Large Magellanic Cloud

The Large Magellanic Cloud (LMC) is a spiral 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. Based on the D25 isophote at the B-band (445 nm wavelength of light), the Large Magellanic Cloud is about 9.86 kiloparsecs (32,200 light-years) across. It is roughly one-hundredth the mass of the Milky Way and is the fourth-largest galaxy in the Local Group, after the Andromeda Galaxy (M31), the Milky Way, and the Triangulum Galaxy (M33).

Large Magellanic Cloud
A map of the Large Magellanic Cloud with the brightest features annotated
Observation data (J2000 epoch)
ConstellationDorado/Mensa
Right ascension05h 23m 34s
Declination−69° 45.4
Distance163,000 light-years (49.97 kpc)
Apparent magnitude (V)0.13
Characteristics
TypeSB(s)m
Mass1×1010 (excluding dark matter), 1.38×1011 (including dark matter). M
Number of stars20 billion
Size9.86 kpc (32,200 ly)
(diameter; 25.0 mag/arcsec2 B-band isophote)
Apparent size (V)10.75° × 9.17°
Other designations
LMC, ESO 56- G 115, PGC 17223, Nubecula Major

The LMC is classified as a Magellanic spiral. It contains a stellar bar that is geometrically off center, suggesting that it was a barred dwarf spiral galaxy before its spiral arms were disrupted, likely by tidal interactions from the Small Magellanic Cloud (SMC) and the Milky Way's gravity.

With a declination of about −70°, the LMC is visible as a faint "cloud" from the southern hemisphere of the Earth and from as far north as 20° N. It straddles the constellations Dorado and Mensa and has an apparent length of about 10° to the naked eye, 20 times the Moon's diameter, from dark sites away from light pollution.

The LMC is predicted to merge with the Milky Way in approximately 2.4 billion years.

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