Cosmic Mistaken Identity: “Supernova” Is Actually Something Much Rarer

Supermassive Black Hole Pulls a Stream of Gas off Star

In a case of cosmic mistaken identification, a world staff of astronomers revealed that what they as soon as thought was a supernova is definitely periodic flaring from a galaxy the place a supermassive black gap provides off bursts of power each 114 days because it tears off chunks of an orbiting star.

Six years after its preliminary discovery—reported in The Astronomer’s Telegram by Carnegie’s Thomas Holoien—the researchers, led by Anna Payne of College of Hawai’i at Mānoa, can now say that the phenomenon they noticed, referred to as ASASSN-14ko, is a periodically recurring flare from the middle of a galaxy greater than 570 million light-years away within the southern constellation Pictor.

Their findings—primarily based on 20 situations of normal outbursts—had been printed in The Astrophysical Journal and introduced by Payne on the American Astronomical Society’s annual assembly.

Monster Black Hole Siphons Gas off Orbiting Giant Star

A monster black gap siphons gasoline off of an orbiting big star on this illustration. Credit score: NASA’s Goddard Area Flight Middle/Chris Smith (USRA/GESTAR)

Energetic galaxies, such because the host of ASASSN-14ko, have unusually shiny and variable facilities. These objects produce way more power than the mixed contribution of all their stars. Astrophysicists assume this is because of gravitational and frictional forces heating up a swirling disk of gasoline and mud that accumulates across the central supermassive black gap. The black gap slowly consumes the fabric, which creates low-level, random modifications within the gentle emitted by the disk.

That is the primary unambiguous instance of such clockwork conduct from an energetic galaxy. Periodically recurring flares, reminiscent of these from ASASSN-14ko, might be proof of observationally elusive cosmic phenomena which have been beforehand predicted by theorists.

“Figuring out the schedule of this extragalactic Outdated Trustworthy permits us to coordinate and research it in additional element,” Payne mentioned.


Watch as a monster black gap partially consumes an orbiting big star. On this illustration, the gasoline pulled from the star collides with the black gap’s particles disk and causes a flare. Astronomers have named this repeating occasion ASASSN-14ko. The flares are probably the most predictable and frequent but seen from an energetic galaxy. Credit score: NASA’s Goddard Area Flight Middle

ASASSN-14ko was first detected by the All-Sky Automated Survey for Supernovae (ASAS-SN), a worldwide community of 20 robotic telescopes headquartered at The Ohio State College (OSU) in Columbus. When Payne examined all of the ASAS-SN information on the phenomenon, she observed a sequence of 17 commonly spaced flares.

Based mostly on this discovery, the astronomers predicted that the galaxy would expertise one other burst on Might 17 of final yr and coordinated ground- and space-based services to make observations. They've since efficiently predicted and witnessed flares on September 7 and December 26.

“ASAS-SN is designed to probe the physics of our universe by in search of transient and variable occasions.” Holoien mentioned. “It’s thrilling that the luminous object we initially thought was a violent supernova explosion—which might be attention-grabbing in its personal proper, however extra commonplace—turned out to be a long-sought-after cosmic occasion.”

For extra on this discovery, see NASA Investigates an “Outdated Trustworthy” Energetic Galaxy That Erupts Each 114 Days.

Reference: “ASASSN-14ko is a Periodic Nuclear Transient in ESO 253-G003” by Anna V. Payne, Benjamin J. Shappee, Jason T. Hinkle, Patrick J. Vallely, Christopher S. Kochanek, Thomas W.-S. Holoien, Katie Auchettl, Ok. Z. Stanek, Todd A. Thompson, Jack M. M. Neustadt, Michael A. Tucker, James D. Armstrong, Joseph Brimacombe, Paulo Cacella, Robert Cornect, Larry Denneau, Michael M. Fausnaugh, Heather Flewelling, Dirk Grupe, A.N. Heinze, Laura A. Lopez, Berto Monard, Jose L. Prieto, Adam C. Schneider, Scott S. Sheppard, John L. Tonry and Henry Weiland, 5 April 2021, The Astrophysical Journal.
DOI: 10.3847/1538-4357/abe38d

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