M75

E505235

M75 is a densely concentrated globular star cluster in the constellation Sagittarius, cataloged by Charles Messier.

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Statements (41)

Predicate Object
instanceOf globular star cluster
absoluteMagnitudeV about −8.5
addedToMessierCatalogBy Charles Messier NERFINISHED
age ~13 billion years
alsoKnownAs GCl 118
Messier 75 NERFINISHED
NGC 6864 NERFINISHED
angularSize 6.8 arcminutes
apparentMagnitudeRange about 8.5–9.0
apparentMagnitudeV 8.6
catalogDesignation GCl 118
M 75 NERFINISHED
Messier 75 NERFINISHED
NGC 6864 NERFINISHED
catalogedBy Charles Messier NERFINISHED
colorIndexBminusV 0.76
concentrationClass I
coreConcentration very high
declination −21° 55′ 17″
discoveredBy Pierre Méchain NERFINISHED
discoveryYear 1780
distanceFromEarth ~20.7 kiloparsecs
~67,500 light-years
distanceFromGalacticCenter ~14.7 kiloparsecs
galacticLatitude −25.75°
galacticLongitude 8.55°
hasCoreRadius ~0.5 arcminutes
hasHalfLightRadius ~0.9 arcminutes
hasMorphologicalType globular cluster
hostGalaxy Milky Way NERFINISHED
locatedIn Milky Way halo NERFINISHED
constellation Sagittarius NERFINISHED
locatedInConstellation Sagittarius NERFINISHED
metallicity low
metallicityFeH −1.29
notes one of the most centrally concentrated globular clusters known
radialVelocity −186 km/s
rightAscension 20h 06m 05.1s
ShapleySawyerConcentrationClass I
stellarPopulation Population II NERFINISHED
visibility best seen with medium to large amateur telescopes

Referenced by (1)

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

Messier 75 otherName M75