Type
Location
In the constellation Ursa Major
Distance
65 million light-years (19.9 megaparsecs)
Mass
9 million times the mass of the Sun
Size
Diameter about one-half the size of the orbit of Mercury
Discovery Methods
Measuring the motions of stars
Because a black hole is both massive and compact, it exerts a strong gravitational pull on the material around it. Astronomers can deduce the presence of a supermassive black hole in the core of a galaxy by measuring the velocities of stars that orbit the black hole. A more-massive black hole will accelerate nearby stars to greater speeds, so the velocities of stars can reveal not only the presence of a black hole, but its mass as well.
More about black hole discovery methods »
This document was last modified: March 14, 2012.
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