{"id":519496,"date":"2026-06-05T04:45:11","date_gmt":"2026-06-05T04:45:11","guid":{"rendered":"https:\/\/www.europesays.com\/ie\/519496\/"},"modified":"2026-06-05T04:45:11","modified_gmt":"2026-06-05T04:45:11","slug":"a-cannibal-star-finally-solves-one-of-astronomys-biggest-mysteries","status":"publish","type":"post","link":"https:\/\/www.europesays.com\/ie\/519496\/","title":{"rendered":"A Cannibal Star Finally Solves One of Astronomy\u2019s Biggest Mysteries"},"content":{"rendered":"<p><a href=\"https:\/\/scitechdaily.com\/images\/Cannibal-Star-White-Dwarf-Red-Binary.jpg\" rel=\"nofollow noopener\" target=\"_blank\"><img fetchpriority=\"high\" decoding=\"async\" class=\"wp-image-521667 size-large\" src=\"https:\/\/www.europesays.com\/ie\/wp-content\/uploads\/2026\/06\/Cannibal-Star-White-Dwarf-Red-Binary-777x518.jpg\" alt=\"Cannibal Star White Dwarf Red Binary\" width=\"777\" height=\"518\"  \/><\/a>Scientists have linked a mysterious class of repeating cosmic signals to a white dwarf star stealing material from a neighboring star. The breakthrough not only solves a long-standing astronomical puzzle but also provides a powerful new tool for understanding similar signals across the galaxy. (Artist\u2019s concept.) Credit: SciTechDaily.com<\/p>\n<p><strong>A star caught feeding on its companion has finally revealed the source of some of the galaxy\u2019s most mysterious repeating signals.<\/strong><\/p>\n<p>An international research team led by scientists at the University of Sydney has uncovered the strongest evidence yet explaining the origin of a puzzling type of cosmic signal. Their work has also revealed a rare stellar system that offers a unique opportunity to study some of the most extreme conditions in the universe.<\/p>\n<p>Using CSIRO\u2019s ASKAP radio telescope, the researchers found a compact white dwarf star pulling material away from a larger companion star. As the stolen matter spirals toward the white dwarf, the system produces powerful bursts of radio waves and X-rays on a repeating cycle every 1.4 hours.<\/p>\n<p>The findings were published in Nature Astronomy.<\/p>\n<p><a href=\"https:\/\/scitechdaily.com\/images\/Accreting-White-Dwarf-Binary-Illustration.jpg\" rel=\"nofollow noopener\" target=\"_blank\"><img loading=\"lazy\" decoding=\"async\" class=\"size-large wp-image-521760\" src=\"https:\/\/www.europesays.com\/ie\/wp-content\/uploads\/2026\/06\/Accreting-White-Dwarf-Binary-Illustration-777x839.jpg\" alt=\"Accreting White Dwarf Binary Illustration\" width=\"777\" height=\"839\"  \/><\/a>Accreting white dwarf illustration. Credit: Carl Knox (OzGrav, Swinburne University of Technology) and Joshua Preston Pritchard (CSIRO)<\/p>\n<p>Lead author Kovi Rose, a PhD student in the University of Sydney\u2019s School of Physics and CSIRO, said the discovery provides the first confirmed explanation for a mysterious class of objects known as long-period radio transients. These unusual signals have been detected in only a handful of locations across the Milky Way.<\/p>\n<p>\u201cFor the first time we have pinpointed the origin of these signals, confirming the source to be a \u2018cataclysmic variable\u2019, or an accreting white dwarf star,\u201d said Mr. Rose.<\/p>\n<p>\u201cLong-period radio transients have puzzled astronomers for years,\u201d Mr. Rose said. \u201cWe\u2019ve only found about a dozen, and their origins have been unclear. Now, we\u2019ve been able to show that the source for one of these transients comes from a white dwarf actively pulling material from a companion star.\u201d<\/p>\n<p><a href=\"https:\/\/scitechdaily.com\/images\/CSIRO-ASKAP-Radio-Telescope-on-Wajarri-Yamaji-Country.jpg\" rel=\"nofollow noopener\" target=\"_blank\"><img loading=\"lazy\" decoding=\"async\" class=\"size-large wp-image-521757\" src=\"https:\/\/www.europesays.com\/ie\/wp-content\/uploads\/2026\/06\/CSIRO-ASKAP-Radio-Telescope-on-Wajarri-Yamaji-Country-777x518.jpg\" alt=\"CSIRO ASKAP Radio Telescope on Wajarri Yamaji Country\" width=\"777\" height=\"518\"  \/><\/a>CSIRO \u2019s ASKAP radio telescope on Wajarri Yamaji Country. Credit: Alex Cherney.Rare Binary Star System Revealed<\/p>\n<p>The newly identified object, known as ASKAP J1745\u22125051, consists of a white dwarf and a red dwarf star locked in an extremely tight orbit. Although the white dwarf is roughly Earth-sized, it contains nearly as much mass as the Sun. Its companion is much larger in size but has only about one-tenth of the Sun\u2019s mass.