfXZZ3AbVj-JxwRj0HJ3mg0eTb5XnwuB3DVRgEpUR9IhaQ6SdYAIlX14e8QpDgeUuYTo/s1600/green+ring.jpg" height="640" width="640" /></a></div>
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<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="line-height: 22.399999618530273px;">http://www.spitzer.caltech.edu/images/3647</span></span></div>
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<dd property="photoshop:Credit" style="font-family: Helvetica, sans-serif; line-height: 12px; margin: 0px; padding: 2px 0px 0px 5px;"><span style="background-color: white;"><span style="color: #274e13;">NASA/JPL-Caltech/GLIMPSE-MIPSGAL Teams</span></span></dd><br />
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<span style="background-color: white;"><span style="color: #274e13;">Named <b><span style="font-size: large;">RCW 120</span></b>, this region of hot gas and glowing dust can be found in the murky clouds encircled by the tail of the constellation Scorpius. The ring of dust is actually glowing in infrared colors that our eyes cannot see, but show up brightly when viewed by Spitzer's infrared detectors. At the center of this ring are a couple of giant stars whose intense ultraviolet light has carved out the bubble, though they blend in with other stars when viewed in infrared.</span></span></div>
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<span style="background-color: white;"><span style="color: #274e13;">The green ring is where dust is being hit by winds and intense light from the massive stars. The green color represents infrared light coming from tiny dust grains called polycyclic aromatic hydrocarbons. These small grains have been destroyed inside the bubble. The red color inside the ring shows slightly larger, hotter dust gr</span><span style="color: #073763;">ains, heated by the massive stars.</span></span></div>
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<span style="color: #274e13;"><b>RCW 120</b> is an <a href="http://en.wikipedia.org/wiki/H_II_region" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="H II region">H II</a> <a href="http://en.wikipedia.org/wiki/Emission_nebula" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Emission nebula">emission nebula</a> in the southern Milky Way and located some 4,300 light-years from Earth. <sup class="reference" id="cite_ref-1" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/RCW_120#cite_note-1" style="background: none; text-decoration: none; white-space: nowrap;">[1]</a></sup><sup class="reference" id="cite_ref-2" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/RCW_120#cite_note-2" style="background: none; text-decoration: none; white-space: nowrap;">[2]</a></sup> Also known as <a href="http://en.wikipedia.org/wiki/Sharpless_catalog" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Sharpless catalog">Sh 2-3</a> and <a href="http://en.wikipedia.org/wiki/Gum_catalog" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Gum catalog">Gum 58</a>, it is situated at Galactic coordinates <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Galactic_longitude" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Galactic longitude">348.25°</a>, <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Galactic_latitude" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Galactic latitude">0.49°</a>.</span></div>
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<span style="color: #274e13;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=Veta_S._Avedisova&action=edit&redlink=1" style="background: none; text-decoration: none;" title="Veta S. Avedisova (page does not exist)">Veta S. Avedisova</a> states that RCW 120 is ionised by the O8 V star <a class="external text" href="http://simbad.u-strasbg.fr/simbad/sim-id?Ident=%402344615&Name=CD-38%2011636" rel="nofollow">CD -38 11636</a> and the B2 V star <a class="external text" href="http://simbad.u-strasbg.fr/simbad/sim-id?Ident=%402330221&Name=VdBH%2084%20B" rel="nofollow">VDBH 84B</a>, and places the nebula in the star formation region<a class="external text" href="http://galaxymap.org/avedisova/html/2932.html" rel="nofollow">SFR 348.26+0.47</a> along with 3 <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Masers" style="background: none; text-decoration: none;" title="Masers">masers</a> and the radio <a class="mw-redirect" href="http://en.wikipedia.org/wiki/HII_region" style="background: none; text-decoration: none;" title="HII region">HII region</a> CH87 347.386+0.266.</span></div>
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<span style="color: #274e13;">The <a href="http://en.wikipedia.org/wiki/Herschel_Space_Observatory" style="background: none; text-decoration: none;" title="Herschel Space Observatory">Herschel infra-red telescope</a>'s image shows an embryonic star not yet sparked by fusion which is likely to become one of the brightest stars in our Galaxy at some time within the next few hundred thousand years. It is already about ten times more massive than the Sun and is set to grow much larger by <a href="http://en.wikipedia.org/wiki/Accretion_(astrophysics)" style="background: none; text-decoration: none;" title="Accretion (astrophysics)">accreting</a> surrounding gas and dust. Current theories of star formation cannot explain star masses greater than about 10 times that of the Sun, even though stars having a mass of 120 Suns are known.<sup class="reference" id="cite_ref-3" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/RCW_120#cite_note-3" style="background: none; text-decoration: none; white-space: nowrap;">[3]</a></sup></span></div>
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<span style="color: #274e13;">The <a href="http://en.wikipedia.org/wiki/RCW_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="RCW Catalogue">RCW Catalogue</a>, first published in 1960, is named after Alexander William <b>R</b>odgers, Colin T. <b>C</b>ampbell and John Bolton <b>W</b>hiteoak, who led by <a href="http://en.wikipedia.org/wiki/Bart_Bok" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Bart Bok">Bart Bok</a>, catalogued southern nebulae while working at the <a href="http://en.wikipedia.org/wiki/Mount_Stromlo_Observatory" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Mount Stromlo Observatory">Mount Stromlo Observatory</a> in Australia.</span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.399999618530273px;"><a href="http://en.wikipedia.org/wiki/RCW_120">http://en.wikipedia.org/wiki/RCW_120</a></span></span></div>
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<span style="color: #252525; font-family: sans-serif;">LEIA MAIS ACESSANDO</span></div>
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Image of RCW 120 Nebula Shows Expanding Bubble of Ionized Gas</h1>
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<span style="color: #252525; font-family: sans-serif;"><a href="http://scitechdaily.com/image-of-rcw-120-nebula-shows-expanding-bubble-of-ionized-gas/">http://scitechdaily.com/image-of-rcw-120-nebula-shows-expanding-bubble-of-ionized-gas/</a></span></div>
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<a class="entry-title" href="http://annesastronomynews.com/annes-image-of-the-day-emission-nebula-rcw-120/" rel="bookmark" style="border: 0px; color: #ededed; margin: 0px; outline: 0px; padding: 0px; text-decoration: none;" title="Anne’s Image of the Day: Emission Nebula RCW 120">Emission Nebula RCW 120</a></h1>
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<span style="color: #252525; font-family: sans-serif;"><a href="http://annesastronomynews.com/annes-image-of-the-day-emission-nebula-rcw-120/">http://annesastronomynews.com/annes-image-of-the-day-emission-nebula-rcw-120/</a></span></div>
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Star formation around RCW 120, the perfect bubble</h1>
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The Galactic HII Region RCW 120</h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;"><span style="font-size: large;">Scorpius X-1</span> - Fonte de Emissão de Raio-X - Estrela Dupla</span></b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta é considerada a mais forte fonte de emissão de raio-x no céu. Este objeto é uma estrela binária, com um dos componentes sendo aparentemente uma estrela de nêutrons de rápida rotação. A radiação de raio-x ocorre durante a transferência de massa (transferência de plasma extremamente quente) da estrela comum para a estrela de nêutrons.<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;"> 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="color: #274e13; font-family: Arial, sans-serif; font-size: 11pt; line-height: 22.399999618530273px; text-align: justify;">Editora Vozes, Petrópolis, ano de 1986</span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> </span></div>
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<span style="color: #274e13;"><b style="font-family: sans-serif; line-height: 22.399999618530273px;"><a href="http://en.wikipedia.org/wiki/Scorpius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Scorpius">Scorpius</a> X-1</b><span style="font-family: sans-serif; line-height: 22.399999618530273px;"> is an </span><a href="http://en.wikipedia.org/wiki/X-ray" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="X-ray">X-ray</a><span style="font-family: sans-serif; line-height: 22.399999618530273px;"> source located roughly 9000 </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Light_year" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Light year">light years</a><span style="font-family: sans-serif; line-height: 22.399999618530273px;"> away in the constellation </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Scorpius_(constellation)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Scorpius (constellation)">Scorpius</a><span style="font-family: sans-serif; line-height: 22.399999618530273px;">. Scorpius X-1 was the first extrasolar X-ray source discovered, and, aside from the </span><a href="http://en.wikipedia.org/wiki/Sun" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Sun">Sun</a><span style="font-family: sans-serif; line-height: 22.399999618530273px;">, it is the strongest apparent source of X-rays in the </span><a href="http://en.wikipedia.org/wiki/Sky" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Sky">sky</a><span style="font-family: sans-serif; line-height: 22.399999618530273px;">.</span><sup class="reference" id="cite_ref-3" style="font-family: sans-serif; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Scorpius_X-1#cite_note-3" style="background: none; text-decoration: none; white-space: nowrap;">[3]</a></sup><span style="font-family: sans-serif; line-height: 22.399999618530273px;"> The X-ray </span><a href="http://en.wikipedia.org/wiki/Flux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; line-height: 22.399999618530273px;" title="Flux">flux</a><span style="font-family: sans-serif; line-height: 22.399999618530273px;"> varies day-to-day, and is associated with an </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Visible_light" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Visible light">optically</a><span style="font-family: sans-serif; line-height: 22.399999618530273px;"> visible </span><a href="http://en.wikipedia.org/wiki/Star" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Star">star</a><span style="font-family: sans-serif; line-height: 22.399999618530273px;">, V818 Scorpii, that has an </span><a href="http://en.wikipedia.org/wiki/Apparent_magnitude" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Apparent magnitude">apparent magnitude</a><span style="font-family: sans-serif; line-height: 22.399999618530273px;"> which fluctuates between 12-13.</span><sup class="reference" id="cite_ref-shklovskii_4-0" style="font-family: sans-serif; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Scorpius_X-1#cite_note-shklovskii-4" style="background: none; text-decoration: none; white-space: nowrap;">[4]</a></sup></span></div>
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<span class="mw-headline" id="Characteristics"><span style="color: #274e13;">Characteristics</span></span></h2>
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<span style="color: #274e13;">Its X-ray output is 2.3×10<sup style="line-height: 1;">31</sup> <a href="http://en.wikipedia.org/wiki/Watt" style="background: none; text-decoration: none;" title="Watt">W</a>, about 60,000 times the total luminosity of the Sun.<sup class="reference" id="cite_ref-par_2-1" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Scorpius_X-1#cite_note-par-2" style="background: none; text-decoration: none; white-space: nowrap;">[2]</a></sup> Scorpius X-1 shows regular variations of up to 1 <a href="http://en.wikipedia.org/wiki/Apparent_magnitude" style="background: none; text-decoration: none;" title="Apparent magnitude">magnitude</a> in its intensity, with a period of around 18.9 hours. The source varies irregularly in optical <a href="http://en.wikipedia.org/wiki/Wavelength" style="background: none; text-decoration: none;" title="Wavelength">wavelengths</a> as well, but these changes are not correlated with the X-ray variations.<sup class="reference" id="cite_ref-shklovskii_4-2" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Scorpius_X-1#cite_note-shklovskii-4" style="background: none; text-decoration: none; white-space: nowrap;">[4]</a></sup> Scorpius X-1 itself is a <a href="http://en.wikipedia.org/wiki/Neutron_star" style="background: none; text-decoration: none;" title="Neutron star">neutron star</a> whose intense gravity draws material off this companion into an <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Accretion_disk" style="background: none; text-decoration: none;" title="Accretion disk">accretion disk</a>, where it ultimately falls onto the surface, releasing a tremendous amount of energy. As this stellar material accelerates in Scorpius X-1's gravitational field, X-rays are emitted. The measured luminosity for Scorpius X-1 is consistent with a neutron star which is accreting matter at its <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Eddington_limit" style="background: none; text-decoration: none;" title="Eddington limit">Eddington limit</a>.<sup class="reference" id="cite_ref-par_2-2" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Scorpius_X-1#cite_note-par-2" style="background: none; text-decoration: none; white-space: nowrap;">[2]</a></sup></span></div>
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<span style="color: #274e13;">This system is classified as a <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Low-mass_X-ray_binary" style="background: none; text-decoration: none;" title="Low-mass X-ray binary">low-mass X-ray binary</a>; the neutron star is roughly 1.4 <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Solar_masses" style="background: none; text-decoration: none;" title="Solar masses">solar masses</a>, while the donor star is only 0.42 solar masses.<sup class="reference" id="cite_ref-10" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Scorpius_X-1#cite_note-10" style="background: none; text-decoration: none; white-space: nowrap;">[10]</a></sup> The two stars were probably not born together; recent research suggests that the binary may have been formed by a close encounter inside a <a href="http://en.wikipedia.org/wiki/Globular_cluster" style="background: none; text-decoration: none;" title="Globular cluster">globular cluster</a>.<sup class="reference" id="cite_ref-11" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Scorpius_X-1#cite_note-11" style="background: none; text-decoration: none; white-space: nowrap;">[11]</a></sup></span></div>
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<span style="color: #274e13;"><b style="background: transparent; border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;">Scorpius X-1</b><b style="background: transparent; border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;">,</b> (catalog number Sco X-1), brightest <a href="http://www.britannica.com/EBchecked/topic/650478/X-ray-source" style="background: transparent; font-style: inherit; margin: 0px; outline: none !important; padding: 0px; text-decoration: none; vertical-align: baseline;"><span href="http://semantic.britannica.com/accepted_headword/core/650478/X-ray-source" property="about" style="background: transparent; border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;">X-ray source</span></a> in the sky, the first such object discovered in the direction of the <a href="http://www.britannica.com/EBchecked/topic/134125/constellation" style="background: transparent; font-style: inherit; margin: 0px; outline: none !important; padding: 0px; text-decoration: none; vertical-align: baseline;"><span href="http://semantic.britannica.com/accepted_headword/core/134125/constellation" property="about" style="background: transparent; border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;">constellation</span></a> <a href="http://www.britannica.com/EBchecked/topic/529385/Scorpius" style="background: transparent; font-style: inherit; margin: 0px; outline: none !important; padding: 0px; text-decoration: none; vertical-align: baseline;"><span href="http://semantic.britannica.com/accepted_headword/core/529385/Scorpius" property="about" style="background: transparent; border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;">Scorpius</span></a>. Detected in 1962, its X-radiation is not only strong but, like other <a href="http://www.britannica.com/EBchecked/topic/650351/X-ray" style="background: transparent; font-style: inherit; margin: 0px; outline: none !important; padding: 0px; text-decoration: none; vertical-align: baseline;"><span href="http://semantic.britannica.com/accepted_headword/core/650351/X-ray" property="about" style="background: transparent; border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;">X-ray</span></a> sources, quite variable as well. Its variability exhibits two states, one at higher output with great variability on a time scale of minutes and another at lower output with the variability correspondingly lessened.</span></div>
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<span style="color: #274e13;">Scorpius X-1 was observed in visible light for the first time in 1966. Optically it is much less impressive, bluish in colour and appearing only faintly. Scorpius X-1 is a close <a href="http://www.britannica.com/EBchecked/topic/65567/binary-star" style="background-attachment: initial; background-clip: initial; background-color: transparent; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-style: inherit; margin: 0px; outline: none !important; padding: 0px; text-decoration: none; vertical-align: baseline;"><span href="http://semantic.britannica.com/accepted_headword/core/65567/binary-star" property="about" style="background: transparent; border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;">double star</span></a>, one component of which is optically invisible—a <a href="http://www.britannica.com/EBchecked/topic/410987/neutron-star" style="background-attachment: initial; background-clip: initial; background-color: transparent; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-style: inherit; margin: 0px; outline: none !important; padding: 0px; text-decoration: none; vertical-align: baseline;"><span href="http://semantic.britannica.com/accepted_headword/core/410987/neutron-star" property="about" style="background: transparent; border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;">neutron star</span></a>. The X-rays are generated when matter from the optically visible, bluish hot <a href="http://www.britannica.com/EBchecked/topic/563395/star" style="background-attachment: initial; background-clip: initial; background-color: transparent; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-style: inherit; margin: 0px; outline: none !important; padding: 0px; text-decoration: none; vertical-align: baseline;"><span href="http://semantic.britannica.com/accepted_headword/core/563395/star" property="about" style="background: transparent; border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;">star</span></a> falls onto the <a href="http://www.britannica.com/EBchecked/topic/410987/neutron-star" style="background-attachment: initial; background-clip: initial; background-color: transparent; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-style: inherit; margin: 0px; outline: none !important; padding: 0px; text-decoration: none; vertical-align: baseline;"><span href="http://semantic.britannica.com/accepted_headword/core/410987/neutron-star" property="about" style="background: transparent; border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;">neutron star</span></a>. This matter is tremendously accelerated and crushed by the enormous <a href="http://www.britannica.com/EBchecked/topic/242523/gravity" style="background-attachment: initial; background-clip: initial; background-color: transparent; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-style: inherit; margin: 0px; outline: none !important; padding: 0px; text-decoration: none; vertical-align: baseline;"><span href="http://semantic.britannica.com/accepted_headword/core/242523/gravity" property="about" style="background: transparent; border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;">gravity</span></a> of the neutron star. Unlike the majority of binary X-ray sources, the visible member does not appear to be very massive; it is only 42 percent the mass of the <a href="http://www.britannica.com/EBchecked/topic/573494/Sun" style="background-attachment: initial; background-clip: initial; background-color: transparent; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-style: inherit; margin: 0px; outline: none !important; padding: 0px; text-decoration: none; vertical-align: baseline;"><span href="http://semantic.britannica.com/accepted_headword/core/573494/Sun" property="about" style="background: transparent; border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;">Sun</span></a>. The neutron star is 1.4 solar masses. Scorpius X-1 is about 9,000 <a href="http://www.britannica.com/EBchecked/topic/340700/light-year" style="background-attachment: initial; background-clip: initial; background-color: transparent; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-style: inherit; margin: 0px; outline: none !important; padding: 0px; text-decoration: none; vertical-align: baseline;"><span href="http://semantic.britannica.com/accepted_headword/core/340700/light-year" property="about" style="background: transparent; border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;">light-years</span></a> from <a href="http://www.britannica.com/EBchecked/topic/175962/Earth" style="background-attachment: initial; background-clip: initial; background-color: transparent; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-style: inherit; margin: 0px; outline: none !important; padding: 0px; text-decoration: none; vertical-align: baseline;"><span href="http://semantic.britannica.com/accepted_headword/core/175962/Earth" property="about" style="background: transparent; border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;">Earth</span></a>.</span></div>
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<span style="color: #444444; font-family: Open Sans, sans-serif;"><span style="line-height: 22.399999618530273px;"><a href="http://www.britannica.com/EBchecked/topic/529390/Scorpius-X-1">http://www.britannica.com/EBchecked/topic/529390/Scorpius-X-1</a></span></span></div>
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<span style="font-family: verdana, arial, sans-serif; font-size: 11px; line-height: normal; text-align: start;"><span style="color: #274e13;">Trajectória possível, na Via Láctea, do microquasar Scorpius X-1 (linha a vermelho) comparada com a trajectória do Sol (linha a amarelo) num período de 230 milhões de anos, ou seja, o correspondente a uma rotação completa da Galáxia. Crédito: Mirabel & Rodrigues, NRAO/AUI/NSF. - See more at: http://www.portaldoastronomo.org/noticia.php?id=158#sthash.8gcKy39J.dpuf</span></span></div>
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<span style="color: #274e13;">Astrónomos reconstituem órbita de um microquasar em torno da Galáxia</span></h1>
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<span style="color: #274e13;">Scorpius X-1 é um sistema binário constituído por uma <a href="http://www.portaldoastronomo.org/noticia.php?id=158#" id="anchor1029" style="text-decoration: none;">estrela</a></span><br />
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<span style="color: #274e13;"> de <a href="http://www.portaldoastronomo.org/noticia.php?id=158#" id="anchor519" style="text-decoration: none;">neutrões</a></span><br />
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<span style="color: #274e13;">, muito densa, que arranca matéria a uma estrela normal, formando-se um disco que gira muito rapidamente em torno da <a href="http://www.portaldoastronomo.org/noticia.php?id=158#" id="anchor520" style="text-decoration: none;">estrela de neutrões</a></span><br />
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<span style="color: #274e13;">. O disco aquece ao ponto de emitir <a href="http://www.portaldoastronomo.org/noticia.php?id=158#" id="anchor855" style="text-decoration: none;">raios-X</a></span><br />
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<span style="color: #274e13;"> e produzir jactos de partículas subatómicas quase à <a href="http://www.portaldoastronomo.org/noticia.php?id=158#" id="anchor733" style="text-decoration: none;">velocidade da luz</a></span><br />
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<span style="color: #274e13;"> - uma combinação conhecida como microquasar.<br /><br />F. Mirabel (Instituto para a Astronomia e Física do Espaço da Argentina, e Comissão Francesa para a Energia Atómica) e I. Rodrigues (Comissão Francesa para a Energia Atómica) utilizaram observações publicadas para determinarem a trajectória de Scorpius X-1. Os cálculos, baseados em dados de posições muito precisas, obtidos com o radiotelescópio <em>Very Long Baseline Array</em> (<a href="http://www.portaldoastronomo.org/noticia.php?id=158#" id="anchor1073" style="text-decoration: none;">NRAO</a></span><br />
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<span style="color: #274e13;">, EUA) e com telescópios ópticos, permitem concluir que a estrela de neutrões e a sua companheira viajam juntas há pelo menos 30 milhões de anos. A <a href="http://www.portaldoastronomo.org/noticia.php?id=158#" id="anchor935" style="text-decoration: none;">órbita</a></span><br />
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<span style="color: #274e13;"> de Scorpius X-1 não se assemelha à maioria das outras estrelas que orbitam o centro da <a href="http://www.portaldoastronomo.org/noticia.php?id=158#" id="anchor495" style="text-decoration: none;">Galáxia</a></span><br />
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<span style="color: #274e13;">, pois segue um caminho excêntrico, que leva o microquasar bastante acima e abaixo do plano da Galáxia.<br /><br />Sobre o local de nascimento de Scorpius X-1, estes astrónomos só podem especular. Sendo as estrelas de neutrões o que resta de uma explosão de <a href="http://www.portaldoastronomo.org/noticia.php?id=158#" id="anchor766" style="text-decoration: none;">supernova</a></span><br />
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<span style="color: #274e13;"> de uma estrela de <a href="http://www.portaldoastronomo.org/noticia.php?id=158#" id="anchor466" style="text-decoration: none;">massa</a></span><br />
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<span style="color: #274e13;"> elevada, há duas possibilidades para a origem da progenitora da estrela de neutrões de Scorpius X-1: ou veio do <a href="http://www.portaldoastronomo.org/noticia.php?id=158#" id="anchor530" style="text-decoration: none;">bojo da Via Láctea</a></span><br />
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<span style="color: #274e13;">, ou de um enxame globular (aglomerados de milhões de estrelas que fazem parte do halo da nossa Galáxia e se encontram a uma considerável distância vertical do disco). Embora seja possível a hipótese da origem de Scorpius X-1 ser no bojo da Galáxia, é pouco provável que a progenitora da estrela de neutrões tenha levado um empurrão tão forte que a pusesse na presente órbita. Estes astrónomos preferem o cenário em que a estrela de neutrões capturou a sua companheira enquanto ainda se encontrava no enxame globular e no qual, após um encontro próximo com outras estrelas no centro do enxame, o par terá sido projectado para fora.<br /><br />Scorpius X-1 é a fonte contínua de raios-X mais brilhante fora do <a href="http://www.portaldoastronomo.org/noticia.php?id=158#" id="anchor715" style="text-decoration: none;">Sistema Solar</a></span><br />
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<span style="color: #274e13;">. Descoberto em 1962 por um telescópio de raios-X, este microquasar encontra-se a 9000 <a href="http://www.portaldoastronomo.org/noticia.php?id=158#" id="anchor424" style="text-decoration: none;">anos-luz</a></span><br />
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<span style="color: #274e13;"> de nós. A sua descoberta e os trabalhos que lhe estão associados contribuíram para a atribuição (repartida) do Prémio Nobel da Física de 2002 a Riccardo Giacconi.<br /><br />O presente estudo encontra-se publicado na revista da especialidade <em>Astronomy and Astrophysics,</em> de 30 de Janeiro de 2003. Os mesmos astrónomos publicaram, no ano passado, uma trajectória semelhante de um <a href="http://www.portaldoastronomo.org/noticia.php?id=158#" id="anchor74" style="text-decoration: none;">buraco negro</a></span><br />
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<span style="color: #274e13;"> e da sua estrela companheira. Também nesse ano, outro grupo de astrónomos produziu um filme mostrando os movimentos no jacto de matéria ejectada do disco à volta da estrela de neutrões de Scorpius X-1.<br /><br />Fonte da notícia: <a class="linkexterno" href="http://www.aoc.nrao.edu/epo/pr/2003/scox1/" style="background: url(http://www.portaldoastronomo.org/imagens/link_setacima.gif) 0px 2px no-repeat; padding-left: 12px; text-decoration: none;" target="_blank">http://www.aoc.nrao.edu/epo/pr/2003/scox1/ </a></span></div>
<span style="font-family: verdana, arial, sans-serif; line-height: normal; text-align: start;"><span style="color: #274e13;">- See more at: http://www.portaldoastronomo.org/noticia.php?id=158#sthash.8gcKy39J.dpuf</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra..., bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b><o:p></o:p></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>VISITE MINHA PÁGINA</b><o:p></o:p></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>DA TERRA AO CÉU E AO INFINITO</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #274e13;">http://daterraaoceueaoinfinito.blogspot.com.br/</span></b><o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">(com dedicatória do próprio autor para mim<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">em evento realizado no Museu de Astronomia do Rio de Janeiro,<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">em 16/06/1989)<o:p></o:p></span></div>
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<span lang="PT" style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">- </span><span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">Mario Jaci Monteiro</span><span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;"> , As Constelações, Cartas Celestes -<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC - com dedicatória do autor para mim, em março de 2004 (quando Mário Jaci generosamente me presenteou com um instrumento de observação (kepleriano) artesanalmente construído por ele).</span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-56858604885659262682013-08-20T08:16:00.001-07:002014-11-29T05:06:01.367-08:00SAGITTARIUS, O ARQUEIRO<div align="center" class="MsoNormal" style="text-align: center;">
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="font-size: small;">Da Terra ao Céu ....</span></span></a></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="font-size: small;">.....<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;">e ao Infinito </a></span></span></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><span style="font-size: small;">- As 88 Constelações</span></a></span></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;">http://daterraaoceueaoinfinito.blogspot.com.br/</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<img src="http://www.raremaps.com/maps/medium/36598.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></div>
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<a href="http://www.raremaps.com/gallery/detail/36598/La_Satittaire_Sagittarius/Flamsteed-Fortin.html" style="color: #274e13; text-decoration: none;">http://www.raremaps.com/gallery/detail/36598/La_Satittaire_Sagittarius/Flamsteed-Fortin.html</a></div>
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<strong>Title: </strong>La Satittaire (Sagittarius)</div>
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<strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1260" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; text-decoration: none;">John Flamsteed</a> / <a href="https://www.raremaps.com/gallery/browse/creator_id/1454" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; text-decoration: none;">MJ Fortin</a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">SAGITTARIUS, O ARQUEIRO</span></b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h41m / 20h15m Declinação -11<sup>o</sup>.8 / -45<sup>o</sup>.4<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Mito:</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Esta constelação representa o sábio e justo Centauro Quíron,</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> que se distinguia dos seus semelhantes, </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">que eram incultos e brutais, pela sua sabedoria.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tendo aprendido dos seus preceptores a arte divina da medicina e da caça,</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> teve como discípulos os Argonautas. </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">Imortal, num combate de Centauros e Paites, acidentalmente foi ferido no tornozelo </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">por uma flecha envenenada atirada por Hercules </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">quando da luta de ambos contra os demais centauros. </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> Como Quíron era um semideus, teria que viver eternamente</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> com aquela ferida que nunca era curada. </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">S</span><span style="font-family: Arial, Helvetica, sans-serif;">ofrendo de dores atrozes, ofereceu Quíron sua imortalidade a Prometeu. </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">Morto, foi colocado por Júpiter entre as estrelas.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Algumas Informações Interessantes acerca esta Constelação:</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Inscrições encontradas na Babilônia e nos monumentos persas mostram esse asterismo personificado como o deus arqueiro da guerra de Nergal.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">No Egito, era representado como um Centauro alado, galopando para o ocidente e trazendo um longo chapéu, com um arco esticado, a fim de arremessar uma flecha no corpo do escorpião.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">No tumulo de Ramsés VI é representado, unicamente, como um flecha.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Fronteiras:</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Sagittarius situa-se entre as constelações Corona Australis, Telescopium, Microscopium, Capricornius, Aquila, Scutum, Serpens, Ophiucus, Scorpius<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Observação a olho nu ou através binóculos e/ou telescópios:</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Quando olhamos para a constelação do Sagitário, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">estamos olhando diretamente em direção ao centro de nossa Galáxia, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">obscurecida por nuvens de estrelas e de material interestelar. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">É possível observar o núcleo da Galáxia, entretanto, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">através ondas infravermelhas ou de radio. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">O núcleo da Galáxia contém uma forte fonte de emissão de radio </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">designada como Sagitário A. <o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A constelação do Sagitário</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> contém muitos aglomerados estelares e nebulosas </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">que estão entre os objetos mais adoráveis em seus tipos.</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://www.iau.org/static/public/constellations/gif/SGR.gif</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Algumas Estrelas, em Sagitário:</b></span><br />
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<span style="font-family: Arial, sans-serif;"><b>Existe um Asterismo denominado de O Bule de Chá</b>, composto pelas estrelas<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Gamma, Epsilon, Delta, Lambda, Fi, Sigma, Tau e Zeta Sagittarii.<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Outro Asterismo, conhecido por Carro de Leite (ou Concha de Leite), Milk Dipper, é composto pelas estrelas Zeta, Gamma, Sigma, Fi e Lambda Sagittarii.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> http://www.stellarium.org/pt/</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></div>
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<span lang="PT" style="font-family: Arial, sans-serif;"><b>Rukbat ou Alrami - Alpha Saggitarius</b><o:p></o:p></span></div>
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<span lang="PT" style="font-family: Arial, sans-serif;">O Joelho do Arqueiro, nome árabe. </span><br />
<span lang="PT" style="font-family: Arial, sans-serif;">Esta estrela situa-se </span><span style="font-family: Arial, sans-serif;">aos pés do arqueiro. <o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;"><b>Arkab</b></span><span style="font-family: Arial, sans-serif;"><b> - Beta Sagittarii</b><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">O Tendão, variante de Urkab, do árabe Al Urkub. </span><br />
<span style="font-family: Arial, sans-serif;">Existem Arkab Prior e Arkab Posterior.<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;"><b>KausAustralis</b></span><span style="font-family: Arial, sans-serif;"><b> - Epsilon Sagittarii</b><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Ascensão Reta 18h22,9m - Declinação -34<sup>o</sup> 24’<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Magnitude visual 1,95 - Distância 124 anos-luz<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">O Sul do Arco, expressão árabe destinada a designar a região austral </span><br />
<span style="font-family: Arial, sans-serif;">do arco-e-flecha do Sagitário. </span><br />
<span style="font-family: Arial, sans-serif;">Esta é a estrela mais brilhante do Sagitário.<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;"><b>Kaus Borealis </b></span><span style="font-family: Arial, sans-serif;"><b>- Lambda Sagittarii</b><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Magnitude 2.8 Distância 71 anos-luz<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">O Norte do Arco. A região boreal do arco-e-flecha do Sagitário.<o:p></o:p></span></div>
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<span lang="PT" style="font-family: Arial, sans-serif;"><b>Delta Sagittarii - Kaus Meridionalis</b><o:p></o:p></span></div>
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<span lang="PT" style="font-family: Arial, sans-serif;">Magnitude 2.21 Distância 85 anos-luz<o:p></o:p></span></div>
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<span lang="PT" style="font-family: Arial, sans-serif;">Meio do Arco, expressão árabe.<o:p></o:p></span></div>
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<span lang="ES-TRAD" style="font-family: Arial, sans-serif;"><b>Pelagus</b></span><span lang="ES-TRAD" style="font-family: Arial, sans-serif;"><b>. Sigma Sagittarii. </b><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Uma pequena estrela situada na flecha da mão do Arqueiro.<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;"><b>Polis</b></span><span style="font-family: Arial, sans-serif;"><b>. Nu Sagittarii. </b><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Um estrela tripla na parte superior do bule, em Sagitário. De Coptic Polis, um potro.<o:p></o:p></span></div>
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<span lang="PT" style="font-family: Arial, sans-serif;"><b>Ascella</b></span><span lang="PT" style="font-family: Arial, sans-serif;"><b>. Zeta Sagittarii. </b><o:p></o:p></span></div>
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<span lang="PT" style="font-family: Arial, sans-serif;">Magnitude 2.61, terceira estrela mais brilhante do Sagitário.</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Uma estrela binária situada no braço do Sagitário.<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;"><b>Terebellum</b></span><span style="font-family: Arial, sans-serif;"><b>. Omega Sagittarii. </b><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">A estrela-chefe da cauda de quatro lados do Arqueiro.<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;"><b>Al Nash</b></span><span style="font-family: Arial, sans-serif;"><b> - Gamma Sagittarii</b><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Magnitude 2.97 Distância 124 anos-luz<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">A Ponta, vocábulo que designa a ponta da flecha.<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Nushaba</span><span style="font-family: Arial, sans-serif;"> - Gamma Sagittarii<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">A Flecha, nome árabe para designar a estrela que está situada na flecha do Arqueiro.<o:p></o:p></span></div>
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<span lang="EN-US" style="font-family: Arial, sans-serif;"><b>Nunki</b></span><span lang="EN-US" style="font-family: Arial, sans-serif;"><b> - Sigma Sagittarii</b><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Ascensão Reta 18h 54,0m - Declinação -26<sup>o</sup> 19’<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Magnitude visual 2,14 - Distância 300 anos-luz<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">O Peito do Arqueiro. Esta é a segunda estrela mais brilhante do Sagitário.<o:p></o:p></span></div>
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<span lang="ES-TRAD" style="font-family: Arial, sans-serif;"><b>Al Baldah</b></span><span lang="ES-TRAD" style="font-family: Arial, sans-serif;"><b> - Pi Sagittarii</b><o:p></o:p></span></div>
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<span lang="PT" style="font-family: Arial, sans-serif;">O Povoado, nome de origem árabe<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;"><b>X Sagittarii - Estrela Variável Cefeida</b><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Ascensão Reta 17h44m Declinação +27<sup>o</sup>.49<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Magnitudes: Max 4,3 Min 5,0 Período 7,0<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Tipo CEF Espectro F8v<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;"><b>W Sagittarii - Estrela Variável Cefeida</b><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Ascensão Reta 18h01m Declinação -29<sup>o</sup>.35<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Magnitudes: Max 4,8 Min 5,8 Período 7,6<o:p></o:p></span></div>
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<span lang="PT" style="font-family: Arial, sans-serif;">Tipo CEF Espectro G0v<o:p></o:p></span></div>
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<span lang="PT" style="font-family: Arial, sans-serif;"><b>Y Sagittarii - Estrela Variável Cefeida</b><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Ascensão Reta 18h18m Declinação 18<sup>o</sup>.53<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Magnitudes: Max 5,4 Min 5,6 Período 5,8<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Tipo CEF Espectro G0v<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span><span style="background-color: white;"><span style="color: #073763;"><br /></span></span><span style="background-color: white;"><img src="http://upload.wikimedia.org/wikipedia/commons/thumb/8/80/Sagittarius_constellation_map.png/800px-Sagittarius_constellation_map.png" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span><br />
<span style="background-color: white;"><span style="color: #073763;"><a href="http://pt.wikipedia.org/wiki/Sagittarius#mediaviewer/File:Sagittarius_constellation_map.png" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Sagittarius#mediaviewer/File:Sagittarius_constellation_map.png</a></span></span><br />
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>OBJETOS MESSIER</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>NA DIREÇÃO DA CONSTELAÇÃO SAGITTARIUS:</b></span></div>
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<span style="background-color: white;"><span style="color: #660000; font-family: Arial, sans-serif;"><b>Spiculum.</b></span><span style="font-family: Arial, sans-serif;"><b><span style="color: #660000;"> M8 e M20 e M21, Sagittarii. </span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;">Dois aglomerados (M8 e M21) e uma nebulosa</span><span style="font-family: Arial, sans-serif;"> (M20),<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">situados na cabeça da flecha do Arqueiro. </span></span><br />
<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;"> Por se situarem bem próximas à linha da Eclíptica, </span></span><br />
<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">sempre podemos observar os Planetas e a Lua passando por suas vizinhanças.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><b><span style="color: #660000;">NGC 6523 - M8 - Sagittarius - Nebulosa de Emissão HII - Lagoa</span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h02m Declinação -24<sup>o</sup>.23<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Tipo Nebulosa Planetária HII Dimensão 40,0 Magnitude 18<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Distância em anos-luz 4,5</span></span></div>
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<span lang="ES-TRAD" style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Tipo ND<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">NGC 6523 - M 8 - Aglomerado Aberto Sagitário<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h01 Declinação - 24<sup>o</sup>.23<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Magnitude fotográfica global 5,2 Magnitude fotográfica da mais brilhante estrela 7,0<o:p></o:p></span></span></div>
<span style="background-color: white; font-family: Arial, sans-serif;"><span style="color: #073763;"> Distância kpc 1,56 Diâmetro 45’ Tipo Espectral O5</span></span><br />
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">NGC 6523 = M8 - Nebulosa da Lagoa. <o:p></o:p></span></span></div>
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<span style="background-color: white; font-family: Arial, sans-serif;"><span style="color: #073763;">A oeste de Gama Sagittarii, Al Nash, encontraremos a Nebulosa da Lagoa e o Aglomerado aberto (M8) que podem ser vistos com visão enviesada ou através um bom par de binóculos e, melhor ainda, através telescópio.</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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A <b>Nebulosa Laguna</b> (Messier 8, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6523</a>) é uma gigantesca <a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa">nuvem interestelar</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagitário</a>. É classificada como uma <a href="http://pt.wikipedia.org/wiki/Nebulosa_de_emiss%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa de emissão">nebulosa de emissão</a>, cujos gases<a href="http://pt.wikipedia.org/wiki/%C3%8Don" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Íon">ionizados</a>, principalmente <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Hidrog%C3%AAnio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hidrogênio">hidrogênio</a>, emitem radiação principalmente no <a href="http://pt.wikipedia.org/wiki/Comprimento_de_onda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Comprimento de onda">comprimento de onda</a> na faixa da <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Luz_vis%C3%ADvel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Luz visível">luz visível</a> vermelha.</div>
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Vista de <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Binóculo">binóculos</a>, a nebulosa parece-se como uma mancha oval distinta com um núcleo definido. Sobreposta à nebulosa existe um pequeno <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto de estrelas</a>. Tem <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 6,0 e situa-se a 4 850 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>.</div>
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A nebulosa foi descoberta pelo astrônomo italiano <a href="http://pt.wikipedia.org/wiki/Giovanni_Battista_Hodierna" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Giovanni Battista Hodierna">Giovanni Battista Hodierna</a> antes de 1654. Foi classificada por ele como uma<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa">nebulosa</a> de brilho intermediário e listada como a entrada II.6 de seu catálogo. Foi redescoberta independemente por <a href="http://pt.wikipedia.org/wiki/John_Flamsteed" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="John Flamsteed">John Flamsteed</a> por volta de 1680, catalogado por ele como a entrada 2446 de seu catálogo. Flamsteed o classificou como um<a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado estelar">aglomerado estelar</a>, segundo Kenneth Glyn Jones, mas as coordenadas dadas por Flamsteed correpondem às dadas por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> referentes à própria nebulosa. De fato há um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> pouco a oeste da nebulosa, conhecida como <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/NGC_6530" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 6530">NGC 6530</a>.<span class="reference" id="cite_ref-seds_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_Laguna#cite_note-seds-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></div>
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Como uma <a href="http://pt.wikipedia.org/wiki/Nebulosa_de_emiss%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa de emissão">nebulosa de emissão</a>, Laguna apresenta uma cor rosácea em fotografias de longa exposição, embora pareça cinza ao<a href="http://pt.wikipedia.org/wiki/Olho_humano" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Olho humano">olho humano</a> em <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Binóculo">binóculos</a> ou pequenos <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a>, já que a distinção de cores não ocorre quando a luminosidade é escassa.<span class="reference" id="cite_ref-seds_3-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_Laguna#cite_note-seds-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></div>
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Foi vista novamente por <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a> em 1746, classificando-a como um aglomerado aberto. Anos mais tarde, foi observada por <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a>, que percebeu a nebulosa associada ao aglomerado. <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a> listou o <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objeto_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Objeto astronômico">objeto astronômico</a> em 1751 ou 1752 como a entrada Lac III.14 de seu catálogo. Em 23 de maio de 1764, Messier incluiu-o como a oitava entrada de seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catálogo</a>, descrevendo primeiramente o aglomerado e afirmando que a nebulosa estava em torno da estrela 9 Sagitarii.<span class="reference" id="cite_ref-seds_3-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_Laguna#cite_note-seds-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></div>
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<a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="William Herschel">William Herschel</a>, descobridor de <a href="http://pt.wikipedia.org/wiki/Urano_(planeta)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Urano (planeta)">Urano</a>, catalogou separadamente as duas partes da nebulosa Laguna (H V.9, GC 4363, <a href="http://pt.wikipedia.org/wiki/NGC_6526" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 6526">NGC 6526</a>; e H V.13, GC 4328, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/NGC_6533" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 6533">NGC 6533</a>), descrevendo que eram nebulosas grandes, mas fracas. Seu filho, <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="John Herschel">John Herschel</a>, catalogou o aglomerado aberto associado à nebulosa como a entrada h 3725 (GC 4366, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/NGC_6530" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 6530">NGC 6530</a>), e a própria nebulosa como a entrada h 3723 (GC 4361, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/NGC_6523" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 6523">NGC 6523</a>). Outra região nebulosa a leste do núcleo, ainda pertecente a nebulosa, tem a designação própria IC 4678.<span class="reference" id="cite_ref-seds_3-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_Laguna#cite_note-seds-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></div>
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LEIA MAIS</div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/a/a8/VST_images_the_Lagoon_Nebula.jpg/1024px-VST_images_the_Lagoon_Nebula.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /><br />
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="background-color: white; font-size: 1.2em; max-width: 60%;"><span style="color: #073763;"></span></span></div>
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<b>VEJA O VÍDEO</b></div>
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<b>DIVING INTO THE LAGOON NEBULA</b></div>
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<b>Mergulhando na Nebulosa Laguna</b></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/9/96/VISTA%27s_infrared_view_of_the_Lagoon_Nebula_%28Messier_8%29.jpg/1920px-VISTA%27s_infrared_view_of_the_Lagoon_Nebula_%28Messier_8%29.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></div>
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<span style="font-family: sans-serif;"><span style="line-height: 24px; white-space: nowrap;">http://pt.wikipedia.org/wiki/Nebulosa_Laguna<span style="background-color: white;"><span style="color: #073763;">#mediaviewer/Ficheiro:VISTA%27s_infrared_view_of_the_Lagoon_Nebula_(Messier_8).jpg</span></span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">VISTA's infrared view of the Lagoon Nebula (Messier 8)</span><a class="mw-mmv-license cc-license" href="http://creativecommons.org/licenses/by/3.0" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; font-size: 0.9em; padding: 0px 10px; text-align: right; text-decoration: none;" target="_blank">CC BY 3.0</a></span></span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span style="color: #073763;"><span class="mw-mmv-author">ESO/VVV</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.eso.org/public/images/eso1101a/" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;">http://www.eso.org/public/images/eso1101a/</a></span></span></span></div>
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<span style="background-color: white;">Messier 8 em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Infravermelho" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Infravermelho">infravermelho</a> (cores falsas), <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Observat%C3%B3rio_do_Paranal&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Observatório do Paranal (página não existe)">Observatório do Paranal</a></span></div>
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<span style="background-color: white;">This new infrared view of the star formation region Messier 8, often called the Lagoon Nebula, was captured by the VISTA telescope at ESO’s Paranal Observatory in Chile. This colour picture was created from images taken through J, H and Ks near-infrared filters, and which were acquired as part of a huge survey of the central parts of the Milky Way. The field of view is about 34 by 15 arcminutes.</span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h19m Declinação -16<sup>o</sup>.12<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Tipo Nebulosa Planetária HII Dimensão 20,0 Magnitude 19<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Distância em anos-luz 3,0</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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A <b>Nebulosa Ômega</b>, também conhecida como a <b>Nebulosa do Cisne</b> ou <b>Nebulosa da Ferradura</b> (Messier 17, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6618</a>) é uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Regi%C3%A3o_HII" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Região HII">região HII</a>, ou seja, uma região composta de gás estelar e poeira que recentemente começou a formar novas <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a>. A nebulosa está localizada na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagitário</a> e foi descoberta pelo astrônomo francês <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Philippe_Loys_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Philippe Loys de Chéseaux">Philippe Loys de Chéseaux</a> em 1745, e catalogada pelo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 1764 em seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catálogo</a> de objetos de aparência semelhante a<a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Cometa">cometas</a>. A nebulosa está localizada em uma região rica em estrelas, na região sagitariana da <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Via-Láctea">Via-Láctea</a>.</div>
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A Nebulosa Ômega está entre 5 000 a 6 000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> e mede cerca de 15 anos-luz de diâmetro. A nuvem de <a href="http://pt.wikipedia.org/wiki/Meio_interestelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Meio interestelar">matéria interestelar</a> onde a Nebulosa Ômega está contida tem cerca de 40 anos-luz de diâmetro. A <a href="http://pt.wikipedia.org/wiki/Massa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Massa">massa</a> total da nebulosa está estimada em 800 <a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Massa solar">massas solares</a>. Um <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado estelar aberto</a>, composto de 35 estrelas, está contida na nebulosa. Sua intensa radiação causa a diminuição do gás estelar em suas vizinhanças.</div>
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa">nebulosa</a> foi descoberta por <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a> em 1745 ou 1746. O astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> redescobriu-a independentemente em 3 de junho de 1764, listando-a em seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catálogo</a> como sua décima sétima entrada. É uma de apenas seis nebulosas verdadeiras pertencentes ao catálogo de Messier.<span class="reference" id="cite_ref-seds_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_%C3%94mega#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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É visível a <a href="http://pt.wikipedia.org/wiki/Olho_nu" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Olho nu">olho nu</a> em um <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Céu noturno">céu noturno</a> sob excelentes condições.<span class="reference" id="cite_ref-seds_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_%C3%94mega#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> A primeira tentativa de desenhar de modo apurado a nebulosa (como parte de uma série de esboços de nebulosas) foi feito pelo inglês <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="John Herschel">John Herschel</a> em 1833, e publicada em 1836. Ele descreveu a nebulosa como:</div>
<dl style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; margin-bottom: 0.5em; margin-top: 0.2em; text-align: start;"><dd style="line-height: 1.5em; margin-bottom: 0.1em; margin-left: 1.6em; margin-right: 0px;">"A figura desta nebulosa é quase aquela da letra maiúscula grega Omega (Ω), mas um pouco distorcida, embora a distribuição de brilho seja desigual. (...) [Charles] Messier percebeu apenas o brilhante braço leste da nebulosa, sem nenhuma das circunvoluções associadas, que foram notadas por meu pai. As peculariedades principais que eu tenho observado no sistema são: Um glóbulo visível na parte leste do braço brilhante da nebulosa, consideravelmente isolada da nebulosa circundante, sugerindo fortemente a ideia de uma absorção de matéria nebulosa, e outro glóbulo, mais pálido e menor do que o primeiro, na ponta noroeste do mesmo braço, onde a nebulosa faz uma súbita curva em um ângulo agudo."<span class="reference" id="cite_ref-psm1876_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_%C3%94mega#cite_note-psm1876-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></dd></dl>
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Um segundo e mais detalhado esboço foi feito por Herschel durante a sua visita à <a href="http://pt.wikipedia.org/wiki/%C3%81frica_do_Sul" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="África do Sul">África do Sul</a> em 1837. A nebulosa também foi estudada pelo alemão <a href="http://pt.wikipedia.org/wiki/Johann_von_Lamont" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Johann von Lamont">Johann von Lamont</a>, e separadamente por Sr. Mason, ainda em graduação no <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Yale_University" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Yale University">Yale College</a>. Quando Herschel publicou seu esboço de 1837 em 1847, escreveu:</div>
<dl style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; margin-bottom: 0.5em; margin-top: 0.2em; text-align: start;"><dd style="line-height: 1.5em; margin-bottom: 0.1em; margin-left: 1.6em; margin-right: 0px;">"Em particular, sobre o arco em forma de ferradura (...) foi representada como muito algongada em seu eixo vertical e com uma proporção muito maior do que o real tamanho do braço leste e do brilho da nebulosa. A difusão nebulosa na ponta [ocidental] daquele arco, formando o ângulo [ocidental] com a linha-base da letra maiúscula grega Ômega (Ω).......................................................................................</dd><dd style="line-height: 1.5em; margin-bottom: 0.1em; margin-left: 1.6em; margin-right: 0px;"><br /></dd><dd style="line-height: 1.5em; margin-bottom: 0.1em; margin-left: 1.6em; margin-right: 0px;">LEIA MAIS</dd><dd style="line-height: 1.5em; margin-bottom: 0.1em; margin-left: 1.6em; margin-right: 0px;">EM</dd></dl>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span class="mw-mmv-author">ESO</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.eso.org/public/images/eso0030a/" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://www.eso.org/public/images/eso0030a/</a> (<a class="external text" href="http://www.eso.org/public/archives/images/original/eso0030a.jpg" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">direct link</a>)</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<b>Messier 18</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6613</a>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado aberto de estrelas</a> localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagitário</a>. Foi descoberto pelo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 1764, que incluiu em seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catálogo</a> de objetos com aparência semelhante a <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Cometa">cometas</a>.</div>
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Do ponto de vista da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>, Messier 18 está situado entre a <a href="http://pt.wikipedia.org/wiki/Nebulosa_%C3%94mega" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa Ômega">Nebulosa Ômega</a> (Messier 17) e da <a href="http://pt.wikipedia.org/wiki/Nuvem_Estelar_de_Sagit%C3%A1rio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nuvem Estelar de Sagitário">Nuvem Estelar de Sagitário</a> (Messier 24). Sua idade é estimada em 32 milhões de anos e está situada a cerca de 4 900 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> de distância.</div>
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LEIA MAIS </div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_18</span></span></div>
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<span style="background-color: white;"><span style="color: #073763;">http://pt.wikipedia.org/wiki/Messier_18#mediaviewer/Ficheiro:Messier18.jpg</span></span><br />
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><b><span style="color: #660000;">NGC 6514 - M 20 - Sagittarius - Nebulosa de Emissão HII - Trífida</span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h01m Declinação -23<sup>o</sup>.02<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Tipo Nebulosa Planetária HII Dimensão 15,0 Magnitude 19<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">M 20 - NGC 6514 - Sagittarius - Nebulosa Difusa<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h01m Declinação -23<sup>o</sup>.02<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Tipo ND<o:p></o:p></span></span><br />
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">M20 - NGC 6514 - A nebulosa Trifid<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">É uma nebulosa difusa e denominada de Trifid em função de sua divisão característica de partes brilhantes acentuadas por três bandas escuras. M20 é bem mais pálida e difícil de ser observada visualmente do que sua vizinha M8. No centro da nebulosa, o lugar onde as três bandas escuras se encontram, existe uma estrela sextupla. A coloração avermelhada é característica de nuvens de hidrogênio. As regiões azuis são preenchidas com partículas de poeria, as quais esfumaçam a luz das estrelas mais jovens e muito quentes.</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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A <b>Nebulosa Trífida</b> (Messier 20, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6514</a>) é uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Regi%C3%A3o_HII" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Região HII">região HII</a>, ou seja uma região composta de gás estelar e poeira onde recentemente, em termos astronômicos, começou formar novas estrelas. Está localizada na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagitário</a> e seu nome significa "dividido em três lóbulos". O objeto é uma combinação incomum de um <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado aberto de estrelas</a>, uma <a href="http://pt.wikipedia.org/wiki/Nebulosa_de_emiss%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa de emissão">nebulosa de emissão</a> (a parte inferior, vermelho, em imagens de telescópios amadores), uma <a href="http://pt.wikipedia.org/wiki/Nebulosa_de_reflex%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa de reflexão">nebulosa de reflexão</a> (a parte superior, azul, em telescópios amadores) e uma <a href="http://pt.wikipedia.org/wiki/Nebulosa_escura" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa escura">nebulosa escura</a> (aparentes "lacunas" na nebulosa de emissão, que causam a aparência trifurcarda, estes são também designados como Barnard 85).</div>
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Vista por um pequeno <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio">telescópio</a>, a nebulosa Trífida é um objeto brilhante e colorido, preferido pelos astrônomos amadores. Situa-se aproximadamente 5 200 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> e tem <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 6,3, sendo fracamente visível a <a href="http://pt.wikipedia.org/wiki/Olho_nu" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Olho nu">olho nu</a>, mesmo sob excelentes condições de observação.</div>
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa">nebulosa</a> foi descoberta pelo astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 5 de junho de 1764, listando-o em seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catálogo</a> como sua vigésima entrada. Messier descreveu-o como um aglomerado contendo <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a> de <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 9 a 8, embebidas em uma aparente nebulosidade.<span class="reference" id="cite_ref-seds_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_Tr%C3%ADfida#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Famosa por exibir três ou quatro lóbulos aparentes, a nebulosa confundiu <a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="William Herschel">William Herschel</a>, descobridor de <a href="http://pt.wikipedia.org/wiki/Urano_(planeta)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Urano (planeta)">Urano</a>, que a catalogou como quatro nebulosas separadas; Herschel, em respeito ao trabalho de Messier, usualmente não atribuía sua própria nomenclatura aos objetos já nomeados por Messier.<span class="reference" id="cite_ref-seds_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_Tr%C3%ADfida#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Nebulosa_Tr%C3%ADfida</span></span></div>
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<span style="background-color: white;"><span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Hs-1999-42-a-full jpg</span><a class="mw-mmv-license" href="http://commons.wikimedia.org/wiki/File:Hs-1999-42-a-full_jpg.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-size: 0.9em; padding: 0px 10px; text-align: right; text-decoration: none;" target="">Domínio público</a></span></div>
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<span class="mw-mmv-source-author mw-mmv-reduce-toolong" original-title="Autor e informação sobre a fonte" style="background-color: white; font-size: 0.8em;"><span class="mw-mmv-author">NASA and Jeff Hester (Arizona State University)</span> - <span class="mw-mmv-source"><a class="external free" href="http://hubblesite.org/newscenter/archive/releases/1999/42/image/a" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://hubblesite.org/newscenter/archive/releases/1999/42/image/a</a> <a class="external free" href="http://mix.msfc.nasa.gov/abstracts.php?p=2761" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://mix.msfc.nasa.gov/abstracts.php?p=2761</a></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><b><span style="color: #660000;">M 21 - NGC 6531 - Sagittarius - Aglomerado Estelar Aberto </span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h03m Declinação -22<sup>o</sup>.30<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Magnitude visual integral 7,0 Tipo AA<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b>Messier 21</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6531</a>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado estelar aberto</a> localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagitário</a>. Foi descoberto pelo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 5 de junho de 1764.</div>
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Messier 21 é um aglomerado relativamente jovem de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a>, com meros 4,6 milhões de anos, e situa-se aproximadamente 4 250 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>. É altamente denso mas contém apenas 57 estrelas Algumas estrelas gigantes azuis foram identificadas no aglomerado, mas a maior parte de suas estrelas são pequenas. Com uma<a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 6,5, Messier 21 não é visível a <a href="http://pt.wikipedia.org/wiki/Olho_nu" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Olho nu">olho nu</a>, embora seja facilmente visível com bons <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Binóculo">binóculos</a> em noite com boas condições de visibilidade.</div>
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<span style="background-color: white;"><span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">M21</span></span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;">Original uploader was <a class="extiw" href="http://fr.wikipedia.org/wiki/User:Edmond_Wells" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="fr:User:Edmond Wells">Edmond Wells</a> </span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><b><span style="color: #660000;">M 22 - NGC 6656 - Sagittarius - Aglomerado Estelar Globular</span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h35m Declinação -23<sup>o</sup>.55<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Magnitude visual integral 5,2 Tipo AG<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">NGC 6656 - M 22 - Aglomerado Globular Sagitário<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h35m Declinação -23<sup>o</sup>.56<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Magnitude fotográfica global 6,2 Diâmetro aparente 26’,2 Tipo Espectral F7<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Magnitude média das 25 mais brilhantes estrelas (excluindo as 5 mais brilhantes) 13,73<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Número conhecido de Variáveis 24 Distância kpc 3,0<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Velocidade Radial (km/s) - 144<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;">Facies</span><span style="font-family: Arial, sans-serif;">. A Nebulosa na Face do Arqueiro. Aglomerado globular visível a olho nu, a meio caminho entre as estrelas Mu e Sigma Sagitarii. Situado a 27.000 anos-luz, constitui o mais extenso objeto deste tipo. Formado de mais de 50.000 estrelas de décima Magnitude visual, é um notável objeto quando observado ou através bons binóculos ou bons telescópios.</span></span><br />
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<span lang="PT" style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">M22 - NGC 6656 - Aglomerado Globular<o:p></o:p></span></span></div>
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<span lang="PT" style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Este é um dos mais brilhantes (e também um dos mais próximos) aglomerados globulares no céu, mais brilhante ainda do que M13, em Hercules.</span></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b>Messier 22</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6656</a>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> <a href="http://pt.wikipedia.org/wiki/Elipsoide" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Elipsoide">elipsoidal</a> de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a> localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagitário</a>, próximo à <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Bulbo_gal%C3%A1ctico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Bulbo galáctico">região central</a> da <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Via-Láctea">Via-Láctea</a> observado na abóbada celeste. Foi decoberto pelo astrônomo <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Johann_Abrahan_Ihle&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Johann Abrahan Ihle (página não existe)">Johann Abrahan Ihle</a> em 1665 enquanto observava a passagem de <a href="http://pt.wikipedia.org/wiki/Saturno_(planeta)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Saturno (planeta)">Saturno</a> pela constelação de Sagitário.</div>
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É um dos mais brilhantes aglomerados globulares visto no céu, com uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> igual a 5,1. Situa-se aproximadamente a 10 400 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> e contém mais de 70 000 estrelas.</div>
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<span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Situa-se apenas a 10 400 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> em relação à </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, um dos </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerados_globulares" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Aglomerados globulares">aglomerados globulares</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> mais próximos de nosso planeta. Seu diâmetro aparente, cerca de 32 </span><a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Minuto de arco">minutos de grau</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, ligeiramente maior do que o diâmetro aparente da </span><a href="http://pt.wikipedia.org/wiki/Fases_da_Lua" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Fases da Lua">Lua Cheia</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, corresponde a um diâmetro real de 97 anos-luz. A </span><a href="http://pt.wikipedia.org/wiki/Olho_nu" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Olho nu">olho nu</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, seu diâmetro aparente é de apenas 17 minutos e é o terceiro aglomerado globular mais brilhante do céu noturno, perdendo apenas para </span><a href="http://pt.wikipedia.org/wiki/Omega_Centauri" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Omega Centauri">Omega Centauri</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> (NGC 5139) e </span><a href="http://pt.wikipedia.org/wiki/47_Tucanae" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="47 Tucanae">47 Tucanae</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> (NGC 104). Está situada em frente ao</span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Bulbo_gal%C3%A1ctico" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Bulbo galáctico">bulbo galáctico</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> da </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Via-Láctea">Via-Láctea</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, tornando-o útl como uma </span><a href="http://pt.wikipedia.org/wiki/Lente_gravitacional" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Lente gravitacional">microlente gravitacional</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> nas estrelas localizadas no bulbo galáctico.</span><span class="reference" id="cite_ref-seds_5-2" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_22#cite_note-seds-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> </span><span class="reference" id="cite_ref-Gaudi2002_4-1" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_22#cite_note-Gaudi2002-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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<span style="background-color: white;"><span style="color: #073763;">http://pt.wikipedia.org/wiki/Messier_22</span></span></div>
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<span style="background-color: white;"><span style="color: #073763;">http://pt.wikipedia.org/wiki/Messier_22#mediaviewer/Ficheiro:Messier22.jpg</span></span><br />
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<span style="background-color: white;"><span style="color: #073763;">Núcleo de Messier 22, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><b><span style="color: #660000;">M 23 - NGC 6494 - Sagittarius - Aglomerado Estelar Aberto</span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 17h55 Declinação -19<sup>o</sup>.00<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Magnitude visual integral 6,0 Tipo AA<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">NGC 6494 - M 23 - Aglomerado Aberto Sagitário<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 17h55m Declinação - 19<sup>o</sup>.01<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Magnitude fotográfica global 5,9 Magnitude fotográfica da mais brilhante estrela 10,2</span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;"> Distância kpc 0,44 Diâmetro 27’ Tipo Espectral B8<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b>Messier 23</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6494</a>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado estelar aberto</a> localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagitário</a>. Foi descoberto pelo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 20 de junho de 1764.</div>
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Messier 23 está localizado a cerca de 2 150 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>, e mede entre 15 a 20 anos-luz de diâmetro. Foi identificado 150 estrelas pertencentes ao aglomerado, sendo que a estrela mais brilhante tem uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 9,2. Messier 23 pode ser encontrado com o uso de <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a> razoáveis entre as númerosas estrelas situadas no <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Bulbo_gal%C3%A1ctico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Bulbo galáctico">bulbo galáctico</a> da <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Via-Láctea">Via-Láctea</a>.</div>
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LEIA MAIS EM</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_23</span></span></div>
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<span style="background-color: white;"><span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Messier 023 2MASS</span><a class="mw-mmv-license" href="http://commons.wikimedia.org/wiki/File:Messier_023_2MASS.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-size: 0.9em; padding: 0px 10px; text-align: right; text-decoration: none;" target="">Domínio público</a></span></div>
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<span class="mw-mmv-source-author mw-mmv-reduce-toolong mw-mmv-truncate-toolong" original-title="Click to show full author and source" style="background-color: white; cursor: pointer; font-size: 0.8em;"><span class="mw-mmv-author">Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aerona</span>…</span></div>
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<span class="mw-mmv-source-author mw-mmv-reduce-toolong mw-mmv-truncate-toolong" original-title="Click to show full author and source" style="background-color: white; cursor: pointer; font-size: 0.8em;"><a class="external text" href="http://www.ipac.caltech.edu/2mass/gallery/messiercat.html" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: normal;">2MASS Atlas Image Gallery: The Messier Catalog</a></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><b><span style="color: #660000;">M 24 - NGC 6603 - Sagittarius - Aglomerado Estelar Aberto</span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h17m Declinação -18<sup>o</sup>.27<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">M24 - uma nuvem de estrelas na Via Láctea<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Esta nuvem pode ser observada a olho nú, localizada a cerca de 3 graus a leste do brilhante Aglomerado aberto M25 (IC 4725). Outro Aglomerado aberto muito belo é M23 (NGC 6494) localizado cerca de 5.5 graus a oeste de M24.</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">NGC 6603</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado estelar aberto</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Sagittarius">constelação de Sagittarius</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">. Foi descoberto pelo astrônomo inglês </span><a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="John Herschel">John Herschel</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> em 1830. Devido a sua moderada</span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> (+11,1), pode ser visto mesmo com pequenos </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> amadores ou equipamentos maiores. Está na mesma região da </span><a href="http://pt.wikipedia.org/wiki/Ab%C3%B3bada_celeste" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Abóbada celeste">abóbada celeste</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> que a </span><a href="http://pt.wikipedia.org/wiki/Nuvem_Estelar_de_Sagit%C3%A1rio" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Nuvem Estelar de Sagitário">Nuvem Estelar de Sagitário</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> (Messier 24) e historicamente é frequentemente confundido com a própria nuvem estelar.</span></div>
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<span style="background-color: white; line-height: 22.3999996185303px; text-align: start;"><span style="color: #252525; font-family: sans-serif;">http://pt.wikipedia.org/wiki/NGC_6603</span></span></div>
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<span style="background-color: white;"><span style="color: #073763;">http://en.wikipedia.org/wiki/NGC_6603#mediaviewer/File:Caustiche.jpg</span></span><br />
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><b><span style="color: #660000;">M 25 - IC 4725 - Sagittarius - Aglomerado Estelar Aberto</span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h30m Declinação - 19<sup>o</sup>.16<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">NGC I4725 - M 25 - Aglomerado Aberto Sagitário<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h30m Declinação - 19<sup>o</sup>.16<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Magnitude fotográfica global 6,2 Magnitude fotográfica da mais brilhante estrela 9,3<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<b>Messier 25</b> (<a href="http://pt.wikipedia.org/wiki/Index_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Index Catalogue">IC 4725</a>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado estelar aberto</a> localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagitário</a>. Foi descoberto pelo suíço <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a> em 1745, e foi incluído por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catálogo de objetos</a> de aparência semelhante a <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Cometa">cometas</a> em 1764.</div>
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Messier 25 está a uma distância de cerca de 2 000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>. Tem cerca de 19 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> de diâmetro. Uma <a href="http://pt.wikipedia.org/wiki/Estrela_vari%C3%A1vel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela variável">estrela variável</a> em brlho, tipo <a href="http://pt.wikipedia.org/wiki/Cefeida" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Cefeida">Delta Cephei</a>, designada como <i>U Sagittari</i>, é membro do aglomerado.</div>
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<span style="background-color: white;"><span style="color: #073763;">http://pt.wikipedia.org/wiki/Messier_25</span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span><img src="http://upload.wikimedia.org/wikipedia/commons/2/20/M25.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></div>
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<span style="background-color: #fbfbfb; color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start;">Messier 25, </span><a href="http://pt.wikipedia.org/wiki/NASA" style="background: none rgb(251, 251, 251); color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start; text-decoration: none;" title="NASA">NASA</a></div>
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<b><span style="color: #660000;">Messier 28</span></b><span style="color: #252525;"> (</span><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6626</a><span style="color: #252525;">), é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="color: #252525;"> na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a><span style="color: #252525;"> de </span><a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagitário</a><span style="color: #252525;">. Foi descoberto por </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="color: #252525;"> em </span><a href="http://pt.wikipedia.org/wiki/1764" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1764">1764</a><span style="color: #252525;">.</span></div>
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Situa-se a uma distância de aproximadamente 18 000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>.</div>
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LEIA MAIS EM</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_28</span></span></div>
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<span style="background-color: white; color: #073763;"><br /></span><span style="background-color: white; color: #073763;">http://pt.wikipedia.org/wiki/Messier_28#mediaviewer/Ficheiro:Messier_28_Hubble_WikiSky.jpg</span><br />
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<span style="background-color: white;"><span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Messier 28 Hubble WikiSky</span></span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span class="mw-mmv-author"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:NASA">en:NASA</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/STScI" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:STScI">en:STScI</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span> - <span class="mw-mmv-source"><a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a>'s snapshot tool - <a class="external autonumber" href="http://server1.sky-map.org/snapshot?img_size=&img_res=&ra=18.408648220844615&de=-24.870597658403195&angle=0.04141311201217398&projection=tan&rotation=42.09164940087089&survey=astrophoto&img_id=60565&width=1480&height=1480&img_borders=0&interpolation=bicubic2&jpeg_quality=0.95&max_preview_size=800&show_params=1&mouse_action=move" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">[1]</a></span></span></div>
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<span style="color: #660000;"><b>Messier 54</b> </span><span style="color: #252525;">(também conhecido como </span><b style="color: #252525;">M54</b><span style="color: #252525;"> ou </span><b style="color: #252525;">NGC 6715</b><span style="color: #252525;">) é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="color: #252525;"> na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a><span style="color: #252525;"> de </span><a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagittarius</a><span style="color: #252525;">. Foi descoberto por </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="color: #252525;"> em 1778 e subsequentemente incluído no seu catálogo de </span><a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Cometa">cometas</a><span style="color: #252525;">.</span></div>
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Modernas estimativas colocam M54 a uma distância de cerca de 87.000 anos-luz, traduzindo-se em um verdadeiro raio de 150 anos-luz de diâmetro. É um dos mais densos globulares, sendo de classe III (I sendo a mais densa e XII a menos densa). Ele brilha com <a href="http://pt.wikipedia.org/wiki/Luminosidade" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Luminosidade">luminosidade</a> de cerca de 850.000 vezes a do <a href="http://pt.wikipedia.org/wiki/Sol" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sol">Sol</a> e tem uma <a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a>de -10,0.</div>
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M54 é facilmente encontrado no céu, estando perto da <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a> <a href="http://pt.wikipedia.org/wiki/Zeta_Sagittarii" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Zeta Sagittarii">ζ Sagittarii</a>. Porém, não resolúvel em estrelas individuais, mesmo com grandes <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a> amadores.</div>
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LEIA MAIS EM</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_54</span></span></div>
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<span style="background-color: white; color: #073763;">http://pt.wikipedia.org/wiki/Messier_54#mediaviewer/Ficheiro:Messier_54_Hubble_WikiSky.jpg</span><br />
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="background-color: white; font-size: 1.2em; max-width: 60%;">Messier 54 Hubble WikiSky</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span class="mw-mmv-author"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:NASA">en:NASA</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/STScI" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:STScI">en:STScI</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span> - <span class="mw-mmv-source"><a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a>'s snapshot tool - <a class="external autonumber" href="http://server1.sky-map.org/snapshot?img_size=&img_res=&ra=18.917612480529517&de=-30.47898345725825&angle=0.05961446135552157&projection=tan&rotation=3.5940140919059433&survey=astrophoto&img_id=60489&width=4280&height=4280&img_borders=0&interpolation=bicubic2&jpeg_quality=0.95&max_preview_size=800&show_params=1&mouse_action=move" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">[1]</a></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><b><span style="color: #660000;">NGC 6809 - M 55 - Aglomerado Globular Sagitário</span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 19h38m Declinação -30<sup>o</sup>.59<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Magnitude fotográfica global 6,7 Diâmetro aparente 21’,1 Tipo Espectral F5<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Magnitude média das 25 mais brilhantes estrelas (excluindo as 5 mais brilhantes) 13,68<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Número conhecido de Variáveis 6 Distância kpc 6,0<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Velocidade Radial (km/s) + 170<span style="font-size: 11pt;"><o:p></o:p></span></span></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Messier 55</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> (também conhecido como </span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">NGC 6809</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> ou </span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">M55</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">) é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> localizado na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Sagittarius">Sagittarius</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> a 17 300 </span><a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Ano-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> da </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">. Foi descoberto por </span><a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> em </span><a href="http://pt.wikipedia.org/wiki/1752" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="1752">1752</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">. Possui um raio de 50 anos-luz e uma dimensão aparente de 19 </span><a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Minuto de arco">minutos de arco</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">.</span><span class="reference" id="cite_ref-seds_2-4" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_55#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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<span style="color: #073763;"><span style="background-color: white;">LEIA MAIS EM</span></span></div>
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<span style="color: #073763;"><span style="background-color: white;">http://pt.wikipedia.org/wiki/Messier_55</span></span></div>
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<span style="color: #073763; font-weight: normal;"><span style="background-color: white;"><br /></span></span><span style="color: #073763; font-weight: normal;"><span style="background-color: white;">http://pt.wikipedia.org/wiki/Messier_55#mediaviewer/Ficheiro:M55.jpg</span></span><br />
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<span style="background-color: #fbfbfb; color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start;">Messier 55, </span><a href="http://pt.wikipedia.org/wiki/NASA" style="background: none rgb(251, 251, 251); color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start; text-decoration: none;" title="NASA">NASA</a></div>
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<b><span style="color: #660000;">Messier 69</span></b><span style="color: #252525;"> (também conhecida como </span><b style="color: #252525;">M69</b><span style="color: #252525;"> ou </span><b style="color: #252525;">NGC 6637</b><span style="color: #252525;">) é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="color: #252525;"> localizado na constelação de </span><a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagittarius</a><span style="color: #252525;">. Foi descoberto por </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="color: #252525;"> em </span><a href="http://pt.wikipedia.org/wiki/31_de_agosto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="31 de agosto">31 de agosto</a><span style="color: #252525;"> de </span><a href="http://pt.wikipedia.org/wiki/1780" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1780">1780</a><span style="color: #252525;">, na mesma noite em que ele descobriu a </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M70" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="M70">M70</a><span style="color: #252525;">.</span></div>
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M69 está a uma distância de cerca de 29,700 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> e tem um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Raio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Raio">raio</a> espacial de 42 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a>. Trata-se de um vizinho próximo do aglomerado globular <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M70" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="M70">M70</a>, 1.800 anos-luz separam os dois objetos, e ambos os pólos estão localizados perto do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Centro_gal%C3%A1ctico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Centro galáctico">centro galáctico</a>. É um dos <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerados_globulares" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerados globulares">aglomerados globulares</a> com miores índices de <a href="http://pt.wikipedia.org/wiki/Metalicidade" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Metalicidade">metalicidade</a>.<span class="reference" id="cite_ref-seds_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_69#cite_note-seds-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span><span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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LEIA MAIS EM</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_69</span></span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/2/23/Messier_69_Hubble_WikiSky.jpg/800px-Messier_69_Hubble_WikiSky.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_69#mediaviewer/Ficheiro:Messier_69_Hubble_WikiSky.jpg</span></span></div>
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<a class="extiw" href="http://en.wikipedia.org/wiki/Messier_69" style="background: none rgb(251, 251, 251); color: #0b0080; font-size: 16px; line-height: 24px; text-decoration: none;" title="en:Messier 69">en:Messier 69</a><span style="background-color: #fbfbfb; color: #555555; font-size: 16px; line-height: 24px;"> globular cluster by </span><a class="extiw" href="http://en.wikipedia.org/wiki/Hubble_Space_Telescope" style="background: none rgb(251, 251, 251); color: #0b0080; font-size: 16px; line-height: 24px; text-decoration: none;" title="en:Hubble Space Telescope">en:Hubble Space Telescope</a></div>
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<b><span style="color: #660000;">Messier 70</span></b><span style="color: #252525;"> (</span><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6681</a><span style="color: #252525;">) é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="color: #252525;"> localizado na constelação de </span><a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagittarius</a><span style="color: #252525;">. Foi descoberto por </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="color: #252525;"> em </span><a href="http://pt.wikipedia.org/wiki/31_de_agosto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="31 de agosto">31 de agosto</a><span style="color: #252525;"> de </span><a href="http://pt.wikipedia.org/wiki/1780" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1780">1780</a><span style="color: #252525;">, na mesma noite em que ele descobriu a </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M69" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="M69">M69</a><span style="color: #252525;">.</span></div>
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M70 está a uma distância de cerca de 29,300 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>. Trata-se de um vizinho próximo (~2 graus) do aglomerado globular <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M69" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="M69">M69</a>, 1.800 anos-luz separam os dois objetos, e ambos os pólos estão localizados perto do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Centro_gal%C3%A1ctico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Centro galáctico">centro galáctico</a>. Esta a meio caminho entre Épsilon e Zeta Sagittarius. São conhecidas apenas duas estrelas variavéis neste aglomerado.<span class="reference" id="cite_ref-seds_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_70#cite_note-seds-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></div>
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LEIA MAIS EM</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_70</span></span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/07/Messier70-HST-Potw1215a.jpg/640px-Messier70-HST-Potw1215a.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_70#mediaviewer/Ficheiro:Messier70-HST-Potw1215a.jpg</span></span></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="background-color: white; font-size: 1.2em; max-width: 60%;">Messier70-HST-Potw1215a</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span class="mw-mmv-author">ESA/Hubble & NASA</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.spacetelescope.org/images/potw1215a/" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://www.spacetelescope.org/images/potw1215a/</a></span></span></div>
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<span style="color: #660000;"><b>Messier 75</b> </span><span style="color: #252525;">(também conhecido como </span><b style="color: #252525;">M72</b><span style="color: #252525;"> ou </span><b style="color: #252525;">NGC 6864</b><span style="color: #252525;">) é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="color: #252525;"> localizado na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a><span style="color: #252525;"> de </span><a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagittarius</a><span style="color: #252525;"> a 67 500 </span><a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a><span style="color: #252525;"> da </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a><span style="color: #252525;">. Foi descoberto por </span><a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a><span style="color: #252525;"> em 1780.</span><span class="reference" id="cite_ref-seds_2-4" style="bottom: 1ex; color: #252525; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_75#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Possui um raio de 53 anos-luz e uma <a href="http://pt.wikipedia.org/wiki/Di%C3%A2metro_angular" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Diâmetro angular">dimensão aparente</a> de 6,6 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a>. É <a href="http://pt.wikipedia.org/wiki/Classe_de_Concentra%C3%A7%C3%A3o_de_Shapley%E2%80%93Sawyer" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Classe de Concentração de Shapley–Sawyer">classificado</a> como classe I, o que significa que é um dos aglomerados mais densos conhecidos. Sua <a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a> é -8,5, e é 180 000 vezes mais luminoso que o Sol.<span class="reference" id="cite_ref-seds_2-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_75#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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O <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> foi descoberto pelo astrônomo francês <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a> em 27 de agosto de 1780, sendo <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catalogado</a> pelo seu colega de observatório, <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a>, em 18 de outubro daquele ano. <a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="William Herschel">William Herschel</a>, descobridor de <a href="http://pt.wikipedia.org/wiki/Urano_(planeta)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Urano (planeta)">Urano</a>, foi o primeiro a resolver suas estrelas mais brilhantes.<span class="reference" id="cite_ref-seds_2-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_75#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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É um dos <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerados globulares</a> mais tênues do catálogo Messier, situando-se a uma distância de 67 500 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à<a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>, muito além do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea#N.C3.BAcleo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Via-Láctea">núcleo da Via-Láctea</a>, que está a uma distância de 47 600 anos-luz em relação ao aglomerado.<span class="reference" id="cite_ref-seds_2-7" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_75#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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LEIA MAIS EM</div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="background-color: #fbfbfb; color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start;">Messier 75 - Globular Cluster The image was produced by </span><a class="external text" href="http://wikisky.org/" rel="nofollow" style="background: none rgb(251, 251, 251); color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start; text-decoration: none;">WikiSky's</a><span style="background-color: #fbfbfb; color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start;"> image cut out tool out of DSS2 data. See </span><a class="external text" href="http://wikisky.org/wiki/Copyright_-_DSS2_images" rel="nofollow" style="background: none rgb(251, 251, 251); color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start; text-decoration: none;">Copyright notice</a><span style="background-color: #fbfbfb; color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start;">. Source url:</span><a class="external free" href="http://server1.wikisky.org/imgcut.jsp?survey=DSS2&img_id=all&angle=0.2&ra=20.101667&de=-21.91667&width=2000&height=2000" rel="nofollow" style="background: none rgb(251, 251, 251); color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start; text-decoration: none;">http://server1.wikisky.org/imgcut.jsp?survey=DSS2&img_id=all&angle=0.2&ra=20.101667&de=-21.91667&width=2000&height=2000</a></span></span></div>
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<span style="background-color: white; font-size: 16px;"><b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">O CORAÇÃO DA VIA LACTEA</span></b></span><span style="font-weight: normal;"><span style="background-color: white;"><span style="color: #073763;"><br /></span></span></span><br />
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<span style="background-color: white; font-family: Arial, sans-serif;"><span style="color: #073763;">O núcleo da Galáxia</span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">contém uma forte fonte de emissão de radio designada como Sagitário A.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;">Este lugar é próximo à Ascensão Reta 18h e à Declinação - 30<sup>o</sup>,</span></span><br />
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;"> na fronteira tripla entre as constelações do Ophiuco, do Escorpião e de Sagitário. </span></span><br />
<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;"> A estrela mais próxima para servir de referência é Gamma Sagittarii, Al Nash</span><span lang="PT" style="font-family: Arial, sans-serif;"><o:p></o:p></span></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span><br />
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<span style="background-color: white;"><b style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Sagittarius A*</b><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> (pronounced "Sagittarius A-star", standard abbreviation </span><b style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Sgr A*</b><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">) is a bright and very compact </span><a href="http://en.wikipedia.org/wiki/Astronomical_radio_source" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Astronomical radio source">astronomical radio source</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> at the </span><a href="http://en.wikipedia.org/wiki/Galactic_Center" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Galactic Center">center</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> of the </span><a href="http://en.wikipedia.org/wiki/Milky_Way" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Milky Way">Milky Way</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">galaxy, near the border of the constellations </span><a href="http://en.wikipedia.org/wiki/Sagittarius_(constellation)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Sagittarius (constellation)">Sagittarius</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> and </span><a href="http://en.wikipedia.org/wiki/Scorpius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Scorpius">Scorpius</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">. It is part of a larger astronomical feature known as </span><a href="http://en.wikipedia.org/wiki/Sagittarius_A" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Sagittarius A">Sagittarius A</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">. Sagittarius A* is believed to be the location of a </span><a href="http://en.wikipedia.org/wiki/Supermassive_black_hole" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Supermassive black hole">supermassive black hole</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">,</span><sup class="reference" id="cite_ref-5" style="color: #252525; font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Sagittarius_A*#cite_note-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[5]</a></sup><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> like those that are now generally accepted to be at the centers of most </span><a href="http://en.wikipedia.org/wiki/Spiral_galaxy" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Spiral galaxy">spiral</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> and </span><a href="http://en.wikipedia.org/wiki/Elliptical_galaxy" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Elliptical galaxy">elliptical galaxies</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">. Observations of the star </span><a href="http://en.wikipedia.org/wiki/S2_(star)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="S2 (star)">S2</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> in orbit around Sagittarius A* have been used to show the presence of, and produce data about, the Milky Way's central supermassive black hole, and have led to the conclusion that Sagittarius A* is the site of that black hole.</span><sup class="reference" id="cite_ref-Henderson_6-0" style="color: #252525; font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Sagittarius_A*#cite_note-Henderson-6" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[6]</a></sup></span></div>
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<span style="background-color: white;">LEIA MUITO MAIS</span></div>
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<span style="background-color: white;"><img alt="Supermassive black hole" src="http://www.nasa.gov/images/content/415459main_image_1559_946-710.jpg" /></span></div>
<span style="background-color: white; color: #073763;">http://www.nasa.gov/multimedia/imagegallery/image_feature_1559.html</span><br />
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<span style="color: #073763;"><i style="background-color: white; font-family: Arial; line-height: 16px; text-align: left;">Image Credit: NASA/CXC/MIT/F. Baganoff, R. Shcherbakov et al. </i></span></div>
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<span style="background-color: white; color: #073763; font-size: small;">Into the Heart of Darkness</span></h3>
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<span style="background-color: white;"><span style="color: #073763;">Astronomers have long known that the supermassive black hole at the center of the Milky Way Galaxy, known as Sagittarius A* (or Sgr A* for short), is a particularly poor eater. The fuel for this black hole comes from powerful winds blown off dozens of massive young stars that are concentrated nearby. These stars are located a relatively large distance away from Sgr A*, where the gravity of the black hole is weak, and so their high-velocity winds are difficult for the black hole to capture and swallow. Scientists have previously calculated that Sgr A* should consume only about 1 percent of the fuel carried in the winds.<br /><br />However, it now appears that Sgr A* consumes even less than expected -- ingesting only about one percent of that one percent. Why does it consume so little? The answer may be found in a new theoretical model developed using data from a very deep exposure made by NASA's Chandra X-ray Observatory. This model considers the flow of energy between two regions around the black hole: an inner region that is close to the so-called event horizon (the boundary beyond which even light cannot escape), and an outer region that includes the black hole's fuel source -- the young stars -- extending up to a million times farther out. Collisions between particles in the hot inner region transfer energy to particles in the cooler outer region via a process called conduction. This, in turn, provides additional outward pressure that makes nearly all of the gas in the outer region flow away from the black hole. The model appears to explain well the extended shape of hot gas detected around Sgr A* in X-rays as well as features seen in other wavelengths.</span></span></div>
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<span style="background-color: white; font-family: Arial; line-height: 16px;"><span style="color: #073763;">.......................................... LEIA MAIS EM </span></span><span style="line-height: 16px; text-align: center;"><span style="color: #073763; font-family: Arial;">http://www.nasa.gov/multimedia/imagegallery/image_feature_1559.html</span></span></div>
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2012 November 2<br /><a href="http://apod.nasa.gov/apod/image/1211/PIA16214nustar.jpg"><img alt="See Explanation. Clicking on the picture will download
the highest resolution version available." src="http://apod.nasa.gov/apod/image/1211/PIA16214nustar900.jpg" /></a></center>
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<b><span style="color: #660000; font-size: large;">The Black Hole in the Milky Way </span></b><br /><b>Image Credit: </b><a href="http://www.nasa.gov/">NASA</a>, JPL-Caltech, <a href="http://www.nustar.caltech.edu/">NuSTAR project</a></center>
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<b>Explanation: </b><a href="http://apod.nasa.gov/apod/ap081211.html">At the center of our Milky Way Galaxy</a>, a mere 27,000 light-years away, lies a black hole with 4 million times the mass of the Sun. Fondly known as Sagittarius A* (pronounced A-star), the Milky Way's black hole is <a href="http://apod.nasa.gov/apod/ap120702.html">fortunately</a> mild-mannered compared to the central black holes in <a href="http://apod.nasa.gov/apod/ap080110.html">distant active galaxies</a>, much more calmly consuming material around it. From time to time it does flare-up, though. An outburst lasting several hours is captured in <a href="http://www.nasa.gov/mission_pages/nustar/news/nustar20121023.html">this series of premier X-ray images</a> from the orbiting <a href="http://www.nustar.caltech.edu/about-nustar">Nuclear Spectroscopic Telescope Array</a> (NuSTAR). Launched last June 13, NuSTAR is the first to provide <a href="http://www.nustar.caltech.edu/for-astronomers">focused views</a> of the area surrounding Sgr A* at X-ray energies higher than those accessible to Chandra and XMM observatories. Spanning two days of NuSTAR observations, the flare sequence is illustrated in the panels at the far right. X-rays are generated in material heated to over 100 million degrees Celsius, accelerated to nearly the speed of light as it falls into the Miky Way's central black hole. <a href="http://www.nasa.gov/mission_pages/nustar/multimedia/pia16213.html">The main inset X-ray image</a> spans about 100 light-years. In it, the bright white region represents the hottest material closest to the black hole, while the pinkish cloud likely belongs to a nearby <a href="http://apod.nasa.gov/apod/ap060602.html">supernova remnant</a></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>http://apod.nasa.gov/apod/ap121102.html</b></span></div>
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2013 September 6<br /><a href="http://apod.nasa.gov/apod/image/1309/sgra_gasChandra.jpg"><img alt="See Explanation. Clicking on the picture will download
the highest resolution version available." src="http://apod.nasa.gov/apod/image/1309/sgra_gasChandra_900c.jpg" /></a></center>
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<b><span style="color: #660000; font-size: large;">The Quiet Sagittarius A* </span></b><br /><b>Credit:</b> X-ray - <a href="http://www.nasa.gov/">NASA</a> / <a href="http://chandra.harvard.edu/">CXC</a> / Q. Daniel Wang (UMASS) <a href="http://arxiv.org/abs/1307.5845">et al.</a>, IR - NASA/STScI</center>
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<b>Explanation:</b></div>
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<b> </b>Hot gas is hard to swallow. <a href="http://chandra.harvard.edu/photo/2013/sgra_gas/">At least that seems to be true</a> for the supermassive black hole <a href="http://apod.nasa.gov/apod/ap081211.html">at the center of our Milky Way Galaxy</a>. Known as source <a href="http://apod.nasa.gov/apod/ap121102.html">Sagittarius A*</a>, the Milky Way's black hole is <a href="http://chandra.harvard.edu/press/13_releases/press_082913.html">centered in this</a> infrared (red and yellow hues) and X-ray (blue) composite. Based on data from an <a href="http://www.sgra-star.com/">extensive campaign</a> of observations by the orbiting Chandra X-ray telescope, the diffuse emission surrounding the black hole is seen in the close-up inset, the inset field spanning about 1/2 light-year across the galactic center some 26,000 light-years away. Astronomers have found that the X-ray emission originates in hot gas drawn from the winds of massive young stars in the region. <a href="http://arxiv.org/abs/1307.5845">The Chandra data</a> indicate that only about 1% or less of the gas within the black hole's gravitational influence ever reaches the event horizon, losing enough heat and angular momentum to fall into the black hole, while the rest of the gas escapes in an outflow. <a href="http://chandra.harvard.edu/blog/node/452">The result explains</a> why the Milky Way's black hole is so quiet, much fainter than might be <a href="http://apod.nasa.gov/apod/ap020309.html">expected</a> in energetic X-rays. It likely holds for most supermassive black holes in galaxies in the nearby Universe.</div>
