Large Magellanic Cloud

E20343

The Large Magellanic Cloud is a nearby irregular dwarf galaxy visible from the Southern Hemisphere and notable for its role in studies of galaxy formation, stellar evolution, and the cosmic distance scale.

Try in SPARQL Jump to: Surface forms Statements Referenced by

All labels observed (3)

Statements (48)

Predicate Object
instanceOf astronomical object
galaxy
irregular dwarf galaxy
satellite galaxy
abbreviation LMC
angularSize about 10 degrees across on the sky
apparentMagnitudeV about 0.9
associatedWith Magellanic Stream
bestSeenFrom southern mid-latitudes
connectedBy Magellanic Bridge
surface form: Magellanic Bridge to the Small Magellanic Cloud
constellation Dorado
contains 30 Doradus
SN 1987A
Tarantula Nebula
numerous H II regions
old globular clusters
young massive star clusters
diameter about 14000 light-years
discovery known since antiquity to southern observers
distanceFromMilkyWay about 160000 light-years
about 50 kiloparsecs
galaxyType Magellanic irregular
barred Magellanic spiral
hasFeature Magellanic Bridge
extended gaseous disk
prominent bar structure
warped disk
interactsGravitationallyWith Milky Way
Small Magellanic Cloud
locatedIn Local Group
mass on the order of 10^10 solar masses
metallicity lower than Milky Way average
name Large Magellanic Cloud self-link
namedAfter Ferdinand Magellan
observedBy Gaia observatory
surface form: Gaia spacecraft

Hubble Space Telescope
ground-based telescopes worldwide
orbitalCompanionOf Small Magellanic Cloud
orbitalStatus possibly on first infall into the Milky Way halo
regionOfSky southern celestial hemisphere
satelliteOf Milky Way
starFormationRate relatively high for its size
stellarMass on the order of 10^9 solar masses
usedFor Cepheid period–luminosity relation calibration
calibration of the cosmic distance scale
studies of galaxy formation
studies of stellar evolution
visibleFrom Southern Hemisphere

Referenced by (31)

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

Milky Way hasSatellite Large Magellanic Cloud
Local Group contains Large Magellanic Cloud
Large Magellanic Cloud name Large Magellanic Cloud self-link
Magellanic Clouds consistsOf Large Magellanic Cloud
Magellanic Clouds connectedTo Large Magellanic Cloud
subject surface form: Small Magellanic Cloud
Magellanic Clouds connects Large Magellanic Cloud
subject surface form: Magellanic Bridge
OGLE-IV survey monitorsRegion Large Magellanic Cloud
Milky Way subgroup hasMember Large Magellanic Cloud
LG containsGalaxy Large Magellanic Cloud
Al-Sufi described Large Magellanic Cloud
this entity surface form: Large Magellanic Cloud as a nebulous patch (for southern observers)
LMC fullName Large Magellanic Cloud
SN 1987A hostGalaxy Large Magellanic Cloud
Dorado containsMostOf Large Magellanic Cloud
Magellanic Bridge connects Large Magellanic Cloud
Magellanic Stream associatedWith Large Magellanic Cloud
SMC interactionWith Large Magellanic Cloud
Nubecula Minor isInteractingWith Large Magellanic Cloud
PGC 3085 interactsWith Large Magellanic Cloud
ESO 029- G 011 interactsGravitationallyWith Large Magellanic Cloud
ESO 029- G 011 isNeighborOf Large Magellanic Cloud
30 Doradus locatedIn Large Magellanic Cloud
30 Doradus hostGalaxy Large Magellanic Cloud
Tarantula Nebula locatedIn Large Magellanic Cloud
Tarantula Nebula hostGalaxy Large Magellanic Cloud
constellation Dorado containsMostOf Large Magellanic Cloud
subject surface form: Dorado
constellation Dorado containsPartOf Large Magellanic Cloud
subject surface form: Dorado
this entity surface form: Milky Way satellite galaxy Large Magellanic Cloud
constellation Dorado containsGalaxy Large Magellanic Cloud
subject surface form: Dorado
OGLE-III monitors Large Magellanic Cloud
OGLE-III hostGalaxyFields Large Magellanic Cloud
Wolf–Rayet stars location Large Magellanic Cloud
subject surface form: Wolf–Rayet star