Messier 62

E489452

Messier 62 is a bright, densely concentrated globular star cluster located in the constellation Ophiuchus, notable for its rich stellar population and asymmetrical appearance.

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Statements (46)

Predicate Object
instanceOf Messier object
NGC object
astronomical object
deep-sky object
globular star cluster
angularSize 15 arcminutes
apparentMagnitudeV 6.5
belongsTo Milky Way NERFINISHED
bestSeenFrom dark skies with binoculars
bestSeenIn early summer
spring
cataloguedBy Charles Messier NERFINISHED
catalogueEntry Messier catalogue NERFINISHED
New General Catalogue NERFINISHED
concentrationClass IV
contains RR Lyrae variable stars NERFINISHED
X-ray sources
blue straggler stars
millisecond pulsars
coreRadius about 0.22 arcminutes
declination −30° 06′ 49″
discoveredBy Charles Messier NERFINISHED
discoveryDate 1771
distanceFromEarth about 22,000 light-years
distanceFromGalacticCenter about 6,100 light-years
galacticLatitude +7.32°
galacticLongitude 353.57°
halfLightRadius about 1.03 arcminutes
hasAbsoluteMagnitudeV about −9.18
hasAge about 11–13 billion years
hasColorIndexBminusV about 0.80
hasDesignation M62 NERFINISHED
NGC 6266 NERFINISHED
hasMass several hundred thousand solar masses
hasMorphology asymmetrical
highly concentrated core
hasProperty rich stellar population
hasStellarPopulation Population II stars NERFINISHED
isNotableFor asymmetrical appearance due to proximity to Galactic center
high central stellar density
locatedIn Milky Way halo NERFINISHED
locatedInConstellation Ophiuchus NERFINISHED
metallicityFeH −1.18
rightAscension 17h 01m 13s
visibleFromHemisphere Southern Hemisphere NERFINISHED
low northern latitudes

Referenced by (1)

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

Ophiuchus containsDeepSkyObject Messier 62