An artist’s impression of a supermassive black hole surrounded by a disc of hot, X-ray emitting debris from a star that wandered too close and was torn apart by the hole’s enormous gravity – a tidal disruption event. Brightness variations in the disc allowed astronomers to measure the spin of a supermassive black hole in a galaxy 290 million light years away. Image: NASA/CXC/M.Weiss)
Astronomers recently caught the sudden flare of a star being ripped apart by the supermassive black hole at the core of a galaxy 290 million light years away, a phenomenon known as a tidal disruption event. The outburst was first detected at optical wavelengths by the All-Sky Automated Survey for Supernovae, or ASASSN, in 2014.
Analysis of X-rays from the flare, using NASA’s Chandra X-ray Observatory, the Neil Gehrels Swift observatory and the European Space Agency’s XMM-Newton, showed repetitive brightness variations that could be clocked as debris whipped around the black hole just outside its event horizon, the point of no return for material being pulled into the singularity.
Researchers concluded the event horizon is about 300 times the diameter of Earth and rotating once every two minutes. That means the black hole is spinning at ...