Little is known about how they form. And some astronomers question whether they behave like other black holes. The finding by University of Maryland astronomy graduate student Dheeraj Pasham and two colleagues reveals that the black hole in question is a just-right-sized version of this class of astral objects. During the study, Pasham focused on one object in Messier 82, a galaxy in the constellation Ursa Major. Messier 82 is our closest "starburst galaxy" where young stars are forming. Among the material circling the suspected black hole, he spotted two repeating flares of light. The flares showed a rhythmic pattern of light pulses, one occurring 5.1 times per second and the other 3.3 times per second - or a ratio of 3:2.
Pasham used the oscillations to estimate that M82 X-1 is 428 times the mass of the sun, give or take 105 solar masses. He, however, does not propose an explanation for how this class of black holes formed. "We needed to confirm their existence observationally first. Now the theorists can get to work." A black hole is a region in space containing a mass so dense that not even light can escape its gravity. Black holes are invisible, but astronomers can find them by tracking their gravitational pull on other objects. The study was published online in the journal Nature.