{"id":533900,"date":"2018-10-12T04:03:00","date_gmt":"2018-10-12T08:03:00","guid":{"rendered":"http:\/\/spaceweekly.com\/?guid=993d9ff91b3d743ae97a263886afb4b4"},"modified":"2018-10-12T04:03:00","modified_gmt":"2018-10-12T08:03:00","slug":"rings-upon-rings","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=533900","title":{"rendered":"Rings upon rings"},"content":{"rendered":"<p>\t\t\t\t\t<img loading=\"lazy\" decoding=\"async\" src=\"http:\/\/www.esa.int\/var\/esa\/storage\/images\/esa_multimedia\/images\/2018\/10\/rings_upon_rings\/17769045-1-eng-GB\/Rings_upon_rings_small.jpg\" width=\"170\" height=\"96\" align=\"left\" hspace=\"8\" \/><\/p>\n<p>\nThis image from the&nbsp;NASA\/ESA Hubble Space Telescope&nbsp;reveals a&nbsp;spiral galaxy&nbsp;named Messier 95 (also known as M95 or NGC 3351). Located about 35 million light-years away in the constellation of&nbsp;Leo (The Lion), this swirling spiral was discovered by astronomer&nbsp;Pierre M\u00e9chain&nbsp;in 1781, and catalogued by French astronomer&nbsp;Charles Messier&nbsp;just four days later. Messier was primarily a comet hunter, and was often left frustrated by objects in the sky that resembled&nbsp;comets&nbsp;but turned out not to be. To help other astronomers avoid confusing these objects in the future, he created his famous catalogue of&nbsp;Messier objects.\n<\/p>\n<p>\nMost definitely not a comet, Messier 95 is actually a&nbsp;barred spiral galaxy. The galaxy has a bar cutting through its centre, surrounded by an inner ring currently forming new stars. Also our own Milky Way is a barred spiral.\n<\/p>\n<p>\nAs well as hosting this stellar nursery, Messier 95 is a known host of the dramatic and explosive final stages in the lives of massive stars:&nbsp;supernovae. In March 2016 a spectacular supernova named SN 2012aw was observed in the outer regions of one of Messier 95\u2019s spiral arms. Once the light from the supernova had faded, astronomers were able to compare observations of the region before and after the explosion to find out which star had \u201cdisappeared\u201d \u2014 the progenitor star. In this case, the star was an especially huge&nbsp;red supergiant&nbsp;up to 26 times more massive than the Sun.<\/p>\n","protected":false},"excerpt":{"rendered":"<p><img loading=\"lazy\" decoding=\"async\" src=\"http:\/\/www.esa.int\/var\/esa\/storage\/images\/esa_multimedia\/images\/2018\/10\/rings_upon_rings\/17769045-1-eng-GB\/Rings_upon_rings_small.jpg\" width=\"170\" height=\"96\" align=\"left\" hspace=\"8\"><\/p>\n<p>\nThis image from the&nbsp;NASA\/ESA Hubble Space Telescope&nbsp;reveals a&nbsp;spiral galaxy&nbsp;named Messier 95 (also known as M95 or NGC 3351). Located about 35 million light-years away in the constellation of&nbsp;Leo (The Lion), this swirling spiral was discovered by astronomer&nbsp;Pierre M&eacute;chain&nbsp;in 1781, and catalogued by French astronomer&nbsp;Charles Messier&nbsp;just four days later. Messier was primarily a comet hunter, and was often left frustrated by objects in the sky that resembled&nbsp;comets&nbsp;but turned out not to be. To help other astronomers avoid confusing these objects in the future, he created his famous catalogue of&nbsp;Messier objects.\n<\/p>\n<p>\nMost definitely not a comet, Messier 95 is actually a&nbsp;barred spiral galaxy. The galaxy has a bar cutting through its centre, surrounded by an inner ring currently forming new stars. Also our own Milky Way is a barred spiral.\n<\/p>\n<p>\nAs well as hosting this stellar nursery, Messier 95 is a known host of the dramatic and explosive final stages in the lives of massive stars:&nbsp;supernovae. In March 2016 a spectacular supernova named SN 2012aw was observed in the outer regions of one of Messier 95&rsquo;s spiral arms. Once the light from the supernova had faded, astronomers were able to compare observations of the region before and after the explosion to find out which star had &ldquo;disappeared&rdquo; &mdash; the progenitor star. In this case, the star was an especially huge&nbsp;red supergiant&nbsp;up to 26 times more massive than the Sun.<\/p>\n","protected":false},"author":5,"featured_media":615444,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[27],"tags":[],"class_list":["post-533900","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-multimedia"],"_links":{"self":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/533900","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/users\/5"}],"replies":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=533900"}],"version-history":[{"count":1,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/533900\/revisions"}],"predecessor-version":[{"id":533901,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/533900\/revisions\/533901"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/media\/615444"}],"wp:attachment":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=533900"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=533900"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=533900"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}