Name: Mistaken identity: A presumed supernova is actually something much rarer
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Mistaken identity: A presumed supernova is actually something much rarer

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January 13, 2021byIn a case of comic mistaken identity, an international team of astronomers revealed that what they once thought was a supernova is actually periodic flaring from a galaxy where a supermassive black hole gives off bursts of energy every 114 days as it tears off chunks of an orbiting star.Six years after its initial discovery—reported in The Astronomer's Telegram by Carnegie's Thomas Holoien—the researchers, led by Anna Payne of University of Hawai'i at Mānoa, can now say that the phenomenon they observed, called ASASSN-14ko, is a periodically recurring from the center of a galaxy more than 570 million light-years away in the southern constellation Pictor.Their findings—based on 20 instances of regular outbursts—will be published in the Astrophysical Journal and presented by Payne at the American Astronomical Society's annual meeting.Active galaxies, such as the host of ASASSN-14ko, have unusually bright and variable centers. These objects produce much more energy than the combined contribution of all their stars. Astrophysicists think this is due to gravitational and frictional forces heating up a swirling disk of gas and dust that accumulates around the central supermassive black hole. The black hole slowly consumes the material, which creates low-level, random changes in the light emitted by the disk.This is the first unambiguous example of such clockwork behavior from an active galaxy. Periodically recurring flares, such as those from ASASSN-14ko, could be evidence of observationally elusive cosmic phenomena that have been previously predicted by theorists."Knowing the schedule of this extragalactic Old Faithful allows us to coordinate and study it in more detail," Payne said.ASASSN-14ko was first detected by the All-Sky Automated Survey for Supernovae (ASAS-SN), a global network of 20 robotic telescopes headquartered at The Ohio State University (OSU) in Columbus. When Payne examined all the ASAS-SN data on the phenomenon, she noticed a series of 17 regularly spaced flares.Based on this discovery, the astronomers predicted that the galaxy would experience another burst on May 17 of last year and coordinated ground- and space-based facilities to make observations. They have since successfully predicted and witnessed flares on September 7 and December 26."ASAS-SN is designed to probe the physics of our universe by looking for transient and variable events." Holoien said. "It's exciting that the luminous object we originally thought was a violent supernova explosion—which would be interesting in its own right, but more commonplace—turned out to be a long-sought-after cosmic event."So, what causes the repeated flares? The team considered several possible explanations, but think the most likely is what's called a partial tidal disruption event.Tidal disruption events, or TDEs, occur when a star gets too close to a , which tears it to shreds. Some of its material gets flung out into space and the rest falls back onto the black hole, forming a disk of hot, bright gas as it is consumed.In this instance, instead of a star being obliterated by interaction with the black hole, it would be slowly stripped during each orbit. The flares occur when the lost material—equal to three times the mass of Jupiter at each pass—falls in towards the black hole.The astronomers are unsure how long the flares will persist. The star can't lose mass forever, and while scientists can estimate the amount of mass it loses during each orbit, they don't know how much it had originally."We plan to keep predicting and observing these bursts or as long as we can," said second author Benjamin Shappee, also of UH Mānoa (and a Carnegie alumnus). "This rare find could reveal new details about black hole physics."Explore furtherMore information:ASASSN-14ko is a Periodic Nuclear Transient in ESO 253−G003. arXiv:2009.03321 [astro-ph.HE]Journal information:Provided byCitation:Mistaken identity: A presumed supernova is actually something much rarer (2021, January 13)retrieved 13 January 2021from https://phys.org/news/2021-01-mistaken-identity-presumed-supernova-rarer.htmlThis document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, nopart may be reproduced without the written permission. The content is provided for information purposes only.2 hours ago2 hours ago2 hours ago2 hours agoJan 12, 20215 hours ago7 hours ago10 hours agoJan 12, 2021Jan 11, 2021Jan 11, 2021More fromWhat do you think about this particular story?Your feedback will go directly to Science X editors.E-mail the storyMistaken identity: A presumed supernova is actually something much rarerThis site uses cookies to assist with navigation, analyse your use of our services, and provide content from third parties.By using our site, you acknowledge that you have read and understand ourand .

January 13, 2021byIn a case of comic mistaken identity, an international team of astronomers revealed that what they once thought was a supernova is actually periodic flaring from a galaxy where a supermassive black hole gives off bursts of energy every 114 days as it tears off chunks of an orbiting star.Six years after its initial discovery—reported in The Astronomer's Telegram by Carnegie's Thomas Holoien—the researchers, led by Anna Payne of University of Hawai'i at Mānoa, can now say that the phenomenon they observed, called ASASSN-14ko, is a periodically recurring from the center of a...

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Mistaken identity: A presumed supernova is actually something much rarer

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