Andromeda central supermassive black hole

E479290

The Andromeda central supermassive black hole is the enormous black hole residing at the core of the Andromeda Galaxy (M31), exerting a dominant gravitational influence on the surrounding stars and gas in its galactic nucleus.

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Statements (50)

Predicate Object
instanceOf astrophysical object
supermassive black hole
activityClassification low-luminosity active galactic nucleus
activityLevel currently quiescent
alternativeName Andromeda nuclear black hole NERFINISHED
M31 central black hole NERFINISHED
M31* NERFINISHED
centralObjectOf Andromeda Galaxy NERFINISHED
Andromeda galactic nucleus NERFINISHED
distanceFromEarth about 2.5 million light-years
about 780 kiloparsecs
electromagneticEmission radio emission
weak X-ray emission
eventHorizonType Schwarzschild or slowly spinning Kerr black hole (uncertain spin)
evidenceType X-ray observations
gas kinematics
radio observations
stellar kinematics
formationScenario growth by accretion of gas
growth by mergers with smaller black holes
growth by tidal disruption of stars
futureEvent expected to form a binary with Sagittarius A* in several billion years
futureInteraction may interact with Milky Way central black hole after Milky Way–Andromeda merger
gravitationalInfluence nuclear star cluster of Andromeda Galaxy NERFINISHED
surrounding gas in galactic nucleus
surrounding stars in galactic bulge
hasAccretion low-luminosity accretion flow
hostGalaxy Andromeda Galaxy NERFINISHED
locatedIn Andromeda Galaxy NERFINISHED
Local Group NERFINISHED
Virgo Supercluster NERFINISHED
constellation Andromeda NERFINISHED
galactic nucleus of Andromeda Galaxy
observable universe
mass about 1.4e8 solar masses
of order 10^8 solar masses
massEstimateMethod gas dynamical modeling
stellar dynamical modeling
massRatioToSagittariusA* roughly 30
moreMassiveThan Sagittarius A* NERFINISHED
observedBy Chandra X-ray Observatory NERFINISHED
Hubble Space Telescope NERFINISHED
Keck Observatory NERFINISHED
Very Large Telescope NERFINISHED
redshift approximately -0.001 (blueshift of host galaxy)
roleInGalaxy dominant gravitational source in central parsec
influences dynamics of nuclear star cluster
similarTo Milky Way central supermassive black hole Sagittarius A* NERFINISHED
surroundedBy double-peaked nuclear star cluster
eccentric nuclear stellar disk

Referenced by (1)

Full triples — surface form annotated when it differs from this entity's canonical label.

M31* alternativeName Andromeda central supermassive black hole