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Black Holes Encyclopedia
Stats

Type

Supermassive

Location

In the constellation Virgo

Distance

75 million light-years (23 megaparsecs)

Mass

300 million times the mass of the Sun

Size

Diameter equal to the diameter of Jupiter’s orbit around the Sun

Discovery Methods

Description

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: February 22, 2013.