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.

All labels observed (1)

Label Occurrences
Messier 62 canonical 2

How this entity was disambiguated

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
bestSeenFrom dark skies with binoculars
bestSeenIn early summer
spring
cataloguedBy Charles Messier
catalogueEntry Messier catalogue
New General Catalogue
concentrationClass IV
contains RR Lyrae variable stars
X-ray sources
blue straggler stars
millisecond pulsars
coreRadius about 0.22 arcminutes
declination −30° 06′ 49″
discoveredBy Charles Messier
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
NGC 6266
hasMass several hundred thousand solar masses
hasMorphology asymmetrical
highly concentrated core
hasProperty rich stellar population
hasStellarPopulation Population II stars
isNotableFor asymmetrical appearance due to proximity to Galactic center
high central stellar density
locatedIn Milky Way halo
locatedInConstellation Ophiuchus
metallicityFeH −1.18
rightAscension 17h 01m 13s
visibleFromHemisphere Southern Hemisphere
low northern latitudes

How these facts were elicited

Referenced by (2)

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

Ophiuchus containsDeepSkyObject Messier 62
Ophiuchus containsDeepSkyObject Messier 62
subject linked to: Oph