\n<\/p>\n
<\/iframe><br \/><em>An animation of the interaction between the Cygnus X-1 black hole and its large companion star. The force of stellar winds from the star bends the jets from Cygnus X-1. Video via the International Center for Radio Astronomy Research (ICRAR)<\/em>.<\/p>\n<ul>\n<li><strong>The black hole Cygnus X-1 has strong jets<\/strong>. And the stellar winds from its companion star bend the jets, which causes them to \u201cdance\u201d in different directions.<\/li>\n<li><strong>The jets travel at half the speed of light<\/strong> and produce 10,000 times the energy output of our sun.<\/li>\n<li><strong>These jets help scientists understand galaxy evolution,<\/strong> because the physics of stellar black holes mirrors that of supermassive black holes at galactic centers.<\/li>\n<\/ul>\n<h3>Cygnus X-1 black hole jets are perturbed by stellar winds<\/h3>\n<p>Cygnus X-1 has a special place in the history of astronomy. In 1971, astronomers confirmed it as the first known black hole. Now, on April 16, 2026, astronomers from the International Centre for Radio Astronomy Research (ICRAR) in Australia said that winds from a large companion star buffet the jets emitted by Cygnus X-1. These observations enabled them to calculate the jets\u2019 power output. It was an astounding 10,000 times that of our sun. Plus, the jets were traveling at half the speed of light! These findings are significant because even though Cygnus X-1 is a stellar black hole, studying its jets ultimately helps astronomers understand the evolution of galaxies.<\/p>\n<p>The black hole Cygnus X-1, about 7,200 light-years away and 21 times the mass of our sun, has a companion. It\u2019s a large blue supergiant star, called HDE 226868, about 40 solar masses. The two objects orbit about their center of gravity every 5.6 days. <\/p>\n<p>Lead author Steve Prabu at Oxford University described the jets as <em>dancing jets<\/em>. That\u2019s because they\u2019re deflected in different directions by stellar winds as the black hole and companion star move in their orbit. <\/p>\n<p>The researchers published their findings in the peer-reviewed journal <em>Nature Astronomy<\/em> on April 16, 2026.<\/p>\n<figure id=\"attachment_543670\" aria-describedby=\"caption-attachment-543670\" style=\"width: 650px\" class=\"wp-caption alignnone\"><figcaption id=\"caption-attachment-543670\" class=\"wp-caption-text\">This map from the Stellarium app shows the location of Cygnus X-1 (the white circle) in the constellation Cygnus the Swan. Image via Stellarium.<\/figcaption><\/figure>\n<h3>Black hole jets<\/h3>\n<p>Some black holes eject jets of plasma \u2013 ionized gases and electrons \u2013 along their rotation axis at very high speeds. In fact, such jets appear in systems where the black hole pulls matter from a nearby companion star. Consequently, the spinning black hole ejects some of that matter as jets. <\/p>\n<p>Astronomers are interested in knowing the <em>instantaneous<\/em> power released by black hole jets for several reasons. That\u2019s because it shows them how the black hole itself grows. Previous methods could only measure the average jet power over thousands or even millions of years. In addition, the energy of these jets drives large-scale shocks across the interstellar medium, as well as distributes gases, cosmic rays and magnetic fields into its neighborhood. They also create large cavities in gas clouds. <\/p>\n<p>The physics of supermassive black holes with jets, which reside in the hearts of some galaxies, are the same as stellar black holes with jets. However, supermassive black holes affect their environment on a much bigger intergalactic scale. Therefore, jets in stellar black holes can, in fact, contribute to our understanding of galaxy evolution. <\/p>\n<figure id=\"attachment_543547\" aria-describedby=\"caption-attachment-543547\" style=\"width: 800px\" class=\"wp-caption aligncenter\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/earthsky.org\/upl\/2026\/04\/International-Centre-for-Radio-Astronomy-Research.jpg\" alt=\"Large blue star with stream of material to a red disk. Bent jets coming from top and bottom of the disk.\" width=\"800\" height=\"450\" class=\"size-full wp-image-543547\" srcset=\"https:\/\/earthsky.org\/upl\/2026\/04\/International-Centre-for-Radio-Astronomy-Research.jpg 800w, https:\/\/earthsky.org\/upl\/2026\/04\/International-Centre-for-Radio-Astronomy-Research-300x169.jpg 300w, https:\/\/earthsky.org\/upl\/2026\/04\/International-Centre-for-Radio-Astronomy-Research-768x432.jpg 768w\" sizes=\"auto, (max-width: 800px) 100vw, 800px\"\/><figcaption id=\"caption-attachment-543547\" class=\"wp-caption-text\">Artist\u2019s illustration of material from a blue supergiant star being pulled into an accretion disk around the black hole. Stellar winds blowing from the star cause the arching shape in the jets. Image via ICRAR\/ Curtin University.