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<b><span style="color: #990000;">http://apod.nasa.gov/apod/ap130906.html</span></b></div>
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2008 December 11<br /><a href="http://apod.nasa.gov/apod/image/0812/mwcenter_eso.jpg"><img alt="See Explanation. Clicking on the picture will download
the highest resolution version available." src="http://apod.nasa.gov/apod/image/0812/mwcenter_eso_c800.jpg" /></a></center>
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<b><span style="color: #660000; font-size: large;">At the Center of the Milky Way </span></b><br /><b>Credit: </b><a href="http://www.eso.org/">ESO</a>, Stefan Gillessen (<a href="http://www.mpe.mpg.de/">MPE</a>), <a href="http://arxiv.org/abs/0810.4674">F. Eisenhauer, S. Trippe, T. Alexander, R. Genzel, F. Martins, T. Ott</a></center>
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<b>Explanation: </b></div>
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At the center of our Milky Way Galaxy lies a <a href="http://www.einstein-online.info/en/elementary/blackHoles/supermassive_bh/index.html">supermassive black hole</a>. Once a controversial claim, this conclusion is now solidly based <a href="http://www.eso.org/public/outreach/press-rel/pr-2008/pr-46-08.html">on 16 years of observations</a> that map the orbits of 28 stars very near <a href="http://www.einstein-online.info/en/spotlights/milkyway_bh/index.html">the galactic center</a>. Using European Southern Observatory <a href="http://apod.nasa.gov/apod/ap061104.html">telescopes</a> and sophisticated near infrared cameras, astronomers patiently measured the positions of the stars over time, following one star, designated S2, through a complete orbit as it came within about 1 <i>light-day</i> of the center of the Milky Way. <a href="http://arxiv.org/abs/0810.4674v1">Their results</a> convincingly show that S2 is moving under the influence of the enormous gravity of a compact, unseen object -- a black hole with 4 million times the mass <a href="http://hypertextbook.com/facts/2000/LeonVaysburd.shtml">of the Sun</a>. Their ability to track stars so close to the <a href="http://www.mpe.mpg.de/www_ir/GC/index.html">galactic center</a> accurately measures the black hole's mass and also determines the distance to the center to be 27,000 light-years. This deep, near-infrared image shows the crowded inner 3 light-years of the central <a href="http://apod.nasa.gov/apod/ap080104.html">Milky Way</a>. Spectacular time-lapse animations of the stars orbiting within light-days of the galactic center <a href="http://www.eso.org/public/outreach/press-rel/pr-2008/phot-46-08.html">can be found here</a>.</div>
<div style="background-color: white; color: #073763; font-size: 16px; font-weight: normal;">
<b><span style="color: #660000;">http://apod.nasa.gov/apod/ap081211.html</span></b></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjWRTdksG9ihFpYZ1SOIS9hymzNjgrLPDjrPwEaDflJtZGGTceh2eT-h6JahLvyBMQXc69RNNfDNk1Fcfk4Vi5LklDzF8qbv83skYnRw3PdsNp2A4lSo2S0t0wsstpt3InoN-zcuSVmWaIc/s1600/14+-+1+(12).jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjWRTdksG9ihFpYZ1SOIS9hymzNjgrLPDjrPwEaDflJtZGGTceh2eT-h6JahLvyBMQXc69RNNfDNk1Fcfk4Vi5LklDzF8qbv83skYnRw3PdsNp2A4lSo2S0t0wsstpt3InoN-zcuSVmWaIc/s1600/14+-+1+(12).jpg" /></a></div>
<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><br />https://plus.google.com/102371865054310418159/posts/75YG8Jc3LHF?pid=6086892779814785362&oid=102371865054310418159</span><br />
<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #404040; font-family: Roboto, arial, sans-serif; line-height: 18.2000007629395px; text-align: start;">The center of the Milky Way galaxy, with the supermassive black hole Sagittarius A* (Sgr A*), located in the middle, is revealed in these images. Astronomers have used NASA’s Chandra X-ray Observatory to take a major step in understanding why material around Sgr A* is extraordinarily faint in X-rays.</span><br style="color: #404040; font-family: Roboto, arial, sans-serif; line-height: 18.2000007629395px; text-align: start;" /><br style="color: #404040; font-family: Roboto, arial, sans-serif; line-height: 18.2000007629395px; text-align: start;" /><span style="color: #404040; font-family: Roboto, arial, sans-serif; line-height: 18.2000007629395px; text-align: start;">The large image contains X-rays from Chandra in blue and infrared emission from the Hubble Space Telescope in red and yellow. The inset shows a close-up view of Sgr A* in X-rays only, covering a region half a light year wide. The diffuse X-ray emission is from hot gas captured by the black hole and being pulled inwards. This hot gas originates from winds produced by a disk-shaped distribution of young massive stars observed in infrared observations.</span><br style="color: #404040; font-family: Roboto, arial, sans-serif; line-height: 18.2000007629395px; text-align: start;" /><br style="color: #404040; font-family: Roboto, arial, sans-serif; line-height: 18.2000007629395px; text-align: start;" /><span style="color: #404040; font-family: Roboto, arial, sans-serif; line-height: 18.2000007629395px; text-align: start;">These new findings are the result of one of the biggest observing campaigns ever performed by Chandra. During 2012, Chandra collected about five weeks worth of observations to capture unprecedented X-ray images and energy signatures of multi-million degree gas swirling around Sgr A*, a black hole with about 4 million times the mass of the Sun. At just 26,000 light years from Earth, Sgr A* is one of very few black holes in the universe where we can actually witness the flow of matter nearby.</span><br style="color: #404040; font-family: Roboto, arial, sans-serif; line-height: 18.2000007629395px; text-align: start;" /><br style="color: #404040; font-family: Roboto, arial, sans-serif; line-height: 18.2000007629395px; text-align: start;" /><span style="color: #404040; font-family: Roboto, arial, sans-serif; line-height: 18.2000007629395px; text-align: start;">Image credit: X-ray: NASA/UMass/D.Wang et al., IR: NASA/STScI</span><span style="color: #660000; font-family: Arial, Helvetica, sans-serif; font-size: large; font-weight: normal;"><b><br /><br /><br /><br /><br /></b></span><span style="color: #660000; font-family: Arial, Helvetica, sans-serif; font-size: large; font-weight: normal;"><b>LEIA </b></span></div>
<div style="background-color: white; color: #073763; font-size: 16px; font-weight: normal;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">este esclarecedor Artigo escrito por Markus Pössel</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre</span></div>
<div style="background-color: white; color: #073763; font-size: 16px; font-weight: normal;">
<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Nosso próprio buraco negro</b></span></div>
<div style="background-color: white; color: #073763; font-size: 16px; font-weight: normal;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>http://www.einstein-online.info/spotlights/milkyway_bh/?set_language=en</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif; font-size: large;"><b><br /></b></span></div>
<h1 class="documentFirstHeading" style="background-color: #f4f4f1; border-bottom-color: rgb(160, 0, 0); border-bottom-style: dotted; border-bottom-width: 1px; color: #a00000; font-family: 'Lucida Grande', Lucida, Helvetica, Arial, Verdana, sans-serif; font-size: 19px; margin: 0px 0px 1em; text-align: center;">
<span class="" id="parent-fieldname-title">The dark heart of the Milky Way</span></h1>
<dl class="portlet toc" id="document-toc" style="background-color: white; border: 1px solid rgb(160, 0, 0); float: right; font-family: 'Lucida Grande', Lucida, Helvetica, Arial, Verdana, sans-serif; font-size: 11px; margin: 1px 0px 3em 1em; text-align: start; width: 184.15625px;">
<dt class="portletHeader" style="background-image: none; border-left-color: rgb(160, 0, 0); border-left-width: 1px; border-right-color: rgb(160, 0, 0); border-right-width: 1px; border-style: none; color: #333333; font-weight: bolder; line-height: 1.6em; margin-left: 0.8em; margin-top: 0.5em; padding-bottom: 0em; padding-left: 0px !important; padding-right: 1em; padding-top: 0em; text-align: center;">An article by</dt>
<dd class="portletItem-rel" style="background-image: url(http://www.einstein-online.info/eoicon_anchor.gif); background-position: 2px 4px; background-repeat: no-repeat; line-height: 1.5em; margin: 0.5em 0.25em 1.5em 0.5em; padding-left: 2em;"><a href="http://www.einstein-online.info/spotlights/milkyway_bh#author" style="background-color: transparent; border-bottom-color: rgb(204, 204, 204); border-bottom-style: solid; border-bottom-width: 1px; color: brown; display: inline-block; text-decoration: none;">Markus Pössel</a></dd>
<dt class="portletHeader" style="background-image: none; border-left-color: rgb(160, 0, 0); border-left-width: 1px; border-right-color: rgb(160, 0, 0); border-right-width: 1px; border-style: none; color: #333333; font-weight: bolder; line-height: 1.6em; margin-left: 0.8em; margin-top: 0.5em; padding-bottom: 0em; padding-left: 0px !important; padding-right: 1em; padding-top: 0em; text-align: center;">Contents</dt>
<dd class="portletItem" style="border-left-style: none; border-right-style: none; line-height: 1.5em; margin: 0px 0px 0px 1.5em; padding: 1em 1em 1em 0px;"><ol class="TOC1Digit" style="line-height: 1.5em; margin: 0px 0px 0px 1em; padding: 0px;">
<li style="margin-bottom: 0.5em; text-align: center;"><a href="http://www.einstein-online.info/spotlights/milkyway_bh/?set_language=en#section-0" style="background-image: none; background-position: initial initial; background-repeat: initial initial; border-bottom-style: none; color: #a00000; padding: 0px; text-decoration: none;">Our very own black hole</a></li>
<li style="margin-bottom: 0.5em; text-align: center;"><a href="http://www.einstein-online.info/spotlights/milkyway_bh/?set_language=en#section-1" style="background-image: none; background-position: initial initial; background-repeat: initial initial; border-bottom-style: none; color: #a00000; padding: 0px; text-decoration: none;">Stars orbiting the central black hole</a></li>
<li style="margin-bottom: 0.5em; text-align: center;"><a href="http://www.einstein-online.info/spotlights/milkyway_bh/?set_language=en#section-2" style="background-image: none; background-position: initial initial; background-repeat: initial initial; border-bottom-style: none; color: #a00000; padding: 0px; text-decoration: none;">Further Information</a></li>
</ol>
</dd></dl>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif; font-size: large;"><span style="line-height: 19.6000003814697px;"><b>ASSISTA AOS VÍDEOS: </b></span></span></div>
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<span style="line-height: 19.6000003814697px;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>https://www.youtube.com/watch?v=36xZsgZ0oSo</b></span></span></div>
<h1 class="yt" id="watch-headline-title" style="background-color: white; border: 0px; color: #222222; font-size: 16px; font-weight: normal; margin: 0px 0px 5px; overflow: hidden; padding: 0px; text-overflow: ellipsis; white-space: nowrap; word-wrap: normal;">
<span class="watch-title yt-uix-expander-head" dir="ltr" id="eow-title" style="-webkit-user-select: auto; border: 0px; color: black; cursor: auto; margin: 0px; padding: 0px;" title="Journey to the Galactic Center"><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;">Journey to the Galactic Center</span></span></h1>
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<span style="line-height: 17px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Credit: ESO</span></span></h1>
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<span style="line-height: 17px;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>https://www.youtube.com/watch?v=XhHUNvEKUY8</b></span></span></div>
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<h1 class="yt" id="watch-headline-title" style="border: 0px; margin: 0px 0px 5px; overflow: hidden; padding: 0px; text-overflow: ellipsis; white-space: nowrap; word-wrap: normal;">
<span class="watch-title long-title yt-uix-expander-head" dir="ltr" id="eow-title" style="-webkit-user-select: auto; border: 0px; cursor: pointer; letter-spacing: -0.03em; margin: 0px; padding: 0px;" title="ESO- Zooming in on the centre of the Milky Way. HD 720P"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">ESO- Zooming in on the centre of the Milky Way. HD 720P</span></span></h1>
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<span style="background-color: white; text-align: start;"><b><span style="line-height: 19.6000003814697px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Credit:ESO/MPE/Nick Risinger (skysurvey.org)/VISTA/J. Emerson/Digitized Sky Survey 2 Music: xxx</span></span></b></span></div>
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<span style="background-color: white; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 19.600000381469727px; text-align: start;"><span style="color: #660000; font-size: large;"><b><br /></b></span></span><span style="background-color: white; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 19.600000381469727px; text-align: start;"><span style="color: #660000; font-size: large;"><b><br /></b></span></span><span style="background-color: white; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 19.600000381469727px; text-align: start;"><span style="color: #660000; font-size: large;"><b><a href="http://www.eso.org/public/videos/eso-jcmw/">http://www.eso.org/public/videos/eso-jcmw/</a></b></span></span><br />
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<span style="font-size: large;">Journey to the Centre of the Milky Way Short Fulldome Planetarium Show</span></h1>
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What lies at the heart of our galaxy? For twenty years, ESO’s Very Large Telescope and the Keck telescopes have observed the centre of the Galaxy, looking at the motion of more than a hundred stars and identifying the position of an otherwise invisible object — the supermassive black hole at the centre of our galaxy. </div>
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Embark on a Journey to the Centre of the Milky Way and during seven minutes travel faster than light, from the driest place on Earth, the Atacama Desert in Chile right to the centre of our own galaxy, where a black hole is consuming anything that strays into its path. 84 million stars will appear in front of your eyes, each hiding mysteries waiting to be solved. Are there planets around them, perhaps with moons? Do they have water? Could they harbour life? </div>
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<em style="box-sizing: border-box;">Journey to the Centre of the Milky Way</em> is the first fulldome planetarium mini-show produced in-house by ESO for its Planetarium and Visitor Centre, the ESO Supernova, due to open in 2017. Available for free in 4k resolution, the mini-show can be downloaded and used by any planetarium in the world. </div>
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ESO</div>
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Directed by: Lars Lindberg Christensen</div>
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Art Direction, Production Design: Luis Calçada</div>
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Producer: Luis Calçada</div>
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Written by: Georgia Bladon & Lars Lindberg Christensen</div>
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Editing: Luis Calçada</div>
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Narration: Sara Mendes da Costa</div>
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Soundtrack & Sound Effects: Michael Stearns Sacred Site (<a href="http://www.michaelstearns.com/" style="background: transparent; box-sizing: border-box; color: #428bca; text-decoration: none;">michaelstearns.com</a>)</div>
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3D animations, footage and photos: Luis Calçada, Martin Kornmesser, Gas cloud simulation: ESO/S. Gillessen/MPE/Marc Schartmann, ALMA (ESO/NAOJ/NRAO), VISTA/J. Emerson, Digitized Sky Survey 2, N. Risinger (<a href="http://www.skysurvey.org/" style="background: transparent; box-sizing: border-box; color: #428bca; text-decoration: none;">skysurvey.org</a>), Stéphane Guisard (<a href="http://www.eso.org/~sguisard" style="background: transparent; box-sizing: border-box; color: #428bca; text-decoration: none;">eso.org/~sguisard</a>), Serge Brunier & B.Tafreshi (<a href="http://www.twanight.org/" style="background: transparent; box-sizing: border-box; color: #428bca; text-decoration: none;">twanight.org</a>)</div>
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Executive producer: Lars Lindberg Christensen.</div>
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<span style="color: #333333; font-family: Neue Helvetica W02, Neue Helvetica W10, Helvetica Neue, Helvetica, Arial, sans-serif;"><span style="font-size: 13px; line-height: 18.5714092254639px;"><a href="http://www.eso.org/public/videos/eso-jcmw/">http://www.eso.org/public/videos/eso-jcmw/</a></span></span></div>
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<span style="background-color: white; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 19.600000381469727px; text-align: start;"></span><span style="background-color: white; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 19.600000381469727px; text-align: start;"><span style="color: #660000; font-size: large;"><b><br /></b></span></span><span style="background-color: white; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 19.600000381469727px; text-align: start;"><span style="color: #660000; font-size: large;"><b>Um Passeio Virtual através o Céu Estrelado!</b></span></span></div>
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<span style="background-color: white; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 19.600000381469727px; text-align: start;"><span style="color: #660000; font-size: large;"><b><br /></b></span></span><span style="background-color: white; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 19.600000381469727px; text-align: start;"><span style="color: #660000; font-size: large;"><b><br /></b></span></span><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">ACESSANDO</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif; font-size: large;"><b>SKY SURVEY</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><a href="http://media.skysurvey.org/interactive360/index.html">http://media.skysurvey.org/interactive360/index.html</a></b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">você se encontrará diante do lugar onde a Lua estará visitando hoje à noite </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e também observará o fato de que vem vivenciando </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">o direcionamento para o Centro da Galáxia nestes momentos recentes</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> quando Selene veio transitando entre Escorpião e Ofiúco e agora, Sagitário!</span></div>
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<span style="font-size: 23px; font-weight: 300;">A Photographic Journey -</span><span style="font-size: small;"> http://skysurvey.org/</span></h1>
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In 2010 I changed careers. Or, rather, I replaced one with a pursuit of passion: capturing the heavens like never before. It was a photographic expedition of 60,000 miles and over 37,000 exposures collected from opposing ends of the Earth. The final mosaic photograph encompassed the entire sphere of celestial darkness, though in that darkness, <span style="line-height: 1.6em; margin-bottom: 0px; margin-top: 0px;"><a href="http://skysurvey.org/survey" style="color: black; margin-bottom: 0px; margin-top: 0px; text-decoration: none;">I found light...</a></span></div>
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© 2013 Nick Risinger, <a href="http://skysurvey.org/" style="color: black; margin-bottom: 0px; margin-top: 0px; text-decoration: none;">skysurvey.org</a></div>
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<span style="color: #073763;">Sky Survey</span></h2>
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<a href="http://media.skysurvey.org/interactive360/index.html" style="color: #ffd966; text-decoration: none;"><img alt="Sky Survey" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhY4TWMRuMsfbWwABqUlT6ZW6G-zWWKCj6KiU_YGiRb0NgkwP9-ufaaH4sQGDvBGMjAWYKNn5SeRZaEod9aKFUf3HTE_thBOROWB0KbDtkgqr__z8aNtBanT_jWIfOhuU4QKx6bBGi7UQpQ/s1600/SKY+SURVEY.jpg" height="636" id="Image15_img" style="border: none; position: relative;" width="1275" /></a></div>
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<span class="caption" style="color: #073763;">Este Programa </span></div>
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<span class="caption" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 19.6000003814697px;"><b><a href="http://media.skysurvey.org/interactive360/index.html">http://media.skysurvey.org/interactive360/index.html</a></b></span></div>
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<span class="caption" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 19.6000003814697px;">é nota dez para que possamos bem estudar o céu estrelado.</span></div>
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<span class="caption" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 19.6000003814697px;"><br /></span></div>
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<span class="caption" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 19.6000003814697px;">Veja abaixo, um excerto da fotografia inicial</span></div>
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<span class="caption" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 19.6000003814697px;">para o momento em que escrevo estas linhas - manhã de domingo, dia 23 de março -,</span></div>
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<span class="caption" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 19.6000003814697px;">onde podemos observar o amarelado-velho de Saturno em Balança</span></div>
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<span class="caption" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 19.6000003814697px;">e o branco retumbante da Lua exatamente mergulhando no lugar de direcionamento</span></div>
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<span class="caption" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 19.6000003814697px;">para o Centro da Galáxia!</span></div>
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<span class="caption" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 19.6000003814697px;">Se você seguir esse Programa diariamente, Caro Leitor,</span></div>
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<span class="caption" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 19.6000003814697px;">certamente se surpreenderá com o mundo de informações que poderá amealhar!</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEilffWhFmogwNCZ5gboV30qJsFQQiacm9tksxupaHihfxb9MNNO30TCJ3HAJPH36cN03rch6CDm926Q-hfEhsyclDQBUocx_hrheX6eI7K0GbDeLBeUPlFyaMDq-I5T23rDlhCvxj_H1lQ/s1600/23+DE+MAR%C3%87O+-+LUA+MERGULHADA+NO+CENTRO+DA+VIA+LACTEAnovo-1.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEilffWhFmogwNCZ5gboV30qJsFQQiacm9tksxupaHihfxb9MNNO30TCJ3HAJPH36cN03rch6CDm926Q-hfEhsyclDQBUocx_hrheX6eI7K0GbDeLBeUPlFyaMDq-I5T23rDlhCvxj_H1lQ/s1600/23+DE+MAR%C3%87O+-+LUA+MERGULHADA+NO+CENTRO+DA+VIA+LACTEAnovo-1.jpg" /></a></div>
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<span class="caption" style="color: #660000;"><b>OUTRO FANTÁSTICO PROGRAMA</b></span></div>
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<span class="caption" style="color: #660000;"><b>É <span style="font-size: large;">CHROMOSCOPE</span></b></span></div>
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<span class="caption" style="color: #660000; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 19.6000003814697px;"><b><a href="http://www.chromoscope.net/">http://www.chromoscope.net/</a></b></span></div>
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<span class="caption" style="color: #073763;">ONDE VOCÊ PODE SURFAR ONDAS DIFERENCIADAS</span></div>
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<span class="caption" style="color: #073763;">PARA BEM OBSERVAR E ESTUDAR NOSSA GALÁXIA, A VIA LACTEA</span></div>
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<span style="color: #073763;">Chromoscope - Versão 1.4.3</span></h2>
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<a href="http://www.chromoscope.net/" style="text-decoration: none;"><img alt="Chromoscope - Versão 1.4.3" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhYnXvTgaDLLSHO4ILLidBedngoH9SKZ68zRjUJv1r6ISB0h3YsUQRRa3uOFsWdXwejHWbJOJWpiOtVVmxFwpgA6kjsklUXR0bLp_wCX2QYBoQ7va6GbUguY1jdTYKPzwKp9pt52OyJqkzy/s1600/UNIVERSO+VIS%25C3%258DVEL+-+CROMO.jpg" height="598" id="Image22_img" style="border: none; position: relative;" width="1363" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Alguma vez desejou ter visão raio-X ou super-humana? </span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">O Chromoscope permite-lhe explorar a nossa Galáxia (a Via Láctea) e o Universo distante numa série de comprimentos de onda desde raios-X até às compridas ondas de rádio</span><span style="color: #660000;">. </span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;"><span style="line-height: normal; text-align: start;">Nick Risinger, </span><a href="http://skysurvey.org/" style="line-height: normal; text-align: start;">skysurvey.org</a> - </span><span style="color: #073763;"><span style="background-color: white; line-height: 18.239999771118164px; text-align: start;">Criado por </span><a href="http://www.jb.man.ac.uk/~slowe/" style="background-color: white; line-height: 18.239999771118164px; text-align: start;">Stuart Lowe</a><span style="background-color: white; line-height: 18.239999771118164px; text-align: start;">, </span><a href="http://www.astro.cf.ac.uk/pub/Robert.Simpson/index.html" style="background-color: white; line-height: 18.239999771118164px; text-align: start;">Rob Simpson</a><span style="background-color: white; line-height: 18.239999771118164px; text-align: start;">, e </span><a href="http://www.astro.cardiff.ac.uk/contactsandpeople/?page=full&id=493" style="background-color: white; line-height: 18.239999771118164px; text-align: start;">Chris North</a><span style="background-color: white; line-height: 18.239999771118164px; text-align: start;">.</span></span></span></div>
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<span class="watch-title yt-uix-expander-head" dir="ltr" id="eow-title" style="-webkit-user-select: auto; border: 0px; cursor: auto; margin: 0px; padding: 0px;" title="Quick Tour of Chromoscope"><span style="color: #660000;">Quick Tour of Chromoscope</span></span></h1>
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<span class="caption" style="color: #660000; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 14px; line-height: 19.6000003814697px;"><b>https://www.youtube.com/watch?v=eE7-6fQ9_48#t=153</b></span></div>
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<span class="caption" style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 17px; text-align: start;">Douglas Pierce-Price explores Chromoscope and shows you how to use it.</span></span></div>
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<span style="color: #660000;">Large Scale Structure in the Local Universe</span></h2>
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<a href="http://upload.wikimedia.org/wikipedia/commons/7/7d/2MASS_LSS_chart-NEW_Nasa.jpg"><img alt="Large Scale Structure in the Local Universe" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEigLs7jdcS2diJAdhpmr5rO7-UjBQLErT5QIjCEBQx6V9p8wAfu6vT1GaUDcCLto4PJbO02Utceg-YKexkLkHmwC__UwWQMpDul9Dwkj2g5D06XlZhnhFIN-T7UC5wO3QRu7JcqOeR5RFGN/s1600/2MASS_LSS_chart-NEW_Nasa.jpg" height="627" id="Image10_img" style="border: none; position: relative;" width="1239" /></a></div>
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<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="line-height: 19.6000003814697px;">http://upload.wikimedia.org/wikipedia/commons/7/7d/2MASS_LSS_chart-NEW_Nasa.jpg</span></span></div>
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<span style="color: #073763;">Panoramic view of the entire near-infrared sky reveals the distribution of galaxies beyond the Milky Way. The image is derived from the 2MASS Extended Source Catalog (XSC)— "Large Scale Structure in the Local Universe: The 2MASS Galaxy Catalog", Jarrett, T.H. 2004, PASA, 21, 396 Author IPAC/Caltech, by Thomas Jarrett</span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>Visitando os Sites abaixo,<o:p></o:p></b></span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b> você conseguirá informações atualizadas e preciosas<o:p></o:p></b></span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>sobre os Objetos Celestiais de seu interesse:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span style="font-family: Arial, sans-serif;">NASA/IPAC</span><span style="font-family: Arial, sans-serif;"> EXTRAGALACTIC DATABASE –</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="color: #274e13; text-decoration: none;"><span style="font-family: Arial, sans-serif;">http://ned.ipac.caltech.edu/</span></a><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="color: #274e13; text-decoration: none;"><span style="font-family: Arial, sans-serif;">http://ned.ipac.caltech.edu/forms/byname.html</span></a><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US" style="font-family: Arial, sans-serif;">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US" style="font-family: Arial, sans-serif;"> </span></i></span><em><span lang="EN-US" style="font-family: Arial, sans-serif;"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US" style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US" style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US" style="font-family: Arial, sans-serif;">The</span><span class="apple-converted-space"><span lang="EN-US" style="font-family: Arial, sans-serif;"> </span></span><span lang="EN-US" style="font-family: Arial, sans-serif;">Internet STELLAR DATABASE</span><span lang="EN-US" style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="color: #274e13; text-decoration: none;"><span lang="EN-US" style="font-family: Arial, sans-serif;">http://www.stellar-database.com/</span></a><span lang="EN-US" style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-size: 16px;"><span style="background-color: white;"></span></span><span style="background-color: white; color: #073763; font-size: 16px; font-weight: normal;"><span style="color: #073763;"><br /></span></span><span style="background-color: white; color: #073763; font-size: 16px; font-weight: normal;"><img src="http://www.ianridpath.com/atlases/urania/urania24.jpg" height="444" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="640" /></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><a href="http://www.ianridpath.com/atlases/urania/urania24.jpg" style="color: #274e13; text-decoration: none;">http://www.ianridpath.com/atlases/urania/urania24.jpg</a></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b><o:p></o:p></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelações, Estrelas e Objetos Celestes<o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Suas histórias, seus mitos, seus significados e suas sintetizadas
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<i><span lang="PT" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></i><br />
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-67121503912574046762013-08-20T08:14:00.002-07:002014-08-19T08:55:29.043-07:00SAGITTA, A FLECHA<div align="center" class="MsoNormal" style="text-align: center;">
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px; text-align: start;">Meu Projeto</span></div>
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;"><span style="font-size: large;">Da Terra ao Céu ....</span></span></span></a></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;"><span style="font-size: large;">.....<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;">e ao Infinito </a></span></span></span></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><span style="color: #660000;"><span style="font-size: large;">- As 88 Constelações</span></span></a></span></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<img src="http://www.raremaps.com/maps/medium/30252.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px; padding: 8px;" /><br style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px;" /><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 22.399999618530273px;">http://www.raremaps.com/gallery/detail/30252/Aquila_and_Antinous_Stars_heightened_in_gold/Hevelius.html</span><br style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px;" /><div class="productDetailItem" style="background-color: white; border: 0px; color: #073763; font-family: verdana, arial, georgia, sans-serif; font-size: 16px; line-height: 22.399999618530273px; margin-bottom: 1em; padding: 0px 0px 10px;">
<strong>Title: </strong>Aquila and Antinous (Stars heightened in gold)</div>
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<strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/2813" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; text-decoration: none;">Johannes Hevelius</a></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif; font-size: large;">SAGITTA, A FLECHA</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Sagitta, a Flecha certeira, é uma pequena constelação, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">bem pequena mesmo, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">porém indubitavelmente bem nomeada enquanto <i>Flecha</i> -</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">pois é bem assim que a visualizamos nos céus estrelados mais ao norte</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e bem ao lado da belíssima Aquila, a Águia que voa trazendo suas três estrelinhas</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(que podemos nomear enquanto as<i> Três Marias do Norte</i>), </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Alshain e Tarazed</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> deixando o centro iluminado</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> para ser ocupado pela maravilhosa Altair, estrela-alpha Aquilae!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Aliás, a Águia é uma constelação bem rica, digamos assim,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">porque traz consigo e já amealhada para si,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> incorporada em seu desenho estelar,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">a antiga constelação de Antinous...</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>(<span style="background-color: white; line-height: 19.049999237060547px;">A parte sul de Aquila foi subdividida por Ptolomeu</span></i></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><span style="background-color: white; line-height: 19.049999237060547px;"> em uma constelação agora obsoleta, chamada Antinous,</span></i></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><span style="background-color: white; line-height: 19.049999237060547px;"> visualizada em alguns mapas </span></i></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><span style="background-color: white; line-height: 19.049999237060547px;">como sendo mantida nas garras da águia)</span></i>,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e em seu voo, a Águia vem sempre acompanhada de Delphinus e Sagitta,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">o Delfim e a Flecha,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">o Delfim nadando através as estrelas </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e a Flecha certeira buscando seu alvo através as estrelas!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;"><span style="font-size: 15px;">http://www.stellarium.org/pt/</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgqbesxt8eLLUIrVMtSPll5oit6valHwANq3b8dobt9kJ0L0vbAqBsKBUczQifBwtnev_Av_bp1GhZ7pDHqKuIlvdo1dVexCatuwRCCr70_V-X4t8HWmiNUP8jIcX3nsRAAvWBC8La8EWI/s1600/SAGITTA,+MARIO+JACI.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgqbesxt8eLLUIrVMtSPll5oit6valHwANq3b8dobt9kJ0L0vbAqBsKBUczQifBwtnev_Av_bp1GhZ7pDHqKuIlvdo1dVexCatuwRCCr70_V-X4t8HWmiNUP8jIcX3nsRAAvWBC8La8EWI/s1600/SAGITTA,+MARIO+JACI.jpg" /></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">SAGITTA, A FLECHA</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 18h56m / 20h18m Declinação +16<sup>o</sup>.0 / +21<sup>o</sup>.4<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Mito:<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação representa a flecha com a qual Hercules matou a águia </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que se nutria do fígado de Prometeus. <o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">História:<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">É uma constelação de pequeno tamanho </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">porém já fazia parte do grupo de 48 constelações relacionadas por Ptolomeu. <o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 13.5pt;">Editora Vozes, Petrópolis, ano de 1986</span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> </span></div>
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<a href="http://www.raremaps.com/gallery/detail/33034op/_Sagitta_Stars_Heightened_in_Gold/Bayer.html">http://www.raremaps.com/gallery/detail/33034op/_Sagitta_Stars_Heightened_in_Gold/Bayer.html</a></div>
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<span style="background-color: white;"><span style="color: #073763;"><strong>Title: </strong>[ Sagitta ] (Stars Heightened in Gold) </span></span><strong style="background-color: white; color: #073763;">Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/247" style="background-color: white; border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">Johann Bayer</a><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Algumas Informações Interessantes acerca esta Constelação:</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Sagitta encontra-se bem acolhida pela Via Láctea, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">podendo ser bem visualizada em pelo menos quatro de suas estrelas, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em lugares de céus escuros e límpidos,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> ao norte de Altair, a estrela Alpha Aquilae.<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A estrela Gamma parece atuar como a ponta afiada da Flecha</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> enquanto as estrelas Alpha e Beta, como a pena que enfeita a Flecha </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e que se encontram sustentadas e amarradas à Flecha através a estrela Delta.<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Fronteiras:<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Sagitta situa-se entre as constelações Vulpecula, Hercules, Aquila, Delphinus<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">Estrelas e objetos interessantes, em Sagitta:</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Sham - Alpha Sagittae</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>S Sagittae - Estrela Variável Cefeida</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 19h53m Declinação +16<sup>o</sup>.30<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitudes: Max 5,4 Min 6,5 Período 8,4<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo CEF Espectro G3v<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b>Sagitta</b> (Sge), a <a href="http://pt.wikipedia.org/wiki/Flecha" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Flecha">Flecha</a>, é uma diminuta <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> do <a href="http://pt.wikipedia.org/wiki/Hemisf%C3%A9rio_celestial_norte" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hemisfério celestial norte">hemisfério celestial norte</a>. O genitivo, usado para formar nomes de estrelas, é <b>Sagittae</b>.</div>
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As constelações vizinhas são <a href="http://pt.wikipedia.org/wiki/Vulpecula" style="background: none; color: #0b0080; text-decoration: none;" title="Vulpecula">Vulpecula</a>, <a href="http://pt.wikipedia.org/wiki/H%C3%A9rcules_(constela%C3%A7%C3%A3o)" style="background: none; color: #0b0080; text-decoration: none;" title="Hércules (constelação)">Hercules</a>, <a href="http://pt.wikipedia.org/wiki/Aquila" style="background: none; color: #0b0080; text-decoration: none;" title="Aquila">Aquila</a> e <a href="http://pt.wikipedia.org/wiki/Delphinus" style="background: none; color: #0b0080; text-decoration: none;" title="Delphinus">Delphinus</a>.</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.399999618530273px;">http://pt.wikipedia.org/wiki/Sagitta</span></span></div>
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">Alpha Sagittae</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> (Sham, Alsahm, 5 Sagittae) é uma </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Estrela">estrela</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Sagitta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Sagitta">Sagitta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de 19h 40m 05.78s e uma </span><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Declinação">declinação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de +18° 00′ 50.2″. Sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é igual a 4.39. Considerando sua distância de 473 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> em relação à </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">, sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é igual a −1.42. Pertence à </span><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Classificação estelar">classe espectral</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> G0II.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> http://pt.wikipedia.org/wiki/Alpha_Sagittae</span></div>
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">Beta Sagittae</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> (6 Sagittae) é uma </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Estrela">estrela</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Sagitta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Sagitta">Sagitta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de 19h 41m 02.93s e uma </span><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Declinação">declinação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de +17° 28′ 34.0″. Sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é igual a 4.39. Considerando sua distância de 466 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> em relação à </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">, sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é igual a −1.39. Pertence à </span><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Classificação estelar">classe espectral</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> G8II.</span></div>
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<span style="background-color: white; line-height: 22.399999618530273px; text-align: start;"><span style="color: #252525; font-family: sans-serif;">http://pt.wikipedia.org/wiki/Beta_Sagittae</span></span></div>
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">Gamma Sagittae</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> (12 Sagittae) é uma </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Estrela">estrela</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/Sagitta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Sagitta">Sagitta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de 19h 58m 45.39s e uma </span><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Declinação">declinação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de +19° 29′ 31.5″. Sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é igual a 3.51. Considerando sua distância de 274 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> em relação à </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">, sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é igual a −1.11. Pertence à</span><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Classificação estelar">classe espectral</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> K5III.</span></div>
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<span style="background-color: white; line-height: 22.399999618530273px; text-align: start;"><span style="color: #252525; font-family: sans-serif;">http://pt.wikipedia.org/wiki/Gamma_Sagittae</span></span></div>
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">Delta Sagittae</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> (7 Sagittae) é uma </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Estrela">estrela</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/Sagitta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Sagitta">Sagitta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de 19h 47m 23.27s e uma </span><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Declinação">declinação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de +18° 32′ 03.3″. Sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é igual a 3.68. Considerando sua distância de 448 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> em relação à </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">, sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é igual a −2.01. Pertence à </span><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Classificação estelar">classe espectral</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> M2II + B6.</span></div>
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<span style="background-color: white; line-height: 22.399999618530273px; text-align: start;"><span style="color: #252525; font-family: sans-serif;">http://pt.wikipedia.org/wiki/Delta_Sagittae</span></span></div>
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">Epsilon Sagittae</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> (4 Sagittae) é uma </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Estrela">estrela</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/Sagitta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Sagitta">Sagitta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de 19h 37m 17.38s e uma </span><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Declinação">declinação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de +16° 27′ 46.0″. Sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é igual a 5.67. Considerando sua distância de 473 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> em relação à </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">, sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é igual a −0.14. Pertence à </span><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Classificação estelar">classe espectral</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> G8IIIvar.</span></div>
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<span style="background-color: white; line-height: 22.399999618530273px; text-align: start;"><span style="color: #252525; font-family: sans-serif;">http://pt.wikipedia.org/wiki/Epsilon_Sagittae</span></span></div>
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">Zeta Sagittae</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> (8 Sagittae) é uma </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Estrela">estrela</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/Sagitta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Sagitta">Sagitta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de 19h 48m 58.65s e uma </span><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Declinação">declinação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de +19° 08′ 31.1″. Sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é igual a 5.01. Considerando sua distância de 326 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> em relação à </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">, sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é igual a 0.01. Pertence à </span><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Classificação estelar">classe espectral</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> A3V.</span></div>
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<span style="background-color: white; line-height: 22.399999618530273px; text-align: start;"><span style="color: #252525; font-family: sans-serif;">http://pt.wikipedia.org/wiki/Zeta_Sagittae</span></span></div>
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">Eta Sagittae</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> (16 Sagittae) é uma </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Estrela">estrela</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/Sagitta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Sagitta">Sagitta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de 20h 05m 09.47s e uma </span><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Declinação">declinação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de +19° 59′ 27.2″. Sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é igual a 5.09. Considerando sua distância de 162 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> em relação à </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">, sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é igual a 1.61. Pertence à </span><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Classificação estelar">classe espectral</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> K2III.</span></div>
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<span style="background-color: white; line-height: 22.399999618530273px; text-align: start;"><span style="color: #252525; font-family: sans-serif;">http://pt.wikipedia.org/wiki/Eta_Sagittae</span></span></div>
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">Theta Sagittae</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> (17 Sagittae) é uma </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Estrela">estrela</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/Sagitta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Sagitta">Sagitta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de 20h 09m 56.61s e uma </span><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Declinação">declinação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> de +20° 54′ 53.2″. Sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é igual a 6.51. Considerando sua distância de 147 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> em relação à </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;">, sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> é igual a 3.24. Pertence à </span><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start; text-decoration: none;" title="Classificação estelar">classe espectral</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px; text-align: start;"> F5IV.</span></div>
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<span style="background-color: white; line-height: 22.399999618530273px; text-align: start;"><span style="color: #252525; font-family: sans-serif;">http://pt.wikipedia.org/wiki/Theta_Sagittae</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">M71 - NGC 6839 - Aglomerado de estrelas</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Um aglomerado bem pouco comum na constelação de Sagitta,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">quanto de ser um aglomerado globular.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span class="mw-mmv-author" style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start; white-space: nowrap;">Till Credner und Sven Kohle, Calar Alto Observatory</span><span style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start; white-space: nowrap;"> - </span><span class="mw-mmv-source" style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start; white-space: nowrap;"><a class="external free" href="http://www.allthesky.com/clusters/preview/m71-p.jpg" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">http://www.allthesky.com/clusters/preview/m71-p.jpg</a> (<a class="external free" href="http://www.allthesky.com/clusters/m71-d.html" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">http://www.allthesky.com/clusters/m71-d.html</a>)</span></div>
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<span style="color: #660000; font-size: large;"><span style="font-family: Arial, Helvetica, sans-serif;"> </span><span style="font-family: Arial, sans-serif;"> </span><b style="background-color: white; font-family: sans-serif; line-height: 22.399999618530273px;">Messier 71</b><span style="background-color: white; font-family: sans-serif; line-height: 22.399999618530273px;"> (também conhecido como </span><b style="background-color: white; font-family: sans-serif; line-height: 22.399999618530273px;">NGC 6838</b><span style="background-color: white; font-family: sans-serif; line-height: 22.399999618530273px;"> ou </span><b style="background-color: white; font-family: sans-serif; line-height: 22.399999618530273px;">M71</b><span style="background-color: white; font-family: sans-serif; line-height: 22.399999618530273px;">)</span></span><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> localizado na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Constelação">constelação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> de </span><a href="http://pt.wikipedia.org/wiki/Sagitta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Sagitta">Sagitta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> a 13 000 </span><a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Ano-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> da </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Terra">Terra</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">. Foi descoberto por</span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Philippe_Loys_de_Ch%C3%A9seaux" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Philippe Loys de Chéseaux">Philippe Loys de Chéseaux</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;"> em </span><a href="http://pt.wikipedia.org/wiki/1746" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="1746">1746</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">. Possui um raio de 13,5 anos-luz e uma dimensão aparente de 7,2 </span><a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.399999618530273px; text-decoration: none;" title="Minuto de arco">minutos de arco</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.399999618530273px;">.</span><span class="reference" id="cite_ref-seds_2-4" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_71#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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O <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> foi rimeiramente visto por <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background: none; color: #0b0080; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>, que o catalogou como o décimo terceiro objeto de sua lista. Foi mais tarde redescoberto por <a href="http://pt.wikipedia.org/wiki/Johann_Gottfried_K%C3%B6hler" style="background: none; color: #0b0080; text-decoration: none;" title="Johann Gottfried Köhler">Johann Gottfried Köhler</a> entre 1772 e 1779 e por <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background: none; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a> em 28 de junho de 1780.<a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catalogou</a> o objeto em 4 de outubro daquele ano com base na descrição de Méchain, e o próprio Messier descreveu-o como "uma nebulosa sem estrelas".<span class="reference" id="cite_ref-seds_2-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_71#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Pode ser visto mesmo em bons <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background: none; color: #0b0080; text-decoration: none;" title="Binóculo">binóculos</a>, embora suas estrelas mais brilhantes possam ser resolvidas a partir de <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a>amadores médios ou mais potentes.<span class="reference" id="cite_ref-seds_2-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_71#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Por um bom tempo, a classificação de M71 como um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> denso, como <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Messier_11" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 11">Messier 11</a>, ou um <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> pouco denso era indefinida. <a href="http://pt.wikipedia.org/wiki/Harlow_Shapley" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Harlow Shapley">Harlow Shapley</a> e <a href="http://pt.wikipedia.org/wiki/Robert_Julius_Trumpler" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Robert Julius Trumpler">Robert Julius Trumpler</a>, alguns dos primeiros a investigar as propriedades físicas do aglomerado, classificaram-no como aberto. <a class="new" href="http://pt.wikipedia.org/w/index.php?title=James_Cuffey&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="James Cuffey (página não existe)">James Cuffey</a> investigou o <a href="http://pt.wikipedia.org/wiki/Diagrama_de_Hertzsprung-Russell" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Diagrama de Hertzsprung-Russell">diagrama de magnitude de cor</a> do objeto, concluindo que o diagrama era mais semelhante a de um aglomerado aberto. Outro critério de classificação, a velocidade do radial do sistema, também não estava definido: seus valores da taxa de afastamento em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> variavam entre -80 a +80 km/s (atualmente aceita-se que M71 está se aproximando radialmente da Terra a uma velocidade de 23 km/s).<span class="reference" id="cite_ref-seds_2-7" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_71#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Atualmente, há um consenso em torno de sua classificação como aglomerado globular. Situa-se a uma distância de 13 000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> do <a href="http://pt.wikipedia.org/wiki/Sistema_Solar" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sistema Solar">Sistema Solar</a> e possui um núcleo mais denso, facilmente visível em <a href="http://pt.wikipedia.org/wiki/Astrofotografia" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Astrofotografia">astrofotografias</a> ou em telescópios amadores, com diâmetro aparente na <a href="http://pt.wikipedia.org/wiki/Esfera_celeste" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Esfera celeste">esfera celeste</a> de 5 a 6 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de grau</a>. Seu diâmetro aparente total é pouco maior, com 7 minutois de grau, correspondendo a um diâmetro real de apenas 27 anos-luz, muio menor comparado a outros aglomerados globulares.<span class="reference" id="cite_ref-seds_2-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_71#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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<a href="http://www.raremaps.com/gallery/enlarge/33140" style="color: #274e13; text-decoration: none;"><span style="font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/enlarge/33140</span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/33140/Aquila_Sagitta_Vulpecula_and_Anser_Delphinus/Flamsteed.html</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><strong>Title: </strong>Aquila, Sagitta, Vulpecula & Anser Delphinus. </span><strong style="font-family: Arial, Helvetica, sans-serif;">Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1260" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; font-family: Arial, Helvetica, sans-serif; text-decoration: none;">John Flamsteed</a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>- AS CONSTELAÇÕES -</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> são como janelas que se abrem para a infinitude do universo</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>entre o céu e a terra..., bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,<o:p></o:p></b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward<o:p></o:p></b></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">VISITE MINHA PÁGINA<o:p></o:p></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">DA TERRA AO CÉU E AO INFINITO<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #274e13;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/">http://daterraaoceueaoinfinito.blogspot.com.br/</a></span></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-85666705657924369182013-08-20T08:12:00.002-07:002017-04-09T10:31:03.923-07:00PYXIS NAUTICA, A BÚSSOLA<div align="center" class="MsoNormal" style="text-align: center;">
<br /><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Caro Leitor,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">suponha que você está perdido</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em meio à Floresta Amazônica....</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">O que você faz</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">para poder orientar-se?</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Bem, primeiramente os céus estrelados</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">funcionam como nossa maior orientação,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">nossa fantástica e natural bússola,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">não é verdade?</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Corre o risco, porém,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">de você não conhecer os céus estrelados,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">as constelações,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">as estrelas mais ao norte e mais ao sul</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e mais ao centro...</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Agora imagine-se viajando, navegando</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em um navio bem antigo.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e por mares nunca dantes navegados;</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Imagine que você é o capitão</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e bem conhece a orientação pelas estrelas, sim.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">No entanto, será que todos seus marinheiros</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e comandados seus</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">também saber ler as orientações trazidas pelas estrelas?</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Talvez você vá precisar se munir</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">com um instrumento realmente espetacular:</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">uma Bússola!</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ainda pensando na imagem de um Navio</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e de uma Bússola,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">vamos encontrar uma pequena e tímida constelação</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">denominada enquanto Pyxis Nautica</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(ou somente Pyxis), a Bússola,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e este pequeno nicho estelar</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">apresenta-se entremeado ao mastro</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">de Argonavis, o Navio Argo da antiguidade.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(Aliás, os antigos gregos </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">denominavam este lugar</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">como Mastro</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e, no século XIV,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> John Herschel </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- filho de William Herschel -</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">assim também designou,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">porém caiu em desuso).</span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Stellarium</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Pyxis parece ter sido inserida</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">pelo astrônomo francês Nicolas Louis La Caille</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">a partir de suas observações nos céus austrais</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">quando de sua estada no Cabo da Boa Esperança,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">África do Sul.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">O que nos parece bem paradoxal</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é o fato de que o mesmo Lacaille </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que criou Pyxis, a Bussola,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">colocando-a entremeada ao Mastro,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">resolveu partir o antigo e imenso Navio Argo</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em três (ainda grandes) constelações</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- Puppis, a Popa; Carina, a Quilha, e Vela!</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Bem, penso que o Caro Leitor já bem percebeu</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que não sou muito afeita </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">à esta partição do belíssimo Argonavis....,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">porque nossa visão a olho nú, à vista desarmada,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">dos céus estrelados mais ao sul</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">visualiza esta constelação por inteiro, </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">certamente,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">o Navio Argo singrando mares nunca dantes navegados,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">mares estelados,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e perdendo sua Proa</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">ao passar pelo Estreito de Bósforo</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e ter pedras rolando e caindo e espatifando-se</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre sua frente </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que ruma </span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">para o sul, </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">sempre mais ao sul.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Alguns autores astrônomos</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">julgam que Pyxis, a Bússola,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é a menos importante constelação dos céus estrelados...</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A bem da verdade,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">mesmo em lugares de céus escuros e transparentes</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e em noites sem a luminosidade da Lua,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">mal podemos notar</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">as estrelas Alpha e Beta e Gamma Pyxidis</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que formam uma espécie de agulha da Bússola.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Isso acontece por várias razões</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e duas delas são:</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">a estrela mais luminosa </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">vem na magnitude 3.68(Alpha Pyxidis)</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e por estar mergulhada esta pequena constelação</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> ao caminho leitoso</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">da Via Lactea</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(assim como todo o Navio).</span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgc2DuAFeYoXIRpKVTC0nWK_EhkXfmikvbQXmcRZZRzb3m8CyjXZ4V1jJ6lJ3tJSI3f6ROlA0B7FsNfcDLZNqGt2GMAev8kcgJUYrnsUVoLW9AFXtu_U6h2L68UyiB0lR1-UGleYgei_ISt/s1600/b%25C3%25BAssula+aproximada.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgc2DuAFeYoXIRpKVTC0nWK_EhkXfmikvbQXmcRZZRzb3m8CyjXZ4V1jJ6lJ3tJSI3f6ROlA0B7FsNfcDLZNqGt2GMAev8kcgJUYrnsUVoLW9AFXtu_U6h2L68UyiB0lR1-UGleYgei_ISt/s1600/b%25C3%25BAssula+aproximada.png" /></span></a></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiqOZv1xj9xhFnf_5JifAQB3d_QLqXqkBQZ4pMIHTcMcUkH3m41CSH5yU3f6fkJekcyCFWD6za1SMIRAUvQufXwMYrJOpGV3jCc851TeqBuiRkiKHGw5O-kOGs558cFZig8oPdHykK4Z-zM/s1600/via+lactea+passando+por+Pyxis.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiqOZv1xj9xhFnf_5JifAQB3d_QLqXqkBQZ4pMIHTcMcUkH3m41CSH5yU3f6fkJekcyCFWD6za1SMIRAUvQufXwMYrJOpGV3jCc851TeqBuiRkiKHGw5O-kOGs558cFZig8oPdHykK4Z-zM/s1600/via+lactea+passando+por+Pyxis.png" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Stellarium</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Mesmo sendo apresentada </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">como uma constelação quase inexpressiva,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">na direção de Pyxis</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">encontram-se objetos celestes bem interessantes</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">como </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- T Pyxidis, uma estrela </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">"recurrent nova and nova remnant";</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- NGC 2818, uma bela nebulosa planetária,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- NGC 2613, uma galáxia espiral,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- Pyxis Globular Cluster </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e ainda alguns outros objetos interessantes</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">contidos neste pequeno lugar</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">dos céus estrelados mais ao sul.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Hoje à noite, Caro Leitor,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">vou aproveitar para buscar uma boa visão do Navio</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e então iidentificar Pyxis, a Bússola.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Por que você também não faz o mesmo?</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A visão dos céus a olho nú</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é sempre uma imensa emoção!</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
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<img src="http://www.ianridpath.com/atlases/urania/urania32.jpg" /><br />
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<b><span style="font-family: Verdana, sans-serif; font-size: 18pt;">A BÚSSOLA</span></b><b><span style="font-family: "Times New Roman", serif; font-size: 12pt;"><o:p></o:p></span></b></div>
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<span style="font-family: Verdana, sans-serif; font-size: 12pt;">A bússola, mais conhecida pelos marinheiros como agulha, é sem dúvida o instrumento de navegação mais importante a bordo. Ela teve sua origem na China do século IV a.C. Sua adaptação e reconhecimento no Ocidente aconteceu cerca de 1.500 anos depois. A primeira referência deste instrumento na Europa aparece em um documento de 1190, chamado "De Naturis Rerum". As primeiras bússolas chinesas não utilizavam agulhas . Eram compostas por um prato quadrangular representando a Terra. O "indicador"(objeto que indica a direção), com forma de concha, era de pedra imantada e a base (prato), de bronze. Um círculo no centro do prato representava o céu e a base quadrada, a terra.</span><span style="font-family: "Times New Roman", serif; font-size: 12pt;"><o:p></o:p></span></div>
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<span style="font-family: Verdana, sans-serif; font-size: 12pt;">Foi Flávio Gioia que em 1302 alterou a bússola para ser usada a bordo, usando a agulha sobre um cartão com o desenho de uma rosa-dos-ventos. Os rumos ou as direções dos ventos têm origem na antigüidade. Na Grécia começaram com dois, quatro, oito e doze rumos. No início do século XVI surgem já 16 e na época do Infante D. Henrique já se usavam rosas-dos-ventos com 32 rumos. Primeiramente o rumo era associado à direção dos ventos e só mais tarde aos pontos cardeais. Em certas rosas-dos-ventos, no local que indicava o Leste, aparecia desenhada uma cruz que mostrava a direção da Terra Santa. A declinação de uma agulha é a diferença que uma bússola marca entre o norte geográfico e o norte magnético.</span><span style="font-family: "Times New Roman", serif; font-size: 12pt;"><o:p></o:p></span></div>
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<span style="font-family: Verdana, sans-serif; font-size: 12pt;">O cabo da concha indicava o sul. A concha é uma representação simbólica da Ursa Maior. A base continha caracteres chineses que assinalavam os oito pontos principais: norte, sul, leste, oeste, nordeste, noroeste, sudeste e sudoeste. A introdução da agulha aumentou a precisão da leitura. Foi nessa época que os chineses introduziram os primeiros marcadores e indicadores, elementos fundamentais da ciência moderna. A Lo Pan é um instrumento complexo, desenvolvido através dos séculos, pelos chineses, para que os praticantes pudessem fazer precisos cálculos de tempo e espaço em sua ciência. O cálculo da direção pode ser efetuado com uma Lo Pan ou com uma bússola normal. Não existe diferença. A Lo Pan apenas nos indica um cálculo mais preciso, e algumas facilidades em relação às direções e as características do local.</span><span style="font-family: "Times New Roman", serif; font-size: 12pt;"><o:p></o:p></span></div>
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<span style="font-family: Verdana, sans-serif; font-size: 12pt;">Ao longo do tempo veio a verificar-se que a declinação variava com o tempo e o lugar. Também foi D. João de Castro o primeiro a descobrir o desvio de uma agulha, ou seja, o efeito que massas de ferro próximas tem sobre uma bússola. Este efeito obrigou a cuidados com o posicionamento da bússola perto de peças da artilharia, âncoras e outros ferros. Esta foi uma das razões para que os morteiros, as caixas que protegem as bússolas, fossem, no início, de madeira.Durante o século XVI as bússolas portuguesas tinham, pelo menos desde 1537, um sistema de balança para manter o morteiro horizontal. O morteiro era colocado numa coluna de madeira, mais tarde de metal, a bitácula, à frente da roda do leme. A bitácula contêm um sistema chamado cardan que permite que o morteiro se mantenha na horizontal apesar das oscilações do barco.</span><span style="font-family: "Times New Roman", serif; font-size: 12pt;"><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As constelações, Cartas Celestes</span></div>
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<span style="font-family: Arial, sans-serif;"><b><span style="color: #660000;">PYXIS NAUTICA, A BÚSSOLA</span></b><span style="color: #0f243e;"><o:p></o:p></span></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; line-height: 24px;">Ascensão Reta 8h26m / 4h26m Declinação -17<sup>o</sup>.3 / -37<sup>o</sup>.0<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">Constelação formada por La Caille em 1752,<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">com as estrelas do mastro do Navio Argo.<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">Esta constelação é a menos interessante de todas as constelações. <o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">Pyxis é rodeada por Hydra, Puppis, Vela e Antlia.<span style="font-size: 11pt;"><o:p></o:p></span></span></div>
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<span style="font-family: arial, helvetica, sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: arial, helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: arial, helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b>Pyxis</b> (Pyx), a <a href="https://pt.wikipedia.org/wiki/B%C3%BAssola" style="background: none; color: #0b0080; text-decoration-line: none;" title="Bússola">Bússola</a>, é uma <a href="https://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration-line: none;" title="Constelação">constelação</a> do <a href="https://pt.wikipedia.org/wiki/Hemisf%C3%A9rio_celestial_sul" style="background: none; color: #0b0080; text-decoration-line: none;" title="Hemisfério celestial sul">hemisfério celestial sul</a>. O genitivo, usado para formar nomes de estrelas, é <b>Pyxidis</b>. É uma das 14 constelações criadas pelo <a href="https://pt.wikipedia.org/wiki/Astr%C3%B4nomo" style="background: none; color: #0b0080; text-decoration-line: none;" title="Astrônomo">astrônomo</a> <a class="mw-disambig" href="https://pt.wikipedia.org/wiki/Franc%C3%AAs" style="background: none; color: #0b0080; text-decoration-line: none;" title="Francês">francês</a> <a class="mw-redirect" href="https://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background: none; color: #0b0080; text-decoration-line: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a> no século XVIII.</div>
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As constelações vizinhas são <a href="https://pt.wikipedia.org/wiki/Hydra" style="background: none; color: #0b0080; text-decoration-line: none;" title="Hydra">Hydra</a>, <a href="https://pt.wikipedia.org/wiki/Puppis" style="background: none; color: #0b0080; text-decoration-line: none;" title="Puppis">Puppis</a>, <a href="https://pt.wikipedia.org/wiki/Vela_(constela%C3%A7%C3%A3o)" style="background: none; color: #0b0080; text-decoration-line: none;" title="Vela (constelação)">Vela</a> e <a href="https://pt.wikipedia.org/wiki/Antlia" style="background: none; color: #0b0080; text-decoration-line: none;" title="Antlia">Antlia</a>.</div>
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<span style="color: #222222; font-family: sans-serif;"><a href="https://pt.wikipedia.org/wiki/Pyxis">https://pt.wikipedia.org/wiki/Pyxis</a></span></div>
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<b style="color: #222222; font-family: sans-serif;">Alpha Pyxidis</b><span style="color: #222222; font-family: sans-serif;"> (</span><b style="color: #222222; font-family: sans-serif;">Alpha Pyx</b><span style="color: #222222; font-family: sans-serif;">, </span><b style="color: #222222; font-family: sans-serif;">α Pyxidis</b><span style="color: #222222; font-family: sans-serif;">, </span><b style="color: #222222; font-family: sans-serif;">α Pyx</b><span style="color: #222222; font-family: sans-serif;">) is a </span><a href="https://en.wikipedia.org/wiki/Giant_star" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Giant star">giant star</a><span style="color: #222222; font-family: sans-serif;"> in the </span><a href="https://en.wikipedia.org/wiki/Constellation" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Constellation">constellation</a><span style="color: #222222; font-family: sans-serif;"> </span><a href="https://en.wikipedia.org/wiki/Pyxis" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Pyxis">Pyxis</a><span style="color: #222222; font-family: sans-serif;">. It has a </span><a href="https://en.wikipedia.org/wiki/Stellar_classification" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Stellar classification">stellar classification</a><span style="color: #222222; font-family: sans-serif;"> of B1.5III and is a </span><a href="https://en.wikipedia.org/wiki/Beta_Cephei_variable" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Beta Cephei variable">Beta Cephei variable</a><span style="color: #222222; font-family: sans-serif;">. This star has more than ten times the </span><a href="https://en.wikipedia.org/wiki/Solar_mass" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Solar mass">mass of the Sun</a><span style="color: #222222; font-family: sans-serif;"> and is more than six times the </span><a href="https://en.wikipedia.org/wiki/Solar_radius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Solar radius">Sun's radius</a><span style="color: #222222; font-family: sans-serif;">. The surface temperature is 24,300 K and the star is about 10,000 times as </span><a href="https://en.wikipedia.org/wiki/Solar_luminosity" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Solar luminosity">luminous as the Sun</a><span style="color: #222222; font-family: sans-serif;">.</span><sup class="reference" id="cite_ref-apj157_3-1" style="color: #222222; font-family: sans-serif; line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Alpha_Pyxidis#cite_note-apj157-3" style="background: none; color: #0b0080; text-decoration-line: none;">[3]</a></sup><sup class="reference" id="cite_ref-Hubrig_et_al_4-3" style="color: #222222; font-family: sans-serif; line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Alpha_Pyxidis#cite_note-Hubrig_et_al-4" style="background: none; color: #0b0080; text-decoration-line: none;">[4]</a></sup><sup class="reference" id="cite_ref-aaa282_7-3" style="color: #222222; font-family: sans-serif; line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Alpha_Pyxidis#cite_note-aaa282-7" style="background: none; color: #0b0080; text-decoration-line: none;">[7]</a></sup><span style="color: #222222; font-family: sans-serif;"> Stars such as this with more than 10 solar masses are expected to end their life by exploding as a </span><a href="https://en.wikipedia.org/wiki/Supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Supernova">supernova</a><span style="color: #222222; font-family: sans-serif;">.</span><sup class="reference" id="cite_ref-aj130_4_1652_10-0" style="color: #222222; font-family: sans-serif; line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Alpha_Pyxidis#cite_note-aj130_4_1652-10" style="background: none; color: #0b0080; text-decoration-line: none;">[10]</a></sup></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Stellarium</span></div>
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<b>Beta Pyxidis</b> (<b>Beta Pyx</b>, <b>β Pyxidis</b>, <b>β Pyx</b>) is a <a href="https://en.wikipedia.org/wiki/Double_star" style="background: none; color: #0b0080; text-decoration-line: none;" title="Double star">double star</a><sup class="reference" id="cite_ref-SIMBAD_3-2" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Beta_Pyxidis#cite_note-SIMBAD-3" style="background: none; color: #0b0080; text-decoration-line: none;">[3]</a></sup> located in the southern <a href="https://en.wikipedia.org/wiki/Constellation" style="background: none; color: #0b0080; text-decoration-line: none;" title="Constellation">constellation</a> <a href="https://en.wikipedia.org/wiki/Pyxis" style="background: none; color: #0b0080; text-decoration-line: none;" title="Pyxis">Pyxis</a>. It has an <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Apparent_visual_magnitude" style="background: none; color: #0b0080; text-decoration-line: none;" title="Apparent visual magnitude">apparent visual magnitude</a> of 3.954, making it the <a href="https://en.wikipedia.org/wiki/List_of_stars_in_Pyxis" style="background: none; color: #0b0080; text-decoration-line: none;" title="List of stars in Pyxis">second brightest star</a> in that faint constellation.</div>
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Based upon <a href="https://en.wikipedia.org/wiki/Parallax" style="background: none; color: #0b0080; text-decoration-line: none;" title="Parallax">parallax</a> measurements, the star is an estimated 420 <a href="https://en.wikipedia.org/wiki/Light-year" style="background: none; color: #0b0080; text-decoration-line: none;" title="Light-year">light-years</a> (128 <a href="https://en.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration-line: none;" title="Parsec">parsecs</a>) from the <a href="https://en.wikipedia.org/wiki/Earth" style="background: none; color: #0b0080; text-decoration-line: none;" title="Earth">Earth</a>.<sup class="reference" id="cite_ref-aaa474_2_653_1-5" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Beta_Pyxidis#cite_note-aaa474_2_653-1" style="background: none; color: #0b0080; text-decoration-line: none;">[1]</a></sup> The <a href="https://en.wikipedia.org/wiki/Spectrum" style="background: none; color: #0b0080; text-decoration-line: none;" title="Spectrum">spectrum</a> matches a <a href="https://en.wikipedia.org/wiki/Bright_giant" style="background: none; color: #0b0080; text-decoration-line: none;" title="Bright giant">bright giant</a> or <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Supergiant" style="background: none; color: #0b0080; text-decoration-line: none;" title="Supergiant">supergiant</a> star of <a href="https://en.wikipedia.org/wiki/Stellar_classification" style="background: none; color: #0b0080; text-decoration-line: none;" title="Stellar classification">stellar classification</a> G7Ib-II. The <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Interferometer" style="background: none; color: #0b0080; text-decoration-line: none;" title="Interferometer">interferometer</a>-measured <a href="https://en.wikipedia.org/wiki/Angular_diameter" style="background: none; color: #0b0080; text-decoration-line: none;" title="Angular diameter">angular diameter</a> of this star is <span class="nowrap" style="white-space: nowrap;">2.05 ± 0.14 <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Milliarcsecond" style="background: none; color: #0b0080; text-decoration-line: none;" title="Milliarcsecond">mas</a></span>.<sup class="reference" id="cite_ref-aaa431_773_8-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Beta_Pyxidis#cite_note-aaa431_773-8" style="background: none; color: #0b0080; text-decoration-line: none;">[8]</a></sup> At its estimated distance, this yields a physical size of about 28 times the <a href="https://en.wikipedia.org/wiki/Solar_radius" style="background: none; color: #0b0080; text-decoration-line: none;" title="Solar radius">radius of the Sun</a>.<sup class="reference" id="cite_ref-lang2006_6-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Beta_Pyxidis#cite_note-lang2006-6" style="background: none; color: #0b0080; text-decoration-line: none;">[6]</a></sup> The <a href="https://en.wikipedia.org/wiki/Effective_temperature" style="background: none; color: #0b0080; text-decoration-line: none;" title="Effective temperature">effective temperature</a> of the star's outer envelope is about 5,400 K, giving it the characteristic yellow hue of a <a class="mw-redirect" href="https://en.wikipedia.org/wiki/G-type_star" style="background: none; color: #0b0080; text-decoration-line: none;" title="G-type star">G-type star</a>.<sup class="reference" id="cite_ref-apj507_2_919_7-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Beta_Pyxidis#cite_note-apj507_2_919-7" style="background: none; color: #0b0080; text-decoration-line: none;">[7]</a></sup><sup class="reference" id="cite_ref-csiro_9-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Beta_Pyxidis#cite_note-csiro-9" style="background: none; color: #0b0080; text-decoration-line: none;">[9]</a></sup></div>
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In 2010, the star was among a survey of massive, lower <a href="https://en.wikipedia.org/wiki/Effective_temperature" style="background: none; color: #0b0080; text-decoration-line: none;" title="Effective temperature">effective temperature</a> supergiants in an attempt to detect a magnetic field. This star may have a longitudinal <a href="https://en.wikipedia.org/wiki/Stellar_magnetic_field" style="background: none; color: #0b0080; text-decoration-line: none;" title="Stellar magnetic field">magnetic field</a> with a strength of less than a <a href="https://en.wikipedia.org/wiki/Gauss_(unit)" style="background: none; color: #0b0080; text-decoration-line: none;" title="Gauss (unit)">Gauss</a>.<sup class="reference" id="cite_ref-mnras408_4_2290_10-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Beta_Pyxidis#cite_note-mnras408_4_2290-10" style="background: none; color: #0b0080; text-decoration-line: none;">[10]</a></sup> It is a <a href="https://en.wikipedia.org/wiki/Metallicity" style="background: none; color: #0b0080; text-decoration-line: none;" title="Metallicity">young disk star</a> system with <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Space_velocity_(astronomy)" style="background: none; color: #0b0080; text-decoration-line: none;" title="Space velocity (astronomy)">space velocity</a> components, <span class="nowrap" style="white-space: nowrap;">[U, V, W]</span> = <span class="nowrap" style="white-space: nowrap;">[–11.0, +11.8, –2.2] km/s</span>.<sup class="reference" id="cite_ref-apj107_5-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Beta_Pyxidis#cite_note-apj107-5" style="background: none; color: #0b0080; text-decoration-line: none;">[5]</a></sup> There is a magnitude 12.5 optical companion, located at an angular separation of 12.7 <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Arcsecond" style="background: none; color: #0b0080; text-decoration-line: none;" title="Arcsecond">arcseconds</a> and a <a href="https://en.wikipedia.org/wiki/Position_angle" style="background: none; color: #0b0080; text-decoration-line: none;" title="Position angle">position angle</a> of 118° as of the year 1943.<sup class="reference" id="cite_ref-wdsc84_11-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Beta_Pyxidis#cite_note-wdsc84-11" style="background: none; color: #0b0080; text-decoration-line: none;">[11]</a></sup></div>
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<b>Gamma Pyxidis</b> (<b>Gamma Pyx</b>, <b>γ Pyxidis</b>, <b>γ Pyx</b>) is a <a href="https://en.wikipedia.org/wiki/Apparent_magnitude" style="background: none; color: #0b0080; text-decoration-line: none;" title="Apparent magnitude">4th magnitude</a> star in the <a href="https://en.wikipedia.org/wiki/Constellation" style="background: none; color: #0b0080; text-decoration-line: none;" title="Constellation">constellation</a> <a href="https://en.wikipedia.org/wiki/Pyxis" style="background: none; color: #0b0080; text-decoration-line: none;" title="Pyxis">Pyxis</a>. It is classified as a <a href="https://en.wikipedia.org/wiki/Giant_star" style="background: none; color: #0b0080; text-decoration-line: none;" title="Giant star">giant star</a> of composition similar to the Sun<sup class="reference" id="cite_ref-apj518_2_859_7-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Gamma_Pyxidis#cite_note-apj518_2_859-7" style="background: none; color: #0b0080; text-decoration-line: none;">[7]</a></sup> with an estimated diameter 3.7 times that of the Sun.<sup class="reference" id="cite_ref-CADARS_8-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Gamma_Pyxidis#cite_note-CADARS-8" style="background: none; color: #0b0080; text-decoration-line: none;">[8]</a></sup> It is located an estimated 207 <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Light_year" style="background: none; color: #0b0080; text-decoration-line: none;" title="Light year">light years</a> from the <a href="https://en.wikipedia.org/wiki/Solar_System" style="background: none; color: #0b0080; text-decoration-line: none;" title="Solar System">Solar System</a>.<sup class="reference" id="cite_ref-van_Leeuwen2007_4-3" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Gamma_Pyxidis#cite_note-van_Leeuwen2007-4" style="background: none; color: #0b0080; text-decoration-line: none;">[4]</a></sup></div>
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Gamma Pyxidis is moving through the Galaxy at a speed of 54.2 km/s relative to the Sun. Its projected Galactic orbit carries it between 21,300 and 30,700 light years from the center of the Galaxy.<sup class="reference" id="cite_ref-astrostudio_9-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Gamma_Pyxidis#cite_note-astrostudio-9" style="background: none; color: #0b0080; text-decoration-line: none;">[9]</a></sup></div>
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<span style="color: #222222; font-family: sans-serif;"><a href="https://en.wikipedia.org/wiki/Gamma_Pyxidis">https://en.wikipedia.org/wiki/Gamma_Pyxidis</a></span></div>
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<span style="color: #222222; font-family: sans-serif; font-size: 16px;">Hubble telescope picture of <b>T Pyxidis</b>, from a compilation of data taken on Feb. 26, 1994, and June 16, Oct. 7, and Nov. 10, 1995, by the Wide Field and Planetary Camera 2.</span></div>
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<a href="https://en.wikipedia.org/wiki/T_Pyxidis#/media/File:Tpyx_hst_big.jpg">https://en.wikipedia.org/wiki/T_Pyxidis#/media/File:Tpyx_hst_big.jpg</a></div>
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<b>T Pyxidis</b> (<i>T Pyx</i>)<sup class="reference" id="cite_ref-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/T_Pyxidis#cite_note-1" style="background: none; color: #0b0080; text-decoration-line: none;">[1]</a></sup> is a <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Recurrent_nova" style="background: none; color: #0b0080; text-decoration-line: none;" title="Recurrent nova">recurrent nova</a><sup class="reference" id="cite_ref-Shara1997_2-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/T_Pyxidis#cite_note-Shara1997-2" style="background: none; color: #0b0080; text-decoration-line: none;">[2]</a></sup> and <a href="https://en.wikipedia.org/wiki/Nova_remnant" style="background: none; color: #0b0080; text-decoration-line: none;" title="Nova remnant">nova remnant</a> in the <a href="https://en.wikipedia.org/wiki/Constellation" style="background: none; color: #0b0080; text-decoration-line: none;" title="Constellation">constellation</a> <a href="https://en.wikipedia.org/wiki/Pyxis" style="background: none; color: #0b0080; text-decoration-line: none;" title="Pyxis">Pyxis</a>. It is a <a href="https://en.wikipedia.org/wiki/Binary_star" style="background: none; color: #0b0080; text-decoration-line: none;" title="Binary star">binary star</a> system and its distance is estimated at about 4,783 parsecs (15,600 light-years) from <a href="https://en.wikipedia.org/wiki/Earth" style="background: none; color: #0b0080; text-decoration-line: none;" title="Earth">Earth</a>. It contains a Sun-like star and a <a href="https://en.wikipedia.org/wiki/White_dwarf" style="background: none; color: #0b0080; text-decoration-line: none;" title="White dwarf">white dwarf</a>. Because of their close proximity and the larger mass of the white dwarf, the latter draws matter from the larger, less massive star. The influx of matter on the white dwarf's surface causes periodic thermonuclear explosions to occur.</div>
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The usual <a href="https://en.wikipedia.org/wiki/Apparent_magnitude" style="background: none; color: #0b0080; text-decoration-line: none;" title="Apparent magnitude">apparent magnitude</a> of this star system is 15.5, but there occurred eruptions with maximal apparent magnitude of about 7.0 in the years 1890, 1902, 1920, 1944, 1966 and 2011.<sup class="reference" id="cite_ref-aavso_alert_3-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/T_Pyxidis#cite_note-aavso_alert-3" style="background: none; color: #0b0080; text-decoration-line: none;">[3]</a></sup> Evidence seems to indicate that T Pyxidis may have increased in mass despite the nova eruptions, and is now close to the <a href="https://en.wikipedia.org/wiki/Chandrasekhar_limit" style="background: none; color: #0b0080; text-decoration-line: none;" title="Chandrasekhar limit">Chandrasekhar limit</a> when it might explode as a supernova.<sup class="reference" id="cite_ref-Sion_soon_4-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/T_Pyxidis#cite_note-Sion_soon-4" style="background: none; color: #0b0080; text-decoration-line: none;">[4]</a></sup> When a white dwarf reaches this limit it will collapse under its own weight and cause a <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Type_1a_supernova" style="background: none; color: #0b0080; text-decoration-line: none;" title="Type 1a supernova">type 1a supernova</a>.</div>
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<span class="mw-headline" id="Effect_on_Earth"><span style="font-size: small;">Effect on Earth</span></span></h2>
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Because of its relative proximity, some—in particular, Edward Sion, astronomer & astrophysicist at <a href="https://en.wikipedia.org/wiki/Villanova_University" style="background: none; color: #0b0080; text-decoration-line: none;" title="Villanova University">Villanova University</a>, and his team therefrom—contend that a type 1a supernova could have a significant impact on Earth. The received <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Gamma_radiation" style="background: none; color: #0b0080; text-decoration-line: none;" title="Gamma radiation">gamma radiation</a> would equal the total (all spectra) radiation of approximately 1,000 solar flares,<sup class="reference" id="cite_ref-TASS_5-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/T_Pyxidis#cite_note-TASS-5" style="background: none; color: #0b0080; text-decoration-line: none;">[5]</a></sup> but the type Ia supernova would have to be closer than 1,000 parsecs (3,300 light-years) to cause significant damage to the <a href="https://en.wikipedia.org/wiki/Ozone_layer" style="background: none; color: #0b0080; text-decoration-line: none;" title="Ozone layer">ozone layer</a>, and perhaps closer than 500 parsecs. The <a href="https://en.wikipedia.org/wiki/X-ray" style="background: none; color: #0b0080; text-decoration-line: none;" title="X-ray">X-radiation</a> that reaches Earth in such an event, however, would be less than the X-radiation of a single average solar flare.<sup class="reference" id="cite_ref-TASS_5-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/T_Pyxidis#cite_note-TASS-5" style="background: none; color: #0b0080; text-decoration-line: none;">[5]</a></sup></div>
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However, Sion's calculations were challenged by <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Alex_Filippenko" style="background: none; color: #0b0080; text-decoration-line: none;" title="Alex Filippenko">Alex Filippenko</a> of the <a class="mw-redirect" href="https://en.wikipedia.org/wiki/University_of_California_at_Berkeley" style="background: none; color: #0b0080; text-decoration-line: none;" title="University of California at Berkeley">University of California at Berkeley</a> who said that Sion had possibly miscalculated the damage that could be caused by a T Pyxidis supernova. He had used data for a far more deadly <a href="https://en.wikipedia.org/wiki/Gamma-ray_burst" style="background: none; color: #0b0080; text-decoration-line: none;" title="Gamma-ray burst">gamma-ray burst</a> (GRB) occurring 1 kilo<a href="https://en.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration-line: none;" title="Parsec">parsec</a> from Earth, not a supernova, and T Pyxidis certainly is not expected to produce a GRB.<sup class="reference" id="cite_ref-Neill_6-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/T_Pyxidis#cite_note-Neill-6" style="background: none; color: #0b0080; text-decoration-line: none;">[6]</a></sup> According to another expert, "[a] supernova would have to be 10 times closer [to Earth] to do the damage described."<sup class="reference" id="cite_ref-Neill_6-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/T_Pyxidis#cite_note-Neill-6" style="background: none; color: #0b0080; text-decoration-line: none;">[6]</a></sup> <a href="https://en.wikipedia.org/wiki/Human" style="background: none; color: #0b0080; text-decoration-line: none;" title="Human">Mankind</a> survived when the <a href="https://en.wikipedia.org/wiki/Crab_Nebula" style="background: none; color: #0b0080; text-decoration-line: none;" title="Crab Nebula">Crab Nebula</a> supernova went off at a distance of about 6,500 light-years in the year 1054. If this star were to explode as a type Ia supernova at its estimated distance of 3,300 light-years, it would have an apparent magnitude of around -9.3, about as bright as the brightest <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Iridium_flare" style="background: none; color: #0b0080; text-decoration-line: none;" title="Iridium flare">Iridium (satellite) flares</a>.<sup class="reference" id="cite_ref-7" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/T_Pyxidis#cite_note-7" style="background: none; color: #0b0080; text-decoration-line: none;">[7]</a></sup></div>
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Recent data indicates his distance estimate is five times too close. Astronomers used NASA's <a href="https://en.wikipedia.org/wiki/Hubble_Space_Telescope" style="background: none; color: #0b0080; text-decoration-line: none;" title="Hubble Space Telescope">Hubble Space Telescope</a> to observe the light emitted during its latest outburst in April 2011. The team also used the light echo to refine estimates of the nova's distance from Earth. The new distance is 15,600 light-years (4780 pc) from Earth. Previous estimates were between 6,500 and 16,000 light-years (2000 and 4900 pc).<sup class="reference" id="cite_ref-8" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/T_Pyxidis#cite_note-8" style="background: none; color: #0b0080; text-decoration-line: none;">[8]</a></sup></div>
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It has been reported that T Pyx would "soon" become a supernova.<sup class="reference" id="cite_ref-Sion_soon_4-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/T_Pyxidis#cite_note-Sion_soon-4" style="background: none; color: #0b0080; text-decoration-line: none;">[4]</a></sup> However, when contacted by <a href="https://en.wikipedia.org/wiki/Scientific_American" style="background: none; color: #0b0080; text-decoration-line: none;" title="Scientific American">Scientific American</a>, it became apparent that "soon" was meant in astronomical terms: Dr. Sion said that "soon" in the press announcement meant "[a]t the accretion rate we derived, the white dwarf in T Pyxidis will reach the Chandrasekhar Limit in ten million years."<sup class="reference" id="cite_ref-9" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/T_Pyxidis#cite_note-9" style="background: none; color: #0b0080; text-decoration-line: none;">[9]</a></sup> By that time it will have moved far enough away from the solar system to have little effect.</div>
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<a class="internal" href="https://en.wikipedia.org/wiki/File:T-Pyx-Lightcurve-AAVSO.gif" style="background: linear-gradient(transparent, transparent), url("data:image/svg+xml,%3C%3Fxml%20version%3D%221.0%22%20encoding%3D%22UTF-8%22%20standalone%3D%22no%22%3F%3E%0A%3Csvg%20xmlns%3D%22http%3A%2F%2Fwww.w3.org%2F2000%2Fsvg%22%20viewBox%3D%220%200%2011%2015%22%20width%3D%2215%22%20height%3D%2211%22%3E%0A%20%20%20%20%3Cg%20id%3D%22magnify-clip%22%20fill%3D%22%23fff%22%20stroke%3D%22%23000%22%3E%0A%20%20%20%20%20%20%20%20%3Cpath%20id%3D%22bigbox%22%20d%3D%22M1.509%201.865h10.99v7.919h-10.99z%22%2F%3E%0A%20%20%20%20%20%20%20%20%3Cpath%20id%3D%22smallbox%22%20d%3D%22M-1.499%206.868h5.943v4.904h-5.943z%22%2F%3E%0A%20%20%20%20%3C%2Fg%3E%0A%3C%2Fsvg%3E%0A"); color: #0b0080; display: block; height: 11px; overflow: hidden; text-decoration-line: none; text-indent: 15px; user-select: none; white-space: nowrap; width: 15px;" title="Enlarge"></a></div>
<a href="https://en.wikipedia.org/wiki/American_Association_of_Variable_Star_Observers" style="background: none; color: #0b0080; text-decoration-line: none;" title="American Association of Variable Star Observers">AAVSO</a> <a href="https://en.wikipedia.org/wiki/Light_curve" style="background: none; color: #0b0080; text-decoration-line: none;" title="Light curve">light curve</a> of <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Recurrent_nova" style="background: none; color: #0b0080; text-decoration-line: none;" title="Recurrent nova">recurrent nova</a> T Pyx from 1 Jan 1966 to 17 Nov 2010. Up is brighter and down is fainter. Day numbers are <a href="https://en.wikipedia.org/wiki/Julian_day" style="background: none; color: #0b0080; text-decoration-line: none;" title="Julian day">Julian days</a>. Different colors reflect different <a href="https://en.wikipedia.org/wiki/Photometric_system" style="background: none; color: #0b0080; text-decoration-line: none;" title="Photometric system">bandpasses</a>.</div>
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<span class="mw-headline" id="2011_Outburst"><span style="font-size: small;">2011 Outburst</span></span></h2>
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Mike Linnolt has detected T Pyx first outburst in nearly 45 years. He detected it on April 14, 2011 at magnitude 13.<sup class="reference" id="cite_ref-aavso_alert_3-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/T_Pyxidis#cite_note-aavso_alert-3" style="background: none; color: #0b0080; text-decoration-line: none;">[3]</a></sup> According to AAVSO observers, it reached magnitude 7.5 in the visual and V bands by April 27,<sup class="reference" id="cite_ref-10" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/T_Pyxidis#cite_note-10" style="background: none; color: #0b0080; text-decoration-line: none;">[10]</a></sup>and reached magnitude 6.8 by May 3.<sup class="reference" id="cite_ref-11" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/T_Pyxidis#cite_note-11" style="background: none; color: #0b0080; text-decoration-line: none;">[11]</a></sup></div>
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<a class="internal" href="https://en.wikipedia.org/wiki/File:T-Pyx-Lightcurve-2011-Eruption-AAVSO.jpg" style="background: linear-gradient(transparent, transparent), url("data:image/svg+xml,%3C%3Fxml%20version%3D%221.0%22%20encoding%3D%22UTF-8%22%20standalone%3D%22no%22%3F%3E%0A%3Csvg%20xmlns%3D%22http%3A%2F%2Fwww.w3.org%2F2000%2Fsvg%22%20viewBox%3D%220%200%2011%2015%22%20width%3D%2215%22%20height%3D%2211%22%3E%0A%20%20%20%20%3Cg%20id%3D%22magnify-clip%22%20fill%3D%22%23fff%22%20stroke%3D%22%23000%22%3E%0A%20%20%20%20%20%20%20%20%3Cpath%20id%3D%22bigbox%22%20d%3D%22M1.509%201.865h10.99v7.919h-10.99z%22%2F%3E%0A%20%20%20%20%20%20%20%20%3Cpath%20id%3D%22smallbox%22%20d%3D%22M-1.499%206.868h5.943v4.904h-5.943z%22%2F%3E%0A%20%20%20%20%3C%2Fg%3E%0A%3C%2Fsvg%3E%0A"); color: #0b0080; display: block; height: 11px; overflow: hidden; text-decoration-line: none; text-indent: 15px; user-select: none; white-space: nowrap; width: 15px;" title="Enlarge"></a></div>
<a href="https://en.wikipedia.org/wiki/American_Association_of_Variable_Star_Observers" style="background: none; color: #0b0080; text-decoration-line: none;" title="American Association of Variable Star Observers">AAVSO</a> <a href="https://en.wikipedia.org/wiki/Light_curve" style="background: none; color: #0b0080; text-decoration-line: none;" title="Light curve">light curve</a> of <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Recurrent_nova" style="background: none; color: #0b0080; text-decoration-line: none;" title="Recurrent nova">recurrent nova</a> T Pyx from April 13 to May 6, 2011. Up is brighter and down is fainter.</div>
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<span style="font-size: small;"><span class="mw-headline" id="X-ray_source">X-ray source</span><span class="mw-editsection" style="display: inline-block; font-family: sans-serif; line-height: 1em; margin-left: 1em; unicode-bidi: isolate; user-select: none; vertical-align: baseline; white-space: nowrap;"></span></span></h2>
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T Pyxidis is a <a href="https://en.wikipedia.org/wiki/Super_soft_X-ray_source" style="background: none; color: #0b0080;" title="Super soft X-ray source">super soft X-ray source</a>.<sup class="reference" id="cite_ref-Ogley_12-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/T_Pyxidis#cite_note-Ogley-12" style="background: none; color: #0b0080; text-decoration-line: none;">[12]</a></sup></div>
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<span style="color: #222222; font-family: sans-serif;"><span style="font-size: 14px;"><b><a href="https://en.wikipedia.org/wiki/T_Pyxidis">https://en.wikipedia.org/wiki/T_Pyxidis</a></b></span></span></div>
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A <b>nova remnant</b> is made up of the material either left behind by a sudden explosive fusion eruption by classical <a href="https://en.wikipedia.org/wiki/Nova" style="background: none; color: #0b0080; text-decoration-line: none;" title="Nova">novae</a>, or from multiple ejections by recurrent <a href="https://en.wikipedia.org/wiki/Nova" style="background: none; color: #0b0080; text-decoration-line: none;" title="Nova">novae</a>. Over their short lifetimes, this novae shell shows expansion velocities are around 1000 km/s<sup class="reference" id="cite_ref-Lloyd1997_1-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Nova_remnant#cite_note-Lloyd1997-1" style="background: none; color: #0b0080; text-decoration-line: none;">[1]</a></sup>, whose faint nebulosity usually are illuminated by their progenitor stars via <a href="https://en.wikipedia.org/wiki/Light_echo" style="background: none; color: #0b0080; text-decoration-line: none;" title="Light echo">light echos</a> as observed with the spherical shell<sup class="reference" id="cite_ref-Lloyd1997_1-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Nova_remnant#cite_note-Lloyd1997-1" style="background: none; color: #0b0080; text-decoration-line: none;">[1]</a></sup> of <a href="https://en.wikipedia.org/wiki/GK_Persei" style="background: none; color: #0b0080; text-decoration-line: none;" title="GK Persei">Nova Persei 1901</a><sup class="reference" id="cite_ref-Liimets2014_2-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Nova_remnant#cite_note-Liimets2014-2" style="background: none; color: #0b0080; text-decoration-line: none;">[2]</a></sup> or the energies remaining in the expanding bubbles like <a href="https://en.wikipedia.org/wiki/T_Pyxidis" style="background: none; color: #0b0080; text-decoration-line: none;" title="T Pyxidis">T Pyxidis</a>.<sup class="reference" id="cite_ref-Ogley_3-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Nova_remnant#cite_note-Ogley-3" style="background: none; color: #0b0080; text-decoration-line: none;">[3]</a></sup></div>
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As most novae require a close binary system, with a white dwarf and main sequence, sub-giant; or the merging of two red dwarfs; so probably all novae remnants must be associated with binaries<sup class="reference" id="cite_ref-Bode2002_4-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Nova_remnant#cite_note-Bode2002-4" style="background: none; color: #0b0080; text-decoration-line: none;">[4]</a></sup>. This theortically means these nebulae shapes might be affected by their central progenitor stars and the amount of matter ejected by novae.<sup class="reference" id="cite_ref-Lloyd1997_1-2" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Nova_remnant#cite_note-Lloyd1997-1" style="background: none; color: #0b0080; text-decoration-line: none;">[1]</a></sup>Shapes of these novae nebulae is of much interest to modern astrophysicists.<sup class="reference" id="cite_ref-Lloyd1997_1-3" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Nova_remnant#cite_note-Lloyd1997-1" style="background: none; color: #0b0080; text-decoration-line: none;">[1]</a></sup><sup class="reference" id="cite_ref-Bode2002_4-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Nova_remnant#cite_note-Bode2002-4" style="background: none; color: #0b0080; text-decoration-line: none;">[4]</a></sup></div>
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<span style="color: #222222; font-family: sans-serif;">A </span><b style="color: #222222; font-family: sans-serif;">nova</b><span style="color: #222222; font-family: sans-serif;"> (plural </span><i style="color: #222222; font-family: sans-serif;"><a class="extiw" href="https://en.wiktionary.org/wiki/nova" style="background: none; color: #663366; text-decoration-line: none;" title="wiktionary:nova">novae</a></i><span style="color: #222222; font-family: sans-serif;"> or </span><i style="color: #222222; font-family: sans-serif;">novas</i><span style="color: #222222; font-family: sans-serif;">) or </span><b style="color: #222222; font-family: sans-serif;">classical nova</b><span style="color: #222222; font-family: sans-serif;"> (CN or plural CNe) is an astronomical event that causes the sudden appearance of a bright "new" star, that slowly fades from view over several weeks or many months. Novae should not be confused with other more energetic astronomical phenomena known as </span><a href="https://en.wikipedia.org/wiki/Supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Supernova">supernovae</a><span style="color: #222222; font-family: sans-serif;"> (SNe), which catastrophically destroys massive stars or white dwarfs.</span></div>
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<span style="color: #222222; font-family: sans-serif;">Recurrent novae (RNe) are objects that have been seen to experience multiple nova eruptions. There are some ten known galactic recurrent novae.</span><sup class="reference" id="cite_ref-Schaefer2009_16-0" style="color: #222222; font-family: sans-serif; line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Nova#cite_note-Schaefer2009-16" style="background: none; color: #0b0080; text-decoration-line: none;">[16]</a></sup><span style="color: #222222; font-family: sans-serif;"> The recurrent nova typically brightens by about 8.6 magnitude, whereas a classic nova brightens by more than 12 magnitude.</span><sup class="reference" id="cite_ref-Schaefer2009_16-1" style="color: #222222; font-family: sans-serif; line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Nova#cite_note-Schaefer2009-16" style="background: none; color: #0b0080; text-decoration-line: none;">[16]</a></sup><span style="color: #222222; font-family: sans-serif;"> </span></div>
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<span style="color: #222222; font-family: sans-serif;"><a href="https://en.wikipedia.org/wiki/Nova#Recurrent_novae">https://en.wikipedia.org/wiki/Nova#Recurrent_novae</a></span></div>
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T Pyxidis in outburst on April 15th. North is up. See <a class="fancybox image" href="http://i176.photobucket.com/albums/w189/walcom77/T_Pyx_animation_April_15_2011.gif" style="border: 0px; color: #006699; margin: 0px; outline: dotted thin; padding: 0px;" target="new_window">before-and-after animation</a>.</div>
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Ernesto Guido and Giovanni Sostero</div>
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<span style="background-color: white; color: #333333; font-family: "Lucida Sans", Arial, Helvetica, sans-serif; text-align: start;">The recurrent nova </span><a href="http://en.wikipedia.org/wiki/T_Pyxidis" style="background-color: white; border: 0px; color: #006699; font-family: "Lucida Sans", Arial, Helvetica, sans-serif; margin: 0px; outline: none; padding: 0px; text-align: start; text-decoration-line: none;" target="new_window">T Pyxidis</a><span style="background-color: white; color: #333333; font-family: "Lucida Sans", Arial, Helvetica, sans-serif; text-align: start;">, which had its last outburst in December 1966 and has been </span><i style="background-color: white; border: 0px; color: #333333; font-family: "Lucida Sans", Arial, Helvetica, sans-serif; margin: 0px; padding: 0px; text-align: start;">very</i><span style="background-color: white; color: #333333; font-family: "Lucida Sans", Arial, Helvetica, sans-serif; text-align: start;"> overdue for its next, finally began a new flareup on April 14th. By the next day it had brightened to about magnitude 8.4. In 1966–67 it reached 6.5 within about a month, and now it has done so again.</span></div>
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Here's a <a class="fancybox image" href="http://i176.photobucket.com/albums/w189/walcom77/T_Pyx_animation_April_15_2011.gif" style="border: 0px; color: #006699; margin: 0px; outline: none; padding: 0px; text-decoration-line: none;" target="new_window">blink animation</a> showing before and after, courtesy Ernesto Guido and Giovanni Sostero in Italy. South is up.</div>
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The star is in the dim constellation Pyxis east of Puppis and Canis Major, sinling out of sight for northern observers in May. (Here are <a class="fancybox image" href="http://www.aavso.org/sites/default/files/images/locatetpyx.jpg" style="border: 0px; color: #006699; margin: 0px; outline: none; padding: 0px; text-decoration-line: none;" target="new_window">finder and comparison-star charts</a> from <i style="border: 0px; margin: 0px; padding: 0px;">Sky & Telescope</i>. For larger-scale comparison-star charts, you can use the <a href="http://www.aavso.org/vsp" style="border: 0px; color: #006699; margin: 0px; outline: none; padding: 0px; text-decoration-line: none;" target="new_window">chart-making site</a> of the American Association of Variable Star Observers).</div>
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<a href="http://remanzacco.blogspot.com/2011/04/t-pyxidis-outburst.html" style="border: 0px; color: #006699; margin: 0px; outline: none; padding: 0px; text-decoration-line: none;" target="new_window">More information</a> on T Pyx. Old but good <a href="http://www.aavso.org/vsots_tpyx" style="border: 0px; color: #006699; margin: 0px; outline: none; padding: 0px; text-decoration-line: none;" target="new_window">AAVSO article</a>. Current <a href="http://www.aavso.org/campaign-monitor-recurrent-nova-t-pyx-throughout-2011-eruption" style="border: 0px; color: #006699; margin: 0px; outline: none; padding: 0px; text-decoration-line: none;" target="new_window">AAVSO observing campaign page</a>.</div>
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As a white dwarf accreting mass from a binary partner, T Pyx is a prime candidate to explode completely as a Type Ia supernova within the next 10 million years. Last year, careless reporting led to a flurry of media buzz that if it blows up soon it could endanger Earth. Not so. At its distance of about 3,000 light-years, T Pyx would shine as brightly as magnitude –9 if it went Type Ia (as bright as a thick crescent Moon), but its radiation wouldn't harm us. The current <a href="http://en.wikipedia.org/wiki/T_Pyxidis" style="border: 0px; color: #006699; margin: 0px; outline: none; padding: 0px; text-decoration-line: none;" target="new_window">Wikipedia article on T Pyx</a> explains this story well.</div>
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In its past known outbursts (1890, 1902, 1920, 1944, and 1966), T Pyx took about 20 days to reach 7th magnitude or so and remained 8th mag or brighter for about two months.</div>
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Elaborating on this, Bradley Schaefer writes: "Judging from the 1967 eruption light curve, the current eruption light curve will... slowly rise to a peak near V=6.4 around 20 May, slowly fade to V=10 by middle August, then have a sudden drop by two magnitudes over the next 20 days (with drop being invisible due to the Sun). The 1967 eruption did show fast intra-night variations, but the old data does not have the time resolution to tell what is going on."</div>
