Magellanic Clouds

E41172

The Magellanic Clouds are two irregular dwarf galaxies orbiting the Milky Way, prominently visible from the Southern Hemisphere as hazy patches in the night sky.


Statements (50)
Predicate Object
instanceOf galactic system
gaseous bridge
gaseous stream
irregular dwarf galaxy
irregular dwarf galaxy
areImportantFor studies of galaxy interaction and evolution
arePartOf Local Group
areTypeOf irregular dwarf galaxies
areUsedAs calibrators for the cosmic distance scale
areVisibleAs hazy patches in the night sky
areVisibleFrom Southern Hemisphere
associatedWith Magellanic Stream
connectedBy Magellanic Bridge
connectedTo Large Magellanic Cloud
connects Large Magellanic Cloud
Small Magellanic Cloud
consistsOf Large Magellanic Cloud
Small Magellanic Cloud
contains 30 Doradus
H II regions
Tarantula Nebula
emission nebulae
numerous star clusters
young star clusters
extendsAround Milky Way
hasAngularSize about 10 degrees
about 3 by 5 degrees
hasApparentMagnitude about 0.9
about 2.7
hasApproximateDistance 160,000 light-years
200,000 light-years
hasMorphologicalType Magellanic spiral / irregular
dwarf irregular
hasStarFormationActivity high
haveComponent interacting gas streams
haveInteractionBetween Large Magellanic Cloud and Small Magellanic Cloud
haveInteractionWith Milky Way
isMemberOf Magellanic Clouds
Magellanic Clouds
isNearest one of the nearest galaxies to the Milky Way
isSatelliteGalaxyOf Milky Way
Milky Way
locatedIn constellation Dorado
constellation Tucana
southern celestial hemisphere
namedAfter Ferdinand Magellan
orbit Milky Way
Milky Way
Milky Way
originatesFrom Magellanic Clouds


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