In the constellation Hydra
340 million times the mass of the Sun
Diameter larger than the size of the orbit of Jupiter
Early black hole studies revealed a possible relationship between the mass of a supermassive black hole in the center of a galaxy and the mass of the "bulge" of stars around it. Later studies showed an even tighter relationship between the black hole and the range of orbital speeds for stars within the bulge. These relationships are crucial for understanding the link between the formation of central black holes and their surrounding galaxies.
To better understand this link, astronomers are using Hubble Space Telescope and ground-based telescopes to measure the masses of central black holes and the velocities of the stars around them in many more galaxies.
A study released in 2009, for example, targeted five galaxies, including NGC 3585, a large lens-shaped galaxy that is relatively close by, at a distance of about 70 million light-years.
The study team included Karl Gebhardt, one of the astronomers who discovered the relationship between the mass of a central black hole and the mass of the surrounding stellar bulge.
The astronomers used two Hubble instruments, the Wide Field Planetary Camera 2 (WFPC2), which takes sharp images of the galaxies, particularly their central regions; and the Space Telescope Imaging Spectrograph, which takes spectra at several locations across a galaxy. The spectra reveal the orbital speeds of stars at different regions within the galaxy. Stars that are near a supermassive black hole move much more quickly. By measuring the speeds of stars close to the galactic center, astronomers can determine the black hole's mass. Measuring speeds across a larger section of the galaxy reveals how the orbital speed changes at different distances from the black hole.
The observations of NGC 3585 reveal that the central black hole is likely between 200 million and 400 million times the mass of the Sun, with the most likely weight at 340 million times the Sun's mass. That places the black hole near the middle of the "supermassive" scale.
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This document was last modified: March 14, 2012.