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Excerpt from Chandra X-ray Center, Operated for NASA by
the Smithsonian Astrophysical Observatory:
RGG 118: Oxymoronic Black Hole Provides Clues to Growth
[Release Date August 11, 2015]
[Distance Estimate About 340 million light years]
. . . ]
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 is also about 200,000 times less massive than the heaviest black holes found in the centers of other galaxies.
Astronomers are trying to understand the formation of billion-solar-mass black holes that have been detected from less than a billion years after the Big Bang. The black hole in RGG 118 gives astronomers an opportunity to study a nearby small supermassive black hole in lieu of the first generation of black holes that are undetectable with current technology.
Astronomers think that supermassive black holes may form when a large cloud of gas, weighing about 10,000 to 100,000 times that of the Sun, collapses into a black hole. Many of these black hole seeds then merge to form much larger supermassive black holes. Alternately, a supermassive black hole seed could come from a giant star, about 100 times the Sun’s mass, that ultimately forms into a black hole after it runs out of fuel and collapses.
. . . ]
chandra.harvard.edu/photo/2015/rgg118/
Excerpt from Chandra X-ray Center, Operated for NASA by
the Smithsonian Astrophysical Observatory:
RGG 118: Oxymoronic Black Hole Provides Clues to Growth
[Release Date August 11, 2015]
[Distance Estimate About 340 million light years]
. . . ]
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 is also about 200,000 times less massive than the heaviest black holes found in the centers of other galaxies.
Astronomers are trying to understand the formation of billion-solar-mass black holes that have been detected from less than a billion years after the Big Bang. The black hole in RGG 118 gives astronomers an opportunity to study a nearby small supermassive black hole in lieu of the first generation of black holes that are undetectable with current technology.
Astronomers think that supermassive black holes may form when a large cloud of gas, weighing about 10,000 to 100,000 times that of the Sun, collapses into a black hole. Many of these black hole seeds then merge to form much larger supermassive black holes. Alternately, a supermassive black hole seed could come from a giant star, about 100 times the Sun’s mass, that ultimately forms into a black hole after it runs out of fuel and collapses.
. . . ]
chandra.harvard.edu/photo/2015/rgg118/