Coma Cluster

E576473

The Coma Cluster is a massive, nearby galaxy cluster rich in elliptical galaxies and dark matter, located in the constellation Coma Berenices.

Jump to: Statements Referenced by

Statements (50)

Predicate Object
instanceOf Abell cluster
galaxy cluster
rich cluster of galaxies
alsoKnownAs Abell 1656 NERFINISHED
cataloguedIn Abell catalogue of rich clusters NERFINISHED
contains IC 4051 NERFINISHED
NGC 4874 NERFINISHED
NGC 4889 NERFINISHED
hot intracluster gas
radio halo
radio relics
thousands of member galaxies
containsLargeAmountOf dark matter
discoveredBy Frederick William Herschel NERFINISHED
discoveryCentury 18th century
distanceFromEarth about 100 megaparsecs
about 320 million light-years
environmentType dense cluster core
hasApproximateMass about 10^15 solar masses
hasCentralGalaxy cD galaxy NGC 4874 NERFINISHED
giant elliptical NGC 4889 NERFINISHED
hasColorMagnitudeRelation prominent red sequence of galaxies
hasDeclination +27° 58′
hasDynamicalState partially relaxed
hasEvidenceFor non-thermal radio emission
hasFew spiral galaxies
hasGalaxyDensity very high in central region
hasGalaxyPopulation dominated by early-type galaxies
hasGravitationalLensing yes
hasIntraclusterMedium X-ray emitting plasma
hasLuminosityFunction well-studied
hasMeanGalaxyMagnitude about 13–15 in V band
hasMorphology roughly spherical
hasOngoing cluster mergers
hasRightAscension about 12h 59m
hasSubstructure multiple galaxy subgroups
hasVelocityDispersion about 1000 km/s
hasXRayEmission yes
intraclusterGasTemperature about 8 keV
isOneOf most studied galaxy clusters
nearest rich clusters of galaxies
locatedInConstellation Coma Berenices NERFINISHED
memberOf Coma Supercluster NERFINISHED
redshift 0.023
richIn elliptical galaxies
lenticular galaxies
usedAs laboratory for galaxy evolution studies
probe of dark matter distribution
usedToTest cosmological models
mass-to-light ratios in clusters

Referenced by (1)

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