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.

All labels observed (1)

Label Occurrences
Messier 80 canonical 2

How this entity was disambiguated

Statements (49)

Predicate Object
instanceOf Messier object ⓘ
deep-sky object ⓘ
globular star cluster ⓘ
absoluteMagnitudeV about −8.2 ⓘ
age about 12 billion years ⓘ
alsoKnownAs M80 ⓘ
NGC 6093 ⓘ
angularSize 10.0 arcminutes ⓘ
apparentMagnitudeV 7.3 ⓘ
appearsAs compact fuzzy ball of light ⓘ
bestSeenIn medium telescopes ⓘ
small telescopes ⓘ
catalogDesignation M80 ⓘ
NGC 6093 ⓘ
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 ⓘ
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 ⓘ
locatedBetween Antares ⓘ
Beta Scorpii ⓘ
locatedIn Milky Way ⓘ
locatedInConstellation Scorpius ⓘ
locatedInGalacticHalo true ⓘ
memberOf Milky Way globular cluster system ⓘ
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 ⓘ
New General Catalogue ⓘ
rightAscension 16h 17m 02s ⓘ
spectralTypeDominant old, low-mass stars ⓘ
visibleFrom 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.

Scorpius → containsDeepSkyObject → Messier 80 ⓘ
Pierre Méchain → discovered → Messier 80 ⓘ