NGC 869

E460835

NGC 869 is a young, massive open star cluster in the constellation Perseus, best known as one half of the prominent Double Cluster visible to the naked eye.

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Statements (44)

Predicate Object
instanceOf astronomical object
open star cluster
star cluster
age about 13 million years
young
angularSize 30 arcminutes
apparentBrightness prominent
apparentMagnitudeV 5.3
appearsIn Perseus OB association region NERFINISHED
bestSeenFrom Northern Hemisphere NERFINISHED
bestSeenInMonth November
CaldwellNumber C14
catalog Caldwell catalog NERFINISHED
NGC NERFINISHED
clusterType rich
constellation Perseus NERFINISHED
contains B-type stars
blue giants
main-sequence stars
massive stars
coreRadius a few arcminutes
declination +57° 09′
discoveredBy Hipparchus NERFINISHED
distanceFromEarth about 2,300 parsecs
about 7,500 light-years
galacticLatitude about +4°
galacticLongitude about 135°
hasAlternativeName Double Cluster in Perseus (component) NERFINISHED
h Persei NERFINISHED
locatedIn Milky Way
Perseus Arm NERFINISHED
mass several thousand solar masses
metallicity near-solar
numberOfStars several hundred visible members
observedSince antiquity
observedWith binoculars
small telescopes
pairedWith NGC 884 NERFINISHED
partOf Double Cluster NERFINISHED
rightAscension 02h 19m
stellarPopulation Population I
usedFor studies of open cluster dynamics
studies of stellar evolution
visibleToNakedEye true

Referenced by (2)

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