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This computer-simulated image shows gas from a tidally shredded star falling into a black hole. Some of the gas also is being ejected at high speeds into space.
Credit: NASA, S. Gezari (JHU), and J. Guillochon (UC Santa Cruz)
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Astral feast
Astronomers get a glimpse of black hole feeding
Supermassive black holes lurk in the centers of galaxies, hungrily vacuuming up everything within reach — or so we think. But the truth is less dramatic. Supermassive black holes snack infrequently, making the recent discovery of a black hole in the act of feeding all the more interesting to astronomers.
“Black holes, like sharks, suffer from a popular misconception that they are perpetual killing machines,” said Ryan Chornock of the Harvard-Smithsonian Center for Astrophysics (CfA). “Actually, they’re quiet for most of their lives. Occasionally a star wanders too close, and that’s when a feeding frenzy begins.”
Chornock and his colleagues, including team leader Suvi Gezari of Johns Hopkins University, reported their discovery of a feeding supermassive black hole in the May 3 issue of the journal Nature.
If a star passes too close to a black hole, tidal forces can rip it apart. Its constituent gases then swirl in toward the black hole. Friction heats the gases and causes them to glow. By searching for newly glowing supermassive black holes, astronomers can get a glimpse of a feast.
The team discovered just such a glow in May 2010 using the Pan-STARRS1 telescope on Mount Haleakala in Hawaii. The flare brightened to a peak on July 12 before fading away over the course of a year.
“We observed the demise of a star and its digestion by the black hole in real time,” said coauthor Edo Berger, John L. Loeb Associate Professor of the Natural Sciences and associate professor of astronomy.
The glow came from a previously dormant supermassive black hole at the center of a galaxy 2.7 billion light-years away. The black hole contains as much mass as 3 million suns, making it about the same size as the Milky Way’s central black hole.
Follow-up observations with the MMT Observatory in Arizona showed that the black hole was consuming large amounts of helium. Therefore, the shredded star likely was the core of a red giant star. The lack of hydrogen showed that the star lost its outer atmosphere on a previous pass by the black hole.
“This star barely survived one encounter with the black hole, only to meet its unfortunate end in round two,” said Chornock.
The discovery demonstrates the sleuthing power of the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS), which was designed to locate all kinds of transient phenomena in the night sky.
