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
32,200 lydiameter
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
Links
Size neighbors
On the logarithmic size axis, Large Magellanic Cloud falls between Small Magellanic Cloud and Sombrero Galaxy. The band uses nearby Dwarf irregular galaxy records.
Sources
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.
About
Scale of Space is a scroll-based journey through the universe, placing objects on a single logarithmic scale so you can compare size across an unbroken range.
Guides explain selected parts of that range, while focused views filter the objects by subject.