{"id":369453,"date":"2017-08-31T04:00:00","date_gmt":"2017-08-31T08:00:00","guid":{"rendered":"https:\/\/spaceweekly.com\/?guid=7cc6a299da261cc53a3459099121ddba"},"modified":"2017-08-31T04:00:00","modified_gmt":"2017-08-31T08:00:00","slug":"waiting-for-a-stellar-encounter-2","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=369453","title":{"rendered":"Waiting for a stellar encounter"},"content":{"rendered":"<p>\t\t\t\t\t<img loading=\"lazy\" decoding=\"async\" src=\"http:\/\/www.esa.int\/var\/esa\/storage\/images\/esa_multimedia\/videos\/2017\/08\/waiting_for_a_stellar_encounter\/17127525-1-eng-GB\/Waiting_for_a_stellar_encounter_small.jpg\" width=\"170\" height=\"96\" align=\"left\" hspace=\"8\" \/><\/p>\n<p>\nA view of a small part of the sky as if you were staring at a star (centre) approaching nearly head on, and then as it passes by and away again.\n<\/p>\n<p>\nThe motion can be likened to what an observer standing beside a road would see looking at an approaching car, and then swinging around to continue to follow it as it moves away. As a result, the objects in the background \u2013 in this case distant stars \u2013 become blurred as you move quickly to maintain a visual on the passing object.\n<\/p>\n<p>\nThe focus of this animation is the star known as Gliese 710. It will have a close encounter with our Sun in 1.3 million years, passing within the Oort Cloud reservoir of comets in the outskirts of our Solar System. The star is predicted to pass within about 2.3 trillion kilometres, the equivalent of about 16 000 Earth\u2013Sun distances. The star\u2019s motion is set against a background of other moving stars and the visualisation covers, very quickly, the timeframe from about 1.1\u20131.5 million years in the future.\n<\/p>\n<p>\nThe size of the field of view is 10 x 5\u00ba (for comparison: the Moon spans 0.5\u00ba on the sky) and the colours represent the astronomical colours of the stars as derived from the Gaia data. Gliese 710 is an orange K-type dwarf star, an ordinary star similar to the Sun but less hot and less massive.\n<\/p>\n<p>\n<a href=\"http:\/\/www.esa.int\/Our_Activities\/Space_Science\/Gaia\/Close_encounters_of_the_stellar_kind\">More information<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p><img loading=\"lazy\" decoding=\"async\" src=\"http:\/\/www.esa.int\/var\/esa\/storage\/images\/esa_multimedia\/videos\/2017\/08\/waiting_for_a_stellar_encounter\/17127525-1-eng-GB\/Waiting_for_a_stellar_encounter_small.jpg\" width=\"170\" height=\"96\" align=\"left\" hspace=\"8\"><\/p>\n<p>\nA view of a small part of the sky as if you were staring at a star (centre) approaching nearly head on, and then as it passes by and away again.\n<\/p>\n<p>\nThe motion can be likened to what an observer standing beside a road would see looking at an approaching car, and then swinging around to continue to follow it as it moves away. As a result, the objects in the background &ndash; in this case distant stars &ndash; become blurred as you move quickly to maintain a visual on the passing object.\n<\/p>\n<p>\nThe focus of this animation is the star known as Gliese 710. It will have a close encounter with our Sun in 1.3 million years, passing within the Oort Cloud reservoir of comets in the outskirts of our Solar System. The star is predicted to pass within about 2.3 trillion kilometres, the equivalent of about 16 000 Earth&ndash;Sun distances. The star&rsquo;s motion is set against a background of other moving stars and the visualisation covers, very quickly, the timeframe from about 1.1&ndash;1.5 million years in the future.\n<\/p>\n<p>\nThe size of the field of view is 10 x 5&ordm; (for comparison: the Moon spans 0.5&ordm; on the sky) and the colours represent the astronomical colours of the stars as derived from the Gaia data. Gliese 710 is an orange K-type dwarf star, an ordinary star similar to the Sun but less hot and less massive.\n<\/p>\n<p>\n<a href=\"http:\/\/www.esa.int\/Our_Activities\/Space_Science\/Gaia\/Close_encounters_of_the_stellar_kind\">More information<\/a><\/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-369453","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\/369453","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=369453"}],"version-history":[{"count":1,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/369453\/revisions"}],"predecessor-version":[{"id":369454,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/369453\/revisions\/369454"}],"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=369453"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=369453"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=369453"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}