Large Magellanic Cloud

32,200 lydiameter

Updated

32,200ly
Visual creditESA / NASA / NASA-JPL / Caltech / Christopher Clark (STScI) / S. Kim (Sejong University) / T. Wong (UIUC) / Public domainSource: Wikimedia Commons

Details

The Large Magellanic Cloud is a nearby satellite galaxy laced with vast star-forming regions and supernova debris. It contains the Tarantula Nebula, the most productive stellar nursery in the Local Group, and it hosted SN 1987A, the closest observed supernova since 1604.

The Large Magellanic Cloud is a gas-rich dwarf galaxy about 160,000 light-years from the Milky Way. Its off-center bar, star-forming regions and extended gas have been shaped by interaction with both the Small Magellanic Cloud and our galaxy.

It contains the Tarantula Nebula, the Local Group’s most luminous star-forming region, and the remnant of SN 1987A. Its proximity lets telescopes resolve individual stars and supernova debris that would blend together in more distant galaxies.

Key facts

Category
Galaxies
Object class
Dwarf irregular galaxy
Host
Local Group
Scale fact
32,200 lydiameter
Composition
~20 billion stars, gas, dust, dark matter
Embed

Size neighbors

Objects near Large Magellanic Cloud on the scale

On the logarithmic size axis, Large Magellanic Cloud falls between Small Magellanic Cloud and Sombrero Galaxy. The band uses nearby Dwarf irregular galaxy records.

Shared physical scale
24,624ly

Sources

References for Large Magellanic Cloud

Measurements and descriptive context are compiled by the Scale of Space team from the references below. If you find an error, please let us know.

Continue with nearby objects or open the full scale.

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