This computer-simulated image shows gas
from a star that is ripped apart by tidal forces as it falls into a black hole.
Some of the gas also is being ejected at high speeds into space.
Using observations from telescopes in
space and on the ground, astronomers gathered the most direct evidence yet for
this violent process: a supermassive black hole shredding a star that wandered
too close. NASA's orbiting Galaxy Evolution Explorer (GALEX) and the
Pan-STARRS1 telescope on the summit of Haleakala in Hawaii were used to help to
identify the stellar remains.
A flare in ultraviolet and optical light
revealed gas falling into the black hole as well as helium-rich gas that was
expelled from the system. When the star is torn apart, some of the material
falls into the black hole, while the rest is ejected at high speeds. The flare
and its properties provide a signature of this scenario and give unprecedented
details about the stellar victim.
To completely rule out the possibility
of an active nucleus flaring up in the galaxy instead of a star being torn
apart, the team used NASA's Chandra X-ray Observatory to study the hot gas.
Chandra showed that the characteristics of the gas didn't match those from an
active galactic nucleus.
The galaxy where the supermassive black
hole ripped apart the passing star in known as PS1-10jh and is located about
2.7 billion light years from Earth. Astronomers estimate the black hole in
PS1-10jh has a mass of several million suns, which is comparable to the
supermassive black hole in our own Milky Way galaxy.
Image Credit: NASA, S. Gezari (The Johns
Hopkins University), and J. Guillochon (University of California, Santa Cruz)
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