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<i style="border: 0px; margin: 0px; padding: 0px;"><b style="border: 0px; margin: 0px; padding: 0px;">UPDATE May 13:</b></i> As T Pyx disappears to the twilight horizon for Northern Hemisphere observers, it has brightened to magnitude 6.5 as of last night according to various observers reporting to the AAVSO. Here are <a href="http://www.aavso.org/ql/results?auid=000-BBQ-228&startjd=2455579.06829" style="border: 0px; color: #006699; margin: 0px; outline: none; padding: 0px; text-decoration-line: none;" target="new_window">recent observations</a> and a <a href="http://www.aavso.org/lcg/plot?auid=000-BBQ-228&starname=T%20PYX&lastdays=50&start=&stop=&obscode=&obscode_symbol=2&obstotals=no&grid=on&visual=on&v=on&pointsize=1&width=800&height=450&mag1=&mag2=&mean=&vmean=" style="border: 0px; color: #006699; margin: 0px; outline: none; padding: 0px; text-decoration-line: none;" target="new_window">light curve</a> for the most recent 50 days.</div>
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<span style="color: #333333; font-family: Lucida Sans, Arial, Helvetica, sans-serif;"><span style="font-size: 13px;"><a href="http://www.skyandtelescope.com/astronomy-news/observing-news/t-pyxidis-finally-blows-again/"><b>http://www.skyandtelescope.com/astronomy-news/observing-news/t-pyxidis-finally-blows-again/</b></a></span></span></div>
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https://pt.wikipedia.org/wiki/Pyxis#/media/File:Pyxis_constellation_map.svg</div>
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<span class="mw-mmv-title" original-title="" style="display: inline-block;"><a href="https://commons.wikimedia.org/wiki/Pyxis" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration-line: none;" title="Pyxis">Pyxis</a> constellation map - </span><span style="background-color: #f8f9fa; color: #54595d; font-size: 13.6px;"> </span><a href="https://commons.wikimedia.org/wiki/File:Pyxis_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-size: 13.6px; text-decoration-line: none;" title="File:Pyxis constellation map.png">Pyxis_constellation_map.png</a><span style="background-color: #f8f9fa; color: #54595d; font-size: 13.6px;">:</span><span style="background-color: #f8f9fa; color: #54595d; font-size: 13.6px;"> </span><a class="extiw" href="https://en.wikipedia.org/wiki/User:Bronger" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-size: 13.6px; text-decoration-line: none;" title="en:User:Bronger">Torsten Bronge</a></div>
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<span style="font-family: "Times New Roman", serif; font-size: 9.5pt;"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/home.html" target="index"><b><span lang="EN-US" style="color: blue; font-size: 13.5pt; text-decoration-line: none;">Star Names </span></b><b><span lang="EN-US" style="color: blue; font-size: 13.5pt; text-decoration-line: none;"><br /></span></b><b><span lang="EN-US" style="color: blue; font-size: 11.5pt; text-decoration-line: none;">Their Lore and Meaning </span></b><b><span lang="EN-US" style="color: blue; text-decoration-line: none;"><br /></span></b><b><span lang="EN-US" style="color: blue;">by</span></b><b><span lang="EN-US" style="color: blue; text-decoration-line: none;"> </span></b><b><span lang="EN-US" style="color: blue; text-decoration-line: none;"><br /></span></b><b><span lang="EN-US" style="color: blue; font-size: 13.5pt; text-decoration-line: none;">Richard Hinckley Allen </span></b></a></span><span lang="EN-US" style="font-family: "Times New Roman", serif; font-size: 9.5pt;"><br />as reprinted</span><span lang="EN-US" style="font-family: "Times New Roman", serif; font-size: 9.5pt;"> </span><span lang="EN-US" style="font-family: "Times New Roman", serif; font-size: 9.5pt;"><br />in the Dover edition, 1963<o:p></o:p></span></div>
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<span lang="EN-US" style="font-family: "Times New Roman", serif; font-size: 9.5pt;">The text is in the public domain.</span></div>
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<span style="font-family: "Times New Roman", serif; font-size: 9.5pt;">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Pyxis*.html<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "Palatino Linotype", serif; font-size: 12pt;">p348</span><b><span lang="EN-US" style="color: #000066; font-family: "Palatino Linotype", serif; font-size: 14.5pt;">Pyxis Nautica, the Mariner's Compass.<o:p></o:p></span></b></div>
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<b><span lang="EN-US" style="color: #000066; font-family: "Palatino Linotype", serif; font-size: 13.5pt;">Pyxis</span></b><span lang="EN-US" style="color: #000066; font-family: "Palatino Linotype", serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "Palatino Linotype", serif; font-size: 13.5pt;">was formed by La Caille from stars in the Mast of Argo, and so associated with the Ship, although there, of course, it is an anachronism.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "Palatino Linotype", serif; font-size: 13.5pt;">Baily reannexed it to Argo, since four of its members had been placed by Ptolemy where La Caille found them, so that for a time it fell into disuse; but Gould inserted it in his</span><span lang="EN-US" style="color: #000066; font-family: "Palatino Linotype", serif; font-size: 13.5pt;"> </span><i><span lang="EN-US" style="color: #000066; font-family: "Palatino Linotype", serif; font-size: 13.5pt;">Uranometria Argentina</span></i><span lang="EN-US" style="color: #000066; font-family: "Palatino Linotype", serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "Palatino Linotype", serif; font-size: 13.5pt;">of 1879, with sixty-six stars from 3.8 to 7th magnitudes.<o:p></o:p></span></div>
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<span lang="EN-US"><span style="font-family: "Times New Roman", serif; font-size: 12.6667px; text-align: center;"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Pyxis*.html">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Pyxis*.html</a></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Stellarium</span></div>
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<b>Pyxis</b> (<span class="nowrap" style="white-space: nowrap;"><span class="IPA nopopups"><a href="https://en.wikipedia.org/wiki/Help:IPA_for_English" style="background: none; color: #0b0080; text-decoration-line: none !important;" title="Help:IPA for English">/<span style="border-bottom: 1px dotted;"><span title="/ˈ/ primary stress follows">ˈ</span><span title="'p' in 'pie'">p</span><span title="/ɪ/ short 'i' in 'bid'">ɪ</span><span title="'k' in 'kind'">k</span><span title="'s' in 'sigh'">s</span><span title="/ɪ/ or /ə/ 'e' in 'roses'">ᵻ</span><span title="'s' in 'sigh'">s</span></span>/</a></span></span>; <a href="https://en.wikipedia.org/wiki/Latin" style="background: none; color: #0b0080; text-decoration-line: none;" title="Latin">Latin</a> for a small medicinal <a href="https://en.wikipedia.org/wiki/Box" style="background: none; color: #0b0080; text-decoration-line: none;" title="Box">box</a>) is a small and faint <a href="https://en.wikipedia.org/wiki/Constellation" style="background: none; color: #0b0080; text-decoration-line: none;" title="Constellation">constellation</a> in the southern sky. Abbreviated from <b>Pyxis Nautica</b>, its name is <a href="https://en.wikipedia.org/wiki/Latin" style="background: none; color: #0b0080; text-decoration-line: none;" title="Latin">Latin</a> for a <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Mariner%27s_compass" style="background: none; color: #0b0080; text-decoration-line: none;" title="Mariner's compass">mariner's compass</a> (contrasting with <a href="https://en.wikipedia.org/wiki/Circinus" style="background: none; color: #0b0080; text-decoration-line: none;" title="Circinus">Circinus</a>, which represents a <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Draftsman%27s_compasses" style="background: none; color: #0b0080; text-decoration-line: none;" title="Draftsman's compasses">draftsman's compasses</a>). Pyxis was introduced by <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background: none; color: #0b0080; text-decoration-line: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a> in the 18th century, and is counted among the <a href="https://en.wikipedia.org/wiki/88_modern_constellations" style="background: none; color: #0b0080; text-decoration-line: none;" title="88 modern constellations">88 modern constellations</a>. The constellation is located close to those forming the old constellation of the ship <a href="https://en.wikipedia.org/wiki/Argo_Navis" style="background: none; color: #0b0080; text-decoration-line: none;" title="Argo Navis">Argo Navis</a>, and in the 19th century astronomer <a href="https://en.wikipedia.org/wiki/John_Herschel" style="background: none; color: #0b0080; text-decoration-line: none;" title="John Herschel">John Herschel</a> suggested renaming Pyxis to Malus, the <a href="https://en.wikipedia.org/wiki/Mast_(sailing)" style="background: none; color: #0b0080; text-decoration-line: none;" title="Mast (sailing)">mast</a>, but the suggestion was not followed. Pyxis is completely visible from latitudes south of <a href="https://en.wikipedia.org/wiki/53rd_parallel_north" style="background: none; color: #0b0080; text-decoration-line: none;" title="53rd parallel north">53 degrees north</a>, with its best evening-sky visibility in February and March.</div>
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The <a href="https://en.wikipedia.org/wiki/Galactic_plane" style="background: none; color: #0b0080; text-decoration-line: none;" title="Galactic plane">plane</a> of the <a href="https://en.wikipedia.org/wiki/Milky_Way" style="background: none; color: #0b0080; text-decoration-line: none;" title="Milky Way">Milky Way</a> passes through Pyxis. A faint constellation, its three brightest stars—<a href="https://en.wikipedia.org/wiki/Alpha_Pyxidis" style="background: none; color: #0b0080; text-decoration-line: none;" title="Alpha Pyxidis">Alpha</a>, <a href="https://en.wikipedia.org/wiki/Beta_Pyxidis" style="background: none; color: #0b0080; text-decoration-line: none;" title="Beta Pyxidis">Beta</a> and <a href="https://en.wikipedia.org/wiki/Gamma_Pyxidis" style="background: none; color: #0b0080; text-decoration-line: none;" title="Gamma Pyxidis">Gamma Pyxidis</a>—are in a rough line. At magnitude 3.68, Alpha is the constellation's brightest star. It is a blue-white star around 22,000 times as <a href="https://en.wikipedia.org/wiki/Luminosity" style="background: none; color: #0b0080; text-decoration-line: none;" title="Luminosity">luminous</a> as the Sun. Near Alpha is <a href="https://en.wikipedia.org/wiki/T_Pyxidis" style="background: none; color: #0b0080; text-decoration-line: none;" title="T Pyxidis">T Pyxidis</a>, a <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Recurrent_nova" style="background: none; color: #0b0080; text-decoration-line: none;" title="Recurrent nova">recurrent nova</a> that has flared up to <a href="https://en.wikipedia.org/wiki/Apparent_magnitude" style="background: none; color: #0b0080; text-decoration-line: none;" title="Apparent magnitude">magnitude</a> 7 every few decades. Three star systems have planets, all discovered by <a href="https://en.wikipedia.org/wiki/Doppler_spectroscopy" style="background: none; color: #0b0080; text-decoration-line: none;" title="Doppler spectroscopy">doppler spectroscopy</a>.</div>
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<span style="font-size: small;">History</span></h2>
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In ancient <a href="https://en.wikipedia.org/wiki/Chinese_astronomy" style="background: none; color: #0b0080; text-decoration-line: none;" title="Chinese astronomy">Chinese astronomy</a>, Alpha, Beta and Gamma Pyxidis formed part of <i>Tianmiao</i>, a celestial temple honouring the ancestors of the emperor, along with stars from neighbouring <a href="https://en.wikipedia.org/wiki/Antlia" style="background: none; color: #0b0080; text-decoration-line: none;" title="Antlia">Antlia</a>.<sup class="reference" id="cite_ref-startales_1-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-startales-1" style="background: none; color: #0b0080; text-decoration-line: none;">[1]</a></sup></div>
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The French astronomer <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background: none; color: #0b0080; text-decoration-line: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a> first described the <a href="https://en.wikipedia.org/wiki/Constellation" style="background: none; color: #0b0080; text-decoration-line: none;" title="Constellation">constellation</a> in French as <i>la Boussole</i> (the Marine Compass) in 1752,<sup class="reference" id="cite_ref-ridpathlac_2-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-ridpathlac-2" style="background: none; color: #0b0080; text-decoration-line: none;">[2]</a></sup><sup class="reference" id="cite_ref-3" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-3" style="background: none; color: #0b0080; text-decoration-line: none;">[3]</a></sup> after he had observed and catalogued almost 10,000 southern stars during a two-year stay at the <a href="https://en.wikipedia.org/wiki/Cape_of_Good_Hope" style="background: none; color: #0b0080; text-decoration-line: none;" title="Cape of Good Hope">Cape of Good Hope</a>. He devised fourteen new constellations in uncharted regions of the <a href="https://en.wikipedia.org/wiki/Southern_Celestial_Hemisphere" style="background: none; color: #0b0080; text-decoration-line: none;" title="Southern Celestial Hemisphere">Southern Celestial Hemisphere</a> not visible from Europe. All but one honoured instruments that symbolised the <a href="https://en.wikipedia.org/wiki/Age_of_Enlightenment" style="background: none; color: #0b0080; text-decoration-line: none;" title="Age of Enlightenment">Age of Enlightenment</a>.<sup class="reference" id="cite_ref-5" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-5" style="background: none; color: #0b0080; text-decoration-line: none;">[a]</a></sup> Lacaille Latinised the name to <i>Pixis</i> [sic] <i>Nautica</i> on his 1763 chart.<sup class="reference" id="cite_ref-wagman_4-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-wagman-4" style="background: none; color: #0b0080; text-decoration-line: none;">[4]</a></sup> The Ancient Greeks identified the four main stars of Pyxis as the mast of the great ship <i><a href="https://en.wikipedia.org/wiki/Argo_Navis" style="background: none; color: #0b0080; text-decoration-line: none;" title="Argo Navis">Argo Navis</a></i>.<sup class="reference" id="cite_ref-6" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-6" style="background: none; color: #0b0080; text-decoration-line: none;">[5]</a></sup></div>
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German astronomer <a href="https://en.wikipedia.org/wiki/Johann_Elert_Bode" style="background: none; color: #0b0080; text-decoration-line: none;" title="Johann Elert Bode">Johann Bode</a> defined the constellation Lochium Funis, the Log and Line—a nautical device once used for measuring speed and distance travelled at sea—around Pyxis in his 1801 star atlas, but the depiction did not survive.<sup class="reference" id="cite_ref-startales2_7-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-startales2-7" style="background: none; color: #0b0080; text-decoration-line: none;">[6]</a></sup> In 1844 <a href="https://en.wikipedia.org/wiki/John_Herschel" style="background: none; color: #0b0080; text-decoration-line: none;" title="John Herschel">John Herschel</a> attempted to resurrect the classical configuration of Argo Navis by renaming it Malus the Mast, a suggestion followed by <a href="https://en.wikipedia.org/wiki/Francis_Baily" style="background: none; color: #0b0080; text-decoration-line: none;" title="Francis Baily">Francis Baily</a>, but <a href="https://en.wikipedia.org/wiki/Benjamin_Apthorp_Gould" style="background: none; color: #0b0080; text-decoration-line: none;" title="Benjamin Apthorp Gould">Benjamin Gould</a> restored Lacaille's nomenclature.<sup class="reference" id="cite_ref-wagman_4-2" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-wagman-4" style="background: none; color: #0b0080; text-decoration-line: none;">[4]</a></sup></div>
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<span style="font-size: small;">Characteristics</span></h2>
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Covering 220.8 square degrees and hence 0.535% of the sky, Pyxis ranks 65th of the <a href="https://en.wikipedia.org/wiki/88_modern_constellations" style="background: none; color: #0b0080; text-decoration-line: none;" title="88 modern constellations">88 modern constellations</a> by area.<sup class="reference" id="cite_ref-tirionconst_8-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-tirionconst-8" style="background: none; color: #0b0080; text-decoration-line: none;">[7]</a></sup> Its position in the <a href="https://en.wikipedia.org/wiki/Southern_Celestial_Hemisphere" style="background: none; color: #0b0080; text-decoration-line: none;" title="Southern Celestial Hemisphere">Southern Celestial Hemisphere</a> means that the whole constellation is visible to observers south of <a href="https://en.wikipedia.org/wiki/52nd_parallel_north" style="background: none; color: #0b0080; text-decoration-line: none;" title="52nd parallel north">52°N</a>.<sup class="reference" id="cite_ref-tirionconst_8-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-tirionconst-8" style="background: none; color: #0b0080; text-decoration-line: none;">[7]</a></sup><sup class="reference" id="cite_ref-9" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-9" style="background: none; color: #0b0080; text-decoration-line: none;">[b]</a></sup> It is most visible in the evening sky in February and March.<sup class="reference" id="cite_ref-saski_boddy2003_10-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-saski_boddy2003-10" style="background: none; color: #0b0080; text-decoration-line: none;">[8]</a></sup> A small constellation, it is bordered by <a href="https://en.wikipedia.org/wiki/Hydra_(constellation)" style="background: none; color: #0b0080; text-decoration-line: none;" title="Hydra (constellation)">Hydra</a> to the north, <a href="https://en.wikipedia.org/wiki/Puppis" style="background: none; color: #0b0080; text-decoration-line: none;" title="Puppis">Puppis</a> to the west, <a href="https://en.wikipedia.org/wiki/Vela_(constellation)" style="background: none; color: #0b0080; text-decoration-line: none;" title="Vela (constellation)">Vela</a> to the south, and Antlia to the east. The three-letter abbreviation for the constellation, as adopted by the <a href="https://en.wikipedia.org/wiki/International_Astronomical_Union" style="background: none; color: #0b0080; text-decoration-line: none;" title="International Astronomical Union">International Astronomical Union</a> in 1922, is 'Pyx'.<sup class="reference" id="cite_ref-pa30_469_11-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-pa30_469-11" style="background: none; color: #0b0080; text-decoration-line: none;">[9]</a></sup> The official constellation boundaries, as set by <a href="https://en.wikipedia.org/wiki/Eug%C3%A8ne_Joseph_Delporte" style="background: none; color: #0b0080; text-decoration-line: none;" title="Eugène Joseph Delporte">Eugène Delporte</a> in 1930, are defined by a <a href="https://en.wikipedia.org/wiki/Polygon" style="background: none; color: #0b0080; text-decoration-line: none;" title="Polygon">polygon</a> of eight sides (<i>illustrated in infobox</i>). In the <a href="https://en.wikipedia.org/wiki/Equatorial_coordinate_system" style="background: none; color: #0b0080; text-decoration-line: none;" title="Equatorial coordinate system">equatorial coordinate system</a>, the <a href="https://en.wikipedia.org/wiki/Right_ascension" style="background: none; color: #0b0080; text-decoration-line: none;" title="Right ascension">right ascension</a> coordinates of these borders lie between 8<sup style="line-height: 1;">h</sup> 27.7<sup style="line-height: 1;">m</sup> and 9<sup style="line-height: 1;">h</sup> 27.6<sup style="line-height: 1;">m</sup>, while the <a href="https://en.wikipedia.org/wiki/Declination" style="background: none; color: #0b0080; text-decoration-line: none;" title="Declination">declination</a> coordinates are between −17.41° and −37.29°.<sup class="reference" id="cite_ref-boundary_12-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-boundary-12" style="background: none; color: #0b0080; text-decoration-line: none;">[10]</a></sup></div>
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<span style="font-size: small;">Features</span></h2>
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<span style="font-size: small;">Stars</span></h3>
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See also: <a href="https://en.wikipedia.org/wiki/List_of_stars_in_Pyxis" style="background: none; color: #0b0080; text-decoration-line: none;" title="List of stars in Pyxis">List of stars in Pyxis</a></div>
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Lacaille gave <a href="https://en.wikipedia.org/wiki/Bayer_designation" style="background: none; color: #0b0080; text-decoration-line: none;" title="Bayer designation">Bayer designations</a> to ten stars now named Alpha to Lambda Pyxidis, skipping the Greek letters iota and kappa. Although a nautical element, the constellation was not an integral part of the old Argo Navis and hence did not share in the original Bayer designations of that constellation, which were split between Carina, Vela and Puppis.<sup class="reference" id="cite_ref-wagman_4-3" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-wagman-4" style="background: none; color: #0b0080; text-decoration-line: none;">[4]</a></sup> Pyxis is a faint constellation, its three brightest stars—<a href="https://en.wikipedia.org/wiki/Alpha_Pyxidis" style="background: none; color: #0b0080; text-decoration-line: none;" title="Alpha Pyxidis">Alpha</a>, <a href="https://en.wikipedia.org/wiki/Beta_Pyxidis" style="background: none; color: #0b0080; text-decoration-line: none;" title="Beta Pyxidis">Beta</a> and <a href="https://en.wikipedia.org/wiki/Gamma_Pyxidis" style="background: none; color: #0b0080; text-decoration-line: none;" title="Gamma Pyxidis">Gamma Pyxidis</a>—form a rough line.<sup class="reference" id="cite_ref-cambridge_13-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-cambridge-13" style="background: none; color: #0b0080; text-decoration-line: none;">[11]</a></sup> Overall, there are 41 stars within the constellation's borders with <a href="https://en.wikipedia.org/wiki/Apparent_magnitude" style="background: none; color: #0b0080; text-decoration-line: none;" title="Apparent magnitude">apparent magnitudes</a> brighter than or equal to 6.5.<sup class="reference" id="cite_ref-15" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-15" style="background: none; color: #0b0080; text-decoration-line: none;">[c]</a></sup><sup class="reference" id="cite_ref-tirionconst_8-3" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-tirionconst-8" style="background: none; color: #0b0080; text-decoration-line: none;">[7]</a></sup></div>
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With an apparent magnitude of 3.68, Alpha Pyxidis is the brightest star in the constellation.<sup class="reference" id="cite_ref-kaleralpha_16-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-kaleralpha-16" style="background: none; color: #0b0080; text-decoration-line: none;">[13]</a></sup> Located 880 ± 30 <a href="https://en.wikipedia.org/wiki/Light-year" style="background: none; color: #0b0080; text-decoration-line: none;" title="Light-year">light-years</a> distant from Earth,<sup class="reference" id="cite_ref-van_Leeuwen2007_17-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-van_Leeuwen2007-17" style="background: none; color: #0b0080; text-decoration-line: none;">[14]</a></sup> it is a blue-white <a href="https://en.wikipedia.org/wiki/Giant_star" style="background: none; color: #0b0080; text-decoration-line: none;" title="Giant star">giant star</a> of spectral type B1.5III that is around 22,000 times as <a href="https://en.wikipedia.org/wiki/Luminosity" style="background: none; color: #0b0080; text-decoration-line: none;" title="Luminosity">luminous</a> as the <a href="https://en.wikipedia.org/wiki/Sun" style="background: none; color: #0b0080; text-decoration-line: none;" title="Sun">Sun</a> and has 9.4 ± 0.7 times its diameter. It began life with a mass 12.1 ± 0.6 times that of the Sun, almost 15 million years ago.<sup class="reference" id="cite_ref-Nieva_2014_18-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-Nieva_2014-18" style="background: none; color: #0b0080; text-decoration-line: none;">[15]</a></sup> Its light is dimmed by 30% due to <a href="https://en.wikipedia.org/wiki/Cosmic_dust" style="background: none; color: #0b0080; text-decoration-line: none;" title="Cosmic dust">interstellar dust</a>, so would have a brighter magnitude of 3.31 if not for this.<sup class="reference" id="cite_ref-kaleralpha_16-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-kaleralpha-16" style="background: none; color: #0b0080; text-decoration-line: none;">[13]</a></sup> The second brightest star at magnitude 3.97 is Beta Pyxidis, a yellow <a href="https://en.wikipedia.org/wiki/Bright_giant" style="background: none; color: #0b0080; text-decoration-line: none;" title="Bright giant">bright giant</a> or <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Supergiant" style="background: none; color: #0b0080; text-decoration-line: none;" title="Supergiant">supergiant</a> of spectral type G7Ib-II that is around 435 times as luminous as the Sun,<sup class="reference" id="cite_ref-Mcdonald_19-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-Mcdonald-19" style="background: none; color: #0b0080; text-decoration-line: none;">[16]</a></sup> lying 420 ± 10 light-years distant away from Earth.<sup class="reference" id="cite_ref-van_Leeuwen2007_17-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-van_Leeuwen2007-17" style="background: none; color: #0b0080; text-decoration-line: none;">[14]</a></sup> It has a companion star of magnitude 12.5 separated by 9 <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Minute_of_arc" style="background: none; color: #0b0080; text-decoration-line: none;" title="Minute of arc">arcseconds</a>.<sup class="reference" id="cite_ref-20" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-20" style="background: none; color: #0b0080; text-decoration-line: none;">[17]</a></sup> Gamma Pyxidis is a star of magnitude 4.02 that lies 207 ± 2 light-years distant.<sup class="reference" id="cite_ref-van_Leeuwen2007_17-2" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-van_Leeuwen2007-17" style="background: none; color: #0b0080; text-decoration-line: none;">[14]</a></sup> It is an orange giant of spectral type K3III that has cooled and swollen to 3.7 times the diameter of the Sun after exhausting its core hydrogen.<sup class="reference" id="cite_ref-CADARS_21-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-CADARS-21" style="background: none; color: #0b0080; text-decoration-line: none;">[18]</a></sup></div>
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<a href="https://en.wikipedia.org/wiki/Kappa_Pyxidis" style="background: none; color: #0b0080; text-decoration-line: none;" title="Kappa Pyxidis">Kappa Pyxidis</a> was catalogued but not given a Bayer designation by Lacaille, however Gould felt the star was bright enough to warrant a letter.<sup class="reference" id="cite_ref-wagman_4-4" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-wagman-4" style="background: none; color: #0b0080; text-decoration-line: none;">[4]</a></sup> Kappa has a magnitude of 4.62 and is 560 ± 50 light-years distant.<sup class="reference" id="cite_ref-van_Leeuwen2007_17-3" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-van_Leeuwen2007-17" style="background: none; color: #0b0080; text-decoration-line: none;">[14]</a></sup>An orange giant of spectral type K4/K5III,<sup class="reference" id="cite_ref-22" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-22" style="background: none; color: #0b0080; text-decoration-line: none;">[19]</a></sup> Kappa has a luminosity approximately 965 times that of the Sun.<sup class="reference" id="cite_ref-Mcdonald_19-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-Mcdonald-19" style="background: none; color: #0b0080; text-decoration-line: none;">[16]</a></sup> It is separated by 2.1 arcseconds from a magnitude 10 star.<sup class="reference" id="cite_ref-23" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-23" style="background: none; color: #0b0080; text-decoration-line: none;">[20]</a></sup> <a href="https://en.wikipedia.org/wiki/Theta_Pyxidis" style="background: none; color: #0b0080; text-decoration-line: none;" title="Theta Pyxidis">Theta Pyxidis</a> is a <a href="https://en.wikipedia.org/wiki/Red_giant" style="background: none; color: #0b0080; text-decoration-line: none;" title="Red giant">red giant</a> of spectral type M1III and semi-regular variable with two measured periods of 13 and 98.3 days, and an average magnitude of 4.71,<sup class="reference" id="cite_ref-tabur_24-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-tabur-24" style="background: none; color: #0b0080; text-decoration-line: none;">[21]</a></sup> and is 500 ± 30 light-years distant from Earth.<sup class="reference" id="cite_ref-van_Leeuwen2007_17-4" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-van_Leeuwen2007-17" style="background: none; color: #0b0080; text-decoration-line: none;">[14]</a></sup> It has expanded to approximately 54 times the diameter of the Sun.<sup class="reference" id="cite_ref-CADARS_21-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-CADARS-21" style="background: none; color: #0b0080; text-decoration-line: none;">[18]</a></sup></div>
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<a class="internal" href="https://en.wikipedia.org/wiki/File:Tpyx_hst_big.jpg" style="background: linear-gradient(transparent, transparent), url("data:image/svg+xml,%3C%3Fxml%20version%3D%221.0%22%20encoding%3D%22UTF-8%22%20standalone%3D%22no%22%3F%3E%0A%3Csvg%20xmlns%3D%22http%3A%2F%2Fwww.w3.org%2F2000%2Fsvg%22%20viewBox%3D%220%200%2011%2015%22%20width%3D%2215%22%20height%3D%2211%22%3E%0A%20%20%20%20%3Cg%20id%3D%22magnify-clip%22%20fill%3D%22%23fff%22%20stroke%3D%22%23000%22%3E%0A%20%20%20%20%20%20%20%20%3Cpath%20id%3D%22bigbox%22%20d%3D%22M1.509%201.865h10.99v7.919h-10.99z%22%2F%3E%0A%20%20%20%20%20%20%20%20%3Cpath%20id%3D%22smallbox%22%20d%3D%22M-1.499%206.868h5.943v4.904h-5.943z%22%2F%3E%0A%20%20%20%20%3C%2Fg%3E%0A%3C%2Fsvg%3E%0A"); color: #0b0080; display: block; height: 11px; overflow: hidden; text-decoration-line: none; text-indent: 15px; user-select: none; white-space: nowrap; width: 15px;" title="Enlarge"></a></div>
<a href="https://en.wikipedia.org/wiki/Hubble_Space_Telescope" style="background: none; color: #0b0080; text-decoration-line: none;" title="Hubble Space Telescope">Hubble Space Telescope</a> picture of <a href="https://en.wikipedia.org/wiki/T_Pyxidis" style="background: none; color: #0b0080; text-decoration-line: none;" title="T Pyxidis">T Pyxidis</a>, showing ejected material from past eruptions</div>
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Located around 4 degrees northeast of Alpha is <a href="https://en.wikipedia.org/wiki/T_Pyxidis" style="background: none; color: #0b0080; text-decoration-line: none;" title="T Pyxidis">T Pyxidis</a>,<sup class="reference" id="cite_ref-25" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-25" style="background: none; color: #0b0080; text-decoration-line: none;">[22]</a></sup> a binary star system composed of a <a href="https://en.wikipedia.org/wiki/White_dwarf" style="background: none; color: #0b0080; text-decoration-line: none;" title="White dwarf">white dwarf</a> with around 0.8 times the Sun's mass and a <a href="https://en.wikipedia.org/wiki/Red_dwarf" style="background: none; color: #0b0080; text-decoration-line: none;" title="Red dwarf">red dwarf</a> that orbit each other every 1.8 hours. This system is located around 15,500 light-years away from Earth.<sup class="reference" id="cite_ref-Chesneau_2011_26-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-Chesneau_2011-26" style="background: none; color: #0b0080; text-decoration-line: none;">[23]</a></sup> A <a href="https://en.wikipedia.org/wiki/Nova#Recurrent_novae" style="background: none; color: #0b0080; text-decoration-line: none;" title="Nova">recurrent nova</a>, it has brightened to the 7th magnitude in the years 1890, 1902, 1920, 1944, 1966 and 2011 from a baseline of around 14th magnitude. These outbursts are thought to be due to the white dwarf accreting material from its companion and ejecting periodically.<sup class="reference" id="cite_ref-AAVSOT_27-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-AAVSOT-27" style="background: none; color: #0b0080; text-decoration-line: none;">[24]</a></sup></div>
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<a href="https://en.wikipedia.org/wiki/TY_Pyxidis" style="background: none; color: #0b0080; text-decoration-line: none;" title="TY Pyxidis">TY Pyxidis</a> is an <a href="https://en.wikipedia.org/wiki/Binary_star#Eclipsing_binaries" style="background: none; color: #0b0080; text-decoration-line: none;" title="Binary star">eclipsing binary star</a> whose apparent magnitude ranges from 6.85 to 7.5 over 3.2 days.<sup class="reference" id="cite_ref-AAVSOTY_28-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-AAVSOTY-28" style="background: none; color: #0b0080; text-decoration-line: none;">[25]</a></sup> The two components are both of spectral type G5IV with a diameter 2.2 times,<sup class="reference" id="cite_ref-Strassmeier_29-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-Strassmeier-29" style="background: none; color: #0b0080; text-decoration-line: none;">[26]</a></sup> and mass 1.2 times that of the Sun, and revolve around each other every 3.2 days.<sup class="reference" id="cite_ref-30" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-30" style="background: none; color: #0b0080; text-decoration-line: none;">[27]</a></sup> The system is classified as a <a href="https://en.wikipedia.org/wiki/RS_Canum_Venaticorum_variable" style="background: none; color: #0b0080; text-decoration-line: none;" title="RS Canum Venaticorum variable">RS Canum Venaticorum variable</a>, a binary system with prominent <a href="https://en.wikipedia.org/wiki/Starspot" style="background: none; color: #0b0080; text-decoration-line: none;" title="Starspot">starspot</a> activity,<sup class="reference" id="cite_ref-AAVSOTY_28-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-AAVSOTY-28" style="background: none; color: #0b0080; text-decoration-line: none;">[25]</a></sup> and lies 184 ± 5 light-years away.<sup class="reference" id="cite_ref-van_Leeuwen2007_17-5" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-van_Leeuwen2007-17" style="background: none; color: #0b0080; text-decoration-line: none;">[14]</a></sup> The system emits X-rays, and analysing the emission curve over time led researchers to conclude that there was a loop of material arcing between the two stars.<sup class="reference" id="cite_ref-Pres_1995_31-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-Pres_1995-31" style="background: none; color: #0b0080; text-decoration-line: none;">[28]</a></sup> <a href="https://en.wikipedia.org/wiki/RZ_Pyxidis" style="background: none; color: #0b0080; text-decoration-line: none;" title="RZ Pyxidis">RZ Pyxidis</a> is another eclipsing binary system, made up of two young stars less than 200,000 years old. Both are hot blue-white stars of spectral type B7V and are around 2.5 times the size of the Sun. One is around five times as luminous as the Sun and the other around four times as luminous.<sup class="reference" id="cite_ref-32" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-32" style="background: none; color: #0b0080; text-decoration-line: none;">[29]</a></sup> The system is classified as a <a href="https://en.wikipedia.org/wiki/Beta_Lyrae_variable" style="background: none; color: #0b0080; text-decoration-line: none;" title="Beta Lyrae variable">Beta Lyrae variable</a>, the apparent magnitude varying from 8.83 to 9.72 over 0.66 days.<sup class="reference" id="cite_ref-AAVSORZ_33-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-AAVSORZ-33" style="background: none; color: #0b0080; text-decoration-line: none;">[30]</a></sup> <a href="https://en.wikipedia.org/wiki/XX_Pyxidis" style="background: none; color: #0b0080; text-decoration-line: none;" title="XX Pyxidis">XX Pyxidis</a> is one of the more-studied members of a class of stars known as <a href="https://en.wikipedia.org/wiki/Delta_Scuti_variable" style="background: none; color: #0b0080; text-decoration-line: none;" title="Delta Scuti variable">Delta Scuti variables</a><sup class="reference" id="cite_ref-Aerts_2002_34-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-Aerts_2002-34" style="background: none; color: #0b0080; text-decoration-line: none;">[31]</a></sup>—short period (six hours at most) pulsating stars that have been used as <a href="https://en.wikipedia.org/wiki/Cosmic_distance_ladder#Standard_candles" style="background: none; color: #0b0080; text-decoration-line: none;" title="Cosmic distance ladder">standard candles</a> and as subjects to study <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Astroseismology" style="background: none; color: #0b0080; text-decoration-line: none;" title="Astroseismology">astroseismology</a>.<sup class="reference" id="cite_ref-35" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-35" style="background: none; color: #0b0080; text-decoration-line: none;">[32]</a></sup> Astronomers made more sense of its pulsations when it became clear that it is also a binary star system. The main star is a white main sequence star of spectral type A4V that is around 1.85 ± 0.05 times as massive as the Sun. Its companion is most likely a red dwarf of spectral type M3V, around 0.3 times as massive as the Sun. The two are very close—possibly only 3 times the diameter of the Sun between them—and orbit each other every 1.15 days. The brighter star is deformed into an egg shape.<sup class="reference" id="cite_ref-Aerts_2002_34-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-Aerts_2002-34" style="background: none; color: #0b0080; text-decoration-line: none;">[31]</a></sup></div>
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<a href="https://en.wikipedia.org/wiki/AK_Pyxidis" style="background: none; color: #0b0080; text-decoration-line: none;" title="AK Pyxidis">AK Pyxidis</a> is a red giant of spectral type M5III and semi-regular variable that varies between magnitudes 6.09 and 6.51.<sup class="reference" id="cite_ref-AAVSOAK_36-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-AAVSOAK-36" style="background: none; color: #0b0080; text-decoration-line: none;">[33]</a></sup> Its pulsations take place over multiple periods simultaneously of 55.5, 57.9, 86.7, 162.9 and 232.6 days.<sup class="reference" id="cite_ref-tabur_24-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-tabur-24" style="background: none; color: #0b0080; text-decoration-line: none;">[21]</a></sup> <a href="https://en.wikipedia.org/wiki/UZ_Pyxidis" style="background: none; color: #0b0080; text-decoration-line: none;" title="UZ Pyxidis">UZ Pyxidis</a> is another semi-regular variable red giant, this time a <a href="https://en.wikipedia.org/wiki/Carbon_star" style="background: none; color: #0b0080; text-decoration-line: none;" title="Carbon star">carbon star</a>, that is around 3560 times as luminous as the Sun with a surface temperature of 3482 K, located some 2116 light-years away from Earth.<sup class="reference" id="cite_ref-Mcdonald_19-2" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-Mcdonald-19" style="background: none; color: #0b0080; text-decoration-line: none;">[16]</a></sup> It varies between magnitudes 6.99 and 7.83 over 159 days.<sup class="reference" id="cite_ref-AAVSOUZ_37-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-AAVSOUZ-37" style="background: none; color: #0b0080; text-decoration-line: none;">[34]</a></sup> <a href="https://en.wikipedia.org/wiki/VY_Pyxidis" style="background: none; color: #0b0080; text-decoration-line: none;" title="VY Pyxidis">VY Pyxidis</a> is a <a href="https://en.wikipedia.org/wiki/BL_Herculis_variable" style="background: none; color: #0b0080; text-decoration-line: none;" title="BL Herculis variable">BL Herculis variable</a> (<a href="https://en.wikipedia.org/wiki/Type_II_Cepheid" style="background: none; color: #0b0080; text-decoration-line: none;" title="Type II Cepheid">type II Cepheid</a>), ranging between <a href="https://en.wikipedia.org/wiki/Apparent_magnitude" style="background: none; color: #0b0080; text-decoration-line: none;" title="Apparent magnitude">apparent magnitudes</a> 7.13 and 7.40 over a period of 1.24 days.<sup class="reference" id="cite_ref-AAVSOVY_38-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-AAVSOVY-38" style="background: none; color: #0b0080; text-decoration-line: none;">[35]</a></sup> Located around 650 light-years distant, it shines with a <a href="https://en.wikipedia.org/wiki/Luminosity" style="background: none; color: #0b0080; text-decoration-line: none;" title="Luminosity">luminosity</a> approximately 45 times that of the Sun.<sup class="reference" id="cite_ref-Mcdonald_19-3" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-Mcdonald-19" style="background: none; color: #0b0080; text-decoration-line: none;">[16]</a></sup></div>
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The closest star to Earth in the constellation is <a href="https://en.wikipedia.org/wiki/Gliese_318" style="background: none; color: #0b0080; text-decoration-line: none;" title="Gliese 318">Gliese 318</a>, a white dwarf of spectral class DA5 and magnitude 11.85.<sup class="reference" id="cite_ref-Gaia_39-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-Gaia-39" style="background: none; color: #0b0080; text-decoration-line: none;">[36]</a></sup> Its distance has been calculated to be 26 light-years,<sup class="reference" id="cite_ref-40" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-40" style="background: none; color: #0b0080; text-decoration-line: none;">[37]</a></sup> or 28.7 ± 0.5 light-years distant from Earth. It has around 45% of the Sun's mass, yet only 0.15% of its luminosity.<sup class="reference" id="cite_ref-Subasavage_41-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-Subasavage-41" style="background: none; color: #0b0080; text-decoration-line: none;">[38]</a></sup> <a class="mw-redirect" href="https://en.wikipedia.org/wiki/WISEPC_J083641.12-185947.2" style="background: none; color: #0b0080; text-decoration-line: none;" title="WISEPC J083641.12-185947.2">WISEPC J083641.12-185947.2</a> is a <a href="https://en.wikipedia.org/wiki/Brown_dwarf" style="background: none; color: #0b0080; text-decoration-line: none;" title="Brown dwarf">brown dwarf</a> of <a href="https://en.wikipedia.org/wiki/Brown_dwarf#Spectral_class_T" style="background: none; color: #0b0080; text-decoration-line: none;" title="Brown dwarf">spectral type T8p</a> located around 72 light-years from Earth. Discovered by infrared astronomy in 2011, it has a magnitude of 18.79<sup class="reference" id="cite_ref-Kirkpatrick2012_42-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-Kirkpatrick2012-42" style="background: none; color: #0b0080; text-decoration-line: none;">[39]</a></sup></div>
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<span style="font-size: small;">Planetary systems</span></h3>
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Pyxis is home to three stars with confirmed planetary systems—all discovered by <a href="https://en.wikipedia.org/wiki/Doppler_spectroscopy" style="background: none; color: #0b0080; text-decoration-line: none;" title="Doppler spectroscopy">doppler spectroscopy</a>. A <a href="https://en.wikipedia.org/wiki/Hot_Jupiter" style="background: none; color: #0b0080; text-decoration-line: none;" title="Hot Jupiter">hot Jupiter</a>, <a href="https://en.wikipedia.org/wiki/HD_73256_b" style="background: none; color: #0b0080; text-decoration-line: none;" title="HD 73256 b">HD 73256 b</a>, that orbits <a href="https://en.wikipedia.org/wiki/HD_73256" style="background: none; color: #0b0080; text-decoration-line: none;" title="HD 73256">HD 73256</a> every 2.55 days, was discovered using the <a class="mw-redirect" href="https://en.wikipedia.org/wiki/CORALIE_spectrograph" style="background: none; color: #0b0080; text-decoration-line: none;" title="CORALIE spectrograph">CORALIE spectrograph</a> in 2003. The host star is a yellow star of spectral type G9V that has 69% of our Sun's luminosity, 89% of its diameter and 105% of its mass. Around 119 light-years away, it shines with an apparent magnitude of 8.08 and is around a billion years old.<sup class="reference" id="cite_ref-Udry2003_43-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-Udry2003-43" style="background: none; color: #0b0080; text-decoration-line: none;">[40]</a></sup> <a href="https://en.wikipedia.org/wiki/HD_73267_b" style="background: none; color: #0b0080; text-decoration-line: none;" title="HD 73267 b">HD 73267 b</a> was discovered with the <a href="https://en.wikipedia.org/wiki/High_Accuracy_Radial_Velocity_Planet_Searcher" style="background: none; color: #0b0080; text-decoration-line: none;" title="High Accuracy Radial Velocity Planet Searcher">High Accuracy Radial Velocity Planet Searcher</a> (HARPS) in 2008. It orbits <a href="https://en.wikipedia.org/wiki/HD_73267" style="background: none; color: #0b0080; text-decoration-line: none;" title="HD 73267">HD 73267</a> every 1260 days, a 7 billion year-old star of spectral type G5V that is around 89% as massive as the Sun.<sup class="reference" id="cite_ref-Moutou2009_44-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-Moutou2009-44" style="background: none; color: #0b0080; text-decoration-line: none;">[41]</a></sup> A <a href="https://en.wikipedia.org/wiki/Red_dwarf" style="background: none; color: #0b0080; text-decoration-line: none;" title="Red dwarf">red dwarf</a> of spectral type M2.5V that has around 42% the Sun's mass, <a href="https://en.wikipedia.org/wiki/Gliese_317" style="background: none; color: #0b0080; text-decoration-line: none;" title="Gliese 317">Gliese 317</a> is orbited by two gas giant planets. Around 50 light-years distant from Earth, it is a good candidate for future searches for more terrestrial rocky planets.<sup class="reference" id="cite_ref-45" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-45" style="background: none; color: #0b0080; text-decoration-line: none;">[42]</a></sup></div>
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<span style="font-size: small;">Deep sky objects</span></h3>
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Pyxis lies in the <a href="https://en.wikipedia.org/wiki/Galactic_plane" style="background: none; color: #0b0080; text-decoration-line: none;" title="Galactic plane">plane</a> of the <a href="https://en.wikipedia.org/wiki/Milky_Way" style="background: none; color: #0b0080; text-decoration-line: none;" title="Milky Way">Milky Way</a>, although part of the eastern edge is dark, with material obscuring our galaxy arm there. <a href="https://en.wikipedia.org/wiki/NGC_2818" style="background: none; color: #0b0080; text-decoration-line: none;" title="NGC 2818">NGC 2818</a> is a <a href="https://en.wikipedia.org/wiki/Planetary_nebula" style="background: none; color: #0b0080; text-decoration-line: none;" title="Planetary nebula">planetary nebula</a> that lies within a dim <a href="https://en.wikipedia.org/wiki/Open_cluster" style="background: none; color: #0b0080; text-decoration-line: none;" title="Open cluster">open cluster</a> of magnitude 8.2.<sup class="reference" id="cite_ref-46" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-46" style="background: none; color: #0b0080; text-decoration-line: none;">[43]</a></sup> <a class="new" href="https://en.wikipedia.org/w/index.php?title=NGC_2818A&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration-line: none;" title="NGC 2818A (page does not exist)">NGC 2818A</a> is an <a href="https://en.wikipedia.org/wiki/Open_cluster" style="background: none; color: #0b0080; text-decoration-line: none;" title="Open cluster">open cluster</a> that lies on line of sight with it.<sup class="reference" id="cite_ref-inglisOC_47-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-inglisOC-47" style="background: none; color: #0b0080; text-decoration-line: none;">[44]</a></sup> <a href="https://en.wikipedia.org/wiki/K_1-2" style="background: none; color: #0b0080; text-decoration-line: none;" title="K 1-2">K 1-2</a> is a planetary nebula whose central star is a <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Spectroscopic_binary" style="background: none; color: #0b0080; text-decoration-line: none;" title="Spectroscopic binary">spectroscopic binary</a> composed of two stars in close orbit with <a href="https://en.wikipedia.org/wiki/Astrophysical_jet" style="background: none; color: #0b0080; text-decoration-line: none;" title="Astrophysical jet">jets</a> emanating from the system. The surface temperature of one component has been estimated at as high as 85,000 K.<sup class="reference" id="cite_ref-Exter_2003_48-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-Exter_2003-48" style="background: none; color: #0b0080; text-decoration-line: none;">[45]</a></sup><a href="https://en.wikipedia.org/wiki/NGC_2627" style="background: none; color: #0b0080; text-decoration-line: none;" title="NGC 2627">NGC 2627</a> is an <a href="https://en.wikipedia.org/wiki/Open_cluster" style="background: none; color: #0b0080; text-decoration-line: none;" title="Open cluster">open cluster</a> of magnitude 8.4 that is visible in binoculars.<sup class="reference" id="cite_ref-inglisOC_47-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-inglisOC-47" style="background: none; color: #0b0080; text-decoration-line: none;">[44]</a></sup></div>
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Discovered in 1995,<sup class="reference" id="cite_ref-Irwin_1995_49-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-Irwin_1995-49" style="background: none; color: #0b0080; text-decoration-line: none;">[46]</a></sup> the <a href="https://en.wikipedia.org/wiki/Pyxis_globular_cluster" style="background: none; color: #0b0080; text-decoration-line: none;" title="Pyxis globular cluster">Pyxis globular cluster</a> is a 13.3 ± 1.3 billion year-old <a href="https://en.wikipedia.org/wiki/Globular_cluster" style="background: none; color: #0b0080; text-decoration-line: none;" title="Globular cluster">globular cluster</a> situated around 130,000 light-years distant from Earth and around 133,000 light-years distant from the centre of the Milky Way—a region not previously thought to contain globular clusters.<sup class="reference" id="cite_ref-1996AJ....112.2013S_50-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-1996AJ....112.2013S-50" style="background: none; color: #0b0080; text-decoration-line: none;">[47]</a></sup> Located in the <a href="https://en.wikipedia.org/wiki/Galactic_halo" style="background: none; color: #0b0080; text-decoration-line: none;" title="Galactic halo">galactic halo</a>, it was noted to lie on the same plane as the <a href="https://en.wikipedia.org/wiki/Large_Magellanic_Cloud" style="background: none; color: #0b0080; text-decoration-line: none;" title="Large Magellanic Cloud">Large Magellanic Cloud</a> and the possibility has been raised that it might be an escaped object from that galaxy.<sup class="reference" id="cite_ref-Irwin_1995_49-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-Irwin_1995-49" style="background: none; color: #0b0080; text-decoration-line: none;">[46]</a></sup></div>
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<a href="https://en.wikipedia.org/wiki/NGC_2613" style="background: none; color: #0b0080; text-decoration-line: none;" title="NGC 2613">NGC 2613</a> is a spiral galaxy of magnitude 10.5 which appears spindle-shaped as it is almost edge-on to observers on Earth.<sup class="reference" id="cite_ref-51" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-51" style="background: none; color: #0b0080; text-decoration-line: none;">[48]</a></sup> <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Henize_2-10" style="background: none; color: #0b0080; text-decoration-line: none;" title="Henize 2-10">Henize 2-10</a> is a dwarf galaxy which lies some 30 million light-years away. It is notable for having a black hole around a million solar masses at its centre. Known as a <a href="https://en.wikipedia.org/wiki/Starburst_galaxy" style="background: none; color: #0b0080; text-decoration-line: none;" title="Starburst galaxy">starburst galaxy</a> due to very high rates of star formation, it has a bluish colour due to the huge numbers of young stars within it.<sup class="reference" id="cite_ref-52" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis#cite_note-52" style="background: none; color: #0b0080; text-decoration-line: none;">[49]</a></sup></div>
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<span style="color: #222222; font-family: sans-serif;">https://en.wikipedia.org/wiki/Pyxis</span></div>
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<b style="color: #222222; font-family: sans-serif;">NGC 2658</b><span style="color: #222222; font-family: sans-serif;"> é um </span><a class="mw-redirect" href="https://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="color: #222222; font-family: sans-serif;"> na direção da </span><a href="https://pt.wikipedia.org/wiki/Pyxis" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Pyxis">constelação de Pyxis</a><span style="color: #222222; font-family: sans-serif;">. O objeto foi descoberto pelo astrônomo </span><a href="https://pt.wikipedia.org/wiki/James_Dunlop" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="James Dunlop">James Dunlop</a><span style="color: #222222; font-family: sans-serif;"> em 1826, usando um </span><a href="https://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Telescópio">telescópio</a><span style="color: #222222; font-family: sans-serif;"> refletor com abertura de 9 polegadas. Devido a sua moderada </span><a href="https://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #222222; font-family: sans-serif;"> (+9,2), é visível apenas com </span><a href="https://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Telescópio">telescópios</a><span style="color: #222222; font-family: sans-serif;"> amadores ou com equipamentos superiores.</span></div>
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<b style="color: #222222; font-family: sans-serif;">NGC 2627</b><span style="color: #222222; font-family: sans-serif;"> é um </span><a class="mw-redirect" href="https://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="color: #222222; font-family: sans-serif;"> na direção da </span><a href="https://pt.wikipedia.org/wiki/Pyxis" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Pyxis">constelação de Pyxis</a><span style="color: #222222; font-family: sans-serif;">. O objeto foi descoberto pelo astrônomo </span><a href="https://pt.wikipedia.org/wiki/William_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="William Herschel">William Herschel</a><span style="color: #222222; font-family: sans-serif;"> em 1793, usando um </span><a href="https://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Telescópio">telescópio</a><span style="color: #222222; font-family: sans-serif;"> refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="https://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #222222; font-family: sans-serif;"> (+8,4), é visível apenas com </span><a href="https://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-decoration-line: none;" title="Telescópio">telescópios</a><span style="color: #222222; font-family: sans-serif;"> amadores ou com equipamentos superiores.</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhXe3VTb2OS-wIdIhb3Q_5atbJflhuk4rhA-2-dNNs0x06nq9eUK74svb2fyWhU2NUIvv87qi7omcXXWZ7wFjpyp41ojIsoJPbTujudz2fs1a3I9DXGqD9j9pZzsm_VtkbAw8y8kBT3xMmN/s1600/ngc+2818.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhXe3VTb2OS-wIdIhb3Q_5atbJflhuk4rhA-2-dNNs0x06nq9eUK74svb2fyWhU2NUIvv87qi7omcXXWZ7wFjpyp41ojIsoJPbTujudz2fs1a3I9DXGqD9j9pZzsm_VtkbAw8y8kBT3xMmN/s1600/ngc+2818.png" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Stellarium</span></div>
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<img alt="Nestled Within" src="https://www.nasa.gov/sites/default/files/styles/full_width_feature/public/images/308010main_hs-2009-05-a-print_full.jpg?itok=5wr8juDs" /></div>
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<span style="color: #222222; font-family: sans-serif;"><span style="font-size: 14px;"><a href="https://www.nasa.gov/multimedia/imagegallery/image_feature_1270.html">https://www.nasa.gov/multimedia/imagegallery/image_feature_1270.html</a></span></span></div>
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<span style="font-family: "Helvetica Neue", Helvetica, Arial, sans-serif; font-size: 14px;">The unique planetary nebula NGC 2818 is nested inside the open star cluster NGC 2818A. Both the cluster and the nebula reside over 10,000 light-years away, in the southern constellation Pyxis (the Compass).</span><br style="box-sizing: border-box; font-family: "Helvetica Neue", Helvetica, Arial, sans-serif; font-size: 14px;" /><br style="box-sizing: border-box; font-family: "Helvetica Neue", Helvetica, Arial, sans-serif; font-size: 14px;" /><span style="font-family: "Helvetica Neue", Helvetica, Arial, sans-serif; font-size: 14px;">NGC 2818 is one of very few planetary nebulae in our galaxy located within an open cluster. Open clusters, in general, are loosely bound and they disperse over hundreds of millions of years. Stars that form planetary nebulae typically live for billions of years. Hence, it is rare that an open cluster survives long enough for one of its members to form a planetary nebula. This open cluster is particularly ancient, estimated to be nearly one billion years old.</span><br style="box-sizing: border-box; font-family: "Helvetica Neue", Helvetica, Arial, sans-serif; font-size: 14px;" /><br style="box-sizing: border-box; font-family: "Helvetica Neue", Helvetica, Arial, sans-serif; font-size: 14px;" /><span style="font-family: "Helvetica Neue", Helvetica, Arial, sans-serif; font-size: 14px;">Planetary nebulae fade away gradually over tens of thousands of years. The hot, remnant stellar core of NGC 2818 will eventually cool off for billions of years as a white dwarf. Our own sun will undergo a similar process, but not for another 5 billion years or so.</span><br style="box-sizing: border-box; font-family: "Helvetica Neue", Helvetica, Arial, sans-serif; font-size: 14px;" /><br style="box-sizing: border-box; font-family: "Helvetica Neue", Helvetica, Arial, sans-serif; font-size: 14px;" /><span style="font-family: "Helvetica Neue", Helvetica, Arial, sans-serif; font-size: 14px;">This Hubble image was taken in November 2008 with the Wide Field Planetary Camera 2. The colors in the image represent a range of emissions coming from the clouds of the nebula: red represents nitrogen, green represents hydrogen, and blue represents oxygen.</span><br style="box-sizing: border-box; font-family: "Helvetica Neue", Helvetica, Arial, sans-serif; font-size: 14px;" /><br style="box-sizing: border-box; font-family: "Helvetica Neue", Helvetica, Arial, sans-serif; font-size: 14px;" /><i style="box-sizing: border-box; font-family: "Helvetica Neue", Helvetica, Arial, sans-serif; font-size: 14px;">Image Credit: NASA, ESA and the Hubble Heritage Team (STScI/AURA)</i><br style="box-sizing: border-box; font-family: "Helvetica Neue", Helvetica, Arial, sans-serif; font-size: 14px;" /><span style="font-family: "Helvetica Neue", Helvetica, Arial, sans-serif; font-size: 14px;"> </span></div>
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<b>NGC 2818</b> é uma <a href="https://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background: none; color: #0b0080; text-decoration-line: none;" title="Nebulosa planetária">nebulosa planetária</a> situada na <a href="https://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration-line: none;" title="Constelação">constelação</a> austral de <a href="https://pt.wikipedia.org/wiki/Pyxis" style="background: none; color: #0b0080; text-decoration-line: none;" title="Pyxis">Pyxis</a>. Grande parte da nebulosa é constituída pelos gases expulsos pelas camadas exteriores de uma <a href="https://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration-line: none;" title="Estrela">estrela</a> no final da sua vida. Esta estrela é uma <a href="https://pt.wikipedia.org/wiki/An%C3%A3_branca" style="background: none; color: #0b0080; text-decoration-line: none;" title="Anã branca">anã branca</a> situada no centro da nebulosa.</div>
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Amiúde é citado como um membro de um <a href="https://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background: none; color: #0b0080; text-decoration-line: none;" title="Aglomerado estelar aberto">aglomerado estelar aberto</a>,<sup class="reference" id="cite_ref-3" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://pt.wikipedia.org/wiki/NGC_2818#cite_note-3" style="background: none; color: #0b0080; text-decoration-line: none;">[3]</a></sup> porém, as diferenças entre a velocidade radial da nebulosa planetária e este cúmulo aberto sugestionam um alinhamento aparente dos dois astros provocado apenas pela nossa posição no espaço. O caso é outro exemplo de um par superposto, unindo-se ao famoso caso de NGC 2438 e <a class="mw-redirect" href="https://pt.wikipedia.org/wiki/M46" style="background: none; color: #0b0080; text-decoration-line: none;" title="M46">M46</a>.</div>
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Em parte devido à sua pequena massa total, os aglomerados estelares abertos apresentam uma coesão relativamente pobre. Em consequência, os aglomerados estelares abertos tendem a ficar dispersos após um tempo relativamente curto, normalmente de cerca de 10 milhões de anos, devido a influências gravitativas externas além de outros fatores. Em condições excepcionais, os aglomerados abertos podem permanecer intatos até 100 milhões de anos.</div>
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Os modelos teóricos predizem que as nebulosas planetárias se podem formar por <a href="https://pt.wikipedia.org/wiki/Sequ%C3%AAncia_principal" style="background: none; color: #0b0080; text-decoration-line: none;" title="Sequência principal">estrelas da sequência principal</a> dentre 1 e 8 <a class="mw-redirect" href="https://pt.wikipedia.org/wiki/Massas_solares" style="background: none; color: #0b0080; text-decoration-line: none;" title="Massas solares">massas solares</a>, o qual põe a sua idade em 40 milhões de anos ou mais. Embora haja poucas centenas de cúmulos abertos a conhecer nessa categoria de idade, várias razões limitam as possibilidades de encontrar um membro de um aglomerado estelar aberto numa fase de nebulosa planetária. Uma delas é que a fase de nebulosa planetária das estrelas mais massivas que pertencem a grupos mais novos é apenas da ordem de milhares de anos. Até a data, nenhuma associação verdadeira foi estabelecida entre os aglomerados estelares abertos e as nebulosas planetárias.</div>
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<span style="color: #222222; font-family: sans-serif;"><b><a href="https://pt.wikipedia.org/wiki/NGC_2818">https://pt.wikipedia.org/wiki/NGC_2818</a></b></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEilBqfOubw0vi8THSMgtA6yUa6kCZMTgQC6kSVr7yVn_aiMJ0FZ9pESzGAMGam4hXeu2Jc5-3b43NqTUUm_C0WMAXtKP2JM4Qsxo8gqiAwHgP3IweaDgskCgIJZYjP4oGv1tG1uC6-41YYe/s1600/ngc+2613.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEilBqfOubw0vi8THSMgtA6yUa6kCZMTgQC6kSVr7yVn_aiMJ0FZ9pESzGAMGam4hXeu2Jc5-3b43NqTUUm_C0WMAXtKP2JM4Qsxo8gqiAwHgP3IweaDgskCgIJZYjP4oGv1tG1uC6-41YYe/s1600/ngc+2613.png" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Stellarium</span></div>
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<img height="445" src="https://upload.wikimedia.org/wikipedia/commons/thumb/0/08/Phot-09g-02-hires.jpg/280px-Phot-09g-02-hires.jpg" width="640" /></div>
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<a href="https://pt.wikipedia.org/wiki/NGC_2613#/media/File:Phot-09g-02-hires.jpg">https://pt.wikipedia.org/wiki/NGC_2613#/media/File:Phot-09g-02-hires.jpg</a></div>
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<span style="color: #222222; font-family: sans-serif; font-size: 16px;">VIMOS photo of NGC 2613, a spiral galaxy that resembles our own Milky Way. Composite VRI image obtained on February 28, 2002</span></div>
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<span class="mw-mmv-author" style="background-color: #f8f9fa; color: #54595d; font-family: sans-serif; font-size: 13.6px;">ESO</span><span style="background-color: #f8f9fa; color: #54595d; font-family: sans-serif; font-size: 13.6px;"> - </span><span class="mw-mmv-source" style="background-color: #f8f9fa; color: #54595d; font-family: sans-serif; font-size: 13.6px;"><a class="external free" href="http://www.eso.org/gallery/v/ESOPIA/Galaxies/phot-09g-02-hires.jpg.html" rel="nofollow" style="background: none; color: #0b0080;">http://www.eso.org/gallery/v/ESOPIA/Galaxies/phot-09g-02-hires.jpg.html</a></span></div>
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<b>NGC 2613</b> é uma <a href="https://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none; color: #0b0080; text-decoration-line: none;" title="Galáxia">galáxia</a> <a href="https://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background: none; color: #0b0080; text-decoration-line: none;" title="Galáxia espiral">espiral</a> (Sb) localizada na direcção da <a href="https://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration-line: none;" title="Constelação">constelação</a> de <a href="https://pt.wikipedia.org/wiki/Pyxis" style="background: none; color: #0b0080; text-decoration-line: none;" title="Pyxis">Pyxis</a>. Possui uma declinação de -22° 58' 22" e uma <a class="mw-redirect" href="https://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background: none; color: #0b0080; text-decoration-line: none;" title="Ascensão recta">ascensão recta</a> de 8 <a href="https://pt.wikipedia.org/wiki/Hora" style="background: none; color: #0b0080; text-decoration-line: none;" title="Hora">horas</a>, 33 <a href="https://pt.wikipedia.org/wiki/Minuto" style="background: none; color: #0b0080; text-decoration-line: none;" title="Minuto">minutos</a> e 22,8 <a href="https://pt.wikipedia.org/wiki/Segundo" style="background: none; color: #0b0080; text-decoration-line: none;" title="Segundo">segundos</a>.</div>
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A galáxia <b>NGC 2613</b> foi descoberta em <a class="mw-redirect" href="https://pt.wikipedia.org/wiki/20_de_Novembro" style="background: none; color: #0b0080; text-decoration-line: none;" title="20 de Novembro">20 de Novembro</a> de <a href="https://pt.wikipedia.org/wiki/1784" style="background: none; color: #0b0080; text-decoration-line: none;" title="1784">1784</a> por <a href="https://pt.wikipedia.org/wiki/William_Herschel" style="background: none; color: #0b0080; text-decoration-line: none;" title="William Herschel">William Herschel</a>.</div>
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<span style="color: #222222; font-family: sans-serif;"><a href="https://pt.wikipedia.org/wiki/NGC_2613">https://pt.wikipedia.org/wiki/NGC_2613</a></span></div>
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<img alt="NGC 2613 (captured by ESO's 1.5-metre Danish telescope).jpg" src="https://upload.wikimedia.org/wikipedia/commons/thumb/2/20/NGC_2613_%28captured_by_ESO%27s_1.5-metre_Danish_telescope%29.jpg/1024px-NGC_2613_%28captured_by_ESO%27s_1.5-metre_Danish_telescope%29.jpg" /></div>
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By ESO/IDA/Danish 1.5 m/R. Gendler, J.-E. Ovaldsen, C. Thöne and C. Féron - http://www.eso.org/gallery/v/ESOPIA/Galaxies/ESO-2613_cc.tif.html (TIFF image), CC BY 4.0, https://commons.wikimedia.org/w/index.php?curid=8324169</div>
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<span class="mw-mmv-author" style="background-color: #f8f9fa; color: #54595d; font-family: sans-serif; font-size: 13.6px;">ESO/IDA/Danish 1.5 m/R. Gendler, J.-E. Ovaldsen, C. Thöne and C. Féron</span><span style="background-color: #f8f9fa; color: #54595d; font-family: sans-serif; font-size: 13.6px;"> - </span><span class="mw-mmv-source" style="background-color: #f8f9fa; color: #54595d; font-family: sans-serif; font-size: 13.6px;"><a class="external free" href="http://www.eso.org/gallery/v/ESOPIA/Galaxies/ESO-2613_cc.tif.html" rel="nofollow" style="background: none; color: #0b0080; text-decoration-line: none;">http://www.eso.org/gallery/v/ESOPIA/Galaxies/ESO-2613_cc.tif.html</a> (<a class="external text" href="http://www.eso.org/gallery/d/97522-3/ESO-2613_cc.tif" rel="nofollow" style="background: none; color: #0b0080; text-decoration-line: none;">TIFF image</a>)</span></div>
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<span class="mw-mmv-source" style="background-color: #f8f9fa; color: #54595d; font-family: sans-serif;"><span style="background-color: white; color: #222222;">The </span><b style="background-color: white; color: #222222;">Pyxis globular cluster</b><span style="background-color: white; color: #222222;"> is a </span><a href="https://en.wikipedia.org/wiki/Globular_cluster" style="background: none rgb(255, 255, 255); color: #0b0080; text-decoration-line: none;" title="Globular cluster">globular cluster</a><span style="background-color: white; color: #222222;"> in the </span><a href="https://en.wikipedia.org/wiki/Constellation" style="background: none rgb(255, 255, 255); color: #0b0080; text-decoration-line: none;" title="Constellation">constellation</a><span style="background-color: white; color: #222222;"> </span><a href="https://en.wikipedia.org/wiki/Pyxis" style="background: none rgb(255, 255, 255); color: #0b0080; text-decoration-line: none;" title="Pyxis">Pyxis</a><span style="background-color: white; color: #222222;">. It lies around 130,000 light-years distant from earth and around 133,000 light-years distant from the centre of the Milky Way—a distance not previously thought to contain globular clusters. It is around 13.3 ± 1.3 billion years old.</span><sup class="reference" id="cite_ref-1996AJ....112.2013S_1-3" style="background-color: white; color: #222222; line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis_globular_cluster#cite_note-1996AJ....112.2013S-1" style="background: none; color: #0b0080; text-decoration-line: none;">[1]</a></sup><span style="background-color: white; color: #222222;"> Discovered in 1995 by astronomer Rainer Wienberger while he was looking for planetary nebulae, it is in the </span><a href="https://en.wikipedia.org/wiki/Galactic_halo" style="background: none rgb(255, 255, 255); color: #0b0080; text-decoration-line: none;" title="Galactic halo">Galactic halo</a><span style="background-color: white; color: #222222;">. Irwin and colleagues noted that it appears to lie on the same plane as the </span><a href="https://en.wikipedia.org/wiki/Large_Magellanic_Cloud" style="background: none rgb(255, 255, 255); color: #0b0080; text-decoration-line: none;" title="Large Magellanic Cloud">Large Magellanic Cloud</a><span style="background-color: white; color: #222222;"> and raised the possibility that it might be an escaped object from that galaxy.</span><sup class="reference" id="cite_ref-Irwin_1995_2-0" style="background-color: white; color: #222222; line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis_globular_cluster#cite_note-Irwin_1995-2" style="background: none; color: #0b0080; text-decoration-line: none;">[2]</a></sup></span></div>
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<table class="infobox" style="background-color: #f8f9fa; border-spacing: 3px; border: 1px solid rgb(162, 169, 177); clear: right; color: black; font-family: sans-serif; font-size: 12.32px; line-height: 1.5em; margin: 0.5em 0px 0.5em 1em; padding: 0.2em; width: 22em;"><tbody>
<tr><th colspan="2" style="background: rgb(255, 204, 153); font-size: 15.4px; text-align: center; vertical-align: top;">Pyxis globular cluster</th></tr>
<tr><th colspan="2" style="background: rgb(255, 204, 153); text-align: center; vertical-align: top;">Observation data (<a class="mw-redirect" href="https://en.wikipedia.org/wiki/J2000" style="background: none; color: #0b0080; text-decoration-line: none;" title="J2000">J2000</a> <a href="https://en.wikipedia.org/wiki/Epoch_(astronomy)" style="background: none; color: #0b0080; text-decoration-line: none;" title="Epoch (astronomy)">epoch</a>)</th></tr>
<tr><th scope="row" style="background: inherit; text-align: left; vertical-align: top;"><a href="https://en.wikipedia.org/wiki/Constellation" style="background: none; color: #0b0080; text-decoration-line: none;" title="Constellation">Constellation</a></th><td style="vertical-align: top;"><a href="https://en.wikipedia.org/wiki/Pyxis" style="background: none; color: #0b0080; text-decoration-line: none;" title="Pyxis">Pyxis</a></td></tr>
<tr><th scope="row" style="background: inherit; text-align: left; vertical-align: top;"><a href="https://en.wikipedia.org/wiki/Right_ascension" style="background: none; color: #0b0080; text-decoration-line: none;" title="Right ascension">Right ascension</a></th><td style="vertical-align: top;">09<sup style="font-size: 9.856px; line-height: 1;">h</sup> 07<sup style="font-size: 9.856px; line-height: 1;">m</sup> 57.80<sup style="font-size: 9.856px; line-height: 1;">s</sup></td></tr>
<tr><th scope="row" style="background: inherit; text-align: left; vertical-align: top;"><a href="https://en.wikipedia.org/wiki/Declination" style="background: none; color: #0b0080; text-decoration-line: none;" title="Declination">Declination</a></th><td style="vertical-align: top;">–37° 13′ 17.0″</td></tr>
<tr><th scope="row" style="background: inherit; text-align: left; vertical-align: top;"><a class="mw-redirect" href="https://en.wikipedia.org/wiki/Distance_(astronomy)" style="background: none; color: #0b0080; text-decoration-line: none;" title="Distance (astronomy)">Distance</a></th><td style="vertical-align: top;">130,000 light-years<sup class="reference" id="cite_ref-1996AJ....112.2013S_1-0" style="font-size: 9.856px; line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis_globular_cluster#cite_note-1996AJ....112.2013S-1" style="background: none; color: #0b0080; text-decoration-line: none;">[1]</a></sup></td></tr>
<tr><th colspan="2" style="background: rgb(255, 204, 153); text-align: center; vertical-align: top;">Physical characteristics</th></tr>
<tr><th scope="row" style="background: inherit; text-align: left; vertical-align: top;"><a href="https://en.wikipedia.org/wiki/Metallicity" style="background: none; color: #0b0080; text-decoration-line: none;" title="Metallicity">Metallicity</a></th><td style="vertical-align: top;"><span class="mwe-math-element" style="max-width: 100%; overflow-x: auto;"><img alt="{\displaystyle {\begin{smallmatrix}\left[{\ce {Fe}}/{\ce {H}}\right]\end{smallmatrix}}}" aria-hidden="true" class="mwe-math-fallback-image-inline" src="https://wikimedia.org/api/rest_v1/media/math/render/svg/4c0821bd80891e071c08e7c7ee8e022baedf522c" style="border: 0px; display: inline-block; height: 2.176ex; vertical-align: -0.671ex; width: 5.568ex;" /></span> = -1.20 ± 0.15<sup class="reference" id="cite_ref-1996AJ....112.2013S_1-1" style="font-size: 9.856px; line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis_globular_cluster#cite_note-1996AJ....112.2013S-1" style="background: none; color: #0b0080; text-decoration-line: none;">[1]</a></sup><a class="mw-redirect" href="https://en.wikipedia.org/wiki/Log_10" style="background: none; color: #0b0080; text-decoration-line: none;" title="Log 10">dex</a></td></tr>
<tr><th scope="row" style="background: inherit; text-align: left; vertical-align: top;">Estimated age</th><td style="vertical-align: top;">13.3 ± 1.3 Gyr<sup class="reference" id="cite_ref-1996AJ....112.2013S_1-2" style="font-size: 9.856px; line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Pyxis_globular_cluster#cite_note-1996AJ....112.2013S-1" style="background: none; color: #0b0080; text-decoration-line: none;">[1]</a></sup></td></tr>
<tr><th scope="row" style="background: inherit; text-align: left; vertical-align: top;">Other designations</th><td style="vertical-align: top;">Pyxis globular cluster</td></tr>
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<a href="https://en.wikipedia.org/wiki/Pyxis_globular_cluster" style="background-color: #f8f9fa; font-family: sans-serif; text-align: start;">https://en.wikipedia.org/wiki/Pyxis_globular_cluster</a><br style="text-align: start;" /><br style="text-align: start;" /><br style="text-align: start;" /><div style="background-color: white; color: #222222; font-family: sans-serif; line-height: inherit; margin-bottom: 0.5em; margin-top: 0.5em; text-align: start;">
A <b>globular cluster</b> is a <a href="https://en.wikipedia.org/wiki/Sphere" style="background: none; color: #0b0080; text-decoration-line: none;" title="Sphere">spherical</a> collection of <a href="https://en.wikipedia.org/wiki/Star" style="background: none; color: #0b0080; text-decoration-line: none;" title="Star">stars</a> that orbits a <a href="https://en.wikipedia.org/wiki/Galactic_Center" style="background: none; color: #0b0080; text-decoration-line: none;" title="Galactic Center">galactic core</a> as a <a href="https://en.wikipedia.org/wiki/Satellite" style="background: none; color: #0b0080; text-decoration-line: none;" title="Satellite">satellite</a>. Globular clusters are very tightly bound by <a href="https://en.wikipedia.org/wiki/Gravity" style="background: none; color: #0b0080; text-decoration-line: none;" title="Gravity">gravity</a>, which gives them their spherical shapes and relatively high stellar densities toward their centers. The name of this category of <a href="https://en.wikipedia.org/wiki/Star_cluster" style="background: none; color: #0b0080; text-decoration-line: none;" title="Star cluster">star cluster</a> is derived from the <a href="https://en.wikipedia.org/wiki/Latin" style="background: none; color: #0b0080; text-decoration-line: none;" title="Latin">Latin</a> <i>globulus</i>—a small sphere. A globular cluster is sometimes known more simply as a <i>globular</i>.</div>
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Globular clusters are found in the <a href="https://en.wikipedia.org/wiki/Galactic_halo" style="background: none; color: #0b0080; text-decoration-line: none;" title="Galactic halo">halo</a> of a <a href="https://en.wikipedia.org/wiki/Galaxy" style="background: none; color: #0b0080; text-decoration-line: none;" title="Galaxy">galaxy</a> and contain considerably more stars and are much older than the less dense <a href="https://en.wikipedia.org/wiki/Open_cluster" style="background: none; color: #0b0080; text-decoration-line: none;" title="Open cluster">open clusters</a>, which are found in the disk of a galaxy. Globular clusters are fairly common; there are about 150<sup class="reference" id="cite_ref-2" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Globular_cluster#cite_note-2" style="background: none; color: #0b0080; text-decoration-line: none;">[2]</a></sup> to 158<sup class="reference" id="cite_ref-3" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Globular_cluster#cite_note-3" style="background: none; color: #0b0080; text-decoration-line: none;">[3]</a></sup> currently known globular clusters in the <a href="https://en.wikipedia.org/wiki/Milky_Way" style="background: none; color: #0b0080; text-decoration-line: none;" title="Milky Way">Milky Way</a>, with perhaps 10 to 20 more still undiscovered.<sup class="reference" id="cite_ref-milky_way_4-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Globular_cluster#cite_note-milky_way-4" style="background: none; color: #0b0080; text-decoration-line: none;">[4]</a></sup> These globular clusters orbit the Galaxy at radii of 40 <a href="https://en.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration-line: none;" title="Parsec">kiloparsecs</a> (130,000 <a href="https://en.wikipedia.org/wiki/Light-year" style="background: none; color: #0b0080; text-decoration-line: none;" title="Light-year">light-years</a>) or more.<sup class="reference" id="cite_ref-5" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Globular_cluster#cite_note-5" style="background: none; color: #0b0080; text-decoration-line: none;">[5]</a></sup> Larger galaxies can have more: <a href="https://en.wikipedia.org/wiki/Andromeda_Galaxy" style="background: none; color: #0b0080; text-decoration-line: none;" title="Andromeda Galaxy">Andromeda Galaxy</a>, for instance, may have as many as 500.<sup class="reference" id="cite_ref-6" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Globular_cluster#cite_note-6" style="background: none; color: #0b0080; text-decoration-line: none;">[6]</a></sup> Some giant <a href="https://en.wikipedia.org/wiki/Elliptical_galaxy" style="background: none; color: #0b0080; text-decoration-line: none;" title="Elliptical galaxy">elliptical galaxies</a> (particularly those at the centers of <a href="https://en.wikipedia.org/wiki/Galaxy_cluster" style="background: none; color: #0b0080; text-decoration-line: none;" title="Galaxy cluster">galaxy clusters</a>) such as <a href="https://en.wikipedia.org/wiki/Messier_87" style="background: none; color: #0b0080; text-decoration-line: none;" title="Messier 87">M87</a>,<sup class="reference" id="cite_ref-7" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Globular_cluster#cite_note-7" style="background: none; color: #0b0080; text-decoration-line: none;">[7]</a></sup>have as many as 13,000 globular clusters.</div>
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Every galaxy of sufficient mass in the <a href="https://en.wikipedia.org/wiki/Local_Group" style="background: none; color: #0b0080; text-decoration-line: none;" title="Local Group">Local Group</a> has an associated group of globular clusters, and almost every large galaxy surveyed has been found to possess a system of globular clusters.<sup class="reference" id="cite_ref-8" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Globular_cluster#cite_note-8" style="background: none; color: #0b0080; text-decoration-line: none;">[8]</a></sup> The <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Sagittarius_Dwarf_Elliptical_Galaxy" style="background: none; color: #0b0080; text-decoration-line: none;" title="Sagittarius Dwarf Elliptical Galaxy">Sagittarius Dwarf</a> galaxy and the <a href="https://en.wikipedia.org/wiki/Canis_Major_Overdensity#Dispute" style="background: none; color: #0b0080; text-decoration-line: none;" title="Canis Major Overdensity">disputed Canis Major Dwarf galaxy</a> appear to be in the process of donating their associated globular clusters (such as <a href="https://en.wikipedia.org/wiki/Palomar_12" style="background: none; color: #0b0080; text-decoration-line: none;" title="Palomar 12">Palomar 12</a>) to the Milky Way.<sup class="reference" id="cite_ref-9" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Globular_cluster#cite_note-9" style="background: none; color: #0b0080; text-decoration-line: none;">[9]</a></sup> This demonstrates how many of this galaxy's globular clusters might have been acquired in the past.</div>
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Although it appears that globular clusters contain some of the first stars to be produced in the galaxy, their <a href="https://en.wikipedia.org/wiki/Galaxy_formation_and_evolution" style="background: none; color: #0b0080; text-decoration-line: none;" title="Galaxy formation and evolution">origins</a> and their role in galactic evolution are still unclear. It does appear clear that globular clusters are significantly different from <a href="https://en.wikipedia.org/wiki/Dwarf_elliptical_galaxy" style="background: none; color: #0b0080; text-decoration-line: none;" title="Dwarf elliptical galaxy">dwarf elliptical galaxies</a> and were formed as part of the star formation of the parent galaxy rather than as a separate galaxy.<sup class="reference" id="cite_ref-apj613_10-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Globular_cluster#cite_note-apj613-10" style="background: none; color: #0b0080; text-decoration-line: none;">[10]</a></sup></div>
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<a href="https://en.wikipedia.org/wiki/Globular_cluster">https://en.wikipedia.org/wiki/Globular_cluster</a></div>
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The <b>galactic halo</b> is an extended, roughly spherical component of a <a href="https://en.wikipedia.org/wiki/Galaxy" style="background: none; color: #0b0080; text-decoration-line: none;" title="Galaxy">galaxy</a> which extends beyond the main, visible component. Several distinct components of galaxies comprise the halo:</div>
<ul style="background-color: white; color: #222222; font-family: sans-serif; list-style-image: url("data:image/svg+xml,%3C%3Fxml%20version%3D%221.0%22%20encoding%3D%22UTF-8%22%3F%3E%0A%3Csvg%20xmlns%3D%22http%3A%2F%2Fwww.w3.org%2F2000%2Fsvg%22%20version%3D%221.1%22%20width%3D%225%22%20height%3D%2213%22%3E%0A%3Ccircle%20cx%3D%222.5%22%20cy%3D%229.5%22%20r%3D%222.5%22%20fill%3D%22%2300528c%22%2F%3E%0A%3C%2Fsvg%3E%0A"); margin: 0.3em 0px 0px 1.6em; padding: 0px; text-align: start;">
<li style="margin-bottom: 0.1em;">the <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Galactic_spheroid" style="background: none; color: #0b0080; text-decoration-line: none;" title="Galactic spheroid">galactic spheroid</a> (<a href="https://en.wikipedia.org/wiki/Star" style="background: none; color: #0b0080; text-decoration-line: none;" title="Star">stars</a>)</li>
<li style="margin-bottom: 0.1em;">the <a href="https://en.wikipedia.org/wiki/Galactic_corona" style="background: none; color: #0b0080; text-decoration-line: none;" title="Galactic corona">galactic corona</a> (hot <a href="https://en.wikipedia.org/wiki/Interstellar_medium" style="background: none; color: #0b0080; text-decoration-line: none;" title="Interstellar medium">gas</a>, i.e. a <a href="https://en.wikipedia.org/wiki/Plasma_(physics)" style="background: none; color: #0b0080; text-decoration-line: none;" title="Plasma (physics)">plasma</a>)</li>
<li style="margin-bottom: 0.1em;">the <a href="https://en.wikipedia.org/wiki/Dark_matter_halo" style="background: none; color: #0b0080; text-decoration-line: none;" title="Dark matter halo">dark matter halo</a></li>
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The distinction between the halo and the main body of the galaxy is clearest in <a href="https://en.wikipedia.org/wiki/Spiral_galaxy" style="background: none; color: #0b0080; text-decoration-line: none;" title="Spiral galaxy">spiral galaxies</a>, where the spherical shape of the halo contrasts with the flat <a href="https://en.wikipedia.org/wiki/Disc_(galaxy)" style="background: none; color: #0b0080; text-decoration-line: none;" title="Disc (galaxy)">disc</a>. In an <a href="https://en.wikipedia.org/wiki/Elliptical_galaxy" style="background: none; color: #0b0080; text-decoration-line: none;" title="Elliptical galaxy">elliptical galaxy</a>, there is no sharp transition between the body of the galaxy and the halo.</div>
<div style="background-color: white; line-height: inherit; margin-bottom: 0.5em; margin-top: 0.5em; text-align: start;">
<span style="color: #222222; font-family: sans-serif;"><a href="https://en.wikipedia.org/wiki/Galactic_halo">https://en.wikipedia.org/wiki/Galactic_halo</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Stellarium</span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, </b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b>entre o céu e a terra..., </b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b>vagarosamente, </b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b>vai se tornando Cosmos </b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b>e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>Quer dizer, </b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>Janine Milward</b></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-11293027320532039462013-08-20T08:11:00.002-07:002014-04-27T13:24:16.721-07:00PUPPIS, A POPA EM ARGO NAVIS, O NAVIO<div align="center" class="MsoNormal" style="text-align: center;">
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<span style="font-family: Arial, Helvetica, sans-serif; font-weight: normal;"><span style="background-color: white; color: #073763; font-size: small;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-weight: bold; text-decoration: none;">Da Terra ao Céu ....</a>.....<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-weight: bold; text-decoration: none;">e ao Infinito </a><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; font-weight: normal;"><span style="background-color: white; color: #073763; font-size: x-small;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...; bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; font-weight: normal;"><span style="background-color: white; color: #073763; font-size: x-small;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; font-weight: normal;"><span style="background-color: white; color: #073763; font-size: x-small;">Com um abraço estrelado,<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small; font-weight: normal; text-align: justify;">Janine Milward</span></h3>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">PUPPIS, A POPA </span></h3>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">EM ARGO NAVIS, O NAVIO</span></h3>
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<a href="http://sobreargonavis.blogspot.com.br/2013/11/puppis-popa-ou-proa-de-argo-navis-o.html" style="font-size: 15px; font-weight: bold; line-height: 23px;"><span style="font-family: Arial, sans-serif; text-decoration: none;"><span style="background-color: white; color: #073763;">http://sobreargonavis.blogspot.com.br/2013/11/puppis-popa-ou-proa-de-argo-navis-o.html</span></span></a></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjXokZcYgv8WYWUZFxEwXwqYlilTC9EwHoTvKPoGcsFlSAcRD5Yzwlu2tM_pGLeRf1W_mOdN3r8IZ5hScYybV4q5Wg43QhMUCSZQWZAzInzhDYgZOzdrJjUxtmRUp3Kfgqe_NdZAG1Bx9iR/s1600/Puppis-A.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjXokZcYgv8WYWUZFxEwXwqYlilTC9EwHoTvKPoGcsFlSAcRD5Yzwlu2tM_pGLeRf1W_mOdN3r8IZ5hScYybV4q5Wg43QhMUCSZQWZAzInzhDYgZOzdrJjUxtmRUp3Kfgqe_NdZAG1Bx9iR/s1600/Puppis-A.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
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<span style="border: 0px; line-height: 25.59375px; margin: 0px; outline: 0px; padding: 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Puppis A, a middle-aged supernova remnant</span></span></div>
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<a href="http://annesastronomynews.com/annes-picture-of-the-day-supernova-remnant-puppis-a/" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://annesastronomynews.com/annes-picture-of-the-day-supernova-remnant-puppis-a/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 25.59375px;">Image Credit: </span><em style="border: 0px; line-height: 25.59375px; margin: 0px; outline: 0px; padding: 0px;">NASA/JPL-Caltech/UCLA/WISE Team</em></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><strong style="border: 0px; line-height: 25.59375px; margin: 0px; outline: 0px; padding: 0px;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></strong><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><img src="http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_027.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><a href="http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_027.jpg" style="text-decoration: none;">http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_027.jpg</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></div>
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<span style="line-height: 11px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></span></div>
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<span style="line-height: 11px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small; line-height: 14px;"> - excerto apresentando ALFABETO GREGO, CONVENÇÕES E USO DA CARTA CELESTE</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>ARGO NAVIS, O NAVIO</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação representa o navio no qual Jasão trouxe o Velocino de Ouro para Colquita - e dizem que foi o primeiro navio a ser construído.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação, o Navio, fazia parte do grupo de 48 constelações relacionado por Ptolomeu. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">La Caille, porém, dividiu o Navio em<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Carina, Vela e Puppis: Quilha, Vela e Popa<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">Argo Navis</b><span style="line-height: 19.1875px; text-align: start;"> era uma grande </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="line-height: 19.1875px; text-align: start;"> meridional, representava o navio utilizado pelos </span><a href="http://pt.wikipedia.org/wiki/Argonautas" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Argonautas">argonautas</a><span style="line-height: 19.1875px; text-align: start;"> em suas viagens. Foi dividida em </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Carina" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Carina">Carina</a><span style="line-height: 19.1875px; text-align: start;">(quilha), </span><a href="http://pt.wikipedia.org/wiki/Puppis" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Puppis">Puppis</a><span style="line-height: 19.1875px; text-align: start;"> (popa) e </span><a href="http://pt.wikipedia.org/wiki/Vela_(constela%C3%A7%C3%A3o)" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Vela (constelação)">Vela</a><span style="line-height: 19.1875px; text-align: start;"> (velame); as </span><a href="http://pt.wikipedia.org/wiki/Designa%C3%A7%C3%A3o_de_Bayer" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Designação de Bayer">designações de Bayer</a><span style="line-height: 19.1875px; text-align: start;">, entretanto, não foram mudadas, de modo que α e β estão em Carina, γ e δ em Vela, ε em Carina, ζ em Puppis e assim por diante. Por outro lado, </span><a href="http://pt.wikipedia.org/wiki/Pyxis" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Pyxis">Pyxis</a><span style="line-height: 19.1875px; text-align: start;">, a constelação da Bússola, embora ocupe uma área que havia sido considerada como os mastros do Argo, possui designações de Bayer próprias.</span></span></div>
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<a href="http://pt.wikipedia.org/wiki/Argo_Navis" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Argo_Navis</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Ficheiro:Argo Navis Hevelius.jpg" src="http://upload.wikimedia.org/wikipedia/commons/c/cc/Argo_Navis_Hevelius.jpg" height="519" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="640" /></span></div>
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<a href="http://pt.wikipedia.org/wiki/Ficheiro:Argo_Navis_Hevelius.jpg" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Ficheiro:Argo_Navis_Hevelius.jpg</span></a><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="external text" href="http://contentdm.lindahall.org/cdm4/document.php?CISOROOT=/star_atlas&CISOPTR=479" rel="nofollow" style="text-decoration: none;">Atlas Coelestis</a><span style="line-height: 19.1875px; text-align: start;">. Johannes Hevelius drew the constellation in Uranographia, his celestial catalogue in 1690.</span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 15.828125px; text-align: left;">Desenho de </span><b style="line-height: 15.828125px; text-align: left;">Argo Navis</b><span style="line-height: 15.828125px; text-align: left;"> por </span><a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-image: none; line-height: 15.828125px; text-align: left; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a><span style="line-height: 15.828125px; text-align: left;"> (</span><a href="http://pt.wikipedia.org/wiki/1690" style="background-image: none; line-height: 15.828125px; text-align: left; text-decoration: none;" title="1690">1690</a><span style="line-height: 15.828125px; text-align: left;">)</span></span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjCyM53UERwH98csn7bTomUlVIIcI_htt4KyN4lQMM7eKiTPEs7zEzSJMVVTa2V-BHS8Xl0TfLs9wb_xTFYXW28dwWL7cuoyiLoIpA7Kt4cPNJ_SDi-sVUbrQXI7q2Gy_q9lIl1Kf0ITYIk/s1600/figura+antigacel4full.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjCyM53UERwH98csn7bTomUlVIIcI_htt4KyN4lQMM7eKiTPEs7zEzSJMVVTa2V-BHS8Xl0TfLs9wb_xTFYXW28dwWL7cuoyiLoIpA7Kt4cPNJ_SDi-sVUbrQXI7q2Gy_q9lIl1Kf0ITYIk/s1600/figura+antigacel4full.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US" style="line-height: 14px;">The image for the "Historical Essay" is taken from<span class="apple-converted-space"> </span></span><a href="http://www.lindahall.org/events_exhib/exhibit/exhibits/stars/cel.htm" style="text-decoration: none;"><span lang="EN-US" style="line-height: 14px;">Andreas Cellarius,</span><span class="apple-converted-space"><span lang="EN-US" style="line-height: 14px;"> </span></span><i><span lang="EN-US" style="line-height: 14px;">Harmonia macrocosmica,</span></i><span class="apple-converted-space"><span lang="EN-US" style="line-height: 14px;"> </span></span><span lang="EN-US" style="line-height: 14px;">1661</span></a><span lang="EN-US" style="line-height: 14px;">.</span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US" style="line-height: 14px;"><o:p></o:p></span><a href="http://www.lindahall.org/events_exhib/exhibit/exhibits/stars/images/cel4full.jpg" style="line-height: 14.25pt; text-decoration: none;">http://www.lindahall.org/events_exhib/exhibit/exhibits/stars/images/cel4full.jpg</a></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Julius Schiller, <i>Coelum stellatum Christianum</i>, 1627</span><br />
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<span style="line-height: 13px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ESA /AOES Medialab</span></span></div>
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<a href="http://spaceinimages.esa.int/Images/2009/05/GOCE_in_orbit" style="text-decoration: none;"><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://spaceinimages.esa.int/Images/2009/05/GOCE_in_orbit</span></span></a></div>
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<span lang="EN-US" style="text-transform: uppercase;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">GOCE IN ORBIT<o:p></o:p></span></span></div>
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<span lang="EN-US" style="text-transform: uppercase;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O NAVIO NAVEGANDO NO ESPAÇO</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="PT"> e ao Infinito</span></b><o:p></o:p></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelações, Estrelas e Objetos Celestes<o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(sob o ponto de vista do Mundo Ocidental)<o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Suas histórias, seus mitos, seus significados e suas sintetizadas descrições<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">Reunião das Informações e Compilação,</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">Tradução para a língua portuguesa (em alguns momentos)</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">bem como Comentários Pessoais:</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><span lang="PT">Janine Milward</span></i><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Alguns dados<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(tais como Ascensão Reta e Declinação, em muitos dos casos)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">são época/equinócio 1980<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e devem requerer do Caminhante do Céu<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NASA/IPAC</b><b> EXTRAGALACTIC DATABASE –</b><b><o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="text-decoration: none;"><b>http://ned.ipac.caltech.edu/</b></a><b><o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="text-decoration: none;"><b>http://ned.ipac.caltech.edu/forms/byname.html</b></a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><b><span lang="EN-US"><o:p></o:p></span></b></span></div>
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<b><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="EN-US">The</span></b><span class="apple-converted-space"><b><span lang="EN-US"> </span></b></span><b><span lang="EN-US">Internet STELLAR DATABASE</span></b><b><span lang="EN-US"><o:p></o:p></span></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="text-decoration: none;"><b><span lang="EN-US">http://www.stellar-database.com/</span></b></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<o:p></o:p></span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhc0V3OCd4x2SuPbHK75pITJnGkzt6K19IrDpW4FR_dSnrpqhYwdE3jgUmSzxkhMTX0DLdGU7-TwiksgZujyOzKoVZ_q4E2gQ-LX8HNKldXPtK0h-MyPJHZYTOjU_vdZ_-UidFQEqC7RUIY/s1600/puppis,+Mario+Jaci.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhc0V3OCd4x2SuPbHK75pITJnGkzt6K19IrDpW4FR_dSnrpqhYwdE3jgUmSzxkhMTX0DLdGU7-TwiksgZujyOzKoVZ_q4E2gQ-LX8HNKldXPtK0h-MyPJHZYTOjU_vdZ_-UidFQEqC7RUIY/s1600/puppis,+Mario+Jaci.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; line-height: 14px;">Mario Jaci Monteiro - As 88 Constelações, Cartas Celestes</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.ianridpath.com/atlases/urania/urania32.jpg" style="text-decoration: none;">http://www.ianridpath.com/atlases/urania/urania32.jpg</a><span style="line-height: 14px;"> </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>PUPPIS, POPA</b><o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Posicionamento:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 6h2m / 8h26m Declinação -11<sup>o</sup>.0 / -50<sup>o</sup>.8<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Mito</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação representa o navio no qual Jasão trouxe o Velocino de Ouro para Colquita - e dizem que foi o primeiro Navio a ser construído.<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Algumas Informações Interessantes acerca esta Constelação:</b><o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação, o Navio, fazia parte do grupo de 48 constelações relacionado por Ptolomeu. Porém, La Caille dividiu o Navio em<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Carina, Vela e Puppis, Quilha, Vela e Popa<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A Popa é facilmente identificável a partir da localização de Canopus, estrela-alpha do Navio Argos e situada na parte de Carina, a Quilha, e buscando o padrão de estrelas que ficam ao norte. (Do ponto de vista de quem está no hemisfério sul, é possível se identificar a Popa já muito próxima a Sirius, a estrela-alpha do Cão Maior, até chegar a Canopus, a estrela-alpha do Navio.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Existem alguns aglomerados abertos nesta constelação sendo que o mais brilhante é M47, visível a olho nu. M46 e M93 são mais pálidos porém também considerados como objetos interessantes a serem observados. M46 e M47 situam-se próximos a Sirius (que atua enquanto ponto de referência, é claro).<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Fronteiras:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Puppis situa-se entre as constelações Canis Major, Columba, Pictor, Carina, Vela, Pyxix, Hydra, Monoceros<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Carina Navis" src="http://www.lindahall.org/services/digital/ebooks/bayer/bigpix/040040bc.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<a href="http://www.lindahall.org/services/digital/ebooks/bayer/bayer92.shtml" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.lindahall.org/services/digital/ebooks/bayer/bayer92.shtml</span></a><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><br /><br /><br /><strong>Kornelii Reissig. <em>Sozviezdiia Predstavlennyia</em>... 1829.</strong><br />Map XXVII. Argo Navis, Monoceros, Columba, Officina Typographica, Canis Minor, and Canis Major.</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Monoceros, Canis Major, Canis Minor, Carina" src="http://www.lindahall.org/services/digital/ebooks/reissig/bigpix/0022084b.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span><br />
<a href="http://www.lindahall.org/services/digital/ebooks/reissig/reissig84.shtml" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.lindahall.org/services/digital/ebooks/reissig/reissig84.shtml</span></a><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="background-color: white; color: #073763;">Algumas Estrelas </span></b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="background-color: white; color: #073763;">e alguns objetos interessantes, </span></b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>em Popa:</b><o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Kappa Puppis - Estrela Dupla</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">AR 07h36m Dec - 26<sup>o</sup>.41<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">M 4,5 e 4,6 Distância entre estrelas 9”,95<o:p></o:p></span><br />
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></b></div>
<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Suhail Hadar ou Naos - Zeta Puppis</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 8h - Declinação - 40<sup>o</sup>.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual 2.23 - Distância 2.300 anos-luz<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Navio, vocábulo grego que designa a estrela situada na popa do Navio, antiga constelação austral.<o:p></o:p></span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj8LqrMebbIxvOUE5AsfGIeEQLuMlL4V6w95RLw1vi80bGKZDHTM80IzYWLWOYE2P6WTIy-3zMpkzGCEzSbbkZMy85u21aAEo6fYr0wZERC98tvjy5I57V9QXZ-jZ33zrUTsStRwFZHu5vL/s1600/stellarium+Naos.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj8LqrMebbIxvOUE5AsfGIeEQLuMlL4V6w95RLw1vi80bGKZDHTM80IzYWLWOYE2P6WTIy-3zMpkzGCEzSbbkZMy85u21aAEo6fYr0wZERC98tvjy5I57V9QXZ-jZ33zrUTsStRwFZHu5vL/s640/stellarium+Naos.jpg" height="422" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium trabalhado no Programa Corel</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Sigma Puppis - Estrela Dupla</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 07h27m Declinação - 43<sup>o</sup>.12<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude 3,3 e 8,5 Distância entre estrelas 22”,36<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>L Puppis - Estrela Variável</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 07h12m Declinação -44<sup>o</sup>.34<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitudes: Max 3,1 Min 6,3 Período 140,7<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo PLG Espectro M5e<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>V Puppis - Estrela Variável do tipo B Lyrae</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 07h56m Declinação -49<sup>o</sup>.06<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitudes: Max 4,1 Min 4,8 Período 1,5<o:p></o:p></span></div>
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<span lang="ES-TRAD"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo LIR Espectro B1<o:p></o:p></span></span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg9bjirg2-EhTWfV7JB933s-utiLi4Hjl0PhGxi8SdnVsDm8rG-QTpbWvp1DextCsZOWDXex9gU_5PbrcLwHQTEi3wDBF3ylOUUAUAS13IwtjgwuWnbRcPk_3opiLI3YMUiEMvMsZp3zAJx/s1600/stellarium+puppis+naos.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg9bjirg2-EhTWfV7JB933s-utiLi4Hjl0PhGxi8SdnVsDm8rG-QTpbWvp1DextCsZOWDXex9gU_5PbrcLwHQTEi3wDBF3ylOUUAUAS13IwtjgwuWnbRcPk_3opiLI3YMUiEMvMsZp3zAJx/s1600/stellarium+puppis+naos.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium trabalhado em Programa Corel</span><br />
<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 2477 - Aglomerado, em Puppis</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O mais rico dos muitos aglomerados existentes na Popa do Navio.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><br /><br /><b style="line-height: 19.1875px; text-align: start;">NGC 2477</b><span style="line-height: 19.1875px; text-align: start;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Puppis" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Puppis">constelação de Puppis</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Nicolas_Lacaille" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Nicolas Lacaille">Nicolas Lacaille</a><span style="line-height: 19.1875px; text-align: start;"> em 1751, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="line-height: 19.1875px; text-align: start;"> refrator com abertura de 0,5 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;"> (+5,8), é fracamente visível a </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Olho_nu" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Olho nu">olho nu</a><span style="line-height: 19.1875px; text-align: start;">, mesmo em regiões distantes de cidades.</span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_2477" style="text-decoration: none;">http://pt.wikipedia.org/wiki/NGC_2477</a><br /><b><br /></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://archive.stsci.edu/cgi-bin/dss_search?e=J2000&c=none&h=30&w=30&f=GIF&r=118.07514242056006&d=-38.5499755551101&v=all" height="640" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="638" /></span></div>
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<a href="http://archive.stsci.edu/cgi-bin/dss_search?e=J2000&c=none&h=30&w=30&f=GIF&r=118.07514242056006&d=-38.5499755551101&v=all" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://archive.stsci.edu/cgi-bin/dss_search?e=J2000&c=none&h=30&w=30&f=GIF&r=118.07514242056006&d=-38.5499755551101&v=all</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><a href="http://www.messier45.com/index.html#s/NGC%202477" style="text-decoration: none;">http://www.messier45.com/index.html#s/NGC%202477</a></span></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><br /><br /><br /><b><br /></b><b>M 46 - Aglomerado Aberto, em Puppis</b><o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M 47 - Aglomerado Aberto, em Puppis</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Estes dois Aglomerados podem ser vistos a olho nu e bem esfumaçadamente,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> próximos ao Cão Maior e sua estrela-Alpha, Sirius.<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 2437 - M 46 - Aglomerado Aberto Puppis<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 07h40m Declinação -14<sup>o</sup>.46<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 6,6 Magnitude fotográfica da mais brilhante estrela 10,8 Distância kpc 1,66 Diâmetro 27’ Tipo Espectral B8<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://cseligman.com/text/stars/messieropen.htm#46" style="text-decoration: none;">http://cseligman.com/text/stars/messieropen.htm#46</a><br /><a href="http://www.blogger.com/blogger.g?blogID=7155777971455253706" name="46" style="text-decoration: none;"><big><b>M46 (= </b></big></a><big><b><a href="http://cseligman.com/text/atlas/ngc24.htm#2437" style="text-decoration: none;">NGC 2437</a>)</b></big><br />Discovered (Feb 19, 1771) by <a href="http://cseligman.com/text/atlas/discoverers.htm#messier" style="text-decoration: none;">Messier</a><br />A 4th-magnitude open cluster in <a href="http://cseligman.com/text/atlas/puppis.htm#m46" style="text-decoration: none;">Puppis</a> (RA 07 36 35, Dec -14 28 47)<br />Click on the image (below) or the NGC link (above) for more information<br /><small>(Image Credit: N.A.Sharp/AURA/NSF/<a href="http://www.noao.edu/image_gallery/html/im0697.html" style="text-decoration: none;" target="noao">NOAO</a>)</small><br /><a href="http://cseligman.com/text/atlas/ngc24.htm#2437" style="text-decoration: none;"><img border="1" src="http://cseligman.com/text/stars/m46.jpg" height="750" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="750" /></a><br /><a href="http://www.blogger.com/blogger.g?blogID=7155777971455253706" name="47" style="text-decoration: none;"><br /><big><b>M47 (= </b></big></a><big><b><a href="http://cseligman.com/text/atlas/ngc24.htm#2422" style="text-decoration: none;">NGC 2422</a> = NGC 2478)</b></big><br />Recorded (1654) by <a href="http://cseligman.com/text/atlas/discoverers.htm#hodierna" style="text-decoration: none;">Giovanni Hodierna</a><br />Discovered (1771) by <a href="http://cseligman.com/text/atlas/discoverers.htm#messier" style="text-decoration: none;">Messier</a><br />A 4th-magnitude open cluster in <a href="http://cseligman.com/text/atlas/puppis.htm#m47" style="text-decoration: none;">Puppis</a> (RA 07 36 35, Dec -14 28 47)<br />Click on the image (below) or the NGC link (above) for more information<br /><small>(Image Credit: AURA/NSF/<a href="http://www.noao.edu/image_gallery/html/im0789.html" style="text-decoration: none;" target="noao">NOAO</a>)</small><br /><a href="http://cseligman.com/text/atlas/ngc24.htm#2422" style="text-decoration: none;"><img border="1" src="http://cseligman.com/text/stars/m47.jpg" height="750" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="750" /></a></span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://cseligman.com/text/stars/messieropen.htm#46" style="background-color: white; text-decoration: none;">http://cseligman.com/text/stars/messieropen.htm#46</a></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M 93 - Aglomerado Aberto, em Puppis</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 2422 - Aglomerado Aberto Puppis<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 07h34m Declinação -14<sup>o</sup>.27<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 4,3 Magnitude fotográfica da mais brilhante estrela 9,8<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distância kpc 0,48 Diâmetro 30’ Tipo Espectral B3<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><img alt="m93.jpg" src="http://www.allthesky.com/constellations/puppis/m93.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: normal; text-align: start;">M 93</b><span style="line-height: normal; text-align: start;">, NGC 2447, open cluster in Puppis (center)</span><br style="line-height: normal; text-align: start;" /><span style="line-height: normal; text-align: start;">visible with binoculars</span></span><br />
<a href="http://www.allthesky.com/constellations/puppis/dsos.html" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.allthesky.com/constellations/puppis/dsos.html</span></a><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><a href="http://www.allthesky.com/copyright.html" style="font-style: italic; line-height: normal; text-decoration: none;" target="_parent">© all photographs</a><span style="font-style: italic; line-height: normal;"> taken by </span><a href="mailto:credner@allthesky.de" style="font-style: italic; line-height: normal; text-decoration: none;">Till Credner</a><span style="font-style: italic; line-height: normal;"> and </span><a href="mailto:kohle@allthesky.de" style="font-style: italic; line-height: normal; text-decoration: none;">Sven Kohle</a></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Messier 93</b> (also known as <b>M93</b> or <b>NGC 2447</b>) is an <a href="http://en.wikipedia.org/wiki/Open_cluster" style="background-image: none; text-decoration: none;" title="Open cluster">open cluster</a> in the <a href="http://en.wikipedia.org/wiki/Constellation" style="background-image: none; text-decoration: none;" title="Constellation">constellation</a> <a href="http://en.wikipedia.org/wiki/Puppis" style="background-image: none; text-decoration: none;" title="Puppis">Puppis</a>. It was discovered by <a href="http://en.wikipedia.org/wiki/Charles_Messier" style="background-image: none; text-decoration: none;" title="Charles Messier">Charles Messier</a> in 1782.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">M93 is at a distance of about 3,600 <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Light_year" style="background-image: none; text-decoration: none;" title="Light year">light years</a> from Earth and has a spatial radius of some 10 to 12 light years. Its age is estimated at some 100 million years.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Walter_Scott_Houston" style="background-image: none; text-decoration: none;" title="Walter Scott Houston">Walter Scott Houston</a> described its appearance as follows:<sup class="reference" id="cite_ref-WSH_1-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_93#cite_note-WSH-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Some observers mention the cluster as having the shape of a starfish. With a fair-sized telescope, this is its appearance on a dull night, but [a four-inch refractor] shows it as a typical star-studded galactic cluster.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Messier_93" style="background-color: white; text-decoration: none;">http://en.wikipedia.org/wiki/Messier_93</a></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><br /><br /><img alt="File:Messier object 093.jpg" src="http://upload.wikimedia.org/wikipedia/commons/f/f0/Messier_object_093.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><br /><a href="http://en.wikipedia.org/wiki/File:Messier_object_093.jpg" style="text-decoration: none;">http://en.wikipedia.org/wiki/File:Messier_object_093.jpg</a></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>SOURCE</b>: <a class="external free" href="http://www.ipac.caltech.edu/2mass/gallery/messiercat.html" rel="nofollow" style="text-decoration: none;">http://www.ipac.caltech.edu/2mass/gallery/messiercat.html</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Acknowledgment</b>: <i>Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation.</i></span></div>
<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><br /><br /><a href="http://cseligman.com/text/stars/messieropen.htm#93" style="text-decoration: none;">http://cseligman.com/text/stars/messieropen.htm#93</a></span></span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.blogger.com/blogger.g?blogID=7155777971455253706" name="93" style="line-height: normal; text-decoration: none;"><big><b>M93 (= </b></big></a><big style="line-height: normal;"><b><a href="http://cseligman.com/text/atlas/ngc24.htm#2447" style="text-decoration: none;">NGC 2447</a> = OCL 649)</b></big><br style="line-height: normal;" /><span style="line-height: normal;">Discovered (Mar 20, 1781) by </span><a href="http://cseligman.com/text/atlas/discoverers.htm#messier" style="line-height: normal; text-decoration: none;">Charles Messier</a><br style="line-height: normal;" /><span style="line-height: normal;">A 6th-magnitude open cluster in </span><a href="http://cseligman.com/text/atlas/puppis.htm#m93" style="line-height: normal; text-decoration: none;">Puppis</a><span style="line-height: normal;"> (RA 07 44 30.0, Dec -23 51 24)</span><br style="line-height: normal;" /><span style="line-height: normal;">Click on the image (below) or the NGC link (above) for more information</span><br style="line-height: normal;" /><a href="http://cseligman.com/text/atlas/ngc24.htm#2447" style="line-height: normal; text-decoration: none;"><img alt="Wikisky image of M93" border="1" src="http://cseligman.com/text/stars/m93.jpg" height="750" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="750" /></a></span><br />
<a href="http://cseligman.com/text/stars/messieropen.htm#93" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://cseligman.com/text/stars/messieropen.htm#93</span></a><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 2451 - Aglomerado Aberto Puppis</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 07h44m Declinação -37<sup>o</sup>.55<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 3,7 Magnitude fotográfica da mais brilhante estrela 6,0 Distância kpc 0,30 Diâmetro 37’Tipo Espectral B5<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><b style="line-height: 19.1875px; text-align: start;">NGC 2451</b><span style="line-height: 19.1875px; text-align: start;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Puppis" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Puppis">constelação de Puppis</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="John Herschel">John Herschel</a><span style="line-height: 19.1875px; text-align: start;"> em 1835, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="line-height: 19.1875px; text-align: start;"> refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;"> (+2,8), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="line-height: 19.1875px; text-align: start;">amadores ou com equipamentos superiores.</span></span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_2451" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_2451</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><br /><br /><img alt="Ficheiro:NGC 2451 a.jpg" src="http://upload.wikimedia.org/wikipedia/commons/d/d7/NGC_2451_a.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><span style="line-height: 19.1875px;">Detalhe de uma das estrelas de NGC 2451</span></span></div>
