{"id":5048,"date":"2015-07-07T05:05:10","date_gmt":"2015-07-07T05:05:10","guid":{"rendered":"http:\/\/revoscience.com\/en\/?p=5048"},"modified":"2015-07-07T05:05:10","modified_gmt":"2015-07-07T05:05:10","slug":"astronomers-use-cosmic-gravity-to-create-a-black-hole-scope","status":"publish","type":"post","link":"https:\/\/www.revoscience.com\/en\/astronomers-use-cosmic-gravity-to-create-a-black-hole-scope\/","title":{"rendered":"Astronomers use cosmic gravity to create a black-hole-scope"},"content":{"rendered":"
\n
\"Gravitational<\/a>
Gravitational lensing<\/figcaption><\/figure>\n

The Integral, Fermi and Swift space observatories have used the magnifying power of a cosmic lens to explore the inner regions of a supermassive black hole.<\/span><\/p>\n

Gamma rays are highly energetic radiation emitted by some of the most extreme objects in our Universe. Jets of gamma rays moving at close to the speed of light stream from the areas around black holes, for example. These jets are thought to be emitted by superheated material spinning wildly as it is devoured by the hungry black hole.<\/span><\/p>\n

Our telescopes will never be powerful enough to reveal these inner regions, and scientists struggle to examine exactly how these jets are unleashed into the Universe.<\/span><\/p>\n

\u201cBecause we can\u2019t clearly see what\u2019s going on, we don\u2019t fully understand this behaviour,\u201d says Andrii Neronov of the University of Geneva, Switzerland, lead author on the\u00a0Nature Physics<\/i>\u00a0paper published online today.<\/span><\/p>\n

\u201cHowever, our method allowed us to \u2018resolve\u2019 this region, and get an insight into the patch of space directly surrounding a supermassive black hole known as PKS 1830-211.\u201d<\/span><\/p>\n

This black hole lies many billions of light-years away. Neither ESA\u2019s Integral satellite nor NASA\u2019s Fermi gamma-ray telescope can observe the region unaided, but a lucky coincidence provides a helping hand: gravitational microlensing.<\/span><\/p>\n<\/div>\n

\n
\"Simulated_microlensing_medium\"<\/a>
Simulated microlensing<\/figcaption><\/figure>\n

\u201cFrom Earth, black holes are tiny. They\u2019re just so very far away,\u201d notes Dr Neronov. \u201cTrying to observe PKS 1830-211 is like trying to look at an ant sitting on the Moon.<\/span><\/p>\n

\u201cNone of our telescopes can observe something so small, so we used a trick to resolve the ant: a huge gravitational lens.\u201d<\/span><\/p>\n

Massive cosmic objects, from single stars to galaxy clusters, bend and focus the light that flows around them with their gravity, acting like giant magnifying glasses.<\/span><\/p>\n

Dr Neronov and colleagues used a star sitting between their target and Earth to \u2018zoom in\u2019 to the black hole and measure the size of the jet-emitting region \u2013 the first time this method has ever been used with gamma rays.<\/span><\/p>\n

They picked out structures on the same angular scale as that of the Moon ant. The observed patch of sky covers a region about 100 times the Earth\u2013Sun distance. In astronomical terms, this is remarkably small.<\/span><\/p>\n

\u201cOur observations demonstrate that the gamma rays come from the direct vicinity of the black hole itself,\u201d says Dr Neronov. \u201cThis gives us some idea about what is and isn\u2019t important in generating the jets.<\/span><\/p>\n

\u201cIt\u2019s amazing to be able to see such tiny things at such enormous distances from us. I\u2019m very excited to have a \u2018black-hole-scope\u2019 to investigate the inner regions of the jets.\u201d<\/span><\/p>\n

\n

Observing the gamma-ray source with ESA\u2019s Integral and NASA\u2019s Fermi and Swift allowed the astronomers to build up a more complete picture of the radiation streaming out.<\/span><\/p>\n

The more energetic gamma rays, detected by Fermi, are seen to be coming from the tiny base of the jet \u2013 the \u2018ant on the Moon\u2019-size region \u2013 while the lower energy gamma rays, detected by Integral, were emitted from a much larger surrounding region.<\/span><\/p>\n

The team also studied X-rays using Integral and Swift. They found these X-rays to be emanating from a region stretching around the hole some 400 billion km or more.<\/span><\/p>\n

\u201cThis black hole is one of the most powerful known objects of its kind. Fully characterising its emission will hopefully give us real insight into how these jets form,\u201d says Erik Kuulkers, ESA\u2019s Integral project scientist.<\/span><\/p>\n

\u201cFortunately, the black hole lies in the field of space located towards the centre of our Galaxy, so Integral sees it often.<\/span><\/p>\n

\u201cThese observations provide unique information about the high-energy processes taking place around supermassive black holes, by allowing us to \u2018look inside\u2019 tiny structures lying very far away from us.\u201d<\/span><\/p>\n<\/div>\n

\n

\n<\/div>\n<\/div>\n","protected":false},"excerpt":{"rendered":"

The Integral, Fermi and Swift space observatories have used the magnifying power of a cosmic lens to explore the inner regions of a supermassive black hole. Gamma rays are highly energetic radiation emitted by some of the most extreme objects in our Universe. Jets of gamma rays moving at close to the speed of light […]<\/p>\n","protected":false},"author":6,"featured_media":5049,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[20],"tags":[],"class_list":["post-5048","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-space-news"],"featured_image_urls":{"full":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/07\/Gravitational_lensing_large.jpg",625,352,false],"thumbnail":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/07\/Gravitational_lensing_large-150x150.jpg",150,150,true],"medium":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/07\/Gravitational_lensing_large-300x168.jpg",300,168,true],"medium_large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/07\/Gravitational_lensing_large.jpg",625,352,false],"large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/07\/Gravitational_lensing_large.jpg",625,352,false],"1536x1536":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/07\/Gravitational_lensing_large.jpg",625,352,false],"2048x2048":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/07\/Gravitational_lensing_large.jpg",625,352,false],"ultp_layout_landscape_large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/07\/Gravitational_lensing_large.jpg",625,352,false],"ultp_layout_landscape":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/07\/Gravitational_lensing_large.jpg",625,352,false],"ultp_layout_portrait":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/07\/Gravitational_lensing_large.jpg",600,338,false],"ultp_layout_square":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/07\/Gravitational_lensing_large.jpg",600,338,false],"newspaper-x-single-post":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/07\/Gravitational_lensing_large.jpg",625,352,false],"newspaper-x-recent-post-big":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/07\/Gravitational_lensing_large.jpg",550,310,false],"newspaper-x-recent-post-list-image":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/07\/Gravitational_lensing_large.jpg",95,54,false],"web-stories-poster-portrait":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/07\/Gravitational_lensing_large.jpg",625,352,false],"web-stories-publisher-logo":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/07\/Gravitational_lensing_large.jpg",96,54,false],"web-stories-thumbnail":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/07\/Gravitational_lensing_large.jpg",150,84,false]},"author_info":{"info":["Amrita Tuladhar"]},"category_info":"Space\/ AstroPhysics<\/a>","tag_info":"Space\/ AstroPhysics","comment_count":"0","_links":{"self":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts\/5048","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/users\/6"}],"replies":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/comments?post=5048"}],"version-history":[{"count":0,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts\/5048\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/media\/5049"}],"wp:attachment":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/media?parent=5048"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/categories?post=5048"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/tags?post=5048"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}