Messier 80

E478912

Messier 80 is a dense globular star cluster located in the constellation Scorpius, notable for its rich population of stars and high central concentration.

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Statements (49)

Predicate Object
instanceOf Messier object
deep-sky object
globular star cluster
absoluteMagnitudeV about −8.2
age about 12 billion years
alsoKnownAs M80 NERFINISHED
NGC 6093 NERFINISHED
angularSize 10.0 arcminutes
apparentMagnitudeV 7.3
appearsAs compact fuzzy ball of light
bestSeenIn medium telescopes
small telescopes
catalogDesignation M80 NERFINISHED
NGC 6093 NERFINISHED
centralDensity high
contains RR Lyrae variables
blue straggler stars
horizontal branch stars
variable stars
coreConcentration high
declination −22° 58′ 30″
diameter about 95 light-years
discoveredBy Charles Messier NERFINISHED
discoveryDate 1781
distanceFromEarth approximately 10,000 parsecs
approximately 32,600 light-years
galacticLatitude +19.85°
galacticLongitude 352.67°
hasCoreCollapse likely core-collapsed or core-collapsing
hostGalaxy Milky Way NERFINISHED
locatedBetween Antares NERFINISHED
Beta Scorpii NERFINISHED
locatedIn Milky Way
locatedInConstellation Scorpius NERFINISHED
locatedInGalacticHalo true
memberOf Milky Way globular cluster system NERFINISHED
metallicity low
metallicityFeH about −1.75
notableFor rich population of blue stragglers
very high central star density
observedIn X-ray wavelengths
optical wavelengths
ultraviolet wavelengths
partOf Messier catalogue NERFINISHED
New General Catalogue NERFINISHED
rightAscension 16h 17m 02s
spectralTypeDominant old, low-mass stars
visibleFrom Southern Hemisphere NERFINISHED
low northern latitudes

Referenced by (1)

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

Scorpius containsDeepSkyObject Messier 80