{"id":577136,"date":"2019-02-08T05:20:00","date_gmt":"2019-02-08T09:20:00","guid":{"rendered":"https:\/\/spaceweekly.com\/?guid=8e06ac92a16762ae048fab1635d848bc"},"modified":"2019-02-08T05:20:00","modified_gmt":"2019-02-08T09:20:00","slug":"the-darkness-within","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=577136","title":{"rendered":"The darkness within?"},"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\/2019\/02\/the_darkness_within\/19226127-1-eng-GB\/The_darkness_within_small.jpg\" width=\"170\" height=\"96\" align=\"left\" hspace=\"8\" \/><\/p>\n<p>\nThis atmospheric image shows a galaxy named&nbsp;Messier 85, captured in all its delicate, hazy glory by the&nbsp;NASA\/ESA Hubble Space Telescope. Messier 85 slants through the constellation of&nbsp;Coma Berenices&nbsp;(Berenice\u2019s Hair), and lies around 50 million light-years from Earth. It was first discovered by&nbsp;Charles Messier\u2019s&nbsp;colleague&nbsp;Pierre M\u00e9chain&nbsp;in 1781, and is included in the&nbsp;Messier catalogue of celestial objects.\n<\/p>\n<p>\nMessier 85 is intriguing \u2014 its properties lie somewhere between those of a&nbsp;lenticular&nbsp;and an&nbsp;elliptical&nbsp;galaxy, and it appears to be interacting with two of its neighbours: the beautiful spiral&nbsp;NGC 4394, located out of frame to the upper left, and the small elliptical MCG 3-32-38, located out of frame to the centre bottom.\n<\/p>\n<p>\nThe galaxy contains some 400 billion stars, most of which are very old. However, the central region hosts a population of relatively young stars of just a few billion years in age; these stars are thought to have formed in a late burst of&nbsp;star formation, likely triggered as Messier 85 merged with another galaxy over four billion years ago. Messier 85 has a further potentially strange quality. Almost every galaxy is thought to have a&nbsp;supermassive black hole&nbsp;at its centre, but from measurements of the velocities of stars in this galaxy, it is unclear whether Messier 85 contains such a black hole.\n<\/p>\n<p>\nThis image combines infrared, visible and ultraviolet observations from Hubble\u2019s&nbsp;Wide Field Camera 3.<\/p>\n","protected":false},"excerpt":{"rendered":"<p><img loading=\"lazy\" decoding=\"async\" src=\"http:\/\/www.esa.int\/var\/esa\/storage\/images\/esa_multimedia\/images\/2019\/02\/the_darkness_within\/19226127-1-eng-GB\/The_darkness_within_small.jpg\" width=\"170\" height=\"96\" align=\"left\" hspace=\"8\"><\/p>\n<p>\nThis atmospheric image shows a galaxy named&nbsp;Messier 85, captured in all its delicate, hazy glory by the&nbsp;NASA\/ESA Hubble Space Telescope. Messier 85 slants through the constellation of&nbsp;Coma Berenices&nbsp;(Berenice&rsquo;s Hair), and lies around 50 million light-years from Earth. It was first discovered by&nbsp;Charles Messier&rsquo;s&nbsp;colleague&nbsp;Pierre M&eacute;chain&nbsp;in 1781, and is included in the&nbsp;Messier catalogue of celestial objects.\n<\/p>\n<p>\nMessier 85 is intriguing &mdash; its properties lie somewhere between those of a&nbsp;lenticular&nbsp;and an&nbsp;elliptical&nbsp;galaxy, and it appears to be interacting with two of its neighbours: the beautiful spiral&nbsp;NGC 4394, located out of frame to the upper left, and the small elliptical MCG 3-32-38, located out of frame to the centre bottom.\n<\/p>\n<p>\nThe galaxy contains some 400 billion stars, most of which are very old. However, the central region hosts a population of relatively young stars of just a few billion years in age; these stars are thought to have formed in a late burst of&nbsp;star formation, likely triggered as Messier 85 merged with another galaxy over four billion years ago. Messier 85 has a further potentially strange quality. Almost every galaxy is thought to have a&nbsp;supermassive black hole&nbsp;at its centre, but from measurements of the velocities of stars in this galaxy, it is unclear whether Messier 85 contains such a black hole.\n<\/p>\n<p>\nThis image combines infrared, visible and ultraviolet observations from Hubble&rsquo;s&nbsp;Wide Field Camera 3.<\/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-577136","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\/577136","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=577136"}],"version-history":[{"count":1,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/577136\/revisions"}],"predecessor-version":[{"id":577137,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/577136\/revisions\/577137"}],"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=577136"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=577136"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=577136"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}