Messier79

E540377

Messier 79 is a dense globular star cluster located in the constellation Lepus, composed of hundreds of thousands of ancient stars.

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Observed surface forms (1)

Surface form Occurrences
Messier 79 0

Statements (44)

Predicate Object
instanceOf globular cluster
age about 11.7 billion years
angularSize 8.7 arcminutes
apparentMagnitudeV 7.7
belongsTo outer halo globular cluster system
bestViewingSeason northern winter
catalogCode M79 NERFINISHED
NGC 1904 NERFINISHED
contains hundreds of thousands of stars
coreConcentration high
declination −24° 33′
discoveredBy Pierre Méchain NERFINISHED
discoveredFor Charles Messier’s catalog
discoveredUsing small refracting telescope
discoveryDate 1780
distanceFromEarth about 13,000 parsecs
about 42,000 light-years
distanceFromGalacticCenter about 60,000 light-years
galacticLatitude −27.7°
galacticLongitude 227.2°
hasAbsoluteMagnitudeV about −7.9
hasAlternativeName GCl 7 NERFINISHED
M 79 NERFINISHED
NGC 1904 NERFINISHED
hasColorIndexBminusV about 0.78
hasHalfLightRadius about 3.5 parsecs
hasRadialVelocity about +205 km/s
includedInCatalog Messier Catalogue NERFINISHED
New General Catalogue NERFINISHED
isComposedOf ancient stars
isLocatedInHemisphere southern celestial hemisphere
locatedIn Galactic halo NERFINISHED
Milky Way
locatedInConstellation Lepus NERFINISHED
metallicityFeH about −1.6
morphologicalType class V globular cluster
namedAfter Charles Messier’s cataloging system
observedIn X-ray wavelengths
infrared wavelengths
optical wavelengths
rightAscension 05h 24m
stellarPopulation Population II stars
visibility best seen with small telescopes
visible from Earth’s southern and mid-northern latitudes

Referenced by (1)

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

Lepus containsDeepSkyObject Messier79