<\/p>\n<p>The two stars circle each other in just over an hour.<\/p>\n<p>As gas from the red dwarf flows toward the white dwarf, it becomes intensely heated and emits X-rays. At the same time, interactions involving the stars\u2019 magnetic fields generate regular radio bursts, creating the repeating signal observed by astronomers.<\/p>\n<p>\u201cThese emissions are all tied to the orbital motion of the system,\u201d Mr. Rose said. \u201cBut interestingly, the radio and X-ray signals don\u2019t peak at the same time, which tells us they\u2019re being produced in different regions of the system.\u201d<\/p>\n<p>The researchers believe the radio bursts originate where the magnetic fields of the two stars interact with the stream of charged material being stripped from the companion star. Those interactions create tightly focused beams of radio emission.<\/p>\n<p><a href=\"https:\/\/scitechdaily.com\/images\/Kovi-Rose-1-scaled.jpg\" rel=\"nofollow noopener\" target=\"_blank\"><img loading=\"lazy\" decoding=\"async\" class=\"size-large wp-image-521759\" src=\"https:\/\/www.europesays.com\/ie\/wp-content\/uploads\/2026\/06\/Kovi-Rose-1-777x486.jpg\" alt=\"Kovi Rose\" width=\"777\" height=\"486\"  \/><\/a>Lead author Kovi Rose from the University of Sydney in front of an illustration of the white dwarf binary. Credit: Carl KnoxSolving the Long-Period Radio Transient Mystery<\/p>\n<p>When long-period radio transients were first discovered, some astronomers suspected they might be slowly rotating neutron stars called pulsars. However, current theories indicate neutron stars spinning this slowly should not be capable of generating these signals.<\/p>\n<p>The new findings support a different explanation. At least some long-period radio transients appear to come from binary star systems involving white dwarfs.<\/p>\n<p>\u201cSome similar objects had been linked to binary systems before, but this is the first one where we can clearly see both stars and the accretion process in action,\u201d said Professor Murphy, Head of School at the University of Sydney School of Physics and Chief Investigator at the ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav).<\/p>\n<p>The system is also only the second known long-period radio transient that produces regular X-rays. It is the first example in which scientists have confirmed exactly what causes the repeating pattern.<\/p>\n<p><a href=\"https:\/\/scitechdaily.com\/images\/Milky-Way-Above-CSIRO-ASKAP-Radio-Telescope-scaled.jpg\" rel=\"nofollow noopener\" target=\"_blank\"><img loading=\"lazy\" decoding=\"async\" class=\"size-large wp-image-521758\" src=\"https:\/\/www.europesays.com\/ie\/wp-content\/uploads\/2026\/06\/Milky-Way-Above-CSIRO-ASKAP-Radio-Telescope-777x518.jpg\" alt=\"Milky Way Above CSIRO ASKAP Radio Telescope\" width=\"777\" height=\"518\"  \/><\/a>The ASKAP radio telescope at Inyarrimanha Ilgari Bundara, the CSIRO Murchison Radio-astronomy Observatory on Wajarri Yamaji Country in Western Australia. Credit: Alex Cherney\/CSIROA Cosmic \u201cRosetta Stone\u201d for Future Discoveries<\/p>\n<p>ASKAP J1745\u22125051 was detected with the ASKAP radio telescope, which is owned and operated by CSIRO, Australia\u2019s national science agency. ASKAP\u2019s combination of sensitivity, resolution, and wide sky coverage allows astronomers to detect unusual signals that might otherwise go unnoticed.<\/p>\n<p>Researchers believe the newly discovered system could become an important reference point for understanding other long-period radio transients.<\/p>\n<p>\u201cThis system gives us a way to decode these signals. It could help us determine whether other long-period transients are more like pulsars or like white dwarf systems, acting like a stellar Rosetta stone,\u201d said Mr. Rose, referring to the archaeological object discovered in Egypt that helped translate ancient hieroglyphics.