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.

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Statements (48)

Predicate Object
instanceOf globular cluster
absoluteMagnitudeV about −8.3
age about 12.9 billion years
alsoKnownAs M30 NERFINISHED
Messier 30 NERFINISHED
angularSize 12 arcminutes
apparentMagnitudeV 7.2
appearsAs bright compact globular cluster
belongsTo outer halo globular cluster system of the Milky Way
bestObservedFrom Southern Hemisphere NERFINISHED
bestObservedIn August
September
catalog Messier catalogue NERFINISHED
New General Catalogue NERFINISHED
constellation Capricornus NERFINISHED
contains RR Lyrae variables NERFINISHED
blue straggler stars
horizontal branch stars
red giant branch stars
variable stars
coreCollapseStatus core-collapsed
coreConcentration high
declination −23° 10′ 47″
discoveredBy Charles Messier NERFINISHED
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 NERFINISHED
Hubble Space Telescope NERFINISHED
partOf Local Group NERFINISHED
radialVelocity about −181 km/s
rightAscension 21h 40m 22s
skyLocation near the star Zeta Capricorni
surfaceBrightness high
visibleWith small telescope

Referenced by (1)

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

Messier 30 alsoKnownAs NGC 7099