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<a href="http://pt.wikipedia.org/wiki/Ficheiro:NGC_2451_a.jpg" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Ficheiro:NGC_2451_a.jpg</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br />Autor: Toraman</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><br /><img alt="ngc2451.jpg" src="http://www.allthesky.com/constellations/puppis/ngc2451.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: normal; text-align: start;">NGC 2451</b><span style="line-height: normal; text-align: start;">, open cluster in Puppis (center)</span><br style="line-height: normal; text-align: start;" /><span style="line-height: normal; text-align: start;">visible by naked eye</span></span></div>
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<a href="http://www.allthesky.com/constellations/puppis/dsos.html" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.allthesky.com/constellations/puppis/dsos.html</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><a href="http://www.allthesky.com/copyright.html" style="font-style: italic; line-height: normal; text-decoration: none;" target="_parent">© all photographs</a><span style="font-style: italic; line-height: normal;"> taken by </span><a href="mailto:credner@allthesky.de" style="font-style: italic; line-height: normal; text-decoration: none;">Till Credner</a><span style="font-style: italic; line-height: normal;"> and </span><a href="mailto:kohle@allthesky.de" style="font-style: italic; line-height: normal; text-decoration: none;">Sven Kohle</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 2546 - Aglomerado Aberto Puppis</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 08h11m Declinação -37<sup>o</sup>.35<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 5,0 Magnitude fotográfica da mais brilhante estrela 7,0<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Distância kpc 0,84 Diâmetro 45’ Tipo Espectral B0<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 2546</b><span style="line-height: 19.1875px; text-align: start;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Puppis" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Puppis">constelação de Puppis</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Nicolas_Lacaille" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Nicolas Lacaille">Nicolas Lacaille</a><span style="line-height: 19.1875px; text-align: start;"> em 1751, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="line-height: 19.1875px; text-align: start;"> refrator com abertura de 0,5 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;"> (+6,3), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="line-height: 19.1875px; text-align: start;">amadores ou com equipamentos superiores.</span></span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_2546" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_2546</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><br /><img alt="ngc2546.jpg" src="http://www.allthesky.com/constellations/puppis/ngc2546.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: normal; text-align: start;">NGC 2546</b><span style="line-height: normal; text-align: start;">, open cluster in Puppis (center)</span><br style="line-height: normal; text-align: start;" /><span style="line-height: normal; text-align: start;">visible with binoculars</span></span></div>
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<a href="http://www.allthesky.com/constellations/puppis/dsos.html" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.allthesky.com/constellations/puppis/dsos.html</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.allthesky.com/copyright.html" style="font-style: italic; line-height: normal; text-decoration: none;" target="_parent">© all photographs</a><span style="font-style: italic; line-height: normal;"> taken by </span><a href="mailto:credner@allthesky.de" style="font-style: italic; line-height: normal; text-decoration: none;">Till Credner</a><span style="font-style: italic; line-height: normal;"> and </span><a href="mailto:kohle@allthesky.de" style="font-style: italic; line-height: normal; text-decoration: none;">Sven Kohle</a></span></div>
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<h2 class="posttitle" style="border-bottom-color: rgb(85, 85, 85); border-bottom-style: dotted; border-width: 0px 0px 1px; font-size: 14px; font-weight: normal; line-height: 1.1em; margin: 3px 0px 2px; outline: 0px; padding: 0px 0px 4px; position: relative;">
<a class="entry-title" href="http://annesastronomynews.com/annes-picture-of-the-day-cometary-globule-cg4/" rel="bookmark" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none;" title="Anne’s Picture of the Day: Cometary Globule CG4"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Cometary Globule CG4</span></a></h2>
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<a href="http://annesastronomynews.com/photo-gallery-ii/nebulae-clouds/cometary-globule-cg4/" rel="attachment wp-att-9183" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="The Hand of God" class="aligncenter size-full wp-image-9183" src="http://annesastronomynews.com/wp-content/uploads/2012/02/Cometary-Globule-CG4.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; display: block; margin: 0px auto; max-width: 100%; outline: 0px; padding: 0px; position: relative;" width="1024" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Image Credit: <em style="border: 0px; margin: 0px; outline: 0px; padding: 0px;">T.A. Rector/University of Alaska Anchorage, T. Abbott and NOAO/AURA/NSF</em></span></div>
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<span style="border: 0px; margin: 0px; outline: 0px; padding: 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">CG4 (also known as The Hand of God) is a cometary globule that lies about 1,300 light-years away from Earth in the southern constellation of Puppis (the Stern). Its “head” is some 1.5 light-years across, and its “tail” is about eight light-years long. This dusty, star-forming region contains enough gas and dust to form several stars about the size of the Sun.</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://annesastronomynews.com/annes-picture-of-the-day-cometary-globule-cg4/" style="background-color: white; text-decoration: none;">http://annesastronomynews.com/annes-picture-of-the-day-cometary-globule-cg4/</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><br /><br /><br /><strong style="border: 0px; line-height: 25.59375px; margin: 0px; outline: 0px; padding: 0px;">Haffner 18, an open star cluster in Puppis</strong></span></div>
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<a href="http://annesastronomynews.com/photo-gallery-ii/galaxies-clusters/haffner-18/" rel="attachment wp-att-10332" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Haffner 18, an open star cluster in Puppis" class="aligncenter size-full wp-image-10332" src="http://annesastronomynews.com/wp-content/uploads/2012/02/Haffner-18.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; display: block; margin: 0px auto; max-width: 100%; outline: 0px; padding: 0px; position: relative;" width="1018" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Image Credit: <em style="border: 0px; margin: 0px; outline: 0px; padding: 0px;">ESO</em></span></div>
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<span style="border: 0px; margin: 0px; outline: 0px; padding: 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Haffner 18 is an open star cluster that lies in the center of the emission nebula NGC 2467, some 19,200 light-years away from Earth in the southern constellation of Puppis (the Stern). Its age is somewhat controversial, some considering it to be as young as only 1 million years.</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://annesastronomynews.com/annes-image-of-the-day-open-star-cluster-haffner-18/" style="background-color: white; text-decoration: none;">http://annesastronomynews.com/annes-image-of-the-day-open-star-cluster-haffner-18/</a></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></span></span></div>
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<strong style="border: 0px; margin: 0px; outline: 0px; padding: 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Puppis A, a middle-aged supernova remnant</span></strong></div>
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<a href="http://annesastronomynews.com/photo-gallery-ii/nebulae-clouds/seen-as-a-red-dusty-cloud-in-this-image-from-nasas-wise-puppis-a-is-the-remnant-of-a-supernova-explosion/" rel="attachment wp-att-6984" style="border: 0px; margin: 0px; outline: 0px; padding: 0px; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Puppis A, a middle-aged supernova remnant" class="aligncenter size-full wp-image-6984" src="http://annesastronomynews.com/wp-content/uploads/2012/02/Puppis-A.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; display: block; margin: 0px auto; max-width: 100%; outline: 0px; padding: 0px; position: relative;" width="1024" /></span></a></div>
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<a href="http://annesastronomynews.com/annes-picture-of-the-day-supernova-remnant-puppis-a/" style="line-height: 14px; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://annesastronomynews.com/annes-picture-of-the-day-supernova-remnant-puppis-a/</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Image Credit: <em style="border: 0px; margin: 0px; outline: 0px; padding: 0px;">NASA/JPL-Caltech/UCLA/WISE Team</em></span></div>
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<span style="border: 0px; margin: 0px; outline: 0px; padding: 0px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Puppis A is a middle-aged supernova remnant of about 10 light-years in diameter, located some 7,000 light-years away in our Milky Way, in the constellation of Puppis. The supernova explosion took place — and would have been seen on Earth as a new bright star in the sky — approximately 3700 years ago, but was eventually forgotten until modern astronomers found it again in October 1971.</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgz8g5ZF51SCwXd9082oz7ynHMvdLOaTAmLmdeg3EQC-i5F7LLOuz2lXP5ao9CzxSWiSWqh4LkOdJme0lTJPaSez4k5kQPSLPN2Jnr8JcbwPBfhHdvWwwCMnVEvRmGMgxPySyfTszhdshBL/s1600/CALABASH+NEBULA+EM+PUPPIS.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgz8g5ZF51SCwXd9082oz7ynHMvdLOaTAmLmdeg3EQC-i5F7LLOuz2lXP5ao9CzxSWiSWqh4LkOdJme0lTJPaSez4k5kQPSLPN2Jnr8JcbwPBfhHdvWwwCMnVEvRmGMgxPySyfTszhdshBL/s320/CALABASH+NEBULA+EM+PUPPIS.jpg" height="287" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(11, 83, 148); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="320" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://upload.wikimedia.org/wikipedia/commons/a/a1/Rotteneggnebula.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(11, 83, 148); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<a href="http://upload.wikimedia.org/wikipedia/commons/a/a1/Rotteneggnebula.jpg" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://upload.wikimedia.org/wikipedia/commons/a/a1/Rotteneggnebula.jpg</span></a></div>
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<span style="line-height: 19.1875px; text-align: start;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Rotten Egg Nebula JPEG converted from [http://www.jpl.nasa.gov/images/wfpc0824.tif TIF] @ JPL, NASA {{PD-USGov-NASA}</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The <b>Calabash Nebula</b>, also known as the <b>Rotten Egg Nebula</b> or by its technical name <b>OH 231.84 +4.22</b>, is a <a href="http://en.wikipedia.org/wiki/Protoplanetary_nebula" style="background-image: none; text-decoration: none;" title="Protoplanetary nebula">protoplanetary nebula</a> (PPN) 1.4 <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Light_year" style="background-image: none; text-decoration: none;" title="Light year">light years</a> (13 Pm) long and located some 5,000 light years (47 Em) from <a href="http://en.wikipedia.org/wiki/Earth" style="background-image: none; text-decoration: none;" title="Earth">Earth</a> in the constellation <a href="http://en.wikipedia.org/wiki/Puppis" style="background-image: none; text-decoration: none;" title="Puppis">Puppis</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Violent gas collisions that produced supersonic shock fronts in a dying star are seen in a new, detailed image from <a href="http://en.wikipedia.org/wiki/NASA" style="background-image: none; text-decoration: none;" title="NASA">NASA</a>'s <a href="http://en.wikipedia.org/wiki/Hubble_Space_Telescope" style="background-image: none; text-decoration: none;" title="Hubble Space Telescope">Hubble Space Telescope</a>.</span></div>
<table cellspacing="3" class="infobox" style="border-spacing: 3px; border: 1px solid rgb(170, 170, 170); clear: right; line-height: 1.5em; margin: 0.5em 0px 0.5em 1em; padding: 0.2em; width: 22em;"><tbody>
<tr><td colspan="2" style="text-align: center; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Calabash Nebula</span></td></tr>
<tr><th colspan="2" style="text-align: center; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Observation data <small>(<a href="http://en.wikipedia.org/wiki/Epoch_(astronomy)" style="background-image: none; text-decoration: none;" title="Epoch (astronomy)">Epoch</a> <a class="mw-redirect" href="http://en.wikipedia.org/wiki/J2000" style="background-image: none; text-decoration: none;" title="J2000">J2000</a>)</small></span></th></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Right_ascension" style="background-image: none; text-decoration: none;" title="Right ascension"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Right ascension</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">07<sup style="line-height: 1em;">h</sup> 42<sup style="line-height: 1em;">m</sup> 16.83<sup style="line-height: 1em;">s</sup> <sup class="reference" id="cite_ref-simbad_1-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Calabash_Nebula#cite_note-simbad-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Declination" style="background-image: none; text-decoration: none;" title="Declination"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Declination</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">−14° 42′ 52.1″<sup class="reference" id="cite_ref-simbad_1-1" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Calabash_Nebula#cite_note-simbad-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distance</span></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="mw-redirect" href="http://en.wikipedia.org/wiki/1_E19_m" style="background-image: none; text-decoration: none;" title="1 E19 m">4.2</a> <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Light_year" style="background-image: none; text-decoration: none;" title="Light year">kly</a> (1.3 <a href="http://en.wikipedia.org/wiki/Parsec" style="background-image: none; text-decoration: none;" title="Parsec">kpc</a>) <sup class="reference" id="cite_ref-Kastneretal1998_2-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Calabash_Nebula#cite_note-Kastneretal1998-2" style="background-image: none; text-decoration: none; white-space: nowrap;">[2]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Apparent_magnitude" style="background-image: none; text-decoration: none;" title="Apparent magnitude">Apparent magnitude</a> <small>(V)</small></span></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">9.47<sup class="reference" id="cite_ref-simbad_1-2" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Calabash_Nebula#cite_note-simbad-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apparent dimensions <small>(V)</small></span></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1′<sup class="Template-Fact" style="line-height: 1em; white-space: nowrap;">[<i><a href="http://en.wikipedia.org/wiki/Wikipedia:Citation_needed" style="background-image: none; text-decoration: none;" title="Wikipedia:Citation needed"><span title="This claim needs references to reliable sources. (February 2007)">citation needed</span></a></i>]</sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Constellation" style="background-image: none; text-decoration: none;" title="Constellation"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constellation</span></a></th><td style="vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Puppis" style="background-image: none; text-decoration: none;" title="Puppis"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Puppis</span></a></td></tr>
<tr><th colspan="2" style="text-align: center; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Physical characteristics</span></th></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Radius" style="background-image: none; text-decoration: none;" title="Radius"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Radius</span></a></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">0.7 ly<sup class="reference" id="ref_Anone" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Calabash_Nebula#endnote_Anone" style="background-image: none; text-decoration: none; white-space: nowrap;">[a]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Absolute_magnitude" style="background-image: none; text-decoration: none;" title="Absolute magnitude">Absolute magnitude</a> <small>(V)</small></span></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-1.4<sup class="reference" id="ref_Bnone" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Calabash_Nebula#endnote_Bnone" style="background-image: none; text-decoration: none; white-space: nowrap;">[b]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Notable features</span></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-</span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-size: inherit; vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Other designations</span></th><td style="vertical-align: top;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">OH 231.84 +4.22,<sup class="reference" id="cite_ref-simbad_1-3" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Calabash_Nebula#cite_note-simbad-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup><br />Rotten Eggs Nebula<sup class="reference" id="cite_ref-simbad_1-4" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Calabash_Nebula#cite_note-simbad-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></td></tr>
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<a href="http://en.wikipedia.org/wiki/Calabash_Nebula" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://en.wikipedia.org/wiki/Calabash_Nebula</span></a><br />
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<a href="http://apod.nasa.gov/apod/image/1309/rspuppis_bryne_3938.jpg" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="See Explanation. Clicking on the picture will download
the highest resolution version available." src="http://apod.nasa.gov/apod/image/1309/rspuppis_bryne_960.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(11, 83, 148); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></center>
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<a href="http://apod.nasa.gov/apod/ap130909.html" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://apod.nasa.gov/apod/ap130909.html</span></a></center>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Nearby Cepheid Variable RS Pup </b><br /><b>Image Credit: </b><a href="http://hla.stsci.edu/" style="text-decoration: none;">Hubble Legacy Archive</a>, <a href="http://www.nasa.gov/" style="text-decoration: none;">NASA</a>, <a href="http://www.esa.int/" style="text-decoration: none;">ESA</a> - <i>Processing: </i><a href="http://www.flickr.com/photos/stephen63/" style="text-decoration: none;">Stephen Byrne</a></span></center>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763;"><b>Authors & editors: </b><a href="http://www.phy.mtu.edu/faculty/Nemiroff.html" style="text-decoration: none;">Robert Nemiroff</a> (<a href="http://www.phy.mtu.edu/" style="text-decoration: none;">MTU</a>) & <a href="http://antwrp.gsfc.nasa.gov/htmltest/jbonnell/www/bonnell.html" style="text-decoration: none;">Jerry Bonnell</a> (<a href="http://www.astro.umd.edu/" style="text-decoration: none;">UMCP</a>)<br /><b>NASA Official: </b>Phillip Newman <a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply" style="text-decoration: none;">Specific rights apply</a>.<br /><a href="http://www.nasa.gov/about/highlights/HP_Privacy.html" style="text-decoration: none;">NASA Web Privacy Policy and Important Notices</a><br /><b>A service of:</b> <a href="http://astrophysics.gsfc.nasa.gov/" style="text-decoration: none;">ASD</a> at <a href="http://www.nasa.gov/" style="text-decoration: none;">NASA</a> / <a href="http://www.nasa.gov/centers/goddard/" style="text-decoration: none;">GSFC</a><br /><b>&</b> <a href="http://www.mtu.edu/" style="text-decoration: none;">Michigan Tech. U.</a></span></span><div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><img alt="The Night Sky Atlas logo image" src="http://www.nightskyatlas.com/logo.gif" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">The Night Sky Atlas</span></h1>
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<tr><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Visible in September before dawn, to May after dusk, best in January.</span></td></tr>
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<b><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Named Stars Index - The Night Sky Atlas<o:p></o:p></span></span></b></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Puppis: Visible in September before dawn, to May after dusk, best in January.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=7.822&declination=-24.860&viewAngle=25" style="text-decoration: none;">Asmidiske</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ξ<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Xi<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">´little shield´<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.astro.uiuc.edu/~jkaler/sow/asmidiske.html" style="text-decoration: none;" target="starnotes" title="Jim Kaler´s star notes for Asmidiske">Jim Kaler Notes</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=8.060&declination=-40.003&viewAngle=25" style="text-decoration: none;">Naos</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ζ<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Zeta<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">´ship´<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/starnames.jsp" style="text-decoration: none;">http://www.nightskyatlas.com/starnames.jsp</a><o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">DSO Names - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Puppis: Visible in September before dawn, to May after dusk, best in January.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=7.7417&declination=-23.8567&viewAngle=20.0" style="text-decoration: none;">Butterfly Cluster</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">M93<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">07h 44.5m<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-23° 51.4´<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(Jeff Bondono)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=7.705&declination=-14.7&viewAngle=20.0" style="text-decoration: none;">Calabash Nebula</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">07h 42.3m<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-14° 42.0´<o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">OH 231.8+4.2, planetary nebula in Pup (around QX Pup), also Rotten Egg Nebula<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=8.4017&declination=-43.0&viewAngle=20.0" style="text-decoration: none;">Puppis A</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">08h 24.1m<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-43° 00.0´<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">SNR, radio source<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=7.705&declination=-14.7&viewAngle=20.0" style="text-decoration: none;">Rotten Egg Nebula</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">07h 42.3m<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-14° 42.0´<o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">OH 231.8+4.2, planetary nebula in Pup (around QX Pup), also Calabash Nebula (STScI PRC99-39)<o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"> </span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/dsoNames.jsp" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/dsoNames.jsp</span></a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Asterisms - The Night Sky Atlas<o:p></o:p></span></h1>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Puppis: Visible in September before dawn, to May after dusk, best in January.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=8&declination=-45" style="text-decoration: none;">Argo Navis</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">0<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">53d X 39d<o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ancient constellation of Ship of the Argonauts; broken into Carina (keel);Puppis (poop deck); Vela (sails) and Carina (keel)<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=8.1333&declination=-15.1833" style="text-decoration: none;">Southern Little Queen</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">8<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">7' X 2'<o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Small Cassiopeia look-alike; not very prominent; by Magda Streicher<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/asterisms.jsp" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/asterisms.jsp</span></a><o:p></o:p></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Principal Stars of Puppis - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/stardata.jsp?id=PUP" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/stardata.jsp?id=PUP</span></a><o:p></o:p></span></h1>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Multiple Stars of Puppis - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/multipleStars.jsp?id=PUP" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/multipleStars.jsp?id=PUP</span></a><o:p></o:p></span></h1>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">NGC Objects in Puppis - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">IC Objects in Puppis - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/icData.jsp?id=PUP" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/icData.jsp?id=PUP</span></a><o:p></o:p></span></h1>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Galaxy Clusters of Puppis - The Night Sky Atlas<o:p></o:p></span></span></h1>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/catAbell.jsp?id=PUP" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/catAbell.jsp?id=PUP</span></a><span lang="EN-US"><o:p></o:p></span></span></h1>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgZZhxsivvQPjt7hhiHWf6Lh18bhwZOfWaTItfRQ61oN8_pAcgE1kOx4lqqoaai9p15ZG_zh6vFNNZiPb1pWn3-KN2RDjGZwim-fIvwVMTDfY-mBhJQztKAAFemvjggecIeKMefnEqHWPeK/s1600/sch4med.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgZZhxsivvQPjt7hhiHWf6Lh18bhwZOfWaTItfRQ61oN8_pAcgE1kOx4lqqoaai9p15ZG_zh6vFNNZiPb1pWn3-KN2RDjGZwim-fIvwVMTDfY-mBhJQztKAAFemvjggecIeKMefnEqHWPeK/s640/sch4med.jpg" height="437" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Julius Schiller, <i>Coelum stellatum Christianum</i>, 1627</span></div>
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<a href="http://www.lindahall.org/events_exhib/exhibit/exhibits/stars/cel_sch.htm" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.lindahall.org/events_exhib/exhibit/exhibits/stars/cel_sch.htm</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas – As Constelações - são como janelas que se abrem para a infinitude do universo e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra ...;</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e sendo por nossa mente conscientizado. </span><br />
<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"> Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">COM UM ABRAÇO ESTRELADO,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>REFERÊNCIAS BIBLIOGRÁFICAS IMPRESSAS:</b><o:p></o:p></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">COMPILAÇÃO E TRADUÇÃO literal (quando necessária) de Janine Milward:<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As Cartas Celestes foram realizadas por Mario Jaci Monteiro e escaneadas por Janine<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- </span><b>Mario Jaci Monteiro</b> , <b>As Constelações, Cartas Celestes</b> -<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- <b>Wil Tirion - Atlas of the Night Sky</b> - The Hamlyn Publishing Group Limited, London, England</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- <b>Antonin Rükl - The Hamlyn Encyclopedia of Stars & Planets</b> - The Hamlyn Publishng Group Limited, London, England</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- <b>Richard Hinckley Allen, Star Names, Their Lore and Meaning</b>, Dover Publications, Inc, New York, USA</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- <b>Bernard Pellequer - Pequeno Guia do Céu</b> - Editora Martins Fontes, São Paulo, Brasil</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- <b>Identificação do Céu</b> (Livro que foi sendo revisado e reeditado algumas vezes) de autoria de <b>Fernando Vieira</b>,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Secretaria Municipal de Cultura, Fundação Planetário da Cidade do Rio de Janeiro<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(com dedicatória do próprio autor para mim em Curso de Identificação do Céu,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em 30/07/1999))<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do <b>Atlas Celeste</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">de autoria de <b>Ronaldo Rogério de Freitas Mourão</b>,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(com dedicatória do próprio autor para mim<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em evento realizado no Museu de Astronomia do Rio de Janeiro,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em 16/06/1989)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As Cartas Celestes foram realizadas por Mario Jaci Monteiro e escaneadas por Janine</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- </span><b>Mario Jaci Monteiro</b> , <b>As Constelações, Cartas Celestes</b> -<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC - com dedicatória do autor para mim, em março de 2004 (quando Mário Jaci generosamente me presenteou com um instrumento de observação (kepleriano) artesanalmente construído por ele).<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 14px;">PUPPIS, A POPA (OU A PROA?) EM ARGO NAVIS, O NAVIO</span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://algarve-saibamais.blogspot.com.br/2013/04/carrancas-ou-figuras-de-proa.html" style="background-color: white; text-decoration: none;">http://algarve-saibamais.blogspot.com.br/2013/04/carrancas-ou-figuras-de-proa.html</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Hemisphaerium Coeli Australe in quo Fixarum loca secundum Eclipticae ductum ad anum 1730 . .</span></h2>
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<a href="http://www.raremaps.com/gallery/detail/35290/Hemisphaerium_Coeli_Australe_in_quo_Fixarum_loca_secundum_Eclipticae_ductum/Doppelmayr.html" style="text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Hemisphaerium Coeli Australe in quo Fixarum loca secundum Eclipticae ductum ad anum 1730 . ." src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEicMxVQEO9u4O0sVR33ZT0E6HH7Zs3a90ZceXwCU3Auix4ELYx57LaFn_2XBuq31UO000yC7nvlPstC5_gSACXakPHoOz3T-FdbYM_03dyGa1FiNEctB-emBFN-Cww2JYRcl7P2oZdBxxzw/s1260/MAPA+CELESTE+GRANDE.jpg" height="1044" id="Image2_img" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; visibility: visible;" width="1240" /> </span></a><br />
<span class="caption" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Nice example of Johanne Doppelmayr's map of the Southern Skies, with the constellations shown and the various stars illustrated in gold. Dopplemayr's decorative celestial chart illustrates the southern sky form the south ecliptic pole to ecliptic. The constellations are delineated based upon the catalogue of Johannes Hevelius and include Orion, Scorpio, Taurus, Eridanus and the Southern Cross. The constellations include some unusal additions, including the Peacock, Toucan, and a lovely unicorn called Monoceros.</span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-17032636603301736102013-08-20T08:09:00.002-07:002014-11-26T03:22:23.641-08:00PISCES AUSTRALIS, O PEIXE AUSTRAL<div align="center" class="MsoNormal" style="text-align: center;">
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px; text-align: start;">Meu Projeto</span></div>
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="font-size: small;">Da Terra ao Céu ....</span></span></a></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="font-size: small;">.....<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;">e ao Infinito </a></span></span></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><span style="font-size: small;">- As 88 Constelações</span></a></span></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;">http://daterraaoceueaoinfinito.blogspot.com.br/</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="background-color: #073763;"><img alt="" class="outset" src="http://www.constellationsofwords.com/images/PSApp.jpg" height="502" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(234, 231, 231); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 11px; padding: 8px;" width="429" /></span><br style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px; text-align: start;" /><span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 22.399999618530273px; text-align: start;">Johann Bode, <em>Uranographia</em>, 1801</span><br />
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<span style="color: #274e13; font-size: x-small; font-weight: normal;">DSS image of Fomalhaut (ground-based image)</span></h1>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.spacetelescope.org/images/heic0821f/" style="color: #274e13; text-decoration: none;">http://www.spacetelescope.org/images/heic0821f/</a></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">This image shows <b>Fomalhaut</b>, the star around which the newly discovered planet orbits. Fomalhaut is much hotter than our Sun, 15 times as bright, and lies 25 light-years from Earth. It is blazing through hydrogen at such a furious rate that it will burn out in only one billion years, 10% the lifespan of our star. The field of view is 2.7 x 2.9 degrees.</span></div>
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<span style="border: 0px; margin: 0px 0px 15px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Credit: </span></span><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">NASA, ESA, and the Digitized Sky Survey 2. Acknowledgment: Davide De Martin (ESA/Hubble)</span></div>
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<span style="color: #274e13;"><span lang="PT" style="font-family: Arial, sans-serif;">- </span><span style="font-family: Arial, sans-serif;">Mario Jaci Monteiro</span><span style="font-family: Arial, sans-serif;"> , As Constelações, Cartas Celestes - </span></span><span style="color: #274e13; font-family: Arial, sans-serif;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC</span><span style="color: #274e13; font-family: Arial, sans-serif;"> </span><span style="color: #274e13; font-family: Arial, sans-serif;">-</span><span style="color: #274e13; font-family: Arial, sans-serif;"> </span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgNhUxNkHzdK4k4FdG6ZOo8BxFiWgH7Y7TzYEwhw911N7co99URz0qGITPgZjVOkZ-ckLxOqvIwH7ixQLSTPP5vl6SaLBnOhGgItOx873cOsre1ThRo9ouoyxreawk50JgKNvM90FIBaJiH/s1600/urania26+(1).jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><span style="color: #073763;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgNhUxNkHzdK4k4FdG6ZOo8BxFiWgH7Y7TzYEwhw911N7co99URz0qGITPgZjVOkZ-ckLxOqvIwH7ixQLSTPP5vl6SaLBnOhGgItOx873cOsre1ThRo9ouoyxreawk50JgKNvM90FIBaJiH/s640/urania26+(1).jpg" height="446" width="640" /></span></a></div>
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<a class="link1" href="http://www.ianridpath.com/atlases/urania/urania26.jpg" style="text-decoration: none;"><span class="text1244" style="font-weight: bold;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Card 26</span></span></a></div>
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<span class="text1745"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; text-decoration: none;"><a class="link1" href="http://www.ianridpath.com/atlases/urania/urania26.jpg" style="text-decoration: none;">Aquarius, Piscis Australis, and Ballon Aerostatique</a></span></span></div>
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<a href="http://www.ianridpath.com/atlases/urania/urania26.jpg"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.ianridpath.com/atlases/urania/urania26.jpg</span></a></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/6/63/PiscisAustrinusCC.jpg" /></div>
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<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="line-height: 22.3999996185303px;">http://en.wikipedia.org/wiki/Piscis_Austrinus#mediaviewer/File:PiscisAustrinusCC.jpg</span></span></div>
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<span class="mw-mmv-title" original-title="" style="background-color: white; max-width: 60%;">The constellation Piscis Austrinus as it can be seen by the naked eye.</span></div>
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<span class="mw-mmv-source-author" original-title="" style="background-color: white; line-height: 1.8em;"><span class="mw-mmv-author"><a href="http://commons.wikimedia.org/wiki/User:Till_Credner" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="User:Till Credner">Till Credner</a></span> - <span class="mw-mmv-source"><span class="int-own-work">Own work</span>: <a class="external text" href="http://www.allthesky.com/constellations/visualconstellations.html" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">AlltheSky.com</a></span></span></div>
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<span style="color: #660000;"><b><span lang="EN-US" style="font-family: Arial, sans-serif;"> </span><span style="font-family: Arial, sans-serif;">PISCES AUSTRALIS, O PEIXE AUSTRAL</span></b></span></div>
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<span style="font-family: Arial, sans-serif;">Ascensão Reta 21h25m / 23h4m Declinação -25<sup>o</sup>.2 / -36<sup>o</sup>.7<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Vênus teria se transformado em um peixe, quando se banhava, certa vez.<o:p></o:p></span><br />
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<span style="font-family: Arial, sans-serif;">Esta constelação situa-se entre Aquarius e Grus e sua estrela Alpha, Fomalhaut, chama a atenção numa região do céu do sul que é bem menos preenchida por estrelas brilhantes - inclusive dentro dessa mesma constelação, onde os demais membros vão além magnitude 3.<o:p></o:p></span></div>
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<span style="color: #073763;"><span style="font-family: Arial, sans-serif;"><b>Fomalhaut</b></span><span style="font-family: Arial, sans-serif;"><b>. Alpha Piscis Australis. </b><o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;">Ascensão Reta 22h 56,5m - Declinação -29<sup>o</sup> 44’<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Magnitude visual 1,29 - Distância 22 anos-luz<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Uma estrela avermelhada na boca do Peixe ao Sul. De Fum al Hut, a Boca do Peixe. Foi uma das quatro estrelas reais da Pérsia, por volta de 3.000 anos a.um, atuando como a Guardiã do Sul e marcando o solstício de inverno.<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="color: #274e13;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986 </span></span><br />
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<a href="http://annesastronomynews.com/photo-gallery-ii/nebulae-clouds/fomalhaut-is-the-brightest-star-25-ly-away-in-piscis-austrinus-its-surrounding-dusty-disk-is-believed-to-be-protoplanetary-it-has-a-planet-in-the-habitable-zone/" rel="attachment wp-att-503" style="border: 0px; margin: 0px; outline: 0px; padding: 0px;"><span style="color: #073763;"><img alt="Fomalhaut" class="aligncenter size-large wp-image-503" src="http://annesastronomynews.com/wp-content/uploads/2012/02/Fomalhaut-is-the-brightest-star-25-ly-away-in-Piscis-Austrinus.-Its-surrounding-dusty-disk-is-believed-to-be-protoplanetary.-It-has-a-planet-in-the-habitable-zone-1024x486.jpg" style="border: none; display: block; margin: 0px auto; max-width: 100%; outline: 0px; padding: 0px;" width="695" /></span></a></div>
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<a href="http://annesastronomynews.com/evidence-for-asteroid-belt-around-the-star-vega/"><span style="color: #073763;">http://annesastronomynews.com/evidence-for-asteroid-belt-around-the-star-vega/</span></a></div>
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<span style="color: #073763;"><em style="border: 0px; margin: 0px; outline: 0px; padding: 0px;">Fomalhaut , approximately 25 light-years away, is the brightest star in the constellation Piscis Austrinus and one of the brightest stars in the sky.</em> Image Credit: <em style="border: 0px; margin: 0px; outline: 0px; padding: 0px;">NASA/Hubble</em></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 15px;"><b><span style="color: #660000;">Fomalhaut system</span></b></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://www.spacetelescope.org/static/archives/images/screen/opo1301b.jpg</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Fomalhaut system.</span></div>
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<span style="border: 0px; margin: 0px 0px 15px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Credit:<b> </b></span></span><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">NASA, ESA and P. Kalas (University of California, Berkeley, USA)</span></div>
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<tr><td colspan="2" style="background-color: #002060; line-height: 16px; margin-left: inherit; text-align: center;"><div style="line-height: inherit; margin-bottom: 0.5em; margin-top: 0.5em;">
<span style="color: white; font-size: small; text-transform: uppercase;"><b>PEIXE AUSTRAL</b></span></div>
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<tr><td colspan="2" style="background-color: white; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Piscis_Austrinus_constellation_map.png" style="background-image: none; color: #0b0080; text-decoration: none;"><img alt="Piscis Austrinus constellation map.png" data-file-height="1419" data-file-width="1789" src="http://upload.wikimedia.org/wikipedia/commons/thumb/9/90/Piscis_Austrinus_constellation_map.png/240px-Piscis_Austrinus_constellation_map.png" height="190" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/9/90/Piscis_Austrinus_constellation_map.png/360px-Piscis_Austrinus_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/9/90/Piscis_Austrinus_constellation_map.png/480px-Piscis_Austrinus_constellation_map.png 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="240" /></a></td></tr>
<tr><td style="padding: 0.4em 1em 0.4em 0.4em; width: 110px;"><b>Nome latino</b><br />
Genitivo</td><td style="padding: 0.4em 1em 0.4em 0.4em;"><div style="line-height: inherit; margin-bottom: 0.5em; margin-top: 0.5em;">
<b>Piscis Austrinus</b><br />
Piscis Austrini</div>
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<tr><td style="border-top-color: rgb(204, 221, 238); border-top-style: solid; border-top-width: 1px; padding: 0.4em 1em 0.4em 0.4em;">Abreviatura</td><td style="border-top-color: rgb(204, 221, 238); border-top-style: solid; border-top-width: 1px; padding: 0.4em 1em 0.4em 0.4em;">PsA</td></tr>
<tr><td colspan="2" style="background-color: #3333cc; border-top-color: rgb(0, 32, 96); border-top-style: solid; border-top-width: 3px; color: white; padding: 0.4em 1em 0.4em 0.4em;"><b> • Coordenadas</b></td></tr>
<tr><td style="padding: 0.4em 1em 0.4em 0.4em; width: 110px;"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-image: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Ascensão reta</a><br />
<a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-image: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="padding: 0.4em 1em 0.4em 0.4em;">h<br />
°</td></tr>
<tr><td style="border-top-color: rgb(204, 221, 238); border-top-style: solid; border-top-width: 1px; padding: 0.4em 1em 0.4em 0.4em;">Área total</td><td style="border-top-color: rgb(204, 221, 238); border-top-style: solid; border-top-width: 1px; padding: 0.4em 1em 0.4em 0.4em;">° quadrados</td></tr>
<tr><td colspan="2" style="background-color: #3333cc; border-top-color: rgb(0, 32, 96); border-top-style: solid; border-top-width: 3px; color: white; padding: 0.4em 1em 0.4em 0.4em;"><b> • Dados observacionais</b></td></tr>
<tr><td style="padding: 0.4em 1em 0.4em 0.4em; width: 110px;"><b>Visibilidade</b><br />
- <a href="http://pt.wikipedia.org/wiki/Latitude" style="background-image: none; color: #0b0080; text-decoration: none;" title="Latitude">Latitude</a> mínima<br />
- <a href="http://pt.wikipedia.org/wiki/Latitude" style="background-image: none; color: #0b0080; text-decoration: none;" title="Latitude">Latitude</a> máxima<br />
- <a href="http://pt.wikipedia.org/wiki/Meridiano_(astronomia)" style="background-image: none; color: #0b0080; text-decoration: none;" title="Meridiano (astronomia)">Meridiano</a></td><td style="padding: 0.4em 1em 0.4em 0.4em;"><br />
°<br />
°</td></tr>
<tr><td style="border-top-color: rgb(204, 221, 238); border-top-style: solid; border-top-width: 1px; padding: 0.4em 1em 0.4em 0.4em;"><b>Estrela principal</b><br />
- <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magn. apar.</a></td><td style="border-top-color: rgb(204, 221, 238); border-top-style: solid; border-top-width: 1px; padding: 0.4em 1em 0.4em 0.4em;"><b><a href="http://pt.wikipedia.org/wiki/Fomalhaut" style="background-image: none; color: #0b0080; text-decoration: none;" title="Fomalhaut">Fomalhaut</a> (α Piscis Austrini)</b><br />
1,16</td></tr>
<tr><td style="border-top-color: rgb(204, 221, 238); border-top-style: solid; border-top-width: 1px; padding: 0.4em 1em 0.4em 0.4em;"><b>Outras estrelas</b><br />
- <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magn. apar.</a> < 3<br />
- <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magn. apar.</a> < 6</td><td style="border-top-color: rgb(204, 221, 238); border-top-style: solid; border-top-width: 1px; padding: 0.4em 1em 0.4em 0.4em;"><br />
1<br />
-</td></tr>
<tr><td colspan="2" style="background-color: #3333cc; border-top-color: rgb(0, 32, 96); border-top-style: solid; border-top-width: 3px; color: white; padding: 0.4em 1em 0.4em 0.4em;"><b> • Chuva de meteoros</b></td></tr>
<tr><td colspan="2" style="padding: 0.4em 1em 0.4em 0.4em;"><div style="line-height: inherit; margin-bottom: 0.5em; margin-top: 0.5em;">
<a href="http://pt.wikipedia.org/wiki/Piscis_Austrin%C3%ADdeos" style="background-image: none; color: #0b0080; text-decoration: none;" title="Piscis Austrinídeos">Piscis Austrinídeos</a></div>
</td></tr>
<tr><td colspan="2" style="background-color: #3333cc; border-top-color: rgb(0, 32, 96); border-top-style: solid; border-top-width: 3px; color: white; padding: 0.4em 1em 0.4em 0.4em;"><b> • Constelações limítrofes</b></td></tr>
<tr><td colspan="2" style="padding: 0.4em 1em 0.4em 0.4em;"><small>Em sentido horário:</small><br />
<ul style="line-height: 1.5em; list-style-image: initial; list-style-position: initial; margin: 0.5em 0px; padding: 0px 2.5em;">
<li style="border: none; color: #073763; margin: 0px 0px 0.1em; padding: 0.25em 0px;"><a href="http://pt.wikipedia.org/wiki/Aquarius" style="background-image: none; color: #0b0080; text-decoration: none;" title="Aquarius">Aquarius</a></li>
<li style="border: none; color: #073763; margin: 0px 0px 0.1em; padding: 0.25em 0px;"><a href="http://pt.wikipedia.org/wiki/Capricornus" style="background-image: none; color: #0b0080; text-decoration: none;" title="Capricornus">Capricornus</a></li>
<li style="border: none; color: #073763; margin: 0px 0px 0.1em; padding: 0.25em 0px;"><a href="http://pt.wikipedia.org/wiki/Microscopium" style="background-image: none; color: #0b0080; text-decoration: none;" title="Microscopium">Microscopium</a></li>
<li style="border: none; color: #073763; margin: 0px 0px 0.1em; padding: 0.25em 0px;"><a href="http://pt.wikipedia.org/wiki/Grus" style="background-image: none; color: #0b0080; text-decoration: none;" title="Grus">Grus</a></li>
<li style="border: none; color: #073763; margin: 0px 0px 0.1em; padding: 0.25em 0px;"><a href="http://pt.wikipedia.org/wiki/Sculptor" style="background-image: none; color: #0b0080; text-decoration: none;" title="Sculptor">Sculptor</a></li>
</ul>
<div>
<span style="line-height: 18px;"><br /></span></div>
<div>
<span style="line-height: 18px;"><a href="http://pt.wikipedia.org/wiki/Piscis_Austrinus" style="color: #274e13; text-decoration: none;"><span style="font-size: x-small;">http://pt.wikipedia.org/wiki/Piscis_Austrinus</span></a></span></div>
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<b><span style="color: #660000; font-size: medium;">Alpha Piscis Austrini</span></b><span style="color: #252525;"> mais conhecida como </span><span style="color: #660000; font-size: medium;"><b>Fomalhaut</b> </span><span style="color: #252525;">é a </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-image: none; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a><span style="color: #252525;"> mais brilhante da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a><span style="color: #252525;"> de Peixe Austral (</span><a href="http://pt.wikipedia.org/wiki/Piscis_Austrinus" style="background-image: none; color: #0b0080; text-decoration: none;" title="Piscis Austrinus">Piscis Austrinus</a><span style="color: #252525;">), e é uma das 4 estrelas reais dos persas – junto com </span><a href="http://pt.wikipedia.org/wiki/Antares" style="background-image: none; color: #0b0080; text-decoration: none;" title="Antares">Antares</a><span style="color: #252525;"> (α Scorpii),</span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aldebaran" style="background-image: none; color: #0b0080; text-decoration: none;" title="Aldebaran">Aldebaran</a><span style="color: #252525;"> (α Tauri) e </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Regulus" style="background-image: none; color: #0b0080; text-decoration: none;" title="Regulus">Regulus</a><span style="color: #252525;"> (α Leonis).</span></div>
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Em torno desta estrela foi detectado um planeta cerca de três vezes mais massivo que Júpiter. Este <a href="http://pt.wikipedia.org/wiki/Exoplaneta" style="background-image: none; color: #0b0080; text-decoration: none;" title="Exoplaneta">exoplaneta</a> (<a href="http://pt.wikipedia.org/wiki/Fomalhaut_b" style="background-image: none; color: #0b0080; text-decoration: none;" title="Fomalhaut b">Fomalhaut b</a>) foi detetado visualmente pela comparação de imagens obtidas pelo <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Hubble" style="background-image: none; color: #0b0080; text-decoration: none;" title="Telescópio Hubble">telescópio Hubble</a>de 2004 e 2006.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Fomalhaut#cite_note-1" style="background-image: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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<span class="mw-headline" id="Etimologia"><span style="font-size: x-small;">Etimologia</span></span></h2>
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<b>Fomalhaut</b> é uma palavra de origem <a href="http://pt.wikipedia.org/wiki/%C3%81rabe" style="background-image: none; color: #0b0080; text-decoration: none;" title="Árabe">árabe</a> e significa "boca do peixe".</div>
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<span class="mw-headline" id="Exoplanetas"><span style="font-size: x-small;">Exoplanetas</span></span></h2>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Fomalhaut_with_Disk_Ring_and_extrasolar_planet_b.jpg" style="background-image: none; color: #0b0080; text-decoration: none;"><img alt="Fomalhaut with Disk Ring and extrasolar planet b.jpg" data-file-height="1899" data-file-width="2843" src="http://upload.wikimedia.org/wikipedia/commons/thumb/a/a3/Fomalhaut_with_Disk_Ring_and_extrasolar_planet_b.jpg/250px-Fomalhaut_with_Disk_Ring_and_extrasolar_planet_b.jpg" height="167" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/a/a3/Fomalhaut_with_Disk_Ring_and_extrasolar_planet_b.jpg/375px-Fomalhaut_with_Disk_Ring_and_extrasolar_planet_b.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/a/a3/Fomalhaut_with_Disk_Ring_and_extrasolar_planet_b.jpg/500px-Fomalhaut_with_Disk_Ring_and_extrasolar_planet_b.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; margin: 0px; padding: 8px; position: relative; vertical-align: middle;" width="250" /></a></div>
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Em <a href="http://pt.wikipedia.org/wiki/13_de_novembro" style="background-image: none; color: #0b0080; text-decoration: none;" title="13 de novembro">13 de novembro</a> de <a href="http://pt.wikipedia.org/wiki/2008" style="background-image: none; color: #0b0080; text-decoration: none;" title="2008">2008</a>, a <a href="http://pt.wikipedia.org/wiki/NASA" style="background-image: none; color: #0b0080; text-decoration: none;" title="NASA">NASA</a> anunciou as primeiras imagens fotográficas obtidas de <a href="http://pt.wikipedia.org/wiki/Fomalhaut_b" style="background-image: none; color: #0b0080; text-decoration: none;" title="Fomalhaut b">Fomalhaut b</a>, através do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Hubble" style="background-image: none; color: #0b0080; text-decoration: none;" title="Telescópio Hubble">telescópio Hubble</a>, o que o torna o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Planeta_extra-solar" style="background-image: none; color: #0b0080; text-decoration: none;" title="Planeta extra-solar">planeta extra-solar</a> fotografado da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-image: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>.<span class="reference" id="cite_ref-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Fomalhaut#cite_note-2" style="background-image: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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<h2 style="background-color: white; background-image: none; border-bottom-color: rgb(170, 170, 170); border-bottom-style: solid; border-bottom-width: 1px; color: #073763; cursor: help; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 14px; margin: 1em 0px 0.25em; overflow: hidden; padding: 0px; position: relative; text-align: start;" title="Esta seção foi configurada para não ser editável diretamente. Edite a página toda ou a seção anterior em vez disso.">
<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><span style="font-weight: normal; line-height: 31.200000762939453px;"><a href="http://pt.wikipedia.org/wiki/Fomalhaut" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Fomalhaut</a></span></span></h2>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">Fomalhaut b</span></b><span style="color: #252525;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Planeta_extra-solar" style="background-image: none; color: #0b0080; text-decoration: none;" title="Planeta extra-solar">planeta extra-solar</a><span style="color: #252525;"> que orbita a </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-image: none; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a><span style="color: #252525;"> </span><a href="http://pt.wikipedia.org/wiki/Fomalhaut" style="background-image: none; color: #0b0080; text-decoration: none;" title="Fomalhaut">Fomalhaut</a><span style="color: #252525;">, três </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Bilh%C3%A3o" style="background-image: none; color: #0b0080; text-decoration: none;" title="Bilhão">bilhões</a><span style="color: #252525;"> de </span><a href="http://pt.wikipedia.org/wiki/Quil%C3%B4metro" style="background-image: none; color: #0b0080; text-decoration: none;" title="Quilômetro">quilômetros</a><span style="color: #252525;"> dentro de seu anel orbital de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Poeira_estelar" style="background-image: none; color: #0b0080; text-decoration: none;" title="Poeira estelar">poeira estelar</a><span class="reference" id="cite_ref-1" style="bottom: 1ex; color: #252525; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Fomalhaut_b#cite_note-1" style="background-image: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span><span style="color: #252525;"> e o primeiro exoplaneta a ser descoberto por fotografias, após oito anos de pesquisas tentando estabelecer sua posição.</span><span class="reference" id="cite_ref-times_2-0" style="bottom: 1ex; color: #252525; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Fomalhaut_b#cite_note-times-2" style="background-image: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Sua existência, antes apenas <a href="http://pt.wikipedia.org/wiki/Teoria" style="background-image: none; color: #0b0080; text-decoration: none;" title="Teoria">teórica</a> foi confirmada pela NASA em <a href="http://pt.wikipedia.org/wiki/13_de_novembro" style="background-image: none; color: #0b0080; text-decoration: none;" title="13 de novembro">13 de novembro</a> de <a href="http://pt.wikipedia.org/wiki/2008" style="background-image: none; color: #0b0080; text-decoration: none;" title="2008">2008</a>, quando a agência espacial norte-americana divulgou fotografias do planeta tiradas pelo <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_espacial_Hubble" style="background-image: none; color: #0b0080; text-decoration: none;" title="Telescópio espacial Hubble">telescópio espacial Hubble</a>. Localizado a 25 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-image: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>, na constelação de <a href="http://pt.wikipedia.org/wiki/Piscis_Austrinus" style="background-image: none; color: #0b0080; text-decoration: none;" title="Piscis Austrinus">Piscis Austrinus</a>,<span class="reference" id="cite_ref-borenstein_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Fomalhaut_b#cite_note-borenstein-3" style="background-image: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> o planeta tem o tamanho de Júpiter<span class="reference" id="cite_ref-times_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Fomalhaut_b#cite_note-times-2" style="background-image: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> e três vezes a sua<a href="http://pt.wikipedia.org/wiki/Massa" style="background-image: none; color: #0b0080; text-decoration: none;" title="Massa">massa</a> e acredita-se ser o objeto com menor massa já visto fora das vizinhanças do nosso <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Sistema_solar" style="background-image: none; color: #0b0080; text-decoration: none;" title="Sistema solar">sistema solar</a>.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Fomalhaut b teve sua existência descoberta em <a href="http://pt.wikipedia.org/wiki/2005" style="background-image: none; color: #0b0080; text-decoration: none;" title="2005">2005</a>, devido ao movimento de sua <a href="http://pt.wikipedia.org/wiki/%C3%93rbita" style="background-image: none; color: #0b0080; text-decoration: none;" title="Órbita">órbita</a> dentro do cinturão de <a href="http://pt.wikipedia.org/wiki/Poeira" style="background-image: none; color: #0b0080; text-decoration: none;" title="Poeira">poeira</a> que envolve a estrela Fomalhaut, mas foi localizado apenas em maio de <a href="http://pt.wikipedia.org/wiki/2008" style="background-image: none; color: #0b0080; text-decoration: none;" title="2008">2008</a> pelo <a href="http://pt.wikipedia.org/wiki/Astr%C3%B4nomo" style="background-image: none; color: #0b0080; text-decoration: none;" title="Astrônomo">astrônomo</a> Paul Kalas, através da comparação de <a href="http://pt.wikipedia.org/wiki/Fotografia" style="background-image: none; color: #0b0080; text-decoration: none;" title="Fotografia">fotografias</a> do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Hubble" style="background-image: none; color: #0b0080; text-decoration: none;" title="Hubble">Hubble</a> tiradas em <a href="http://pt.wikipedia.org/wiki/2004" style="background-image: none; color: #0b0080; text-decoration: none;" title="2004">2004</a> e <a href="http://pt.wikipedia.org/wiki/2006" style="background-image: none; color: #0b0080; text-decoration: none;" title="2006">2006</a>.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">O planeta se localiza a cerca de dezoito bilhões de quilômetros de seu sol e sua órbita em torno dele leva 872 anos terrestres para ser completada.<span class="reference" id="cite_ref-times_2-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Fomalhaut_b#cite_note-times-2" style="background-image: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> Também acredita-se que seja circundado por anéis, em maior quantidade e mais largos que aqueles que envolvem <a href="http://pt.wikipedia.org/wiki/An%C3%A9is_de_Saturno" style="background-image: none; color: #0b0080; text-decoration: none;" title="Anéis de Saturno">Saturno</a>.<span class="reference" id="cite_ref-times_2-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Fomalhaut_b#cite_note-times-2" style="background-image: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></span></div>
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<span style="color: #7f6000; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Fomalhaut_b" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Fomalhaut_b</a></span></div>
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<span style="font-size: medium;">Hubble directly observes planet orbiting Fomalhaut</span></h1>
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The NASA/ESA Hubble Space Telescope has taken the first visible light snapshot of a planet circling another star.</div>
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Estimated to be no more than three times Jupiter's mass, the planet, called Fomalhaut b, orbits the bright southern star Fomalhaut, located 25 light-years away in the constellation Piscis Austrinus (the Southern Fish).</div>
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Fomalhaut has been a candidate for planet hunting ever since an excess of dust was discovered around the star in the early 1980s by the US- UK-Dutch Infrared Astronomy Satellite (IRAS).</div>
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SAIBA MAIS ACESSANDO</div>
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<span style="color: #274e13; font-family: Arial, Helvetica, san-serif;"><span style="line-height: 15px;"><a href="http://www.spacetelescope.org/news/heic0821/" style="color: #274e13; text-decoration: none;">http://www.spacetelescope.org/news/heic0821/</a></span></span></div>
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<span style="color: #274e13;"><a href="http://www.spacetelescope.org/static/archives/images/pl_screen/heic0821a.jpg" style="color: #274e13; text-decoration: none;">http://www.spacetelescope.org/static/archives/images/pl_screen/heic0821a.jpg</a></span></div>
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This image, taken with the Advanced Camera for Surveys aboard the NASA/ESA Hubble Space Telescope, shows the newly discovered planet, Fomalhaut b, orbiting its parent star, Fomalhaut.</div>
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The small white box at lower right pinpoints the planet's location. Fomalhaut b has carved a path along the inner edge of a vast, dusty debris ring encircling Fomalhaut that is 34.5 billion kilometres across. Fomalhaut b lies three billion kilometres inside the ring's inner edge and orbits 17 billion kilometres from its star.</div>
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The inset at bottom right is a composite image showing the planet's position during Hubble observations taken in 2004 and 2006. Astronomers have calculated that Fomalhaut b completes an orbit around its parent star every 872 years.</div>
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The white dot in the centre of the image marks the star's location. The region around Fomalhaut's location is black because astronomers used the Advanced Camera's coronagraph to block out the star's bright glare so that the dim planet could be seen. Fomalhaut b is 100 million times fainter than its star. The radial streaks are scattered starlight. The red dot at lower left is a background star.</div>
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The Fomalhaut system is 25 light-years away in the constellation Piscis Austrinus.</div>
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This false-colour image was taken in October 2004 and July 2006.</div>
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<span style="border: 0px; margin: 0px 0px 15px; outline: 0px; padding: 0px; vertical-align: baseline;">Credit:</span></div>
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NASA, ESA and P. Kalas (University of California, Berkeley, USA)</div>
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<span style="color: #274e13;">This annotated image shows key features of the Fomalhaut system, including the newly discovered planet Fomalhaut b, and the dust ring. Also included are a distance scale and an insert, showing how the planet has moved around its parent star over the course of 21 months. The Fomalhaut system is located approximately 25 light-years from the Earth.</span></div>
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<span style="border: 0px; margin: 0px 0px 15px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="color: #274e13;">Credit:</span></span></div>
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<span style="color: #274e13;">NASA, ESA, and Z. Levay (STScI)</span></div>
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<span style="color: #274e13;">This diagram shows the orbit of the exoplanet Fomalhaut b as calculated from recent Hubble Space Telescope observations. The planet follows a highly elliptical orbit that carries it across a wide belt of debris encircling the bright star Fomalhaut. The planet swings as close to its star as 7.4 billion kilometres, and the outermost point of its orbit is 43 billion kilometres away from the star. The orbital period is approximately 2000 years.</span></div>
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<span style="color: #274e13;">Illustration Credit: NASA, ESA and A. Feild (STScI).</span></div>
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<span style="color: #274e13;">Science Credit: NASA, ESA and P. Kalas (University of California, Berkeley, USA)</span></div>
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Hubblecast 22: Hubble directly observes planet orbiting Fomalhaut</span></span></h1>
<span style="background-color: white;"><span class="small" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.spacetelescope.org/videos/heic0821a/" style="color: #274e13; text-decoration: none;">http://www.spacetelescope.org/videos/heic0821a/</a></span></span><br style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px; text-align: start;" /><span class="small" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 8px;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></span><span style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px; text-align: start;"></span><span class="small" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 8px;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></span><span style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px; text-align: start;"></span><span class="small" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 8px;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></span><span style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px; text-align: start;"></span><span style="font-size: large;"><span class="small" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></span><span style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px; text-align: start;"></span><span class="small" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"></span></span></span><br />
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Zomming on Fomalhaut b</span></span></h1>
<span class="small" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.spacetelescope.org/videos/heic0821c/" style="background-color: white; color: #274e13; text-decoration: none;">http://www.spacetelescope.org/videos/heic0821c/</a></span></span><br style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px; text-align: start;" /><span class="small" style="background-color: #eae7e7; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"><br /></span><span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px; text-align: start;"></span></span><span class="small" style="background-color: #eae7e7; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"><br /></span><span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px; text-align: start;"></span></span><span class="small" style="background-color: #eae7e7; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"><br /></span><span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px; text-align: start;"></span></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Fomalhaut é uma das quatro estrelas reais </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>(assim consideradas pelos antigos persas),</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>sendo a única estrela (entre as quatro)</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>que se situa mais distanciada da Linha da Eclíptica </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>- pois que as demais três estrelas reais assim beijavam </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>este aparente caminho do Sol durante a Era de Touro</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>- Aldebaran (alpha Tauri), Regulus (alpha Leonis) e Antares (alpha Scorpii).</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><span style="font-size: medium;">As Quatro Estrelas-Reais dos antigos Persas </span></b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><span style="font-size: medium;">ocupando os quatro cantos dos céus estrelados.....</span></b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><span style="font-size: medium;"> - nos dias de hoje:</span></b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Caro Leitor, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">observe nestas Ilustrações abaixo as mudanças que ocorreram em termos dos posicionamentos dos pontos dos Equinócios e dos Solstícios entre as estrelas mencionadas - as quatro estrelas-reais dos Persas - e a Linha da Eclíptica e do Equador Celeste nos dias de hoje.</span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjQ9wuxVam-ixMZtKfYOE6j34HnLejv29U5gAaXjDnAG-Wdb-Me0rYhw8B7DfOlrnZKeZIry-cxcgNvMeqURtwudNBHQX8f8pb1m99CxIkUt3IYYyIDp3HkqcMCCsHIfV5v3WV0jOwXW0c/s1600/touro+e+regulus.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjQ9wuxVam-ixMZtKfYOE6j34HnLejv29U5gAaXjDnAG-Wdb-Me0rYhw8B7DfOlrnZKeZIry-cxcgNvMeqURtwudNBHQX8f8pb1m99CxIkUt3IYYyIDp3HkqcMCCsHIfV5v3WV0jOwXW0c/s1600/touro+e+regulus.jpg" height="564" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></a></div>
<span style="font-family: Arial, Helvetica, sans-serif; font-size: xx-small;">Programa Stellarium trabalhado no Programa Corel</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Vemos nesta Ilustração, a estrela-alpha Tauri, <b>Aldebaran, trazendo a Primavera, a Guardiã do Leste</b>, uma das quatro estrelas-reais dos Persas. </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"> E vemos também a estrela-alpha Leonis, <b>Regulus, trazendo o Verão, a Guardiã do Sul.</b></span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjqfZiNt-j-yqlMo9A6ZWv55SrtsHmTn3-iS9lay4L02zBDMVWvQRTX31JSONc5hbPiQWX4nR3cO8XRasiBKm_C5EjEZX4T_q06cmTUc6zPr1D519lxhVd1W8DlWyqx-ZuKZqYBjucnnsg/s1600/antares+e+fomalhaut.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjqfZiNt-j-yqlMo9A6ZWv55SrtsHmTn3-iS9lay4L02zBDMVWvQRTX31JSONc5hbPiQWX4nR3cO8XRasiBKm_C5EjEZX4T_q06cmTUc6zPr1D519lxhVd1W8DlWyqx-ZuKZqYBjucnnsg/s1600/antares+e+fomalhaut.jpg" height="540" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></a></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: xx-small;">Programa Sellarium trabalhado no Programa Corel</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Vemos nesta Ilustração, a estrela-alpha Scorpii, <b>Antares, trazendo o Outono, a guardiã do Oeste. </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">E vemos também a estrela-alpha Piscis Austrinus, <b>Fomalhaut, trazendo o Inverno, a Guardiã do Norte</b><br /><span style="text-align: start;"></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Sabemos que a estrela Fomalhaut não fez parte das constelações da Linha da Eclíptica. Porém, esta é a estrela mais proeminente durante o céu noturno do inverno, a partir do ponto de vista do hemisfério norte.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Excerto de minha Página </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Sobre a Constelação de Cancer, o Caranguejo:</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><a href="http://sobrecaranguejo.blogspot.com.br/" style="color: #274e13; text-decoration: none;">http://sobrecaranguejo.blogspot.com.br/</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;">É realmente interessante que possamos perceber</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;"> as questões relativas às mudanças de Eras</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;"> em termos de onde caem os Pontos de Equinócios e de Solstícios:</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A Era de Gêmeos trouxe o Ponto Vernal a acontecer dentro desta constelação ocupando o lugar de Primavera, Virgem ocupando o lugar do Solstício do Verão, Sagitário ocupando o lugar do Equinócio do Outono e Peixes ocupando o lugar do Solstício de Inverno.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #274e13;">Quadro sobre a Precessão dos Equinócios durante 4 Eras, mostrando o Caminho do Sol contra o pano de fundo das constelações do Zodíaco. As cores originais foram invertidas.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #274e13;">Inserido no Artigo “When the Zodiac Climbed into the Sky” por Alexander Gurshtein para a Revista Sky & Telescope edição de outubro de 1995, página 30, publicada por Sky Publishing Corporation, Cambridge, MA, USA.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A Era de Touro trouxe o Ponto Vernal a acontecer dentro desta constelação ocupando o lugar de Equinócio da Primavera; Leão ocupando o lugar do Solstício do Verão; Sagitário ocupando o lugar do Equinócio do Outono e Peixes ocupando o lugar do Solstício de Inverno.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Permita-me lhes dizer, caro Amigo das Estrelas, que teria sido naquela Era que surgiu o conceito das Quatro Estrelas Reais, Guardiãs das Quatro Estações do Ano e da Vida: em Touro, Aldebarã, o olho iluminado, guardiã do Leste; em Leão, Regulus, sua pata dianteira, guardiã do Sul; em Escorpião, Antares, a rival de Marte, Anti-Ars, gigante vermelha maravilhosa, guardiã do Oeste; e finalmente, Fomalhaut, em Pisces Austrinus, guardiã do Norte.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A Era de Áries trouxe o Ponto Vernal a acontecer dentro desta constelação ocupando o lugar de Equinócio da Primavera; Câncer ocupando o lugar de Solstício do Verão; Balança ocupando o lugar do Equinócio do Outono e Capricórnio ocupando o lugar do Solstício de Inverno.</span><br /><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span><br /><span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<b><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">HD 216770 b</span><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Planeta_extrassolar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Planeta extrassolar">planeta extrassolar</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> orbitando a estrela </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=HD_216770&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="HD 216770 (página não existe)">HD 216770</a></b><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">. Sua massa equivale a dois terços da massa de </span><a href="http://pt.wikipedia.org/wiki/J%C3%BApiter_(planeta)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Júpiter (planeta)">Júpiter</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, o maior planeta do sistema solar. Mas diferentemente do </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Gigante_gasoso" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Gigante gasoso">gigante gasoso</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> do sistema solar, este </span><a href="http://pt.wikipedia.org/wiki/Planeta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Planeta">planeta</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> segue uma órbita muito mais </span><a href="http://pt.wikipedia.org/wiki/Excentricidade_orbital" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Excentricidade orbital">excêntrica</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> ao redor de sua estrela. A distância média entre HD 216770 b e sua estrela-mãe é ligeiramente maior que a de </span><a href="http://pt.wikipedia.org/wiki/Merc%C3%BArio_(planeta)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Mercúrio (planeta)">Mercúrio</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> em relação ao </span><a href="http://pt.wikipedia.org/wiki/Sol" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Sol">Sol</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">. Sua revolução dura 118 </span><a href="http://pt.wikipedia.org/wiki/Dia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Dia">dias</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">.</span><br />
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<tr><th colspan="2" style="background-color: #a0b0ff;" width="140px"><small><a href="http://pt.wikipedia.org/wiki/Exoplaneta" style="background: none; color: #0b0080; text-decoration: none;" title="Exoplaneta">Exoplaneta</a></small></th><td align="center" width="160px"><small><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anexo:Lista_de_estrelas_com_exoplaneta" style="background: none; color: #0b0080; text-decoration: none;" title="Anexo:Lista de estrelas com exoplaneta">Lista de exoplanetas</a></small></td></tr>
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<tr><th colspan="3" style="background-color: #a0b0ff;">Estrela mãe</th></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">Estrela</a></b></td><td align="left"><a class="new" href="http://pt.wikipedia.org/w/index.php?title=HD_216770&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="HD 216770 (página não existe)">HD 216770</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/Piscis_Austrinus" style="background: none; color: #0b0080; text-decoration: none;" title="Piscis Austrinus">Piscis Austrinus</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Ascensão reta</a></b></td><td align="left">22<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 55<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 53.7097<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></b></td><td align="left">–26° 39′ 31.547″</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Dist%C3%A2ncia" style="background: none; color: #0b0080; text-decoration: none;" title="Distância">Distância</a></b></td><td align="left">123.5 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (37.89 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</td></tr>
<tr><td align="left" colspan="2"><b><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Tipo_espectral" style="background: none; color: #0b0080; text-decoration: none;" title="Tipo espectral">Tipo espectral</a></b></td><td align="left">K1V</td></tr>
<tr><th colspan="3" style="background-color: #a0b0ff;"><a href="http://pt.wikipedia.org/wiki/Elementos_orbitais" style="background: none; color: #0b0080; text-decoration: none;" title="Elementos orbitais">Elementos orbitais</a></th></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Semieixo_maior" style="background: none; color: #0b0080; text-decoration: none;" title="Semieixo maior">Semieixo maior</a></b></td><td align="left">0.46 <a href="http://pt.wikipedia.org/wiki/Unidade_astron%C3%B4mica" style="background: none; color: #0b0080; text-decoration: none;" title="Unidade astronômica">UA</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Periastro" style="background: none; color: #0b0080; text-decoration: none;" title="Periastro">Periastro</a></b></td><td align="left">0.29 <a href="http://pt.wikipedia.org/wiki/Unidade_astron%C3%B4mica" style="background: none; color: #0b0080; text-decoration: none;" title="Unidade astronômica">UA</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Apoastro" style="background: none; color: #0b0080; text-decoration: none;" title="Apoastro">Apoastro</a></b></td><td align="left">0.63 <a href="http://pt.wikipedia.org/wiki/Unidade_astron%C3%B4mica" style="background: none; color: #0b0080; text-decoration: none;" title="Unidade astronômica">UA</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Excentricidade_orbital" style="background: none; color: #0b0080; text-decoration: none;" title="Excentricidade orbital">Excentricidade</a></b></td><td align="left">0.37 ± 0.06</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Per%C3%ADodo_orbital" style="background: none; color: #0b0080; text-decoration: none;" title="Período orbital">Período orbital</a></b></td><td align="left">118.45 ± 0.55 <a href="http://pt.wikipedia.org/wiki/Dia" style="background: none; color: #0b0080; text-decoration: none;" title="Dia">dias</a> (0.32429<a href="http://pt.wikipedia.org/wiki/Ano" style="background: none; color: #0b0080; text-decoration: none;" title="Ano">anos</a>)</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Velocidade_orbital" style="background: none; color: #0b0080; text-decoration: none;" title="Velocidade orbital">Velocidade orbital</a></b></td><td align="left">42 <a href="http://pt.wikipedia.org/wiki/Quil%C3%B4metro_por_segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Quilômetro por segundo">km/s</a></td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Argumento_do_periastro" style="background: none; color: #0b0080; text-decoration: none;" title="Argumento do periastro">Argumento do periastro</a></b></td><td align="left">281 ± 10</td></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Amplitude" style="background: none; color: #0b0080; text-decoration: none;" title="Amplitude">Semi-amplitude</a></b></td><td align="left">30.9 ± 1.9 <a href="http://pt.wikipedia.org/wiki/Metro_por_segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Metro por segundo">m/s</a></td></tr>
<tr><th colspan="3" style="background-color: #a0b0ff;">Características físicas</th></tr>
<tr><td align="left" colspan="2"><b><a href="http://pt.wikipedia.org/wiki/Massa" style="background: none; color: #0b0080; text-decoration: none;" title="Massa">Massa</a></b></td><td align="left">>0.65 <a href="http://pt.wikipedia.org/wiki/Massa_de_J%C3%BApiter" style="background: none; color: #0b0080; text-decoration: none;" title="Massa de Júpiter"><i>M</i><span style="height: 0px; line-height: 1; position: relative; top: 0.5ex; vertical-align: baseline;">J</span></a></td></tr>
<tr><th colspan="3" style="background-color: #a0b0ff;">Descoberta</th></tr>
<tr><td align="left" colspan="2"><b>Data da descoberta</b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/30_de_junho" style="background: none; color: #0b0080; text-decoration: none;" title="30 de junho">30 de junho</a> de <a href="http://pt.wikipedia.org/wiki/2003" style="background: none; color: #0b0080; text-decoration: none;" title="2003">2003</a></td></tr>
<tr><td align="left" colspan="2"><b>Descobridores</b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/Michel_Mayor" style="background: none; color: #0b0080; text-decoration: none;" title="Michel Mayor">Mayor</a> <i>et al.</i></td></tr>
<tr><td align="left" colspan="2"><b>Método de detecção</b></td><td align="left"><a href="http://pt.wikipedia.org/wiki/Velocidade_radial" style="background: none; color: #0b0080; text-decoration: none;" title="Velocidade radial">Velocidade radial</a></td></tr>
<tr><td align="left" colspan="2"><b>Estado da descoberta</b></td><td align="left">Publicada</td></tr>
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<span style="font-size: 14px; line-height: 22.3999996185303px; text-align: start;"><span style="color: #252525; font-family: sans-serif;"><a href="http://pt.wikipedia.org/wiki/HD_216770_b">http://pt.wikipedia.org/wiki/HD_216770_b</a></span></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 7314</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral_barrada" style="background-image: none; text-decoration: none;" title="Galáxia espiral barrada">espiral barrada</a> (SBbc) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Piscis_Austrinus" style="background-image: none; text-decoration: none;" title="Piscis Austrinus">Piscis Austrinus</a>. Possui uma declinação de -26° 03' 01" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 22 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; text-decoration: none;" title="Hora">horas</a>, 35 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; text-decoration: none;" title="Minuto">minutos</a> e 45,9 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; text-decoration: none;" title="Segundo">segundos</a>.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A galáxia <b>NGC 7314</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/29_de_Julho" style="background-image: none; text-decoration: none;" title="29 de Julho">29 de Julho</a> de <a href="http://pt.wikipedia.org/wiki/1834" style="background-image: none; text-decoration: none;" title="1834">1834</a> por <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-image: none; text-decoration: none;" title="John Herschel">John Herschel</a>.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_7314">http://pt.wikipedia.org/wiki/NGC_7314</a></span></div>
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<span style="color: #073763;"><img alt="Ficheiro:NGC7314-HST-R814GB450.jpg" src="http://upload.wikimedia.org/wikipedia/commons/thumb/f/f8/NGC7314-HST-R814GB450.jpg/607px-NGC7314-HST-R814GB450.jpg" height="632" width="640" /></span></div>
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<a href="http://pt.wikipedia.org/wiki/Ficheiro:NGC7314-HST-R814GB450.jpg"><span style="color: #073763;">http://pt.wikipedia.org/wiki/Ficheiro:NGC7314-HST-R814GB450.jpg</span></a></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 156.140625px;"><span style="color: #073763;">Autor</span></td><td><a href="http://commons.wikimedia.org/wiki/User:Fabian_RRRR" style="background-image: none; text-decoration: none;" title="User:Fabian RRRR"><span style="color: #073763;">Fabian RRRR</span></a></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_perm" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 156.140625px;"><span style="color: #073763;">Permissão<br /><small>(<a href="http://commons.wikimedia.org/wiki/Commons:Reutiliza%C3%A7%C3%A3o_de_conte%C3%BAdo_fora_da_Wikimedia" style="background-image: none; text-decoration: none;" title="Commons:Reutilização de conteúdo fora da Wikimedia">Reutilizar este ficheiro</a>)</small></span></td><td><div style="line-height: 1.5em; margin-bottom: 0.5em; margin-top: 0.4em;">
<span style="color: #073763;">ACKNOWLEDGMENT FOR PUBLICATIONS</span></div>
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<span style="color: #073763;">All refereed publications based on data obtained from the HLA are requested to carry the following footnote:</span></div>
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<i><span style="color: #073763;">Based on observations made with the NASA/ESA Hubble Space Telescope, and obtained from the Hubble Legacy Archive, which is a collaboration between the Space Telescope Science Institute (STScI/NASA), the Space Telescope European Coordinating Facility (ST-ECF/ESA) and the Canadian Astronomy Data Centre (CADC/NRC/CSA)</span></i></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgNhUxNkHzdK4k4FdG6ZOo8BxFiWgH7Y7TzYEwhw911N7co99URz0qGITPgZjVOkZ-ckLxOqvIwH7ixQLSTPP5vl6SaLBnOhGgItOx873cOsre1ThRo9ouoyxreawk50JgKNvM90FIBaJiH/s1600/urania26+(1).jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><span style="color: #073763;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgNhUxNkHzdK4k4FdG6ZOo8BxFiWgH7Y7TzYEwhw911N7co99URz0qGITPgZjVOkZ-ckLxOqvIwH7ixQLSTPP5vl6SaLBnOhGgItOx873cOsre1ThRo9ouoyxreawk50JgKNvM90FIBaJiH/s640/urania26+(1).jpg" height="446" width="640" /></span></a></div>
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<a class="link1" href="http://www.ianridpath.com/atlases/urania/urania26.jpg" style="text-decoration: none;"><span class="text1244" style="font-weight: bold;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Card 26</span></span></a></div>
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<span class="text1745"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; text-decoration: none;"><a class="link1" href="http://www.ianridpath.com/atlases/urania/urania26.jpg" style="text-decoration: none;">Aquarius, Piscis Australis, and Ballon Aerostatique</a></span></span></div>
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<a href="http://www.ianridpath.com/atlases/urania/urania26.jpg"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.ianridpath.com/atlases/urania/urania26.jpg</span></a></div>
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<span style="background-color: #073763;"><span class="small" style="background-color: #eae7e7; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px; text-align: start;"></span><span class="small" style="background-color: #eae7e7; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.399999618530273px;"><br /></span></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b><o:p></o:p></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<b style="color: #660000; font-family: Arial, Helvetica, sans-serif; line-height: 16.8pt;">Janine Milward</b></div>
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<span lang="PT" style="background-color: white; color: #073763; font-family: Arial, sans-serif;">Da Terra ao Céu<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763;"><span lang="PT" style="font-family: Arial, sans-serif;"> e ao Infinito</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span lang="PT" style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Constelações, Estrelas e Objetos Celestes<o:p></o:p></span></span></div>
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<span lang="PT" style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">(sob o ponto de vista do Mundo Ocidental)<o:p></o:p></span></span></div>
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<span lang="PT" style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Suas histórias, seus mitos, seus significados e suas sintetizadas descrições<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="PT" style="font-family: Arial, sans-serif;">Reunião das Informações e Compilação,</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="PT" style="font-family: Arial, sans-serif;">Tradução para a língua portuguesa (em alguns momentos)</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="PT" style="font-family: Arial, sans-serif;">bem como Comentários Pessoais:</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><i><span lang="PT" style="font-family: Arial, sans-serif;">Janine Milward</span></i><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;">Visitando os Sites abaixo,</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;"> você conseguirá informações atualizadas e preciosas</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;">sobre os Objetos Celestiais de seu interesse:</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">NASA/IPAC</span><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"> EXTRAGALACTIC DATABASE –</span><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://ned.ipac.caltech.edu/"><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">http://ned.ipac.caltech.edu/</span></a><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://ned.ipac.caltech.edu/forms/byname.html"><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">http://ned.ipac.caltech.edu/forms/byname.html</span></a><span style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><em><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"> </span></i></span><em><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://www.nightskyatlas.com/index.jsp"><span lang="EN-US" style="font-family: Arial, sans-serif;">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">The</span><span class="apple-converted-space"><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"> </span></span><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">Internet STELLAR DATABASE</span><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://www.stellar-database.com/"><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;">http://www.stellar-database.com/</span></a><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<o:p></o:p></span></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-52303899243745063182013-08-20T08:08:00.000-07:002015-01-29T09:25:06.478-08:00PISCES, OS PEIXES<div align="center" class="MsoNormal" style="text-align: center;">
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px; text-align: start;">Meu Projeto</span></div>
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="font-size: large;">Da Terra ao Céu ....</span></span></a></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="font-size: large;">.....<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;">e ao Infinito </a></span></span></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><span style="font-size: large;">- As 88 Constelações</span></a></span></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;">http://daterraaoceueaoinfinito.blogspot.com.br/</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/enlarge/36551</span></div>
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<span style="color: #274e13;"><span style="font-family: Arial, Helvetica, sans-serif;"><strong>Title: </strong>Les Poissons (Pisces) </span><strong style="font-family: Arial, Helvetica, sans-serif;">Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1260" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; font-family: Arial, Helvetica, sans-serif; text-decoration: none;">John Flamsteed</a><span style="font-family: Arial, Helvetica, sans-serif;"> / </span><span style="font-family: Arial, Helvetica, sans-serif;"> </span><a href="https://www.raremaps.com/gallery/browse/creator_id/1454" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; font-family: Arial, Helvetica, sans-serif; text-decoration: none;">MJ Fortin</a></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/36551/Les_Poissons_Pisces/Flamsteed-Fortin.html</span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">PISCES, OS PEIXES</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Mito:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Enquanto estavam sentados às margens do Rio Eufrates, Vênus e seu filho, Cupido, viram Tifão, o inimigo dos Deuses, se aproximando. Ambos mergulharam no rio e foram salvos de se afogarem por dois peixes, que mais tarde foram colocados nos céus por Vênus, em agradecimento.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os babilônios, os assírios e os persas representavam este grupo de estrelas por dois peixes.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Para os egípcios, esse asterismo registrava a aproximação da primavera e da estação da pesca. No zodíaco de Denderah, está representado por dois grandes peixes ligados por uma faixa, em meio de um retângulo que simboliza a água. No tumulo de Ramsés VI é representado por um único peixe.<o:p></o:p></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhvgSiqPczh_QtdPo5Y0mdhnPlxeS0On02Hks_t3hUUQ9uB9n2uxf-Ic9bNKCWSrDbd6glOtxLEVPLaYer4Y3uZXQpL35VpqmXROX0tSiom1wnRq3Cfv-ENfrztlH-cICtdMKl-3GRZCHA/s1600/PEIXES.gif" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhvgSiqPczh_QtdPo5Y0mdhnPlxeS0On02Hks_t3hUUQ9uB9n2uxf-Ic9bNKCWSrDbd6glOtxLEVPLaYer4Y3uZXQpL35VpqmXROX0tSiom1wnRq3Cfv-ENfrztlH-cICtdMKl-3GRZCHA/s1600/PEIXES.gif" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Algumas Informações Interessantes acerca esta Constelação:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Embora não seja uma constelação que apresente estrelas proeminentes, Peixes faz parte das constelações zodiacais desde os tempos das mais antigas civilizações.<o:p></o:p></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjKOlL98ZBJsjD0VPMvH1J2M1WAGmZlJGCEuzMdosIoQ6PfxYUUetObWekqITnBlOt7rCyBHP9iogjXOaHlhMl2qQ9aIe87pLOTnTYHZxWQG3HDNYKzPR_W5slZd15_Pgx4AIdNMIWwwRY/s1600/dia+15,+com+ilustra%C3%A7%C3%B5es.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjKOlL98ZBJsjD0VPMvH1J2M1WAGmZlJGCEuzMdosIoQ6PfxYUUetObWekqITnBlOt7rCyBHP9iogjXOaHlhMl2qQ9aIe87pLOTnTYHZxWQG3HDNYKzPR_W5slZd15_Pgx4AIdNMIWwwRY/s1600/dia+15,+com+ilustra%C3%A7%C3%B5es.jpg" /></span></a></div>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> http://www.stellarium.org/pt/</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Devido à Precessão, o equinócio vernal situa-se em Peixes, na linha de sua estrela Omega Piscium.</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Segundo o astrônomo Ronaldo Rogério de Freitas Mourão, em sua 6<sup>a</sup>. edição do Atlas Celeste, página 163, podemos ler:</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><o:p> </o:p><b><i>Ponto Vernal.</i></b><i> Ponto da esfera celeste, situado na interseção da eclíptica com o equador, na qual o Sol, em seu movimento aparente anual, passa do hemisfério sul para o norte. O ponto vernal serve de origem para as ascensões retas e as longitudes celestes, intervindo desse modo nas definições de tempo. O ponto vernal é habitualmente designado como equinócio da primavera, equinócio vernal, primeiro ponto de Áries.</i></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Excerto da constelação dos Peixes - Mario Jaci Monteiro, Cartas Celestes, As Constelações</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b> Asterismo </b>nomeado de<b> Circlet, Pequeno Círculo</b>, composto pelas estrelas Gamma, Beta, Teta, Iota, 19, Lambda e Kappa Piscium<b><o:p></o:p></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Este Pequeno Círculo - um dos dois Peixes - marca a proximidade do Ponto Vernal, o cruzamento entre as Linhas do Equador celestial e da Eclíptica. Em lugares de céus escuros e transparentes, podemos sempre bem visualizar este Pequeno Círculo, realmente.</span></div>
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<span style="color: #274e13;"><b><span style="font-family: Arial, sans-serif; font-size: 12pt;">Este Asterismo é
muitíssimo interessante</span></b><span style="font-family: Arial, sans-serif; font-size: 12pt;"><o:p></o:p></span></span></div>
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<b><span style="font-family: Arial, sans-serif; font-size: 12pt;"><span style="color: #274e13;">porque,</span></span></b></div>
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<span style="color: #274e13;"><b><span style="font-family: Arial, sans-serif; font-size: 12pt;"> se o
observarmos através nossa visão a olho nu</span></b><span style="font-family: Arial, sans-serif; font-size: 12pt;"><o:p></o:p></span></span></div>
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<span style="color: #274e13;"><b><span style="font-family: Arial, sans-serif; font-size: 12pt;">- sempre em
momentos de ausência de Lua e em lugares de céus escuros e transparentes -,</span></b><span style="font-family: Arial, sans-serif; font-size: 12pt;"><o:p></o:p></span></span></div>
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<span style="color: #274e13;"><b><span style="font-family: Arial, sans-serif; font-size: 12pt;">conseguiremos
detectar um pequeno círculo de estrelas tímidas</span></b><span style="font-family: Arial, sans-serif; font-size: 12pt;"><o:p></o:p></span></span></div>
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<b><span style="font-family: Arial, sans-serif; font-size: 12pt;"><span style="color: #274e13;">e que se
diferenciam muitíssimo </span></span></b></div>
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<span style="color: #274e13;"><b><span style="font-family: Arial, sans-serif; font-size: 12pt;">do tom meio caótico de disposição em ziguezague</span></b><span style="font-family: Arial, sans-serif; font-size: 12pt;"><o:p></o:p></span></span></div>
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<span style="color: #274e13;"><span style="font-family: Arial, sans-serif; font-size: 12pt;"><b> das
estrelinhas</b> </span><b style="line-height: 16.8pt;"><span style="font-family: Arial, sans-serif; font-size: 12pt;">que compõem o Jarro
e a Água entornando pelo Aguadeiro...., </span></b></span></div>
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<span style="color: #274e13;"><b><span style="font-family: Arial, sans-serif; font-size: 12pt;">água que acaba
fazendo parte</span></b><span style="font-family: Arial, sans-serif; font-size: 12pt;"><o:p></o:p></span></span></div>
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<b><span style="font-family: Arial, sans-serif; font-size: 12pt;"><span style="color: #274e13;">dos mares dos
Peixes!</span></span></b><span style="color: #073763; font-family: "Arial","sans-serif"; font-size: 12.0pt; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Fronteiras:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A constelação de Pisces faz fronteira com Áries, Triangulum, Andrômeda, Pegasus, Aquário e Cetus.<o:p></o:p></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">Algumas Estrelas e alguns objetos interessantes, </span></b></span><br />
<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">em Peixes:</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Asterismo nomeado de Circlet, Pequeno Círculo, composto pelas estrelas Gamma, Beta, Teta, Iota, 19, Lambda e Kappa Piscium<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT"><b>Al Rischa</b></span><span lang="PT"><b> - Alpha Piscium - Estrela Dupla</b><o:p></o:p></span></span></div>
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<span lang="PT" style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 01h69m Declinação +02º.31<o:p></o:p></span></span></div>
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<span lang="PT" style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual 4,3 e 5,2 Ângulo de Posição 281<sup>o</sup>.,2 Distância entre estrelas 1”,73<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A Medula Espinhal, nome de origem árabe.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="ES-TRAD"><b>Al Pherg</b></span><span lang="ES-TRAD"><b>. Eta Piscium</b>.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="ES-TRAD">Magnitude 3.9</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela dupla na corda próxima à cauda do Peixe ao norte. Esta estrela é associada com a Cabeça do Tifão, dos gregos.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Zeta Piscium - Estrela Dupla</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 01h11m Declinação +07<sup>o</sup>.19 Magnitude 5,6 e 6,5<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ângulo de Posição 63<sup>o</sup>.,5 Distância entre estrelas 23”,54<o:p></o:p></span></div>
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<span lang="ES-TRAD" style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Sigma Piscium - Estrela de Van Maanen</b><o:p></o:p></span></span></div>
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<span lang="PT" style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta é uma anã branca descoberta em 1917 por A. van Maanen, distante apenas 13.8 anos-luz. É uma das menores estrelas conhecidas, com um diâmetro calculado em cerca de 12.500 km - o que é bem próximo ao diâmetro da Terra. No entanto, a massa dessa estrela é comparável ao de nosso Sol.<o:p></o:p></span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiINXwVt4JLXBOKO6yTEJ5hQFsUabvYchSl1jDyP4wSZxQxvDUR3JWHiUPc_hq0cTQgj27Pa_kVFrdhwBdB7Icxhxf5MkETBhI840Z7LLT-7vMgojAqBHJgueTeB4e2ydWwzVwNTW0vQOYd/s1600/PSC.gif" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiINXwVt4JLXBOKO6yTEJ5hQFsUabvYchSl1jDyP4wSZxQxvDUR3JWHiUPc_hq0cTQgj27Pa_kVFrdhwBdB7Icxhxf5MkETBhI840Z7LLT-7vMgojAqBHJgueTeB4e2ydWwzVwNTW0vQOYd/s1600/PSC.gif" /></a></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">NGC 628 = M74 - Galáxia Espiral</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Galáxia bem grande porém de magnitude 11.0, situada bem próxima à estrela Eta Piscium<o:p></o:p></span></div>
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<span style="background-color: white;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>Messier 74</b> (também conhecida como <b>NGC 628</b>) é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-image: none; color: #274e13; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a> na constelação de <a href="http://pt.wikipedia.org/wiki/Pisces" style="background-image: none; color: #274e13; text-decoration: none;" title="Pisces">Pisces</a>.<span class="reference" id="cite_ref-seds_1-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-seds-1" style="background-image: none; color: #274e13; text-decoration: none;">1</a></span> Foi descoberta em setembro de <a href="http://pt.wikipedia.org/wiki/1780" style="background-image: none; color: #274e13; text-decoration: none;" title="1780">1780</a> por <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-image: none; color: #274e13; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a>. Ele reportou sua descoberta a <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-image: none; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a>, que listou a galáxia em seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-image: none; color: #274e13; text-decoration: none;" title="Catálogo Messier">catálogo</a>.<span class="reference" id="cite_ref-seds_1-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-seds-1" style="background-image: none; color: #274e13; text-decoration: none;">1</a></span></span></span></div>
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<span style="background-color: white;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">M74 possui dois braços espirais bem definidos e é usada como protótipo de uma <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Gal%C3%A1xia_espiral_de_grande_desenho&action=edit&redlink=1" style="background-image: none; color: #274e13; text-decoration: none;" title="Galáxia espiral de grande desenho (página não existe)">galáxia espiral de grande desenho</a>.<span class="reference" id="cite_ref-seds_1-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-seds-1" style="background-image: none; color: #274e13; text-decoration: none;">1</a></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13; line-height: 19.200000762939453px;">http://pt.wikipedia.org/wiki/Messier_74</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEi3jxjP84-s6xkzNLXqztsYQGp6vz6cgG5z6X6bGVzcyT2amwELd2FB2pjiq1tKU3YBe0T1B6EvPuLavYFlFpzakVGYIoQEDNlWZaT6qXzcQgByp_ZZD6TEPJ71ZggUo1_lCtSQZukO-o4/s1600/Messier_74_by_HST.jpg" imageanchor="1" style="background-color: white; color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEi3jxjP84-s6xkzNLXqztsYQGp6vz6cgG5z6X6bGVzcyT2amwELd2FB2pjiq1tKU3YBe0T1B6EvPuLavYFlFpzakVGYIoQEDNlWZaT6qXzcQgByp_ZZD6TEPJ71ZggUo1_lCtSQZukO-o4/s1600/Messier_74_by_HST.jpg" height="616" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Origem</span></span></td><td><a class="external free" href="http://hubblesite.org/newscenter/archive/releases/galaxy/spiral/2007/41/image/a/" rel="nofollow" style="background-color: white; color: #274e13; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/galaxy/spiral/2007/41/image/a/</span></a></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Autor</span></span></td><td><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: R. Chandar (University of Toledo) and J. Miller (University of Michigan)</span></span></td></tr>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">NGC 520 - Galáxia</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta é uma galáxia de um formato pouco usual - e que deve estar ainda ejetando matéria. Magnitude 12.4. situa-se abaixo da estrela Upsilon Piscium e já bem próxima à fronteira com Cetus, a Baleia.<o:p></o:p></span></div>
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<span style="background-color: white;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>NGC 520</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_irregular" style="background-image: none; color: #274e13; text-decoration: none;" title="Galáxia irregular">galáxia irregular</a> localizada a cerca de cem milhões de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; color: #274e13; text-decoration: none;" title="Anos-luz">anos-luz</a> (aproximadamente 30,65 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Megaparsec" style="background-image: none; color: #274e13; text-decoration: none;" title="Megaparsec">megaparsecs</a>) de distância na direção da <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o_de_Peixes" style="background-image: none; color: #274e13; text-decoration: none;" title="Constelação de Peixes">constelação de Peixes</a>. Possui uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; color: #274e13; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 11,3, uma declinação de +03º 47' 42" e uma <a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-image: none; color: #274e13; text-decoration: none;" title="Ascensão reta">ascensão reta</a> de 01 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; color: #274e13; text-decoration: none;" title="Hora">horas</a>, 24 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; color: #274e13; text-decoration: none;" title="Minuto">minutos</a> e 34,3 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; color: #274e13; text-decoration: none;" title="Segundo">segundos</a>.</span></span></div>
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<span style="background-color: white;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Acredita-se que a estranha forma adquirida por esta galáxia seja o resultado de uma colisão ocorrida entre duas <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-image: none; color: #274e13; text-decoration: none;" title="Galáxia espiral">galáxias espirais</a> há cerca de trezentos milhões de <a href="http://pt.wikipedia.org/wiki/Ano" style="background-image: none; color: #274e13; text-decoration: none;" title="Ano">anos</a>.</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13; line-height: 19.200000762939453px;">http://pt.wikipedia.org/wiki/NGC_520</span></span></div>
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<span style="background-color: white;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">NGC 520</span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> is the product of a collision between two disk galaxies that started 300 million years ago. It exemplifies the middle stages of the merging process: the disks of the parent galaxies have merged together, but the nuclei have not yet coalesced. It features an odd-looking tail of stars and a prominent dust lane that runs diagonally across the center of the image and obscures the galaxy. NGC 520 is one of the brightest galaxy pairs on the sky, and can be observed with a small telescope toward the constellation of Pisces, the Fish, having the appearance of a comet. It is about 100 million light-years away and about 100,000 light-years across. The galaxy pair is included in Arp's catalog of peculiar galaxies as Arp 157.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">This image is part of a large collection of 59 images of merging galaxies taken by the Hubble Space Telescope and released on the occasion of its 18th anniversary on 24th April 2008.</span></span></div>
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<tr style="vertical-align: top;"><td><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="external free" href="http://hubblesite.org/newscenter/archive/releases/2008/16/image/bo/" rel="nofollow" style="color: #274e13; text-decoration: none;">http://hubblesite.org/newscenter/archive/releases/2008/16/image/bo/</a> (<a class="external text" href="http://imgsrc.hubblesite.org/hu/db/2008/16/images/bo/formats/full_jpg.jpg" rel="nofollow" style="color: #274e13; text-decoration: none;">direct link</a>)</span></span></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Autor</span></span></td><td><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">NASA, ESA, the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration, and B. Whitmore (STScI)</span></span></td></tr>
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<b>NGC 7714</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral_barrada" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia espiral barrada">espiral barrada</a> (SBb/P) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Pisces" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pisces">Pisces</a>. Possui uma declinação de +02° 09' 17" e uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 23 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hora">horas</a>, 36 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto">minutos</a> e 14,1 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a>.</div>
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A galáxia <b>NGC 7714</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/18_de_Setembro" style="background: none; color: #0b0080; text-decoration: none;" title="18 de Setembro">18 de Setembro</a> de <a href="http://pt.wikipedia.org/wiki/1830" style="background: none; color: #0b0080; text-decoration: none;" title="1830">1830</a> por <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background: none; color: #0b0080; text-decoration: none;" title="John Herschel">John Herschel</a>.</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/NGC_7714</span></span></div>
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This NASA Hubble Space Telescope photo of NGC 7714 presents an especially striking view of the galaxy's smoke-ring-like structure. The golden loop is made of Sun-like stars that have been pulled deep into space, far from the galaxy's center. The galaxy is located approximately 100 million light-years from Earth in the direction of the constellation Pisces.</div>
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The universe is full of such galaxies that are gravitationally stretched and pulled and otherwise distorted in gravitational tug-o'-wars with bypassing galaxies.</div>
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The companion galaxy doing the "taffy pulling" in this case, NGC 7715, lies just out of the field of view in this image. A very faint bridge of stars extends to the unseen companion. The close encounter has compressed interstellar gas to trigger bursts of star formation seen in bright blue arcs extending around NGC 7714's center.</div>
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The gravitational disruption of NGC 7714 began between 100 million and 200 million years ago, at the epoch when dinosaurs ruled the Earth.</div>
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The image was taken with the Wide Field Camera 3 and the Advanced Camera for Surveys in October 2011.</div>
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<span style="font-family: arial, sans-serif;"><span style="font-size: 13px; line-height: 18.2000007629395px;">http://hubblesite.org/newscenter/archive/releases/2015/04/image/a/</span></span></div>
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<span lang="PT" style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000; font-size: medium;">Superaglomerado Perseus-Pisces</span></b></span></span></div>
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<span lang="PT" style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000; font-size: medium;">Complexo de Superaglomerados Pisces-Cetus</span></b></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;"><span style="line-height: 19.200000762939453px; text-align: start;">O </span><span style="line-height: 19.200000762939453px; text-align: start;">superaglomerado Perseus-Pisces</span><span style="line-height: 19.200000762939453px; text-align: start;"> (</span><span style="line-height: 19.200000762939453px; text-align: start;">SCl 40</span></span></b><span style="line-height: 19.200000762939453px; text-align: start;"><b><span style="color: #660000;">) </span></b></span></span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 19.200000762939453px; text-align: start;">é um </span><a href="http://pt.wikipedia.org/wiki/Superaglomerado_de_gal%C3%A1xias" style="background-image: none; color: #274e13; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Superaglomerado de galáxias">superaglomerado</a><span style="line-height: 19.200000762939453px; text-align: start;"> próximo distante a 70 </span><a href="http://pt.wikipedia.org/wiki/Parsec" style="background-image: none; color: #274e13; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Parsec">Mpc</a><span style="line-height: 19.200000762939453px; text-align: start;"> da </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background-image: none; color: #274e13; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Superaglomerado_Perseus-Pisces#cite_note-1" style="background-image: none; color: #274e13; text-decoration: none;">1</a></span><span style="line-height: 19.200000762939453px; text-align: start;"> e é uma das maiores estruturas conhecidas do </span><a href="http://pt.wikipedia.org/wiki/Universo" style="background-image: none; color: #274e13; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Universo">universo</a><span style="line-height: 19.200000762939453px; text-align: start;">. Os principais aglomerados são </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Abell_262&action=edit&redlink=1" style="background-image: none; color: #274e13; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Abell 262 (página não existe)">Abell 262</a><span style="line-height: 19.200000762939453px; text-align: start;">, </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Abell_347&action=edit&redlink=1" style="background-image: none; color: #274e13; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Abell 347 (página não existe)">Abell 347</a><span style="line-height: 19.200000762939453px; text-align: start;"> e </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Abell_426&action=edit&redlink=1" style="background-image: none; color: #274e13; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Abell 426 (página não existe)">Abell 426</a><span class="reference" id="cite_ref-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Superaglomerado_Perseus-Pisces#cite_note-2" style="background-image: none; color: #274e13; text-decoration: none;">2</a></span><span style="line-height: 19.200000762939453px; text-align: start;"> .</span></span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Superaglomerado_Perseus-Pisces</span></div>
