M31*

E110379

M31* is the supermassive black hole located at the core of the Andromeda Galaxy.

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All labels observed (1)

Label Occurrences
M31* canonical 1

Statements (48)

Predicate Object
instanceOf astronomical object
supermassive black hole
alternativeName Andromeda central supermassive black hole
central black hole of Andromeda
belongsToSystem nuclear star cluster of Andromeda
category central black holes of spiral galaxies
supermassive black holes in nearby galaxies
centralRole dominant mass concentration in the nucleus of Andromeda
comparedTo less massive than Sagittarius A*
less massive than many quasar black holes
discoveredIn 20th century
distanceFromEarth approximately 2.5 million light-years
approximately 780 kiloparsecs
emissionType X-ray emission
radio emission
environment central bulge of Andromeda
dense nuclear stellar cluster
evidenceType X-ray observations
gas kinematics
stellar dynamics
galaxyTypeOfHost barred spiral galaxy
gravitationalEffect governs orbits of nearby nuclear stars
influences dynamics of central gas in Andromeda
hasAccretionActivity low-luminosity active nucleus
hasProperty accretion flow
event horizon
very strong gravitational field
hostGalaxy Andromeda Galaxy
hostGalaxyConstellation Andromeda Galaxy
surface form: Andromeda
hostGalaxyDistanceFromEarth approximately 2.5 million light-years
hostGalaxyMessierNumber Andromeda Galaxy
surface form: M31
hostGalaxyNGCNumber NGC 224
locatedIn Andromeda Galaxy
Local Group
Virgo Supercluster
core of the Andromeda Galaxy
observable universe
mass approximately 1.4e8 solar masses
on the order of 100 million solar masses
observedBy Chandra X-ray Observatory
Hubble Space Telescope
ground-based optical telescopes
radio telescopes
partOf Andromeda Galaxy nucleus
redshift approximately -0.001
researchField black hole astrophysics
galactic nuclei
roleInGalaxyEvolution influences evolution of Andromeda’s central region

Referenced by (1)

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