Messier 75

E118336

Messier 75 is a densely concentrated globular star cluster located in the constellation Sagittarius, notable for its great distance from Earth and rich population of ancient stars.

All labels observed (1)

Label Occurrences
Messier 75 canonical 1

How this entity was disambiguated

Statements (45)

Predicate Object
instanceOf Messier object
NGC object
globular star cluster
absoluteMagnitudeV −8.57
age ~13 billion years
angularSize 6.8 arcminutes
apparentMagnitudeV 8.5
belongsTo Milky Way stellar halo
surface form: Milky Way halo
bestObservedInMonth August
catalog Messier catalogue
surface form: Messier Catalogue

New General Catalogue
cataloguedBy Charles Messier
constellation Sagittarius
coreConcentrationClass II
coreRadius ~0.44 arcminutes
declination −21° 55′ 17″
discoverer Pierre Méchain
discoveryDate 1780
discoveryMethod telescopic observation
distanceFromEarth ~20.7 kiloparsecs
~67,500 light-years
distanceFromGalacticCenter ~14.7 kiloparsecs
galacticLatitude −25.75°
galacticLongitude 12.18°
halfLightRadius ~0.86 arcminutes
hemisphereVisibility Southern sky
locatedIn Milky Way
mass ~1,000,000 solar masses
MessierNumber 75
metallicityFeH −1.29
NGCNumber 6864
notableFeature rich population of old, metal-poor stars
very high central concentration of stars
observedIn optical wavelengths
otherName GCl 117
M75
NGC 6864
population ancient stars
radialVelocity ~−190 km/s
rightAscension 20h 06m 05.0s
ShapleySawyerConcentrationClass I
skyLocation near the border of Sagittarius and Capricornus
stellarPopulationType Population II
surfaceBrightness high
visibility best seen with small telescope

How these facts were elicited

Referenced by (1)

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

Sagittarius contains Messier 75