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<span style="background-color: white; line-height: 15.834113121032715px; text-align: left;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">O superaglomerado Perseus-Pisces, num contexto maior, abrangendo outros superaglomerados situados a 500 milhões de anos-luz da Terra.</span></span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 15.834113121032715px; text-align: left;">Mapa dos </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Superaglomerado" style="background-image: none; color: #274e13; line-height: 15.834113121032715px; margin-left: auto; margin-right: auto; text-align: left; text-decoration: none;" title="Superaglomerado">superaglomerados</a><span style="line-height: 15.834113121032715px; text-align: left;"> mais próximos de nosso </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Superaglomerado_de_Virgem" style="background-image: none; color: #274e13; line-height: 15.834113121032715px; margin-left: auto; margin-right: auto; text-align: left; text-decoration: none;" title="Superaglomerado de Virgem">superaglomerado de Virgem</a><span style="line-height: 15.834113121032715px; text-align: left;">, do qual se pode inferir a dimensão do </span><i style="line-height: 15.834113121032715px; margin-left: auto; margin-right: auto; text-align: left;">complexo de aglomerados Peixes-Baleia</i><span style="line-height: 15.834113121032715px; text-align: left;"> conforme as informações fornecidas pelo artigo.</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj5w9NJWnXdgT8vgncctM8QIqznrXUEYy8RSI50e50VXgCrib3kvfaufbI6Mp4jlzQU3V0NbWpRfBAn4LPFeK_eByBCDz7AuKnDXFT0cAFoybibqFby3FSnn2UfWVjK-lWNR3uYgZTnDBI/s1600/Superaglomerados_pr%C3%B3ximos.gif" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj5w9NJWnXdgT8vgncctM8QIqznrXUEYy8RSI50e50VXgCrib3kvfaufbI6Mp4jlzQU3V0NbWpRfBAn4LPFeK_eByBCDz7AuKnDXFT0cAFoybibqFby3FSnn2UfWVjK-lWNR3uYgZTnDBI/s1600/Superaglomerados_pr%C3%B3ximos.gif" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://upload.wikimedia.org/wikipedia/commons/a/ab/Superaglomerados_pr%C3%B3ximos.gif</span></div>
<table cellpadding="4" class="toccolours vevent mw-content-ltr" style="border: 1px solid rgb(170, 170, 170); direction: ltr; line-height: 19.200000762939453px; padding: 5px; width: 1348px;"><tbody>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_desc" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">Description</span></td><td class="description"><div style="line-height: 1.5em; margin-bottom: 0.5em; margin-top: 0.4em;">
<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">Map of voids and superclusters within 500 million light years from Milky May</span></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_date" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">Date</span></td><td><span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">08/11/09</span></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">Source</span></td><td><a class="external free" href="http://www.atlasoftheuniverse.com/nearsc.html" rel="nofollow" style="color: #274e13; text-decoration: none;"><span style="background-color: white; font-family: Arial, Helvetica, sans-serif;">http://www.atlasoftheuniverse.com/nearsc.html</span></a></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">Author</span></td><td><span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">Richard Powell</span></td></tr>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">The Perseus-Pisces Supercluster</span></h1>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">The Perseus-Pisces supercluster is the most obvious supercluster in the sky. Although, like all superclusters, it is much too faint to be seen with the naked eye, this plot of bright galaxies in this region of the sky (from the Principal Galaxies Catalogue) shows how prominant it is. The Perseus-Pisces supercluster is a long, dense wall of galaxies with a length of almost 300 million light years. At the left end of the supercluster lies the massive <em>Perseus cluster</em> (A426), one of the most massive clusters of galaxies within 500 million light years.</span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;"><img alt="The Perseus-Pisces Supercluster" src="http://www.atlasoftheuniverse.com/superc/perpsc.gif" height="480" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="760" /></span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://www.atlasoftheuniverse.com/superc/perpsc.html</span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span style="text-align: start;">This website belongs to </span><a href="http://www.atlasoftheuniverse.com/me.html" style="color: #274e13; text-align: start; text-decoration: none;">Richard Powell</a><span style="text-align: start;">.</span></span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>COMPLEXO DE SUPERAGLOMERADOS DE PISCES-CETUS</b></span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">O <b>complexo de aglomerados de Peixes-Baleia</b> (alternativamente,<b> complexo de superaglomerados de Pisces-Cetus</b>) é um complexo de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Superaglomerado" style="background-image: none; color: #274e13; text-decoration: none;" title="Superaglomerado">superaglomerados</a> de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Gal%C3%A1xias" style="background-image: none; color: #274e13; text-decoration: none;" title="Galáxias">galáxias</a> ou <a href="http://pt.wikipedia.org/wiki/Filamento_gal%C3%A1ctico" style="background-image: none; color: #274e13; text-decoration: none;" title="Filamento galáctico">filamentos galácticos</a> que inclui o <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Superaglomerado_de_Virgem" style="background-image: none; color: #274e13; text-decoration: none;" title="Superaglomerado de Virgem">superaglomerado de Virgem</a> (que por sua vez inclui o <a href="http://pt.wikipedia.org/wiki/Grupo_Local" style="background-image: none; color: #274e13; text-decoration: none;" title="Grupo Local">Grupo Local</a>, o aglomerado galáctico em que a <a href="http://pt.wikipedia.org/wiki/Via_L%C3%A1ctea" style="background-image: none; color: #274e13; text-decoration: none;" title="Via Láctea">Via Láctea</a> está localizada).<span class="reference" id="cite_ref-tully86_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Complexo_de_superaglomerados_Peixes-Baleia#cite_note-tully86-1" style="background-image: none; color: #274e13; text-decoration: none;">1</a></span><span class="mw-headline" id="Descoberta">Descoberta</span><span class="mw-editsection mw-editsection-expanded" style="-webkit-user-select: none; direction: ltr; display: inline-block; line-height: 1em; margin-left: 1em; padding-right: 0.25em; unicode-bidi: -webkit-isolate; vertical-align: baseline; white-space: nowrap;"><span class="mw-editsection-bracket" style="margin-left: -0.25em; margin-right: 0.25em;">[</span><a class="mw-editsection-visualeditor" href="http://pt.wikipedia.org/w/index.php?title=Complexo_de_superaglomerados_Peixes-Baleia&veaction=edit&section=1" style="background-image: none; color: #274e13; text-decoration: none;" title="Editar secção: Descoberta">editar</a><span class="mw-editsection-divider"> | </span><a href="http://pt.wikipedia.org/w/index.php?title=Complexo_de_superaglomerados_Peixes-Baleia&action=edit&section=1" style="background-image: none; color: #274e13; text-decoration: none;" title="Editar secção: Descoberta">editar código-fonte</a><span class="mw-editsection-bracket" style="margin-left: 0.25em; margin-right: -0.25em;">]</span></span></span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">O <a href="http://pt.wikipedia.org/wiki/Astr%C3%B4nomo" style="background-image: none; color: #274e13; text-decoration: none;" title="Astrônomo">astrônomo</a> <a class="new" href="http://pt.wikipedia.org/w/index.php?title=R._Brent_Tully&action=edit&redlink=1" style="background-image: none; color: #274e13; text-decoration: none;" title="R. Brent Tully (página não existe)">R. Brent Tully</a>, do Instituto de Astronomia da <a href="http://pt.wikipedia.org/wiki/Universidade_do_Hava%C3%AD" style="background-image: none; color: #274e13; text-decoration: none;" title="Universidade do Havaí">Universidade do Havaí</a> identificou o complexo em 1987.<span class="reference" id="cite_ref-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Complexo_de_superaglomerados_Peixes-Baleia#cite_note-2" style="background-image: none; color: #274e13; text-decoration: none;">2</a></span></span></div>
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<span class="mw-headline" id="Dimens.C3.A3o" style="background-color: white;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Dimensão</span></span></h2>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">Estima-se que o complexo de superaglomerados Peixes-Baleia se estenda por 1.0 bilhão de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; color: #274e13; text-decoration: none;" title="Anos-luz">anos-luz</a> e possua uma largura de 150 milhões de anos-luz. Este complexo é uma das maiores estruturas já identificadas no <a href="http://pt.wikipedia.org/wiki/Universo" style="background-image: none; color: #274e13; text-decoration: none;" title="Universo">universo</a>, sendo superado apenas pela <a href="http://pt.wikipedia.org/wiki/Grande_Muralha_Sloan" style="background-image: none; color: #274e13; text-decoration: none;" title="Grande Muralha Sloan">Grande Muralha Sloan</a>, que se estende por 1,37 bilhão de anos-luz.</span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">O complexo abrange aproximadamente 60 aglomerados e possui uma massa estimada de 10<span class="exposant" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">18</span> <a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background-image: none; color: #274e13; text-decoration: none;" title="Massa solar">M<span style="height: 0px; line-height: 1; position: relative; top: 0.5ex; vertical-align: baseline;">☉</span></a>.<span class="reference" id="cite_ref-tully87_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Complexo_de_superaglomerados_Peixes-Baleia#cite_note-tully87-3" style="background-image: none; color: #274e13; text-decoration: none;">3</a></span> De acordo com o descobridor, este complexo é composto por 5 partes:</span></div>
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<li style="margin: 0px 0px 0.1em; padding: 0px;"><span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">O <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Superaglomerado_Peixes-Baleia&action=edit&redlink=1" style="background-image: none; color: #274e13; text-decoration: none;" title="Superaglomerado Peixes-Baleia (página não existe)">superaglomerado Peixes-Baleia</a></span></li>
<li style="margin: 0px 0px 0.1em; padding: 0px;"><span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">A <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Cadeia_Perseu-P%C3%A9gaso&action=edit&redlink=1" style="background-image: none; color: #274e13; text-decoration: none;" title="Cadeia Perseu-Pégaso (página não existe)">cadeia Perseu-Pégaso</a>, incluindo o <a href="http://pt.wikipedia.org/wiki/Superaglomerado_Perseus-Pisces" style="background-image: none; color: #274e13; text-decoration: none;" title="Superaglomerado Perseus-Pisces">superaglomerado Perseu-Peixes</a></span></li>
<li style="margin: 0px 0px 0.1em; padding: 0px;"><span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">A <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Cadeia_P%C3%A9gaso-Peixes&action=edit&redlink=1" style="background-image: none; color: #274e13; text-decoration: none;" title="Cadeia Pégaso-Peixes (página não existe)">cadeia Pégaso-Peixes</a></span></li>
<li style="margin: 0px 0px 0.1em; padding: 0px;"><span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">A <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Regi%C3%A3o_do_Escultor&action=edit&redlink=1" style="background-image: none; color: #274e13; text-decoration: none;" title="Região do Escultor (página não existe)">região do Escultor</a>, incluindo o <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Superaglomerado_de_Escultor&action=edit&redlink=1" style="background-image: none; color: #274e13; text-decoration: none;" title="Superaglomerado de Escultor (página não existe)">superaglomerado de Escultor</a> e o <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Superaglomerado_de_H%C3%A9rcules" style="background-image: none; color: #274e13; text-decoration: none;" title="Superaglomerado de Hércules">superaglomerado de Hércules</a></span></li>
<li style="margin: 0px 0px 0.1em; padding: 0px;"><span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">O <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Superaglomerado_Virgem-Hidra-Centauro&action=edit&redlink=1" style="background-image: none; color: #274e13; text-decoration: none;" title="Superaglomerado Virgem-Hidra-Centauro (página não existe)">superaglomerado Virgem-Hidra-Centauro</a>, que contém o <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Superaglomerado_de_Virgem" style="background-image: none; color: #274e13; text-decoration: none;" title="Superaglomerado de Virgem">superaglomerado de Virgem</a> (superaglomerado Local) e também o <a href="http://pt.wikipedia.org/wiki/Superaglomerado_Hidra-Centauro" style="background-image: none; color: #274e13; text-decoration: none;" title="Superaglomerado Hidra-Centauro">superaglomerado Hidra-Centauro</a><span class="reference" id="cite_ref-tully87_3-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Complexo_de_superaglomerados_Peixes-Baleia#cite_note-tully87-3" style="background-image: none; color: #274e13; text-decoration: none;">3</a></span> .</span></li>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">Com uma massa de 10<span class="exposant" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">15</span> <a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background-image: none; color: #274e13; text-decoration: none;" title="Massa solar">M<span style="height: 0px; line-height: 1; position: relative; top: 0.5ex; vertical-align: baseline;">☉</span></a>, o <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Superaglomerado_de_Virgem" style="background-image: none; color: #274e13; text-decoration: none;" title="Superaglomerado de Virgem">superaglomerado de Virgem</a> contribui com apenas 0.1 por cento da massa total do superaglomerado.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13; line-height: 19.200000762939453px;">http://pt.wikipedia.org/wiki/Complexo_de_superaglomerados_Peixes-Baleia</span></span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">The Nearest Superclusters</span></h1>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">This is a map of the universe within 500 million light years. It shows most of the major galaxy superclusters that surround the Virgo supercluster. These superclusters are not isolated in space but together with many other smaller concentrations of galaxies they form parts of extensive walls of galaxies surrounding large voids. Three of the biggest walls near us are marked on the map as well as several of the largest voids. There are several hundred thousand large galaxies within 500 million light years, so even on this scale our galaxy is a very insignificant object. </span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span style="text-align: start;">This website belongs to </span><a href="http://www.atlasoftheuniverse.com/me.html" style="color: #274e13; text-align: start; text-decoration: none;">Richard Powell</a><span style="text-align: start;">.</span></span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra..., bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.<o:p></o:p></span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></b></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>VISITE MINHA PÁGINA</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>DA TERRA AO CÉU E AO INFINITO</b><o:p></o:p></span></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">http://daterraaoceueaoinfinito.blogspot.com.br/</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do <b>Atlas Celeste</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de<b> Ronaldo Rogério de Freitas Mourão</b> </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- <span style="line-height: 13.5pt;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(com dedicatória do próprio autor para mim <span style="line-height: 13.5pt;">em evento realizado no Museu de Astronomia do Rio de Janeiro, </span></span><span style="font-family: Arial, Helvetica, sans-serif; line-height: 13.5pt;">em 16/06/1989)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="PT">- </span><b>Mario Jaci Monteiro</b> , <b>As Constelações, Cartas Celestes</b> -<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC - com dedicatória do autor para mim, em março de 2004 (quando Mário Jaci generosamente me presenteou com um instrumento de observação (kepleriano) artesanalmente construído por ele).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, sans-serif;">Alguns dados<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, sans-serif;">(tais como Ascensão Reta e Declinação, em muitos dos casos)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, sans-serif;">são época/equinócio 1980<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, sans-serif;">e devem requerer do Caminhante do Céu<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;">Visitando os Sites abaixo,</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;"> você conseguirá informações atualizadas e preciosas</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;">sobre os Objetos Celestiais de seu interesse:</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, sans-serif;">NASA/IPAC</span><span style="font-family: Arial, sans-serif;"> EXTRAGALACTIC DATABASE –</span><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://ned.ipac.caltech.edu/"><span style="font-family: Arial, sans-serif;">http://ned.ipac.caltech.edu/</span></a><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://ned.ipac.caltech.edu/forms/byname.html"><span style="font-family: Arial, sans-serif;">http://ned.ipac.caltech.edu/forms/byname.html</span></a><span style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><em><span lang="EN-US" style="font-family: Arial, sans-serif;">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US" style="font-family: Arial, sans-serif;"> </span></i></span><em><span lang="EN-US" style="font-family: Arial, sans-serif;"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US" style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://www.nightskyatlas.com/index.jsp"><span lang="EN-US" style="font-family: Arial, sans-serif;">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US" style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763;"><span lang="EN-US" style="font-family: Arial, sans-serif;">The</span><span class="apple-converted-space"><span lang="EN-US" style="font-family: Arial, sans-serif;"> </span></span><span lang="EN-US" style="font-family: Arial, sans-serif;">Internet STELLAR DATABASE</span><span lang="EN-US" style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://www.stellar-database.com/"><span lang="EN-US" style="font-family: Arial, sans-serif;">http://www.stellar-database.com/</span></a><span lang="EN-US" style="font-family: Arial, sans-serif;"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<o:p></o:p></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-14102625285097886552013-08-20T08:02:00.003-07:002016-11-23T10:01:42.987-08:00PHOENIX, A FÊNIX<div align="center" class="MsoNormal" style="text-align: center;">
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<span style="font-family: "arial" , "helvetica" , sans-serif; font-size: large; line-height: 18px;"><b>Meu Projeto</b></span></div>
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; font-size: large;">Da Terra ao Céu ....</span></a></h1>
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<span style="font-family: "arial" , "helvetica" , sans-serif; font-size: large;">.....<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;">e ao Infinito </a></span></h1>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><span style="font-size: large;">- As 88 Constelações</span></a></span></h1>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;">http://daterraaoceueaoinfinito.blogspot.com.br/</a><o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><br /></span><span style="font-family: "arial" , "helvetica" , sans-serif;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><br /></span><span style="font-family: "arial" , "helvetica" , sans-serif;">Com um abraço estrelado,</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Janine Milward</span></div>
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<span style="font-family: "arial" , sans-serif;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgwH2Y8x6GQWdHKXwx7EiYefZwWuk2itNZcUy03fKTqS73hyphenhyphenbjSMB72-D4eU13k5BoSeTUxsBvoX2ygoCNsw6_plaj3bioAcFQnQA9da5NiXUqnoY_YG-w8NIFCBRZ-n54jpkFDiav372o/s1600/33613+(1).jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgwH2Y8x6GQWdHKXwx7EiYefZwWuk2itNZcUy03fKTqS73hyphenhyphenbjSMB72-D4eU13k5BoSeTUxsBvoX2ygoCNsw6_plaj3bioAcFQnQA9da5NiXUqnoY_YG-w8NIFCBRZ-n54jpkFDiav372o/s1600/33613+(1).jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; cursor: move; padding: 8px; position: relative;" /></a></span></div>
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<span style="font-family: "arial" , sans-serif;">http://www.raremaps.com/gallery/enlarge/33613</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">http://www.raremaps.com/gallery/detail/33613/Celestial_Map_of_the_Southern_Hemisphere/Pardies.html</span></div>
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<strong>Title: </strong>[Celestial Map of the Southern Hemisphere] <strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/3418" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; text-decoration: none;">Ignace Gaston Pardies</a></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white;"><b>Pássaros do Sul</b></span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white;"><b>Tucano, Grou, Pavão</b></span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white;"><b>e</b></span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white;"><b>Fênix....</b></span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white;"><b>e não podemos nos esquecer de Apus, a ave-do-paraíso!?</b></span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white;"><b>e a Pomba de Noé?! </b></span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white;"><b>...........................</b></span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white;"><b> E o Peixe Voador?!</b></span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white;"><b>Pássaros reais e Pássaros Míticos.</b></span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white; font-family: "arial" , "helvetica" , sans-serif; font-size: large;"><span style="background-color: #f9f9f9; color: #252525; font-family: sans-serif;">The "Southern Birds", </span><a class="extiw" href="https://en.wikipedia.org/wiki/Pavo_(constellation)" style="background: none rgb(249, 249, 249); color: #663366; font-family: sans-serif; text-decoration: none;" title="en:Pavo (constellation)">Pavo</a><span style="background-color: #f9f9f9; color: #252525; font-family: sans-serif;">, </span><a class="extiw" href="https://en.wikipedia.org/wiki/Phoenix_(constellation)" style="background: none rgb(249, 249, 249); color: #663366; font-family: sans-serif; text-decoration: none;" title="en:Phoenix (constellation)">Phoenix</a><span style="background-color: #f9f9f9; color: #252525; font-family: sans-serif;">, </span><a class="extiw" href="https://en.wikipedia.org/wiki/Grus_(constellation)" style="background: none rgb(249, 249, 249); color: #663366; font-family: sans-serif; text-decoration: none;" title="en:Grus (constellation)">Grus</a><span style="background-color: #f9f9f9; color: #252525; font-family: sans-serif;">, and </span><a class="extiw" href="https://en.wikipedia.org/wiki/Tucana_(constellation)" style="background: none rgb(249, 249, 249); color: #663366; font-family: sans-serif; text-decoration: none;" title="en:Tucana (constellation)">Tucana</a><span style="background-color: #f9f9f9; color: #252525; font-family: sans-serif;"> from </span><a class="extiw" href="https://en.wikipedia.org/wiki/Johann_Bayer" style="background: none rgb(249, 249, 249); color: #663366; font-family: sans-serif;" title="en:Johann Bayer">Johann Bayer</a><span style="background-color: #f9f9f9; color: #252525; font-family: sans-serif;">'s </span><i style="background-color: #f9f9f9; color: #252525; font-family: sans-serif;"><a class="extiw" href="https://en.wikipedia.org/wiki/Uranometria" style="background: none; color: #663366; text-decoration: none;" title="en:Uranometria">Uranometria</a></i><span style="background-color: #f9f9f9; color: #252525; font-family: sans-serif;"> of 1603, the first celestial atlas to include the southern constellations. </span><a class="extiw" href="https://en.wikipedia.org/wiki/Indus_(constellation)" style="background: none rgb(249, 249, 249); color: #663366; font-family: sans-serif; text-decoration: none;" title="en:Indus (constellation)">Indus</a><span style="background-color: #f9f9f9; color: #252525; font-family: sans-serif;"> and </span><a class="extiw" href="https://en.wikipedia.org/wiki/Hydrus_(constellation)" style="background: none rgb(249, 249, 249); color: #663366; font-family: sans-serif; text-decoration: none;" title="en:Hydrus (constellation)">Hydrus</a><span style="background-color: #f9f9f9; color: #252525; font-family: sans-serif;"> also appear.</span></span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white; font-family: "arial" , "helvetica" , sans-serif;"><img alt="Resultado de imagem para Johann Bayer" src="https://upload.wikimedia.org/wikipedia/commons/thumb/b/b5/Johann_Bayer_-_Uraniometria_-_Southern_Birds.jpg/838px-Johann_Bayer_-_Uraniometria_-_Southern_Birds.jpg" /></span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white; font-family: "arial" , "helvetica" , sans-serif;">https://upload.wikimedia.org/wikipedia/commons/thumb/b/b5/<b><span style="font-size: large;">Johann_Bayer_-_Uraniometria_-_Southern_Birds.</span></b>jpg/838px-Johann_Bayer_-_Uraniometria_-_Southern_Birds.jpg</span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white; font-family: "arial" , "helvetica" , sans-serif;">Caro Leitor,</span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white; font-family: "arial" , "helvetica" , sans-serif;">É interessante percebermos o fato de que</span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white; font-family: "arial" , "helvetica" , sans-serif;">muitas das constelações mais ao sul</span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white; font-family: "arial" , "helvetica" , sans-serif;">foram figuradas e nomeadas </span></span><br />
<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white; font-family: "arial" , "helvetica" , sans-serif;">nos Séculos XVI (bem ao final), XVII e XVIII.</span></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Petrus Plancius</b></span><br />
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<b style="background-color: white; color: #252525; font-family: sans-serif;">Petrus Plancius</b><span style="background-color: white; color: #252525; font-family: sans-serif;"> (1552 – May 15, 1622) was a </span><a href="https://en.wikipedia.org/wiki/Flanders" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; text-decoration: none;" title="Flanders">Flemish</a><span style="background-color: white; color: #252525; font-family: sans-serif;"> </span><a href="https://en.wikipedia.org/wiki/Astronomer" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; text-decoration: none;" title="Astronomer">astronomer</a><span style="background-color: white; color: #252525; font-family: sans-serif;">, </span><a href="https://en.wikipedia.org/wiki/Cartography" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; text-decoration: none;" title="Cartography">cartographer</a><span style="background-color: white; color: #252525; font-family: sans-serif;"> and </span><a class="mw-redirect" href="https://en.wikipedia.org/wiki/Clergyman" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; text-decoration: none;" title="Clergyman">clergyman</a><span style="background-color: white; color: #252525; font-family: sans-serif;">. He was born as </span><b style="background-color: white; color: #252525; font-family: sans-serif;">Pieter Platevoet</b><span style="background-color: white; color: #252525; font-family: sans-serif;"> in </span><a href="https://en.wikipedia.org/wiki/Dranouter" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; text-decoration: none;" title="Dranouter">Dranouter</a><span style="background-color: white; color: #252525; font-family: sans-serif;">, now in </span><a href="https://en.wikipedia.org/wiki/Heuvelland" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; text-decoration: none;" title="Heuvelland">Heuvelland</a><span style="background-color: white; color: #252525; font-family: sans-serif;">, </span><a href="https://en.wikipedia.org/wiki/West_Flanders" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; text-decoration: none;" title="West Flanders">West Flanders</a><span style="background-color: white; color: #252525; font-family: sans-serif;">. He studied </span><a href="https://en.wikipedia.org/wiki/Theology" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; text-decoration: none;" title="Theology">theology</a><span style="background-color: white; color: #252525; font-family: sans-serif;"> in Germany and England. At the age of 24 he became a </span><a class="mw-redirect" href="https://en.wikipedia.org/wiki/Religious_minister" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; text-decoration: none;" title="Religious minister">minister</a><span style="background-color: white; color: #252525; font-family: sans-serif;"> in the </span><a href="https://en.wikipedia.org/wiki/Dutch_Reformed_Church" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; text-decoration: none;" title="Dutch Reformed Church">Dutch Reformed Church</a><span style="background-color: white; color: #252525; font-family: sans-serif;">.</span><br />
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In 1589 Plancius collaborated with the Amsterdam cartographer <a href="https://en.wikipedia.org/wiki/Jacob_Floris_van_Langren" style="background: none; color: #0b0080; text-decoration: none;" title="Jacob Floris van Langren">Jacob Floris van Langren</a> on a 32.5-cm celestial globe, which, using the sparse information available about southern celestial features, for the first time depicted: <a href="https://en.wikipedia.org/wiki/Crux" style="background: none; color: #0b0080; text-decoration: none;" title="Crux">Crux</a> the southern cross, <a href="https://en.wikipedia.org/wiki/Triangulum_Australe" style="background: none; color: #0b0080; text-decoration: none;" title="Triangulum Australe">Triangulum Australe</a> the southern triangle, and the <a href="https://en.wikipedia.org/wiki/Ferdinand_Magellan" style="background: none; color: #0b0080; text-decoration: none;" title="Ferdinand Magellan">Magellanic Clouds</a>, <a href="https://en.wikipedia.org/wiki/Large_Magellanic_Cloud" style="background: none; color: #0b0080; text-decoration: none;" title="Large Magellanic Cloud">Nubecula Major</a> and <a href="https://en.wikipedia.org/wiki/Small_Magellanic_Cloud" style="background: none; color: #0b0080; text-decoration: none;" title="Small Magellanic Cloud">Minor</a>.</div>
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In 1595 Plancius asked <a href="https://en.wikipedia.org/wiki/Pieter_Dirkszoon_Keyser" style="background: none; color: #0b0080; text-decoration: none;" title="Pieter Dirkszoon Keyser">Pieter Dirkszoon Keyser</a>, the chief pilot on the <i>Hollandia</i>, to make observations to fill in the blank area around the south celestial pole on European maps of the southern sky. Keyser died in <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Java_(island)" style="background: none; color: #0b0080; text-decoration: none;" title="Java (island)">Java</a> the following year – the expedition had many casualties – but his catalogue of 135 <a href="https://en.wikipedia.org/wiki/Star" style="background: none; color: #0b0080; text-decoration: none;" title="Star">stars</a>,<sup class="reference" id="cite_ref-knobel_dehoutman_3-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Petrus_Plancius#cite_note-knobel_dehoutman-3" style="background: none; color: #0b0080; text-decoration: none;">[3]</a></sup> probably measured up with the help of explorer-colleague <a href="https://en.wikipedia.org/wiki/Frederick_de_Houtman" style="background: none; color: #0b0080; text-decoration: none;" title="Frederick de Houtman">Frederick de Houtman</a>,<sup class="reference" id="cite_ref-ridpath_ch1_c_4-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Petrus_Plancius#cite_note-ridpath_ch1_c-4" style="background: none; color: #0b0080; text-decoration: none;">[4]</a></sup> was delivered to Plancius. These stars appear as 12 new southern <a href="https://en.wikipedia.org/wiki/Constellation" style="background: none; color: #0b0080; text-decoration: none;" title="Constellation">constellations</a>,<sup class="reference" id="cite_ref-ridpath_ch1_c_4-1" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Petrus_Plancius#cite_note-ridpath_ch1_c-4" style="background: none; color: #0b0080; text-decoration: none;">[4]</a></sup> on a 35-cm celestial globe designed by Plancius in late 1597 (or early 1598) and produced in collaboration with the Amsterdam cartographer <a href="https://en.wikipedia.org/wiki/Jodocus_Hondius" style="background: none; color: #0b0080; text-decoration: none;" title="Jodocus Hondius">Jodocus Hondius the Elder</a>. The 12 new constellations (mostly referring to animals and subjects described in natural history books and travellers' journals of his day) are <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Apis_(constellation)" style="background: none; color: #0b0080; text-decoration: none;" title="Apis (constellation)">Apis</a> the Bee (later changed to <a href="https://en.wikipedia.org/wiki/Musca" style="background: none; color: #0b0080; text-decoration: none;" title="Musca">Musca</a> by <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Lacaille" style="background: none; color: #0b0080; text-decoration: none;" title="Lacaille">Lacaille</a>), <b><a href="https://en.wikipedia.org/wiki/Apus" style="background: none; color: #0b0080; text-decoration: none;" title="Apus">Apus</a> the Bird of Paradise</b>, <a href="https://en.wikipedia.org/wiki/Chamaeleon" style="background: none; color: #0b0080; text-decoration: none;" title="Chamaeleon">Chamaeleon</a>, <a href="https://en.wikipedia.org/wiki/Dorado" style="background: none; color: #0b0080; text-decoration: none;" title="Dorado">Dorado</a> the Goldfish (or Swordfish), <b><a href="https://en.wikipedia.org/wiki/Grus_(constellation)" style="background: none; color: #0b0080; text-decoration: none;" title="Grus (constellation)">Grus</a> the Crane</b>, <a href="https://en.wikipedia.org/wiki/Hydrus" style="background: none; color: #0b0080; text-decoration: none;" title="Hydrus">Hydrus</a>the Small Water Snake, <a href="https://en.wikipedia.org/wiki/Indus_(constellation)" style="background: none; color: #0b0080; text-decoration: none;" title="Indus (constellation)">Indus</a> the Indian,<b> <a href="https://en.wikipedia.org/wiki/Pavo_(constellation)" style="background: none; color: #0b0080; text-decoration: none;" title="Pavo (constellation)">Pavo</a> the Peacock, <a href="https://en.wikipedia.org/wiki/Phoenix_(constellation)" style="background: none; color: #0b0080; text-decoration: none;" title="Phoenix (constellation)">Phoenix</a></b>, <a href="https://en.wikipedia.org/wiki/Triangulum_Australe" style="background: none; color: #0b0080; text-decoration: none;" title="Triangulum Australe">Triangulum Australe</a> the Southern Triangle, <b><a href="https://en.wikipedia.org/wiki/Tucana" style="background: none; color: #0b0080; text-decoration: none;" title="Tucana">Tucana</a> the Toucan, and <a href="https://en.wikipedia.org/wiki/Volans" style="background: none; color: #0b0080; text-decoration: none;" title="Volans">Volans</a> the Flying Fish</b>. (The Southern Triangle and Southern Cross were reported as asterisms by earlier navigators and appear on earlier charts,<sup class="reference" id="cite_ref-Dekker_5-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/Petrus_Plancius#cite_note-Dekker-5" style="background: none; color: #0b0080; text-decoration: none;">[5]</a></sup> but the globe of 1598 is the first surviving source that plots their locations reasonably accurately.) Also notable is the inclusion of Achernar as Alpha Eridani.</div>
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These constellations, together with the constellation <a href="https://en.wikipedia.org/wiki/Columba_(constellation)" style="background: none; color: #0b0080; text-decoration: none;" title="Columba (constellation)"><b>Columba</b></a> illustrated by Plancius on his large wall map of the world of 1592, were then incorporated in 1603 by <a href="https://en.wikipedia.org/wiki/Johann_Bayer" style="background: none; color: #0b0080; text-decoration: none;" title="Johann Bayer">Johann Bayer</a> in his sky atlas, the <i><a href="https://en.wikipedia.org/wiki/Uranometria" style="background: none; color: #0b0080; text-decoration: none;" title="Uranometria">Uranometria</a></i>.</div>
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<span style="color: #252525; font-family: sans-serif;"><a href="https://en.wikipedia.org/wiki/Petrus_Plancius">https://en.wikipedia.org/wiki/Petrus_Plancius</a></span></div>
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<span style="color: #252525; font-family: sans-serif;"><a href="http://www.atlascoelestis.com/desu%20Plancius.htm">http://www.atlascoelestis.com/desu%20Plancius.htm</a></span></div>
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<span style="font-family: "arial" , sans-serif;"><b>Johann Bayer</b></span><span style="font-family: "arial" , sans-serif; font-size: 11pt;">, 1603, astrônomo. Obra: Uranometria. </span></div>
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<span style="font-family: "arial" , sans-serif; font-size: 11pt;">Relaciona 60 constelações, incluindo as circumpolares Sul, cuja nomenclatura conclui e unifica. </span></div>
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<span style="font-family: "arial" , sans-serif; font-size: 11pt;">Acrescenta 12 constelações.<o:p></o:p></span></div>
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<span style="font-family: "arial" , sans-serif; font-size: 11pt;"><b>Ave-do-Paraíso</b>, Camaleão, Dourado, <b>Grou</b>, Hidra Macho, Índio, Mosca, <b>Pavão, Fênix</b>, Triângulo Austral, <b>Tucano, Peixe-Voador<o:p></o:p></b></span></div>
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<span style="font-family: "arial" , sans-serif; font-size: 11pt;"><b>??? Jacob Bartsch</b></span><span style="font-family: "arial" , sans-serif; font-size: 11pt;">, 1624. </span><span lang="ES-TRAD" style="font-family: "arial" , sans-serif; font-size: 11pt;"><b>Pomba ??</b></span><br />
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<span lang="ES-TRAD"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white; font-family: "arial" , "helvetica" , sans-serif;"><span style="font-family: sans-serif; font-size: 14px;"><b><span style="color: #660000;">Bayer</span></b><span style="color: #252525;"> é mais famoso pelo seu </span></span><a class="mw-redirect" href="https://pt.wikipedia.org/wiki/Atlas_estelar" style="background-image: none; color: #0b0080; font-family: sans-serif; text-decoration: none;" title="Atlas estelar">atlas estelar</a><span style="color: #252525; font-family: sans-serif; font-size: 14px;"> </span><i style="color: #252525; font-family: sans-serif;"><a href="https://pt.wikipedia.org/wiki/Uranometria" style="background: none; color: #0b0080; text-decoration: none;" title="Uranometria">Uranometria</a></i><span style="color: #252525; font-family: sans-serif; font-size: 14px;">, publicado em </span><a href="https://pt.wikipedia.org/wiki/1603" style="background-image: none; color: #0b0080; font-family: sans-serif; text-decoration: none;" title="1603">1603</a><span style="color: #252525; font-family: sans-serif; font-size: 14px;"> e que foi o primeiro </span><a href="https://pt.wikipedia.org/wiki/Atlas_(cartografia)" style="background-image: none; color: #0b0080; font-family: sans-serif; text-decoration: none;" title="Atlas (cartografia)">atlas</a><span style="color: #252525; font-family: sans-serif; font-size: 14px;"> a cobrir toda a </span><a href="https://pt.wikipedia.org/wiki/Esfera_celeste" style="background-image: none; color: #0b0080; font-family: sans-serif; text-decoration: none;" title="Esfera celeste">esfera celeste</a><span style="color: #252525; font-family: sans-serif; font-size: 14px;">. Este trabalho introduziu um novo sistema para designar as estrelas, usando a notação grega e latina, que se tornou conhecido com nomenclatura, ou </span><a href="https://pt.wikipedia.org/wiki/Designa%C3%A7%C3%A3o_de_Bayer" style="background-image: none; color: #0b0080; font-family: sans-serif; text-decoration: none;" title="Designação de Bayer">designação, de Bayer</a><span style="color: #252525; font-family: sans-serif; font-size: 14px;">. A maioria das notações atribuídas por Bayer e por astrónomos posteriores que adoptaram o seu sistema permanece em uso até aos dias de hoje.</span></span></span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #252525; font-family: sans-serif; font-size: 14px;"><a href="https://pt.wikipedia.org/wiki/Johann_Bayer">https://pt.wikipedia.org/wiki/Johann_Bayer</a></span></span></div>
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E vamos encontrar</div>
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Hevelius, Royer e La Caille </div>
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nomeando e reafirmando<br />
várias outras constelações,</div>
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algumas mais ao sul e outras não:</div>
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<span style="font-family: "arial" , sans-serif;"><span style="font-size: medium;"><b>Hevelius</b></span></span><span style="font-family: "arial" , sans-serif; font-size: 11pt;">, 1690, astrônomo amador, selenógrafo. Obra: Sete Cartas Celestes. </span></div>
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<span style="font-family: "arial" , sans-serif; font-size: 11pt;">Dá nome a 9 constelações:<o:p></o:p></span></div>
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<span style="font-family: "arial" , sans-serif; font-size: 11pt;">Girafa, Cães de Caça, Lagarto, Leão Menor, Lince, Unicórnio, Escudo, Sextante, Raposa<o:p></o:p></span></div>
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<span style="font-family: "arial" , sans-serif;"><b><span style="font-size: medium;">Royer</span></b></span><span style="font-family: "arial" , sans-serif; font-size: 11pt;">, 1697, navegante francês. Obra: Carta Celeste. Desmembra a Cruz Australis da constelação do Centauro. Cruzeiro do Sul<o:p></o:p></span></div>
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<span lang="ES-TRAD" style="font-family: "arial" , sans-serif;"><b><span style="font-size: medium;">La Caille</span></b></span><span lang="ES-TRAD" style="font-family: "arial" , sans-serif; font-size: 11pt;">, 1752, astrônomo. </span><span style="font-family: "arial" , sans-serif; font-size: 11pt;">Obras: Memórias e Céu Estrelado. </span></div>
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<span style="font-family: "arial" , sans-serif; font-size: 11pt;">Introduz 14 novas constelações:</span></div>
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<span style="font-family: "arial" , sans-serif; font-size: 11pt;"> Máquina Pneumática, Buril, Compasso, Forno, Relógio, Mesa, Microscópio, Esquadro, Oitante, Pintor, Bússula, Retículo, Escultor, Telescópio<o:p></o:p></span></div>
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<span style="font-family: "arial" , sans-serif; font-size: 11pt;">E divide a extensa constelação ptolomaica Argo, o Navio, em Carina, Puppis e Vela.<o:p></o:p></span></div>
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<span style="font-family: "arial" , sans-serif; font-size: 11pt;">Quilha, Popa, Vela<o:p></o:p></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Olá!</span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Pássaros reais e Pássaros Míticos</span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white; font-family: "arial" , "helvetica" , sans-serif;">são representados através conjuntos estelares</span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white; font-family: "arial" , "helvetica" , sans-serif;">e é sempre um grande prazer morarmos no Hemisfério Sul</span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white; font-family: "arial" , "helvetica" , sans-serif;">e podermos observar</span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white; font-family: "arial" , "helvetica" , sans-serif;">estas joias!</span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Em nossa Postagem,</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Caro Leitor,</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">encontre alguma informação</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">sobre um Pássaro extremamente interessante</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">e nomeado por Johann Bayer</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">para simbolizar este agrupamento estelar:</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">é a constelação <b>Fênix, Phoenix</b>.</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">A Fênix é conhecida,</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">mitologicamente,</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">por renascer das próprias cinzas.</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">E, como disse Richard H. Allen,</span></div>
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<span style="color: #000066; font-family: "arial" , "helvetica" , sans-serif; text-align: justify;">em seu famoso e imperdível livro</span></div>
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<span style="line-height: 24px; text-align: justify;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Star Names - Their Lore and Meaning:</span></span></div>
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<span style="line-height: 24px; text-align: justify;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><i>Porém, mesmo que Bayer soubesse ou não, seu título (para esta constelação, Phoenix) é muito apropriado em função do fato de que em várias outras nações mais antigas </i></span></span></div>
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<span style="line-height: 24px; text-align: justify;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><i>- China, Egito, Índia e Pérsia -,</i></span></span></div>
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<span style="line-height: 24px; text-align: justify;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><i> este pássaro foi considerado "como um símbolo astronômico de período cíclico". </i> </span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Duas estrelas podem nos ajudar</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">a encontrar a estrela-alpha Phoenicis,</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Ankaa:</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">são Achernar, estrela-alpha Eridanii,</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">e Fomalhaut, estrela-alpha Piscis Austrinii:</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Ankaa situa-se entre essas estrelas</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">que são sempre bem conhecidas</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">em nossos céus mais ao sul.</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Também a constelação Grou, Grus,</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">encontra-se nas proximidades</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">e a estrela-alpha Gruis, Al Nair,</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">também nos ajuda a encontrar a Fênix.</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Este pássaro mítico</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">e imortalizado nas estrelas</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">nos revela também </span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">alguns objetos de céu profundo</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">bem interessantes</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">(principalmente o chamado Quarteto de Robert)</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">e ainda dois Aglomerados de Galáxias!</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">E ao final de nossa Postagem,</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Caro Leitor,</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">encontre também algumas informações</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">sobre a ave mítica Fênix,</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">cujo eterno renascimento das próprias cinzas</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">transformaram-na em símbolo de imortalidade</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">e de renascimento espiritual.</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Com um abraço estrelado,</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Janine Milward</span></div>
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<tr><td class="tr-caption" style="font-size: 12.8px;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif; font-size: small;">Mario Jaci Monteiro - As Constelações, Cartas Celestees</span></td></tr>
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<span style="background-color: white; color: #660000;"><b><span lang="EN-US" style="font-family: "arial" , sans-serif;"> </span><span style="font-family: "arial" , sans-serif;">PHOENIX, A FÊNIX</span></b></span></div>
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<span style="font-family: "arial" , sans-serif; line-height: 22px;"><span style="background-color: white; color: #073763;">Ascensão Reta 23h24m / 2h24m Declinação -39<sup>o</sup>.8 / -58<sup>o</sup>.2<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Constelação adicionada por Bayer em 1604.<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">O nome desta constelação retrata o pássaro mitológico que renascia das próprias cinzas. <o:p></o:p></span></span><br />
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<b>Phoenix</b> is a minor <a href="https://en.wikipedia.org/wiki/Constellation" style="background: none; color: #0b0080; text-decoration: none;" title="Constellation">constellation</a> in the <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Southern_sky" style="background: none; color: #0b0080; text-decoration: none;" title="Southern sky">southern sky</a>. Named after the mythical <a href="https://en.wikipedia.org/wiki/Phoenix_(mythology)" style="background: none; color: #0b0080; text-decoration: none;" title="Phoenix (mythology)">phoenix</a>, it was first depicted on a celestial atlas by <a href="https://en.wikipedia.org/wiki/Johann_Bayer" style="background: none; color: #0b0080; text-decoration: none;" title="Johann Bayer">Johann Bayer</a> in his 1603 <i><a href="https://en.wikipedia.org/wiki/Uranometria" style="background: none; color: #0b0080; text-decoration: none;" title="Uranometria">Uranometria</a></i>. The French explorer and astronomer <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background: none; color: #0b0080; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a> charted the brighter stars and gave their <a href="https://en.wikipedia.org/wiki/Bayer_designation" style="background: none; color: #0b0080; text-decoration: none;" title="Bayer designation">Bayer designations</a> in 1756. The constellation stretches from roughly −39° to −57° <a href="https://en.wikipedia.org/wiki/Declination" style="background: none; color: #0b0080; text-decoration: none;" title="Declination">declination</a>, and from 23.5h to 2.5h of <a href="https://en.wikipedia.org/wiki/Right_ascension" style="background: none; color: #0b0080; text-decoration: none;" title="Right ascension">right ascension</a>. The constellations Phoenix, <a href="https://en.wikipedia.org/wiki/Grus_(constellation)" style="background: none; color: #0b0080; text-decoration: none;" title="Grus (constellation)">Grus</a>, <a href="https://en.wikipedia.org/wiki/Pavo_(constellation)" style="background: none; color: #0b0080; text-decoration: none;" title="Pavo (constellation)">Pavo</a> and <a href="https://en.wikipedia.org/wiki/Tucana" style="background: none; color: #0b0080; text-decoration: none;" title="Tucana">Tucana</a>, are known as the Southern Birds.</div>
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The brightest star, <a href="https://en.wikipedia.org/wiki/Alpha_Phoenicis" style="background: none; color: #0b0080; text-decoration: none;" title="Alpha Phoenicis">Alpha Phoenicis</a>, is named Ankaa, an <a href="https://en.wikipedia.org/wiki/Arabic" style="background: none; color: #0b0080; text-decoration: none;" title="Arabic">Arabic</a> word meaning 'the Phoenix'. It is an orange giant of apparent magnitude 2.4. Next is <a href="https://en.wikipedia.org/wiki/Beta_Phoenicis" style="background: none; color: #0b0080; text-decoration: none;" title="Beta Phoenicis">Beta Phoenicis</a>, actually a <a href="https://en.wikipedia.org/wiki/Binary_star" style="background: none; color: #0b0080; text-decoration: none;" title="Binary star">binary</a> system composed of two yellow giants with a combined apparent magnitude of 3.3. <a href="https://en.wikipedia.org/wiki/Nu_Phoenicis" style="background: none; color: #0b0080; text-decoration: none;" title="Nu Phoenicis">Nu Phoenicis</a> has a dust disk, while the constellation has ten star systems with known planets and the recently discovered <a href="https://en.wikipedia.org/wiki/Galaxy_cluster" style="background: none; color: #0b0080; text-decoration: none;" title="Galaxy cluster">galaxy clusters</a> <a href="https://en.wikipedia.org/wiki/El_Gordo_(galaxy_cluster)" style="background: none; color: #0b0080; text-decoration: none;" title="El Gordo (galaxy cluster)">El Gordo</a> and the <a href="https://en.wikipedia.org/wiki/Phoenix_Cluster" style="background: none; color: #0b0080; text-decoration: none;" title="Phoenix Cluster">Phoenix Cluster</a>—located 7.2 and 5.7 billion light years away respectively, two of the largest objects in the <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Visible_universe" style="background: none; color: #0b0080; text-decoration: none;" title="Visible universe">visible universe</a>. Phoenix is the <a href="https://en.wikipedia.org/wiki/Radiant_(meteor_shower)" style="background: none; color: #0b0080; text-decoration: none;" title="Radiant (meteor shower)">radiant</a> of two annual <a href="https://en.wikipedia.org/wiki/Meteor_shower" style="background: none; color: #0b0080; text-decoration: none;" title="Meteor shower">meteor showers</a>: the <a href="https://en.wikipedia.org/wiki/Phoenicids" style="background: none; color: #0b0080; text-decoration: none;" title="Phoenicids">Phoenicids</a> in December, and the July Phoenicids.<span style="font-size: 11pt;"><span style="background-color: white; color: #073763; font-family: "georgia" , "times new roman" , serif;"><br /></span></span></div>
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<span style="color: #252525; font-family: sans-serif;"><a href="https://en.wikipedia.org/wiki/Phoenix_(constellation)">https://en.wikipedia.org/wiki/Phoenix_(constellation)</a></span></div>
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<span style="font-size: 11pt;"><span style="background-color: white; color: #073763; font-family: "georgia" , "times new roman" , serif;"><img alt="Phoenix constellation map.svg" height="428" src="https://upload.wikimedia.org/wikipedia/commons/thumb/1/12/Phoenix_constellation_map.svg/320px-Phoenix_constellation_map.svg.png" width="640" /></span></span><br />
<span style="font-size: 11pt;"><span style="background-color: white; color: #073763; font-family: "georgia" , "times new roman" , serif; font-size: 14.6667px;">Por Phoenix_constellation_map.png: Torsten Brongerderivative work: Kxx (talk) - Phoenix_constellation_map.png, CC BY-SA 3.0, https://commons.wikimedia.org/w/index.php?curid=10850946</span></span><br />
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<span style="color: #000066; line-height: 24px; text-align: justify;"><span style="font-family: "georgia" , "times new roman" , serif;">But, whether Bayer knew it or not, his title is an appropriate one, for with various early nations — at all events, in China, Egypt, India, and Persia — this bird has been "an astronomical symbol of cyclic period,"..................</span></span><br />
<span style="color: #000066; line-height: 24px; text-align: justify;"><span style="font-family: "georgia" , "times new roman" , serif;"><br /></span></span><span style="line-height: 24px; text-align: justify;"><span style="color: #000066; font-family: "palatino linotype" , "palatino" , "gentium plus" , serif;"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Phoenix*.html">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Phoenix*.html</a></span></span><br />
<span style="line-height: 24px; text-align: justify;"><br /></span><span style="line-height: 24px; text-align: justify;"><span style="color: #000066; font-family: "arial" , "helvetica" , sans-serif;">Richard H. Allen - em seu famoso e imperdível livro</span></span><br />
<span style="line-height: 24px; text-align: justify;"><span style="color: #000066; font-family: "arial" , "helvetica" , sans-serif;">Star Names - Their Lore and Meaning</span></span><br />
<span style="line-height: 24px; text-align: justify;"><span style="color: #000066; font-family: "arial" , "helvetica" , sans-serif;">nos revela que... </span></span><br />
<span style="line-height: 24px; text-align: justify;"><span style="color: #000066; font-family: "arial" , "helvetica" , sans-serif;"><i>Porém, mesmo que Bayer soubesse ou não, seu título (para esta constelação, Phoenix) é muito apropriado em função do fato de que em várias outras nações mais antigas </i></span></span><br />
<span style="line-height: 24px; text-align: justify;"><span style="color: #000066; font-family: "arial" , "helvetica" , sans-serif;"><i>- China, Egito, Índia e Pérsia -,</i></span></span><br />
<span style="line-height: 24px; text-align: justify;"><span style="color: #000066; font-family: "arial" , "helvetica" , sans-serif;"><i> este pássaro foi considerado "como um símbolo astronômico de período cíclico". </i> </span></span><br />
<span style="line-height: 24px; text-align: justify;"><span style="color: #000066; font-family: "arial" , "helvetica" , sans-serif;">(tradução simples e literal minha, Janine)</span></span><br />
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<span style="line-height: 24px; text-align: justify;"><span style="color: #000066; font-family: "arial" , "helvetica" , sans-serif;"><img height="640" src="https://upload.wikimedia.org/wikipedia/en/thumb/1/12/Phoenix_in_Doppelmayr%27s_Atlas_Coelestis.jpg/800px-Phoenix_in_Doppelmayr%27s_Atlas_Coelestis.jpg" width="636" /></span></span><br />
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By Johann Gabriel Doppelmayr(Life time: 1677-1750) - Original publication: <b><span style="color: #073763;">Johann Doppelmayr, Atlas Coelestis (plate 19), Nuremberg, ca. 1742</span></b>Immediate source: I own this map and took the photograph myself., Public Domain, https://en.wikipedia.org/w/index.php?curid=41271309</div>
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<span style="line-height: 24px; text-align: justify;"><span style="color: #000066; font-family: "palatino linotype" , "palatino" , "gentium plus" , serif;"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Phoenix*.html">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Phoenix*.html</a></span></span><br />
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<span style="font-family: "times new roman" , serif; font-size: 9.5pt;"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/home.html" target="index"><b><span lang="EN-US" style="color: blue; font-size: 13.5pt; text-decoration: none;">Star Names </span></b><b><span lang="EN-US" style="color: blue; font-size: 13.5pt; text-decoration: none;"><br /></span></b><b><span lang="EN-US" style="color: blue; font-size: 11.5pt; text-decoration: none;">Their Lore and Meaning </span></b><b><span lang="EN-US" style="color: blue; text-decoration: none;"><br /></span></b><b><span lang="EN-US" style="color: blue;">by</span></b><b><span lang="EN-US" style="color: blue; text-decoration: none;"> </span></b><b><span lang="EN-US" style="color: blue; text-decoration: none;"><br /></span></b><b><span lang="EN-US" style="color: blue; font-size: 13.5pt; text-decoration: none;">Richard Hinckley Allen </span></b></a></span><span lang="EN-US" style="font-family: "times new roman" , serif; font-size: 9.5pt;"><br />as reprinted</span><span lang="EN-US" style="font-family: "times new roman" , serif; font-size: 9.5pt;"> </span><span lang="EN-US" style="font-family: "times new roman" , serif; font-size: 9.5pt;"><br />in the Dover edition, 1963<o:p></o:p></span></div>
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<span lang="EN-US" style="font-family: "times new roman" , serif; font-size: 9.5pt;">The text is in the public domain.<o:p></o:p></span></div>
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<b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 14.5pt;">Phoenix,<o:p></o:p></span></b></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 12pt;"><span lang="EN-US" style="font-size: 12pt;">p336</span><span lang="EN-US" style="font-size: 13.5pt;">Others changed the figure to that of a</span><span lang="EN-US" style="font-size: 13.5pt;"> </span><b><span lang="EN-US" style="font-size: 13.5pt;">Griffin</span></b><span lang="EN-US" style="font-size: 13.5pt;">, or</span><span lang="EN-US" style="font-size: 13.5pt;"> </span><b><span lang="EN-US" style="font-size: 13.5pt;">Eagle</span></b><span lang="EN-US" style="font-size: 13.5pt;">, so that the introduction of a Phoenix into modern astronomy was, in a measure, by adoption rather than by invention.</span>p335</span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 14.5pt;">Phoenix,<o:p></o:p></span></b></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">the French</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Phénix</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the German</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Phönix</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, and the Italian</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Fenice</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, is one of Bayer's new figures, between</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Eridanus*.html"><span lang="EN-US" style="color: blue;">Eridanus</span><span lang="EN-US" style="color: blue; text-decoration: none;"> </span></a></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">and</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Grus*.html"><span lang="EN-US" style="color: blue;">Grus</span></a></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, south of</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Fornax*.html"><span lang="EN-US" style="color: blue;">Fornax</span><span lang="EN-US" style="color: blue; text-decoration: none;"> </span></a></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">and</span><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Sculptor*.html"><span lang="EN-US" style="color: blue; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Sculptor</span></a><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, — its</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">α</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">κ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">μ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">β</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">ν</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, and </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">γ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">in a line curving toward the south like that of a primitive</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Boat</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, by which figure, as</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Zaura</b></span><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ḳ</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Arabs knew them. Al Sufi cited another name, —</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Ri</b></span><b><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">᾽</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">āl</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Young Ostriches, — which Hyde wrongly read</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Al Zibal</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, perhaps a synonymous title; and Kazwini used Al Sufi's term in describing some stars of Al Nahr, the River, in which our Phoenix was then included by Arabian astronomers.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">But, whether Bayer knew it or not, his title is an appropriate one, for with various early nations — at all events, in China, Egypt, India, and Persia — this bird has been "an astronomical symbol of cyclic period," some versions of the well-known fable making its life coincident with the Great Year of the ancients beginning at noon of the day when the sun entered among the stars of Aries; and, in Egypt, with the Sothic Period when the sun and Sirius rose together on the 20th of July. Thompson further writes of this:<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "helvetica" , sans-serif; font-size: 10pt;">A new Phoenix-period is said to have commenced</span><span lang="EN-US" style="color: #000066; font-family: "helvetica" , sans-serif; font-size: 10pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "helvetica" , sans-serif; font-size: 8.5pt;">A.D.</span><span lang="EN-US" style="color: #000066; font-family: "helvetica" , sans-serif; font-size: 10pt;"> 139, in the reign of Antoninus Pius; and a recrudescence of astronomical symbolism associated therewith is manifested on the coins of that Emperor.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Coincidently, Ptolemy adopted as the epoch of his catalogue the year 138, the first of Antoninus. With the Egyptians, who knew this bird as</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Bennu </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">and showed it on their coins, it was an emblem of immortality; indeed it generally has been such in pagan as well as in Christian times.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">In China the constellation was</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Ho Neaou</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Fire Bird, showing its derivation there from the Jesuits.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Julius Schiller combined it with Grus in his</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Aaron the High Priest</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Gould catalogues 139 naked-eye stars here, from 2.4 to 7.<o:p></o:p></span></div>
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<i><span style="color: #000066; font-family: "verdana" , sans-serif;">α</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, of 2.2. magnitude, was Al Tizini's</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Nā</b></span><b><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">᾽</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">ir al Zaura</span></b><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ḳ</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Bright One in the Boat, rendered in Hyde's translation</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> lucida Cymbae</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">. It culminates just above the horizon of New York City on the 17th of November, and is quite conspicuous from its solitary position southeast from Fomalhaut.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">A 14th‑magnitude companion, purple in tint, has recently been discovered by See, 9ʺ away, with a position angle of 280°.<o:p></o:p></span></div>
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<span style="line-height: 24px; text-align: justify;"><span style="color: #000066; font-family: "arial" , "helvetica" , sans-serif;">Stellarium</span></span><span style="line-height: 24px; text-align: justify;"><span style="color: #000066; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span><br />
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<span style="background-color: white; color: #073763;"><span style="font-family: "arial" , sans-serif;"><b>Ankaa</b></span><span style="font-family: "arial" , sans-serif;"><b> - Alpha Phoenicis</b><o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Asc. Reta 00h25,3m - Declinação -42,25<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;"> Magnitude visual 2,44 - Distância 93 anos-luz<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Extremidade, termo árabe.<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;"><b>Beta Phoenicis - Estrela Dupla</b><o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 01h03m Declinação -46<sup>o</sup>.59 Magnitude 4,0 e 4,2<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Ângulo de Posição 345<sup>o</sup>.,4 Distância entre estrelas 1”,63<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;">- 6<sup>a</sup>. Edição do <b>Atlas Celeste</b></span><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></div>
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<span style="font-family: "arial" , sans-serif;">de autoria de <b>Ronaldo Rogério de Freitas Mourão</b>,</span></div>
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<span style="font-family: "arial" , sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="background-color: white;"><span style="color: #073763;"><b style="font-family: sans-serif; line-height: 22.4px;">Phoenix</b><span style="font-family: sans-serif; line-height: 22.4px;"> (Phe), a </span><a href="http://pt.wikipedia.org/wiki/F%C3%AAnix" style="background-image: none; font-family: sans-serif; line-height: 22.4px; text-decoration: none;" title="Fênix">Fênix</a><span style="font-family: sans-serif; line-height: 22.4px;">, é uma </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; font-family: sans-serif; line-height: 22.4px; text-decoration: none;" title="Constelação">constelação</a><span style="font-family: sans-serif; line-height: 22.4px;"> do </span><a href="http://pt.wikipedia.org/wiki/Hemisf%C3%A9rio_celestial_sul" style="background-image: none; font-family: sans-serif; line-height: 22.4px; text-decoration: none;" title="Hemisfério celestial sul">hemisfério celestial sul</a><span style="font-family: sans-serif; line-height: 22.4px;">. O genitivo, usado para formar nomes de estrelas, é </span><b style="font-family: sans-serif; line-height: 22.4px;">Phoenicis</b><span style="font-family: sans-serif; line-height: 22.4px;">. Sua </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-image: none; font-family: sans-serif; line-height: 22.4px; text-decoration: none;" title="Estrela">estrela</a><span style="font-family: sans-serif; line-height: 22.4px;"> mais brilhante é </span><a href="http://pt.wikipedia.org/wiki/Alpha_Phoenicis" style="background-image: none; font-family: sans-serif; line-height: 22.4px; text-decoration: none;" title="Alpha Phoenicis">Alpha Phoenicis</a><span style="font-family: sans-serif; line-height: 22.4px;"> (Ankaa). A constelação se situa a aproximadamente entre -41° e -57° de </span><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-image: none; font-family: sans-serif; line-height: 22.4px; text-decoration: none;" title="Declinação">declinação</a><span style="font-family: sans-serif; line-height: 22.4px;"> e 23,5h e 2h de </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-image: none; font-family: sans-serif; line-height: 22.4px; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="font-family: sans-serif; line-height: 22.4px;">, e é visível entre as latitudes +40° e -90°.</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><a href="http://pt.wikipedia.org/wiki/Phoenix_(constela%C3%A7%C3%A3o">http://pt.wikipedia.org/wiki/Phoenix_(constela%C3%A7%C3%A3o</a>)</span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><b>Alpha Phoenicis</b> (α Phe, α Phoenicis), também chamada de <b>Ankaa</b>, é a <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Estrela">estrela</a> mais brilhante da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Phoenix_(constela%C3%A7%C3%A3o)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Phoenix (constelação)">Phoenix</a>. Se localiza a cerca de 77 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Ano-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Terra">Terra</a>.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763;">Alpha Phoenicis é uma <a href="http://pt.wikipedia.org/wiki/Estrela_gigante" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Estrela gigante">estrela gigante</a> de <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Classificação estelar">tipo</a> K com <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 2,37. Tem uma estrela companheira <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Bin%C3%A1ria_espectrosc%C3%B3pica" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Binária espectroscópica">espectroscópica</a> de baixa massa, que a orbita a cada 10,5 <a href="http://pt.wikipedia.org/wiki/Ano" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Ano">anos</a> a uma distância média de 7 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Unidade_Astron%C3%B4mica" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Unidade Astronômica">UA</a> (aproximadamente um bilhão de <a href="http://pt.wikipedia.org/wiki/Quil%C3%B4metro" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Quilômetro">quilômetros</a>).</span></span></div>
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<span style="background-color: white; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif;"><a href="http://pt.wikipedia.org/wiki/Alpha_Phoenicis">http://pt.wikipedia.org/wiki/Alpha_Phoenicis</a></span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhODH5aij5Nd7Ke0RkPtdVQD4uCWxxNc12mKjkMQyQvhMY8OrZRskm0jT5KPnMNYMN8FH-G8kx60RjDi_rseXHIo9ksEcAGVYMvAy_2bTRrC9CrYhAUOUTereRhEX3o77nGi6PFUKT1pys/s1600/ankaa.jpg" imageanchor="1" style="background-color: white; margin-left: 1em; margin-right: 1em;"><span style="color: #073763;"><img border="0" height="320" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhODH5aij5Nd7Ke0RkPtdVQD4uCWxxNc12mKjkMQyQvhMY8OrZRskm0jT5KPnMNYMN8FH-G8kx60RjDi_rseXHIo9ksEcAGVYMvAy_2bTRrC9CrYhAUOUTereRhEX3o77nGi6PFUKT1pys/s1600/ankaa.jpg" width="640" /></span></a></div>
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<span style="color: #073763; font-family: sans-serif;"><span style="background-color: white; font-size: 14px; line-height: 22.4px;">http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=ALPHA+PHOENICIS</span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><b style="font-family: sans-serif; line-height: 22.4px;">Beta Phoenicis</b><span style="font-family: sans-serif; line-height: 22.4px;"> (β Phe / β Phoenicis) é a segunda </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-image: none; font-family: sans-serif; line-height: 22.4px; text-decoration: none;" title="Estrela">estrela</a><span style="font-family: sans-serif; line-height: 22.4px;"> mais brilhante da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; font-family: sans-serif; line-height: 22.4px; text-decoration: none;" title="Constelação">constelação</a><span style="font-family: sans-serif; line-height: 22.4px;"> de </span><a href="http://pt.wikipedia.org/wiki/Phoenix_(constela%C3%A7%C3%A3o)" style="background-image: none; font-family: sans-serif; line-height: 22.4px; text-decoration: none;" title="Phoenix (constelação)">Phoenix</a><span style="font-family: sans-serif; line-height: 22.4px;">. É uma </span><a href="http://pt.wikipedia.org/wiki/Estrela_gigante" style="background-image: none; font-family: sans-serif; line-height: 22.4px; text-decoration: none;" title="Estrela gigante">estrela gigante</a><span style="font-family: sans-serif; line-height: 22.4px;"> amarela de </span><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-image: none; font-family: sans-serif; line-height: 22.4px; text-decoration: none;" title="Classificação estelar">classe</a><span style="font-family: sans-serif; line-height: 22.4px;"> G com </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; font-family: sans-serif; line-height: 22.4px; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="font-family: sans-serif; line-height: 22.4px;">de 3,232. Está localizada a aproximadamente 200 </span><a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-image: none; font-family: sans-serif; line-height: 22.4px; text-decoration: none;" title="Ano-luz">anos-luz</a><span style="font-family: sans-serif; line-height: 22.4px;"> da </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background-image: none; font-family: sans-serif; line-height: 22.4px; text-decoration: none;" title="Terra">Terra</a><span style="font-family: sans-serif; line-height: 22.4px;">.</span></span></span></div>
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<span style="background-color: white; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif;"><a href="http://pt.wikipedia.org/wiki/Beta_Phoenicis">http://pt.wikipedia.org/wiki/Beta_Phoenicis</a></span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhlau3UEP34DNIjWG6yNcd26kahYu3xOETdOaXtc8cqGz6Gu76MjKndtOyICiDM05fo_xdwzGqt4xvN0xelDeQVFfZANMPfgNmraQ14OrHWlo0NZE8L3W80F2qO67zAZNpP7hyphenhyphengfEX7YmM/s1600/BETA+PHOENICIS.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="322" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhlau3UEP34DNIjWG6yNcd26kahYu3xOETdOaXtc8cqGz6Gu76MjKndtOyICiDM05fo_xdwzGqt4xvN0xelDeQVFfZANMPfgNmraQ14OrHWlo0NZE8L3W80F2qO67zAZNpP7hyphenhyphengfEX7YmM/s1600/BETA+PHOENICIS.jpg" width="640" /></a></div>
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<span style="background-color: white; font-size: 14px; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif;">http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=BETA+PHOENICIS</span></span></div>
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<span style="background-color: white; font-size: 14px; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif;"><span style="color: #333333; font-size: 20px;">The constellation Phoenix as it can be seen by the naked eye.</span></span></span><br />
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<span style="background-color: white; font-size: 14px; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif;"><img height="640" src="https://upload.wikimedia.org/wikipedia/commons/thumb/9/95/Constellation_Phoenix.jpg/256px-Constellation_Phoenix.jpg" width="426" /></span></span><br />
<span style="background-color: white; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif; font-size: 14px;">https://en.wikipedia.org/wiki/Phoenix_(constellation)#/media/File:Constellation_Phoenix.jpg</span></span><br />
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<span style="background-color: white; line-height: 22.4px;"><span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif;"><b>OBJETOS DE CÉU PROFUNDO</b></span></span><br />
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<span style="background-color: white; font-size: 14px; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif;"><span style="color: #333333; font-size: 20px;">Robert's quartet</span></span></span><br />
<span style="background-color: white; font-size: 14px; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif;"><span style="color: #333333; font-size: 20px;">O Quarteto de Robert</span></span></span><br />
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<b>Robert's Quartet</b> is a compact <a href="https://en.wikipedia.org/wiki/Galaxy_group" style="background: none; color: #0b0080; text-decoration: none;" title="Galaxy group">galaxy group</a> approximately 160 million <a href="https://en.wikipedia.org/wiki/Light-year" style="background: none; color: #0b0080; text-decoration: none;" title="Light-year">light-years</a> away in the <a href="https://en.wikipedia.org/wiki/Constellation" style="background: none; color: #0b0080; text-decoration: none;" title="Constellation">constellation</a> <a href="https://en.wikipedia.org/wiki/Phoenix_(constellation)" style="background: none; color: #0b0080; text-decoration: none;" title="Phoenix (constellation)">Phoenix</a>. It is a family of four very different <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Galaxies" style="background: none; color: #0b0080; text-decoration: none;" title="Galaxies">galaxies</a> in the process of <a class="mw-redirect" href="https://en.wikipedia.org/wiki/Colliding_and_merging" style="background: none; color: #0b0080; text-decoration: none;" title="Colliding and merging">colliding and merging</a>. Its members are <a href="https://en.wikipedia.org/wiki/NGC_87" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 87">NGC 87</a>, <a href="https://en.wikipedia.org/wiki/NGC_88" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 88">NGC 88</a>, <a href="https://en.wikipedia.org/wiki/NGC_89" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 89">NGC 89</a> and <a href="https://en.wikipedia.org/wiki/NGC_92" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 92">NGC 92</a>, discovered by <a href="https://en.wikipedia.org/wiki/John_Herschel" style="background: none; color: #0b0080; text-decoration: none;" title="John Herschel">John Herschel</a> in the 1830s. <a href="https://en.wikipedia.org/wiki/NGC_101" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 101">NGC 101</a> is also a loosely related member.</div>
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The quartet is one of the finest examples of compact groups of galaxies. Because such groups contain four to eight galaxies in a very small region, they are excellent laboratories for the study of galactic interactions and their effects, in particular on the formation of stars. The quartet has a total visual magnitude of almost 13. The brightest member of the group has a magnitude of about 14. On the sky, the four galaxies are all within a circle of radius of 1.6 arcmin, corresponding to about 75,000 light-years. It was named by <a href="https://en.wikipedia.org/wiki/Halton_Arp" style="background: none; color: #0b0080; text-decoration: none;" title="Halton Arp">Halton Arp</a> and <a class="new" href="https://en.wikipedia.org/w/index.php?title=Barry_F._Madore&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Barry F. Madore (page does not exist)">Barry F. Madore</a>, who compiled <i>A Catalogue of Southern Peculiar Galaxies and Associations</i> in 1987.</div>
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<span class="mw-headline" id="Members">Members</span><span class="mw-editsection" style="display: inline-block; font-family: sans-serif; font-size: x-small; line-height: 1em; margin-left: 1em; vertical-align: baseline; white-space: nowrap;"><span class="mw-editsection-bracket" style="color: #555555; margin-right: 0.25em;">[</span><a href="https://en.wikipedia.org/w/index.php?title=Robert%27s_Quartet&action=edit&section=1" style="background: none; color: #0b0080; text-decoration: none;" title="Edit section: Members">edit</a><span class="mw-editsection-bracket" style="color: #555555; margin-left: 0.25em;">]</span></span></h2>
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<table cellpadding="2" class="wikitable" style="background-color: #f9f9f9; border-collapse: collapse; border: 1px solid rgb(170, 170, 170); color: black; font-family: sans-serif; font-size: 14px; margin: 1em 0px; text-align: center;"><caption style="font-weight: bold;"><b>Members of Robert's Quartet</b></caption><tbody>
<tr><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em; text-align: center;">Name</th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em; text-align: center;"><a href="https://en.wikipedia.org/wiki/Galaxy_morphological_classification" style="background: none; color: #0b0080; text-decoration: none;" title="Galaxy morphological classification">Type</a></th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em; text-align: center;">Distance from <a href="https://en.wikipedia.org/wiki/Sun" style="background: none; color: #0b0080; text-decoration: none;" title="Sun">Sun</a><br />
(million <a href="https://en.wikipedia.org/wiki/Light-year" style="background: none; color: #0b0080; text-decoration: none;" title="Light-year">ly</a>)</th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em; text-align: center;"><a href="https://en.wikipedia.org/wiki/Apparent_magnitude" style="background: none; color: #0b0080; text-decoration: none;" title="Apparent magnitude">Magnitude</a></th></tr>
<tr style="background: rgb(238, 238, 255);"><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em;"><a href="https://en.wikipedia.org/wiki/NGC_87" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 87">NGC 87</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em;">IBm pec.</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em;">155</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em;">+14.5</td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em;"><a href="https://en.wikipedia.org/wiki/NGC_88" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 88">NGC 88</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em;">SB(rs)a pec.</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em;">156</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em;">+15.21</td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em;"><a href="https://en.wikipedia.org/wiki/NGC_89" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 89">NGC 89</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em;">SB0(s)a pec.</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em;">149</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em;">+14.57</td></tr>
<tr style="background: rgb(204, 204, 255);"><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em;"><a href="https://en.wikipedia.org/wiki/NGC_92" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 92">NGC 92</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em;">SAa pec.</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em;">146</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em;">+14.29</td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em;"><a href="https://en.wikipedia.org/wiki/NGC_101" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 101">NGC 101</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em;">Sc</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em;">154</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em 0.4em;">+13.46</td></tr>
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<span style="background-color: white; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif; font-size: 14px;"><a href="https://en.wikipedia.org/wiki/Robert%27s_Quartet">https://en.wikipedia.org/wiki/Robert%27s_Quartet</a></span></span><br />
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O <b>Quarteto de Robert</b> é um <a href="https://pt.wikipedia.org/wiki/Aglomerado_de_gal%C3%A1xias" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado de galáxias">grupo</a> de <a href="https://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia">galáxias</a> cerca de 160 milhões de anos-luz de distância na direção da <a href="https://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a class="mw-disambig" href="https://pt.wikipedia.org/wiki/Phoenix" style="background: none; color: #0b0080; text-decoration: none;" title="Phoenix">Phoenix</a>. Trata-se de uma família de quatro diferentes galáxias no processo de colisão e fusão. Os seus membros são <a href="https://pt.wikipedia.org/wiki/NGC_87" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 87">NGC 87</a>, <a href="https://pt.wikipedia.org/wiki/NGC_88" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 88">NGC 88</a>, <a href="https://pt.wikipedia.org/wiki/NGC_89" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 89">NGC 89</a> e <a href="https://pt.wikipedia.org/wiki/NGC_92" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 92">NGC 92</a>, descobertas por <a href="https://pt.wikipedia.org/wiki/John_Herschel" style="background: none; color: #0b0080; text-decoration: none;" title="John Herschel">John Herschel</a>, nos anos <a href="https://pt.wikipedia.org/wiki/1830" style="background: none; color: #0b0080; text-decoration: none;" title="1830">1830</a>.</div>
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O quarteto é um dos mais belos exemplos de grupos compactos de <a href="https://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia">galáxias</a>. Porque esses grupos contêm quatro a oito galáxias em uma região muito pequena, eles são excelentes laboratórios para o estudo da galáxia interações e seus efeitos, em especial, sobre a formação de <a href="https://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a>. O quarteto tem um total de quase 13 de <a href="https://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a>. O mais brilhante membro do grupo tem uma <a class="mw-disambig" href="https://pt.wikipedia.org/wiki/Magnitude" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude">magnitude</a> de cerca de 14. Sobre o céu, as quatro galáxias estão todas dentro de um círculo de raio de 1,6 arco de minuto, o que corresponde a cerca de 75000 <a class="mw-redirect" href="https://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a>. Ele foi nomeado por <a href="https://pt.wikipedia.org/wiki/Halton_Arp" style="background: none; color: #0b0080; text-decoration: none;" title="Halton Arp">Halton Arp</a> e <a class="new" href="https://pt.wikipedia.org/w/index.php?title=Barry_F._Madore&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Barry F. Madore (página não existe)">Barry F. Madore</a>, que compilou um <i>Catálogo de Galáxias e Associações Peculiares Austrais</i>, em 1987.</div>
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<span style="color: #252525; font-family: sans-serif;"><a href="https://pt.wikipedia.org/wiki/Quarteto_de_Robert">https://pt.wikipedia.org/wiki/Quarteto_de_Robert</a></span></div>
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<span style="background-color: white; font-size: 14px; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif;"><img alt="Robert's quartet.jpg" src="https://upload.wikimedia.org/wikipedia/commons/b/b3/Robert%27s_quartet.jpg" /></span></span><br />
<span style="background-color: white; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif; font-size: 14px;">CC BY 4.0, https://commons.wikimedia.org/w/index.php?curid=3984951</span></span><br />
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<b>NGC 87</b> é uma <a href="https://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia">galáxia</a> <a href="https://pt.wikipedia.org/wiki/Gal%C3%A1xia_irregular" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia irregular">irregular</a> (IBm/P) localizada na direcção da <a href="https://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="https://pt.wikipedia.org/wiki/Phoenix_(constela%C3%A7%C3%A3o)" style="background: none; color: #0b0080; text-decoration: none;" title="Phoenix (constelação)">Phoenix</a>. Possui uma declinação de -48° 37' 44" e uma <a class="mw-redirect" href="https://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 0 <a href="https://pt.wikipedia.org/wiki/Hora" style="background: none; color: #0b0080; text-decoration: none;" title="Hora">horas</a>, 21 <a href="https://pt.wikipedia.org/wiki/Minuto" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto">minutos</a> e 14,2 <a href="https://pt.wikipedia.org/wiki/Segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a>.</div>
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A galáxia <b>NGC 87</b> foi descoberta em <a class="mw-redirect" href="https://pt.wikipedia.org/wiki/30_de_Setembro" style="background: none; color: #0b0080; text-decoration: none;" title="30 de Setembro">30 de Setembro</a> de <a href="https://pt.wikipedia.org/wiki/1834" style="background: none; color: #0b0080; text-decoration: none;" title="1834">1834</a> por <a href="https://pt.wikipedia.org/wiki/John_Herschel" style="background: none; color: #0b0080; text-decoration: none;" title="John Herschel">John Herschel</a>.</div>
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<span style="color: #252525; font-family: sans-serif;">https://pt.wikipedia.org/wiki/NGC_87</span></div>
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<span style="background-color: white; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif;"><b style="color: #252525; text-align: start;">NGC 87</b><span style="color: #252525; text-align: start;"> is a diffuse, highly disorganized barred </span><a href="https://en.wikipedia.org/wiki/Irregular_galaxy" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Irregular galaxy">irregular galaxy</a><span style="color: #252525; text-align: start;">, part of </span><a href="https://en.wikipedia.org/wiki/Robert%27s_Quartet" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Robert's Quartet">Robert's Quartet</a><span style="color: #252525; text-align: start;">, a group of four </span><a class="mw-redirect" href="https://en.wikipedia.org/wiki/Interacting_galaxies" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Interacting galaxies">interacting galaxies</a><span style="color: #252525; text-align: start;">.</span></span></span><br />
<span style="background-color: white; line-height: 22.4px;"><span style="color: #252525; font-family: sans-serif;"><span style="text-align: start;">https://en.wikipedia.org/wiki/NGC_87</span></span></span><br />
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<b>NGC 88</b> é uma <a href="https://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia">galáxia</a> <a href="https://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral_barrada" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia espiral barrada">espiral barrada</a> (SB0-a) localizada na direcção da <a href="https://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="https://pt.wikipedia.org/wiki/Phoenix_(constela%C3%A7%C3%A3o)" style="background: none; color: #0b0080; text-decoration: none;" title="Phoenix (constelação)">Phoenix</a>. Possui uma declinação de -48° 38' 23" e uma <a class="mw-redirect" href="https://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 0 <a href="https://pt.wikipedia.org/wiki/Hora" style="background: none; color: #0b0080; text-decoration: none;" title="Hora">horas</a>, 21 <a href="https://pt.wikipedia.org/wiki/Minuto" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto">minutos</a> e 22,0 <a href="https://pt.wikipedia.org/wiki/Segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a>.</div>
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A galáxia <b>NGC 88</b> foi descoberta em <a class="mw-redirect" href="https://pt.wikipedia.org/wiki/30_de_Setembro" style="background: none; color: #0b0080; text-decoration: none;" title="30 de Setembro">30 de Setembro</a> de <a href="https://pt.wikipedia.org/wiki/1834" style="background: none; color: #0b0080; text-decoration: none;" title="1834">1834</a> por <a href="https://pt.wikipedia.org/wiki/John_Herschel" style="background: none; color: #0b0080; text-decoration: none;" title="John Herschel">John Herschel</a>.</div>
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<span style="color: #252525; font-family: sans-serif;">https://pt.wikipedia.org/wiki/NGC_88</span></div>
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<span style="background-color: white; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif;"><b style="color: #252525; text-align: start;">NGC 88</b><span style="color: #252525; text-align: start;"> is a </span><a href="https://en.wikipedia.org/wiki/Barred_spiral_galaxy" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Barred spiral galaxy">barred spiral galaxy</a><span style="color: #252525; text-align: start;"> exhibiting an inner ring structure located about 160 million </span><a class="mw-redirect" href="https://en.wikipedia.org/wiki/Light_year" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Light year">light years</a><span style="color: #252525; text-align: start;"> from the </span><a href="https://en.wikipedia.org/wiki/Earth" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Earth">Earth</a><span style="color: #252525; text-align: start;"> in the </span><a href="https://en.wikipedia.org/wiki/Phoenix_(constellation)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Phoenix (constellation)">Phoenix constellation</a><span style="color: #252525; text-align: start;">. NGC 88 is interacting with the galaxies </span><a href="https://en.wikipedia.org/wiki/NGC_92" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="NGC 92">NGC 92</a><span style="color: #252525; text-align: start;">, </span><a href="https://en.wikipedia.org/wiki/NGC_87" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="NGC 87">NGC 87</a><span style="color: #252525; text-align: start;"> and </span><a href="https://en.wikipedia.org/wiki/NGC_89" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="NGC 89">NGC 89</a><span style="color: #252525; text-align: start;">. It is part of a family of galaxies called </span><a href="https://en.wikipedia.org/wiki/Robert%27s_Quartet" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Robert's Quartet">Robert's Quartet</a><span style="color: #252525; text-align: start;"> discovered by astronomer </span><a href="https://en.wikipedia.org/wiki/John_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="John Herschel">John Herschel</a><span style="color: #252525; text-align: start;"> in the 1830s.</span></span></span><br />
<span style="background-color: white; line-height: 22.4px;"><span style="color: #252525; font-family: sans-serif;"><span style="text-align: start;">https://en.wikipedia.org/wiki/NGC_88</span></span></span><br />
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<b>NGC 89</b> é uma <a href="https://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia">galáxia</a> <a href="https://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral_barrada" style="background: none; color: #0b0080;" title="Galáxia espiral barrada">espiral barrada</a> (SB0-a) localizada na direcção da <a href="https://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="https://pt.wikipedia.org/wiki/Phoenix_(constela%C3%A7%C3%A3o)" style="background: none; color: #0b0080; text-decoration: none;" title="Phoenix (constelação)">Phoenix</a>. Possui uma declinação de -48° 39' 55" e uma <a class="mw-redirect" href="https://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 0 <a href="https://pt.wikipedia.org/wiki/Hora" style="background: none; color: #0b0080; text-decoration: none;" title="Hora">horas</a>, 21 <a href="https://pt.wikipedia.org/wiki/Minuto" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto">minutos</a> e 24,3 <a href="https://pt.wikipedia.org/wiki/Segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a>.</div>
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A galáxia <b>NGC 89</b> foi descoberta em <a class="mw-redirect" href="https://pt.wikipedia.org/wiki/30_de_Setembro" style="background: none; color: #0b0080; text-decoration: none;" title="30 de Setembro">30 de Setembro</a> de <a href="https://pt.wikipedia.org/wiki/1834" style="background: none; color: #0b0080; text-decoration: none;" title="1834">1834</a> por <a href="https://pt.wikipedia.org/wiki/John_Herschel" style="background: none; color: #0b0080; text-decoration: none;" title="John Herschel">John Herschel</a>.</div>
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<span style="color: #252525; font-family: sans-serif;">https://pt.wikipedia.org/wiki/NGC_89</span></div>
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<span style="background-color: white; font-size: 14px; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif;"><b style="color: #252525; text-align: start;">NGC 89</b><span style="color: #252525; text-align: start;"> is a </span><a href="https://en.wikipedia.org/wiki/Barred_spiral_galaxy" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Barred spiral galaxy">barred spiral</a><span style="color: #252525; text-align: start;"> or </span><a href="https://en.wikipedia.org/wiki/Lenticular_galaxy" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Lenticular galaxy">lenticular galaxy</a><span style="color: #252525; text-align: start;">, part of </span><a href="https://en.wikipedia.org/wiki/Robert%27s_Quartet" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Robert's Quartet">Robert's Quartet</a><span style="color: #252525; text-align: start;">, a group of four </span><a class="mw-redirect" href="https://en.wikipedia.org/wiki/Interacting_galaxies" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Interacting galaxies">interacting galaxies</a><span style="color: #252525; text-align: start;">. This member has a </span><a href="https://en.wikipedia.org/wiki/Seyfert_galaxy" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Seyfert galaxy">Seyfert 2 nucleus</a><span style="color: #252525; text-align: start;"> with extra-planar features emitting </span><a href="https://en.wikipedia.org/wiki/H-alpha" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="H-alpha">H-alpha</a><span style="color: #252525; text-align: start;"> radiation. There are filamentary features on each side of the disk, including a jet-like structure extending about 4 kpc in the NE direction. It may have lost its </span><a class="mw-redirect" href="https://en.wikipedia.org/wiki/Neutral_hydrogen" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Neutral hydrogen">neutral hydrogen</a><span style="color: #252525; text-align: start;"> (H1) gas due to interactions with the other members of the clusters—most likely </span><a href="https://en.wikipedia.org/wiki/NGC_92" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="NGC 92">NGC 92</a><span style="color: #252525; text-align: start;">.</span><sup class="reference" id="cite_ref-Presotto2009_4-1" style="color: #252525; font-size: 11.2px; line-height: 1; text-align: start; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/NGC_89#cite_note-Presotto2009-4" style="background: none; color: #0b0080; text-decoration: none;">[4]</a></sup></span></span><br />
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<span style="background-color: white; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif; font-size: 14px;">https://en.wikipedia.org/wiki/NGC_89</span></span></div>
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<span style="background-color: white; font-size: 14px; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif;"><span style="color: #333333; font-size: 20px;">The largest member of the galaxy group known as Roberts Quartet is NGC 92, a spiral Sa galaxy with an unusual appearance.</span></span></span><br />
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<span style="background-color: white; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif; font-size: 14px;"><a href="https://en.wikipedia.org/wiki/Robert%27s_Quartet#/media/File:Phot-34b-05-fullres.jpg">https://en.wikipedia.org/wiki/Robert%27s_Quartet#/media/File:Phot-34b-05-fullres.jpg</a></span></span><br />
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<b>NGC 92</b> é uma <a href="https://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia">galáxia</a> <a href="https://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia espiral">espiral</a> (Sa) localizada na direcção da <a href="https://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="https://pt.wikipedia.org/wiki/Phoenix_(constela%C3%A7%C3%A3o)" style="background: none; color: #0b0080; text-decoration: none;" title="Phoenix (constelação)">Phoenix</a>. Possui uma declinação de -48° 37' 29" e uma <a class="mw-redirect" href="https://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 0 <a href="https://pt.wikipedia.org/wiki/Hora" style="background: none; color: #0b0080; text-decoration: none;" title="Hora">horas</a>, 21 <a href="https://pt.wikipedia.org/wiki/Minuto" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto">minutos</a> e 31,4 <a href="https://pt.wikipedia.org/wiki/Segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a>.</div>
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A galáxia <b>NGC 92</b> foi descoberta em <a class="mw-redirect" href="https://pt.wikipedia.org/wiki/30_de_Setembro" style="background: none; color: #0b0080; text-decoration: none;" title="30 de Setembro">30 de Setembro</a> de <a href="https://pt.wikipedia.org/wiki/1834" style="background: none; color: #0b0080; text-decoration: none;" title="1834">1834</a> por <a href="https://pt.wikipedia.org/wiki/John_Herschel" style="background: none; color: #0b0080; text-decoration: none;" title="John Herschel">John Herschel</a>.</div>
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<span style="color: #252525; font-family: sans-serif;">https://pt.wikipedia.org/wiki/NGC_92</span></div>
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<span style="background-color: white; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif;"><b style="color: #252525; text-align: start;">NGC 92</b><span style="color: #252525; text-align: start;"> is a highly warped interacting </span><a href="https://en.wikipedia.org/wiki/Unbarred_spiral_galaxy" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Unbarred spiral galaxy">unbarred spiral galaxy</a><span style="color: #252525; text-align: start;"> in </span><a href="https://en.wikipedia.org/wiki/Robert%27s_Quartet" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Robert's Quartet">Robert's Quartet</a><span style="color: #252525; text-align: start;">; it is interacting with three neighbouring galaxies </span><a href="https://en.wikipedia.org/wiki/NGC_87" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="NGC 87">NGC 87</a><span style="color: #252525; text-align: start;">, </span><a href="https://en.wikipedia.org/wiki/NGC_88" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="NGC 88">NGC 88</a><span style="color: #252525; text-align: start;"> and </span><a href="https://en.wikipedia.org/wiki/NGC_89" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="NGC 89">NGC 89</a><span style="color: #252525; text-align: start;">.</span></span></span><br />
<span style="background-color: white; line-height: 22.4px;"><span style="color: #252525; font-family: sans-serif;"><span style="text-align: start;">https://en.wikipedia.org/wiki/NGC_92</span></span></span><br />
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<b>NGC 625</b> é uma <a href="https://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia">galáxia</a> <a href="https://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral_barrada" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia espiral barrada">espiral barrada</a> (SBm) localizada na direcção da <a href="https://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="https://pt.wikipedia.org/wiki/Phoenix_(constela%C3%A7%C3%A3o)" style="background: none; color: #0b0080; text-decoration: none;" title="Phoenix (constelação)">Phoenix</a>. Possui uma declinação de -41° 26' 15" e uma <a class="mw-redirect" href="https://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 1 <a href="https://pt.wikipedia.org/wiki/Hora" style="background: none; color: #0b0080; text-decoration: none;" title="Hora">horas</a>, 35 <a href="https://pt.wikipedia.org/wiki/Minuto" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto">minutos</a> e 04,4 <a href="https://pt.wikipedia.org/wiki/Segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a>.</div>
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A galáxia NGC 625 foi descoberta em <a class="mw-redirect" href="https://pt.wikipedia.org/wiki/2_de_Setembro" style="background: none; color: #0b0080; text-decoration: none;" title="2 de Setembro">2 de Setembro</a> de <a href="https://pt.wikipedia.org/wiki/1826" style="background: none; color: #0b0080; text-decoration: none;" title="1826">1826</a> por <a href="https://pt.wikipedia.org/wiki/James_Dunlop" style="background: none; color: #0b0080; text-decoration: none;" title="James Dunlop">James Dunlop</a>.</div>
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<span style="color: #252525; font-family: sans-serif;"><a href="https://pt.wikipedia.org/wiki/NGC_625">https://pt.wikipedia.org/wiki/NGC_625</a></span></div>
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<span style="background-color: white; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif;"><b style="color: #252525; text-align: start;">NGC 625</b><span style="color: #252525; text-align: start;"> is a </span><a href="https://en.wikipedia.org/wiki/Dwarf_spiral_galaxy" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Dwarf spiral galaxy">dwarf</a><span style="color: #252525; text-align: start;"> </span><a href="https://en.wikipedia.org/wiki/Barred_spiral_galaxy" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Barred spiral galaxy">barred spiral galaxy</a><span style="color: #252525; text-align: start;"> about </span><a class="mw-redirect" href="https://en.wikipedia.org/wiki/1_E23_m" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="1 E23 m">12.7</a><span style="color: #252525; text-align: start;"> </span><a href="https://en.wikipedia.org/wiki/Light-year" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Light-year">Mly</a><span style="color: #252525; text-align: start;"> away in the </span><a href="https://en.wikipedia.org/wiki/Constellation" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Constellation">constellation</a><span style="color: #252525; text-align: start;"> </span><a href="https://en.wikipedia.org/wiki/Phoenix_(constellation)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Phoenix (constellation)">Phoenix</a><span style="color: #252525; text-align: start;">. NGC 625 is a member of the </span><a href="https://en.wikipedia.org/wiki/Sculptor_Group" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Sculptor Group">Sculptor Group</a><span style="color: #252525; text-align: start;">.</span><sup class="reference" id="cite_ref-Cannon_3-0" style="color: #252525; line-height: 1; text-align: start; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/NGC_625#cite_note-Cannon-3" style="background: none; color: #0b0080; text-decoration: none;">[3]</a></sup></span></span><br />
<span style="background-color: white; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif;"><a href="https://en.wikipedia.org/wiki/NGC_625">https://en.wikipedia.org/wiki/NGC_625</a></span></span><br />
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<span style="background-color: white; font-size: 14px; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif;"><img alt="NGC 625 GALEX.jpg" src="https://upload.wikimedia.org/wikipedia/commons/2/2f/NGC_625_GALEX.jpg" /></span></span></div>
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<span style="background-color: white; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif; font-size: 14px;">By WikiSky/GALEX/NASA - http://wikisky.org/snapshot?img_size=&img_res=&ra=1.5846388&de=-41.437219999999996&angle=0.3421532846715329&projection=tan&rotation=0.0&survey=GALEX&img_id=all&width=800&height=800&img_borders=&interpolation=bicubic&jpeg_quality=0.8&max_preview_size=800&show_params=1&mouse_action=zoom, Public Domain, https://commons.wikimedia.org/w/index.php?curid=5567839</span></span><br />
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<b>NGC 37</b> é uma <a href="https://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia">galáxia</a> <a href="https://pt.wikipedia.org/wiki/Gal%C3%A1xia_lenticular" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia lenticular">lenticular</a> (SB0) localizada na direcção da <a href="https://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="https://pt.wikipedia.org/wiki/Phoenix_(constela%C3%A7%C3%A3o)" style="background: none; color: #0b0080; text-decoration: none;" title="Phoenix (constelação)">Phoenix</a>. Possui uma declinação de -56° 57' 25" e uma <a class="mw-redirect" href="https://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 0 <a href="https://pt.wikipedia.org/wiki/Hora" style="background: none; color: #0b0080; text-decoration: none;" title="Hora">horas</a>, 11 <a href="https://pt.wikipedia.org/wiki/Minuto" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto">minutos</a> e 23,0 <a href="https://pt.wikipedia.org/wiki/Segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a>.</div>
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A galáxia <b>NGC 37</b> foi descoberta em <a class="mw-redirect" href="https://pt.wikipedia.org/wiki/2_de_Outubro" style="background: none; color: #0b0080; text-decoration: none;" title="2 de Outubro">2 de Outubro</a> de <a href="https://pt.wikipedia.org/wiki/1836" style="background: none; color: #0b0080; text-decoration: none;" title="1836">1836</a> por <a href="https://pt.wikipedia.org/wiki/John_Herschel" style="background: none; color: #0b0080; text-decoration: none;" title="John Herschel">John Herschel</a>.</div>
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<span style="color: #252525; font-family: sans-serif;">https://pt.wikipedia.org/wiki/NGC_37</span></div>
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<span style="background-color: white; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif;"><b style="color: #252525; text-align: start;">NGC 37</b><span style="color: #252525; text-align: start;"> is a </span><a href="https://en.wikipedia.org/wiki/Lenticular_galaxy" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Lenticular galaxy">lenticular galaxy</a><span style="color: #252525; text-align: start;"> located in the </span><a href="https://en.wikipedia.org/wiki/Phoenix_(constellation)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Phoenix (constellation)">Phoenix</a><span style="color: #252525; text-align: start;"> constellation. It is approximately 42 </span><a class="mw-redirect" href="https://en.wikipedia.org/wiki/Kiloparsecs" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Kiloparsecs">kiloparsecs</a><span style="color: #252525; text-align: start;"> (137,000 </span><a class="mw-redirect" href="https://en.wikipedia.org/wiki/Light-years" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start;" title="Light-years">light-years</a><span style="color: #252525; text-align: start;">) in diameter and about 12.9 </span><a href="https://en.wikipedia.org/wiki/Billion" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Billion">billion</a><span style="color: #252525; text-align: start;"> years old.</span><sup class="reference" id="cite_ref-NED_1-5" style="color: #252525; line-height: 1; text-align: start; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/NGC_37#cite_note-NED-1" style="background: none; color: #0b0080; text-decoration: none;">[1]</a></sup></span></span><br />
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<span style="background-color: white; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif; font-size: 14px;"><img height="640" src="https://upload.wikimedia.org/wikipedia/commons/6/6f/NGC_0037_2MASS.jpg" width="640" /></span></span><br />
<span style="background-color: white; line-height: 22.4px;"><span style="color: #073763; font-family: sans-serif; font-size: 14px;">Por Desconhecido - Two Micron All Sky Survey (2MASS)http://nedwww.ipac.caltech.edu/cgi-bin/nph-imgdata?objname=NGC+0037, Domínio público, https://commons.wikimedia.org/w/index.php?curid=3908540</span></span><br />
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<span style="background-color: white; line-height: 22.4px;"><span style="color: #660000; font-family: sans-serif;"><b>AGLOMERADOS DE GALÁXIAS,</b></span></span></div>
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<span style="background-color: white; line-height: 22.4px;"><span style="color: #660000; font-family: sans-serif;"><b>EM PHOENIX, O PÁSSARO FÊNIX</b></span></span><br />
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<span style="background-color: white; line-height: 22.4px;"><span style="color: #660000; font-family: sans-serif;"><span style="color: #333333; font-size: 20px;">Hubble image of ACT-CL J0102-4915</span></span></span><br />
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<span style="font-family: sans-serif;"><span style="background-color: white;">https://www.nasa.gov/mission_pages/chandra/multimedia/elgordo-2014.html</span></span></div>
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<span style="font-size: large;"><b>El Gordo</b> (lit. <i>The Fat One</i>) (<b>ACT-CL J0102-4915</b> or <b>SPT-CL J0102-4915</b>)</span> is the largest distant <a href="https://en.wikipedia.org/wiki/Galaxy_cluster" style="background: none; color: #0b0080; text-decoration: none;" title="Galaxy cluster">galaxy cluster</a> observed at its distance or beyond, as of 2011. As of 2014, it still holds the record for being the largest distant galaxy cluster to have been discovered with a mass of 3 quadrillion suns.<sup class="reference" id="cite_ref-3" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/El_Gordo_(galaxy_cluster)#cite_note-3" style="background: none; color: #0b0080; text-decoration: none;">[3]</a></sup><sup class="reference" id="cite_ref-NASA-20140416_4-0" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/El_Gordo_(galaxy_cluster)#cite_note-NASA-20140416-4" style="background: none; color: #0b0080; text-decoration: none;">[4]</a></sup><sup class="reference" id="cite_ref-5" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/El_Gordo_(galaxy_cluster)#cite_note-5" style="background: none; color: #0b0080; text-decoration: none;">[5]</a></sup><sup class="reference" id="cite_ref-6" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/El_Gordo_(galaxy_cluster)#cite_note-6" style="background: none; color: #0b0080; text-decoration: none;">[6]</a></sup> It was found by <a href="https://en.wikipedia.org/wiki/NASA" style="background: none; color: #0b0080; text-decoration: none;" title="NASA">NASA</a>'s <a href="https://en.wikipedia.org/wiki/Chandra_X-ray_Observatory" style="background: none; color: #0b0080; text-decoration: none;" title="Chandra X-ray Observatory">Chandra X-ray Observatory</a>, <a href="https://en.wikipedia.org/wiki/Atacama_Cosmology_Telescope" style="background: none; color: #0b0080; text-decoration: none;" title="Atacama Cosmology Telescope">Atacama Cosmology Telescope</a> - funded by <a href="https://en.wikipedia.org/wiki/National_Science_Foundation" style="background: none; color: #0b0080; text-decoration: none;" title="National Science Foundation">National Science Foundation</a>, and <a href="https://en.wikipedia.org/wiki/Very_Large_Telescope" style="background: none; color: #0b0080; text-decoration: none;" title="Very Large Telescope">European Southern Observatory's Very Large Telescope</a>.<sup class="reference" id="cite_ref-7" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/El_Gordo_(galaxy_cluster)#cite_note-7" style="background: none; color: #0b0080; text-decoration: none;">[7]</a></sup></div>
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This galaxy cluster, officially named as, 'ACT-CL J0102-4915', has been given a 'nickname' by the researchers as 'El Gordo', which stands for "the Fat One" or "the Big One" in <a href="https://en.wikipedia.org/wiki/Spanish_language" style="background: none; color: #0b0080; text-decoration: none;" title="Spanish language">Spanish</a>. It is located more than 7 billion <a href="https://en.wikipedia.org/wiki/Light-year" style="background: none; color: #0b0080; text-decoration: none;" title="Light-year">light-years</a> from <a href="https://en.wikipedia.org/wiki/Earth" style="background: none; color: #0b0080; text-decoration: none;" title="Earth">Earth</a>.<sup class="reference" id="cite_ref-8" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/El_Gordo_(galaxy_cluster)#cite_note-8" style="background: none; color: #0b0080; text-decoration: none;">[8]</a></sup></div>
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Felipe Menanteau (then of <a href="https://en.wikipedia.org/wiki/Rutgers_University" style="background: none; color: #0b0080; text-decoration: none;" title="Rutgers University">Rutgers University</a>) who led the study stated "this cluster is the most massive, the hottest, and gives off the most X-rays of any known cluster at this distance or beyond."<sup class="reference" id="cite_ref-10" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/El_Gordo_(galaxy_cluster)#cite_note-10" style="background: none; color: #0b0080; text-decoration: none;">[10]</a></sup></div>
