Smallest supermassive black hole that can provide clues to growth detected
This oxymoronic object could provide clues to how larger black holes formed along with their host galaxies 13 billion years or more in the past, NASA said Tuesday.
Astronomers estimate this supermassive black hole is about 50,000 times the mass of the sun. This is less than half the mass of the previous smallest black hole at the center of a galaxy.
"It might sound contradictory, but finding such a small, large black hole is very important," said Vivienne Baldassare of the University of Michigan in Ann Arbor, first author of a paper on these results published in The Astrophysical Journal Letters.
"We can use observations of the lightest supermassive black holes to better understand how black holes of different sizes grow."
The tiny heavyweight black hole is in the center of a dwarf disk galaxy, called RGG 118, located about 340 million light years from Earth, and was originally discovered using the Sloan Digital Sky Survey.
Researchers estimated the mass of the black hole by studying the motion of cool gas near the center of the galaxy using visible light data from the Clay Telescope. They used the Chandra data to figure out the X-ray brightness of hot gas swirling toward the black hole.
They found the outward push of radiation pressure of this hot gas is about 1 percent of the black hole's inward pull of gravity, matching the properties of other supermassive black holes.
The black hole in RGG 118 is nearly 100 times less massive than the supermassive black hole found in the center of the Milky Way. It's also about 200,000 times less massive than the heaviest black holes found in the centers of other galaxies.
Researchers will continue to look for other supermassive black holes that are comparable in size or even smaller than the one in RGG 118 to help decide which of the models is more accurate and refine their understanding of how these objects grow.
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