Type

Supermassive

Location

in the constellation Coma Berenices

Distance

325 million light-years (100 megaparsecs)

Mass

1 billion to 9 billion times the mass of the Sun

Size

Diameter at least equal to the diameter of Neptune's orbit around the Sun

Discovery Methods

• Measuring the motions of gas
• Measuring the motions of stars

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: November 19, 2009.