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Findings from the <a href="https://en.wikipedia.org/wiki/Very_Large_Telescope" style="background: none; color: #0b0080; text-decoration: none;" title="Very Large Telescope">European Southern Observatory's Very Large Telescope</a> and the <a href="https://en.wikipedia.org/wiki/Chandra_X-ray_Observatory" style="background: none; color: #0b0080; text-decoration: none;" title="Chandra X-ray Observatory">Chandra X-ray Observatory</a> show that El Gordo is composed of two separate <a href="https://en.wikipedia.org/wiki/Galaxy_groups_and_clusters" style="background: none; color: #0b0080; text-decoration: none;" title="Galaxy groups and clusters">galaxy subclusters</a>, colliding at several million kilometers per hour.<sup class="reference" id="cite_ref-11" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/El_Gordo_(galaxy_cluster)#cite_note-11" style="background: none; color: #0b0080; text-decoration: none;">[11]</a></sup> These observations (using X-ray data and other characteristics) suggest that 'El Gordo' most probably formed in the same manner as the <a href="https://en.wikipedia.org/wiki/Bullet_Cluster" style="background: none; color: #0b0080; text-decoration: none;" title="Bullet Cluster">Bullet Cluster</a> (which is located 4 billion <a href="https://en.wikipedia.org/wiki/Light-year" style="background: none; color: #0b0080; text-decoration: none;" title="Light-year">light years</a> from <a href="https://en.wikipedia.org/wiki/Earth" style="background: none; color: #0b0080; text-decoration: none;" title="Earth">Earth</a>).<sup class="reference" id="cite_ref-12" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/El_Gordo_(galaxy_cluster)#cite_note-12" style="background: none; color: #0b0080; text-decoration: none;">[12]</a></sup><sup class="reference" id="cite_ref-13" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/El_Gordo_(galaxy_cluster)#cite_note-13" style="background: none; color: #0b0080; text-decoration: none;">[13]</a></sup><sup class="reference" id="cite_ref-14" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/El_Gordo_(galaxy_cluster)#cite_note-14" style="background: none; color: #0b0080; text-decoration: none;">[14]</a></sup><sup class="reference" id="cite_ref-15" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/El_Gordo_(galaxy_cluster)#cite_note-15" style="background: none; color: #0b0080; text-decoration: none;">[15]</a></sup> According to Cristóbal Sifón from <a href="https://en.wikipedia.org/wiki/Pontifical_Catholic_University_of_Chile" style="background: none; color: #0b0080; text-decoration: none;" title="Pontifical Catholic University of Chile">Pontifical Catholic University of Chile</a> "this is the first time we've found a system like the <a href="https://en.wikipedia.org/wiki/Bullet_Cluster" style="background: none; color: #0b0080; text-decoration: none;" title="Bullet Cluster">Bullet Cluster</a> at such a large distance."<sup class="reference" id="cite_ref-16" style="line-height: 1; unicode-bidi: isolate; white-space: nowrap;"><a href="https://en.wikipedia.org/wiki/El_Gordo_(galaxy_cluster)#cite_note-16" style="background: none; color: #0b0080; text-decoration: none;">[16]</a></sup></div>
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<span style="color: #252525; font-family: sans-serif;"><a href="https://en.wikipedia.org/wiki/El_Gordo_(galaxy_cluster)">https://en.wikipedia.org/wiki/El_Gordo_(galaxy_cluster)</a></span></div>
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<span style="background-color: white; line-height: 22.4px;"><span style="color: #660000; font-family: sans-serif;"><a href="https://commons.wikimedia.org/w/index.php?title=File%3AEl_Gordo.ogv" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #666666; font-size: 14px; text-align: left;" title="El Gordo.ogv"><img border="0" src="https://upload.wikimedia.org/wikipedia/commons/thumb/a/a0/El_Gordo.ogv/800px--El_Gordo.ogv.jpg" style="border: none; float: left; height: 67px; margin: 4px; vertical-align: middle; width: 120px;" /></a></span></span><br />
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Title: <a href="https://commons.wikimedia.org/w/index.php?title=File%3AEl_Gordo.ogv" style="background: none; color: #666666;" title="El Gordo.ogv">El Gordo.ogv</a><br />
Author: ESO/SOAR/NASA<br />
Date: <span style="white-space: nowrap;">10 January 2012</span></div>
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<span style="background-color: white; line-height: 22.4px;"><span style="color: #660000; font-family: sans-serif;"><a href="https://en.wikipedia.org/wiki/File:El_Gordo.ogv">https://en.wikipedia.org/wiki/File:El_Gordo.ogv</a></span></span></div>
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A composite X-ray (purple), optical (red/green/blue), and UV (blue) image of the newly discovered Phoenix Cluster. This galaxy cluster has been dubbed the Phoenix Cluster because it is located in the constellation of the Phoenix, and because new stars are forming there at the highest rate ever observed in a cluster.</div>
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X-ray: NASA/CXC/MIT/M.McDonald; UV: NASA/JPL-Caltech/M.McDonald; Optical: AURA/NOAO/CTIO/MIT/M.McDonald; Illustration: NASA/CXC/M.Weiss</div>
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<span style="color: #999999; font-family: "tahoma" , "arial" , "verdana" , sans-serif;"><span style="line-height: 18px;"><a href="http://www.cfa.harvard.edu/news/su201233">http://www.cfa.harvard.edu/news/su201233</a></span></span></div>
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CfA astronomers Ryan Foley, Matt Ashby, Bill Forman, Steve Murray, Brian Stalder, Tony Stark, Chris Stubbs, and Alex Vikhlinin are part of a team of astronomers who have discovered one of the largest and most luminous <a class="textTag" href="http://phys.org/tags/galaxy+clusters/" rel="tag" style="color: #313d57; outline: 0px;">galaxy clusters</a> in the universe, the so-called Phoenix Cluster, about 5.7 billion light-years away. Using the Chandra X-Ray Observatory, the Magellan telescopes in Chile, the South Pole Telescope in Antarctica, and a suite of other space and ground-based facilities, the team finds that the cluster (at least currently) is undergoing a massive burst of star formation with about 740 solar-masses worth of new stars being created every year (for reference, the Milky Way forms about one star per year).</div>
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This was unexpected: most clusters support only modest star formation. At the same time, the team finds that the dominant black hole in the cluster does not show especially powerful jet activity. Writing in last week's issue of the journal <i style="margin: 0px; padding: 0px;">Nature</i>, the team concludes that this massive starburst is powered by the infalling material. They speculate that in this cluster the dominant black hole, although steadily growing in mass, has jets that are unable to halt the "cooling flow." The implication is that either this cluster is of a very rare kind, or that with subsequent evolution it will develop more effective and customary ways to inhibit the infalling material.</div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Read more at: </span><a href="http://phys.org/news/2012-08-super-cluster-galaxies.html#jCp">http://phys.org/news/2012-08-super-cluster-galaxies.html#jCp</a></div>
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<span style="font-size: large;">The <b>Phoenix Cluster</b> (SPT-CL J2344-4243)</span> is a <a href="http://en.wikipedia.org/wiki/Galaxy_cluster" style="background: none; color: #0b0080; text-decoration: none;" title="Galaxy cluster">galaxy cluster</a> located in the <a href="http://en.wikipedia.org/wiki/Phoenix_(constellation)" style="background: none; color: #0b0080; text-decoration: none;" title="Phoenix (constellation)">constellation Phoenix</a>, at a distance of roughly 5.7 billion light years. It has a mass of 2.5<span style="margin: 0px 0.15em 0px 0.25em;">×</span>10<sup style="line-height: 1;">15</sup> <a href="http://en.wikipedia.org/wiki/Solar_mass" style="background: none; color: #0b0080; text-decoration: none;" title="Solar mass">solar masses</a>, making it one of the most massive galaxy clusters.<sup class="reference" id="cite_ref-NATURE_2-2" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Phoenix_Cluster#cite_note-NATURE-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup></div>
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Possibly dormant for billions of years, it has recently revealed a high rate of activity in <a href="http://en.wikipedia.org/wiki/Star_formation" style="background: none; color: #0b0080; text-decoration: none;" title="Star formation">star formation</a> – the highest ever recorded in the middle of a galaxy cluster, although there are many individual high redshift galaxies which produce this many stars per year, or more. <sup class="reference" id="cite_ref-arXiv-1109.6286_4-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Phoenix_Cluster#cite_note-arXiv-1109.6286-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[4]</a></sup> Observations by a variety of telescopes including the <a href="http://en.wikipedia.org/wiki/GALEX" style="background: none; color: #0b0080; text-decoration: none;" title="GALEX">GALEX</a> and<a href="http://en.wikipedia.org/wiki/Herschel_Space_Observatory" style="background: none; color: #0b0080; text-decoration: none;" title="Herschel Space Observatory">Herschel</a> space telescopes show a creation of 740 solar masses (stars) per year.<sup class="reference" id="cite_ref-NATURE_2-3" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Phoenix_Cluster#cite_note-NATURE-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup> This is considerably higher than the <a href="http://en.wikipedia.org/wiki/Perseus_Cluster" style="background: none; color: #0b0080; text-decoration: none;" title="Perseus Cluster">Perseus Cluster</a>, where stars are formed around 20 times slower, or the one per year rate of star formation in our own galaxy.<sup class="reference" id="cite_ref-APrdmag_5-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Phoenix_Cluster#cite_note-APrdmag-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[5]</a></sup></div>
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Phoenix Cluster is also producing more <a href="http://en.wikipedia.org/wiki/X-ray" style="background: none; color: #0b0080; text-decoration: none;" title="X-ray">X-rays</a> than any other known massive cluster.<sup class="reference" id="cite_ref-NATURE_2-4" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Phoenix_Cluster#cite_note-NATURE-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup> Data from observations suggest that hot gas is cooling in the central regions at the highest rate ever recorded. The central galaxy in the cluster contains vast amounts of hot gas. More normal matter is present there than the total of all the other galaxies in the cluster.</div>
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In the center of the system, there is a <a href="http://en.wikipedia.org/wiki/Supermassive_black_hole" style="background: none; color: #0b0080; text-decoration: none;" title="Supermassive black hole">supermassive black hole</a> growing very rapidly, expanding at a rate of about 60 solar masses per year. It is currently about 20 billion times the mass of the Sun, one of the <a href="http://en.wikipedia.org/wiki/List_of_most_massive_black_holes" style="background: none; color: #0b0080; text-decoration: none;" title="List of most massive black holes">largest known</a>.<sup class="reference" id="cite_ref-NATURE_2-5" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Phoenix_Cluster#cite_note-NATURE-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup></div>
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The Phoenix Cluster was initially detected using the <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Sunyaev-Zeldovich_effect" style="background: none; color: #0b0080; text-decoration: none;" title="Sunyaev-Zeldovich effect">Sunyaev-Zeldovich effect</a> by the <a href="http://en.wikipedia.org/wiki/South_Pole_Telescope" style="background: none; color: #0b0080; text-decoration: none;" title="South Pole Telescope">South Pole Telescope</a> collaboration.<sup class="reference" id="cite_ref-arXiv-1101.1290_3-1" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Phoenix_Cluster#cite_note-arXiv-1101.1290-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[3]</a></sup></div>
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<span class="mw-mmv-author" original-title="Author" style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; font-size: 16px; line-height: 24px; white-space: nowrap;">Richard Powell</span><span style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; font-size: 16px; line-height: 24px; white-space: nowrap;"> - </span><span class="mw-mmv-source" original-title="Source" style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; font-size: 16px; line-height: 24px; white-space: nowrap;"><a class="external free" href="http://www.atlasoftheuniverse.com/nearsc.html" rel="nofollow" style="background: none; color: #0b0080;">http://www.atlasoftheuniverse.com/nearsc.html</a></span></div>
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<span lang="EN-US" style="font-family: "arial" , sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">A2870 01 07.7 -46 55 251.0 -13.5 0 .0225 311 Phoenix<o:p></o:p></span></span></div>
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<span lang="EN-US" style="font-family: "arial" , sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">A2877 01 09.8 -45 54 252.1 -13.8 0 .0235 324 Phoenix<o:p></o:p></span></span></div>
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<span lang="EN-US" style="font-family: "arial" , sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">A2806 00 40.2 -56 10 240.9 -11.0 0 .0265 365 Phoenix<o:p></o:p></span></span></div>
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<span lang="EN-US" style="font-family: "arial" , sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">A2836 00 53.7 -47 37 249.9 -11.3 0 .0288 397 Phoenix<o:p></o:p></span></span></div>
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<span lang="EN-US" style="font-family: "arial" , sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">A2731 00 10.2 -56 59 239.1 -7.2 0 .0300 413 Phoenix<o:p></o:p></span></span></div>
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<span lang="EN-US" style="font-family: "arial" , sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;">A2896 01 18.3 -37 06 261.3 -14.0 0 .0306 421 Phoenix<o:p></o:p></span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj0j6JtLVEyO58nGSgo6qJH95AfYd3TQHwyfkWm6aj8hH4RiPnorI1fyKeVwc1ZXPeyyGEjEnlC51i6Cfv23yZ9F_28YxECROL0yLK9luFxTlNk7bAXEIB8q21oUcL48LUpLJCuF4M7skg/s1600/Phoenix_rising_from_its_ashes.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><span style="color: #073763;"><img border="0" height="640" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj0j6JtLVEyO58nGSgo6qJH95AfYd3TQHwyfkWm6aj8hH4RiPnorI1fyKeVwc1ZXPeyyGEjEnlC51i6Cfv23yZ9F_28YxECROL0yLK9luFxTlNk7bAXEIB8q21oUcL48LUpLJCuF4M7skg/s1600/Phoenix_rising_from_its_ashes.jpg" width="558" /></span></a></div>
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<span style="color: #073763;"><span style="color: #660000; font-family: sans-serif; font-size: large; line-height: 22.4px;">A </span><span class="no-conversion" style="font-family: sans-serif; line-height: 22.4px;"><b><span lang="pt-br" style="color: #660000; font-size: large;" xml:lang="pt-br">fênix</span></b><span style="color: #073763;"> </span><span style="bottom: 1ex; color: #073763; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">(<a href="http://pt.wikipedia.org/wiki/Portugu%C3%AAs_brasileiro" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Português brasileiro">português brasileiro</a>)</span><span style="color: #073763;"> ou </span><b style="color: #073763;"><span lang="pt-pt" xml:lang="pt-pt">fénix</span></b><span style="color: #073763;"> </span><span style="bottom: 1ex; color: #073763; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">(<a href="http://pt.wikipedia.org/wiki/Portugu%C3%AAs_europeu" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Português europeu">português europeu</a>)</span></span><span style="color: #073763; font-family: sans-serif; line-height: 22.4px;"> (em </span><a href="http://pt.wikipedia.org/wiki/L%C3%ADngua_grega_antiga" style="background-image: none; color: #073763; font-family: sans-serif; line-height: 22.4px; text-decoration: none;" title="Língua grega antiga">grego clássico</a><span style="color: #073763; font-family: sans-serif; line-height: 22.4px;">: </span><span class="politonico" lang="el" style="color: #073763; font-family: "athena unicode" , "gentium" , "palatino linotype" , "arial unicode ms" , "lucida sans unicode" , "lucida grande" , "code2000"; line-height: 22.4px;" xml:lang="el">ϕοῖνιξ</span><span style="color: #073763; font-family: sans-serif; line-height: 22.4px;">) é um pássaro da </span><a href="http://pt.wikipedia.org/wiki/Mitologia_grega" style="background-image: none; color: #073763; font-family: sans-serif; line-height: 22.4px; text-decoration: none;" title="Mitologia grega">mitologia grega</a><span style="color: #073763; font-family: sans-serif; line-height: 22.4px;"> que, quando morria, entrava em auto-combustão e, passado algum tempo, renascia das próprias cinzas.</span></span></div>
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<b><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;">No final de cada ciclo de vida, a fênix queimava-se numa </span><a href="http://pt.wikipedia.org/wiki/Pira" style="background-image: none; color: #0b0080; font-family: sans-serif; line-height: 22.4px; text-decoration: none;" title="Pira">pira</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"> funerária. A vida longa da fênix e o seu dramático renascimento das próprias cinzas transformaram-na em símbolo da </span><a href="http://pt.wikipedia.org/wiki/Imortalidade" style="background-image: none; color: #0b0080; font-family: sans-serif; line-height: 22.4px; text-decoration: none;" title="Imortalidade">imortalidade</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"> e do renascimento espiritual.</span></b></div>
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<li style="margin-bottom: 0.1em;">A crença na ave lendária que renasce das próprias cinzas existiu em vários povos da <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Antiguidade" style="background: none; color: #0b0080; text-decoration: none;" title="Antiguidade">Antiguidade</a> como gregos, egípcios e chineses. Em todas as mitologias o significado é preservado: a perpetuação, a ressurreição, a esperança que nunca têm fim.</li>
<li style="margin-bottom: 0.1em;">Para os gregos, a fênix por vezes estava ligada ao deus <a href="http://pt.wikipedia.org/wiki/Hermes" style="background: none; color: #0b0080; text-decoration: none;" title="Hermes">Hermes</a> e é representada em muitos templos antigos. Há um paralelo da fênix com o Sol, que morre todos os dias no horizonte para renascer no dia seguinte, tornando-se o eterno símbolo da morte e do renascimento da natureza.</li>
<li style="margin-bottom: 0.1em;">Os egípcios a tinham por "Bennu" e estava relacionada a <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a> "Sótis", ou estrela de cinco pontas, estrela flamejante, que é pintada ao seu lado.</li>
<li style="margin-bottom: 0.1em;">Na <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/China" style="background: none; color: #0b0080; text-decoration: none;" title="China">China</a> antiga a fênix foi representada como uma ave maravilhosa e transformada em símbolo da <a href="http://pt.wikipedia.org/wiki/Felicidade" style="background: none; color: #0b0080; text-decoration: none;" title="Felicidade">felicidade</a>, da <a href="http://pt.wikipedia.org/wiki/Virtude" style="background: none; color: #0b0080; text-decoration: none;" title="Virtude">virtude</a>, da força, da liberdade, e da <a href="http://pt.wikipedia.org/wiki/Intelig%C3%AAncia" style="background: none; color: #0b0080; text-decoration: none;" title="Inteligência">inteligência</a>. Na sua<a href="http://pt.wikipedia.org/wiki/Plumagem" style="background: none; color: #0b0080; text-decoration: none;" title="Plumagem">plumagem</a>, brilham as cinco cores sagradas.<a href="http://pt.wikipedia.org/wiki/P%C3%BArpura" style="background: none; color: #0b0080; text-decoration: none;" title="Púrpura">Púrpura</a>, <a href="http://pt.wikipedia.org/wiki/Azul" style="background: none; color: #0b0080; text-decoration: none;" title="Azul">azul</a>, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Vermelha" style="background: none; color: #0b0080; text-decoration: none;" title="Vermelha">vermelha</a>, <a href="http://pt.wikipedia.org/wiki/Branco" style="background: none; color: #0b0080; text-decoration: none;" title="Branco">branco</a> e <a href="http://pt.wikipedia.org/wiki/Dourado_(cor)" style="background: none; color: #0b0080; text-decoration: none;" title="Dourado (cor)">dourado</a>.</li>
<li style="margin-bottom: 0.1em;">No início da era Cristã esta ave fabulosa foi símbolo do renascimento e da ressurreição. Neste sentido, ela simboliza o Cristo ou o <a href="http://pt.wikipedia.org/wiki/Iniciado" style="background: none; color: #0b0080; text-decoration: none;" title="Iniciado">Iniciado</a>, recebendo uma segunda vida, em troca daquela que sacrificou.</li>
<li style="margin-bottom: 0.1em;">A bandeira da cidade de <a href="http://pt.wikipedia.org/wiki/S%C3%A3o_Francisco_(Calif%C3%B3rnia)" style="background: none; color: #0b0080; text-decoration: none;" title="São Francisco (Califórnia)">São Francisco</a> mostra uma fênix, acreditado de estar um símbolo de renovação depois o <a href="http://pt.wikipedia.org/wiki/Sismo_de_S%C3%A3o_Francisco_de_1906" style="background: none; color: #0b0080; text-decoration: none;" title="Sismo de São Francisco de 1906">sismo que devastou a cidade em 1906</a>. A bandeira e o selo da cidade de <a href="http://pt.wikipedia.org/wiki/Atlanta" style="background: none; color: #0b0080; text-decoration: none;" title="Atlanta">Atlanta</a> mostram uma fênix também.</li>
<li style="margin-bottom: 0.1em;">No <a href="http://pt.wikipedia.org/wiki/Acidente_na_mina_San_Jos%C3%A9_em_2010" style="background: none; color: #0b0080; text-decoration: none;" title="Acidente na mina San José em 2010">Acidente na mina San José em 2010</a>, a cápsula que estava retirando um por um dos 33 mineiros foi chamada de Fênix, porque o resgate deles a uma profundidade muito funda de terra lembra a ressurreição da ave mítica das cinzas.</li>
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<span style="font-family: "arial" , sans-serif;">http://www.raremaps.com/gallery/enlarge/33613</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">http://www.raremaps.com/gallery/detail/33613/Celestial_Map_of_the_Southern_Hemisphere/Pardies.html</span><br />
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<strong>Title: </strong>[Celestial Map of the Southern Hemisphere] <strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/3418" style="border-bottom: 0px solid rgb(255, 255, 255); color: #274e13; text-decoration: none;">Ignace Gaston Pardies</a></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>Os desenhos formados pelas estrelas </b></span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>– As Constelações - </b></span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, </b></span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>entre o céu e a terra </b></span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>bem como percebendo que o caos, vagarosamente, </b></span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>vai se tornando Cosmos e sendo por nossa mente conscientizado. </b></span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>Quer dizer, </b></span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>COM UM ABRAÇO ESTRELADO,<o:p></o:p></b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>Janine Milward</b></span></div>
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<span style="background-color: white; color: #073763;"><b><span lang="PT" style="font-family: "arial" , sans-serif; font-size: 12pt;">Da Terra ao Céu<o:p></o:p></span></b></span></div>
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<span style="background-color: white; color: #073763;"><b><span lang="PT" style="font-family: "arial" , sans-serif; font-size: 12pt;"> e ao Infinito</span></b><span style="font-family: "arial" , sans-serif; font-size: 12pt;"><o:p></o:p></span></span></div>
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<span lang="PT" style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Constelações, Estrelas e Objetos Celestes<o:p></o:p></span></span></div>
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<span lang="PT" style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">(sob o ponto de vista do Mundo Ocidental)<o:p></o:p></span></span></div>
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<span lang="PT" style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Suas histórias, seus mitos, seus significados e suas sintetizadas descrições<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="PT" style="font-family: "arial" , sans-serif;">Reunião das Informações e Compilação,</span><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="PT" style="font-family: "arial" , sans-serif;">Tradução para a língua portuguesa (em alguns momentos)</span><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="PT" style="font-family: "arial" , sans-serif;">bem como Comentários Pessoais:</span><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><i><span lang="PT" style="font-family: "arial" , sans-serif;">Janine Milward</span></i></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: "arial" , sans-serif;">Visitando os Sites abaixo,</span><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: "arial" , sans-serif;"> você conseguirá informações atualizadas e preciosas</span><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: "arial" , sans-serif;">sobre os Objetos Celestiais de seu interesse:</span><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: "arial" , sans-serif;">NASA/IPAC</span><span style="font-family: "arial" , sans-serif;"> EXTRAGALACTIC DATABASE –</span><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://ned.ipac.caltech.edu/"><span style="font-family: "arial" , sans-serif;">http://ned.ipac.caltech.edu/</span></a><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://ned.ipac.caltech.edu/forms/byname.html"><span style="font-family: "arial" , sans-serif;">http://ned.ipac.caltech.edu/forms/byname.html</span></a><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><em><span lang="EN-US" style="font-family: "arial" , sans-serif;">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US" style="font-family: "arial" , sans-serif;"> </span></i></span><em><span lang="EN-US" style="font-family: "arial" , sans-serif;"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US" style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://www.nightskyatlas.com/index.jsp"><span lang="EN-US" style="font-family: "arial" , sans-serif;">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US" style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span lang="EN-US" style="font-family: "arial" , sans-serif;">The</span><span class="apple-converted-space"><span lang="EN-US" style="font-family: "arial" , sans-serif;"> </span></span><span lang="EN-US" style="font-family: "arial" , sans-serif;">Internet STELLAR DATABASE</span><span lang="EN-US" style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><a href="http://www.stellar-database.com/"><span lang="EN-US" style="font-family: "arial" , sans-serif;">http://www.stellar-database.com/</span></a><span lang="EN-US" style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<o:p></o:p></span></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-3301818565207114772013-08-20T08:01:00.001-07:002014-11-10T08:05:41.850-08:00PERSEUS, O CAMPEÃO<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Herói Perseus e seu troféu, a Cabeça da Medusa</b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b> sendo representada (o olho) pela estrela-beta Persei, Algol!</b></span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgiU6knCW8Sw81-gcoZhNOJzqRxCvo7iVqlX_NvwYaYsLhlV4FKh44A1qDe96vaZgHyOe1cq7tbaWXyRbsGCdI4cFmDzbli9LUjYEz9rpKhBd34r9psNlucudR9RTD9wm77Y28ENByjB3I/s1600/450px-medusaPersus_by_Antonio_Canova_-_Vatican.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgiU6knCW8Sw81-gcoZhNOJzqRxCvo7iVqlX_NvwYaYsLhlV4FKh44A1qDe96vaZgHyOe1cq7tbaWXyRbsGCdI4cFmDzbli9LUjYEz9rpKhBd34r9psNlucudR9RTD9wm77Y28ENByjB3I/s1600/450px-medusaPersus_by_Antonio_Canova_-_Vatican.jpg" height="423" width="640" /></a></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Ficheiro:Persus_by_Antonio_Canova_-_Vatican.jpg</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="fn" id="creator" style="line-height: 19.2000007629395px; text-align: left;"><bdi><a class="extiw" href="http://pt.wikipedia.org/wiki/Antonio_Canova" style="background-image: none; text-decoration: none;" title="pt:Antonio Canova">Antonio Canova</a></bdi></span><span style="line-height: 19.2000007629395px; text-align: left;"> (1757–1822) </span></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Excerto: Perseu com a cabeça da Medusa</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sabemos que o salvamento de Andromeda, a Princesa Acorrentada,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">de seu destino cruel </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(o de ser devorada pelo monstro-marinho, Cetus),</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">foi realizado pelo herói e campeão Perseus</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">que chegou na ilha </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(onde a donzela encontrava-se acorrentada a uma imensa pedra)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> montado em Pegasus, o cavalo alado,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> e trazendo consigo </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">a cabeça decepada da Medusa, a Gorgona</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- cujo olhar (ainda vivo) transformava em pedra a tudo e a todos que a fitavam.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Perseus salvou Andromeda </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e mostrou a cara da Medusa a Cetus </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- que petrificou-se.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Perseus e Andromeda casaram-se e foram felizes</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> para (quase) todo o sempre.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Nos céus estrelados do norte,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">a constelação de Perseus encerra este Mito</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(após Cepheus, Cassiopea, Pegasus e Andromeda e Peixes e Cetus)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e, certamente, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">este término mostra-se intensamente contundente</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">através da figura considerada incrível e medonha e amedrontadora</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">de ALGOL, estrela-beta Persei,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">o olho esquerdo da Medusa </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">- cuja cabeça ainda viva Perseus segura</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">por secula seculorom, ad infinitum, para todo o sempre...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 22.3999996185303px;">http://www.stellarium.org/pt/</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><img alt="The Perseus Cluster (Abell 426)" src="http://annesastronomynews.com/wp-content/uploads/2012/02/The-Perseus-Cluster-Abell-426-contains-thousands-of-galaxies-immersed-in-a-vast-cloud-of-multimillion-degree-gas.-Near-the-cluster-center-237-million-ly-away-is-the-clusters-dominant-galaxy-NGC-1275.jpg" /></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><a href="http://annesastronomynews.com/photo-gallery-ii/galaxies-clusters/the-perseus-cluster-abell-426-contains-thousands-of-galaxies-immersed-in-a-vast-cloud-of-multimillion-degree-gas-near-the-cluster-center-237-million-ly-away-is-the-clusters-dominant-galaxy-ngc/">http://annesastronomynews.com/photo-gallery-ii/galaxies-clusters/the-perseus-cluster-abell-426-contains-thousands-of-galaxies-immersed-in-a-vast-cloud-of-multimillion-degree-gas-near-the-cluster-center-237-million-ly-away-is-the-clusters-dominant-galaxy-ngc/</a></span><br />
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">The Perseus Cluster (</span><span style="font-family: Arial, Helvetica, sans-serif;">Abell 426</span><span style="font-family: Arial, Helvetica, sans-serif;">)</span></span></div>
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<a href="http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_004.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_004.jpg</span></a><br />
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<tr><td style="text-align: center;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj0QZijBSrOPf6nfu1Cb2_x1NqHJQYgJtIEc1F4T1MmbTSxatemxQl7Q_-jOo8Bin9-eq_EbRTiVYr-zucREFc9c7uaYuUWGAx4tzJ0Z-1Q6M3QIoGhF-J7IFfy7-Ve13m9s6LLAQ5BVUOR/s1600/PERSEUS.JPG" imageanchor="1" style="margin-left: auto; margin-right: auto;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj0QZijBSrOPf6nfu1Cb2_x1NqHJQYgJtIEc1F4T1MmbTSxatemxQl7Q_-jOo8Bin9-eq_EbRTiVYr-zucREFc9c7uaYuUWGAx4tzJ0Z-1Q6M3QIoGhF-J7IFfy7-Ve13m9s6LLAQ5BVUOR/s1600/PERSEUS.JPG" /></span></a></td></tr>
<tr><td class="tr-caption" style="text-align: center;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></td></tr>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">PERSEUS, O CAMPEÃO</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 1h26m / 4h46m
Declinação +30<sup>o</sup>.9 / +58<sup>o</sup>.9<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Mito:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Perseus, era filho de Júpiter e Danae, portanto, um semideus a
quem Mercúrio deu de presente espada, capa e asas nos pés e também o escudo
pertencente à Minerva. O herói matou a
Medusa ao cortar sua cabeça e mais tarde, salvou Andrômeda, com quem se casou e
teve alguns filhos. Quando retornava para
sua casa, ele matou acidentalmente seu próprio avô e endoideceu de tanta dor,
mas Júpiter apiedou-se dele e o colocou entre as estrelas.<o:p></o:p></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">6a. Edição do Atlas Celeste</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986 </span></div>
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<tr><td class="tr-caption"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Stellarium 0.11.1 (para a latitude 21s52 e longitude 43w00) - www.stellarium.org<br />trabalhado no Corel Photo-Paint X3 </span></td></tr>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>SAIBA MAIS SOBRE O MITO </b></span><br />
<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>DE PERSEUS E ANDROMEDA</b></span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj4vTAz_UY2k1TsORmkzXzHibUs97w4idZViSR-9SfYq30pkZfkKxTaFiNU2Hkvl4KVDUa2QWcD_U7bL0ICZYSoUa6T1aGcpQW9CpHE4jqu7z4eBZbN3x86icDyLEMjyGgQYkVSaB08ZU0/s1600/36137.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj4vTAz_UY2k1TsORmkzXzHibUs97w4idZViSR-9SfYq30pkZfkKxTaFiNU2Hkvl4KVDUa2QWcD_U7bL0ICZYSoUa6T1aGcpQW9CpHE4jqu7z4eBZbN3x86icDyLEMjyGgQYkVSaB08ZU0/s1600/36137.jpg" /></a></div>
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/36137/Andromede_Persee_Le_Triangle_Andromeda_Perseus_and_Triangle/Flamsteed-Fortin.html</span></span><br />
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Title: </strong>Andromede, Persee, Le Triangle (Andromeda, Perseus & Triangle)</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1260" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">John Flamsteed</a> / <a href="https://www.raremaps.com/gallery/browse/creator_id/1454" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">MJ Fortin</a></span></span></div>
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<b><span style="background-color: white;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">AS CONSTELAÇÕES QUE FAZEM PARTE</span></span></b></div>
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<span style="background-color: white;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b> DO MITO DE ANDROMEDA E PERSEUS</b></span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhAdCACSPijNrn5v_OxgXj-6MoQ2YeqVNu6DT3L2WUcUV9ZDfYcB7TV8n7hzXGu695nZ-nsYfDJ6LFXY_PLpjMGn2EPDkP9GK5SeOV6juipkHPeu7DlcGfawG8NEu7F0EcwRCbTSLPeV3oE/s1600/andromeda,+perseus+-+guido+reni+-+1635.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhAdCACSPijNrn5v_OxgXj-6MoQ2YeqVNu6DT3L2WUcUV9ZDfYcB7TV8n7hzXGu695nZ-nsYfDJ6LFXY_PLpjMGn2EPDkP9GK5SeOV6juipkHPeu7DlcGfawG8NEu7F0EcwRCbTSLPeV3oE/s640/andromeda,+perseus+-+guido+reni+-+1635.jpg" height="640" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="512" /></span></span></a></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Andromeda e Perseus - Guido Reni, 1635</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>A Constelação dos Peixes</b></span></span><br />
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">É neste cenário - nos mares dos Peixes - que podemos encontrar a Ilha</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">onde Andromeda está amarrada às pedras e sendo ameaçada</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">pelo Monstro Marinho, Cetus, a Baleia.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/enlarge/36551</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Title: </strong>Les Poissons (Pisces) <strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1260" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">John Flamsteed</a> / <a href="https://www.raremaps.com/gallery/browse/creator_id/1454" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">MJ Fortin</a></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/36551/Les_Poissons_Pisces/Flamsteed-Fortin.html</span></span></div>
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<span style="background-color: white;"><b><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A constelação de Andromeda, a Princesa Acorrentada</span></b></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Andrômeda era a filha de Cefeus, rei da Etiópia, e de Cassiopeia. Por causa dos boatos espalhados por Cassiopéia de que a beleza de Andrômeda superava a das Nereidas, Netuno enviou um mostro marinho, Cetus, a Baleia, para devastar aquele país. Porém, Netuno fez a promessa de libertar o país dessa devastação caso Andromeda fosse oferecida em sacrifício, sendo acorrentada a uma rocha, para ser devorada pelo monstro marinho. No entanto, Perseus soube desse caso e salvou Andrômeda de seu tormento matando o monstro e o transformando em pedra ao lhe mostrar a cara da Medusa. Ambos, Perseus e Andrômeda, alçaram vôo alto, sobre Pegasus, o cavalo alado, e se dirigiram para o altar onde se casaram.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://www.raremaps.com/maps/medium/33014op.jpg" height="296" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="400" /><br /><a href="http://www.raremaps.com/gallery/detail/33014op/Andromeda/Bayer.html" style="text-decoration: none;"></a></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Johann Bayer — Andromeda</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.aradergalleries.com/detail.php?id=3623</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>A constelação de Perseus</b>, <b>o Herói e Campeão</b><o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Perseus, era filho de júpiter e Danae, portanto, um semideus a quem Mercúrio deu de presente espada, capa e asas nos pés e também o escudo pertencente à Minerva. O herói matou a Medusa ao cortar sua cabeça e mais tarde, salvou Andrômeda, com quem se casou e teve alguns filhos. Quando retornava para sua casa, ele matou acidentalmente seu próprio avô e endoideceu de tanta dor, mas Júpiter apiedou-se dele e o colocou entre as estrelas.<o:p></o:p></span></span></div>
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<span style="background-color: white; margin-left: 1em; margin-right: 1em;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgicSZSSiQI1DqmMfHiQntj7FRonWt0fa2Ku_dZsOdvUQi2Yfuyk3bQUPE5fPNAHAKUo-crQAxIu0lUBIv_u4m0dlkioa9N-aQRFsQurRhbnbQIHCCDb28vBwBoz6FL84cnJiO7KJsJO-zq/s1600/br_perseus.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgicSZSSiQI1DqmMfHiQntj7FRonWt0fa2Ku_dZsOdvUQi2Yfuyk3bQUPE5fPNAHAKUo-crQAxIu0lUBIv_u4m0dlkioa9N-aQRFsQurRhbnbQIHCCDb28vBwBoz6FL84cnJiO7KJsJO-zq/s400/br_perseus.jpg" height="303" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="400" /></span></a></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.aradergalleries.com/detail.php?id=3660</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Johann Bayer — Perseus</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>A Constelação de Cetus</b>, <b>a Baleia ou Monstro Marinho</b><o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Cetus representa o monstro marinho enviado por Netuno para devorar Andrômeda. <o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://www.raremaps.com/maps/medium/34421ac.jpg" height="302" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="400" /><br /><a href="http://www.raremaps.com/gallery/detail/34421ac/_Cetus_Stars_Heightened_in_Gold/Bayer.html" style="text-decoration: none;">http://www.raremaps.com/gallery/detail/34421ac/_Cetus_Stars_Heightened_in_Gold/Bayer.html</a></span></span><br />
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/247" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">Johann Bayer</a></span></span><br />
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<b><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A Constelação de Pegasus, o Cavalo Alado<o:p></o:p></span></span></b></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Dizem que Pegasus nasceu a partir do sangue da Medusa quando Perseus cortou fora sua cabeça. Mais tarde, o cavalo foi domado e cavalgado por Bellerofonte que se cansou das questões pertinentes à Terra e tentou voar em direção aos céus porém caiu. Pegasus, no entanto, continuou sua cavalgada, entrando no céu e tomando seu lugar entre as estrelas.<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://www.raremaps.com/maps/medium/35069.jpg" height="320" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="400" /></span></span></div>
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.raremaps.com/gallery/detail/35069/Pagase_Le_Petit_Cheval_Le_Dauphin_Pegasus_Pisces_and_Equuleus/Flamsteed-Fortin.html" style="text-decoration: none;">http://www.raremaps.com/gallery/detail/35069/Pagase_Le_Petit_Cheval_Le_Dauphin_Pegasus_Pisces_and_Equuleus/Flamsteed-Fortin.html</a></span></span><br />
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong style="text-align: start;">Map Maker: </strong><span style="text-align: start;"></span><a href="https://www.raremaps.com/gallery/browse/creator_id/1260" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-align: start; text-decoration: none;">John Flamsteed</a><span style="text-align: start;"> / </span><a href="https://www.raremaps.com/gallery/browse/creator_id/1454" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-align: start; text-decoration: none;">MJ Fortin</a></span></span></div>
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<b><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A Constelação de Cassiopeia, a Rainha Invejosa, a Mulher Sentada</span></span></b></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Andrômeda era a esposa do rei Cefeus, da Etiópia, e mãe de Andrômeda. Ambas eram belíssimas mas alguns dizem que Cassiopéia era muitíssimo invejosa da beleza de sua filha... e espalhou o boato que esta era ainda mais bela do que as Nereidas. Um monstro marinho, Cetus, a Baleia, foi então enviado por Netuno ou para devastar todo o país ou somente para devorar Andrômeda, que seria acorrentada a uma rocha. Sabemos que Perseus salvou Andrômeda e com ela se casou. Mas por todos esses acontecimentos, Cassiopeia foi condenada a se sentar em seu trono e rodear o pólo norte de cabeça para baixo, como um lição de humildade.<o:p></o:p><br /><br /><img src="http://www.raremaps.com/maps/medium/33323op.jpg" height="298" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="400" /></span></span></div>
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<a href="http://www.raremaps.com/gallery/detail/33323op/Cassiopeia/Bayer.html" style="text-decoration: none;"><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/33323op/Cassiopeia/Bayer.html</span></span></a></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/247" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">Johann Baye</a>r</span></span></div>
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<b><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A Constelação de Cefeus, o pai de Andrômeda <o:p></o:p></span></span></b></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Cefeus, rei da Etiópia, foi levado aos céus conjuntamente com sua esposa, Cassiopeia, e sua filha Andrômeda em comemoração sobre os eventos e realizações atuados por Perseus.<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://www.raremaps.com/maps/medium/30845op.jpg" height="400" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="301" /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.raremaps.com/gallery/detail/30845op/_Cepheus_Stars_Heightened_in_Gold/Bayer.html" style="text-decoration: none;">http://www.raremaps.com/gallery/detail/30845op/_Cepheus_Stars_Heightened_in_Gold/Bayer.html</a></span></span><br />
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/247" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">Johann Bayer</a></span></span><br />
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<span style="background-color: white;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Algumas Considerações sobre as constelações que fazem parte do </b></span></span><br />
<span style="background-color: white;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Mito de Andromeda e Perseus</b></span></span><br />
<span style="background-color: white;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>e seus posicionamentos nos céus estrelados</b></span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>Janine Milward</i></span></span><br />
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">É realmente interessante percebermos que as constelações de Cepheus e de Cassipeia se posicionam muitíssimo próximas ao círculo polar - e mal podem ser visualisadas por inteiro por mim (que moro em Latitude 21S52 e Longitude 43W00). No entanto, as constelações de Perseus, de Pegasus e de Andromeda já se situam a meio caminho entre o norte propriamente dito e o Equador celestial. </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">O mito de Andromeda e Perseus nos fala sobre o fato de que a Princesa foi acorrentada numa ilha.... Podemos, então, perceber que exatamente no Ponto Vernal, quer dizer, o ponto de entrecruzamento entre as Linhas do Equador Celestial e da Eclíptica se situa um tantinho abaixo do Grande Quadrado que une as constelações do Cavalo Alado Pegasus e de Andromeda, na simpática e tímida em suas estrelinhas formando dois círculos, a constelação Pisces, os Peixes. Quer dizer, o mar está implícito neste Mito de Andromeda!</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">E também não podemos deixar de notar que neste mar - porém um tanto mais distante, digamos assim -, nada e se apresenta de maneira absolutamente imensa o Monstro Cetus, a Baleia...., porém já no chamado hemisfério sul do Globo Celestial! </span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Quer dizer, Cetus é uma ameaça, sim - assim como o Mito insiste -, mas situa-se mais distanciado (mesmo que imensamente grande e chamando nossa atenção exatamente por seu tamanho descomunal....)</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Estas questões sempre podem ser apreciadas em lugares de céus escuros e transparentes.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Title: </strong>Le Globe Celeste <strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/3554" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">Pherotee De La Croix</a></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">The map exhibits the constellations in the northern and southern skies in fine detail.Scarce decorative double hemisphere celestial map, published in Paris by De La Croix, for his <em>Nouvelle methode pour apprendre facilement la Geographie universelle</em> and engraved by Demasso.</span></span></div>
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<tr><td class="tr-caption" style="font-size: 13px;"><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Stellarium 0.11.1 (para a latitude 21s52 e longitude 43w00)<br /> - www.stellarium.org trabalhado no Corel Photo-Paint X3</span></span></td></tr>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">Algumas Estrelas e alguns objetos interessantes, </span></b></span><br />
<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">em Perseus:</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Mirfak ou Algenib - Alpha Persei</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 03h22,9m - Declinação +49<sup>o</sup> 47’<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual 1,90 (variável) - Distância 570 anos-luz<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Sino. O Badalo, nome árabe que indica uma das partes da constelação</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> quando esta é representada como um sino.<o:p></o:p></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;"><b>Algol.</b><b> Beta Persei. Estrela Dupla e Eclipsante</b></span><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 03h06,6m - Declinação +40<sup>o</sup> 52’<o:p></o:p></span></div>
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<span style="line-height: 22px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual 2,60 (variável) - Distância 105 anos-luz<o:p></o:p></span></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É uma estrela binária e branca e variável,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> marcando a cabeça da Medusa segura pelas mãos de Perseus. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Algol nos chama a atenção</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> por ser uma estrela binária e eclipsando </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">juntamente com sua companheira</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> - do mesmo tamanho e que não se situa muito distante -, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em um período de não mais do que três dias! </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Existe, no entanto, uma terceira estrela, muito menor,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> e que órbita esse sistema binário em 23 meses. </span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A companheira mais pálida e mais fria,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> regularmente acaba eclipsando a mais brilhante, mais quente companheira. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A magnitude de Algol varia entre 2.1 e 3.4 </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">num período de 2 dias, 20 horas, 48 minutos e 56 segundos!<o:p></o:p></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão, </span></span></div>
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<span style="background-color: white;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; line-height: 13.5pt;">Editora Vozes, Petrópolis, ano de 1986</span><span style="font-family: Arial, Helvetica, sans-serif;"> </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes - excerto de Perseus</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Algol é uma palavra que advém de Ra’s al Ghul, a Cabeça do Demônio. </b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Algol representa a cabeça da Górgona Medusa que foi degolada por Perseus. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Medusa, que era a única mortal entre as três irmãs Gorgónas, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">era originalmente uma jovem bela </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">porém seu cabelo foi mudando e acrescendo serpentes</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> - feito realizado por Pallas Athenas</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> por causa do fato de que a Medusa ter se encontrado com Mercúrio</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> e ter dado a luz a Chrysaor e Pegasus, seus filhos, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em um dos templos da deusa. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A aparência da Medusa tornou-se tão medonha </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">que qualquer pessoa que olhasse para ela, transformava-se em pedra.<o:p></o:p></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão, </span></span></div>
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<span style="background-color: white;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; line-height: 13.5pt;">Editora Vozes, Petrópolis, ano de 1986</span><span style="font-family: Arial, Helvetica, sans-serif;"> </span></span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="background-color: white; line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/Medusa_(Caravaggio)">http://pt.wikipedia.org/wiki/Medusa_(Caravaggio)</a></span></span></div>
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<span style="background-color: white;"><i><b>Medusa</b></i> é uma <a href="http://pt.wikipedia.org/wiki/Pintura" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pintura">pintura</a> a óleo sobre tela montada sobre madeira, de Michel Angelo Merisi da Caravaggio, também conhecido apenas como <a href="http://pt.wikipedia.org/wiki/Caravaggio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Caravaggio">Caravaggio</a>. Duas versões foram pintadas, a primeira em <a href="http://pt.wikipedia.org/wiki/1596" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1596">1596</a> e outra presumidamente em 1597.</span></div>
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<span style="background-color: white; font-size: small;">Head of Medusa</span></h3>
<span style="background-color: white;">1598-99<br />Oil on canvas mounted on wood, diameter 58 cm<br />Galleria degli Uffizi, Florence</span></td></tr>
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<span style="background-color: white;">In Greek myth, Perseus used the severed snake-haired head of the Gorgon <span style="color: red;">Medusa</span> as a shield with which to turn his enemies to stone. By the sixteenth century <span style="color: red;">Medusa</span> was said to symbolize the triumph of reason over the senses; and this may have been why Cardinal Del Monte commissioned Caravaggio to paint <span style="color: red;">Medusa</span> as the figure on a ceremonial shield presented in 1601 to Ferdinand I de' Medici, Grand Duke of Tuscany. The poet Marino claimed that it symbolized the Duke's courage in defeating his enemies.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; font-size: 12px;"><a href="http://www.wga.hu/framex-e.html?file=html/c/caravagg/03/20medusa.html&find=medusa">http://www.wga.hu/framex-e.html?file=html/c/caravagg/03/20medusa.html&find=medusa</a></span></span></div>
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<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">Beta Persei conhecida como Algol</span></b><span style="color: #073763;"> é a segunda </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-image: none; color: #073763; text-decoration: none;" title="Estrela">estrela</a><span style="color: #073763;"> mais brilhante da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; color: #073763; text-decoration: none;" title="Constelação">constelação</a><span style="color: #073763;"> de </span><a href="http://pt.wikipedia.org/wiki/Perseus" style="background-image: none; color: #073763; text-decoration: none;" title="Perseus">Perseus</a><span style="color: #073763;">.</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">É uma <a href="http://pt.wikipedia.org/wiki/Estrela_bin%C3%A1ria" style="background-image: none; text-decoration: none;" title="Estrela binária">estrela binária</a> ou eclipsante, cuja variação foi observada por <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Montanari&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="Montanari (página não existe)">Montanari</a> em <a href="http://pt.wikipedia.org/wiki/1669" style="background-image: none; text-decoration: none;" title="1669">1669</a>.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">É a estrela-tipo das chamadas <a href="http://pt.wikipedia.org/wiki/Bin%C3%A1ria_eclipsante" style="background-image: none; text-decoration: none;" title="Binária eclipsante">binárias eclipsantes</a> ou algólidas.</span></span></div>
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<span class="mw-headline" id="Etimologia" style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Etimologia</span></span></h2>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Seu nome em <a href="http://pt.wikipedia.org/wiki/%C3%81rabe" style="background-image: none; text-decoration: none;" title="Árabe">árabe</a>, "<i>al Ghul</i>", significa "o <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Dem%C3%B4nio" style="background-image: none; text-decoration: none;" title="Demônio">Demônio</a>". Na constelação, Algol representa o olho esquerdo da <a href="http://pt.wikipedia.org/wiki/G%C3%B3rgona" style="background-image: none; text-decoration: none;" title="Górgona">Górgona</a> <a href="http://pt.wikipedia.org/wiki/Medusa_(mitologia)" style="background-image: none; text-decoration: none;" title="Medusa (mitologia)">Medusa</a>, cuja cabeça foi usada por <a href="http://pt.wikipedia.org/wiki/Perseu" style="background-image: none; text-decoration: none;" title="Perseu">Perseu</a> para transformar <a href="http://pt.wikipedia.org/wiki/Cetus_(mitologia)" style="background-image: none; text-decoration: none;" title="Cetus (mitologia)">Cetus</a> em pedra e assim salvar <a href="http://pt.wikipedia.org/wiki/Andr%C3%B4meda_(mitologia)" style="background-image: none; text-decoration: none;" title="Andrômeda (mitologia)">Andrômeda</a>; a estrela foi considerada de "má sorte" por séculos.</span></span></div>
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<span class="mw-headline" id="Hist.C3.B3ria" style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">História</span></span></h2>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Em <a href="http://pt.wikipedia.org/wiki/1881" style="background-image: none; text-decoration: none;" title="1881">1881</a>, o astrônomo de Harvard <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Edward_Pickering" style="background-image: none; text-decoration: none;" title="Edward Pickering">Edward Charles Pickering</a> apresentou evidências de que <a href="http://pt.wikipedia.org/wiki/Algol" style="background-image: none; text-decoration: none;" title="Algol">Algol</a> era uma <a href="http://pt.wikipedia.org/wiki/Bin%C3%A1ria_eclipsante" style="background-image: none; text-decoration: none;" title="Binária eclipsante">estrela binária eclipsante</a>. Isso foi confirmado alguns anos depois, em <a href="http://pt.wikipedia.org/wiki/1889" style="background-image: none; text-decoration: none;" title="1889">1889</a>, pelo astrônomo de Petsdam <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Hermann_Vogel&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="Hermann Vogel (página não existe)">Hermann Vogel</a>. Uma curiosidade bastante interessante é que a estrela diminui, em cerca de três dias, 50% do seu brilho e o recupera depois de um pequeno intervalo de tempo.</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; line-height: 19.2000007629395px;"><b>http://pt.wikipedia.org/wiki/Beta_Persei</b></span></span></div>
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<span class="mw-headline" id="Etimologia_e_significato_culturale" style="background-color: white;">Etimologia e significado cultural </span></h2>
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<span style="background-color: white;">O nome <i>Algol</i> deriva ' <a href="http://it.wikipedia.org/wiki/Lingua_araba" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Árabe">árabe </a><b>رأس الغول </b><i>da ra al-Ghul</i> , o que significa que <i>a cabeça do diabo </i><sup class="reference" id="cite_ref-18" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://it.wikipedia.org/wiki/Algol_(astronomia)#cite_note-18" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">[18]</a></sup> e o nome de " <i>Estrela do Diabo</i> "ou" <i>Demônio da estrela</i> "em Inglês é a tradução direta deste significado <sup class="reference" id="cite_ref-allen1899_19-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://it.wikipedia.org/wiki/Algol_(astronomia)#cite_note-allen1899-19" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">[19]</a></sup></span></div>
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<span style="background-color: white;">Em <a href="http://it.wikipedia.org/wiki/Lingua_ebraica" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Língua hebraica">hebraico</a> , Algol era conhecido como <i>Rosh ha Satanás</i> ou "Cabeça de Satanás", como afirma Edmund Chilmead, que o chamou de "a cabeça Divels" ou <i>Rosch hassatan</i> , e também foi vinculado com " <a href="http://it.wikipedia.org/wiki/Lilith" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Lilith">Lilith</a> ", a lendária primeira mulher de <a href="http://it.wikipedia.org/wiki/Adamo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Adam">Adão</a> . Em <a href="http://it.wikipedia.org/wiki/Lingua_latina" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Latina">Latina</a> Algol no <a href="http://it.wikipedia.org/wiki/XVI_secolo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Século XVI">século XVI</a> foi chamado <i>Caput Larvas</i> ou "a cabeça do espectro", e <a href="http://it.wikipedia.org/wiki/Ipparco_di_Nicea" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hiparco de Nicéia">Hiparco</a> e <a class="mw-redirect" href="http://it.wikipedia.org/wiki/Plinio_il_Vecchio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Plínio, o Velho">Plínio</a>tornou uma constelação separada, nomeando o <i>chefe da Medusa </i><sup class="reference" id="cite_ref-allen1899_19-1" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://it.wikipedia.org/wiki/Algol_(astronomia)#cite_note-allen1899-19" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">[19]</a></sup> .</span></div>
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<span style="background-color: white;">Na <a href="http://it.wikipedia.org/wiki/Lingua_cinese" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Idioma chinês">China</a> era大陵(Ling), o <a href="http://it.wikipedia.org/wiki/Mausoleo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Mausoléu">Mausoléu</a> , um <a href="http://it.wikipedia.org/wiki/Asterismo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Asterism">asterismo</a> da China, à qual pertencia, com <a class="new" href="http://it.wikipedia.org/w/index.php?title=9_Persei&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="9 Persei (página não existe)">9 Persei</a> , <a href="http://it.wikipedia.org/wiki/Tau_Persei" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Tau Persei">τ Persei</a> , <a href="http://it.wikipedia.org/wiki/Iota_Persei" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Iota Persei">ι Persei</a> , <a href="http://it.wikipedia.org/wiki/Kappa_Persei" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Kappa Persei">κ Persei</a> , <a href="http://it.wikipedia.org/wiki/Rho_Persei" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Rho Persei">ρ Persei</a> , 16 e 12 Persei Persei. Como resultado, Algol era conhecido como大陵五(wu Da Ling), a quinta estrela do Mausoléu <sup class="reference" id="cite_ref-20" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://it.wikipedia.org/wiki/Algol_(astronomia)#cite_note-20" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">[20]</a></sup> .</span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i style="line-height: 15.8341131210327px; text-align: left;">Medusa</i><span style="line-height: 15.8341131210327px; text-align: left;">, obra de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Bernini" style="background-image: none; line-height: 15.8341131210327px; text-align: left; text-decoration: none;" title="Bernini">Bernini</a><span style="line-height: 15.8341131210327px; text-align: left;">.</span><br style="line-height: 15.8341131210327px; text-align: left;" /><a href="http://pt.wikipedia.org/wiki/Museus_Capitolinos" style="background-image: none; line-height: 15.8341131210327px; text-align: left; text-decoration: none;" title="Museus Capitolinos">Museus Capitolinos</a><span style="line-height: 15.8341131210327px; text-align: left;">, </span><a href="http://pt.wikipedia.org/wiki/Roma" style="background-image: none; line-height: 15.8341131210327px; text-align: left; text-decoration: none;" title="Roma">Roma</a></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 19.200000762939453px; text-align: start;">A </span><b style="line-height: 19.200000762939453px; text-align: start;">Medusa</b><span style="line-height: 19.200000762939453px; text-align: start;"> (em </span><a href="http://pt.wikipedia.org/wiki/L%C3%ADngua_grega" style="background-image: none; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Língua grega">grego</a><span style="line-height: 19.200000762939453px; text-align: start;">: </span><span class="politonico" lang="el" style="line-height: 19.200000762939453px; text-align: start;" xml:lang="el">Μέδουσα</span><span style="line-height: 19.200000762939453px; text-align: start;">, </span><i style="line-height: 19.200000762939453px; text-align: start;">Médousa</i><span style="line-height: 19.200000762939453px; text-align: start;">, "guardiã", "protetora"</span><span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Medusa_(mitologia)#cite_note-1" style="background-image: none; text-decoration: none;">1</a></span><span style="line-height: 19.200000762939453px; text-align: start;"> ), na </span><a href="http://pt.wikipedia.org/wiki/Mitologia_grega" style="background-image: none; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Mitologia grega">mitologia grega</a><span style="line-height: 19.200000762939453px; text-align: start;">, era um </span><a href="http://pt.wikipedia.org/wiki/Monstro" style="background-image: none; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Monstro">monstro</a><span style="line-height: 19.200000762939453px; text-align: start;"> </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ct%C3%B4nico" style="background-image: none; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Ctônico">ctônico</a><span style="line-height: 19.200000762939453px; text-align: start;"> do sexo feminino, uma das três </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/G%C3%B3rgonas" style="background-image: none; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Górgonas">Górgonas</a><span style="line-height: 19.200000762939453px; text-align: start;">. Filha de </span><a href="http://pt.wikipedia.org/wiki/F%C3%B3rcis" style="background-image: none; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Fórcis">Fórcis</a><span style="line-height: 19.200000762939453px; text-align: start;"> e </span><a href="http://pt.wikipedia.org/wiki/Ceto_(mitologia)" style="background-image: none; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Ceto (mitologia)">Ceto</a><span class="reference" id="cite_ref-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Medusa_(mitologia)#cite_note-2" style="background-image: none; text-decoration: none;">2</a></span><span style="line-height: 19.200000762939453px; text-align: start;"> (embora o autor antigo </span><a href="http://pt.wikipedia.org/wiki/Higino" style="background-image: none; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Higino">Higino</a><span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Medusa_(mitologia)#cite_note-3" style="background-image: none; text-decoration: none;">3</a></span><span style="line-height: 19.200000762939453px; text-align: start;"> interpole uma geração e cite outro casal ctônico como os pais da Medusa),</span><span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Medusa_(mitologia)#cite_note-4" style="background-image: none; text-decoration: none;">4</a></span><span style="line-height: 19.200000762939453px; text-align: start;"> quem quer que olhasse diretamente para ela era transformado em </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Pedra" style="background-image: none; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Pedra">pedra</a><span style="line-height: 19.200000762939453px; text-align: start;">. Ao contrário de suas irmãs Górgonas, </span><a href="http://pt.wikipedia.org/wiki/Esteno" style="background-image: none; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Esteno">Esteno</a><span style="line-height: 19.200000762939453px; text-align: start;"> e </span><a href="http://pt.wikipedia.org/wiki/Eur%C3%ADale" style="background-image: none; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Euríale">Euríale</a><span style="line-height: 19.200000762939453px; text-align: start;">, Medusa era mortal;</span><span class="reference" id="cite_ref-Livro_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Medusa_(mitologia)#cite_note-Livro-5" style="background-image: none; text-decoration: none;">5</a></span><span style="line-height: 19.200000762939453px; text-align: start;"> foi decapitada pelo herói</span><a href="http://pt.wikipedia.org/wiki/Perseu" style="background-image: none; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Perseu">Perseu</a><span style="line-height: 19.200000762939453px; text-align: start;">, que utilizou posteriormente sua cabeça como arma,</span><span class="reference" id="cite_ref-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Medusa_(mitologia)#cite_note-6" style="background-image: none; text-decoration: none;">6</a></span><span style="line-height: 19.200000762939453px; text-align: start;"> até dá-la para a deusa </span><a href="http://pt.wikipedia.org/wiki/Atena" style="background-image: none; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Atena">Atena</a><span style="line-height: 19.200000762939453px; text-align: start;">, que a colocou em seu </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aegis" style="background-image: none; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Aegis">escudo</a><span style="line-height: 19.200000762939453px; text-align: start;">. Na </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Antiguidade_Cl%C3%A1ssica" style="background-image: none; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Antiguidade Clássica">Antiguidade Clássica</a><span style="line-height: 19.200000762939453px; text-align: start;"> a imagem da cabeça da Medusa aparecia no objeto utilizado </span><a href="http://pt.wikipedia.org/wiki/Apotropismo" style="background-image: none; line-height: 19.200000762939453px; text-align: start; text-decoration: none;" title="Apotropismo">para afugentar o mal</a><span style="line-height: 19.200000762939453px; text-align: start;">conhecido como </span><i style="line-height: 19.200000762939453px; text-align: start;"><a href="http://pt.wikipedia.org/wiki/Gorgoneion" style="background-image: none; text-decoration: none;" title="Gorgoneion">Gorgoneion</a></i><span style="line-height: 19.200000762939453px; text-align: start;">.</span></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">- </span><b><span lang="EN-US">Richard Hinckley Allen, Star Names, Their Lore and Meaning</span></b><span lang="EN-US">, Dover Publications, Inc, New York, USA <o:p></o:p></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b>Richard Hinckley Allen, em seu famoso e importantíssimo livro<br />Star Names — Their Lore and Meaning -,</b></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000; font-size: large;">ALGOL:</span></b></span></div>
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<a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Perseus*.html" style="background-color: white;">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Perseus*.html</a></div>
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<span style="background-color: white;"><span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-size: 16px; font-style: italic;">β</span>, Spectroscopic binary and variable, 2.3 to 3.5, white.</span></h3>
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<span style="background-color: white;"><b>Algol</b>, the <b>Demon</b>, the <b>Demon Star</b>, and the <b>Blinking Demon</b>, from the Arabians' <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Ra᾽s al Ghul</span></b>, the Demon's Head, is said to have been thus called from its rapid and wonderful variations; but I find no evidence of this, and that people probably took the title from Ptolemy. <span class="archaic" style="color: rgb(102, 102, 0) !important;">Al Ghul</span> literally signifies a Mischief-maker, and the name still appears in the Ghoul of the <i>Arabian Nights</i> and of our day. It degenerated into the <b>Alove</b> often used some centuries ago for this star.</span></div>
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<span style="background-color: white;">Ptolemy catalogued it as <span class="Greek" style="color: rgb(153, 102, 0) !important; font-family: Avdira, 'Titus Cyberbit Basic', serif !important;">τῶν ἐν γοργονίῳ<a class="correction" href="https://www.blogger.com/null" style="color: rgb(255, 0, 0) !important; cursor: crosshair; font-family: Verdana, sans-serif; vertical-align: top;">º</a> ὁ λαμπρός</span>, "the bright one of those in the Gorgon's head," which Al Tizini followed in his <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Nā᾽ir</span></b>, for, with <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-style: italic;">π</span>, <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-style: italic;">ρ</span>, and <span class="star" style="color: rgb(136, 0, 204) !important; font-family: Verdana, Ariel, Helvetica, sans-serif; font-style: italic;">ω</span>, it made up that well-known group, itself being the <b>Gorgonea prima</b>; the <span class="Greek" style="color: rgb(153, 102, 0) !important; font-family: Avdira, 'Titus Cyberbit Basic', serif !important;">Γοργόνιον</span> of Chrysococca, <b><span class="Latin" style="color: rgb(153, 0, 0) !important;">Gorgoneum Caput</span></b> of Vitruvius <a class="added_link" href="http://penelope.uchicago.edu/Thayer/L/Roman/Texts/Vitruvius/9*.html#4.2" style="color: rgb(85, 85, 255) !important; font-style: italic; font-weight: bold; text-decoration: none;" target="Vitruvius">[<span class="small">IX</span>.4.2]</a>,<b><span class="Latin" style="color: rgb(153, 0, 0) !important;">Caput Gorgonis</span></b> of Hyginus, and the <b><span class="Latin" style="color: rgb(153, 0, 0) !important;">Gorgonis Ora</span></b> of Manilius.</span></div>
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<span style="background-color: white;">With astronomical writers of three centuries ago Algol was <b><span class="Latin" style="color: rgb(153, 0, 0) !important;">Caput Larvae</span></b>, the Spectre's Head. Hipparchos and Pliny made a separate constellation of the Gorgon stars as the <b>Head of Medusa</b>, this descending almost to our own day, although always connected with Perseus.</span></div>
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<span style="background-color: white;">The Hebrews knew Algol as <b><span class="archaic" style="color: rgb(102, 102, 0) !important;">Rōsh ha Sāṭān</span></b>, Satan's Head, Chilmead's <b>Rosch hassatan</b>, <b>the Divels head</b>; but also as <b>Līlīth</b>, Adam's legendary first wife,<a class="ref" href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Perseus*.html#note2" id="ref2" style="color: rgb(255, 0, 0) !important; font-family: Verdana, sans-serif; font-weight: bold; padding: 0.2em; text-decoration: none; vertical-align: super;">2</a> the nocturnal vampire from the lower world that reappeared in the demonology of the Middle Ages as the witch Lilis, one of the characters in Goethe's <i>Walpurgis Nacht</i>.</span></div>
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<span style="background-color: white;">The Chinese gave it the gruesome title <b><span class="Chinese" style="color: rgb(218, 83, 0) !important;">Tseih She</span></b>, the Piled-up Corpses.</span></div>
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<span class="pagenum" style="color: rgb(255, 51, 0) !important; position: absolute; right: 1.5em; text-align: right; top: auto; width: 70px;"><span style="background-color: white;">p333</span></span><span style="background-color: white;">Astrologers of course said that it was the most unfortunate, violent, and dangerous star in the heavens, and it certainly has been one of the best observed, as the most noteworthy variable in the northern sky. It "continues sensibly constant at 2.3 magnitude during 2½ days, then decreases, at first gradually, and afterward with increasing rapidity, to 3.5 magnitude"; its light oscillations occupying about nine hours; its total period being stated as 2 days 20 hours 48 minutes 55 seconds. Al Sufi, a good observer for his day, yet strangely making no allusion to its variability, called it a 2nd‑magnitude; and the phenomenon was first scientifically noted by Montanari during several years preceding 1672. This was confirmed by Maraldi's observations of 1694, and, later, by those of the Saxon farmer Palitsch,<a class="ref" href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Perseus*.html#note3" id="ref3" style="color: rgb(255, 0, 0) !important; font-family: Verdana, sans-serif; font-weight: bold; padding: 0.2em; text-decoration: none; vertical-align: super;">3</a> but its approximate period seems to have been first announced by Goodricke in 1782, who even then advanced the theory of a dark companion revolving around it with immense velocity, which periodically cut off its light. This, reaffirmed by Pickering in 1880, was made certain by the spectroscope in the hands of Vogel of Potsdam in 1889. Chandler thinks that there must exist another invisible body larger than either Algol or its companion, around which both revolve in a period of 130 years; but Tisserand has shown that the phenomenon on which Chandler bases this opinion can be explained in a different and simpler way. Its name is used for the type indicating short-period variables whose changes may be explained by this theory of "eclipses." Of these seventeen are now known.</span></div>
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<span style="background-color: white;">Although classed among the white stars with a Sirian spectrum, Al Sufi wrote of it as red, which Schmidt confirmed as seen by him at Athens for a short time in 1841. It seems to be approaching us at the rate of about a mile a second; and is estimated as a little more than a million miles in diameter.</span></div>
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<span style="background-color: white;">When on the meridian Algol is almost exactly in the zenith of New York City. This is at nine o'clock in the evening of the 23d of December.</span></div>
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<a href="http://pt.wikipedia.org/wiki/G%C3%B3rgona#mediaviewer/Ficheiro:Berninimedusa.jpg" style="background-color: white;">http://pt.wikipedia.org/wiki/G%C3%B3rgona#mediaviewer/Ficheiro:Berninimedusa.jpg</a></div>
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<span style="background-color: white;"><a href="http://pt.wikipedia.org/wiki/Medusa_(mitologia)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px; text-decoration: none;" title="Medusa (mitologia)">Medusa</a><span style="color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px;">, obra de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Bernini" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px; text-decoration: none;" title="Bernini">Bernini</a><span style="color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px;">. </span><a href="http://pt.wikipedia.org/wiki/Museus_Capitolinos" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px; text-decoration: none;" title="Museus Capitolinos">Museus Capitolinos</a><span style="color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px;">, </span><a href="http://pt.wikipedia.org/wiki/Roma" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px; text-decoration: none;" title="Roma">Roma</a></span></div>
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<span style="background-color: white;"><span style="color: #660000; font-size: large;"><b>A Górgona</b></span><span style="color: #252525;"> (em </span><a href="http://pt.wikipedia.org/wiki/L%C3%ADngua_grega_antiga" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Língua grega antiga">grego clássico</a><span style="color: #252525;">: </span><span class="politonico" lang="el" style="color: #252525; font-family: 'Athena Unicode', Gentium, 'Palatino Linotype', 'Arial Unicode MS', 'Lucida Sans Unicode', 'Lucida Grande', Code2000;" xml:lang="el">Γοργών/Γοργώ</span><span style="color: #252525;">; </span><a href="http://pt.wikipedia.org/wiki/Translitera%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Transliteração">transl</a><span style="color: #252525;">.: </span><span class="Unicode" lang="grc-Latn" style="color: #252525; font-family: Code2000, Code2001, 'Free Serif', 'TITUS Cyberbit Basic', 'Doulos SIL', 'Chrysanthi Unicode', 'Bitstream Cyberbit', 'Bitstream CyberBase', Thryomanes, Gentium, GentiumAlt, 'Lucida Grande', 'Free Sans', 'Arial Unicode MS', 'Microsoft Sans Serif', 'Lucida Sans Unicode';" title="ISO 843 Greek" xml:lang="grc-Latn"><i>Gorgón</i>/<i>Gorgó</i></span><span style="color: #252525;">) é uma criatura da </span><a href="http://pt.wikipedia.org/wiki/Mitologia_grega" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Mitologia grega">mitologia grega</a><span style="color: #252525;">, representada como um </span><a href="http://pt.wikipedia.org/wiki/Monstro" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Monstro">monstro</a><span style="color: #252525;"> feroz, de aspecto </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Sexo_feminino" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sexo feminino">feminino</a><span style="color: #252525;">, e com grandes presas. Tinha o poder de transformar todos que olhassem para ela em pedra, o que fazia que, muitas vezes, </span><a href="http://pt.wikipedia.org/wiki/Imagem" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Imagem">imagens</a><span style="color: #252525;"> suas fossem utilizadas como uma forma de </span><a href="http://pt.wikipedia.org/wiki/Amuleto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Amuleto">amuleto</a><span style="color: #252525;">. A górgona também vestia um </span><a href="http://pt.wikipedia.org/wiki/Cinto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Cinto">cinto</a><span style="color: #252525;"> de </span><a href="http://pt.wikipedia.org/wiki/Serpente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Serpente">serpentes</a><span style="color: #252525;"> entrelaçadas.</span></span></div>
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<span style="background-color: white;">Na mitologia grega tardia, diziam-se que existiam três górgonas: as três filhas de <a href="http://pt.wikipedia.org/wiki/F%C3%B3rcis" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Fórcis">Fórcis</a> e <a href="http://pt.wikipedia.org/wiki/Ceto_(mitologia)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ceto (mitologia)">Ceto</a>. Seus nomes eram <a href="http://pt.wikipedia.org/wiki/Medusa_(mitologia)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Medusa (mitologia)">Medusa</a>, "a impetuosa", <a href="http://pt.wikipedia.org/wiki/Esteno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Esteno">Esteno</a>, "a que oprime" e <a href="http://pt.wikipedia.org/wiki/Eur%C3%ADale" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Euríale">Euríale</a>, "a que está ao largo". Como a mãe, as górgonas eram extremamente belas e seus <a href="http://pt.wikipedia.org/wiki/Cabelo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Cabelo">cabelos</a> eram invejáveis; todavia, eram desregradas e sem escrúpulos. Isso causou a irritação dos demais deuses, principalmente de <a href="http://pt.wikipedia.org/wiki/Atena" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Atena">Atena</a>, a deusa da sabedoria, que admirou-se de ver que a beleza das górgonas as fazia exatamente idênticas a ela.</span></div>
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<span style="background-color: white;">Atena então, para não permitir que deusas iguais a ela mostrassem um comportamento maligno, tão diferente do seu, deformou-lhes a aparência, determinada a diferenciar-se. Atena transformou os belos cachos das irmãs em ninhos de <a href="http://pt.wikipedia.org/wiki/Serpente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Serpente">serpentes</a> letais e violentas, que picavam suas faces. Transformou seus belos dentes em presas de <a href="http://pt.wikipedia.org/wiki/Javali" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Javali">javalis</a>, e fez com que seus pés e mãos macias se tornassem em bronze frio e pesado. Cobrindo suas peles com escamas douradas e para terminar, Atena condenou-as a transformar em pedra tudo aquilo que pudesse contemplar seus olhos. Assim, o belo olhar das górgonas se transformou em algo perigoso.</span></div>
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<span style="background-color: white;">Envergonhadas e desesperadas por seu infortúnio, as górgonas fugiram para o Ocidente, e se esconderem na <a href="http://pt.wikipedia.org/wiki/Crimeia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Crimeia">Ciméria</a>, conhecido como "o país da noite eterna".</span></div>
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<span style="background-color: white;">Mesmo monstruosa, Medusa foi assediada por <a href="http://pt.wikipedia.org/wiki/Pos%C3%ADdon" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Posídon">Posídon</a>, que amava Atena. Para vingar-se, Medusa cedeu e Posídon desposou-a. Após isso, Posídon fez com que Atena soubesse que ele tivera aquela que era sua semelhante. Atena sentiu-se tão ultrajada que tomou de Medusa sua imortalidade, fazendo-a a única mortal entre as górgonas. Em outras versões, Atena amaldiçoou as górgonas justamente porque quando Medusa ainda era bela, ela e Posídon se uniram em um templo de Atena, a deusa ficou ultrajada e as amaldiçoou.</span></div>
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<span style="background-color: white;">Mais tarde, <a href="http://pt.wikipedia.org/wiki/Perseu" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Perseu">Perseu</a>, filho de <a href="http://pt.wikipedia.org/wiki/Zeus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Zeus">Zeus</a> e da princesa <a href="http://pt.wikipedia.org/wiki/D%C3%A2nae" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Dânae">Dânae</a>, contou com a ajuda de Atena para encontrar Medusa e cortar a sua cabeça, com a qual realizou prodígios. Pois mesmo depois de morta, a cabeça continuava viva e aquele que a olhasse nos olhos se tornava pedra. Medusa deu à luz dois filhos de Posídon, <a href="http://pt.wikipedia.org/wiki/P%C3%A9gaso" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pégaso">Pégaso</a> e<a href="http://pt.wikipedia.org/wiki/Crisaor" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Crisaor">Crisaor</a>.<span class="reference" id="cite_ref-apolodoro.2.4.2_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/G%C3%B3rgona#cite_note-apolodoro.2.4.2-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg4H8NBK5161ShVl9Qt5rXiITz6cx9GFE0VpWKeHuMkLVck1GyOYKHs4fj2n7XNDUP5wXntJQdoKq1nx5f02XLqKvn-br89aAMr2s8r9QyZLLqRZK5WrD1NVKU1T38rLMAOWoJ2MhGUz0k/s1600/450px-PerseusSignoriaStatue.jpg" imageanchor="1" style="background-color: white; margin-left: 1em; margin-right: 1em;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg4H8NBK5161ShVl9Qt5rXiITz6cx9GFE0VpWKeHuMkLVck1GyOYKHs4fj2n7XNDUP5wXntJQdoKq1nx5f02XLqKvn-br89aAMr2s8r9QyZLLqRZK5WrD1NVKU1T38rLMAOWoJ2MhGUz0k/s1600/450px-PerseusSignoriaStatue.jpg" height="640" width="480" /></span></a></div>
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<span style="background-color: white; line-height: 18.239999771118164px; text-align: start;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Statue of Perseus, Piazza della Signoria, Florence</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i style="line-height: 15.8341131210327px; text-align: left;"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Perseu_com_a_Cabe%C3%A7a_da_Medusa" style="background-image: none; text-decoration: none;" title="Perseu com a Cabeça da Medusa">Perseu com a Cabeça da Medusa</a></i><span style="line-height: 15.8341131210327px; text-align: left;">, de </span><a href="http://pt.wikipedia.org/wiki/Benvenuto_Cellini" style="background-image: none; line-height: 15.8341131210327px; text-align: left; text-decoration: none;" title="Benvenuto Cellini">Benvenuto Cellini</a><span style="line-height: 15.8341131210327px; text-align: left;">, de 1554.</span></span></span></div>
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<span style="background-color: white;"><b><span style="color: #660000; font-size: large;">Algol ( <a href="http://it.wikipedia.org/wiki/Nomenclatura_di_Bayer" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Nomenclatura de Bayer">β For / β Persei</a> )</span></b><span style="color: #252525;"> é um </span><a href="http://it.wikipedia.org/wiki/Sistema_stellare" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sistema de estrelas">sistema de estrelas</a><span style="color: #252525;"> na </span><a href="http://it.wikipedia.org/wiki/Costellazione" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constellation">constelação</a><span style="color: #252525;"> de </span><a href="http://it.wikipedia.org/wiki/Perseo_(costellazione)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Perseus (constelação)">Perseus</a><span style="color: #252525;"> , que está a 93 </span><a class="mw-redirect" href="http://it.wikipedia.org/wiki/Anni_luce" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="color: #252525;"> do </span><a href="http://it.wikipedia.org/wiki/Sistema_solare" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sistema solar">sistema solar </a><sup class="reference" id="cite_ref-Anderson_2-0" style="color: #252525; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://it.wikipedia.org/wiki/Algol_(astronomia)#cite_note-Anderson-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">[2]</a></sup><span style="color: #252525;"> . É o mais conhecido </span><a href="http://it.wikipedia.org/wiki/Binaria_a_eclisse" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Eclipsando binário">binário eclipsando</a><span style="color: #252525;"> , o primeiro de seu tipo a ser descoberto, e é também um dos primeiros-nova (não) </span><a class="mw-redirect" href="http://it.wikipedia.org/wiki/Stelle_variabili" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrelas variáveis">estrelas variáveis</a><span style="color: #252525;"> descobertas de longe.</span></span></div>
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<span style="background-color: white;"><span class="">Algol é um dos poucos visíveis a olho nu para mostrar uma acentuada </span><a href="http://it.wikipedia.org/wiki/Stella_variabile" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela variável">variabilidade</a><span class=""> : é o protótipo das </span><a href="http://it.wikipedia.org/wiki/Variabile_Algol" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Algol Variável">variáveis Algol</a><span class=""> e é na verdade uma </span><a href="http://it.wikipedia.org/wiki/Stella_tripla" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estelar triplo">estrela tripla</a><span class=""> , onde a estrela principal, Algol A é regularmente </span><a class="mw-redirect" href="http://it.wikipedia.org/wiki/Eclisse" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Eclipse">eclipsado</a><span class=""> pelo companheiro mais fraco, Algol B. Sua </span><a href="http://it.wikipedia.org/wiki/Magnitudine_apparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span class=""> , geralmente de 2,12, cai para 3,39 a cada 2 dias, 20 horas e 49 minutos, por um período de 10 horas, o que é equivalente à duração do eclipse parcial. </span><span class="goog-text-highlight" style="-webkit-box-shadow: rgb(153, 153, 170) 2px 2px 4px; box-shadow: rgb(153, 153, 170) 2px 2px 4px; box-sizing: border-box; position: relative;">O eclipse secundário, o que ocorre quando a passagem principal na frente do secundário, apenas pode ser detectado photoelectrically </span><sup class="reference" id="cite_ref-AAVSO_3-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://it.wikipedia.org/wiki/Algol_(astronomia)#cite_note-AAVSO-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><span class="goog-text-highlight" style="-webkit-box-shadow: rgb(153, 153, 170) 2px 2px 4px; box-shadow: rgb(153, 153, 170) 2px 2px 4px; box-sizing: border-box; position: relative;">[3]</span></a></sup><span class="goog-text-highlight" style="-webkit-box-shadow: rgb(153, 153, 170) 2px 2px 4px; box-shadow: rgb(153, 153, 170) 2px 2px 4px; box-sizing: border-box; position: relative;"> .</span></span></div>
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<span style="background-color: white;"><span class="">A 2,69 </span><a href="http://it.wikipedia.org/wiki/Unit%C3%A0_astronomica" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Unidade astronômica">UA</a><span class=""> roda, em torno do comum </span><a href="http://it.wikipedia.org/wiki/Centro_di_massa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Centro de massa">centro de massa</a><span class=""> e em um período de 680 dias, Algol C, uma </span><a href="http://it.wikipedia.org/wiki/Stella_di_classe_A_V" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Star Class AV">estrela branca</a><span class=""> de </span><a href="http://it.wikipedia.org/wiki/Sequenza_principale" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Seqüência Principal">sequência principal</a><span class=""> que tem uma </span><a href="http://it.wikipedia.org/wiki/Massa_(fisica)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Massa (física)">massa</a><span class=""> 1,7 vezes a do Sol </span><sup class="reference" id="cite_ref-JK_4-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://it.wikipedia.org/wiki/Algol_(astronomia)#cite_note-JK-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><span class="">[4] </span></a></sup><sup class="reference" id="cite_ref-Sixth_5-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://it.wikipedia.org/wiki/Algol_(astronomia)#cite_note-Sixth-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><span class="">[5]</span></a></sup><span class=""> .</span></span></div>
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<span class="" style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">http://it.wikipedia.org/wiki/Algol_(astronomia)</span></div>
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<span class="" style="background-color: white;"><img src="http://upload.wikimedia.org/wikipedia/commons/thumb/4/43/Algol_AB_movie_imaged_with_the_CHARA_interferometer.gif/220px-Algol_AB_movie_imaged_with_the_CHARA_interferometer.gif" height="640" width="640" /></span></div>
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<span class="" style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.3999996185303px;">http://it.wikipedia.org/wiki/Algol_(astronomia)#mediaviewer/File:Algol_AB_movie_imaged_with_the_CHARA_interferometer.gif</span></div>
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<span class="mw-mmv-title" original-title="Nome del file" style="background-color: white; max-width: 60%;"><span style="color: #073763;">Algol AB filme fotografada com o interferômetro CHARA </span></span></div>
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<span class="mw-mmv-source-author mw-mmv-reduce-toolong mw-mmv-truncate-toolong" original-title="Informazioni su autore e fonte" style="background-color: white; cursor: pointer;"><span style="color: #073763;"><span class="mw-mmv-author"><span class="goog-text-highlight" style="-webkit-box-shadow: rgb(153, 153, 170) 2px 2px 4px; box-shadow: rgb(153, 153, 170) 2px 2px 4px; box-sizing: border-box; position: relative;">Dr. Fabien Baron, Departamento de Astronomia da Universidade de Michigan, Ann Arbor, MI 48109-1090</span></span><span class="goog-text-highlight" style="-webkit-box-shadow: rgb(153, 153, 170) 2px 2px 4px; box-shadow: rgb(153, 153, 170) 2px 2px 4px; box-sizing: border-box; position: relative;"> - </span><span class="mw-mmv-source"><a class="external free" href="http://www.oculum.de/newsletter/astro/100/60/2/2-02_algol_movie.gif" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;"><span class="goog-text-highlight" style="-webkit-box-shadow: rgb(153, 153, 170) 2px 2px 4px; box-shadow: rgb(153, 153, 170) 2px 2px 4px; box-sizing: border-box; position: relative;">http://www.oculum.de/newsletter/astro/100/60/2/2-02_algol_movie.gif</span></a><span class="goog-text-highlight" style="-webkit-box-shadow: rgb(153, 153, 170) 2px 2px 4px; box-shadow: rgb(153, 153, 170) 2px 2px 4px; box-sizing: border-box; position: relative;"> , </span><span class="goog-text-highlight" style="-webkit-box-shadow: rgb(153, 153, 170) 2px 2px 4px; background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; box-shadow: rgb(153, 153, 170) 2px 2px 4px; box-sizing: border-box; position: relative; text-decoration: none;"><a class="external free" href="http://www.oculum.de/newsletter/astro/100/60/2/162.fa1cn.asp" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;">http://www.oculum.de/newsletter/astro/100/60/2/162.fa1cn.asp</a></span></span></span></span></div>
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<h1 class="firstHeading" id="firstHeading" lang="it" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-color: rgb(170, 170, 170); border-bottom-style: solid; border-bottom-width: 1px; font-family: 'Linux Libertine', Georgia, Times, serif; font-size: 1.8em; font-weight: normal; line-height: 1.3; margin: 0px 0px 0.25em; overflow: hidden; padding: 0px;">
<span dir="auto" style="background-color: white;">Paradoxo da Algol</span></h1>
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<span style="background-color: white;">Em <a href="http://it.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Astronomia">astronomia</a> , o <b>paradoxo Algol</b> refere-se<span style="font-size: 0.875em;"> à</span> situação aparentemente <a href="http://it.wikipedia.org/wiki/Paradosso" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Paradox">paradoxal</a> em que se encontram, por vezes, os componentes de uma <a href="http://it.wikipedia.org/wiki/Stella_binaria" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela binária">estrela binária</a> que parece ter <a href="http://it.wikipedia.org/wiki/Evoluzione_stellare" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Evolução estelar">evoluído</a> de uma forma diferente do que eles fornecem as mais estabelecidas <a href="http://it.wikipedia.org/wiki/Teoria#Teorie_scientifiche" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Teoria">teorias científicas</a> sobre o assunto. Estas teorias prever que a taxa de evolução de uma estrela depende da sua <a href="http://it.wikipedia.org/wiki/Massa_(fisica)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Massa (física)">massa</a> : o mais massiva uma estrela, mais rápida será a sua evolução e, portanto, menor o tempo gasto na <a href="http://it.wikipedia.org/wiki/Sequenza_principale" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Seqüência Principal">sequência principal</a> , antes de evoluir um <a href="http://it.wikipedia.org/wiki/Stella_subgigante" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Stella subgigante">subgigante</a> ou <a href="http://it.wikipedia.org/wiki/Stella_gigante" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela gigante">gigante</a> .</span></div>
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<span style="background-color: white;">No caso de <a href="http://it.wikipedia.org/wiki/Algol_(astronomia)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Algol (astronomia)">Algol</a> (β Persei) e algumas outras estrelas binárias é observado o contrário: quanto menos massiva estrela já atingiu o estágio de subgigante, enquanto o mais maciço ainda está na seqüência principal.A situação parece paradoxal, pois os componentes de uma estrela binária geralmente <a href="http://it.wikipedia.org/wiki/Formazione_stellare" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="A formação de estrelas">surgem</a> quase ao mesmo tempo e, portanto, têm idades semelhantes. Portanto, a estrela mais massiva deve ser o mais evoluído.</span></div>
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<span style="background-color: white;">O paradoxo é resolvido pelo fato de que no sistema binário como estes há uma transferência de <a href="http://it.wikipedia.org/wiki/Materia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Matéria">matéria</a> de uma estrela para outra. A estrela de maior massa no final de sua estada na <a href="http://it.wikipedia.org/wiki/Sequenza_principale" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Seqüência Principal">seqüência principal</a> , que começa a aumentar de tamanho. Se ele estiver em um sistema binário próximo, pode haver vazamento de seu <a href="http://it.wikipedia.org/wiki/Lobo_di_Roche" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Roche lobo">lóbulo de Roche</a> , ou seja, suas camadas exteriores passam por uma ' <a href="http://it.wikipedia.org/wiki/Interazione_gravitazionale" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Interação gravitacional">força gravitacional</a> do companheiro é maior do que o previsto pela própria estrela <sup class="reference" id="cite_ref-1" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://it.wikipedia.org/wiki/Paradosso_di_Algol#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">[1]</a></sup> . <span class="">O processo de transferência altera a evolução normal dos dois componentes teriam se fossem estrelas individuais </span><sup class="reference" id="cite_ref-2" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://it.wikipedia.org/wiki/Paradosso_di_Algol#cite_note-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><span class="">[2] </span></a></sup><sup class="reference" id="cite_ref-3" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://it.wikipedia.org/wiki/Paradosso_di_Algol#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><span class="">[3]</span></a></sup><span class=""> : na verdade, esta transferência tem como resultado que a estrela inicialmente menos massiva que se torna mais maciça. </span>Em alguns binários semelhantes a Algol é possível observar a transferência de gás de uma estrela para outra<sup class="reference" id="cite_ref-4" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://it.wikipedia.org/wiki/Paradosso_di_Algol#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">[4]</a></sup> .</span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="background-color: white; line-height: 22.3999996185303px;"><a href="http://it.wikipedia.org/wiki/Paradosso_di_Algol">http://it.wikipedia.org/wiki/Paradosso_di_Algol</a></span></span></div>
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<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000; font-size: large;">Uma estrela binária</span></b><span style="color: #073763;"> é um </span><a href="http://pt.wikipedia.org/wiki/Sistema_estelar" style="background-image: none; color: #073763; text-decoration: none;" title="Sistema estelar">sistema estelar</a><span style="color: #073763;"> que consiste de duas </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-image: none; color: #073763; text-decoration: none;" title="Estrela">estrelas</a><span style="color: #073763;"> </span><a href="http://pt.wikipedia.org/wiki/%C3%93rbita" style="background-image: none; color: #073763; text-decoration: none;" title="Órbita">orbitando</a><span style="color: #073763;"> um baricentro (</span><a href="http://pt.wikipedia.org/wiki/Centro_de_massas" style="background-image: none; color: #073763; text-decoration: none;" title="Centro de massas">centro de massas</a><span style="color: #073763;">) comum. A estrela mais brilhante é chamada de </span><b style="color: #073763;">primária</b><span style="color: #073763;">, enquanto a estrela menos brilhante é chamada de </span><b style="color: #073763;">estrela companheira</b><span style="color: #073763;"> ou </span><b style="color: #073763;">secundária</b><span style="color: #073763;">. Pesquisas desde o início do século XIX sugerem que muitas estrelas são parte de um sistema binário ou de sistemas com mais de duas estrelas, chamados </span><a href="http://pt.wikipedia.org/wiki/Estrela_m%C3%BAltipla" style="background-image: none; color: #073763; text-decoration: none;" title="Estrela múltipla">sistemas múltiplos de estrelas</a><span style="color: #073763;">. O termo </span><i style="color: #073763;"><a href="http://pt.wikipedia.org/wiki/Estrela_dupla" style="background-image: none; text-decoration: none;" title="Estrela dupla">estrela dupla</a></i><span style="color: #073763;"> é por vezes utilizado como sinônimo, embora, na definição astronômica moderna, estrelas duplas sejam quaisquer estrelas próximas entre si no </span><a href="http://pt.wikipedia.org/wiki/C%C3%A9u" style="background-image: none; color: #073763; text-decoration: none;" title="Céu">céu</a><span style="color: #073763;"> terrestre, podendo ser uma estrela binária ou uma </span><i style="color: #073763;">estrela dupla óptica</i><span style="color: #073763;">, a última consistindo de duas estrelas que não possuem nenhuma conexão física, mas aparentam estar próximas umas das outras no céu, vistas da </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background-image: none; color: #073763; text-decoration: none;" title="Terra">Terra</a><span style="color: #073763;">. Estrelas duplas podem ser determinadas como ópticas se seus componentes possuem </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Movimento_pr%C3%B3prio" style="background-image: none; color: #073763; text-decoration: none;" title="Movimento próprio">movimento próprio</a><span style="color: #073763;"> ou </span><a href="http://pt.wikipedia.org/wiki/Velocidade_radial" style="background-image: none; color: #073763; text-decoration: none;" title="Velocidade radial">velocidade radial</a><span style="color: #073763;"> diferentes, ou medidas de </span><a href="http://pt.wikipedia.org/wiki/Paralaxe" style="background-image: none; color: #073763; text-decoration: none;" title="Paralaxe">paralaxe</a><span style="color: #073763;"> revelando que as distâncias da Terra das duas estrelas envolvidas são significativamente diferentes. Não se sabe se a maior parte das estrelas duplas conhecidas atualmente são estrelas binárias propriamente ditas ou estrelas duplas ópticas.</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Sistemas de estrelas binárias são muito importantes na <a href="http://pt.wikipedia.org/wiki/Astrof%C3%ADsica" style="background-image: none; text-decoration: none;" title="Astrofísica">astrofísica</a>, porque os cálculos de suas órbitas permitem que a <a href="http://pt.wikipedia.org/wiki/Massa" style="background-image: none; text-decoration: none;" title="Massa">massa</a> das estrelas componentes seja diretamente calculada, permitindo então uma estimativa indireta do seu <a href="http://pt.wikipedia.org/wiki/Raio_(geometria)" style="background-image: none; text-decoration: none;" title="Raio (geometria)">raio</a> e <a href="http://pt.wikipedia.org/wiki/Densidade" style="background-image: none; text-decoration: none;" title="Densidade">densidade</a>, bem como uma relação empírica entre massa e luminosidade, pela qual as massas de estrelas individuais podem ser estimadas.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Estrelas binárias são frequentemente detectadas visualmente, caso em que são chamadas de <i>binárias visuais</i>. Várias binárias visuais possuem longos períodos orbitais de vários séculos ou milênios e, portanto, as características de suas órbitas são pouco conhecidas ou não são conhecidas com precisão. Estrelas binárias também podem ser detectadas através de técnicas indiretas, tais como <a href="http://pt.wikipedia.org/wiki/Espectroscopia" style="background-image: none; text-decoration: none;" title="Espectroscopia">espectroscopia</a> (<i>binárias espectroscópicas</i>) ou <a href="http://pt.wikipedia.org/wiki/Astrometria" style="background-image: none; text-decoration: none;" title="Astrometria">astrometria</a> (<i>binárias astrométricas</i>). Se as estrelas de um sistema binário orbitam em um plano ao longo da linha de visão da Terra, tais estrelas se <a href="http://pt.wikipedia.org/wiki/Eclipse" style="background-image: none; text-decoration: none;" title="Eclipse">eclipsam</a> mutuamente; esses pares são chamados de <i><a href="http://pt.wikipedia.org/wiki/Bin%C3%A1ria_eclipsante" style="background-image: none; text-decoration: none;" title="Binária eclipsante">binárias eclipsantes</a></i> ou <i>binárias fotométricas</i>, devido ao fato de serem detectadas pela mudança de <a href="http://pt.wikipedia.org/wiki/Brilho_aparente" style="background-image: none; text-decoration: none;" title="Brilho aparente">brilho</a>durante eclipses e <a href="http://pt.wikipedia.org/wiki/Tr%C3%A2nsito_astron%C3%B4mico" style="background-image: none; text-decoration: none;" title="Trânsito astronômico">trânsitos estelares</a>.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Se as componentes de um sistema binário estelar estão suficientemente próximas uma da outra, as estrelas podem mutuamente distorcer <a href="http://pt.wikipedia.org/wiki/Gravidade" style="background-image: none; text-decoration: none;" title="Gravidade">gravitacionalmente</a> a <a href="http://pt.wikipedia.org/wiki/Atmosfera" style="background-image: none; text-decoration: none;" title="Atmosfera">atmosfera</a> da sua companheira. Em alguns casos, pode haver transferência gravitacional de material de uma estrela para outra, fazendo com que estrelas de sistemas binários atinjam estágios da <a href="http://pt.wikipedia.org/wiki/Evolu%C3%A7%C3%A3o_estelar" style="background-image: none; text-decoration: none;" title="Evolução estelar">evolução estelar</a> que seriam impossíveis em uma estrela solitária. Exemplos de sistemas binários incluem <a href="http://pt.wikipedia.org/wiki/Sirius" style="background-image: none; text-decoration: none;" title="Sirius">Sirius</a> e <a href="http://pt.wikipedia.org/wiki/Cygnus_X-1" style="background-image: none; text-decoration: none;" title="Cygnus X-1">Cygnus X-1</a> (do qual um dos membros é provavelmente um <a href="http://pt.wikipedia.org/wiki/Buraco_negro" style="background-image: none; text-decoration: none;" title="Buraco negro">buraco negro</a>). Estrelas binárias também são comuns como núcleo de várias <a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background-image: none; text-decoration: none;" title="Nebulosa planetária">nebulosas planetárias</a> e são progenitoras de <a href="http://pt.wikipedia.org/wiki/Nova" style="background-image: none; text-decoration: none;" title="Nova">novas</a> e <a href="http://pt.wikipedia.org/wiki/Supernova_tipo_Ia" style="background-image: none; text-decoration: none;" title="Supernova tipo Ia">supernovas tipo Ia</a>.</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; line-height: 19.2000007629395px;"><b>http://pt.wikipedia.org/wiki/Estrela_bin%C3%A1ria</b></span></span></div>
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<span dir="auto" style="background-color: white;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif; font-size: large;">Binária eclipsante</span></span></h1>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela <b>binária eclipsante</b>, ou <b>algólida</b>, é uma <a href="http://pt.wikipedia.org/wiki/Estrela_bin%C3%A1ria" style="background-image: none; text-decoration: none;" title="Estrela binária">estrela binária</a> em que o plano de órbita das duas estrelas se aproxima de tal forma da linha de visão do observador que as componentes passam por eclipses mútuos. As estrelas deste tipo que são também <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Bin%C3%A1ria_espectrosc%C3%B3pica" style="background-image: none; text-decoration: none;" title="Binária espectroscópica">binárias espectroscópicas</a> e em que se conhece a <a href="http://pt.wikipedia.org/wiki/Paralaxe" style="background-image: none; text-decoration: none;" title="Paralaxe">paralaxe</a> do sistema tornam-se importantes no que diz respeito à análise estelar.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A binárias eclipsantes são estrelas variáveis, não porque a luz de cada uma das estrelas componentes varie, mas por causa do movimento eclipsante. A estrela mais notável deste grupo é <a href="http://pt.wikipedia.org/wiki/Beta_Persei" style="background-image: none; text-decoration: none;" title="Beta Persei">Algol</a>, conhecida como "estrela demónio" pelos <a href="http://pt.wikipedia.org/wiki/%C3%81rabes" style="background-image: none; text-decoration: none;" title="Árabes">Árabes</a>, provavelmente porque terão notado a sua insólita variação de luminosidade.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A <a href="http://pt.wikipedia.org/wiki/Curva_de_luz" style="background-image: none; text-decoration: none;" title="Curva de luz">curva de luz</a> de uma binária eclipsante é caracterizada por períodos de luz praticamente constante com descidas abruptas na intensidade. Se uma das estrelas tiver maior dimensão que a outra, uma será obscurecida periodicamente por um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Eclipse_total" style="background-image: none; text-decoration: none;" title="Eclipse total">eclipse total</a> enquanto que a outra será obscurecida por um <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Eclipse_anular&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="Eclipse anular (página não existe)">eclipse anular</a>.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">O período <a href="http://pt.wikipedia.org/wiki/%C3%93rbita" style="background-image: none; text-decoration: none;" title="Órbita">orbital</a> de uma binária eclipsante pode ser determinado pelo estudo da curva de luz. Os tamanhos relativos de cada uma das estrelas podem ser determinados em termos de raios de órbita, a partir da observação da velocidade com que a luminosidade varia quando o disco da estrela mais próxima se sobrepõe ao disco da estrela mais distante. Se for uma estrela binária espectroscópica, também poderão ser determinados os elementos orbitais e, de forma relativamente fácil, a massa das estrelas, o que significa que se poderá também determinar as <a href="http://pt.wikipedia.org/wiki/Densidade" style="background-image: none; text-decoration: none;" title="Densidade">densidades</a> relativas de cada uma.</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763;"><b>http://pt.wikipedia.org/wiki/Bin%C3%A1ria_eclipsante</b></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 03h02m Declinação +38<sup>o</sup>.39<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 03h06m Declinação +40<sup>o</sup>.52<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão, </span></span></div>
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<span style="background-color: white;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; line-height: 13.5pt;">Editora Vozes, Petrópolis, ano de 1986</span><span style="font-family: Arial, Helvetica, sans-serif;"> </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.aradergalleries.com/detail.php?id=3660</span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Johann Bayer — Perseus</span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>M34 E M76</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>OS OBJETOS MESSIER</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>NA DIREÇÃO DA CONSTELAÇÃO PERSEUS</b></span></div>
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<h1>
Messier 34</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Open Cluster</a> M34 (NGC 1039)</i>, type 'd', in <a href="http://messier.obspm.fr/map/Per.html">Perseus</a></center>
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<a href="http://messier.obspm.fr/Jpg/m34.jpg"><img align="right" alt="[m34.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m34.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">02 : 42.0 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+42 : 47 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">1.4 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">5.5 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">35.0 (arc min)</td></tr>
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Discovered by Giovanni Batista Hodierna before 1654.</div>
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Open star cluster Messier 34 (M34, NGC 1039) is an intermediate aged open cluster of about 100 stars (according to H.S. Hogg), and lies about 1,400 light years and is scattered over 35 arc minutes, more than the diameter of the full Moon. This angular diameter corresponds to a linear 14 light years; Wallenquist has estimated a little more (42' corresponding to 18.5 light years).</div>
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M34 was probably first found by <a href="http://messier.obspm.fr/xtra/similar/hodierna.html">Giovanni Batista Hodierna</a> before 1654, and independently rediscovered by <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> in on <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M34">August 25, 1764</a>.</div>
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Open cluster M34 can quite easily be found (even with the naked eye under good conditions as a faint nebulous patch) as it lies just north of the line from Algol (Beta Persei) to Gamma Andromedae.</div>
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http://messier.obspm.fr/m/m034.html</div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1039 = M34 - Aglomerado Aberto</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Um aglomerado aberto e contendo cerca de 80 estrelas.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Aglomerado Aberto - Perseus<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 03h21m Declinação +48<sup>o</sup>.32<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 2,3 Distância kpc 0,17</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Diâmetro 240’ Tipo Espectral B1<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Messier 34</b> (também conhecido como <b>M34</b> ou <b>NGC 1039</b>) é um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-image: none; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> localizado na constelação de <a href="http://pt.wikipedia.org/wiki/Perseus" style="background-image: none; text-decoration: none;" title="Perseus">Perseus</a>. Foi descoberto por<a href="http://pt.wikipedia.org/wiki/Giovanni_Battista_Hodierna" style="background-image: none; text-decoration: none;" title="Giovanni Battista Hodierna">Giovanni Battista Hodierna</a> antes de <a href="http://pt.wikipedia.org/wiki/1654" style="background-image: none; text-decoration: none;" title="1654">1654</a> e incluido por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-image: none; text-decoration: none;" title="Charles Messier">Charles Messier</a> no seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-image: none; text-decoration: none;" title="Catálogo Messier">catálogo de objetos</a> em <a href="http://pt.wikipedia.org/wiki/1764" style="background-image: none; text-decoration: none;" title="1764">1764</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A M34 está a uma distância de 1.400 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-image: none; text-decoration: none;" title="Terra">Terra</a> e é constituído por 100 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Estrelas" style="background-image: none; text-decoration: none;" title="Estrelas">estrelas</a>. Abrange cerca de 35 ' no céu, o que equivale a ráio verdadeiro de 7 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; text-decoration: none;" title="Anos-luz">anos-luz</a>. O aglomerado só é visível a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Olho_nu" style="background-image: none; text-decoration: none;" title="Olho nu">olho nu</a> em condições muito escuras, fora das luzes da cidade. É bem visto com <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Bin%C3%B3culos" style="background-image: none; text-decoration: none;" title="Binóculos">binóculos</a>.</span><br />
