LMC

E110989

LMC is a nearby irregular dwarf galaxy and satellite of the Milky Way, notable for its active star formation and role in studies of galactic structure and evolution.

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All labels observed (1)

Label Occurrences
LMC canonical 1

Statements (51)

Predicate Object
instanceOf galaxy
irregular dwarf galaxy
satellite galaxy
angularSize_degrees ~10
apparentMagnitudeV ~0.9
associatedWith Magellanic Stream
catalogDesignation ESO 56- G 115
connectedBy Magellanic Bridge
contains 30 Doradus
Cepheid variable stars
Tarantula Nebula
surface form: N44 nebula

SN 1987A
surface form: SN 1987A remnant

Tarantula Nebula
numerous H II regions
young massive star clusters
darkMatterDominated true
diameter_ly ~14000
discoveredBy unknown ancient observers
distanceAnchorFor extragalactic distance scale
distanceFromEarth_ly ~163000
distanceFromMilkyWayCenter_ly ~163000
distanceFromSun_kpc ~50
extendsIntoConstellation Mensa
fullName Large Magellanic Cloud
galaxyType Magellanic irregular
hasProperty gas rich
high star formation rate
metallicity lower than Milky Way
hemisphere southern sky
influences Milky Way dark matter halo
interactsGravitationallyWith Small Magellanic Cloud
locatedInConstellation Dorado
mass_solarMasses ~1e10
metallicity_relativeToSun ~0.5
morphologicalType IBm
namedAfter Ferdinand Magellan
observedBy Magellan–Elcano expedition
surface form: Ferdinand Magellan expedition
orbitalPeriod_estimate_years ~1.5e9
orbitalStatus satellite of Milky Way
possibleFirstInfall true
properMotionMeasuredBy Hubble Space Telescope
radialVelocity_kmPerS ~262
satelliteOf Milky Way
stellarMass_solarMasses ~3e9
usedForStudyOf distance scale calibration
galactic structure
galaxy evolution
star formation
stellar evolution
visibility naked eye
visibleFrom Southern Hemisphere

Referenced by (1)

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