Explanation: The Tarantula Nebula is a giant emission nebula within our neighboring galaxy the Large Magellanic Cloud. Inside this cosmic arachnid lies a huge central young cluster of massive stars, cataloged as R136 and partially visible on the upper right. The energetic light and winds from this cluster light up the nebula and sculpt the surrounding gas and dust into vast complex filaments. These "tentacles" give the Tarantula Nebula its name. In this impressive color image from the Wide-Field Imager camera on ESO's 2.2-meter telescope at La Silla Observatory, intricacies of the nebula's complex array of dust and gas are visible. A 300 light-year portion of the Tarantula Nebula is imaged. The Tarantula Nebula, also dubbed 30 Doradus, lies 170,000 light years away toward the constellation of Dorado.

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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: Tarantula Nebula - LMC - 30 Doradus - Tumannost' Tarantul - BMO Publikacii so slovami: Tarantula Nebula - LMC - 30 Doradus - Tumannost' Tarantul - BMO
Sm. takzhe: Zona Tarantula Bol'shoe Magellanovo Oblako Tri galaktiki i kometa Tumannost' Tarantul ot teleskopa SuperBIT Glubokoe pole: Bol'shoe Magellanovo Oblako Zvezdy v tumannosti Tarantul ot teleskopa "Dzheims Vebb" Zvezdnoe skoplenie R136 Vse publikacii na tu zhe temu >>