NGC 7099

E869023

NGC 7099 is a dense globular star cluster in the constellation Capricornus, notable for its age, brightness, and rich population of ancient stars.

All labels observed (1)

Label Occurrences
NGC 7099 canonical 3

How this entity was disambiguated

Statements (48)

Predicate Object
instanceOf globular cluster ⓘ
absoluteMagnitudeV about −8.3 ⓘ
age about 12.9 billion years ⓘ
alsoKnownAs M30 ⓘ
Messier 30 ⓘ
angularSize 12 arcminutes ⓘ
apparentMagnitudeV 7.2 ⓘ
appearsAs bright compact globular cluster ⓘ
belongsTo outer halo globular cluster system of the Milky Way ⓘ
bestObservedFrom Southern Hemisphere ⓘ
bestObservedIn August ⓘ
September ⓘ
catalog Messier catalogue ⓘ
New General Catalogue ⓘ
constellation Capricornus ⓘ
contains RR Lyrae variables ⓘ
blue straggler stars ⓘ
horizontal branch stars ⓘ
red giant branch stars ⓘ
variable stars ⓘ
coreCollapseStatus core-collapsed ⓘ
coreConcentration high ⓘ
declination −23° 10′ 47″ ⓘ
discoveredBy Charles Messier ⓘ
discoveryDate 1764 ⓘ
distanceFromEarth about 27,000 light-years ⓘ
about 8.3 kiloparsecs ⓘ
galacticLatitude −23.18 degrees ⓘ
galacticLongitude 27.18 degrees ⓘ
galacticPopulation Population II stars ⓘ
hasColorIndexBminusV about 0.71 ⓘ
locatedIn Galactic halo ⓘ
Milky Way ⓘ
mass on the order of 10^5 solar masses ⓘ
metallicity low ⓘ
metallicityFeH about −2.3 ⓘ
morphologicalType concentrated globular cluster ⓘ
notableFor ancient stellar population ⓘ
dense core ⓘ
low metallicity ⓘ
observedBy Gaia spacecraft ⓘ
linked to: Gaia observatory

Hubble Space Telescope ⓘ
partOf Local Group ⓘ
radialVelocity about −181 km/s ⓘ
rightAscension 21h 40m 22s ⓘ
skyLocation near the star Zeta Capricorni ⓘ
surfaceBrightness high ⓘ
visibleWith small telescope ⓘ

How these facts were elicited

Referenced by (3)

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

Messier 30 → alsoKnownAs → NGC 7099 ⓘ
M30 → alsoKnownAs → NGC 7099 ⓘ
M30 → catalogNumber → NGC 7099 ⓘ