NGC 4709

E613347

NGC 4709 is a giant elliptical galaxy located in the Centaurus Cluster, notable as one of its brightest and most massive members.

Jump to: Surface forms Statements Referenced by

Observed surface forms (1)

Surface form Occurrences
NGC 4706 1

Statements (41)

Predicate Object
instanceOf elliptical galaxy
galaxy
giant elliptical galaxy
alternateName ESO 323- G 018 NERFINISHED
PGC 43414 NERFINISHED
apparentMagnitudeV ~11.5
belongsToSupercluster Hydra–Centaurus Supercluster NERFINISHED
brightnessRole brightest cluster galaxy candidate
one of the brightest galaxies in the Centaurus Cluster
catalog New General Catalogue NERFINISHED
centralBlackHole supermassive black hole (inferred)
clusterType galaxy cluster member
color red
constellation Centaurus NERFINISHED
discoveredBy John Herschel NERFINISHED
discoveryYear 1834
distanceFromEarth ~150 million light-years
~45 Mpc
dustContent low dust content
environment dense cluster environment
gasContent gas-poor
hasFeature dominant bulge component
smooth light profile
hasStellarPopulation predominantly old stars
hostCluster Centaurus Cluster core region
isPartOf Abell 3526 NERFINISHED
locatedIn Centaurus Cluster NERFINISHED
massRole one of the most massive galaxies in the Centaurus Cluster
memberOf Centaurus Cluster NERFINISHED
morphologicalType E
observedBy Hubble Space Telescope NERFINISHED
ground-based observatories
observedIn X-ray wavelengths
optical wavelengths
radialVelocity ~3300 km/s
redshift ~0.011
scientificInterest brightest cluster galaxy studies
galaxy cluster dynamics
galaxy evolution in dense environments
skyPositionReference J2000 equinox
surfaceBrightnessProfile de Vaucouleurs-like

Referenced by (3)

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

Centaurus Cluster containsGalaxy NGC 4709
this entity surface form: NGC 4706