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The Large Magellanic Cloud (LMC) is a dwarf galaxy and satellite galaxy of the Milky Way. [7] At a distance of around 50 kiloparsecs (163,000 light-years), [2] [8] [9] [10] 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.
The Large Magellanic Cloud was the host galaxy to a supernova , the brightest observed in over four centuries. Measurements with the Hubble Space Telescope, announced in 2006, suggest the Magellanic Clouds may be moving too fast to be long term companions of the Milky Way . [ 34 ]
Large Magellanic Cloud L/T eff: HD 269551 A 1,439 [110] Large Magellanic Cloud L/T eff: HV 12463 1,420 [110] Large Magellanic Cloud L/T eff: IRAS 05280–6910: 1,367 [111] Large Magellanic Cloud L/T eff: The most reddened object in the Large Magellanic Cloud. [109] MSX LMC 597 1,278 [112] –1,444 [109] Large Magellanic Cloud L/T eff: OGLE ...
The Large Magellanic Cloud, for instance, has less dust than the Milky Way and a smaller content of what astronomers call metallic elements - those other than hydrogen and helium. That ...
The N 70 Nebula, in the Large Magellanic Cloud has a shell structure and is really a bubble in space. It is a "Super Bubble". Barnard's Loop: 300 ly (92 pc) [49] [50] H II region: Supernova over the last 4 million years probably carved cavities in gas clouds forming the semi circle shape of Barnard’s loop. Sh2-54: 252 ly (77 pc) [51] [52] H ...
The Tarantula Nebula (also known as 30 Doradus) is a large H II region in the Large Magellanic Cloud (LMC), forming its south-east corner (from Earth's perspective).
The Large Magellanic Cloud, a satellite galaxy of the Milky Way. A dwarf galaxy is a small galaxy composed of about 1000 up to several billion stars, as compared to the Milky Way's 200–400 billion stars. [1]
The Large and Small Magellanic Clouds are the largest satellite galaxies of the Milky Way and, unlike the rest of the satellite galaxies, are still actively forming stars — and at a rapid pace. The depth of these survey data can be appreciated by the number of stars visible in the outer regions of the galaxy, as seen in the lower part of the ...