SMC

E114707

SMC is a nearby dwarf irregular galaxy and satellite of the Milky Way, visible from the Southern Hemisphere and important for studies of galactic evolution and stellar populations.

All labels observed (1)

Label Occurrences
SMC canonical 5

How this entity was disambiguated

Statements (49)

Predicate Object
instanceOf Local Group galaxy ⓘ
dwarf irregular galaxy ⓘ
satellite galaxy ⓘ
alternateName SMC galaxy ⓘ
Small Magellanic Cloud ⓘ
angularSize_deg ~3 ⓘ
apparentMagnitudeV ~2.7 ⓘ
bestSeenIn dark skies away from city lights ⓘ
constellation Tucana ⓘ
contains Cepheid variable stars ⓘ
H II regions ⓘ
RR Lyrae variable stars ⓘ
globular clusters ⓘ
intermediate-age stellar populations ⓘ
old stellar populations ⓘ
planetary nebulae ⓘ
star clusters ⓘ
star-forming regions ⓘ
supernova remnants ⓘ
young stellar populations ⓘ
discoveredBy known to pre-telescopic southern observers ⓘ
distanceFromEarth_kpc ~60 ⓘ
distanceFromEarth_ly ~200000 ⓘ
distanceFromMilkyWay_kpc ~60 ⓘ
galaxyType dwarf irregular ⓘ
gasMass_solarMasses ~3e8 ⓘ
hasFeature Magellanic Bridge connection to LMC ⓘ
linked to: Magellanic Bridge

distorted morphology ⓘ
extended gas envelope ⓘ
irregular structure ⓘ
interactionWith Large Magellanic Cloud ⓘ
Milky Way ⓘ
locatedIn southern celestial hemisphere ⓘ
mass_solarMasses ~7e8 ⓘ
memberOf Local Group ⓘ
metallicity low ⓘ
metallicityRelativeToSun ~0.2 Z☉ ⓘ
morphologicalType Im ⓘ
observedBy Ferdinand Magellan expedition ⓘ
satelliteOf Milky Way ⓘ
starFormationActivity ongoing ⓘ
stellarMass_solarMasses ~4e8 ⓘ
usedFor chemical evolution studies ⓘ
distance scale calibration ⓘ
star formation studies ⓘ
studies of galactic evolution ⓘ
studies of stellar populations ⓘ
visibility naked-eye object ⓘ
visibleFrom Southern Hemisphere ⓘ

How these facts were elicited

Referenced by (5)

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