Type

Supermassive

Location

in the constellation Cetus

Finder Chart

Distance

216 million light-years (67 megaparsecs)

Mass

Unknown 0 times the mass of the Sun

Size

Unknown

Discovery Methods

• Detection of a jet
• 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: March 15, 2012.