Intermediate-mass black hole found in Messier 82 (M82).

Astronomers in the US have used X-rays to pin down the mass of a black hole in the nearby galaxy M82, has been thought to be an intermediate-mass black hole (100 to 10,000 solar masses). This means it is of the rarest, mid-sized black-hole type.



Image of the starburst galaxy, Messier 82 (M82). (Courtesy: NASA, ESA and The Hubble Heritage Team (STScI/AURA))


Mass is a fundamental property of any black hole, which has so much gravity that nothing can escape its grip. Not even light can escape, when it strays close enough. Black holes usually come in two main types: stellar-mass black holes that are roughly 10 times as massive as the Sun, such as Cygnus X-1, and supermassive black holes, which are typically millions or billions of times as massive as the Sun and inhabit the centres of large galaxies. The largest supermassive black hole is believed to reside in  the quasar APM 08279+5255, with a mass of 21 billion solar masses.

On the other hand, intermediate-mass black holes are much less studied compared with stellar and supermassive black holes, and that is because intermediate-mass black holes are rare.

With this confirmed candidate: the black holeM82 X-1. Previous mass estimates for this object ranged from just 20 solar masses to more than 1000, so astronomers did not know whether it was an ordinary stellar-mass black hole or a rare intermediate-mass black hole. Indeed, it was already suggested in 2006 that the black hole was an intermediate mass one, but this was yet to be confirmed. The black hole lies in M82, a “starburst” galaxy only 12 million light-years away, which spawns lots of new stars. M82 orbits M81, a giant spiral whose gravity stirs it up and triggers the starburst.

Stars are often caught by a black hole’s immense gravitational force and lose material to the objects. Before plunging into the black hole though, the trapped stellar material gets so hot it emits X-rays. The team analysed six years of X-ray observations and discovered two oscillations every 0.2 and 0.3 seconds. These periods indicate how long the hottest material takes to orbit the black hole, and far exceed the periods of similar oscillations seen around stellar-mass black holes. The longer period suggests a much greater mass, because the more massive a black hole, the larger it is and the longer material takes to revolve around it. Using two different methods, the researchers conclude that M82’s black hole is 428±105 and 415±63 times as massive as the Sun.

Supermassive black holes grow to millions or billions of times the Sun’s mass because they occupy galactic centres that attract stars and gas. But M82 X-1 is not at the centre of its galaxy. Astronomers have suggested that one way in which this black hole could have grown to such an abnormal size is thanks to a cluster of stars near its location, which could have fed the object, before a massive star’s approach ejected the black hole from the cluster.

The research is published in Nature

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