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Large Magellanic Cloud
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Large Magellanic Cloud

Satellite galaxy of the Milky Way

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Population III star (1) Β· Sloan Digital Sky Survey (1) Β· stellar migration (1) Β· Large Magellanic Cloud (1) Β· metallicity (1) Β· University of Chicago (1) Β· ancient star (1) Β· astrophysics education (1)

πŸ“– Key Information

The Large Magellanic Cloud (LMC) is a dwarf galaxy and satellite galaxy of the Milky Way. At a distance of around 50 kiloparsecs (163,000 light-years), the LMC is the second- or third-closest galaxy to the Milky Way, after the Sagittarius Dwarf Spheroidal (c. 16 kiloparsecs (52,000 light-years) away) and the possible dwarf irregular galaxy called the Canis Major Overdensity. It is about 9.86 kiloparsecs (32,200 light-years) across, and has roughly one-hundredth the mass of the Milky Way making it the fourth-largest galaxy in the Local Group, after the Andromeda Galaxy (M31), the Milky Way, and the Triangulum Galaxy (M33).

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Sloan Digital Sky Survey(1)Stellar population(1)University of Chicago(1)Large Magellanic Cloud

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