Home » What Happens When A Hungry Black Hole Snacks On A Bypassing Star? Hubble Telescope Captures The Answer

What Happens When A Hungry Black Hole Snacks On A Bypassing Star? Hubble Telescope Captures The Answer

by Coffee Table Science
16 minutes read

A very rare and intense cosmic drama has been captured by NASA’s Hubble Telescope recently. Scientists are using the Hubble telescope to understand what happens when an unpredictable star falls into a black hole.

Black holes are infamous for their exceptional gravitational pull that even light fails to escape. They aren’t hunters but gatherers. They wait for a hapless star to make the mistake of traveling too closely, only to rip it apart violently, spewing out extreme radiation while sloppily ingesting it. In other words, they are messy eaters. 

What are Tidal Disruption Events?


Scientists have recorded a star’s final moments in detail as it gets devoured by a black hole, which they call ‘Tidal disruption events’. As extreme as this event sounds, it is quite a rare occurrence as it approximately happens only a few times in every 100,000 years in any given galaxy with a stable supermassive black hole at its core. Astronomers have detected about 100 tidal disruption events so far using various telescopes.


Image credits: Wikimedia commons

These events are usually difficult to observe. Maybe a few observations can be drawn at the beginning of the disruption when it’s really bright. Because of how close and bright this intense collision was, Hubble astronomers were able to conduct ultraviolet spectroscopy for a longer length of time than usual. Ultraviolet Spectroscopy is helpful as a lot of information can be drawn using this spectrum. However, very few tidal events are observed in UV light given the observing time.

Since this star, namely AT2022dsb, is nearly 300 million light-years away at the centre of the galaxy ESO 583-G004, the Hubble telescope cannot take its tidal event’s picture. Astronomers used Hubble’s powerful ultraviolet sensitivity to study the light from the destroyed star constituting hydrogen, carbon, and more. The spectroscopy provided clues to the stellar assassination committed by the black hole.

Star becomes a giant gaseous donut


The All-Sky Automated Survey for Supernovae (ASAS-SN or “Assassin”), a network of ground-based telescopes that surveys the extragalactic sky for violent, variable, and transient cosmic happenings, first caught this AT2022dsb stellar snacking event on 1 March 2022.


Image credits: NASA, ESA, Leah Hustak (STScI)


“We saw this early enough that we could observe it at these very intense black hole accretion stages. We saw the accretion rate drop as it turned to a trickle over time,” said Peter Maksym of the Center for Astrophysics (CfA) in Cambridge, Massachusetts, one of the astronomers behind Hubble observations.


According to the interpretation of the Hubble spectroscopic data, the former star is now a very bright, hot, doughnut-shaped (torus) region of gas which is as big as the solar system. It is swirling around a black hole at its centre. “We’re looking somewhere on the edge of that donut. We’re seeing a stellar wind from the black hole sweeping over the surface that’s being projected towards us at speeds of 20 million miles per hour (three percent the speed of light),” said Maksym.

Researchers are excited to get the details about what the star debris is doing. This is an exciting place for scientists to be, right at the interface of the known and the unknown as tidal events can reveal a lot about Black holes.


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