Large Magellanic Cloud
(somewhat irregular satellite galaxy of the Milky Way)
The Large Magellanic Cloud (LMC)
is a satellite galaxy
orbiting the Milky Way, about 160,000 light-years away.
It is the third closest galaxy,
after the Sagittarius Dwarf Elliptical Galaxy
Canis Major Dwarf Galaxy.
Its mass is about 10 billion solar masses,
about 1/100 as massive as the
Milky Way. Its diameter is 14,000 light-years
and it the fourth largest galaxy in the
Local Group after Andromeda, the Milky Way,
and the Triangulum Galaxy.
It was formerly classified as irregular, but
is currently considered a single-armed spiral galaxy
and a galaxy classification variant
has been invented for its morphology:
Magellanic spiral galaxy
("Magellanic" indicated by an appended lower-case "m").
Interaction with the Milky Way and the Small Magellanic Cloud appear
to contribute to its irregularity. A stream of gas
exists between it and the Small Magellanic Cloud
which is a star-forming region.
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|~0||50kpc||163kly||Large Magellanic Cloud|
Referenced by pages:
luminous blue variable (LBV)
Local Group (LG)
Magellanic Catalogue of Stars (MACS)
Magellanic clouds (MC)
Milky Way subgroup
rare designator prefixes
Radcliffe Observatory Magellanic Clouds Catalogue (RMC)
SN 1987A (1987A)
VLT-FLAMES Tarantula Survey (VFTS)