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;">Aglomerado aberto M34</td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Giovanni_Battista_Hodierna" style="background: none; color: #0b0080; text-decoration: none;" title="Giovanni Battista Hodierna">Giovanni Battista Hodierna</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Perseus" style="background: none; color: #0b0080; text-decoration: none;" title="Perseus">Perseus</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">02<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 42.1<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">+42° 46′</td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">1.400 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">al</a> (0.4 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">5.5</td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">35.0′</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">7 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">al</a></td></tr>
<tr style="vertical-align: top;"><td>Nº estrelas</td><td style="background-color: #f8f8f8;">100</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 1039</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 34"><img alt="Messier 34" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; vertical-align: middle;" width="15" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Perseus_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Perseus constellation map.png" data-file-height="2559" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/09/Perseus_constellation_map.png/250px-Perseus_constellation_map.png" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/09/Perseus_constellation_map.png/375px-Perseus_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/09/Perseus_constellation_map.png/500px-Perseus_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<a href="http://pt.wikipedia.org/wiki/Messier_34"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Messier_34</span></a><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><a href="http://pt.wikipedia.org/wiki/Ficheiro:M34_2mass_atlas.jpg">http://pt.wikipedia.org/wiki/Ficheiro:M34_2mass_atlas.jpg</a></span><br />
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Messier 76</h1>
<i><a href="http://messier.obspm.fr/nebula.html">Planetary Nebula</a> M76 (NGC 650)</i>, type 3+6, in <a href="http://messier.obspm.fr/map/Per.html">Perseus</a><b>Little Dumbbell Nebula</b></center>
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<a href="http://messier.obspm.fr/Jpg/m76.jpg"><img align="right" alt="[m76.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m76.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">01 : 42.4 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+51 : 34 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">3.4 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">10.1 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">2.7x1.8 (arc min)</td></tr>
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Dicovered by Pierre Méchain in 1780.</div>
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Planetary Nebula Messier 76 (M76, NGC 650/651) is one of the faintest Messier Objects, and one of only four planetary nebulae in Messier's catalog, situated in the Eastern part of constellation Perseus.</div>
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M76 was discovered by <a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a> on September 5, 1780, who reported it to <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, who observed it on October 21, 1780, determined its position and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M76">added it to his catalog</a>. While Méchain found it to be a nebula without stars, Messier thought it was composed of small stars with some nebulosity, probably being fooled by foreground or background stars. <a href="http://messier.obspm.fr/xtra/Bios/rosse.html">Lord Rosse</a> erroneously suspected to have detected some spiral structure in this nebula. In 1866, <a href="http://messier.obspm.fr/xtra/Bios/huggins.html">William Huggins</a>, the pioneer of spectroscopy, found its spectrum to be gaseous, showing Nebulium lines. Pioneer astrophotographer <a href="http://messier.obspm.fr/xtra/Bios/roberts.html">Isaac Roberts</a> found that this was not a double, but a single nebula, and first suspected it might be a broad ring seen edgewise. In 1918, <a href="http://messier.obspm.fr/xtra/Bios/curtis.html">Heber D. Curtis</a> correctly classified it as a planetary nebula for the first time.</div>
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M76 is among the fainter Messier objects. It is known under the names <b>Little Dumbbell Nebula</b> (the most common), Cork Nebula, Butterfly Nebula, and Barbell Nebula, and it was given two NGC numbers ..............</div>
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LEIA MAIS</div>
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acessando</div>
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<a href="http://messier.obspm.fr/m/m076.html">http://messier.obspm.fr/m/m076.html</a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 650/1 - M 76 - Nebulosa Planetária</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 01h40m Declinação +51<sup>o</sup>.28<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo Nebulosa Planetária NP Dimensão 1,5 Magnitude 20 Magnitude da Estrela associada 17 Distância em anos-luz 15,0</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Uma nebulosa planetária pálida e denominada The Little Dumbbell.</b></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">A </span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Pequena Nebulosa do Haltere</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> (</span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Messier 76</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, </span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 650/651</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">) é uma </span><a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Nebulosa planetária">nebulosa planetária</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> que tem cerca de 1 ano-luz de diametro e está a cerca de 3 a 5 mil anos-luzes da Terra. É reconhecida como uma Nebulosa Planetária assim como seu homônimo mais brilhante, a M27 (a </span><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Nebulosa do Haltere">Nebulosa do Haltere</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">).</span><br />
<span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">..........................................</span><br />
<span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"><br /></span><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Sua aparência é semelhante à da </span><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;" title="Nebulosa do Haltere">nebulosa do Haltere</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, que justifica seu nome como a "Pequena Nebulosa do Haltere".</span><br />
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #a0d8a0; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Perseus" style="background: none; color: #0b0080; text-decoration: none;" title="Perseus">Perseus</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">01<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 42<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 24,00<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">+51° 34′ 31,00″</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">10,1</td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">2 500 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">al</a> (780 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>) <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a></td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">2.7 × 1.8 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a> <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #a0d8a0; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Raio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Raio">Raio</a></td><td style="background-color: #f8f8f8;">0,617 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">al</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude absoluta">Magnit. absol.</a></td><td style="background-color: #f8f8f8;">-0,6 (± 0,4</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #a0d8a0; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;">M76, NGC 650/651</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pequena Nebulosa do Haltere"><img alt="Pequena Nebulosa do Haltere" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" height="12" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; vertical-align: middle;" width="12" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Perseus_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Perseus constellation map.png" data-file-height="2559" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/09/Perseus_constellation_map.png/250px-Perseus_constellation_map.png" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/09/Perseus_constellation_map.png/375px-Perseus_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/09/Perseus_constellation_map.png/500px-Perseus_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Pequena_Nebulosa_do_Haltere">http://pt.wikipedia.org/wiki/Pequena_Nebulosa_do_Haltere</a></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Em Tempo, Caro Leitor:</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">M27, Dumbbell Nebula, a Nebulosa dos Halteres,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">pode ser encontrada</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em meu Trabalho sobre</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Vulpecula et Anser, a Raposa e o Ganso,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/08/vulpecula-et-anser-raposa-e-o-ganso.html</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><img alt="File:M76-RL5-DDmin-Gamma-LRGB 883x628.jpg" src="http://upload.wikimedia.org/wikipedia/commons/thumb/f/f0/M76-RL5-DDmin-Gamma-LRGB_883x628.jpg/800px-M76-RL5-DDmin-Gamma-LRGB_883x628.jpg" /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><a href="http://en.wikipedia.org/wiki/File:M76-RL5-DDmin-Gamma-LRGB_883x628.jpg">http://en.wikipedia.org/wiki/File:M76-RL5-DDmin-Gamma-LRGB_883x628.jpg</a></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18.234375px; text-align: start;">Image of planetary nebula M76 (</span><a class="external free" href="http://www.princeton.edu/~rvdb/images/NJP/m76.html" rel="nofollow">http://www.princeton.edu/~rvdb/images/NJP/m76.html</a><span style="line-height: 18.234375px; text-align: start;">) taken by Robert J. Vanderbei.</span></span><br />
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Philippe La Hire, <i>Planisphere celeste,</i> 1705<b><o:p></o:p></b></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;"><b>Capulus</b><b>. Aglomerados Abertos. A Espada de Perseu</b></span><span style="color: #073763;"><o:p></o:p></span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhSSggS2zRpQRT8cokimhsZgbnzXv1mONMaTHK3321s6pznYJBzUYJDYaLeJlfdDFQxH1gqrIz6_WCJKFAY3QvHzS7gasOsTYYpRYvgtDMEZGVSzgKjLo5NU8A9hCrgGIHc8fWP0q7nw8Hy/s1600/espada.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhSSggS2zRpQRT8cokimhsZgbnzXv1mONMaTHK3321s6pznYJBzUYJDYaLeJlfdDFQxH1gqrIz6_WCJKFAY3QvHzS7gasOsTYYpRYvgtDMEZGVSzgKjLo5NU8A9hCrgGIHc8fWP0q7nw8Hy/s640/espada.jpg" height="360" width="640" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes - Extrato de Perseus</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> <b style="line-height: 19.1875px; text-align: start;">NGC 1528</b><span style="line-height: 19.1875px; text-align: start;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Perseus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Perseus">constelação de Perseus</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="William Herschel">William Herschel</a><span style="line-height: 19.1875px; text-align: start;"> em 1790, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="line-height: 19.1875px; text-align: start;"> refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;"> (+6,4), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="line-height: 19.1875px; text-align: start;">amadores ou com equipamentos superiores.</span></span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_1528"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_1528</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 1513</b><span style="line-height: 19.1875px; text-align: start;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Perseus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Perseus">constelação de Perseus</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="William Herschel">William Herschel</a><span style="line-height: 19.1875px; text-align: start;"> em 1790, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="line-height: 19.1875px; text-align: start;"> refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;"> (+8,4), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="line-height: 19.1875px; text-align: start;">amadores ou com equipamentos superiores.</span></span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_1513"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_1513</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 1545</b><span style="line-height: 19.1875px; text-align: start;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Perseus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Perseus">constelação de Perseus</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="William Herschel">William Herschel</a><span style="line-height: 19.1875px; text-align: start;"> em 1790, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="line-height: 19.1875px; text-align: start;"> refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;"> (+6,2), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="line-height: 19.1875px; text-align: start;">amadores ou com equipamentos superiores.</span></span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_1545"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_1545</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 884 E 869 - Qui e H Persei -Aglomerado Duplo</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Um clássico exemplo de aglomerado aberto e visível para os olhos nus como uma pequena e inefável nuvem. Um objeto lindíssimo a ser observado com um telescópio de grande abertura e de baixa magnificação. Cada um dos aglomerados tem um diâmetro aparente de 30’ e um diâmetro real de cerca de 70 anos-luz.</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão, </span></span></div>
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<span style="background-color: white;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; line-height: 13.5pt;">Editora Vozes, Petrópolis, ano de 1986</span><span style="font-family: Arial, Helvetica, sans-serif;"> </span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj8gCuVhd77kvSFTJ66h-c1B146s07CcMTGXKx-3mBUreoveVMFREa2DtEaZL8NeUpd_-MiE0aDB2Z9xT3ylY3KQfkOAmH-mkAzo6pztRD4gfjDAyxzyEUQfG2JtCJF5F7qz6vPST3kRNdj/s1600/aglomerados+abertos.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj8gCuVhd77kvSFTJ66h-c1B146s07CcMTGXKx-3mBUreoveVMFREa2DtEaZL8NeUpd_-MiE0aDB2Z9xT3ylY3KQfkOAmH-mkAzo6pztRD4gfjDAyxzyEUQfG2JtCJF5F7qz6vPST3kRNdj/s640/aglomerados+abertos.jpg" height="284" width="640" /></span></a></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes - extrato Perseus</span></div>
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<b style="line-height: 19.1875px; text-align: start;">NGC 957</b><span style="line-height: 19.1875px; text-align: start;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Perseus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Perseus">constelação de Perseus</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="John Herschel">John Herschel</a><span style="line-height: 19.1875px; text-align: start;"> em 1831, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="line-height: 19.1875px; text-align: start;"> refletor com abertura de 18,6 polegadas. Devido a sua moderada </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;"> (+7,6), é visível apenas com </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="line-height: 19.1875px; text-align: start;">amadores ou com equipamentos superiores.</span></span><br />
<a href="http://pt.wikipedia.org/wiki/NGC_957"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_957</span></a><br />
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<b>NGC 869 - Aglomerado Aberto Eta Persei
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 02h17m
Declinação +57<sup>o</sup>.04<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 4,3
Distância kpc 2,15<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Diâmetro 30’ Tipo Espectral B1<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 869</b><span style="line-height: 19.1875px; text-align: start;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-image: none; line-height: 19.1875px; text-align: start;" title="Aglomerado aberto">aglomerado aberto</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Perseus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Perseus">constelação de Perseus</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto por </span><a href="http://pt.wikipedia.org/wiki/Hiparco" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Hiparco">Hiparco</a><span style="line-height: 19.1875px; text-align: start;"> em 130 a.C. Devido a sua moderada</span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;"> (+5,3), é visível a </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Olho_nu" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Olho nu">olho nu</a><span style="line-height: 19.1875px; text-align: start;"> em regiões distantes de cidades.</span> </span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_869"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_869</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 884/869 - The Double Cluster</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightsky.at/Photo/GalClu/h_chi_Per_WN.html">http://www.nightsky.at/Photo/GalClu/h_chi_Per_WN.html</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 884 - Aglomerado Aberto Xi Persei</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 02h21m
Declinação +57<sup>o</sup>.02<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 4,4
Distância kpc 2,48<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Diâmetro 30’ Tipo Espectral B0<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Um aglomerado duplo situado na mão da espada de Perseus, também
conhecido como A Espada de Perseus.
Visível a olho nú, com mais de 700 estrelas de 7<sup>a</sup>. e 12<sup>a</sup>.
Magnitude visuals. Espetáculo belíssimo,
também podendo ser observado por um par de binóculos simples. Perseus é o herói que voa no cavalo Pegasus,
o cavalo branco e alado, para salvar ndrômeda, acorrentada numa pedra, numa
ilha solitária. Perseus salva Andrômeda e
com ela se casa. <o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão, </span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; line-height: 13.5pt;">Editora Vozes, Petrópolis, ano de 1986</span><span style="font-family: Arial, Helvetica, sans-serif;"> </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 884</b><span style="line-height: 19.1875px; text-align: start;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Perseus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Perseus">constelação de Perseus</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto por </span><a href="http://pt.wikipedia.org/wiki/Hiparco" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Hiparco">Hiparco</a><span style="line-height: 19.1875px; text-align: start;"> em 130 a.C.. Devido a sua moderada</span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="line-height: 19.1875px; text-align: start;"> (+6,1), é fracamente visível a </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Olho_nu" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Olho nu">olho nu</a><span style="line-height: 19.1875px; text-align: start;">, mesmo em regiões distantes de cidades.</span></span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_884"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_884</span></a></div>
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<a href="http://cseligman.com/text/atlas/ngc8a.htm#869"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://cseligman.com/text/atlas/ngc8a.htm#869</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.blogger.com/blogger.g?blogID=7155777971455253706" name="869"><big><b>NGC 869 (= OCL 350 = h (or traditionally, part of </b></big></a><big><b><a href="http://www.blogger.com/blogger.g?blogID=7155777971455253706" title="Chi">χ</a>) Persei)</b></big><br />Known in prehistory<br />Recorded (130 B.C.E.) by <a href="http://cseligman.com/text/atlas/discoverers.htm#hipparchos</a">Hipparchus</a><br />A 5th-magnitude open cluster (type I3r) in <a href="http://cseligman.com/text/atlas/perseus.htm#869">Perseus</a> (RA 02 19 04.0, +57 08 06)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Per Dreyer, NGC 869 (GC 512, JH 207, WH VI 33, Hipparchus, 1860 RA 02 09 15, NPD 33 29.9) is "a remarkable object, a cluster, very very large, very rich, stars from 7th to 14th magnitude". (The description is taken from John Herschel's General Catalog.) The position precesses to RA 02 19 03.4, Dec +57 09 05, well within the 18 arcmin apparent size of the cluster, and in any event the millennia of naked-eye observations would firmly establish the identity. The designation of the star clusters has evolved over the last few hundred years. The last and greatest naked-eye observer, Tycho Brahe, measured a single position for the "nebulous star" which is the double cluster, and Johann Bayer designated that as <a href="http://www.blogger.com/blogger.g?blogID=7155777971455253706" title="Chi">χ</a> Persei. The title "h Persei" was presumably assigned to some faint star in the same neighborhood at a later date. However, in about the 1840's it became common usage to designate the brighter western cluster as h and the fainter eastern one as <a href="http://www.blogger.com/blogger.g?blogID=7155777971455253706" title="Chi">χ</a>, and that usage has stuck ever since. The point at which the stellar nature of the cluster was first noticed is not as clear, but it must have been known before 1654, when <a href="http://cseligman.com/text/atlas/discoverers.htm#hodierna">Hodierna</a> listed the pair as #3 in his catalog of nebulous objects that were resolved into stars by a telescope. Recent studies of the two clusters have somewhat revised previous estimates of their nature. It was previously thought that they are about 7000 light years away, but more recent estimates are around 10000 light years. Similarly, earlier estimates of their ages, based on the hottest, brightest stars still on the Main Sequence, have been substantially revised upward (primarily because of a large number of B-emission stars, which make it difficult to determine the "turn-off" point), from about 5 million years to around 12 to 14 million years for h Persei, and from around 3 million years to about 10 million years for <a href="http://www.blogger.com/blogger.g?blogID=7155777971455253706" title="Chi">χ</a>. Other estimates of the cluster characteristics remain as before: They are separated by only a few hundred light years, and probably originated in the same star-forming region. Each cluster contains more than 300 blue-white supergiants (very hot, very bright upper Main Sequence stars), which give off substantial amounts of UV and X-radiation as well as visible light, and since fainter stars are generally far more numerous than bright ones, the total membership of each cluster (including fainter stars) must measure in the thousands or even tens of thousands. Although hundreds of times younger than the Sun, the hottest, brightest stars in these clusters are near the end of their lives, and the most massive ones have already turned into red giants, the last stage of stellar "life". These red giants are particularly obvious in the eastern cluster, as seen in the images below. Each cluster is approaching us at a little over 20 km/sec, but the proper motions and space velocity appear to be unknown (that should change soon, as newer space telescopes are achieving remarkable results in measuring such quantities).</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="DSS image of open cluster NGC 869, or h Persei" border="1" src="http://cseligman.com/text/atlas/ngc869.jpg" height="750" title="DSS image of open cluster NGC 869, or h Persei" width="750" /><br />Above, a 30 arcmin wide "closeup" of NGC 869<br />Below, a 1.2 degree wide region showing h and <a href="http://www.blogger.com/blogger.g?blogID=7155777971455253706" title="Chi">χ</a> Persei (<a href="http://cseligman.com/text/atlas/ngc8a.htm#884">NGC 884</a>)<br /><img alt="DSS image of open clusters NGC 869 and 884, commonly known as h and Chi Persei" border="1" src="http://cseligman.com/text/stars/hchipersei.jpg" height="750" title="DSS image of open clusters NGC 869 and 884, commonly known as h and Chi Persei" width="750" /></span></div>
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<a href="http://cseligman.com/text/atlas/ngc8a.htm#869"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://cseligman.com/text/atlas/ngc8a.htm#869</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 1333</b><span style="line-height: 19.1875px; text-align: start;"> é uma </span><a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-image: none; line-height: 19.1875px; text-align: start;" title="Nebulosa">nebulosa</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Perseus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Perseus">constelação de Perseus</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Eduard_Sch%C3%B6nfeld&action=edit&redlink=1" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Eduard Schönfeld (página não existe)">Eduard Schönfeld</a><span style="line-height: 19.1875px; text-align: start;"> em 1855, usando um</span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="line-height: 19.1875px; text-align: start;"> refrator com abertura de 3 polegadas.</span></span></div>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/NGC_1333" style="background-color: white;">http://pt.wikipedia.org/wiki/NGC_1333</a></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Ficheiro:NGC_1333-IRAS_4B.jpg" style="background-color: white;">http://pt.wikipedia.org/wiki/Ficheiro:NGC_1333-IRAS_4B.jpg</a></span><br />
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<li style="margin-bottom: 0.1em;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="external free" href="http://www.nasa.gov/images/content/188092main_D-Protoplanetary-082907-full.jpg" rel="nofollow" style="background-image: url(data:image/png; background-position: 100% 50%; background-repeat: no-repeat no-repeat; padding-right: 13px;">http://www.nasa.gov/images/content/188092main_D-Protoplanetary-082907-full.jpg</a> (image) - <span style="line-height: 19.1875px;">NASA/JPL-Caltech</span></span></li>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 19.1875px; text-align: start;">NASA's Spitzer Space Telescope observed a fledgling solar system, like the one depicted in this artist's concept, and discovered deep within it enough water vapor to fill the oceans on Earth five times. This water vapor starts</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 115%;">Crédito da imagem: RA Gutermuth (Harvard-Smithsonian CfA) et
al / JPL-Caltech / NASA.</span><span style="line-height: 115%;"><br />
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<span style="background-position: initial initial; background-repeat: initial initial;">NGC 1333 é uma nebulosa de reflexão difusa de
cerca de 4 anos-luz de diâmetro, e tem menos de um milhão de anos de idade.
Está localizada a apenas cerca de 1.000 anos-luz de distância da Terra, na
constelação de Perseus norte, na borda da nuvem molecular Perseus.</span><br />
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<span style="background-position: initial initial; background-repeat: initial initial;">Veja mais em:<span class="apple-converted-space"> </span></span></span><a href="http://annesastronomynews.com/annes-image-of-the-day-reflection-nebula-ngc-1333/#.UhiuyUjwoVA.facebook" target="_blank"><span style="line-height: 115%; text-decoration: none;">http://annesastronomynews.com/annes-image-of-the-day-reflection-nebula-ngc-1333/#.UhiuyUjwoVA.facebook</span></a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Aglomerado de Estrelas em Perseus</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Um aglomerado que se movimenta e que contém mais de 100 estrelas
em torno a Perseus A (NGC 1275). Um
objeto maravilhoso para ser observado por bons pares de binóculos ou por
telescópios simples. Distante 570
anos-luz.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1275 - Perseus A - Galáxia</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma galáxia bem pouco usual que é uma intensa fonte de emissão de radio e de radiação de Raio-X. A matéria vem sendo ejetada da galáxia numa velocidade de mais de 2.400 km por segundo. A magnitude é de 13.0 e dista cerca de 300 milhões de anos-luz.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão, </span></span></div>
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<span style="background-color: white;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; line-height: 13.5pt;">Editora Vozes, Petrópolis, ano de 1986</span><span style="font-family: Arial, Helvetica, sans-serif;"> </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1275</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_lenticular" style="background-image: none; text-decoration: none;" title="Galáxia lenticular">lenticular</a> (S0) localizada na direcção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Perseus" style="background-image: none; text-decoration: none;" title="Perseus">Perseus</a>. Possui uma declinação de +41° 30' 41" e uma<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background-image: none;" title="Ascensão recta">ascensão recta</a> de 3 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; text-decoration: none;" title="Hora">horas</a>, 19 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; text-decoration: none;" title="Minuto">minutos</a> e 48,1 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; text-decoration: none;" title="Segundo">segundos</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A galáxia <b>NGC 1275</b> foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/14_de_Fevereiro" style="background-image: none; text-decoration: none;" title="14 de Fevereiro">14 de Fevereiro</a> de <a href="http://pt.wikipedia.org/wiki/1863" style="background-image: none; text-decoration: none;" title="1863">1863</a> por <a href="http://pt.wikipedia.org/wiki/Heinrich_Louis_d%27Arrest" style="background-image: none; text-decoration: none;" title="Heinrich Louis d'Arrest">Heinrich Louis d'Arrest</a>.</span></div>
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<a href="http://pt.wikipedia.org/wiki/NGC_1275"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/NGC_1275</span></a></div>
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<a href="http://cseligman.com/text/atlas/ngc12a.htm#1275"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://cseligman.com/text/atlas/ngc12a.htm#1275</span></b></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.blogger.com/blogger.g?blogID=7155777971455253706" name="1275" style="line-height: normal;"><big><b>NGC 1275 (= PGC 12429), Perseus A</b></big><br />Discovered (Oct 17, 1786) by </a><a href="http://cseligman.com/text/atlas/discoverers.htm#fwherschel" style="line-height: normal;">William Herschel</a><br style="line-height: normal;" /><span style="line-height: normal;">A 12th-magnitude peculiar galaxy (type cD + S0? pec) in </span><a href="http://cseligman.com/text/atlas/perseus.htm#1275" style="line-height: normal;">Perseus</a><span style="line-height: normal;"> (RA 03 19 48.1, Dec +41 30 41)</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1275 is the central, dominant member of the Perseus Cluster of galaxies. A Seyfert galaxy (type Sy 1.5). It is actually two galaxies, a dusty spiral galaxy whose distorted arms are seen as dark filaments against the background of the massive elliptical galaxy with which it is colliding (and probably merging). Each galaxy is distorted by the gravity of the other one, and as clouds of gas in the galaxies collide or are compressed by the interaction, bursts of star formation occur. Among other things, the interaction produces intense radio radiation (probably from gas falling into a supermassive black hole near the center of the elliptical galaxy), hence the galaxies' designation as Perseus A (meaning the brightest radio source in Perseus). As emphasized by a false-color composite in the bottom image, the collision creates glowing filaments of gas which are kept from dissipating by strong magnetic fields extending from the core of the elliptical galaxy. Based on a recessional velocity of 5265 km/sec, NGC 1275 is about 245 million light years away, in good agreement with redshift-independent distance estimates of 210 to 270 million light years. Given that and an apparent size of 2.3 by 1.7 arcmin, the pair span 165 thousand light years.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="SDSS image of the colliding pair of galaxies listed as NGC 1275, and also known as radio source Perseus A" border="1" src="http://cseligman.com/text/atlas/ngc1275.jpg" height="750" style="line-height: normal;" title="SDSS image of the colliding pair of galaxies listed as NGC 1275, and also known as radio source Perseus A" width="750" /><br style="line-height: normal;" /><span style="line-height: normal;">Above, a 3 arcmin wide closeup of NGC 1275</span><br style="line-height: normal;" /><span style="line-height: normal;">Below, a HST image of almost the same region, showing far more detail</span><br style="line-height: normal;" /><small style="line-height: normal;">(Image Credits: ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration, <a href="http://hubblesite.org/newscenter/archive/releases/2008/28/image/a/" target="external">NASA</a>)</small><br style="line-height: normal;" /><img alt="HST image of the colliding pair of galaxies listed as NGC 1275, and also known as radio source Perseus A" border="1" src="http://cseligman.com/text/atlas/ngc1275hst.jpg" height="750" style="line-height: normal;" title="HST image of the colliding pair of galaxies listed as NGC 1275, and also known as radio source Perseus A" width="750" /><br style="line-height: normal;" /><span style="line-height: normal;">Below, a detail of the nuclear region (the following image shows its position and orientation)</span><br style="line-height: normal;" /><small style="line-height: normal;">(Image Credits: Hubble Heritage Team (STScI/AURA), M. Donahue (STScI) & J. Trauger (JPL), <a href="http://heritage.stsci.edu/2003/14/big.html" target="nasa">NASA</a>)</small><br style="line-height: normal;" /><img alt="HST image of a portion of the colliding pair of galaxies listed as NGC 1275, and also known as radio source Perseus A" border="1" src="http://cseligman.com/text/galaxies/ngc1275.jpg" height="1030" style="line-height: normal;" title="HST image of a portion of the colliding pair of galaxies listed as NGC 1275, and also known as radio source Perseus A" width="750" /><br style="line-height: normal;" /><span style="line-height: normal;">Below, for reference, the HST detail is overlaid on the 3 arcmin wide SDSS image</span><br style="line-height: normal;" /><img alt="Composite of HST and SDSS images of the colliding pair of galaxies listed as NGC 1275, and also known as radio source Perseus A" border="1" src="http://cseligman.com/text/atlas/ngc1275a.jpg" height="750" style="line-height: normal;" title="Composite of HST and SDSS images of the colliding pair of galaxies listed as NGC 1275, and also known as radio source Perseus A" width="750" /><br style="line-height: normal;" /><span style="line-height: normal;">Below, an NOAO image uses an H</span><a href="http://www.blogger.com/blogger.g?blogID=7155777971455253706" style="line-height: normal;" title="Alpha">α</a><span style="line-height: normal;"> filter to emphasize the gaseous filaments</span><br style="line-height: normal;" /><small style="line-height: normal;">(Image Credits: C. Conselice/Caltech and WIYN/AURA/NSF/<a href="http://www.noao.edu/image_gallery/html/im0990.html" target="external">NOAO</a>)</small><br style="line-height: normal;" /><img alt="NOAO H-alpha image of the colliding pair of galaxies listed as NGC 1275, and also known as radio source Perseus A" border="1" src="http://cseligman.com/text/atlas/ngc1275noao.jpg" height="899" style="line-height: normal;" title="NOAO H-alpha image of the colliding pair of galaxies listed as NGC 1275, and also known as radio source Perseus A" width="750" /><br style="line-height: normal;" /><span style="line-height: normal;">Below, a 12 arcmin wide region centered on the galaxy; also shown are </span><a href="http://cseligman.com/text/atlas/ngc12a.htm#1272" style="line-height: normal;">NGC 1272</a><span style="line-height: normal;">, </span><a href="http://cseligman.com/text/atlas/ngc12a.htm#1273" style="line-height: normal;">1273</a><span style="line-height: normal;">, </span><a href="http://cseligman.com/text/atlas/ngc12a.htm#1274" style="line-height: normal;">1274</a><span style="line-height: normal;">, </span><a href="http://cseligman.com/text/atlas/ngc12a.htm#1277" style="line-height: normal;">1277</a><span style="line-height: normal;">, </span><a href="http://cseligman.com/text/atlas/ngc12a.htm#1278" style="line-height: normal;">1278</a><span style="line-height: normal;">and </span><a href="http://cseligman.com/text/atlas/ngc12a.htm#1279" style="line-height: normal;">1279</a><span style="line-height: normal;">, </span><a href="http://cseligman.com/text/atlas/ic19.htm#pgc12405" style="line-height: normal;">PGC 12405</a><span style="line-height: normal;"> (often misidentified as </span><a href="http://cseligman.com/text/atlas/ic19.htm#ic1907" style="line-height: normal;">IC 1907</a><span style="line-height: normal;">) and </span><a href="http://cseligman.com/text/atlas/ngc12a.htm#pgc12441" style="line-height: normal;">PGC 12441</a><span style="line-height: normal;"> (often misidentified as NGC 1279)</span><br style="line-height: normal;" /><img alt="SDSS image of region near the colliding pair of galaxies listed as NGC 1275, and also known as Perseus A; also shown are elliptical galaxies NGC 1272, 1274, 1278, PGC 12405 (often misidentified as IC 1907) and PGC 12241 (often misidentified as NGC 1279), and lenticular galaxies NGC 1273, 1277 and 1279" border="1" src="http://cseligman.com/text/atlas/ngc1275wide.jpg" height="750" style="line-height: normal;" title="SDSS image of region near the colliding pair of galaxies listed as NGC 1275, and also known as Perseus A; also shown are elliptical galaxies NGC 1272, 1274, 1278, PGC 12405 (often misidentified as IC 1907) and PGC 12241 (often misidentified as NGC 1279), and lenticular galaxies NGC 1273, 1277 and 1279" width="750" /></span></div>
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<a href="http://cseligman.com/text/atlas/ngc12a.htm#1275"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://cseligman.com/text/atlas/ngc12a.htm#1275</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 650/1 - M 76 - Nebulosa Planetária</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 01h40m
Declinação +51<sup>o</sup>.28<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo Nebulosa Planetária NP
Dimensão 1,5 Magnitude 20 Magnitude da Estrela associada 17 Distância em anos-luz 15,0</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma nebulosa planetária pálida e denominada The Little Dumbbell.</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão, </span></span></div>
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<span style="background-color: white;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; line-height: 13.5pt;">Editora Vozes, Petrópolis, ano de 1986</span><span style="font-family: Arial, Helvetica, sans-serif;"> </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18.234375px; text-align: start;">Image of planetary nebula M76 (</span><a class="external free" href="http://www.princeton.edu/~rvdb/images/NJP/m76.html" rel="nofollow" style="background-image: url(data:image/png; background-position: 100% 50%; background-repeat: no-repeat no-repeat; font-family: sans-serif; font-size: 12px; line-height: 18.234375px; padding-right: 13px; text-align: start; text-decoration: none;">http://www.princeton.edu/~rvdb/images/NJP/m76.html</a><span style="line-height: 18.234375px; text-align: start;">) taken by Robert J. Vanderbei.</span></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1348 - Perseus - Nebulosa de
Reflexão</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 03h43m
Declinação +32<sup>o</sup>.07<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo Nebulosa Planetária
NR Dimensão 3,0 Magnitude 21 <o:p></o:p></span></div>
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8 Distância em
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão, </span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; line-height: 13.5pt;">Editora Vozes, Petrópolis, ano de 1986</span><span style="font-family: Arial, Helvetica, sans-serif;"> </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">NGC 1348</b><span style="line-height: 19.1875px; text-align: start;"> é um </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="line-height: 19.1875px; text-align: start;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Perseus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Perseus">constelação de Perseus</a><span style="line-height: 19.1875px; text-align: start;">. O objeto foi descoberto pelo astrônomo </span><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="William Herschel">William Herschel</a><span style="line-height: 19.1875px; text-align: start;"> em 1790, usando um </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-image: none; line-height: 19.1875px; text-align: start;" title="Telescópio">telescópio</a><span style="line-height: 19.1875px; text-align: start;"> refletor com abertura de 18,6 polegadas.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 1039 = M34 - Aglomerado Aberto<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Um aglomerado aberto e contendo cerca de 80 estrelas.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Messier 34</b> (também conhecido como <b>M34</b> ou <b>NGC 1039</b>) é um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-image: none; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> localizado na constelação de <a href="http://pt.wikipedia.org/wiki/Perseus" style="background-image: none; text-decoration: none;" title="Perseus">Perseus</a>. Foi descoberto por<a href="http://pt.wikipedia.org/wiki/Giovanni_Battista_Hodierna" style="background-image: none; text-decoration: none;" title="Giovanni Battista Hodierna">Giovanni Battista Hodierna</a> antes de <a href="http://pt.wikipedia.org/wiki/1654" style="background-image: none; text-decoration: none;" title="1654">1654</a> e incluido por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-image: none; text-decoration: none;" title="Charles Messier">Charles Messier</a> no seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-image: none; text-decoration: none;" title="Catálogo Messier">catálogo de objetos</a> em <a href="http://pt.wikipedia.org/wiki/1764" style="background-image: none; text-decoration: none;" title="1764">1764</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A M34 está a uma distância de 1.400 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-image: none; text-decoration: none;" title="Terra">Terra</a> e é constituído por 100 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Estrelas" style="background-image: none; text-decoration: none;" title="Estrelas">estrelas</a>. Abrange cerca de 35 ' no céu, o que equivale a ráio verdadeiro de 7 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; text-decoration: none;" title="Anos-luz">anos-luz</a>. O aglomerado só é visível a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Olho_nu" style="background-image: none; text-decoration: none;" title="Olho nu">olho nu</a> em condições muito escuras, fora das luzes da cidade. É bem visto com <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Bin%C3%B3culos" style="background-image: none; text-decoration: none;" title="Binóculos">binóculos</a>.</span></div>
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<a href="http://pt.wikipedia.org/wiki/Messier_34"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Messier_34</span></a><br />
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<img alt="Ficheiro:M34 2mass atlas.jpg" src="http://upload.wikimedia.org/wikipedia/commons/thumb/7/7e/M34_2mass_atlas.jpg/508px-M34_2mass_atlas.jpg" height="640" width="542" /></span><br />
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<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="external free" href="http://www.ipac.caltech.edu/2mass/gallery/messiercat.html" rel="nofollow" style="background-image: url(data:image/png; background-position: 100% 50%; background-repeat: no-repeat no-repeat; padding-right: 13px; text-decoration: none;">http://www.ipac.caltech.edu/2mass/gallery/messiercat.html</a> Atlas Image [or Atlas Image mosaic] courtesy of 2MASS/UMass/IPAC-Caltech/NASA/NSF.</span></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Aglomerado Aberto - Perseus</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 03h21m
Declinação +48<sup>o</sup>.32<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 2,3
Distância kpc 0,17<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Diâmetro 240’ Tipo
Espectral B1<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão, </span></span></div>
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<span style="background-color: white;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; line-height: 13.5pt;">Editora Vozes, Petrópolis, ano de 1986</span><span style="font-family: Arial, Helvetica, sans-serif;"> </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1499 - Nebulosa Califórnia</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma nebulosa difusa e difícil de ser observada visualmente.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> <a href="http://cseligman.com/text/atlas/ngc14a.htm">http://cseligman.com/text/atlas/ngc14a.htm</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.blogger.com/blogger.g?blogID=7155777971455253706" name="1499"><big><b>NGC 1499, the California Nebula</b></big><br />Discovered (Nov 3, 1885) by </a><a href="http://cseligman.com/text/atlas/discoverers.htm#barnard">Edward Barnard</a><br />A 5th-magnitude emission nebula in <a href="http://cseligman.com/text/atlas/perseus.htm#1499">Perseus</a> (RA 04 03 14.0, Dec +36 22 00)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The first IC notes (per <a href="http://cseligman.com/text/atlas/discoverers.htm#scheiner">Scheiner</a>) "is about half a degree in length". Apparent size 200 by 60 arcmin.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="DSS image of emission nebula NGC 1499, the California Nebula, rotated to show more detail" border="1" src="http://cseligman.com/text/atlas/ngc1499.jpg" height="1669" title="DSS image of emission nebula NGC 1499, the California Nebula, rotated to show more detail" width="750" /></span></div>
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<a href="http://cseligman.com/text/atlas/ngc14a.htm"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://cseligman.com/text/atlas/ngc14a.htm</span></a></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">THE PERSEUS-PISCES SUPERCLUSTER</span></b></div>
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<a href="http://www.atlasoftheuniverse.com/superc/perpsc.html"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.atlasoftheuniverse.com/superc/perpsc.html</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Aglomerado de Galáxias<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN"><a href="http://en.wikipedia.org/wiki/Abell_426" title="Abell 426"><span lang="PT" style="text-decoration: none;">Abell 426</span></a></span><span lang="PT"> - O Aglomerado Perseus<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Superaglomerado Perseus-Pisces foi um dos primeiros superaglomerados a serem descobertos. Certamente este superaglomerado vem atuando
de forma importante para o estudo das amplas escalas estruturais do universo e,
por causa de tantos estudos, é um dos superaglomerados mais bem
conhecidos. Hoje sabemos que o universo
consiste de imensos superaglomerados de galáxias rodeando imensos vazios.<o:p></o:p></span></div>
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<img alt="The Perseus-Pisces Supercluster" src="http://www.atlasoftheuniverse.com/superc/perpsc.gif" /></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O superaglomerado Perseus - Pisces é o mais óbvio do céu.
No entanto, como todos os demais de sua espécie, é muito pálido para ser
visto a olho nú. Este superaglomerado é
uma longa e densa muralha de galáxias numa extensão de quase 300 milhões de
anos-luz. Ao final do supercluster
existe o massivo Perseus aglomerado <b>(A426</b>) um dos mais massivos aglomerados de
galáxias em 500 milhões de anos-luz.<o:p></o:p></span></div>
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<img alt="The Perseus Cluster (Abell 426)" src="http://annesastronomynews.com/wp-content/uploads/2012/02/The-Perseus-Cluster-Abell-426-contains-thousands-of-galaxies-immersed-in-a-vast-cloud-of-multimillion-degree-gas.-Near-the-cluster-center-237-million-ly-away-is-the-clusters-dominant-galaxy-NGC-1275.jpg" /></span><br />
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<a href="http://annesastronomynews.com/photo-gallery-ii/galaxies-clusters/the-perseus-cluster-abell-426-contains-thousands-of-galaxies-immersed-in-a-vast-cloud-of-multimillion-degree-gas-near-the-cluster-center-237-million-ly-away-is-the-clusters-dominant-galaxy-ngc/">http://annesastronomynews.com/photo-gallery-ii/galaxies-clusters/the-perseus-cluster-abell-426-contains-thousands-of-galaxies-immersed-in-a-vast-cloud-of-multimillion-degree-gas-near-the-cluster-center-237-million-ly-away-is-the-clusters-dominant-galaxy-ngc/</a></span><br />
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<span style="background-color: white; color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">The Perseus Cluster (</span><span style="font-family: Arial, Helvetica, sans-serif;">Abell 426</span><span style="font-family: Arial, Helvetica, sans-serif;">), located 237 million light-years awayin the constellation of Perseus, contains thousands of galaxies immersed in a vast cloud of multimillion degree gas. Near the cluster center is the cluster’s dominant galaxy NGC 1275 (also known as Perseus A).</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Image Credit: Jean-Charles Cuillandre (CFHT) & Giovanni Anselmi (Coelum Astronomia), Hawaiian Starlight</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O aglomerado Perseus A426 é o segundo mais próximo dos reais
ricos aglomerados de galáxias que contêm milhares de galáxias. O mais próximo - A3627 - situa-se quase que
escondido pelo plano de nossa galáxia e não é
fácil de ser observado.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Não somente o superaglomerado Perseus-Pisces é o mais óbvio de
sua espécie no céu como também situa-se próximo ao mais obvio Vazio no
céu. O Vazio Taurus - Taurus Void - é um
imenso Vazio circular cercado de muralhas de galáxias em cada um de seus
lados. O Vazio possui um diâmetro de
cerca de 100 milhões de anos-luz. Muitas
das galáxias encontradas na área do Vazio pertencem ao plano de fundo, são
galáxias situadas por detrás do Vazio.<o:p></o:p></span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">THE PERSEUS-PISCES SUPERCLUSTER</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.atlasoftheuniverse.com/superc/perpsc.html">http://www.atlasoftheuniverse.com/superc/perpsc.html</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">The Night Sky Atlas</span></h1>
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<tr><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Visible in July before dawn, to March after dusk, best in November.</span></td></tr>
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<b><span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Named Stars Index - The Night Sky Atlas<o:p></o:p></span></span></b></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Perseus: Visible
in August before dawn, to April after dusk, best in December.<o:p></o:p></span></span></div>
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<tr>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3.136&declination=40.956&viewAngle=25">Algol</a><o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">β<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Beta<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 0cm 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">´the ghoul´<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt;"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.astro.uiuc.edu/~jkaler/sow/algol.html" target="starnotes" title="Jim Kaler´s star notes for Algol">Jim Kaler Notes</a><o:p></o:p></span></div>
</td>
</tr>
<tr>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3.739&declination=32.288&viewAngle=25">Atik</a><o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">ο<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Omicron<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 0cm 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">´shoulder´ (of the Pleiades)<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt;"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.astro.uiuc.edu/~jkaler/sow/atik.html" target="starnotes" title="Jim Kaler´s star notes for Atik">Jim Kaler Notes</a><o:p></o:p></span></div>
</td>
</tr>
<tr>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3.983&declination=35.791&viewAngle=25">Menkib</a><o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">ξ<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Xi<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 0cm 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">´shoulder´<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt;"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.astro.uiuc.edu/~jkaler/sow/menkib.html" target="starnotes" title="Jim Kaler´s star notes for Menkib">Jim Kaler Notes</a><o:p></o:p></span></div>
</td>
</tr>
<tr>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3.405&declination=49.861&viewAngle=25">Mirfak or Marfak</a><o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">α<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Alpha<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 0cm 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">´elbow´<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 0cm 0cm 0cm;"></td>
</tr>
</tbody></table>
</div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/starnames.jsp">http://www.nightskyatlas.com/starnames.jsp</a><o:p></o:p></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><br /></span></div>
<h1 align="center" style="text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">DSO
Names - The Night Sky Atlas<o:p></o:p></span></span></h1>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><br /></span></div>
<div align="center">
<table border="0" cellpadding="0" cellspacing="0" class="MsoNormalTable">
<tbody>
<tr style="height: 27.0pt; mso-yfti-firstrow: yes; mso-yfti-irow: 0;">
<td colspan="5" style="height: 27.0pt; padding: 0cm 0cm 0cm 0cm;" valign="bottom"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Perseus: Visible
in August before dawn, to April after dusk, best in December.<o:p></o:p></span></span></div>
</td>
</tr>
<tr>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3.3667&declination=49.0&viewAngle=20.0">Alpha Persei Cluster</a><o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"></td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">03h 22.0m<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">+49° 00.0´<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 225.0pt;" valign="top" width="300"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Melotte 20 open cluster<o:p></o:p></span></div>
</td>
</tr>
<tr>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3.4633&declination=50.5833&viewAngle=20.0">Andromeda VII</a><o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"></td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">03h 27.8m<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">+50° 35.0´<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 225.0pt;" valign="top" width="300"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">also Cassiopeia dSph, in
Local Group<o:p></o:p></span></span></div>
</td>
</tr>
<tr>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=1.705&declination=51.5717&viewAngle=20.0">Barbell Nebula</a><o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">M76<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">01h 42.3m<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">+51° 34.3´<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 225.0pt;" valign="top" width="300"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">also Little Dumbbell,
Butterfly, or Cork Nebula; Apple Core Nebula (Mike Frazier)<o:p></o:p></span></span></div>
</td>
</tr>
<tr>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=4.0533&declination=36.3667&viewAngle=20.0">California Nebula</a><o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">NGC1499<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">04h 03.2m<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">+36° 22.0´<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 225.0pt;" valign="top" width="300"></td>
</tr>
<tr>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3.4633&declination=50.5833&viewAngle=20.0">Cassiopeia dSph</a><o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"></td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">03h 27.8m<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">+50° 35.0´<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 225.0pt;" valign="top" width="300"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">also Andromeda VII, in
Local Group<o:p></o:p></span></span></div>
</td>
</tr>
<tr>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=2.3717&declination=57.1333&viewAngle=20.0">Chi Persei</a><o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">NGC884<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">02h 22.3m<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">+57° 08.0´<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 225.0pt;" valign="top" width="300"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Double Cluster with NGC
869 (h Persei)<o:p></o:p></span></span></div>
</td>
</tr>
<tr>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=1.705&declination=51.5717&viewAngle=20.0">Cork Nebula</a><o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">M76<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">01h 42.3m<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">+51° 34.3´<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 225.0pt;" valign="top" width="300"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">also Little Dumbbell,
Butterfly, or Barbell Nebula; Apple Core Nebula (Mike Frazier)<o:p></o:p></span></span></div>
</td>
</tr>
<tr>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=2.3167&declination=57.1283&viewAngle=20.0">Double Cluster</a><o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">NGC869 NGC884<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">02h 19.0m<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">+57° 07.7´<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 225.0pt;" valign="top" width="300"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">h+Chi Persei<o:p></o:p></span></div>
</td>
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<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=1.705&declination=51.5717&viewAngle=20.0">Dumbbell Nebula, Little</a><o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">M76<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">01h 42.3m<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">+51° 34.3´<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 225.0pt;" valign="top" width="300"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">(Sky Catalogue 2000) also
Cork, Butterfly, or Barbell Nebula; Apple Core Nebula (Mike Frazier)<o:p></o:p></span></span></div>
</td>
</tr>
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<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=2.3167&declination=57.1283&viewAngle=20.0">H Persei</a><o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">NGC869<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">02h 19.0m<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">+57° 07.7´<o:p></o:p></span></div>
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<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 225.0pt;" valign="top" width="300"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Double Cluster with NGC
884 (Chi Persei)<o:p></o:p></span></span></div>
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<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=1.705&declination=51.5717&viewAngle=20.0">Little Dumbbell Nebula</a><o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">M76<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">01h 42.3m<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">+51° 34.3´<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 225.0pt;" valign="top" width="300"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">(Sky Catalogue 2000) also
Cork, Butterfly, or Barbell Nebula; Apple Core Nebula (Mike Frazier)<o:p></o:p></span></span></div>
</td>
</tr>
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<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3.33&declination=41.5117&viewAngle=20.0">Perseus A</a><o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">NGC1275 NGC1276<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">03h 19.8m<o:p></o:p></span></div>
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<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">+41° 30.7´<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 225.0pt;" valign="top" width="300"></td>
</tr>
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<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=2.3167&declination=57.1283&viewAngle=20.0">Perseus Double Cluster</a><o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">NGC869 NGC884<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">02h 19.0m<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">+57° 07.7´<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 225.0pt;" valign="top" width="300"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">h+Chi Persei<o:p></o:p></span></div>
</td>
</tr>
<tr>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=2.7017&declination=42.7617&viewAngle=20.0">Spiral Cluster</a><o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 112.5pt;" valign="top" width="150"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">M34<o:p></o:p></span></div>
<div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><br /></span></div>
<div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><br /></span></div>
<div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/dsoNames.jsp">http://www.nightskyatlas.com/dsoNames.jsp</a><o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">02h 42.1m<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">+42° 45.7´<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt; width: 225.0pt;" valign="top" width="300"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">(Jeff Bondono)<o:p></o:p></span></div>
<div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><br /></span></div>
<div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><br /></span></div>
<div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><br /></span></div>
</td>
</tr>
</tbody></table>
</div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><br /></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><br /></span></div>
<h1 align="center" style="text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Asterisms
- The Night Sky Atlas<o:p></o:p></span></span></h1>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><br /></span></div>
<div align="center">
<table border="0" cellpadding="0" cellspacing="0" class="MsoNormalTable" style="mso-cellspacing: 0cm; mso-padding-alt: 0cm 0cm 0cm 0cm; mso-yfti-tbllook: 1184; width: 800px;">
<tbody>
<tr style="height: 27.0pt; mso-yfti-firstrow: yes; mso-yfti-irow: 0;">
<td colspan="4" style="height: 27.0pt; padding: 0cm 0cm 0cm 0cm;" valign="bottom"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Perseus: Visible
in July before dawn, to March after dusk, best in November.<o:p></o:p></span></span></div>
</td>
</tr>
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<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3&declination=40">Medusa´s Head</a><o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">3<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">2 deg<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Beta; Omega; Rho; Pi; 20;
15; 12 Persei; the Gorgon´s Head<o:p></o:p></span></span></div>
</td>
</tr>
<tr>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3.405&declination=49.8667">Saxophone</a><o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">2<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">2 deg<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Alpha Per Cluster; Mel
20; long curved star chain like musical instrument<o:p></o:p></span></span></div>
</td>
</tr>
<tr>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=3.6667&declination=48">Segment of Perseus</a><o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">3<o:p></o:p></span></div>
</td>
<td nowrap="" style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">25 deg<o:p></o:p></span></div>
</td>
<td style="padding: 0cm 3.75pt 0cm 3.75pt;" valign="top"><div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">A chain of the major
stars of Perseus; In order: Eta; Gamma; Alpha; Delta; Epsilon and Zeta<o:p></o:p></span></span></div>
</td>
</tr>
</tbody></table>
</div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://www.nightskyatlas.com/asterisms.jsp"><span lang="EN-US">http://www.nightskyatlas.com/asterisms.jsp</span></a><o:p></o:p></span></div>
<div align="center" class="MsoNormal" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><br /></span></div>
<h1 align="center" style="text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Principal
Stars of Perseus - The Night Sky Atlas<span style="font-weight: normal;"><o:p></o:p></span></span></span></h1>
<h1 align="center" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small; font-weight: normal;"><a href="http://www.nightskyatlas.com/stardata.jsp?id=PER"><span lang="EN-US">http://www.nightskyatlas.com/stardata.jsp?id=PER</span></a><o:p></o:p></span></h1>
<h1 align="center" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small; font-weight: normal;"> </span></h1>
<h1 align="center" style="text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small; font-weight: normal;">Multiple
Stars of Perseus - The Night Sky Atlas<o:p></o:p></span></span></h1>
<h1 align="center" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small; font-weight: normal;"><a href="http://www.nightskyatlas.com/multipleStars.jsp?id=PER"><span lang="EN-US">http://www.nightskyatlas.com/multipleStars.jsp?id=PER</span></a><o:p></o:p></span></h1>
<h1 align="center" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small; font-weight: normal;"> </span></h1>
<h1 align="center" style="text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small; font-weight: normal;">NGC
Objects in Perseus - The Night Sky Atlas<o:p></o:p></span></span></h1>
<h1 align="center" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small; font-weight: normal;"><a href="http://www.nightskyatlas.com/ngcData.jsp?id=PER"><span lang="EN-US">http://www.nightskyatlas.com/ngcData.jsp?id=PER</span></a><o:p></o:p></span></h1>
<h1 align="center" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small; font-weight: normal;"> </span></h1>
<h1 align="center" style="text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small; font-weight: normal;">NGC
Objects in Perseus - The Night Sky Atlas<o:p></o:p></span></span></h1>
<h1 align="center" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small; font-weight: normal;"><a href="http://www.nightskyatlas.com/ngcData.jsp?id=PER"><span lang="EN-US">http://www.nightskyatlas.com/ngcData.jsp?id=PER</span></a><span lang="EN-US"><o:p></o:p></span></span></h1>
<h1 align="center" style="text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small; font-weight: normal;"> </span></span></h1>
<h1 align="center" style="text-align: center;">
<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small; font-weight: normal;">IC
Objects in Perseus - The Night Sky Atlas<o:p></o:p></span></span></h1>
<h1 align="center" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small; font-weight: normal;"><a href="http://www.nightskyatlas.com/icData.jsp?id=PER"><span lang="EN-US">http://www.nightskyatlas.com/icData.jsp?id=PER</span></a><o:p></o:p></span></h1>
<h1 align="center" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small; font-weight: normal;"> </span></h1>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small; font-weight: normal;">Galaxy
Clusters of Perseus - The Night Sky Atlas<o:p></o:p></span></span></h1>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">
</span><br />
<h1 align="center" style="text-align: center;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small; font-weight: normal;"><span lang="EN-US"><a href="http://www.nightskyatlas.com/catAbell.jsp?id=PER">http://www.nightskyatlas.com/catAbell.jsp?id=PER</a></span><span lang="EN-US"><o:p></o:p></span></span></h1>
<h1 align="center" style="text-align: center;">
<div style="font-size: medium; font-weight: normal;">
<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><img src="http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_004.jpg" /></span></span></span></div>
<div style="font-size: medium; font-weight: normal;">
<a href="http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_004.jpg"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_004.jpg</span></a></div>
<div style="font-size: medium; font-weight: normal;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
</h1>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 16.8pt; margin: 0cm; text-align: -webkit-center;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 16.8pt; margin: 0cm; text-align: -webkit-center;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 16.8pt; margin: 0cm; text-align: -webkit-center;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 16.8pt; margin: 0cm; text-align: -webkit-center;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 16.8pt; margin: 0cm; text-align: -webkit-center;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 16.8pt; margin: 0cm; text-align: -webkit-center;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 16.8pt; margin: 0cm; text-align: -webkit-center;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 16.8pt; margin: 0cm; text-align: -webkit-center;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 16.8pt; margin: 0cm; text-align: -webkit-center;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 16.8pt; margin: 0cm; text-align: -webkit-center;">
<b><br /></b></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 16.8pt; margin: 0cm; text-align: -webkit-center;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 16.8pt; margin: 0cm; text-align: -webkit-center;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 16.8pt; margin: 0cm; text-align: -webkit-center;">
<b><br /></b></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 16.8pt; margin: 0cm; text-align: -webkit-center;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,<o:p></o:p></b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 16.8pt; margin: 0cm; text-align: -webkit-center;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span></div>
</div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"><img src="http://www.raremaps.com/maps/large/36137.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 18px;"><a href="http://www.raremaps.com/gallery/enlarge/36137" style="color: #274e13; text-decoration: none;">http://www.raremaps.com/gallery/enlarge/36137</a></span><br />
<div class="productDetailItem" style="background-color: white; border: 0px; color: #073763; font-family: verdana, arial, georgia, sans-serif; font-size: 12px; margin-bottom: 1em; padding: 0px 0px 10px;">
<strong>Title: </strong>Andromede, Persee, Le Triangle (Andromeda, Perseus & Triangle)<br />
<strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1260" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; text-decoration: none;">John Flamsteed</a> / <a href="https://www.raremaps.com/gallery/browse/creator_id/1454" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; text-decoration: none;">MJ Fortin</a></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>REFERÊNCIAS BIBLIOGRÁFICAS IMPRESSAS:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">COMPILAÇÃO E TRADUÇÃO literal
(quando necessária) de Janine Milward:<o:p></o:p></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As Cartas Celestes foram realizadas por Mario Jaci Monteiro e escaneadas
por Janine<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT" style="background-position: initial initial; background-repeat: initial initial;">- </span><b>Mario Jaci
Monteiro</b> , <b>As
Constelações, Cartas Celestes</b> -<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
<div align="center" class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: center;">
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
</div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial;">- <b>Wil Tirion
- Atlas of the Night Sky</b> - The Hamlyn Publishing Group Limited,
London, England</span><span lang="EN-US" style="mso-ansi-language: EN-US; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial;">- <b>Antonin
Rükl - The Hamlyn Encyclopedia of Stars & Planets</b> - The Hamlyn
Publishng Group Limited, London, England</span><span lang="EN-US" style="mso-ansi-language: EN-US; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial;">- <b>Richard Hinckley
Allen, Star Names, Their Lore and Meaning</b>, Dover Publications, Inc, New
York, USA</span><span lang="EN-US" style="mso-ansi-language: EN-US; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT" style="background-position: initial initial; background-repeat: initial initial;">- <b>Bernard
Pellequer - Pequeno Guia do Céu</b> - Editora Martins Fontes, São Paulo,
Brasil</span><o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- <b>Identificação do Céu</b> (Livro
que foi sendo revisado e reeditado algumas vezes) de autoria de <b>Fernando
Vieira</b>,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Secretaria Municipal de Cultura, Fundação
Planetário da Cidade do Rio de Janeiro<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(com dedicatória do próprio autor para mim em Curso
de Identificação do Céu,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em 30/07/1999))<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do <b>Atlas Celeste</b><o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">de autoria de <b>Ronaldo Rogério de Freitas
Mourão</b>,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(com dedicatória do próprio autor para mim<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em evento realizado no Museu de Astronomia do Rio
de Janeiro,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em 16/06/1989)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As Cartas Celestes foram realizadas por Mario Jaci Monteiro e escaneadas
por Janine<span lang="PT"><br />
<!--[if !supportLineBreakNewLine]--><br />
<!--[endif]--></span><o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT" style="background-position: initial initial; background-repeat: initial initial;">- </span><b>Mario Jaci
Monteiro</b> , <b>As
Constelações, Cartas Celestes</b> -<o:p></o:p></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Apoio:
CARJ/MEC/CAPES/PADCT-SPEC - com dedicatória do autor para
mim, em março de 2004 (quando Mário Jaci generosamente me presenteou com um
instrumento de observação (kepleriano) artesanalmente construído por ele).</span></div>
</div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="DSS image of emission nebula NGC 1499, the California Nebula, rotated to show more detail" border="1" src="http://cseligman.com/text/atlas/ngc1499.jpg" title="DSS image of emission nebula NGC 1499, the California Nebula, rotated to show more detail" /></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://cseligman.com/text/atlas/ngc14a.htm">http://cseligman.com/text/atlas/ngc14a.htm</a></span><br />
<br />
<div align="center" class="MsoNormal" style="line-height: 14.25pt;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="PT">Da Terra ao Céu<o:p></o:p></span></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="PT"> e ao Infinito</span></b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelações, Estrelas e Objetos Celestes<o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(sob o ponto de vista do Mundo Ocidental)<o:p></o:p></span></span></div>
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<span lang="PT"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Suas histórias, seus mitos, seus significados e suas sintetizadas descrições<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">Reunião das Informações e Compilação,</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">Tradução para a língua portuguesa (em alguns momentos)</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="PT">bem como Comentários Pessoais:</span><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><span lang="PT">Janine Milward</span></i><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado. Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Alguns dados<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(tais como Ascensão Reta e Declinação, em muitos dos casos)<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">são época/equinócio 1980<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e devem requerer do Caminhante do Céu<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial;">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial;"> </span></i></span><em><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial;"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial;"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial;"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial;">The</span><span class="apple-converted-space"><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial;"> </span></span><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial;">Internet STELLAR DATABASE</span><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/"><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial;">http://www.stellar-database.com/</span></a><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial;"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<o:p></o:p></span></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-7155777971455253706.post-24933493090740307202013-08-20T08:00:00.002-07:002016-12-16T02:51:50.762-08:00PEGASUS, O CAVALO ALADO<div align="center" class="MsoNormal" style="text-align: center;">
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Meu Projeto</span></div>
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<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><span style="font-size: small;">Da Terra ao Céu ....</span></span></a></h1>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><span style="font-size: small;">.....<a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;">e ao Infinito </a></span></span></h1>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; text-decoration: none;"><span style="font-size: small;">- As 88 Constelações</span></a></span></h1>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/" style="color: #274e13; line-height: 18px; text-decoration: none;"><span style="font-size: small;">http://daterraaoceueaoinfinito.blogspot.com.br/</span></a></span></h1>
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<span style="font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são como janelas que se abrem para a infinitude do universo</span><br /><span style="font-family: Arial, Helvetica, sans-serif;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra...;</span><br /><span style="font-family: Arial, Helvetica, sans-serif;">bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este por nossa mente sendo conscientizado.</span><br /><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Quer dizer, nossa mente é tão infinita quanto infinito é o Cosmos.</span><br /><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span><br /><span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Olá!</span><br />
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span>
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Se você estiver sob um céu mais escuro e transparente</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">e </span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">em um lugar mais distanciado das luzes poluentes urbanas,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">poderá identificar o Grande Quadrado </span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">de estrelas </span></span><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">que formam </span><br />
<span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">o corpanzil do Cavalo Alado Pegasus</span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">ao mesmo tempo </span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">em que uma dessas estrelas </span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">- Alpheratz -</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">também atua enquanto estrela-alpha Andromedae!</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span>
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Aliás,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">se você tiver em mãos</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">um simpático par de binóculos,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">tente encontrar</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">um tantinho próximo visualmente a Alpheratz</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">a belíssima M31,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">ou seja,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">a Galáxia Andrômeda,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">nossa querida irmã...</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">(com quem possivelmente</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">nos fusionaremos</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">mais dia, menos dia,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">algum dia</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">em futuro tão distante</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">que nem dá para pensarmos</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">sobre isso</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">agora.</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span>
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Nesta Postagem, Caro Leitor,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">encontre alguma informação</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">sobre a interessante constelação Pegasus,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">o Cavalo Alado,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">sobre algumas de suas estrelas,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">sobre Alpheratz fazendo parte</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">tanto de Pegasus quanto de Andromeda;</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">sobre o Ponto Vernal</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">que situa-se nos Peixes</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">que nadam nos mares</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">sobrevoados por Pégaso;</span></span><br />
<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white;">sobre algumas galáxias</span></span><br />
<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white;">e aglomerados</span></span><br />
<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white;">(inclusive o famoso Quinteto/Quarteto de Stephan);</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">sobre M15,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">o único Objeto Messier</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">nesta simpática constelação</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">e que situa-se bem na pontinha</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">do nariz do Cavalo Alado,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">marcado pela estrela Enif,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">estrela-epsilon Pegasi,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">a estrela mais brilhante</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">desse asterismo voador.</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span>
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Ah, bem ao final,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Caro Leitor,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">encontre os textos</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">sempre profícuos em informações</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">sobre a constelação Pegasus</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">e suas estrelas</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">advindos das transcrições </span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">da mente incrível</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">de Richard H. Allen</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">em seu livro</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Star Names,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Their Lore and Meaning.</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span>
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Com um abraço estrelado,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Janine Milward</span></span><br />
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Stellarium</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>O MITO DE ANDROMEDA, </b></span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>A PRINCESA ACORRENTADA,</b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>E PERSEUS, </b></span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>O HERÓI.</b></span></div>
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<b><span style="font-family: "arial" , "helvetica" , sans-serif;"><br /></span></b></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Andrômeda era a filha de Cefeus, rei da Etiópia, e de Cassiopeia. </span><br />
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<span style="font-family: "arial" , "helvetica" , sans-serif;"> Por causa dos boatos espalhados por Cassiopéia </span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">de que a beleza de Andrômeda superava a das Nereidas,</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"> Netuno enviou um mostro marinho, Cetus, a Baleia, para devastar aquele país. </span><br />
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<span style="font-family: "arial" , "helvetica" , sans-serif;"> Porém, Netuno fez a promessa de libertar o país dessa devastação</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"> caso Andromeda fosse oferecida em sacrifício, </span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">sendo acorrentada a uma rocha, para ser devorada pelo monstro marinho. </span><br />
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<span style="font-family: "arial" , "helvetica" , sans-serif;">No entanto, Perseus soube desse caso</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"> e salvou Andrômeda de seu tormento </span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">matando o monstro</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"> e o transformando em pedra ao lhe mostrar a cara da Medusa. </span><br />
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Ambos, Perseus e Andrômeda, alçaram vôo alto, </span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;">montados sobre Pegasus, o cavalo alado,</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"> e se dirigiram para o altar onde se casaram.<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><a href="https://www.facebook.com/MuseoImmaginarioArtisenzaTempo?ref=ts&fref=ts" style="color: #274e13; text-decoration: none;">https://www.facebook.com/MuseoImmaginarioArtisenzaTempo?ref=ts&fref=ts</a><br /><span style="color: #274e13;">Andromeda e Perseus - Guido Reni, 1635</span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></div>
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<span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif;"><b>Pegasus, </b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b><span style="color: #660000;">O CAVALO ALADO</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><b>Algumas Informações Interessantes acerca esta Constelação:</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Pegasus é uma constelação muito fácil de ser reconhecida por apresentar um proeminente quadrado formado por três membros Alpha Pegasi, Markab, Beta Pegasi, Scheat e Gamma Pegasi, Algenib, e ainda acolhendo a estrela Alpha Andromedae, Alpheratz. <o:p></o:p></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Este Asterismo é chamado de O Quadrado de Pegasus:</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Imagem extraída do Facebook e sem créditos, infelizmente</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Stellarium</span></div>
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<span style="background-color: #073763;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><b style="background-color: white;"><span lang="EN-US" style="font-family: "arial" , sans-serif;"> </span><span style="text-align: center;">PEGASUS, O CAVALO ALADO</span></b></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Posicionamento:<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Ascensão Reta 21h5m / 0h13m Declinação +2<sup>o</sup>.2 / +36<sup>o</sup>.3<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Mito:<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Dizem que Pegasus nasceu a partir do sangue da Medusa quando Perseus cortou fora sua cabeça. Mais tarde, o cavalo foi domado e cavalgado por Bellerofonte que se cansou das questões pertinentes à Terra e tentou voar em direção aos céus porém caiu. Pegasus, no entanto, continuou sua cavalgada, entrando no céu e tomando seu lugar entre as estrelas.<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Algumas Informações Interessantes acerca esta Constelação:<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Pegasus é uma constelação muito fácil de ser reconhecida por apresentar um proeminente quadrado formado por três membros Alpha Pegasi, Markab, Beta Pegasi, Scheat e Gamma Pegasi, Algenib, e ainda acolhendo a estrela Alpha Andromedae, Alpheratz.<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Fronteiras:<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">A constelação de Pegasus faz fronteira com Andrômeda, Lacerta, Cygnus, Vulpecula, Delphinus, Equuleus, Aquário e Peixes<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><b>Algumas Estrelas e alguns objetos interessantes, em Pégaso:</b><o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Existe um Asterismo chamado de O Quadrado de Pegaso </span></span><br />
<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">e composto pelas estrelas Alpha, Beta e Gamma Pegasi e ainda Alpha Andromedae.<o:p></o:p></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span lang="ES-TRAD" style="font-family: "arial" , sans-serif;"><b>Markab</b></span><span lang="ES-TRAD" style="font-family: "arial" , sans-serif;"><b>. Alpha Pegasi. </b><o:p></o:p></span></span></span></div>
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<span lang="PT" style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Ascensão Reta 23h 03,8m - Declinação +15<sup>o</sup> 05’<o:p></o:p></span></span></div>
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<span lang="PT" style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Magnitude visual 2,57 - Distância 109 anos-luz<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Uma estrela branca situada na asa de Pegaso. De Marka, Navio ou Veículo ou também Retornando de Longe. Em outra versão, a Sela, vocábulo árabe para designar o dorso de Pegaso.<o:p></o:p></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span lang="EN-US" style="font-family: "arial" , sans-serif;"><b>Scheat</b></span><span lang="EN-US" style="font-family: "arial" , sans-serif;"><b>. Beta Pegasi.</b> Estrela Variável.</span><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Uma estrela de amarelo profundo e irregularmente variável (de 2,1 a 3,0) e distante 210 anos-luz, situada na perna esquerda de Pegaso. O Peito, nome árabe.<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Esta é uma das quatro estrelas que compõem o Grande Quadrado do Cavalo Alado (as outras são Alpheratz (ou Sirrah) que Pegasus compartilha com Andrômeda (sua Alpha), a estrela-alpha Pegasi, Markab e a estrela-gamma, Algenib.<o:p></o:p></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span lang="ES-TRAD" style="font-family: "arial" , sans-serif;"><b>Algenib</b></span><span lang="ES-TRAD" style="font-family: "arial" , sans-serif;"><b>. Gamma Pegasi.</b><o:p></o:p></span></span></span></div>
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<span lang="ES-TRAD" style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Magnitude 2.84<o:p></o:p></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="font-family: "arial" , sans-serif;">Uma estrela branca situada na ponta da Asa de Pegaso. De Al Janah, a Asa, ou Al Jamb, o Lado. </span><span lang="PT" style="font-family: "arial" , sans-serif;">Significa Aquele que Carrega. A Asa do Cavalo Alado.<o:p></o:p></span></span></span></div>
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<span lang="PT" style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><b>Alpheratz</b><o:p></o:p></span></span></div>
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<span lang="PT" style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"> Uma estrela situada entre Andrômeda e Pegasus - Alpha Andromedae<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Ascensão Reta 00h07,3 - Declinação +28’58<o:p></o:p></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="font-family: "arial" , sans-serif;">Magnitude visual 2,15 - Distância 90 anos-luz</span><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">A cabeça de Andrômeda e parte do Cavalo Alado, Andrômeda. É uma estrela colocada na constelação de Andrômeda mas que possui seu grande simbolismo em relação ao conceito de Andrômeda. <o:p></o:p></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span lang="PT" style="font-family: "arial" , sans-serif;"><b>Enif</b></span><span lang="PT" style="font-family: "arial" , sans-serif;"><b> - Epsilon Pegasi</b><o:p></o:p></span></span></span></div>
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<span lang="PT" style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Ascensão Reta 21h 43,2m - Declinação +09<sup>o</sup> 47’<o:p></o:p></span></span></div>
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<span lang="PT" style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Magnitude visual 2,54 - Distância 780 anos-luz<o:p></o:p></span></span></div>
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<span lang="PT" style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">O Nariz do Cavalo Alado<o:p></o:p></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span lang="ES-TRAD" style="font-family: "arial" , sans-serif;"><b>Sad - </b></span><span lang="ES-TRAD" style="font-family: "arial" , sans-serif;"><b>Lambda Pegasi</b><o:p></o:p></span></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">A Boa Sorte, da expressão árabe Sad al Bari.<o:p></o:p></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="font-family: "arial" , sans-serif;"><b>Salm</b></span><span style="font-family: "arial" , sans-serif;"><b> - Tau Pegasi</b><o:p></o:p></span></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Bolsa de Couro, do árabe Salma.<o:p></o:p></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="font-family: "arial" , sans-serif;"><b>Matar - </b></span><span style="font-family: "arial" , sans-serif;"><b>Eta Pegasi</b><o:p></o:p></span></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Magnitude 2.95<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Chuva, designação proveniente da expressão árabe Al Sad al Matar, que significa A Chuva de Sorte.<o:p></o:p></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="font-family: "arial" , sans-serif;"><b>Baham</b></span><span style="font-family: "arial" , sans-serif;"><b> -Theta Pegasi</b><o:p></o:p></span></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Bestas, nome usado por Al Sufi que provém da expressão árabe As’d Al Bahaim, ou seja, as boas sortes de duas bestas.<o:p></o:p></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="font-family: "arial" , sans-serif;"><b>Homam</b></span><span style="font-family: "arial" , sans-serif;"><b> - Zeta Pegasi</b><o:p></o:p></span></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">A Sorte do Herói, nome árabe que faz alusão ao herói mitológico. Perseu, que voou no Cavalo Alado conduzindo a cabeça da medusa após vencer o monstro.<o:p></o:p></span></span></div>
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<span style="color: #0f243e; font-family: "arial" , sans-serif; font-size: 11pt;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: "arial" , sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: "arial" , sans-serif; font-size: 11pt;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="color: #0f243e; font-family: "arial" , sans-serif; font-size: 11pt;"><a href="https://pt.wikipedia.org/wiki/Markab" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Markab">Alpha Pegasi</a><span style="color: #252525; font-family: sans-serif; text-align: start;"> (Markab), </span><a href="https://pt.wikipedia.org/wiki/Beta_Pegasi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Beta Pegasi">Beta Pegasi</a><span style="color: #252525; font-family: sans-serif; text-align: start;"> (Beta-Scheat), e </span><a href="https://pt.wikipedia.org/wiki/Gamma_Pegasi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Gamma Pegasi">Gamma Pegasi</a><span style="color: #252525; font-family: sans-serif; text-align: start;"> (Gama-Algenil), em conjunto com </span><a href="https://pt.wikipedia.org/wiki/Alpha_Andromedae" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Alpha Andromedae">Alpha Andromedae</a><span style="color: #252525; font-family: sans-serif; text-align: start;"> (Alpheratz, Sirrah ou alfa-Andrómeda-Sirrah) formam o grande asterismo conhecido como </span><i style="color: #252525; font-family: sans-serif; text-align: start;">Quadrado do Pégaso</i><span style="color: #252525; font-family: sans-serif; text-align: start;">. A estrela </span><a href="https://pt.wikipedia.org/wiki/51_Pegasi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="51 Pegasi">51 Pegasi</a><span style="color: #252525; font-family: sans-serif; text-align: start;"> é notável por ser a primeira estrela parecida com o </span><a href="https://pt.wikipedia.org/wiki/Sol" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Sol">Sol</a><span style="color: #252525; font-family: sans-serif; text-align: start;"> a ter um </span><a class="mw-redirect" href="https://pt.wikipedia.org/wiki/Planeta_extrassolar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; text-align: start; text-decoration: none;" title="Planeta extrassolar">planeta extrassolar</a><span style="color: #252525; font-family: sans-serif; text-align: start;"> conhecido.</span></span></div>
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<b style="color: #660000; font-family: arial, helvetica, sans-serif;"> A ESTRELA COMPARTILHADA </b></div>
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<span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif;"><span style="line-height: 22.4px;"><b>PELAS CONSTELAÇÕES</b></span></span></div>
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<span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif;"><span style="line-height: 22.4px;"><b>PEGASUS E ANDROMEDA:</b></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">http://www.stellarium.org/pt/</span></span></div>
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<b><span style="background-color: white; font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;">A Constelação de Pegasus, o Cavalo Alado<o:p></o:p></span></span></b></div>
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<span style="background-color: white; font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;">Dizem que Pegasus nasceu a partir do sangue da Medusa quando Perseus cortou fora sua cabeça. Foi também cavalgando o Cavalo Alado Pegasus que Perseus pôde salvar Andromeda de sua morte pelo monstro marinho, Cetus, nos mares dos Peixes.</span></span><br />
<span style="background-color: white; font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;"> Mais tarde, o cavalo foi domado e cavalgado por Bellerofonte que se cansou das questões pertinentes à Terra e tentou voar em direção aos céus porém caiu. Pegasus, no entanto, continuou sua cavalgada, entrando no céu e tomando seu lugar entre as estrelas.<o:p></o:p></span></span></div>
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<span style="background-color: white; font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;"><img src="http://www.raremaps.com/maps/medium/35069.jpg" style="border-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></span></div>
<span style="background-color: white;"><span style="color: #073763;"><a href="http://www.raremaps.com/gallery/detail/35069/Pagase_Le_Petit_Cheval_Le_Dauphin_Pegasus_Pisces_and_Equuleus/Flamsteed-Fortin.html" style="text-decoration: none;"><span style="font-family: "arial" , "helvetica" , sans-serif;">http://www.raremaps.com/gallery/detail/35069/Pagase_Le_Petit_Cheval_Le_Dauphin_Pegasus_Pisces_and_Equuleus/Flamsteed-Fortin.html</span></a></span></span><br />
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<span style="background-color: white; font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;"><strong style="line-height: normal; text-align: start;">Map Maker: </strong><span style="line-height: normal; text-align: start;"></span><a href="https://www.raremaps.com/gallery/browse/creator_id/1260" style="border-bottom: 0px solid rgb(255, 255, 255); line-height: normal; text-decoration: none;">John Flamsteed</a><span style="line-height: normal; text-align: start;"> / </span><a href="https://www.raremaps.com/gallery/browse/creator_id/1454" style="border-bottom: 0px solid rgb(255, 255, 255); line-height: normal; text-decoration: none;">MJ Fortin</a></span></span></div>
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<span style="background-color: white; font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;">Detailed star chart of Pegasus, Pisces and Equuleus, from Fortin's <em>Atlas Celeste de Flamsteed </em>. . , published in Paris. </span></span></div>
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<span style="background-color: white; font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;">John Flamsteed was the first Astronomer Royal at the London Observatory, winning out over Edmund Halley and Isaac Newton</span></span><br />
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<span lang="PT"><span style="font-family: "arial" , "helvetica" , sans-serif;"><b><span style="color: #660000; font-size: large;">Alpheratz</span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span lang="PT"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"> Uma estrela situada entre Andrômeda e Pegasus - Alpha Andromedae<o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Ascensão Reta 00h07,3 - Declinação +28’58<o:p></o:p></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Magnitude visual 2,15 - Distância 90 anos-luz<o:p></o:p></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">A cabeça de Andrômeda e parte do Cavalo Alado, Pegasus. </span><br />
<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"> É uma estrela colocada na constelação de Andrômeda</span><br />
<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"> mas que possui seu grande simbolismo em relação ao conceito de Andrômeda. <o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: "arial" , sans-serif; font-size: 11pt;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: "arial" , sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: "arial" , sans-serif; font-size: 11pt;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="font-size: large;"><span style="font-family: "symbol";">δ</span> Pegasi</span></center>
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<tr><td width="650"><span style="background-color: white; font-size: large;">Delta Pegasi is rarely called ‘delta’ since it also goes by the name of alpha Andromedae (Sirrah or Alpheratz).</span><br />
<span style="background-color: white; font-size: large;">The star forms the northeastern corner of The Great Square of Pegasus: <a href="http://www.dibonsmith.com/peg_6.gif">binoculars</a>.</span><br />
<span style="background-color: white; font-size: large;">In the same region is the notable binary <i>85 Pegasi</i>, (BU 733), a multiple system:<br /> AB (yellow-orange and orange-reddish): 5.8, 8.9; 273º, 0.8" with an <a href="http://www.dibonsmith.com/peg_85.gif">orbit</a> of 26.27 years.<br /> AC (orange): 5.8, 9.9; 326º, 173.8".</span></td></tr>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 18px;">http://www.dibonsmith.com/peg_d.htm</span><br />
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<span style="background-color: white;"><span style="font-size: x-small;">© 1998-2014 by Richard Dibon-Smith.</span></span></h4>
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<span style="box-sizing: border-box; font-weight: 700;">THE GREAT SQUARE OF PEGASUS – ASTERISM</span></div>
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The Great Square of Pegasus represents the main body of Pegasus. It is a prominent asterism made up of three bright stars in Pegasus and Alpha Andromedae, which in ancient times was considered to belong to both Pegasus and <a href="http://www.constellation-guide.com/constellation-list/andromeda-constellation/" style="box-sizing: border-box; transition: all 0.1s ease-in-out;">Andromeda</a>constellations and marked both the navel of the horse and the top of Andromeda’s head. In the 17th century, Johann Bayer gave the star a dual designation, Alpha Andromedae and Delta Pegasi. The name Delta Pegasi has long been retired and the star is now known only as Alpha Andromedae, or by its proper name, Alpheratz.</div>
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The other stars that form the Great Square of Pegasus are Markab (Alpha Pegasi), Scheat (Beta Pegasi), and Algenib (Gamma Pegasi).</div>
<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 18px;"><a href="http://www.constellation-guide.com/constellation-list/pegasus-constellation/">http://www.constellation-guide.com/constellation-list/pegasus-constellation/</a></span><br />
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<span style="background-color: white;"><span style="font-family: "arial" , "helvetica" , sans-serif;"><b><span style="color: #660000;"><span style="font-size: large;">O Mito de Andromeda</span></span></b></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Andrômeda era a filha de Cefeus, rei da Etiópia, e de Cassiopeia. Por causa dos boatos espalhados por Cassiopéia de que a beleza de Andrômeda superava a das Nereidas, Netuno enviou um mostro marinho, Cetus, a Baleia, para devastar aquele país. Porém, Netuno fez a promessa de libertar o país dessa devastação caso Andromeda fosse oferecida em sacrifício, sendo acorrentada a uma rocha, para ser devorada pelo monstro marinho. No entanto, Perseus soube desse caso e salvou Andrômeda de seu tormento matando o monstro e o transformando em pedra ao lhe mostrar a cara da Medusa. Ambos, Perseus e Andrômeda, alçaram vôo alto, sobre Pegasus, o cavalo alado, e se dirigiram para o altar onde se casaram.</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif; line-height: 18px;">http://www.raremaps.com/gallery/detail/36137/Andromede_Persee_Le_Triangle_Andromeda_Perseus_and_Triangle/Flamsteed-Fortin.html</span><br />
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<span style="background-color: white;"><strong>Title: </strong>Andromede, Persee, Le Triangle (Andromeda, Perseus & Triangle)</span></div>
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<span style="background-color: white;"><span style="color: #073763;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1260" style="border-bottom: 0px solid rgb(255, 255, 255); text-decoration: none;">John Flamsteed</a> / <a href="https://www.raremaps.com/gallery/browse/creator_id/1454" style="border-bottom: 0px solid rgb(255, 255, 255); text-decoration: none;">MJ Fortin</a></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes<b></b></span></span></div>
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<b><span style="background-color: white;"><span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif;">Andromeda,</span></span></b></div>
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<b><span style="background-color: white;"><span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #660000;">A PRINCESA ACORRENTADA</span><span style="color: #073763;"><o:p></o:p></span></span></span></b></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><b>História:</b><o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Esta é uma das mais antigas constelações nomeadas e que faziam parte do Catalogo de Ptolomeu no Século Segundo depois de Cristo. ( Século 2 DC).</span></span><br />
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><b><span style="color: #660000; font-size: large;">Alpheratz ou Sirrah</span></b><span style="color: #073763; font-size: 16px;">. Alpha Andromedae.<o:p></o:p></span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Ascensão Reta 00h07,3 - Declinação +28’58<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Magnitude visual 2,15 - Distância 90 anos-luz<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Uma estrela dupla, branca avermelhada, no cabelo de Andromeda. </span></span></div>
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"> De Al Surrat al Farás, falando sobre a parte do cavalo</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"> - por ter sido pertencente a Pegasus, anteriormente. </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Esta estrela também é conhecida por <b>Sirrah</b>.</span></span></div>
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<span style="color: #0f243e; font-family: "arial" , sans-serif; font-size: 11pt;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: "arial" , sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: "arial" , sans-serif; font-size: 11pt;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="line-height: 18px;"><img src="http://upload.wikimedia.org/wikipedia/commons/4/44/Alpheratz.gif" height="640" width="640" /></span><span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /><span style="line-height: 18px;">http://en.wikipedia.org/wiki/Alpha_Andromedae#mediaviewer/File:Alpheratz.gif</span></span></span></div>
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<span style="color: #660000; font-size: large;"><b>Alpha Andromedae</b>, também chamada <b>Alpheratz</b>, <b>Sirah</b> ou <b>Delta Pegasi</b></span><span style="color: #252525;">, é a </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-image: none; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a><span style="color: #252525;"> mais brilhante da constelação de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Andromeda" style="background-image: none; color: #0b0080; text-decoration: none;" title="Andromeda">Andrômeda</a><span style="color: #252525;">. Está situada no extremo nordeste da constelação de </span><a href="http://pt.wikipedia.org/wiki/Pegasus" style="background-image: none; color: #0b0080; text-decoration: none;" title="Pegasus">Pegasus</a><span style="color: #252525;"> e como tal também pode ser designada por </span><b style="color: #252525;">Delta Pegasi</b><span style="color: #252525;"> (δ Peg), apesar de este nome não ser mais utilizado. Está localizada a 97 anos-luz da Terra.</span></div>
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É uma <a href="http://pt.wikipedia.org/wiki/Estrela_bin%C3%A1ria" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela binária">estrela binária</a> de magnitude 2,2, de classe B (azul-branco). É composta por duas estrelas que orbitam próximas e que só se conseguem distinguir através de análise <a href="http://pt.wikipedia.org/wiki/Espectroscopia" style="background: none; color: #0b0080; text-decoration: none;" title="Espectroscopia">espectroscópica</a> cuidada. A maior das duas tem um tamanho dez vezes superior. O <a href="http://pt.wikipedia.org/wiki/Per%C3%ADodo_orbital" style="background: none; color: #0b0080; text-decoration: none;" title="Período orbital">período orbital</a> tem 96,7 dias. A <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">classe espectral</a> é B8 e o par é 200 vezes mais luminoso que o <a href="http://pt.wikipedia.org/wiki/Sol" style="background: none; color: #0b0080; text-decoration: none;" title="Sol">Sol</a>, com uma temperatura à superfície de 13000 <a href="http://pt.wikipedia.org/wiki/Kelvin" style="background: none; color: #0b0080; text-decoration: none;" title="Kelvin">Kelvin</a></div>
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A estrela maior possui uma grande abundância de vários elementos, tais como <a href="http://pt.wikipedia.org/wiki/Merc%C3%BArio_(elemento_qu%C3%ADmico)" style="background: none; color: #0b0080; text-decoration: none;" title="Mercúrio (elemento químico)">mercúrio</a>, <a href="http://pt.wikipedia.org/wiki/G%C3%A1lio" style="background: none; color: #0b0080; text-decoration: none;" title="Gálio">gálio</a>, <a href="http://pt.wikipedia.org/wiki/Mangan%C3%AAs" style="background: none; color: #0b0080; text-decoration: none;" title="Manganês">manganês</a> e <a href="http://pt.wikipedia.org/wiki/Eur%C3%B3pio" style="background: none; color: #0b0080; text-decoration: none;" title="Európio">európio</a>, na sua atmosfera. Por outro lado, outros elementos têm concentrações muito baixas. Estas anomalias podem ser o resultado da pressão gravitacional da estrela.</div>
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A estrela é classificada como do tipo <a href="http://pt.wikipedia.org/wiki/Estrela_vari%C3%A1vel" style="background-image: none; color: #0b0080; text-decoration: none;" title="Estrela variável">variável</a> <a href="http://pt.wikipedia.org/wiki/Vari%C3%A1vel_Alpha%C2%B2_Canum_Venaticorum" style="background-image: none; color: #0b0080; text-decoration: none;" title="Variável Alpha² Canum Venaticorum">Alpha2 Canum Venaticorum</a> e a sua magnitude varia de +2,02 até +2.06, com um período de 23,19 horas.</div>
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<span style="line-height: 19px;"><a href="http://pt.wikipedia.org/wiki/Alpha_Andromedae">http://pt.wikipedia.org/wiki/Alpha_Andromedae</a></span></div>
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<span class="mw-headline" id="Etymology_and_cultural_significance"><span style="font-size: small;">Etymology and cultural significance</span></span></h2>
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The names <i>Alpheratz</i> and <i>Sirrah</i> both derive from the Arabic name, <b>سرة الفرس</b> <i>surrat al-faras</i> "the navel of the mare". (سرة alone is <i>surrah.</i>) The word <i>horse</i>reflects the star's historical placement in <a href="http://en.wikipedia.org/wiki/Pegasus_(constellation)" style="background-image: none; color: #0b0080; text-decoration: none;" title="Pegasus (constellation)">Pegasus</a>.<sup class="reference" id="cite_ref-allen_24-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Alpha_Andromedae#cite_note-allen-24" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[24]</a></sup> Another term for this star used by medieval astronomers writing in <a href="http://en.wikipedia.org/wiki/Arabic_language" style="background-image: none; color: #0b0080; text-decoration: none;" title="Arabic language">Arabic</a> was راس المراة المسلسلة <i>rās al-mar'a al-musalsala</i> "the head of the woman in chains",<sup class="reference" id="cite_ref-allen_24-1" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Alpha_Andromedae#cite_note-allen-24" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[24]</a></sup> the chained woman here being <a href="http://en.wikipedia.org/wiki/Andromeda_(mythology)" style="background-image: none; color: #0b0080; text-decoration: none;" title="Andromeda (mythology)">Andromeda</a>. Other Arabic names include <i>al-kaff al-khaḍīb</i> and <i>kaff al-naṣīr</i>.<sup class="reference" id="cite_ref-Goldstein1985_25-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Alpha_Andromedae#cite_note-Goldstein1985-25" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[25]</a></sup></div>
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In the <a href="http://en.wikipedia.org/wiki/Hinduism" style="background: none; color: #0b0080; text-decoration: none;" title="Hinduism">Hindu</a> lunar zodiac, this star, together with the other stars in the Great Square of Pegasus (<a class="mw-redirect" href="http://en.wikipedia.org/wiki/%CE%91_Pegasi" style="background: none; color: #0b0080; text-decoration: none;" title="Α Pegasi">α</a>, <a class="mw-redirect" href="http://en.wikipedia.org/wiki/%CE%92_Pegasi" style="background: none; color: #0b0080; text-decoration: none;" title="Β Pegasi">β</a>, and <a class="mw-redirect" href="http://en.wikipedia.org/wiki/%CE%93_Pegasi" style="background: none; color: #0b0080; text-decoration: none;" title="Γ Pegasi">γ Pegasi</a>), makes up the <a href="http://en.wikipedia.org/wiki/Nakshatra" style="background: none; color: #0b0080; text-decoration: none;" title="Nakshatra">nakshatras</a> of <a href="http://en.wikipedia.org/wiki/P%C5%ABrva_Bh%C4%81drapad%C4%81" style="background: none; color: #0b0080; text-decoration: none;" title="Pūrva Bhādrapadā">Pūrva Bhādrapadā</a> and <a href="http://en.wikipedia.org/wiki/Uttara_Bh%C4%81drapad%C4%81" style="background: none; color: #0b0080; text-decoration: none;" title="Uttara Bhādrapadā">Uttara Bhādrapadā</a>.<sup class="reference" id="cite_ref-allen_24-2" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Alpha_Andromedae#cite_note-allen-24" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[24]</a></sup></div>
