supermassive black hole oor Masedonies
supermassive black hole
en
(astronomy) Any black hole with a mass 10 <sup>5</sup> to a few times 10 <sup>10</sup> times that of the Sun.
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en
largest type of black hole; usually found at the centers of galaxies
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Supermassive black holes have properties that distinguish them from lower-mass classifications.
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The only thing that scientists can imagine that would possibly fit this description is a supermassive black hole.
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Binary supermassive black holes are believed to be a common consequence of galactic mergers.
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The origin of supermassive black holes remains an open field of research.
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Stellar black holes have much greater average densities than supermassive black holes.
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At the core, most galaxies have a supermassive black hole, which may result in an active galactic nucleus.
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Every massive elliptical galaxy contains a supermassive black hole at its center.
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(Supermassive black holes up to 21 billion (2.1 × 1010) M☉ have been detected, such as NGC 4889.)
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This suggests that supermassive black holes arose very early in the Universe, inside the first massive galaxies.
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Unlike stellar mass black holes, supermassive black holes have comparatively low average densities.
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Cygnus A—Is It a Supermassive Black Hole?
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On March 28, 2011, a supermassive black hole was seen tearing a mid-size star apart.
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The quasar SDSS J092712.65+294344.0 is thought to contain a recoiling supermassive black hole.
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In addition, the tidal forces in the vicinity of the event horizon are significantly weaker for supermassive black holes.
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In our own galaxy, for instance, the object called Sagittarius A* is believed to be a supermassive black hole.
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This was, therefore, the first indication that a supermassive black hole exists in the center of the Milky Way.
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Blazar – very compact quasar associated with a presumed supermassive black hole at the center of an active, giant elliptical galaxy.
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As such, peculiar galaxies tend to host more active galactic nuclei than normal galaxies, indicating that they contain supermassive black holes.
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There are, however, several hypotheses for the formation mechanisms and initial masses of the progenitors, or "seeds", of supermassive black holes.
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At a distance of 400 million light-years, this "butterfly-shaped" galaxy has two supermassive black holes 3,000 light-years apart.
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It is thought that supermassive black holes like these do not form immediately from the singular collapse of a cluster of stars.
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Some galaxies, such as the galaxy 4C +37.11, appear to have two supermassive black holes at their centers, forming a binary system.
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The difficulty in forming a supermassive black hole resides in the need for enough matter to be in a small enough volume.
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After two supermassive black holes coalesce, emission of linear momentum can produce a "kick" with amplitude as large as 4000 km/s.
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Observations reveal that quasars were much more frequent when the Universe was younger, indicating that supermassive black holes formed and grew early.
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