{"id":7863,"date":"2021-03-15T11:57:23","date_gmt":"2021-03-15T15:57:23","guid":{"rendered":"https:\/\/spaceandplanetarynewswire.com\/?p=7863"},"modified":"2021-03-15T11:57:23","modified_gmt":"2021-03-15T15:57:23","slug":"astronomers-detect-a-black-hole-on-the-move","status":"publish","type":"post","link":"https:\/\/spaceandplanetarynewswire.com\/?p=7863","title":{"rendered":"Astronomers Detect a Black Hole on the Move"},"content":{"rendered":"<figure style=\"width: 720px\" class=\"wp-caption alignnone\"><img decoding=\"async\" class=\"size-medium lazyload\" data-src=\"https:\/\/media.eurekalert.org\/multimedia_prod\/pub\/web\/259033_web.jpg\" width=\"720\" height=\"722\" src=\"data:image\/svg+xml;base64,PHN2ZyB3aWR0aD0iMSIgaGVpZ2h0PSIxIiB4bWxucz0iaHR0cDovL3d3dy53My5vcmcvMjAwMC9zdmciPjwvc3ZnPg==\" style=\"--smush-placeholder-width: 720px; --smush-placeholder-aspect-ratio: 720\/722;\"><figcaption class=\"wp-caption-text\">Galaxy J0437+2456 is thought to be home to a supermassive, moving black hole.<\/figcaption><\/figure>\n<p>Scientists have long theorized that supermassive black holes can wander through space&#8211;but catching them in the act has proven difficult.<\/p>\n<p>Now, researchers at the Center for Astrophysics | Harvard &amp; Smithsonian have identified the clearest case to date of a supermassive black hole in motion. Their&nbsp;<a href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/1538-4357\/abde3d\" target=\"_blank\" rel=\"noopener\">results<\/a>&nbsp;are published today in the&nbsp;<em>Astrophysical Journal<\/em>.<\/p>\n<p>&#8220;We don&#8217;t expect the majority of supermassive black holes to be moving; they&#8217;re usually content to just sit around,&#8221; says Dominic Pesce, an astronomer at the Center for Astrophysics who led the study. &#8220;They&#8217;re just so heavy that it&#8217;s tough to get them going. Consider how much more difficult it is to kick a bowling ball into motion than it is to kick a soccer ball &#8212; realizing that in this case, the &#8216;bowling ball&#8217; is several million times the mass of our Sun. That&#8217;s going to require a pretty mighty kick.&#8221;<\/p>\n<p>Pesce and his collaborators have been working to observe this rare occurrence for the last five years by comparing the velocities of supermassive black holes and galaxies.<\/p>\n<p>&#8220;We asked: Are the velocities of the black holes the same as the velocities of the galaxies they reside in?&#8221; he explains. &#8220;We expect them to have the same velocity. If they don&#8217;t, that implies the black hole has been disturbed.&#8221;<\/p>\n<p>For their search, the team initially&nbsp;<a href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/1538-4357\/aad3c2\" target=\"_blank\" rel=\"noopener\">surveyed 10 distant galaxies<\/a>&nbsp;and the supermassive black holes at their cores. They specifically studied black holes that contained water within their accretion disks &#8212; the spiral structures that spin inward towards the black hole.<\/p>\n<p>As the water orbits around the black hole, it produces a laser-like beam of radio light known as a maser. When studied with a combined network of radio antennas using a technique known as very long baseline interferometry (VLBI), masers can help measure a black hole&#8217;s velocity very precisely, Pesce says.<\/p>\n<p>The technique helped the team determine that nine of the 10 supermassive black holes were at rest&#8211;but one stood out and seemed to be in motion.<\/p>\n<p>Located 230 million light-years away from Earth, the black hole sits at the center of a galaxy named J0437+2456. Its mass is about three million times that of our Sun.<\/p>\n<p>Using follow-up observations with the Arecibo and Gemini Observatories, the team has now confirmed their initial findings. The supermassive black hole is moving with a speed of about 110,000 miles per hour inside the galaxy J0437+2456.<\/p>\n<p>But what&#8217;s causing the motion is not known. The team suspects there are two possibilities.<\/p>\n<p>&#8220;We may be observing the aftermath of two supermassive black holes merging,&#8221; says Jim Condon, a radio astronomer at the National Radio Astronomy Observatory who was involved in the study. &#8220;The result of such a merger can cause the newborn black hole to recoil, and we may be watching it in the act of recoiling or as it settles down again.&#8221;<\/p>\n<p>But there&#8217;s another, perhaps even more exciting possibility: the black hole may be part of a binary system.<\/p>\n<p>&#8220;Despite every expectation that they really ought to be out there in some abundance, scientists have had a hard time identifying clear examples of binary supermassive black holes,&#8221; Pesce says. &#8220;What we could be seeing in the galaxy J0437+2456 is one of the black holes in such a pair, with the other remaining hidden to our radio observations because of its lack of maser emission.&#8221;<\/p>\n<p>Further observations, however, will ultimately be needed to pin down the true cause of this supermassive black hole&#8217;s unusual motion.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Scientists have long theorized that supermassive black holes can wander through space&#8211;but catching them in the act has proven difficult. Now, researchers at the Center for Astrophysics | Harvard &amp; Smithsonian have identified the clearest case to date of a supermassive black hole in motion. Their&nbsp;results&nbsp;are published today in the&nbsp;Astrophysical Journal. &#8220;We don&#8217;t expect the&hellip;<\/p>\n","protected":false},"author":71,"featured_media":7865,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"ngg_post_thumbnail":0,"fifu_image_url":"https:\/\/media.eurekalert.org\/multimedia_prod\/pub\/web\/259033_web.jpg","fifu_image_alt":"Astronomers Detect a Black Hole on the Move","footnotes":""},"categories":[216],"tags":[],"class_list":["post-7863","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-discovery"],"_links":{"self":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/7863","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/users\/71"}],"replies":[{"embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=7863"}],"version-history":[{"count":1,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/7863\/revisions"}],"predecessor-version":[{"id":7864,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/7863\/revisions\/7864"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/media\/7865"}],"wp:attachment":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=7863"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=7863"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=7863"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}