{"id":316167,"date":"2021-08-05T23:10:47","date_gmt":"2021-08-05T20:10:47","guid":{"rendered":"https:\/\/en.buradabiliyorum.com\/huge-rings-around-a-black-hole\/"},"modified":"2021-08-05T23:10:47","modified_gmt":"2021-08-05T20:10:47","slug":"huge-rings-around-a-black-hole","status":"publish","type":"post","link":"https:\/\/buradabiliyorum.com\/en\/huge-rings-around-a-black-hole\/","title":{"rendered":"#Huge rings around a black hole"},"content":{"rendered":"<p>&#8220;<strong>#Huge rings around a black hole<\/strong>&#8221;<\/p>\n<div>\n<div class=\"article-gallery lightGallery\">\n<div data-thumb=\"https:\/\/scx1.b-cdn.net\/csz\/news\/tmb\/2021\/v404-cygni-huge-rings.jpg\" data-src=\"https:\/\/scx2.b-cdn.net\/gfx\/news\/hires\/2021\/v404-cygni-huge-rings.jpg\" data-sub-html=\"Credit: X-ray: NASA\/CXC\/U.Wisc-Madison\/S. Heinz et al.; Optical\/IR: Pan-STARRS\">\n<figure class=\"article-img\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/scx1.b-cdn.net\/csz\/news\/800a\/2021\/v404-cygni-huge-rings.jpg\" alt=\"V404 Cygni: Huge Rings Around a Black Hole\" title=\"Credit: X-ray: NASA\/CXC\/U.Wisc-Madison\/S. Heinz et al.; Optical\/IR: Pan-STARRS\" width=\"800\" height=\"454\"\/><figcaption class=\"text-darken text-low-up text-truncate-js text-truncate mt-3\">\n                Credit: X-ray: NASA\/CXC\/U.Wisc-Madison\/S. Heinz et al.; Optical\/IR: Pan-STARRS<br \/>\n            <\/figcaption><\/figure>\n<\/div>\n<\/div>\n<p>This image features a spectacular set of rings around a black hole, captured using NASA&#8217;s Chandra X-ray Observatory and Neil Gehrels Swift Observatory. The X-ray images of the giant rings reveal information about dust located in our galaxy, using a similar principle to the X-rays performed in doctor&#8217;s offices and airports.<\/p>\n<section class=\"article-banner first-banner ads-336x280\"><!-- \/4988204\/Phys_Story_InText_Box --><br \/>\n      <\/section>\n<p>The black hole is part of a binary system called V404 Cygni, located about 7,800 light years away from Earth. The black hole is actively pulling material away from a companion star\u2014with about half the mass of the Sun\u2014into a disk around the invisible object. This material glows in X-rays, so astronomers refer to these systems as &#8220;X-ray binaries.&#8221;<\/p>\n<p>On June 5, 2015, Swift discovered a burst of X-rays from V404 Cygni. The burst created the high-energy rings from a phenomenon known as light echoes. Instead of sound waves bouncing off a canyon wall, the light echoes around V404 Cygni were produced when a burst of X-rays from the black hole system bounced off of dust clouds between V404 Cygni and Earth. Cosmic dust is not like household dust but is more like smoke, and consists of tiny, solid particles.<\/p>\n<p>In this composite image, X-rays from Chandra (light blue) were combined with optical data from the Pan-STARRS telescope in Hawaii that show the stars in the field of view. The image contains eight separate concentric rings. Each ring is created by X-rays from V404 Cygni flares observed in 2015 that reflect off different dust clouds. (An artist&#8217;s illustration explains how the rings seen by Chandra and Swift were produced. To simplify the graphic, the illustration shows only four rings instead of eight.)<\/p>\n<figure class=\"mb-4\" itemscope=\"\" itemtype=\"http:\/\/schema.org\/VideoObject\"><meta itemprop=\"name\" content=\"V404 Cygni: huge rings around a black hole\"\/><meta itemprop=\"url\" content=\"https:\/\/www.youtube.com\/watch\/?v=IlV98452xpc\"\/><meta itemprop=\"description\" content=\"V404 Cygni: huge rings around a black hole\"\/><meta itemprop=\"uploadDate\" content=\"2021-08-05T16:08:39-04:00\"\/><meta itemprop=\"embedUrl\" content=\"https:\/\/www.youtube.com\/embed\/IlV98452xpc\"\/><meta itemprop=\"thumbnailUrl\" content=\"https:\/\/img.youtube.com\/vi\/IlV98452xpc\/maxresdefault.jpg\"\/><br \/>\n             <iframe loading=\"lazy\" title=\"A Quick Look at V404 Cygni\" width=\"640\" height=\"360\" src=\"https:\/\/www.youtube.com\/embed\/IlV98452xpc?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" referrerpolicy=\"strict-origin-when-cross-origin\" allowfullscreen><\/iframe><\/p>\n<\/figure>\n<p>A team of researchers led by Sebastian Heinz of the University of Wisconsin in Madison analyzed 50 Swift observations of the system made in 2015 between June 30 and August 25, and Chandra observations made on July 11 and 25, 2015. It was such a bright event that the operators of Chandra purposely placed V404 Cygni in between the detectors so that another bright burst would not damage the instrument.