Explanation: The 16th century Portuguese navigator Ferdinand Magellan and his crew had plenty of time to study the southern sky during the first circumnavigation of planet Earth. As a result, two fuzzy cloud-like objects easily visible to southern hemisphere skygazers are known as the Clouds of Magellan, now understood to be satellite galaxies of our much larger, spiral Milky Way galaxy. About 160,000 light-years distant in the constellation Dorado, the Large Magellanic Cloud (LMC) is seen here in a remarkably deep, colorful, image. Spanning about 15,000 light-years or so, it is the most massive of the Milky Way's satellite galaxies and is the home of the closest supernova in modern times, SN 1987A. The prominent patch below center is 30 Doradus, also known as the magnificent Tarantula Nebula, a giant star-forming region about 1,000 light-years across.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Publikacii s klyuchevymi slovami: LMC - BMO - Bol'shoe Magellanovo Oblako Publikacii so slovami: LMC - BMO - Bol'shoe Magellanovo Oblako
Sm. takzhe: Galaktika Bol'shoe Magellanovo Oblako Zona Tarantula Bol'shoe Magellanovo Oblako Tri galaktiki i kometa Tumannost' Tarantul ot teleskopa SuperBIT Glubokoe pole: Bol'shoe Magellanovo Oblako N11: zvezdnye oblaka v Bol'shom Magellanovom Oblake Vse publikacii na tu zhe temu >>