NGC 5286

E518173

NGC 5286 is a bright, densely packed globular star cluster located in the southern sky and often studied for its old, metal-poor stellar population.

All labels observed (1)

Label Occurrences
NGC 5286 canonical 1

How this entity was disambiguated

Statements (46)

Predicate Object
instanceOf globular cluster ⓘ
absoluteMagnitudeV about −8.7 ⓘ
age about 12.5 billion years ⓘ
old stellar population ⓘ
angularSize 9.6 arcminutes ⓘ
apparentMagnitudeV 7.3 ⓘ
belongsTo Milky Way globular cluster system ⓘ
bestObservedIn spring months in Southern Hemisphere ⓘ
bestSeenFrom Southern Hemisphere ⓘ
catalog New General Catalogue ⓘ
concentrationClass high ⓘ
contains RR Lyrae variable stars ⓘ
blue straggler stars ⓘ
coreCollapsed no ⓘ
declination −51° 22′ 27″ ⓘ
discoveredBy James Dunlop ⓘ
discoveryYear 1826 ⓘ
distanceFromEarth about 11.7 kiloparsecs ⓘ
about 38,000 light-years ⓘ
GalacticLatitude about +10.6 degrees ⓘ
GalacticLongitude about 311.6 degrees ⓘ
halfLightRadius about 2.4 arcminutes ⓘ
horizontalBranchMorphology blue horizontal branch ⓘ
isPartOf Local Group ⓘ
locatedIn Galactic halo ⓘ
Milky Way ⓘ
locatedInConstellation Centaurus ⓘ
mass on the order of 10^5 solar masses ⓘ
metallicity metal-poor ⓘ
metallicityFeH about −1.7 ⓘ
morphologicalType concentrated globular cluster ⓘ
notableFor dense central region ⓘ
multiple stellar populations ⓘ
old metal-poor stars ⓘ
observedBy Hubble Space Telescope ⓘ
observedIn infrared wavelengths ⓘ
optical wavelengths ⓘ
otherDesignation C 1343-512 ⓘ
ESO 221- SC5 ⓘ
rightAscension 13h 46m 26.8s ⓘ
ShapleySawyerConcentrationClass II ⓘ
stellarPopulation Population II ⓘ
studiedFor chemical evolution of the Galactic halo ⓘ
dynamics of dense stellar systems ⓘ
surfaceBrightness high central surface brightness ⓘ
visibility southern sky ⓘ

How these facts were elicited

Referenced by (1)

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