<\/p>\n<p>The discovery also opens a window into physical processes that cannot be recreated in laboratories on Earth. Scientists can use the system to study how matter behaves in powerful magnetic fields and under intense gravitational forces.<\/p>\n<p>\u201cThese systems are natural laboratories,\u201d Mr. Rose said. \u201cThey allow us to test our understanding of how matter behaves in strong magnetic fields and under intense gravitational forces.\u201d<\/p>\n<p>Future Observations Planned<\/p>\n<p>The team intends to continue studying the system with a combination of radio, optical, and X-ray telescopes. Future observations will help researchers better understand how the emissions are produced and whether similar processes can explain the broader population of long-period radio transients.<\/p>\n<p>\u201cEach new discovery is helping us piece together the bigger picture,\u201d Mr. Rose said. \u201cWe\u2019re only just beginning to understand this new class of cosmic events.\u201d<\/p>\n<p>Reference: \u201cPeriodic radio and X-ray emission from an accreting white dwarf binary\u201d by Kovi Rose, Joshua Pritchard, Tara Murphy, L. N. Driessen, D. L. Kaplan, M. Caleb, Ziteng Wang, A. Zic, I. Andreoni, J. Carney, B. N. Barlow, D. Dobie, M. Gu, G. Heald, D. Huber, E. Lenc, J. K. Leung, W. Lu, R. Momose, M. G. Pedersen, Y. Qu, N. Rea, I. de Ruiter, K. Shaji, G. R. Sivakoff, A. J. M. Thomson, Y. L. Wang, G. J. Yang and F. Zahedy, 1 June 2026, Nature Astronomy.<br \/><a href=\"https:\/\/www.nature.com\/articles\/s41550-026-02882-x\" rel=\"nofollow noopener\" target=\"_blank\">DOI: 10.1038\/s41550-026-02882-x<\/a><\/p>\n<p>The international collaboration included researchers from Australia, the United States, Canada, China, Spain, and Israel. Observations were carried out using CSIRO\u2019s ASKAP and Australia Telescope Compact Array in Australia, the MeerKAT radio telescope in South Africa, the SOAR and Magellan optical telescopes in Chile, and the Swift (UV\/X-ray) and Einstein Probe (X-ray) space telescopes.<\/p>\n<p>The authors reported no competing interests. Funding for the research was provided by the Australian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav), NASA, the Alfred P. Sloan Foundation, the Professor Harry Messel Research Fellowship in Physics Endowment, the European Research Council, and the China Scholarship Council.<\/p>\n<p><b>Never miss a breakthrough: <a href=\"https:\/\/scitechdaily.com\/newsletter\/\" rel=\"nofollow noopener\" target=\"_blank\">Join the SciTechDaily newsletter.<\/a><\/b><br \/><b>Follow us on <a href=\"https:\/\/www.google.com\/preferences\/source?q=scitechdaily.com\" rel=\"nofollow noopener\" target=\"_blank\">Google<\/a> and <a href=\"https:\/\/news.google.com\/publications\/CAAqLAgKIiZDQklTRmdnTWFoSUtFSE5qYVhSbFkyaGtZV2xzZVM1amIyMG9BQVAB?hl=en-US&amp;gl=US&amp;ceid=US%3Aen\" rel=\"nofollow noopener\" target=\"_blank\">Google News<\/a>.<\/b><\/p>\n","protected":false},"excerpt":{"rendered":"Scientists have linked a mysterious class of repeating cosmic signals to a white dwarf star stealing material from&hellip;\n","protected":false},"author":2,"featured_media":519497,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":"","_share_on_mastodon":"0"},"categories":[270],"tags":[582,1025,62335,18,19,17,133,451,18376],"class_list":["post-519496","post","type-post","status-publish","format-standard","has-post-thumbnail","category-space","tag-astronomy","tag-astrophysics","tag-csiro","tag-eire","tag-ie","tag-ireland","tag-science","tag-space","tag-university-of-sydney"],"share_on_mastodon":{"url":"https:\/\/pubeurope.com\/@ie\/116695684867392366","error":""},"_links":{"self":[{"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/posts\/519496","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/comments?post=519496"}],"version-history":[{"count":0,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/posts\/519496\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/media\/519497"}],"wp:attachment":[{"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/media?parent=519496"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/categories?post=519496"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/tags?post=519496"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}