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.

All labels observed (2)

Label Occurrences
NGC 869 canonical 4
NGC 869 (likely common origin) 1

How this entity was disambiguated

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
bestSeenFrom Northern Hemisphere
bestSeenInMonth November
CaldwellNumber C14
catalog Caldwell catalog
linked to: Caldwell catalogue

NGC
clusterType rich
constellation Perseus
contains B-type stars
blue giants
main-sequence stars
massive stars
coreRadius a few arcminutes
declination +57° 09′
discoveredBy Hipparchus
distanceFromEarth about 2,300 parsecs
about 7,500 light-years
galacticLatitude about +4°
galacticLongitude about 135°
hasAlternativeName Double Cluster in Perseus (component)
linked to: Double Cluster

h Persei
locatedIn Milky Way
Perseus Arm
mass several thousand solar masses
metallicity near-solar
numberOfStars several hundred visible members
observedSince antiquity
observedWith binoculars
small telescopes
pairedWith NGC 884
partOf Double Cluster
rightAscension 02h 19m
stellarPopulation Population I
usedFor studies of open cluster dynamics
studies of stellar evolution
visibleToNakedEye true

How these facts were elicited

Referenced by (5)

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

Double Cluster hasComponent NGC 869
NGC 884 hasNeighboringObject NGC 869
NGC 884 isGravitationallyBoundTo NGC 869 (likely common origin)
linked to: NGC 869
Caldwell 14 alsoKnownAs NGC 869