<\/p>\n<p>The rings tell astronomers not only about the black hole&#8217;s behavior, but also about the landscape between V404 Cygni and Earth. For example, the diameter of the rings in X-rays reveals the distances to the intervening dust clouds the light ricocheted off. If the cloud is closer to Earth, the ring <a href=\"https:\/\/buradabiliyorum.com\/en\/category\/download-scripts-themes-apps\/\" data-internallinksmanager029f6b8e52c=\"9\" title=\"Download Scripts &amp; Themes &amp; Apps\" target=\"_blank\" rel=\"noopener\">app<\/a>ears to be larger, and vice versa. The light echoes appear as narrow rings rather than wide rings or haloes because the X-ray burst lasted only a relatively short period of time.<\/p>\n<p>The researchers also used the rings to probe the properties of the dust clouds themselves. They compared the X-ray spectra\u2014that is, the brightness of X-rays over a range of wavelengths\u2014to computer models of dust with different compositions. Different compositions of dust will result in different amounts of the lower energy X-rays being absorbed and prevented from being detected with Chandra. This is a similar principle to how different parts of our body or our luggage absorb different amounts of X-rays, giving information about their structure and composition.<\/p>\n<p>The team determined that the dust most likely contains mixtures of graphite and silicate grains. In addition, by analyzing the inner rings with Chandra, they found that the densities of the dust clouds are not uniform in all directions. Previous studies have assumed that they did not.<\/p>\n<div class=\"article-gallery lightGallery\">\n<div data-thumb=\"https:\/\/scx1.b-cdn.net\/csz\/news\/tmb\/2021\/v404-cygni-huge-rings-1.jpg\" data-src=\"https:\/\/scx2.b-cdn.net\/gfx\/news\/2021\/v404-cygni-huge-rings-1.jpg\" data-sub-html=\"This artist's illustration shows in detail how the ringed structure seen by Chandra and Swift is produced. Each ring is caused by X-rays bouncing off of different dust clouds. If the cloud is closer to us, the ring appears to be larger. The result is a set of concentric rings with different apparent sizes depending on the distance of the intervening cloud from us. Credit: Univ. of Wisconsin-Madison\/S.Heinz\">\n<figure class=\"article-img text-center\"><img decoding=\"async\" src=\"https:\/\/scx1.b-cdn.net\/csz\/news\/800a\/2021\/v404-cygni-huge-rings-1.jpg\" alt=\"V404 Cygni: huge rings around a black hole\" title=\"This artist's illustration shows in detail how the ringed structure seen by Chandra and Swift is produced. Each ring is caused by X-rays bouncing off of different dust clouds. If the cloud is closer to us, the ring appears to be larger. The result is a set of concentric rings with different apparent sizes depending on the distance of the intervening cloud from us. Credit: Univ. of Wisconsin-Madison\/S.Heinz\"\/><figcaption class=\"text-left text-darken text-truncate text-low-up mt-3\">\n                This artist&#8217;s illustration shows in detail how the ringed structure seen by Chandra and Swift is produced. Each ring is caused by X-rays bouncing off of different dust clouds. If the cloud is closer to us, the ring appears to be larger. The result is a set of concentric rings with different apparent sizes depending on the distance of the intervening cloud from us. Credit: Univ. of Wisconsin-Madison\/S.Heinz<br \/>\n            <\/figcaption><\/figure>\n<\/div>\n<\/div>\n<p>A paper describing the V404 Cygni results was published in the July 1, 2016, issue of The Astrophysical Journal (preprint). The authors of the study are Sebastian Heinz, Lia Corrales (University of Michigan); Randall Smith (Center for Astrophysics | Harvard &amp; Smithsonian); Niel Brandt (The Pennsylvania State University); Peter Jonker (Netherlands Institute for Space Research); Richard Plotkin (University of Nevada, Reno); and Joey Neilson (Villanova University).<\/p>\n<p>This result is related to a similar finding of the X-ray binary Circinus X-1, which contains a neutron star rather than a black hole, published in a paper in the June 20, 2015, issue of The <i>Astrophysical Journal<\/i>, titled, &#8220;Lord of the Rings: A Kinematic Distance to Circinus X-1 from a Giant X-Ray Light Echo&#8221; (preprint). This study was also led by Sebastian Heinz.