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In <a href="http://en.wikipedia.org/wiki/Chinese_language" style="background: none; color: #0b0080; text-decoration: none;" title="Chinese language">Chinese</a>, <span lang="zh" xml:lang="zh">壁宿</span> (<span lang="zh-Latn" xml:lang="zh-Latn">Bì Sù</span>), meaning <i><a href="http://en.wikipedia.org/wiki/Wall_(Chinese_constellation)" style="background: none; color: #0b0080; text-decoration: none;" title="Wall (Chinese constellation)">wall</a></i>, refers to an asterism consisting of α Andromedae and <a class="mw-redirect" href="http://en.wikipedia.org/wiki/%CE%93_Pegasi" style="background: none; color: #0b0080; text-decoration: none;" title="Γ Pegasi">γ Pegasi</a>.<sup class="reference" id="cite_ref-26" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Alpha_Andromedae#cite_note-26" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[26]</a></sup> Consequently, α Andromedae itself is known as <span lang="zh" xml:lang="zh">壁宿二</span> (<span lang="zh-Latn" xml:lang="zh-Latn">Bì Sù èr</span>, English: the second star of the wall.)<sup class="reference" id="cite_ref-27" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Alpha_Andromedae#cite_note-27" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[27]</a></sup></div>
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It is also known as one of the "Three Guides" that mark the prime meridian of the heavens, the other two being <a href="http://en.wikipedia.org/wiki/Beta_Cassiopeiae" style="background-image: none; color: #0b0080; text-decoration: none;" title="Beta Cassiopeiae">Beta Cassiopeiae</a> and <a href="http://en.wikipedia.org/wiki/Gamma_Pegasi" style="background-image: none; color: #0b0080; text-decoration: none;" title="Gamma Pegasi">Gamma Pegasi</a>. It was believed to bless those born under its influence with honour and riches.<sup class="reference" id="cite_ref-Olcott_28-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Alpha_Andromedae#cite_note-Olcott-28" style="background-image: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[28]</a></sup></div>
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<span class="mw-headline" id="Observation"><span style="font-size: small;">Observation</span></span></h2>
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<a class="image" href="http://en.wikipedia.org/wiki/File:Andromeda_constellation_map_(1).png" style="background: none; color: #0b0080; text-decoration: none;"><img alt="" class="thumbimage" data-file-height="420" data-file-width="562" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/02/Andromeda_constellation_map_%281%29.png/250px-Andromeda_constellation_map_%281%29.png" height="187" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/02/Andromeda_constellation_map_%281%29.png/375px-Andromeda_constellation_map_%281%29.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/02/Andromeda_constellation_map_%281%29.png/500px-Andromeda_constellation_map_%281%29.png 2x" style="background-color: white; border: 1px solid rgb(204, 204, 204); vertical-align: middle;" width="250" /></a><br />
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Andromeda constellation. α Andromedae, labeled <i>Sirrah</i>, is at the lower right of the constellation, bordering Pegasus.</div>
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The location of α Andromedae in the sky is shown on the left. It can be seen by the naked eye and is theoretically visible at all latitudes north of 60° S. During evening from August to October, it will be high in the sky as seen from the northern midlatitudes.<sup class="reference" id="cite_ref-29" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Alpha_Andromedae#cite_note-29" style="background-image: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[29]</a></sup></div>
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<span class="mw-headline" id="Optical_companion"><span style="font-size: small;">Optical companion</span></span></h2>
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The <a href="http://en.wikipedia.org/wiki/Binary_star" style="background-image: none; color: #0b0080; text-decoration: none;" title="Binary star">binary system</a> described above has an optical <a href="http://en.wikipedia.org/wiki/Double_star" style="background-image: none; color: #0b0080; text-decoration: none;" title="Double star">visual companion</a>, discovered by <a href="http://en.wikipedia.org/wiki/William_Herschel" style="background-image: none; color: #0b0080; text-decoration: none;" title="William Herschel">William Herschel</a> on July 21, 1781.<sup class="reference" id="cite_ref-usno_7-4" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Alpha_Andromedae#cite_note-usno-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[7]</a></sup><sup class="reference" id="cite_ref-burnham_31-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Alpha_Andromedae#cite_note-burnham-31" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[31]</a></sup><sup class="reference" id="cite_ref-32" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Alpha_Andromedae#cite_note-32" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[32]</a></sup> Designated as <i>ADS 94 B</i> in the <a href="http://en.wikipedia.org/wiki/Aitken_Double_Star_Catalogue" style="background-image: none; color: #0b0080; text-decoration: none;" title="Aitken Double Star Catalogue">Aitken Double Star Catalogue</a>, it is a <a class="mw-redirect" href="http://en.wikipedia.org/wiki/G-type_star" style="background-image: none; color: #0b0080; text-decoration: none;" title="G-type star">G-type</a> <a href="http://en.wikipedia.org/wiki/Star" style="background-image: none; color: #0b0080; text-decoration: none;" title="Star">star</a> with an <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Apparent_visual_magnitude" style="background-image: none; color: #0b0080; text-decoration: none;" title="Apparent visual magnitude">apparent visual magnitude</a> of approximately 10.8.<sup class="reference" id="cite_ref-sb0_30-8" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Alpha_Andromedae#cite_note-sb0-30" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[30]</a></sup> Although by coincidence it appears near to the other two stars in the sky, it is not close to them in space.<sup class="reference" id="cite_ref-burnham_31-1" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Alpha_Andromedae#cite_note-burnham-31" style="background-image: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[31<br />]</a></sup></div>
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<span style="line-height: 19px;"><a href="http://en.wikipedia.org/wiki/Alpha_Andromedae">http://en.wikipedia.org/wiki/Alpha_Andromedae</a></span></div>
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<span style="background-color: white; color: #660000; font-family: "arial" , "helvetica" , sans-serif;"><b style="line-height: 22.4px;"> Asterismo </b><span style="line-height: 22.4px;">nomeado de</span><b style="line-height: 22.4px;"> Circlet, Pequeno Círculo</b></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Excerto da constelação dos Peixes - Mario Jaci Monteiro, Cartas Celestes, As Constelações</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><b> Asterismo </b>nomeado de<b> Circlet, Pequeno Círculo</b>, </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">composto pelas estrelas Gamma, Beta, Teta, Iota, 19, Lambda e Kappa Piscium<b><o:p></o:p></b></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Este Pequeno Círculo - um dos dois Peixes - marca a proximidade do Ponto Vernal, o cruzamento entre as Linhas do Equador celestial e da Eclíptica. Em lugares de céus escuros e transparentes, podemos sempre bem visualizar este Pequeno Círculo, realmente.</span></span><br />
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Mario Jaci Monteiro , As Constelações, Cartas Celestes <o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="font-family: "arial" , "helvetica" , sans-serif;"><b><span style="color: #660000;">O Ponto Vernal</span></b><span style="color: #073763;"> <b>acontece na constelação dos Peixes </b></span><b><br /><span style="color: #073763;">exatamente sob o Grande Quadrado do Cavalo Pegasus </span><br /><span style="color: #073763;">e próximo à estrela, Alpheratz, Alpha Andromedae </span></b><br /><span style="color: #073763;">- estrela que vivencia a fronteira entre a constelação do Cavalo Alado </span><br /><span style="color: #073763;">(fazendo parte, inclusive, do asterismo do Grande Quadrado</span><br /><span style="color: #073763;"> composto ainda pelas estrelas Alpha, Beta e Gamma Pegasi) </span><br /><span style="color: #073763;">e a constelação de Andromeda</span><br /><span style="color: #073763;"> (a famosa galáxia Andromeda, M31, </span><br /><span style="color: #073763;">pode ser observada inserida nesta constelação). </span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><b>Leia mais sobre o Ponto Vernal</b></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><b>acessando</b></span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white; line-height: 22.4px;">http://oceudomes.blogspot.com.br/2014/07/lua-no-ponto-vernal.html</span></span></div>
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<span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif;"><b>ALGUMAS GALÁXIAS</b></span><br />
<span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif;"><b>E AGLOMERADOS</b></span><br />
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<img src="http://www.iau.org/static/public/constellations/gif/PEG.gif" /><br />
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><b>NGC 7479 - Galáxia Espiral Barrada</b><o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Um objeto bem pálido, de magnitude 11.8, situado um pouco ao sul da Estrela Alpha Pegasi, Markab.<o:p></o:p></span></span></div>
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<span lang="PT" style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><b>NGC 7814 - Galáxia</b><o:p></o:p></span></span></div>
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<span lang="PT" style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Galáxia observada exatamente em sua extremidade e apresentando uma proeminente banda de poeira escura interestelar ao longo do plano equatorial ndrômeda. Magnitude 12.0. situa-se bem próxima à estrela Gamma Pegasi, Algenib.<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><b>M 15 - NGC 7078 - Pegasus - Aglomerado Estelar Globular</b><o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Ascensão Reta 21h29m Declinação +23<sup>o</sup>.05<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Magnitude visual integral 6,3 Tipo AG<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><b>NGC 7078 - M 15 - Aglomerado Globular Pegasus</b><o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Ascensão Reta 21h29m Declinação +12<sup>o</sup>.05<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Magnitude fotográfica global 7,0 Diâmetro aparente 9’,4 Tipo Espectral F2<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Magnitude média das 25 mais brilhantes estrelas (excluindo as 5 mais brilhantes) 14,44<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><b>NGC 7331 - Galáxia Espiral</b><o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"> Esta é uma galáxia que possui dimensões e estrutura bem similares às de nossa Galáxia e distante cerca de 50 milhões de anos-luz. Situa-se mais ao norte da Eta Pegasi, Matar, e bem próxima à NGC 7320, o Quinteto de Stephan.<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif; font-size: xx-small;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif; font-size: xx-small;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif; font-size: xx-small;">Editora Vozes, Petrópolis, ano de 1986</span><br />
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Por NASA, ESA, and the Hubble SM4 ERO Team - http://www.hubblesite.org/newscenter/archive/releases/2009/25/image/x/ (direct link), Domínio público, https://commons.wikimedia.org/w/index.php?curid=7775623</span></span><br />
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<span style="background-color: white; color: #333333; font-family: sans-serif; font-size: 16px;">Galactic Wreckage in Stephan's Quintet A clash among members of a famous galaxy quintet reveals an assortment of stars across a wide color range, from young, blue stars to aging, red stars. This portrait of Stephan's Quintet, also known as Hickson Compact Group 92, was taken by the new Wide Field Camera 3 (WFC3) aboard NASA's Hubble Space Telescope. Stephan's Quintet, as the name implies, is a group of five galaxies. The name, however, is a bit of a misnomer. Studies have shown that group member NGC 7320, at upper left, is actually a foreground galaxy about seven times closer to Earth than the rest of the group. Three of the galaxies have distorted shapes, elongated spiral arms, and long, gaseous tidal tails containing myriad star clusters, proof of their close encounters. These interactions have sparked a frenzy of star birth in the central pair of galaxies. This drama is being played out against a rich backdrop of faraway galaxies. The image, taken in visible and near-infrared light, showcases WFC3's broad wavelength range. The colors trace the ages of the stellar populations, showing that star birth occurred at different epochs, stretching over hundreds of millions of years. The camera's infrared vision also peers through curtains of dust to see groupings of stars that cannot be seen in visible light. NGC 7319, at top right, is a barred spiral with distinct spiral arms that follow nearly 180 degrees back to the bar. The blue specks in the spiral arm at the top of NGC 7319 and the red dots just above and to the right of the core are clusters of many thousands of stars. Most of the quintet is too far away even for Hubble to resolve individual stars. Continuing clockwise, the next galaxy appears to have two cores, but it is actually two galaxies, NGC 7318A and NGC 7318B. Encircling the galaxies are young, bright blue star clusters and pinkish clouds of glowing hydrogen where infant stars are being born. These stars are less than 10 million years old and have not yet blown away their natal cloud. Far away from the galaxies, at right, is a patch of intergalactic space where many star clusters are forming. NGC 7317, at bottom left, is a normal-looking elliptical galaxy that is less affected by the interactions. Sharply contrasting with these galaxies is the dwarf galaxy NGC 7320 at upper left. Bursts of star formation are occurring in the galaxy's disk, as seen by the blue and pink dots. In this galaxy, Hubble can resolve individual stars, evidence that NGC 7320 is closer to Earth. NGC 7320 is 40 million light-years from Earth. The other members of the quintet reside 290 million light-years away in the constellation Pegasus. These farther members are markedly redder than the foreground galaxy, suggesting that older stars reside in their cores. The stars' light also may be further reddened by dust stirred up in the encounters. Spied by Edouard M. Stephan in 1877, Stephan's Quintet is the first compact group ever discovered. WFC3 observed the quintet in July and August 2009. The composite image was made by using filters that isolate light from the blue, green, and infrared portions of the spectrum, as well as emission from ionized hydrogen. These Hubble observations are part of the Hubble Servicing Mission 4 Early Release Observations. NASA astronauts installed the WFC3 camera during a servicing mission in May to upgrade and repair the 19-year-old Hubble telescope.</span><br />
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Grupo de galáxias consistindo de NGC 7320, NGC 7317, 7318<sup> </sup>A e B e 7319. Este grupo situa-se bem próximo à NGC 7331 e ambos ao norte de Matar, Eta Pegasi.<o:p></o:p></span></span></div>
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<b>NGC 7320</b> é uma <a href="https://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia">galáxia</a> <a href="https://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia espiral">espiral</a> (Scd) localizada na <a href="https://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="https://pt.wikipedia.org/wiki/Pegasus" style="background: none; color: #0b0080; text-decoration: none;" title="Pegasus">Pegasus</a> que pertence visualmente ao <a href="https://pt.wikipedia.org/wiki/Quinteto_de_Stephan" style="background: none; color: #0b0080; text-decoration: none;" title="Quinteto de Stephan">Quinteto de Stephan</a>. Não é um verdadeiro membro do grupo, apenas uma coincidência na linha de visão. Está a cerca de 40 milhões de <a href="https://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080;" title="Ano-luz">anos-luz</a> da Terra, enquanto os outros membros do grupo estão a cerca de 300 milhões de anos-luz. Possui uma declinação de +33° 56' 54" e uma <a class="mw-redirect" href="https://pt.wikipedia.org/wiki/Ascens%C3%A3o_recta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão recta">ascensão recta</a> de 22 <a href="https://pt.wikipedia.org/wiki/Hora" style="background: none; color: #0b0080; text-decoration: none;" title="Hora">horas</a>, 36 <a href="https://pt.wikipedia.org/wiki/Minuto" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto">minutos</a> e 03,5 <a href="https://pt.wikipedia.org/wiki/Segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a>.</div>
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Foi descoberta em <a href="https://pt.wikipedia.org/wiki/23_de_setembro" style="background: none; color: #0b0080; text-decoration: none;" title="23 de setembro">23 de setembro</a> de <a href="https://pt.wikipedia.org/wiki/1876" style="background: none; color: #0b0080; text-decoration: none;" title="1876">1876</a> por <a href="https://pt.wikipedia.org/wiki/%C3%89douard_Jean-Marie_Stephan" style="background: none; color: #0b0080; text-decoration: none;" title="Édouard Jean-Marie Stephan">Édouard Jean-Marie Stephan</a>.</div>
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<span style="color: #252525; font-family: sans-serif;"><a href="https://pt.wikipedia.org/wiki/NGC_7320">https://pt.wikipedia.org/wiki/NGC_7320</a></span></div>
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By NASA, ESA, and the Hubble SM4 ERO Team - →This file has been extracted from another file: Stephan's Quintet Hubble 2009.full.jpg, Public Domain, https://commons.wikimedia.org/w/index.php?curid=16874455<br />
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<span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif;"><b>M15,</b></span></div>
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<span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif;"><b>O OBJETO MESSIER</b></span></div>
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<span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif;"><b>NA DIREÇÃO DA CONSTELAÇÃO PEGASUS</b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Stellarium</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">O Objeto Messier 15</span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;">pode ser encontrado bem na fronteira</span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;">entre a constelações de Pégaso</span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;">e as constelações Delfim e Cavalo Menor</span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;">- a partir da estrela-epsilon Pegasi, Enif, o nariz do Cavalo Alado,</span><br />
<span style="font-family: "arial" , "helvetica" , sans-serif;">e a estrela mais brilhante desta constelação.</span></div>
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<span style="color: #073763; font-size: small; font-weight: normal;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Pegasi">http://pt.wikipedia.org/wiki/Epsilon_Pegasi</a></span></h1>
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<b>Epsilon Pegasi</b> (ε Peg, ε Pegasi) é a <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-image: none; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a> mais brilhante da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Pegasus" style="background-image: none; color: #0b0080; text-decoration: none;" title="Pegasus">Pegasus</a>, com uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 2,399.<span class="reference" id="cite_ref-saaoc8_59_2-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Pegasi#cite_note-saaoc8_59-2" style="background-image: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> É conhecida também pelo nome tradicional <b>Enif</b>, que é derivado da palavra árabe para nariz, devido à sua posição na constelação.<span class="reference" id="cite_ref-stars_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Pegasi#cite_note-stars-9" style="background-image: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span> A distância a ela pode ser estimada usando medições de <a href="http://pt.wikipedia.org/wiki/Paralaxe" style="background-image: none; color: #0b0080; text-decoration: none;" title="Paralaxe">paralaxe</a> da missão <a href="http://pt.wikipedia.org/wiki/Hipparcos" style="background-image: none; color: #0b0080; text-decoration: none;" title="Hipparcos">Hipparcos</a>, dando um valor de 690 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-image: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (211 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-image: none; color: #0b0080; text-decoration: none;" title="Parsec">parsecs</a>) da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-image: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>, com uma <a href="http://pt.wikipedia.org/wiki/Margem_de_erro" style="background-image: none; color: #0b0080; text-decoration: none;" title="Margem de erro">margem de erro</a> de 20 anos-luz.<span class="reference" id="cite_ref-simbad_1-8" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Pegasi#cite_note-simbad-1" style="background-image: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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Epsilon Pegasi é uma estrela <a href="http://pt.wikipedia.org/wiki/Evolu%C3%A7%C3%A3o_estelar" style="background-image: none; color: #0b0080; text-decoration: none;" title="Evolução estelar">evoluída</a> que está no estágio de <a href="http://pt.wikipedia.org/wiki/Estrela_supergigante" style="background-image: none; color: #0b0080; text-decoration: none;" title="Estrela supergigante">supergigante</a>, confome indicado pela <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-image: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">classificação estelar</a> de K2 Ib.<span class="reference" id="cite_ref-simbad_1-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Pegasi#cite_note-simbad-1" style="background-image: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> Estima-se que tenha 12 vezes a<a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background-image: none; color: #0b0080; text-decoration: none;" title="Massa solar">massa do Sol</a>.<span class="reference" id="cite_ref-mnras410_1_190_5-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Pegasi#cite_note-mnras410_1_190-5" style="background-image: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> </div>
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Em algumas ocasiões, o brilho de Epsilon Pegasi aumentou radicalmente, ficando até mais brilhante que <a href="http://pt.wikipedia.org/wiki/Altair_(estrela)" style="background-image: none; color: #0b0080; text-decoration: none;" title="Altair (estrela)">Altair</a>, a estrela mais brilhante da constelação de <a href="http://pt.wikipedia.org/wiki/Aquila" style="background-image: none; color: #0b0080; text-decoration: none;" title="Aquila">Aquila</a>.<span class="reference" id="cite_ref-stars_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Pegasi#cite_note-stars-9" style="background-image: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span></div>
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Como uma supergigante, Epsilon Pegasi está no fim de sua vida, porém, como sua massa está na divisa entre estrelas destinadas a explodir ou não, não se sabe se irá explodir em uma <a href="http://pt.wikipedia.org/wiki/Supernova" style="background-image: none; color: #0b0080; text-decoration: none;" title="Supernova">supernova</a> ou se tornar uma rara <a href="http://pt.wikipedia.org/wiki/An%C3%A3_branca" style="background-image: none; color: #0b0080; text-decoration: none;" title="Anã branca">anã branca</a> de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ne%C3%B4nio" style="background-image: none; color: #0b0080; text-decoration: none;" title="Neônio">neônio</a> e <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Oxig%C3%AAnio" style="background-image: none; color: #0b0080; text-decoration: none;" title="Oxigênio">oxigênio</a> com menos da metade do tamanho da Terra.<span class="reference" id="cite_ref-stars_9-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Pegasi#cite_note-stars-9" style="background-image: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span></div>
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LEIA MAIS</div>
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<a href="http://pt.wikipedia.org/wiki/Epsilon_Pegasi">http://pt.wikipedia.org/wiki/Epsilon_Pegasi</a></div>
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m15atlas.jpg" /><br />
http://www.ipac.caltech.edu/2mass/gallery/m15atlas.jpg<br />
<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a><br />
<a href="https://www.blogger.com/null" name="m81" style="background-color: white;"><br /></a><a href="https://www.blogger.com/null" name="m81" style="background-color: white;"><br /></a></div>
<h1>
Messier 15</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Globular Cluster</a> M15 (NGC 7078)</i>, class IV, in <a href="http://messier.obspm.fr/map/Peg.html">Pegasus</a></center>
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<a href="http://messier.obspm.fr/Jpg/m15.jpg"><img align="right" alt="[m15.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m15.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">21 : 30.0 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+12 : 10 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">33.6 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">6.2 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">18.0 (arc min)</td></tr>
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Discovered by Jean-Dominique Maraldi in 1746.</div>
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Globular cluster Messier 15 (M15, NGC 7078) is among the more conspicuous of these great stellar swarms. At a distance of about 33,600 light years, its diameter of 18.0 arc min corresponds to a linear extension of about 175 light-years, and its total visual brightness of 6.2 magnitudes corresponds to an absolute magnitude of -9.17, or roughly 360,000 times that of our sun.</div>
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M15 is perhaps the densest of all (globular) star clusters in our Milky Way galaxy.</div>
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M15 was discovered by <a href="http://messier.obspm.fr/xtra/Bios/maraldi.html">Jean-Dominique Maraldi (Maraldi II, 1709-88)</a> on September 7, 1746 while he was looking for De Chéseaux' comet; he described it as 'A nebulous star, fairly bright and composed of many stars'. <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, who<a href="http://messier.obspm.fr/xtra/history/m-cat.html#M15">cataloged it on June 3, 1764</a>, and <a href="http://messier.obspm.fr/xtra/similar/bode.html">Johann Elert Bode</a> couldn't make this out and described it as 'nebula without stars,' so that it remained to <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html">William Herschel</a> in 1783 to resolve this fine star cluster.</div>
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LEIA MAIS</div>
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acessando</div>
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<a href="http://messier.obspm.fr/m/m015.html">http://messier.obspm.fr/m/m015.html</a></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;"><b>NGC 7078 - M 15 - Aglomerado Globular Pegasus</b><o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 21h29m Declinação +12<sup>o</sup>.05<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Magnitude fotográfica global 7,0 Diâmetro aparente 9’,4 Tipo Espectral F2<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Magnitude média das 25 mais brilhantes estrelas (excluindo as 5 mais brilhantes) 14,44<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Número conhecido de Variáveis 103 Distância kpc 10,5<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Velocidade Radial (km/s) - 107</span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif; font-size: x-small;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif; font-size: x-small;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif; font-size: x-small;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b>Messier 15</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 7078</a>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a> localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Pegasus" style="background: none; color: #0b0080; text-decoration: none;" title="Pegasus">Pégaso</a>. Foi descobeto pelo astrônomo ítalo-francês <a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background: none; color: #0b0080; text-decoration: none;" title="Giovanni Domenico Maraldi">Jean-Dominique Maraldi</a> em 1746, e posteriormente incluído pelo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catálogo</a> de objetos semelhantes a <a href="http://pt.wikipedia.org/wiki/Cometa" style="background: none; color: #0b0080; text-decoration: none;" title="Cometa">cometas</a> em 1764. Com uma idade estimada de 13,2 bilhões de anos, Messier 15 é um dos mais velhos aglomerados globulares conhecidos.</div>
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O aglomerado está a cerca de 33 600 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>, e tem uma <a href="http://pt.wikipedia.org/wiki/Luminosidade" style="background: none; color: #0b0080; text-decoration: none;" title="Luminosidade">luminosidade</a> total 360 000 vezes maior do que a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Luminosidade_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Luminosidade solar">luminosidade solar</a>, o que dá ao objeto uma <a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a> de -9,2. Messier 15 é um dos aglomerados globulares mais densos conhecidos da <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea" style="background: none; color: #0b0080; text-decoration: none;" title="Via-Láctea">Via-Láctea</a>. Seu núcleo sofre uma contração conhecida como "<a class="new" href="http://pt.wikipedia.org/w/index.php?title=Colapso_de_n%C3%BAcleo&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Colapso de núcleo (página não existe)">colapso de núcleo</a>"; seu núcleo tem uma densidade estelar elevada, com uma quantidade enorme de estrelas orbitando o que pode ser um <a href="http://pt.wikipedia.org/wiki/Buraco_negro" style="background: none; color: #0b0080; text-decoration: none;" title="Buraco negro">buraco negro</a> central.</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.4px;"><a href="http://pt.wikipedia.org/wiki/Messier_15">http://pt.wikipedia.org/wiki/Messier_15</a></span></span></div>
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<a class="extiw" href="http://en.wikipedia.org/wiki/Messier_15" style="background: none rgb(251, 251, 251); color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px; text-decoration: none;" title="en:Messier 15">en:Messier 15</a><span style="background-color: #fbfbfb; color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px;"> by </span><a class="extiw" href="http://en.wikipedia.org/wiki/Hubble_Space_Telescope" style="background: none rgb(251, 251, 251); color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px;" title="en:Hubble Space Telescope">en:Hubble Space Telescope</a><span style="background-color: #fbfbfb; color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px;">; 3.4′ view</span></div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Messier 15</b></td></tr>
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Messier 15 pelo Telescópio Espacial Hubble</td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1764" style="background: none; color: #0b0080; text-decoration: none;" title="1764">1764</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Pegasus" style="background: none; color: #0b0080; text-decoration: none;" title="Pegasus">Pegasus</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-image: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">21<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 29<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 58,38<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_15#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-image: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">+12° 10′ 00,6″<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_15#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">33 600 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (10,3 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">6,2<span class="reference" id="cite_ref-simbad_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_15#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">18',0</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">88 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a></td></tr>
<tr style="vertical-align: top;"><td>Idade estimada</td><td style="background-color: #f8f8f8;">13,2 bilhões de anos</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 7078</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-image: none; color: #0b0080; text-decoration: none;" title="Messier 15"><img alt="Messier 15" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; vertical-align: middle;" width="15" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Pegasus_constellation_map.png" style="background-image: none; color: #0b0080; text-decoration: none;"><img alt="Pegasus constellation map.png" data-file-height="2269" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/1/1e/Pegasus_constellation_map.png/250px-Pegasus_constellation_map.png" height="222" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/1e/Pegasus_constellation_map.png/375px-Pegasus_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/1/1e/Pegasus_constellation_map.png/500px-Pegasus_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<b>Foi o primeiro aglomerado globular a ter uma <a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa planetária">nebulosa planetária</a>, Pease I</b>, descoberta por <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Francis_Gladheim_Pease&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Francis Gladheim Pease (página não existe)">Francis Gladheim Pease</a> no <a href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_Monte_Wilson" style="background: none; color: #0b0080; text-decoration: none;" title="Observatório Monte Wilson">Observatório Monte Wilson</a>, em 1927. Até hoje, conhece-se apenas quatro nebulosas planetárias pertencentes a aglomerados globulares na Via-Láctea.<span class="reference" id="cite_ref-Gillettetal1989_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_15#cite_note-Gillettetal1989-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> <span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_15#cite_note-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> </div>
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<span style="color: black; font-family: "times new roman"; line-height: normal;"><a href="http://pt.wikipedia.org/wiki/Messier_15">http://pt.wikipedia.org/wiki/Messier_15</a></span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.4px;">http://pt.wikipedia.org/wiki/Messier_15#mediaviewer/File:M15pease1_(HST).jpg</span></span></div>
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<span style="background-color: white;">A <a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background-image: none; color: #0b0080;" title="Nebulosa planetária">nebulosa planetária</a> Pease I, contida em M15, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-image: none; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a></span></div>
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<span style="background-color: white;">HST (WFPC2)</span></div>
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Pease 1: Planetary Nebula in M15</h2>
<i><a href="http://messier.obspm.fr/planetar.html">Planetary Nebula</a> Pease 1</i> (PK 065-27.1, Kuster 648) in globular cluster <a href="http://messier.obspm.fr/m/m015.html"><b>M15</b></a> in <a href="http://messier.obspm.fr/map/Peg.html">Pegasus</a></center>
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<a href="http://messier.obspm.fr/Pics/Jpg/m15_p1cap.jpg"><img align="right" alt="[Pease 1 in M15, Stan Moore]" border="0" src="http://messier.obspm.fr/Pics/More/m15_p1sm.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">21 : 30.02 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+12 : 10.2 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">32.6 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">15.5 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">3 (arc seconds)</td></tr>
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Pease 1 was the first planetary nebula found in a globular cluster, in 1928 by <a href="http://messier.obspm.fr/more/m015_pease1.html#pease1928">Francis Gladheim Pease</a>. It had been previously cataloged as a star by <a href="http://messier.obspm.fr/more/m015_pease1.html#kustner1921">Friedrich Kustner (1921)</a>.</div>
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Stan Moore has been able to image Pease 1 in an RGB image obtained with a ST-7 CCD camera on a 12.5-inch RC telescope.</div>
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SAIBA MAIS</div>
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sobre Pease 1</div>
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acessando</div>
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A Golden Planetary</h2>
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<span style="text-align: -webkit-center;">by </span><a href="http://leo.astronomy.cz/" style="text-align: -webkit-center;">Leos Ondra</a></div>
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<a href="http://messier.obspm.fr/xtra/leos/pease1.html">http://messier.obspm.fr/xtra/leos/pease1.html</a></div>
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Existem também nove <a href="http://pt.wikipedia.org/wiki/Pulsar" style="background-image: none; color: #0b0080; text-decoration: none;" title="Pulsar">pulsares</a>, <a href="http://pt.wikipedia.org/wiki/Estrela_de_n%C3%AAutrons" style="background-image: none; color: #0b0080; text-decoration: none;" title="Estrela de nêutrons">estrelas de nêutrons</a> remanescentes de <a href="http://pt.wikipedia.org/wiki/Supernova" style="background-image: none; color: #0b0080; text-decoration: none;" title="Supernova">supernovas</a> da época que o aglomerado ainda era jovem. Estas têm as designações PSR 2127+11 A a PSR 2127+11 H. PSR 2127+11 C é um <a href="http://pt.wikipedia.org/wiki/Estrela_bin%C3%A1ria" style="background-image: none; color: #0b0080; text-decoration: none;" title="Estrela binária">binário</a> de estrelas de nêutrons. De forma semelhante aos binários de pulsares <a href="http://pt.wikipedia.org/wiki/PSR_1913%2B16" style="background-image: none; color: #0b0080; text-decoration: none;" title="PSR 1913+16">PSR 1913+16</a> e <a class="new" href="http://pt.wikipedia.org/w/index.php?title=PSR_1534%2B12&action=edit&redlink=1" style="background-image: none; color: #a55858; text-decoration: none;" title="PSR 1534+12 (página não existe)">PSR 1534+12</a>, o binário de pulsares de Messier 15 exibe efeitos gravitacionais drásticos e a constatação de alguns efeitos previstos pela <a href="http://pt.wikipedia.org/wiki/Relatividade_geral" style="background-image: none; color: #0b0080; text-decoration: none;" title="Relatividade geral">relatividade geral</a> no sistema são evidentes, como mudanças significativas nos periastros das estrelas de nêutrons, efeitos na luz e emissão de <a href="http://pt.wikipedia.org/wiki/Radia%C3%A7%C3%A3o_gravitacional" style="background-image: none; color: #0b0080; text-decoration: none;" title="Radiação gravitacional">radiação gravitacional</a>, que causa uma perda energética no binário e consequentemente uma diminuição no período de <a href="http://pt.wikipedia.org/wiki/Rota%C3%A7%C3%A3o" style="background-image: none; color: #0b0080; text-decoration: none;" title="Rotação">rotação</a> dos pulsares e a diminuição no período de suas órbitas.<span class="reference" id="cite_ref-seds_2-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_15#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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<span class="mw-headline" id="Fonte_de_raios-X"><span style="font-size: small;">Fonte de raios-X</span></span></h2>
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O quarto catálogo "Uhuru" (designada como "4U") contém uma fonte de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Raios-x" style="background: none; color: #0b0080; text-decoration: none;" title="Raios-x">raios-x</a> detectada durante o primeiro ano de funcionamento do satélite observatório de raios-X <a href="http://pt.wikipedia.org/wiki/Uhuru" style="background: none; color: #0b0080; text-decoration: none;" title="Uhuru">Uhuru</a>.<span class="reference" id="cite_ref-Forman_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_15#cite_note-Forman-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> Esta fonte foi catalogada no quarto catálogo "Uhuru" como "4U 2129+12", e é um <a href="http://pt.wikipedia.org/wiki/Bin%C3%A1rio_de_raio_X" style="background: none; color: #0b0080; text-decoration: none;" title="Binário de raio X">sistema binário, emissor de raios-X</a> e de baixa massa. Também foi catalogada como Messier 15 X-1. Além do mais, o <a href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_de_raios-X_Chandra" style="background: none; color: #0b0080; text-decoration: none;" title="Observatório de raios-X Chandra">observatório de raios-X Chandra</a> detectou outro emissor de raios-X no aglomerado que foi catalogado como Messier 15 X-2. Messier 15 X-1 é a primeira <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Fontes_astron%C3%B4micas_de_raios-X&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Fontes astronômicas de raios-X (página não existe)">fonte astronômica de raios-X</a> detectada na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Pegasus" style="background: none; color: #0b0080; text-decoration: none;" title="Pegasus">Pégaso</a>.<span class="reference" id="cite_ref-White_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_15#cite_note-White-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">http://www.raremaps.com/gallery/enlarge/36551</span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: "arial" , "helvetica" , sans-serif;"><strong>Title: </strong>Les Poissons (Pisces) </span><strong style="font-family: Arial, Helvetica, sans-serif;">Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1260" style="border-bottom: 0px solid rgb(255, 255, 255); font-family: arial, helvetica, sans-serif; text-decoration: none;">John Flamsteed</a><span style="font-family: "arial" , "helvetica" , sans-serif;"> / </span><span style="font-family: "arial" , "helvetica" , sans-serif;"> </span><a href="https://www.raremaps.com/gallery/browse/creator_id/1454" style="border-bottom: 0px solid rgb(255, 255, 255); font-family: arial, helvetica, sans-serif; text-decoration: none;">MJ Fortin</a></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white;"><span style="color: #073763;"><a href="http://www.raremaps.com/gallery/detail/36551/Les_Poissons_Pisces/Flamsteed-Fortin.html">http://www.raremaps.com/gallery/detail/36551/Les_Poissons_Pisces/Flamsteed-Fortin.html</a></span></span></span></div>
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<span style="font-family: "times new roman" , serif;"><b><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Pegasus*.html">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Pegasus*.html</a></b><span style="font-size: 9.5pt;"><o:p></o:p></span></span></div>
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<span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 12pt;">p321</span><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"><o:p></o:p></span></div>
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<span lang="EN-US" style="font-family: "helvetica" , sans-serif; font-size: 8.5pt;">That poetic steed,<o:p></o:p></span></div>
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<span lang="EN-US" style="font-family: "helvetica" , sans-serif; font-size: 8.5pt;">With beamy mane, whose hoof struck out from earth<o:p></o:p></span></div>
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<span lang="EN-US" style="font-family: "helvetica" , sans-serif; font-size: 8.5pt;">The fount of Hippocrene.<o:p></o:p></span></div>
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<span lang="EN-US" style="font-family: "helvetica" , sans-serif; font-size: 7.5pt;">Bryant's</span><span lang="EN-US" style="font-family: "helvetica" , sans-serif; font-size: 7.5pt;"> </span><i><span lang="EN-US" style="font-family: "helvetica" , sans-serif; font-size: 7.5pt;">The Constellations</span></i><span lang="EN-US" style="font-family: "helvetica" , sans-serif; font-size: 7.5pt;">.<o:p></o:p></span></div>
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<b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 14.5pt;">Pegasus,<o:p></o:p></span></b></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">called thus in Germany, but</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Pégase</b> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">in France and</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Pegaso</b> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">in Italy, lies north of the Urn of Aquarius and the easternmost Fish, the stars of the Great Square inclosing the body of the Horse.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Mythologically he was the son of Neptune and Medusa, sprung by his father's command from the blood of the latter which dropped into the sea after her head had been severed by Perseus; and he was named either from</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Πηγαί</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Springs of the Ocean, the place of his birth, or from</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Πηγός</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, Strong. He was snowy white in color, and the favorite of the Muses, for he had caused to flow their fountain Pirene on Helicon, — or Hippocrene on the Acrocorinthus, — whence came one of the constellation titles,</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Fontis Musarum Inventor</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">. Longfellow prettily reproduced in modern dress this portion of the story, in his</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Pegasus in Pound</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, where "this wondrous winged steed with mane of gold," straying into a quiet country village, was put in pound; but, finding his quarters uncomfortable, made his escape, and<o:p></o:p></span></div>
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<span lang="EN-US" style="font-family: "palatino linotype" , serif; font-size: 12pt;">p322</span><span lang="EN-US" style="font-family: "helvetica" , sans-serif; font-size: 10pt;">To those stars he soared again.<o:p></o:p></span></div>
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<span lang="EN-US" style="font-family: "helvetica" , sans-serif; font-size: 10pt; letter-spacing: 24pt;">. . . .<o:p></o:p></span></div>
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<span lang="EN-US" style="font-family: "helvetica" , sans-serif; font-size: 10pt;">But they found upon the greensward<o:p></o:p></span></div>
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<span lang="EN-US" style="font-family: "helvetica" , sans-serif; font-size: 10pt;">Where his struggling hoofs had trod,<o:p></o:p></span></div>
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<span lang="EN-US" style="font-family: "helvetica" , sans-serif; font-size: 10pt;">Pure and bright a fountain flowing<o:p></o:p></span></div>
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<span lang="EN-US" style="font-family: "helvetica" , sans-serif; font-size: 10pt;">From the hoofmarks in the sod.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">He seems, however, to have come back to earth again, for he was subsequently caught by Bellerophon at the waters of his fountain, and ridden by him when he slew the Chimaera, helping in the latter's destruction. By this time classical legend had given him wings, and Bellerophon sought by their aid to ascend to heaven; but Jupiter, incensed by his boldness, caused an insect to sting the steed, which threw his rider, and, as Wordsworth wrote:<o:p></o:p></span></div>
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<span lang="EN-US" style="font-family: "helvetica" , sans-serif; font-size: 10pt;">Bold Bellerophon (so Jove decreed<o:p></o:p></span></div>
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<span lang="EN-US" style="font-family: "helvetica" , sans-serif; font-size: 10pt;">In wrath) fell headlong from the fields of air.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Pegasus then rose alone to his permanent place among the stars, becoming the Thundering Horse of Jove that carried the divine lightning.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Ptolemy mentioned the wings as well recognized in his day; and this has continued till ours, for the sky figure is now known as the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Winged Horse</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, — a recurrence to Etruscan, Euphratean, and Hittite ideas, for the wings are clearly represented on a horse's figure on tablets, vases, etc., of those countries, where this constellation may have been known in pre-classical times. Indeed, it is said to have been placed in the heavens by the early Aryans to represent Asva, the Sun.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Early classical mythology did not associate the Horse with Perseus, although artists and authors do not seem to have remembered this, for the celebrated picture by Rubens in the Berlin Gallery shows the winged Pegasus held by a Cupid, while Perseus in full armor is unbinding Andromeda from the rocks, Cetus raging in the waters close by; and the late Lord Leighton left unfinished his</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Perseus on Pegasus</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">at the cliffs of Joppa, with the Gorgoneion in his hand; while in</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Troilus and Cressida</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Shakespeare mentioned "Perseus' horse."<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">The Greeks called the constellation simply</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Ίππος</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, although Aratos added</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">ἱερός</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, "divine," and Eratosthenes alluded to it as</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Πήγασος</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, but distinctly asserted that it was without wings, and until after middle classical times it generally was so drawn, although loose plumes at the shoulders occasionally were added. The figure was considered incomplete, a possible reason for this being given under Aries. Thus it was characterized as</span><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">ἡμιτελής</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">and</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">ἡμίτομος</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, "cut in two," or as if partly hidden in the clouds; while Nonnus had</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Ἡμιφανής</span></b><b><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span></b><b><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Λίβῦς</span></b><b><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span></b><b><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">ἴππος</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Half-visible Libyan Horse.</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 12pt;">p323</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Thus the Equi Sectio used by Tycho and others for Equuleus would seem equally appropriate for this.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Euripides is said to have called it</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Melanippe</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, after a daughter of Chiron, also known as Euippe, changed by the goddess Artemis into a Black Mare and placed in the sky; but Bayer quoted from some later writer</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Menalippe</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">. The</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Θεαιανα</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">,º</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">or</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Theano</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, of Nonnus does not seem intelligible.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Translated from Greece by the Romans, it was</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Equus</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, and later on</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Equus Ales</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, qualified at times by the adjectives</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> alter</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">,</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> major</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">,</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Gorgoneus</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, and</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Medusaeus</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">; but Isidorus and Lampridius degraded it to</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Sagmarius Caballus</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, a Pack-horse;</span><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Pegasus*.html#noteA"><b><sup><span lang="EN-US" style="color: blue; font-family: "verdana" , sans-serif; font-size: 7pt;">a</span></sup></b></a><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">La Lande cited</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Ephippiatus</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, Caparisoned; and elsewhere it was</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Cornipes</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, Horn-footed;</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Sonipes</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, Noisy-footed; and</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Sonipes Ales</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">. Germanicus was apparently the first of Latin authors to style it Pegasus.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">In the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Alfonsine Tables</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">it was</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Alatus</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, Winged,</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Secundus </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">sometimes being added to distinguish it from Equuleus, which preceded it on the sphere; the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Almagest</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">of 1551 had</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Equus Pegasus</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, which the 17th‑century astronomers extended to</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Pegasus Equus alatus</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">. Caesius cited</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Pegasides</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, and Bayer quoted</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Equus posterior</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">,</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">volans</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">,</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">aëreus</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, and</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">dimidiatus</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">,</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Bellerophon</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, and</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Bellerophontes</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Jewish legends made it the mighty</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Nimrod's Horse</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">; Caesius, one of those of</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><a href="http://www.newadvent.org/bible/jer004.htm#13" target="offsite"><i><span lang="EN-US" style="color: blue; font-family: "palatino linotype" , serif; font-size: 12pt;">Jeremiah</span></i><span lang="EN-US" style="color: blue; font-family: "palatino linotype" , serif; font-size: 13.5pt; text-decoration: none;"> </span><span lang="EN-US" style="color: blue; font-family: "palatino linotype" , serif; font-size: 12pt;">iv, 13</span></a><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, that "are swifter than eagles"; other pious people, the<b>Ass</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">on which Christ made his triumphal entry into Jerusalem; but Julius Schiller exalted it into the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Archangel Gabriel</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">. Weigel drew it as the heraldic</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Lüneburg Horse</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Pegasus appears on coins of Corinth from 500 to 430 </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 10pt;">B.C.</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, and from 350 to 338 </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 10pt;">B.C.</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, and 200 years thereafter, on the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">decadrachma</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, complete and with wings; as well as on coins of Lampsacus, Scepsis, and Carthage, — on these last with the asterisk of the sun, or with the winged disc, and the hooded snakes over its back. It is also shown on a coin of Narbonne as a sectional winged figure, and as a winged horse on a Euphratean gem, with a bull's head, a crescent moon, and three stars in the field. A coin of Panormus, the modern Palermo, has the Horse's head with what was probably intended for a dorsal plume.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Bochart said that the word is a compound of the Phoenician</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Pag</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, or</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Pega</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, and</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Sūs</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Bridled Horse, used for the figurehead on a ship, which would account for the constellation being shown with only the head and fore quarters; but others have considered it of Egyptian origin, from</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Pag</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, "to cease," and</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Sūs</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, "a vessel," thus symbolizing the cessation of navigation at the change of the Nile flow. From this, Pegasus seems to have been regarded, in those countries at least, as the sky emblem of a ship. In the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 12pt;">p324</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">old work the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Destruction of Troye</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, we read of "a ship built by Perseus, and named Pegasus, which was likened to a flying horse."<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Brugsch mentions as in its location an Egyptian constellation, the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Servant</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">; and some of its stars would seem to be shown on the Denderah planisphere as a</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Jackal</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">The Arabs knew the familiar quadrangle as</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Dalw</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Water-bucket, the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Amphora</b> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">of some Latin imitator, which generally was used for the Urn in Aquarius; and the Arabian astronomers followed Ptolemy in</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Faras al Thānī</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Second Horse, which Bayer turned into</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Alpheras</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">; Chilmead, into</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Alfaras Alathem</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">; and La Lande, into</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Alpharès</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Argelander catalogued 108 stars here, down to the 6th magnitude; and Heis, 178, to the 6½.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">The starless region toward Pisces was Al Bīrūnī's</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Baldah</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Fox's Kennel</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, a term for whose stellar connection I find no explanation.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Before leaving this constellation, it is worth while to note that an asterism, now virtually lost to us and seldom mentioned except in the lists of Al Sufi, Al Amasch, and Kazwini, is described by the last-named under the title</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Faras al Tamm</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Complete Horse. Although somewhat indefinitely marked out, it is said to have occupied the space between the eastern wing of the Swan, the chest of Pegasus, Equuleus, and the tail of Lacerta, drawing for its components from the last three; but Beigel held that it could have existed only with the grammarians, — the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Tāmm </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">in its title being easily confused, in transcription, with the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Thānī </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">in the Arabians' name for Pegasus. Ideler's</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Sternnamen</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">is the sole modern work in which I find any reference to this Complete Horse, and even that author, in one passage, seems to regard</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Monoceros*.html"><span lang="EN-US" style="color: blue; font-family: "palatino linotype" , serif; font-size: 12pt;">Monoceros</span><span lang="EN-US" style="color: blue; font-family: "palatino linotype" , serif; font-size: 13.5pt; text-decoration: none;"> </span></a><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">as the modern representative of this somewhat mythical constellation; but this is impossible if Kazwini's description be accepted. Indeed, Ideler himself, later on in his book, changed his opinion to agree with that of Beigel.<o:p></o:p></span></div>
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<i><span style="color: #000066; font-family: "verdana" , sans-serif; font-size: 12pt;">α</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, 2.5, white.<o:p></o:p></span></div>
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<b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Markab</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">— Flamsteed's</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Marchab</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">— is the Arabs' word for a Saddle, Ship, or Vehicle, — anything ridden upon, — that was early applied to this star; but they also designated it at</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Matn al Faras</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Horse's Withers or Shoulder, and Bayer cited</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Yed Alpheras</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Horse's Hand, or, more properly, Forearm, — the Arabian</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Yad</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">. Kazwini knew it and </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">β</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">as</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al </b></span><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ʽ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Ar</span></b><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ḳ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">uwah</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Cross-bar of the well in which Al Dalw, the Bucket, was used.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">In India it was noted as the junction star of the Bhādra-padā</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> nakshatra</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">s, detailed</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Pegasus*.html#Beta"><span lang="EN-US" style="color: blue; font-family: "palatino linotype" , serif; font-size: 12pt;">under </span><i><span style="color: blue; font-family: "verdana" , sans-serif; text-decoration: none;">β</span></i></a><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 12pt;">p325</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">In China it was</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Shih</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, a title borrowed from the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> sieu </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">that it marked.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Brown thinks that, with </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">γ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">and </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">ζ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, it was the Euphratean asterism</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Lik‑bar‑ra</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Hyaena, — perhaps</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Ur‑bar‑ra</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Among astrologers it portended danger to life from cuts, or stabs, and fire. It culminates on the 3d of November, and when on the meridian forms, with </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">γ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the southern side of the Great Square,</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">β</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> and </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">δ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">forming the northern, and all 15° to 18° apart.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Markab's spectrum is Sirian, and it is receding from us at the rate of three quarters of a mile a second.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">It is one of the so‑called lunar stars, much observed in navigation.<o:p></o:p></span></div>
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<i><span style="color: #000066; font-family: "verdana" , sans-serif; font-size: 12pt;">β</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, Irregularly variable, 2.2 to 2.7, deep yellow.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">This is the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Scheat</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">of Tycho, the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Palermo Catalogue</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, and modern lists generally, either from</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Sā</b></span><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ʽ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">id</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Upper Part of the Arm, or, as Hyde suggested, from the early</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Sa</b></span><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ʽ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">d</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, appearing in the subsequent three pairs of stars. Bayer had</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Seat Alpheras</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">; Chilmead,</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Seat Alfaras</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">; Riccioli,<b>Scheat Alpheraz</b>; and Schickard,</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Saidol-pharazi</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Arabian astronomers knew it as</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Mankib al Faras</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Horse's Shoulder, mentioned by Ulug Beg and still occasionally seen as</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Menkib</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">. Chilmead had</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Almenkeb</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">The Great Square, of which</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">β</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> formed one corner, constituted the double asterism, the 24th and 25th </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">nakshatra</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">s,</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Pūrva</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, Former, and</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Uttara</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, Latter,</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Bhādra-padā</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, Beautiful, Auspicious, or Happy Feet, sometimes also called</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Proshtha-padā</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">,</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Proshtha </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">meaning a Carp or Ox; but Professor Whitney translated it "Footstool Feet," and said that the authorities do not agree as to the figures by which they are represented, for by some the one, by others the other, is called a Couch or Bed, the alternate one, in either case, being pronounced a Bifaced Figure, or Twins. This Couch is not an inapt representation of the group if both asterisms are taken together, the four stars well marking the feet. Weber calls them</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Pratish</b></span><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ṭ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">hana</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, a Stand or Support, as Whitney wrote,<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "helvetica" , sans-serif; font-size: 10pt;">an evident allusion to the disposition of the four bright stars which compose it, like the four feet of a stand, table, bedstead, or the like;<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">the regents of these</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> nakshatra</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">s being Augusta Ekapāt, the One-footed Goat, and Ahi Budhya, the Bottom Snake, "two mythical figures, of obscure significance, from the Vedic Pantheon." The 24th </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">manzil</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, formed by </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">α</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">and </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">β</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, was</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Fargh al Mu</b></span><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ḳ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">dim</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Fore Spout,</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">i.e.</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> of the water-bucket, — Al </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 12pt;">p326</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Bīrūnī's</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Fargh al Awwal</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the First, or the Upper, Spout; and the 24th </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">sieu </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">was these same stars known as</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Ying She</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, or</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Shih</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, a House, anciently</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Sal</b> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">and</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Shat</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">; but it also comprised parts of Aquarius and Capricornus. They also were the Persian</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Vaht</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Sogdian and Khorasmian<b>Farshat Bath</b>, and the Coptic</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Artulos</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, all signifying something pertaining to Water; while in astrology</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">β</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> indicated danger to mankind from that element.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Within the area of this Square Argelander counted only about 30 naked-eye stars, but in the clearer sky of Athens Schmidt saw 102.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">It was in the 24th </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">sieu </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">that the Chinese record a conjunction of the planets Mercury, Mars, Jupiter, and Saturn, on the 28th of February, 2449 </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 10pt;">B.C.</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, according to Bailly's computations; but we sometimes see this statement made as to five planets, Venus being added, and as having taken place on the 29th of February, that year being bissextile. Smyth indefinitely mentions this conjunction as at some point between</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">α</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Arietis and the Pleiades; Flammarion states that it was in Capricorn; and Steele alludes to it as of 2246 </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 10pt;">B.C.</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, and between the tenth and eighteenth degrees of Pisces. At that date the signs and constellations were about coincident.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">The variability of </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">β</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">was discovered by Schmidt in 1847, and Argelander found a period of forty-one days; but Schoenfeld thinks that irregular oscillations, in a period of thirty to fifty days, are more probable.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">The spectrum of Scheat is of the third type of Secchi's classification, which includes the red and orange stars and most of the variables: "</span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">α</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Orionis,</span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">α</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Herculis, Antares, and</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">ο</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Ceti (Mira) are good examples."<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">The star is receding from us about four miles a second.<o:p></o:p></span></div>
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<i><span style="color: #000066; font-family: "verdana" , sans-serif; font-size: 12pt;">γ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, 3, white,<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">erroneously placed by Tycho in Pisces, marks the extreme tip of the Horse's wing, so that its name</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Algenib</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">has been considered as derived from</span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Al Janā</span></b><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ḥ</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Wing, but it probably is from</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Janb</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Side. It has sometimes been written</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Algemo</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">. Al Bīrūnī quoted it, with </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">δ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">(</span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">α</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Andromedae), as</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Fargh al Thānī</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Second, or Lower, Spout,</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">i.e.</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> of the Bucket. This also is the title of the 25th</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> manzil</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, but appears in Professor Whitney's list as</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Fargh al Mu</b></span><b><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">᾽</span></b><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ḥ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">ir</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Rear Spout, and in Smyth's as</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Fargu</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Chrysococca called it</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Πήγασος</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">from the constellation.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Reeves said that it is the Chinese</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Peih</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, a Wall or Partition, thus taking the title of the 25th </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">sieu</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, which it marked and, with </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">δ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, constituted. It lies at the junction of the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> nakshatra</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">s Bhādrapadā and Revatī; and, with </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">δ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, was included in the corresponding lunar station of several other nations.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 12pt;">p327</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">With the same star and</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">β</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Cassiopeiae it makes up the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Three Guides</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, all these being almost exactly on the prime meridian, the vernal equinox lying in a starless region of Pisces about 15° south of</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">γ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Pegasi. Two 11th‑magnitude stars are close by.<o:p></o:p></span></div>
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<i><span style="color: #000066; font-family: "verdana" , sans-serif; font-size: 12pt;">δ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, 2.2, white.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">This, as already noted, is the same as </span><span lang="EN-US" style="font-family: "palatino linotype" , serif; font-size: 13.5pt;"><span style="color: #660000;"><b>Alpheratz</b></span></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Andromeda*.html#Alpha" style="color: #073763;"><span lang="EN-US" style="color: blue; font-family: "palatino linotype" , serif; font-size: 12pt;">(</span><i><span style="color: blue; font-family: "verdana" , sans-serif; text-decoration: none;">α</span></i><span lang="EN-US" style="color: blue; font-family: "palatino linotype" , serif; font-size: 12pt;"> Andromedae)</span></a><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, and recognized by astronomers of every age as in either constellation; or, as Aratos wrote,</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">ξυνός</span><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">ἀστήρ</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, "a common star." It seems to be unnamed as a member of Pegasus.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Al Achsasi included it with </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">γ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">in the Fargh al Mu</span><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">᾽</span><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ḥ</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">ir.</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"><o:p></o:p></span></div>
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<i><span style="color: #000066; font-family: "verdana" , sans-serif; font-size: 12pt;">ε</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, Triple, 2.5, 11.5, and 8.8, yellow, <span style="letter-spacing: -3pt;">––––</span>–, and blue.<o:p></o:p></span></div>
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<span style="color: #660000;"><b><span lang="EN-US" style="font-family: "palatino linotype" , serif; font-size: 13.5pt;">Enif</span></b><span lang="EN-US" style="font-family: "palatino linotype" , serif; font-size: 13.5pt;">,</span><span lang="EN-US" style="font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="font-family: "palatino linotype" , serif; font-size: 13.5pt;">Enf</span></b><span lang="EN-US" style="font-family: "palatino linotype" , serif; font-size: 13.5pt;">, and</span><span lang="EN-US" style="font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="font-family: "palatino linotype" , serif; font-size: 13.5pt;">Enir</span></b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, all titles for this, are from</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Anf</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Nose, by which the Arabians designated it. Scaliger had</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b style="color: #073763;"><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Enf Alpharas</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, and Schickard<b>Aniphol Pharasi</b>. It was also</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Fum al Faras</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Horse's Mouth; and</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Ja</b></span><b style="color: #073763;"><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ḥ</span></b><b style="color: #073763;"><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">falah</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Lip, this last being found on one of their globes.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Bayer quoted from "the interpreters of the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Almagest</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">"</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Grumium</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">and</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Muscida</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, respectively Jaw and Muzzle, so describing its position; but these have become proper names for</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">ξ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Draconis and</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">π</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Ursae Majoris. Flamsteed knew it as</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Os Pegasi</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">With </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">θ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, and the star</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">α</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Aquarii, it was the 23d </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">sieu</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">,</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Goei</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, or</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Wei</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, Steep or Danger, anciently</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Gui</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Enif's spectrum is Solar, and it is receding from us about five miles a second. Gould thinks it probably variable.<o:p></o:p></span></div>
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<i><span style="color: #000066; font-family: "verdana" , sans-serif; font-size: 12pt;">ζ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, 3.7, light yellow.<o:p></o:p></span></div>
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<b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Homam</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">seems to have been first given to this in the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Palermo Catalogue</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, from</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Sa</b></span><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ʽ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">d</span></b><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Pegasus*.html#note1"><b><sup><span lang="EN-US" style="color: blue; font-family: "verdana" , sans-serif; font-size: 7pt;">1</span></sup></b></a><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> al Humām</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Lucky Star of the Hero, in which Ulug Beg included </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">ξ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">; other lists have</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Homan</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">. But Hyde said that the original was</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Hammām</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, Whisperer. Al Tizini mentioned it as</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Sa</b></span><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ʽ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">d al </span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 12pt;">p328</span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Na</span></b><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ʽ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">amah</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Lucky Star of the Ostriches; and Al Achsasi, as</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Nā</b></span><b><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">᾽</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">ir Sa</span></b><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ʽ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">d al Bahāim</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Bright Fortunate One of the Two Beasts, which Al Sufi had said were </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">θ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">and </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">ν</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">. Thus</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">ξ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> was one of the general group</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Su</b></span><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ʽ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">ūd al Nujūm</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Fortunate Stars.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">The Chinese called it</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Luy Tien</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, Thunder.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">7° to the north of </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">ζ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">is the point assigned by Denning as the radiant of the first stream of</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Pegasids</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the meteors visible about the 28th of June; although Espin locates it near</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">δ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Cygni.<o:p></o:p></span></div>
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<i><span style="color: #000066; font-family: "verdana" , sans-serif; font-size: 12pt;">η</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, Double, 3.2,<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">on the left forearm, is the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Matar</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> of Whitall's</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Planisphere</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, from</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Sa</b></span><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ʽ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">d al Ma</span></b><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ṭ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">ar</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Fortunate Rain; as such, however,</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">ο</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> was included with it.<o:p></o:p></span></div>
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<i><span style="color: #000066; font-family: "verdana" , sans-serif; font-size: 12pt;">θ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, 3.8, and </span><i><span style="color: #000066; font-family: "verdana" , sans-serif; font-size: 12pt;">ν</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, 4.8,<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">were Al Sufi's</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Sa</b></span><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ʽ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">d al Bahāim</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Good Luck of the Two Beasts; Al Achsasi adding to the group the still brighter </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">ζ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">.</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">θ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> alone is</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Baham</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">in some modern lists; but Ulug Beg had</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Bihām</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Young of domestic animals.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">It appears on the Dresden globe as</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al </b></span><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">Ḥ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">awā</span></b><b><span style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">᾽</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">im</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Thirsty Camels.<o:p></o:p></span></div>
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<i><span style="color: #000066; font-family: "verdana" , sans-serif; font-size: 12pt;">κ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, Triple and binary, 4.8. 5.3, and 10.8, yellowish and orange,<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">marking the right forearm, is unnamed except in China, where it is</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Jih</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Sun, a title also for</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">κ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> and </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">λ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Librae.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">The two largest stars were divided by Burnham in 1880 and found to be 0ʺ.2 apart, this decreasing to 0ʺ.1 in 1891. Their orbital period of revolution is 11½ years, and, with that of</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">δ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Equulei, the most rapid known to astronomers until See discovered the binary character of</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span lang="EN-US" style="color: #000066; font-family: "verdana" , sans-serif;">Ll. 9091</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">in Orion. The first and third stars are 11ʺ apart, at a position angle of 308°.5.<o:p></o:p></span></div>
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<i><span style="color: #000066; font-family: "verdana" , sans-serif; font-size: 12pt;">λ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, 4.1, and </span><i><span style="color: #000066; font-family: "verdana" , sans-serif; font-size: 12pt;">μ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, 3.4,<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">were</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Sa</b></span><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ʽ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">d al Bārī</span></b><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ʽ</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Good Luck of the Excelling One; but Kazwini designated it as</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Sa</b></span><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ʽ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">d al Nāzi</span></b><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ʽ</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Good Luck of the Camel Striving to Get to Pasture.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 12pt;">p329</span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">ν</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> was</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Fum al Faras</b> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">and</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Ja</b></span><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ḥ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">falah</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, but both titles are more correctly applied to </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">ε</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">.<o:p></o:p></span></div>
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<i><span style="color: #000066; font-family: "verdana" , sans-serif;">π</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> was the Chinese</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Woo</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, a Pestle.<o:p></o:p></span></div>
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<i><span style="color: #000066; font-family: "verdana" , sans-serif; font-size: 12pt;">τ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, 4.5,<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">with </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">υ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, was Al Sufi's</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Sa</b></span><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ʽ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">d al Na</span></b><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ʽ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">amah</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, which Knobel thinks should be</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Na</b></span><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ʽ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">āim</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Cross-bars over a well; but they also were known as</span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Al Karab</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Bucket-rope.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">The usual titles for </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">τ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">—</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Markab</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">and</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Sagma</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">or</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Salma</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">— are from Bayer, but the last two should be</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Salm</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, a Leathern Bucket.<o:p></o:p></span></div>
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<i><span style="color: #000066; font-family: "verdana" , sans-serif;">λ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">μ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">,</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">η</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">ο</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, and</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">υ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span style="color: #000066; font-family: "verdana" , sans-serif;">τ</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, forming a group of three pairs, were a noted asterism in Chian, under the title</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Li Kung</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">This long list of names for rather inconspicuous stars shows unusual early interest in the constellation.<o:p></o:p></span></div>
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<b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 14.5pt;">The Author's Notes:<o:p></o:p></span></b></div>
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<a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Pegasus*.html#ref1"><b><sup><span lang="EN-US" style="color: blue; font-family: "verdana" , sans-serif; font-size: 7pt;">1</span></sup></b></a><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">This Arabic</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> Sa</span><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ʽ</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">d</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">is our "Good Luck" and a component word of many titles in the Desert sky, all of which seem to have been applied to stars rising in the morning twilight at the commencement of the pleasant season of spring.</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Sa</b></span><b><span lang="EN-US" style="color: #000066; font-family: "times new roman" , serif; font-size: 13.5pt;">ʽ</span></b><b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">dain</span></b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the dual form, was the title for Jupiter and Venus, the Two Fortunate Planets;</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> <b>Al Nahsān</b></span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, the Unlucky, referring to Mars and Saturn.<o:p></o:p></span></div>
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<b><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 14.5pt;">Thayer's Note:<o:p></o:p></span></b></div>
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<a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Pegasus*.html#refA"><b><sup><span lang="EN-US" style="color: blue; font-family: "verdana" , sans-serif; font-size: 7pt;">a</span></sup></b></a><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Though Isidore refers to a</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> caballus sagmarius</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, just once,</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><a href="http://penelope.uchicago.edu/Thayer/L/Roman/Texts/Isidore/20*.html#16.5" target="Isidore"><i><span lang="EN-US" style="color: blue; font-family: "palatino linotype" , serif; font-size: 12pt;">Etym.</span></i><span lang="EN-US" style="color: blue; font-family: "palatino linotype" , serif; font-size: 12pt;"> </span><span lang="EN-US" style="color: blue; font-family: "palatino linotype" , serif; font-size: 10pt; text-decoration: none;">XX</span><span lang="EN-US" style="color: blue; font-family: "palatino linotype" , serif; font-size: 12pt;">.16.5</span></a><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">, it is not in the context of the stars or mythology, and he is not speaking of Pegasus; merely of saddlery. Similarly, "Lampridius" — better: the author of the</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">Historia Augusta</span></i><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">— refers to</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> sagmarii </span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">twice, but each time in the horsy context of normal military operations: once in the Life of Elagabalus</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><a href="http://penelope.uchicago.edu/Thayer/L/Roman/Texts/Historia_Augusta/Elagabalus/1*.html#4.4" target="Historia_Augusta"><span lang="EN-US" style="color: blue; font-family: "palatino linotype" , serif; font-size: 12pt;">(4.4)</span><span lang="EN-US" style="color: blue; font-family: "palatino linotype" , serif; font-size: 13.5pt; text-decoration: none;"> </span></a><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">and once in the Life of Aurelian</span><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;"> </span><a href="http://penelope.uchicago.edu/Thayer/L/Roman/Texts/Historia_Augusta/Aurelian/1*.html#7.7" target="Historia_Augusta"><span lang="EN-US" style="color: blue; font-family: "palatino linotype" , serif; font-size: 12pt;">(7.7)</span></a><span lang="EN-US" style="color: #000066; font-family: "palatino linotype" , serif; font-size: 13.5pt;">.<o:p></o:p></span></div>
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<span style="font-family: "times new roman" , serif;"><b><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Pegasus*.html">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Pegasus*.html</a></b></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhAdCACSPijNrn5v_OxgXj-6MoQ2YeqVNu6DT3L2WUcUV9ZDfYcB7TV8n7hzXGu695nZ-nsYfDJ6LFXY_PLpjMGn2EPDkP9GK5SeOV6juipkHPeu7DlcGfawG8NEu7F0EcwRCbTSLPeV3oE/s1600/andromeda,+perseus+-+guido+reni+-+1635.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><img border="0" height="640" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhAdCACSPijNrn5v_OxgXj-6MoQ2YeqVNu6DT3L2WUcUV9ZDfYcB7TV8n7hzXGu695nZ-nsYfDJ6LFXY_PLpjMGn2EPDkP9GK5SeOV6juipkHPeu7DlcGfawG8NEu7F0EcwRCbTSLPeV3oE/s640/andromeda,+perseus+-+guido+reni+-+1635.jpg" style="border-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="512" /></span></a></div>
<span style="font-family: "arial" , "helvetica" , sans-serif;"><a href="https://www.facebook.com/MuseoImmaginarioArtisenzaTempo?ref=ts&fref=ts" style="color: #274e13; text-decoration: none;">https://www.facebook.com/MuseoImmaginarioArtisenzaTempo?ref=ts&fref=ts</a><br />Andromeda e Perseus - Guido Reni, 1635</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEizDCVUGV1Hx7mJGG5LmSAIsC51RN7feoHI0QjP-KO_WlI-MXOY3nXXF85M3nfU-oWEVSN6nFU2jCwB2HBJbma_BB_lrKM3X5ZXewSYgQnvSRwaEFVhcteyJ7ENnK7TDZt3GAX5zUg2muR3/s1600/hir2full.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"></span></a></div>
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<b><span style="color: #274e13; font-family: "arial" , sans-serif;">Os desenhos formados pelas estrelas </span></b><br />
<b><span style="color: #274e13; font-family: "arial" , sans-serif;">- AS CONSTELAÇÕES - </span></b><br />
<b><span style="color: #274e13; font-family: "arial" , sans-serif;">são como janelas que se abrem para a infinitude do universo </span></b><br />
<b><span style="color: #274e13; font-family: "arial" , sans-serif;">e que possibilitam nossa mente a ir percebendo que existe mais, </span></b><br />
<b><span style="color: #274e13; font-family: "arial" , sans-serif;">bem mais, </span></b><br />
<b><span style="color: #274e13; font-family: "arial" , sans-serif;">entre o céu e a terra..., </span></b><br />
<b><span style="color: #274e13; font-family: "arial" , sans-serif;">bem como percebendo que o caos, </span></b><br />
<b><span style="color: #274e13; font-family: "arial" , sans-serif;">vagarosamente, </span></b><br />
<b><span style="color: #274e13; font-family: "arial" , sans-serif;">vai se tornando Cosmos e este por nossa mente sendo conscientizado.<o:p></o:p></span><br /><span style="color: #274e13; font-family: "arial" , sans-serif;"><br /></span></b></div>
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<b><span style="color: #274e13;"><span style="font-family: "arial" , sans-serif;"></span><span style="font-family: "arial" , sans-serif;">Quer dizer, </span></span></b><br />
<b><span style="color: #274e13;"><span style="font-family: "arial" , sans-serif;">nossa mente é tão infinita quanto infinito é o Cosmos.</span></span><br /><span style="color: #274e13; font-family: "arial" , sans-serif;"><br /></span></b></div>
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<span style="color: #274e13;"><b><span style="font-family: "arial" , sans-serif;"></span><span style="font-family: "arial" , sans-serif;">Com um abraço estrelado,</span></b></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="color: #274e13;"><b>Janine Milward</b></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><b><span style="font-family: "arial" , sans-serif;"><br />
</span></b><b><span lang="PT" style="font-family: "arial" , sans-serif;">Da Terra ao Céu <o:p></o:p></span></b></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><b><span lang="PT" style="font-family: "arial" , sans-serif;"> e ao Infinito </span></b><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
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<span lang="PT" style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Constelações, Estrelas e Objetos Celestes<o:p></o:p></span></span></div>
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<span lang="PT" style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">(sob o ponto de vista do Mundo Ocidental)<o:p></o:p></span></span></div>
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<span lang="PT" style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Suas histórias, seus mitos, seus significados e suas sintetizadas
descrições<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span lang="PT" style="font-family: "arial" , sans-serif;">Reunião das
Informações e Compilação,</span><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span lang="PT" style="font-family: "arial" , sans-serif;">Tradução para a
língua portuguesa (em alguns momentos)</span><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span lang="PT" style="font-family: "arial" , sans-serif;">bem como
Comentários Pessoais:</span><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><i><span lang="PT" style="font-family: "arial" , sans-serif;">Janine Milward</span></i><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">Os desenhos formados pelas estrelas - AS CONSTELAÇÕES - são
como janelas que se abrem para a infinitude do universo e que possibilitam
nossa mente a ir percebendo que existe mais, bem mais, entre o céu e a terra
bem como percebendo que o caos, vagarosamente, vai se tornando Cosmos e este
por nossa mente sendo conscientizado. Quer dizer, nossa mente é tão infinita
quanto infinito é o Cosmos.</span><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Alguns dados<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">(tais como Ascensão Reta e Declinação, em muitos dos casos)<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">são época/equinócio 1980<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">e devem requerer do Caminhante do Céu<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">alguma pequena retificação.<o:p></o:p></span></span></div>
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<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="font-family: "arial" , sans-serif;">Visitando os Sites abaixo,</span><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="font-family: "arial" , sans-serif;"> você conseguirá informações
atualizadas e preciosas</span><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="font-family: "arial" , sans-serif;">sobre os Objetos Celestiais de
seu interesse:</span><span style="font-family: "arial" , sans-serif;"><o:p></o:p></span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><b><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">NASA/IPAC</span></b><b><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;"> EXTRAGALACTIC DATABASE
–</span></b><b><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;"><o:p></o:p></span></b></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><a href="http://ned.ipac.caltech.edu/"><b><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">http://ned.ipac.caltech.edu/</span></b></a><b><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;"><o:p></o:p></span></b></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html"><b><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">http://ned.ipac.caltech.edu/forms/byname.html</span></b></a><b><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;"><o:p></o:p></span></b></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><em><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">NASA/IPAC Extragalactic Database (NED) -</span></b></em><span class="apple-converted-space"><b><i><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;"> </span></i></b></span><em><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;"> operated by the Jet Propulsion Laboratory,
California Institute of Technology, under contract with the National
Aeronautics and Space Administration.</span></b></em><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;"><o:p></o:p></span></b></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
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<b><span lang="EN-US" style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">THE NIGHT SKY
ATLAS<o:p></o:p></span></span></b></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp"><span lang="EN-US" style="font-family: "arial" , sans-serif;">http://www.nightskyatlas.com/index.jsp</span></a><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;"><o:p></o:p></span></b></span></span></div>
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<b><span lang="EN-US" style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">The night sky atlas creates images of any part of the night sky,
allowing easy location of any object. Detailed chart images show all stars
visible to the naked eye, the constellations, Messier objects, and names of the
brightest stars.<o:p></o:p></span></span></b></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">The</span></b><span class="apple-converted-space"><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;"> </span></b></span><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">Internet STELLAR DATABASE</span></b><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;"><o:p></o:p></span></b></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><a href="http://www.stellar-database.com/"><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">http://www.stellar-database.com/</span></b></a><b><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;"><o:p></o:p></span></b></span></span></div>
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<b><span lang="EN-US" style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">- stars within 75
light-years. (Plus some of the more well-known "name brand"
stars farther away.)<o:p></o:p></span></span></b></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
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<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><b><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">REFERÊNCIAS BIBLIOGRÁFICAS:</span></b><span style="font-family: "arial" , "sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
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<span lang="PT" style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">COMPILAÇÃO E TRADUÇÃO literal
(quando necessária) de Janine Milward:<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="font-family: "arial" , sans-serif;">As Cartas Celestes foram realizadas por Mario Jaci Monteiro e escaneadas
por Janine</span><span style="font-family: "times new roman" , serif;"><o:p></o:p></span></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span lang="PT" style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">- </span><b><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">Mario Jaci
Monteiro</span></b><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;"> , <b>As
Constelações, Cartas Celestes</b> -</span><span style="font-family: "times new roman" , serif;"><o:p></o:p></span></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC</span><span style="font-family: "times new roman" , serif;"><o:p></o:p></span></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span lang="PT" style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;"><br />
<!--[if !supportLineBreakNewLine]--><br />
<!--[endif]--></span><span style="font-family: "times new roman" , serif;"><o:p></o:p></span></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">- <b>Wil Tirion
- Atlas of the Night Sky</b> - The Hamlyn Publishing Group Limited,
London, England</span><span lang="EN-US" style="font-family: "arial" , "sans-serif"; mso-ansi-language: EN-US; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">- <b>Antonin
Rükl - The Hamlyn Encyclopedia of Stars & Planets</b> - The Hamlyn
Publishng Group Limited, London, England</span><span lang="EN-US" style="font-family: "arial" , "sans-serif"; mso-ansi-language: EN-US; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span lang="EN-US" style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">- <b>Richard Hinckley
Allen, Star Names, Their Lore and Meaning</b>, Dover Publications, Inc, New
York, USA</span><span lang="EN-US" style="font-family: "arial" , "sans-serif"; mso-ansi-language: EN-US; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span lang="PT" style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">- <b>Bernard
Pellequer - Pequeno Guia do Céu</b> - Editora Martins Fontes, São Paulo,
Brasil</span><span style="font-family: "arial" , "sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">- <b>Identificação do Céu</b> (Livro
que foi sendo revisado e reeditado algumas vezes) de autoria de <b>Fernando
Vieira</b>,</span><span style="font-family: "arial" , "sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">Secretaria Municipal de Cultura, Fundação
Planetário da Cidade do Rio de Janeiro</span><span style="font-family: "arial" , "sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">(com dedicatória do próprio autor para mim em Curso
de Identificação do Céu,</span><span style="font-family: "arial" , "sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">em 30/07/1999))</span><span style="font-family: "arial" , "sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">- 6<sup>a</sup>. Edição do <b>Atlas Celeste</b></span><span style="font-family: "arial" , "sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">de autoria de <b>Ronaldo Rogério de Freitas
Mourão</b>,</span><span style="font-family: "arial" , "sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span><span style="font-family: "arial" , "sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">(com dedicatória do próprio autor para mim</span><span style="font-family: "arial" , "sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">em evento realizado no Museu de Astronomia do Rio
de Janeiro,</span><span style="font-family: "arial" , "sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">em 16/06/1989)</span><span style="font-family: "arial" , "sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="font-family: "arial" , sans-serif;">As Cartas Celestes foram realizadas por Mario Jaci Monteiro e escaneadas
por Janine</span><span lang="PT" style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;"><br />
<!--[if !supportLineBreakNewLine]--><br />
<!--[endif]--></span><span style="font-family: "times new roman" , serif;"><o:p></o:p></span></span></span></div>
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span lang="PT" style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">- </span><b><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;">Mario Jaci
Monteiro</span></b><span style="background-position: initial initial; background-repeat: initial initial; font-family: "arial" , sans-serif;"> , <b>As
Constelações, Cartas Celestes</b> -</span><span style="font-family: "arial" , "sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></span></span></div>
<span style="background-color: white;"><span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><br /></span></span>
<br />
<div class="MsoNormal" style="margin-bottom: 0.0001pt; text-align: justify;">
<span style="background-color: #073763; font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Apoio:
CARJ/MEC/CAPES/PADCT-SPEC - com dedicatória do autor para
mim, em março de 2004 (quando Mário Jaci generosamente me presenteou com um
instrumento de observação (kepleriano) artesanalmente construído por ele).</span></span><span style="font-family: "arial" , "sans-serif"; mso-fareast-font-family: "Times New Roman"; mso-fareast-language: PT-BR;"><o:p></o:p></span></div>
</div>
Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.com