<\/figcaption><\/figure>\n<h3>Determining the power in Cygnus X-1 jets<\/h3>\n<p>In the past, astronomers did not quite grasp how the energy from black hole jets affected their surrounding environment. That\u2019s because they could not determine the instantaneous power of those jets. Until now. <\/p>\n<p>The team studied x-rays emitted by the Cygnus X-1 jets using high-resolution radio images they collected over 18 years. They used radio telescopes spaced over vast distances across the world, using an observation technique called very long baseline interferometry. As the black hole and its companion star moved in their orbit, the astronomers were able to see patterns of motion in the black hole jets, thanks to the stellar winds from the companion star deflecting the jets. In addition, they also knew the power of the stellar winds streaming out of the star. <\/p>\n<p>So the astronomers entered the observed sequences of jet deflections and the known stellar wind power into mathematical models. As a result, they were able to calculate the instantaneous power released by the jets. They discovered that these jets emitted the power output of 10,000 suns. In addition, they traveled blazingly fast at half the speed of light (93,000 miles per second or 150,000 km per second). <\/p>\n<figure id=\"attachment_543549\" aria-describedby=\"caption-attachment-543549\" style=\"width: 650px\" class=\"wp-caption aligncenter\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/earthsky.org\/upl\/2026\/04\/Radio_Telescope_at_Mauna_Kea-ZimZalaBim-Wikimedia-Commons.jpg\" alt=\"A large dish-shaped antenna on a barren brown mountaintop under a deep blue sky. A fence in the foreground.\" width=\"650\" height=\"867\" class=\"size-full wp-image-543549\" srcset=\"https:\/\/earthsky.org\/upl\/2026\/04\/Radio_Telescope_at_Mauna_Kea-ZimZalaBim-Wikimedia-Commons.jpg 650w, https:\/\/earthsky.org\/upl\/2026\/04\/Radio_Telescope_at_Mauna_Kea-ZimZalaBim-Wikimedia-Commons-225x300.jpg 225w\" sizes=\"auto, (max-width: 650px) 100vw, 650px\"\/><figcaption id=\"caption-attachment-543549\" class=\"wp-caption-text\">Radio telescope at Mauna Kea, Hawaii. It is part of the Very Long Baseline Array, which includes 10 radio telescopes at different locations across North America and in Hawaii. Astronomers used this network of telescopes, as well as the European VLBI Network, to obtain radio images of Cygnus X-1. Image via ZimZalaBim\/ Wikimedia Commons (CC BY-SA 4.0).<\/figcaption><\/figure>\n<h3>How Cygnus X-1 helps us understand how galaxies evolve<\/h3>\n<p>Prabu said:<\/p>\n<blockquote>\n<p>A key finding from this research is that about 10% of the energy released as matter falls in towards the black hole is carried away by the jets.<\/p>\n<p>This is what scientists usually assume in large-scale simulated models of the universe, but it has been hard to confirm by observation until now.<\/p>\n<\/blockquote>\n<p>James Miller-Jones of Curtin University is a paper co-author. He added: <\/p>\n<blockquote>\n<p>And because our theories suggest that the physics around black holes are very similar, we can now use this measurement to anchor our understanding of jets, whether they are from black holes 10 or 10 million times the mass of the sun.<\/p>\n<p>With radio telescope projects such as the Square Kilometer Array Observatory currently under construction in Western Australia and South Africa, we expect to detect jets from black holes in millions of distant galaxies, and the anchor point provided by this new measurement will help calibrate their overall power output.<\/p>\n<p>Black hole jets provide an important source of feedback to the surrounding environment and are critical to understanding the evolution of galaxies.<\/p>\n<\/blockquote>\n<p><strong>You deserve a daily dose of good news.<\/strong> For the latest in science and the night sky, subscribe to EarthSky\u2019s free daily newsletter.<\/p>\n<p>Bottom line: The Cygnus X-1 black hole emits strong jets. The stellar winds from a companion star bend these jets, and this has enabled astronomers to calculate the jets\u2019 power.<\/p>\n<p>Source: A jet bent by a stellar wind in the black hole X-ray binary Cygnus X-1<\/p>\n<p>Via International Centre for Radio Astronomy Research (ICRAR)<\/p>\n<p>Read more: How the world came to understand black holes<\/p>\n<p>Read more: Black hole belches radiation long after eating a star<\/p>\n<p><span class=\"cp-load-after-post\"\/><\/div>\n<div>\n<div class=\"post-author\">\n<h4>Shireen Gonzaga<\/h4>\n<p> View Articles\n <\/p><\/div>\n<div class=\"post-tags\">\n<h6 data-udy-fe=\"text_7c58270d\">About the Author:<\/h6>\n<p>Shireen Gonzaga is a freelance writer who enjoys writing about natural history. She is also a technical editor at an astronomical observatory where she works on documentation for astronomers.<\/p>\n<\/p><\/div>\n<\/p><\/div>\n<p><br \/>\n<br \/><a href=\"https:\/\/earthsky.org\/space\/black-hole-cygnus-x-1-dancing-jets\/?rand=772280\">Source link <\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>An animation of the interaction between the Cygnus X-1 black hole and its large companion star. The force of stellar winds from the star bends the jets from Cygnus X-1.… <\/p>\n","protected":false},"author":1,"featured_media":801846,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[46],"tags":[],"class_list":["post-801845","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-earth-sky"],"_links":{"self":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/801845","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\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=801845"}],"version-history":[{"count":0,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/801845\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/media\/801846"}],"wp:attachment":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=801845"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=801845"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=801845"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}