This artist’s illustration shows the region around a supermassive black hole after a star wandered too close and was ripped apart. Some of the remains of the star are pulled into an X-ray-bright disk where they circle the black hole before passing over the “event horizon,” the boundary beyond which nothing, including light, can escape. The elongated spot depicts a bright region in the disk, which causes a regular variation in the X-ray brightness of the source, allowing the spin rate of the black hole to be estimated.
(Illustration: NASA/CXC/M.Weiss; X-ray: NASA/CXC/MIT/D. Pasham et al: Optical: HST/STScI/I. Arcavi)
The crumbs left over from a supermassive black hole’s recent meal have allowed scientists to calculate the monster’s rotation rate, and the results are mind-boggling.
The huge black hole, known as ASASSN-14li, is spinning at least 50 percent the speed of light, research team members said.
“This black hole’s event horizon is about 300 times bigger than the Earth,” study co-author Ron Remillard, of the Massachusetts Institute of Technology (MIT), said in a statement. (The event horizon is the limit beyond which nothing, not even light, can escape a black hole’s gravitational clutches.) [Images: Black Holes of the Universe]
“Yet the black hole is spinning so fast it completes one rotation in about two minutes, compared to the 24 hours it takes our planet to rotate,” Remillard added.
ASASSN-14li lies at the heart of a galaxy 290 million miles away from Earth and harbors between 1 million and 10 million times the mass of the sun. So, it’s about as hefty as the black hole at the Milky Way’s core, known as Sagittarius A*, which contains about 4 million solar masses. (Supermassive black holes can get much weightier; some tip the scales at tens of billions of solar masses.)
ASASSN-14li was discovered in November 2014, after it tore apart a star that strayed too close. This dramatic event caused a flash of bright light, which was spotted by a system of optical telescopes called the All-Sky Automated Survey for Supernovae (hence the black hole’s name).
In the new study, a team led by Dheeraj Pasham, also of MIT, observed the X-ray light coming from the ASASSN-14li system. The researchers analyzed data gathered by a number of instruments, including NASA’s Chandra X-ray Observatory and Neil Gehrels Swift space telescopes, as well as the European Space Agency’s XMM-Newton spacecraft.
These datasets revealed a consistent flickering: ASASSN-14li’s X-ray emissions rise and fall every 131 seconds. This clockwork signal is likely caused by a clump of the torn-apart star circling the black hole very close to the event horizon, study team members said.
“The fact that we can track this region of bright X-ray emission as it circles the black hole lets us track just how quickly material in the disk is spinning,” Pasham said in the same statement. “That gives us information about the spin rate of the supermassive black hole itself.”
That spin speed is impressive but not unprecedented. The few supermassive black holes whose rotation rates have been clocked to date are in the same extreme neighborhood, generally whipping around between 33 percent and 84 percent the speed of light.
The new results — which Pasham presented Wednesday (Jan. 9) at the 233rd meeting of the American Astronomical Society (AAS) in Seattle — could help astronomers better understand how supermassive black holes evolve.
These behemoths can grow in two main ways, Pasham said — by galaxy-scale mergers, and/or by steadily accreting smaller bits of surrounding material. A relatively low rotation rate would implicate mergers as the primary factor, because these random smashups likely wouldn’t keep spinning the growing black hole up in the same direction.
However, “if you have a high-spin black hole, supermassive black hole, that’s telling us that maybe steady accretion was dominant,” Pasham said during a news conference at AAS Wednesday.
Originally published on Space.com.
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