globular cluster NGC 6712

E481662

Globular cluster NGC 6712 is a relatively loose, heavily reddened globular star cluster in the Milky Way, notable for its interaction with the Galactic disk and significant tidal stripping.

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Observed surface forms (1)

Surface form Occurrences
NGC 6712 0

Statements (49)

Predicate Object
instanceOf astronomical object
globular cluster
age ~12 billion years
angularSize ~7.2 arcminutes
apparentMagnitudeV ~8.1
belongsTo Galactic halo
bestObservedIn summer months
catalogCode NGC 6712 NERFINISHED
clusterType Galactic globular cluster
colorExcess heavily reddened
concentration relatively loose
contains X-ray sources
blue straggler stars
variable stars
declination −08° 42′ 22″
discoveredBy William Herschel NERFINISHED
discoveryDate 1784
discoveryMethod optical telescope observation
distanceFromEarth ~22,500 light-years
~6.9 kiloparsecs
dynamicalStatus strongly tidally disturbed
foregroundEffect strong interstellar extinction
galacticComponent inner halo
galacticLatitude −4.3°
hostGalaxy Milky Way NERFINISHED
locatedIn Milky Way
constellation Scutum NERFINISHED
memberOf New General Catalogue NERFINISHED
metallicity low metallicity
metallicityFeH about −1.0
notableFor interaction with Galactic disk
significant tidal stripping
observedBy Hubble Space Telescope NERFINISHED
ground-based observatories
observedIn infrared wavelengths
optical wavelengths
orbits Milky Way center NERFINISHED
otherDesignation C 1851-084
GCl 110 NERFINISHED
reddeningEBV ~0.45
rightAscension 18h 53m 04s
showsFeature depleted low-mass stars
evidence of mass loss
skyLocation near the Scutum Star Cloud
stellarDensity moderate central concentration
stellarPopulation old stars
structuralConcentrationClass IX
tidalInteractionWith Milky Way disk NERFINISHED
visibility best seen from southern hemisphere

Referenced by (1)

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

Scutum constellation contains globular cluster NGC 6712
subject surface form: Scutum