globular cluster Messier 92

E922161

Globular cluster Messier 92 is a bright, compact, and very old spherical star cluster in the constellation Hercules, notable as one of the Milky Way’s most luminous and metal-poor globular clusters.

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Observed surface forms (1)

Surface form Occurrences
Messier 92 0

Statements (48)

Predicate Object
instanceOf Milky Way globular cluster
deep-sky object
globular cluster
absoluteMagnitudeV about −8.2
age about 13 billion years
on the order of the age of the Universe
alsoKnownAs M92 NERFINISHED
NGC 6341 NERFINISHED
angularSize about 14 arcminutes
apparentMagnitudeV about 6.3
bestSeenIn northern spring
northern summer
cataloguedBy Charles Messier NERFINISHED
celestialCategory globular cluster
concentrationClass IV
contains RR Lyrae variable stars NERFINISHED
blue straggler stars
coreDescription bright and compact core
coreRadius about 0.26 arcminutes
declination +43° 08′ 11″
discoveredBy Johann Elert Bode NERFINISHED
discoveryDate 1777
distanceFromEarth about 26,700 light-years
about 8.2 kiloparsecs
distanceFromGalacticCenter about 9.6 kiloparsecs
epoch J2000
galacticComponent Galactic halo NERFINISHED
galacticLatitude +34.9 degrees
galacticLongitude 68.3 degrees
halfLightRadius about 1.0 arcminutes
locatedInConstellation Hercules NERFINISHED
luminosity about 3×10^5 times the Sun
mass about 3×10^5 solar masses
memberOf Milky Way NERFINISHED
messierNumber 92
metallicityClass metal-poor
metallicityFeH about −2.3
nearbyOnSky north of the star Eta Herculis
ngcNumber 6341
notableFor high luminosity among Milky Way globular clusters
very low metallicity
orbitType halo orbit around the Milky Way
rightAscension 17h 17m 07.4s
shape spherical
ShapleySawyerConcentrationClass IV
stellarPopulation Population II
visibility barely visible to the naked eye under very dark skies
visible in small telescopes

Referenced by (1)

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

Hercules contains globular cluster Messier 92