NGC 185

E460840

NGC 185 is a dwarf spheroidal satellite galaxy of the Andromeda Galaxy, notable for its proximity to the Milky Way and its population of old stars and star clusters.

Try in SPARQL Jump to: Statements Referenced by

Statements (45)

Predicate Object
instanceOf Local Group galaxy
dwarf spheroidal galaxy
galaxy
satellite galaxy
absoluteMagnitudeV about −15.5
alsoKnownAs Caldwell 18 NERFINISHED
angularSize 11.7′ × 10.0′
apparentMagnitudeV 9.2
catalogCode NGC 185 NERFINISHED
classifiedAs dwarf elliptical in some catalogs
constellation Cassiopeia NERFINISHED
contains dust clouds
globular clusters
molecular gas
planetary nebulae
star clusters
declination +48° 20′ 15″
discoveredBy William Herschel NERFINISHED
discoveryDate 27 November 1787
distanceFromAndromedaGalaxy about 175 kiloparsecs
distanceFromEarth about 2.0 million light-years
about 620 kiloparsecs
formsPairWith NGC 147 NERFINISHED
has resolved stellar population in deep imaging
hasNucleus central stellar nucleus
hasStellarPopulation intermediate-age stars
old stars
hostGalaxy Milky Way sky northern hemisphere
isCloseTo NGC 147 NERFINISHED
memberOf Local Group NERFINISHED
metallicity low metallicity compared to the Sun
morphologicalType dSph
observableWith small amateur telescopes
radialVelocity about −202 km/s
redshift −0.000674
rightAscension 00h 38m 58s
satelliteOf Andromeda Galaxy NERFINISHED
shows evidence of a past nuclear starburst
evidence of past star formation
low-level recent star formation
stellarMass on the order of 10^8 solar masses
surfaceBrightness relatively high for a dwarf spheroidal
usedFor studies of chemical enrichment in dwarf galaxies
studies of dwarf galaxy evolution
studies of stellar populations

Referenced by (2)

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

LG containsGalaxy NGC 185
Andromeda subgroup hasMember NGC 185