<\/p>\n<p>There have been multiple papers published every year reporting studies of the V404 Cygni outburst in 2015 that caused these rings. Previous outbursts were recorded in 1938, 1956 and 1989, so astronomers may still have many years to continue analyzing the 2015 one.<\/p>\n<hr\/>\n<div class=\"article-main__explore my-4 d-print-none\">\n<p>                                            Swift satellite reveals a black hole bull&#8217;s-eye\n                                        <\/p><\/div>\n<hr class=\"mb-4\"\/>\n<div class=\"article-main__more p-4\">\n                                                                                                <strong>More information:<\/strong><br \/>\n                                                S. Heinz et al, A Joint Chandra and Swift View of the 2015 X-Ray Dust Scattering Echo of V404 Cygni, <i>The Astrophysical Journal<\/i> (2016).  <a rel=\"nofollow noopener\" target=\"_blank\" data-doi=\"1\" href=\"http:\/\/dx.doi.org\/10.3847\/0004-637X\/825\/1\/15\">DOI: 10.3847\/0004-637X\/825\/1\/15<\/a> , <a rel=\"nofollow noopener\" target=\"_blank\" href=\"https:\/\/arxiv.org\/abs\/1605.01648\">arxiv.org\/abs\/1605.01648<\/a><\/p><\/div>\n<div class=\"d-inline-block text-medium my-4\">\n                                                Provided by<br \/>\n                                                                                                    Chandra X-ray Center<br \/>\n                                                                                                        <a rel=\"nofollow noopener\" target=\"_blank\" class=\"icon_open\" href=\"http:\/\/chandra.harvard.edu\/\"><br \/>\n                                                        <svg><use href=\"https:\/\/phys.b-cdn.net\/tmpl\/v6\/img\/svg\/sprite.svg#icon_open\" x=\"0\" y=\"0\"\/><\/svg><\/a><\/p><\/div>\n<p>                                        <!-- print only --><\/p>\n<div class=\"d-none d-print-block\">\n<p>                                                 <strong>Citation<\/strong>:<br \/>\n                                                 V404 Cygni: Huge rings around a black hole (2021, August  5)<br \/>\n                                                 retrieved  5 August 2021<br \/>\n                                                 from https:\/\/phys.org\/<a href=\"https:\/\/buradabiliyorum.com\/en\/category\/news\/\" data-internallinksmanager029f6b8e52c=\"2\" title=\"News\" target=\"_blank\" rel=\"noopener\">news<\/a>\/2021-08-v404-cygni-huge-black-hole.html<\/p>\n<p>                                            This document is subject to copyright. 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Heinz et al.; Optical\/IR: Pan-STARRS This image features a spectacular set of rings around a black hole, captured using NASA&#8217;s Chandra X-ray Observatory and Neil Gehrels Swift Observatory. The X-ray images of the giant rings reveal information about dust located in our galaxy, using a similar&#8230;<\/p>\n","protected":false},"author":1,"featured_media":316168,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"fifu_image_url":"https:\/\/scx2.b-cdn.net\/gfx\/news\/hires\/2021\/v404-cygni-huge-rings.jpg","fifu_image_alt":"","footnotes":""},"categories":[16],"tags":[],"class_list":["post-316167","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-sciencee"],"_links":{"self":[{"href":"https:\/\/buradabiliyorum.com\/en\/wp-json\/wp\/v2\/posts\/316167","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/buradabiliyorum.com\/en\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/buradabiliyorum.com\/en\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/buradabiliyorum.com\/en\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/buradabiliyorum.com\/en\/wp-json\/wp\/v2\/comments?post=316167"}],"version-history":[{"count":0,"href":"https:\/\/buradabiliyorum.com\/en\/wp-json\/wp\/v2\/posts\/316167\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/buradabiliyorum.com\/en\/wp-json\/wp\/v2\/media\/316168"}],"wp:attachment":[{"href":"https:\/\/buradabiliyorum.com\/en\/wp-json\/wp\/v2\/media?parent=316167"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/buradabiliyorum.com\/en\/wp-json\/wp\/v2\/categories?post=316167"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/buradabiliyorum.com\/en\/wp-json\/wp\/v2\/tags?post=316167"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}