Supermassive black hole

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Top: artist's conception of a supermassive black hole drawing material from a nearby star. Bottom: images believed to show a supermassive black hole devouring a star in galaxy RXJ 1242-11. Left: X-ray image, Right: optical image. Source: [1]
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Top: artist's conception of a supermassive black hole drawing material from a nearby star. Bottom: images believed to show a supermassive black hole devouring a star in galaxy RXJ 1242-11. Left: X-ray image, Right: optical image. Source: [1]

A supermassive black hole is a black hole with a mass in the range of millions or billions of solar masses. It is currently thought that most if not all galaxies, including the Milky Way, contain a supermassive black hole at their galactic centers.

Supermassive black holes have some interesting properties which distinguish them from relatively low-mass cousins:

  • The average density of a supermassive black hole can be very low, and may actually be lower than the density of water. This is because the Schwarzschild radius is directly proportional to mass, such that density is inversely proportional to the square of the mass.
  • The tidal forces in the vicinity of the event horizon are significantly weaker. Since the central singularity is so far away from the horizon, a hypothetical astronaut travelling towards the black hole center would not experience significant tidal force until very deep into the black hole.

Black holes of this size can only form in two ways: by slow accretion of matter (starting from a stellar size), or directly from external pressure in the first instants of Big Bang. The first method requires a long time and large amounts of matter available for the black hole growth.

Direct Doppler measures of the matter surrounding the nucleus of nearby galaxies have revealed a very fast motion, only possible with a high concentration of matter in the center. Currently, the only known object that can pack enough matter in such a small space is a black hole. For active galaxies farther away, the width of broad spectral lines is thought to be related to the mass of the black hole that powers the active galaxy's "engine".

Such supermassive black holes in the center of many galaxies are thought to be the "engine" of active objects such as Seyfert galaxies and quasars. The Max-Planck Institute for Extraterrestrial Physics provided evidence that Sagittarius A* is the supermassive black hole residing at the center of the Milky Way based on data from the ESO[2]. Our galactic central black hole was calculated to have a mass of 2.6 million solar masses.

In May 2004, Paolo Padovani and other leading astronomers announced their discovery of 30 previously-hidden supermassive black holes outside the Milky Way. Their discovery also suggests there are at least twice as many of these black holes as previously thought.

See also

Classification by type:

Classification by mass:

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