Explanation: In the heart of monstrous Tarantula Nebula lies one of the most unusual star clusters. Known as NGC 2070 or R136, it is home to a great number of hot young stars. The energetic light from these stars continually ionizes nebula gas, while their energetic particle wind blows bubbles and defines intricate filaments. The above representative-color picture of this great LMC cluster details its tumultuous center in gas, dust and young stars. The 30 Doradus nebula is one of the largest star-formation regions known, and has been creating unusually strong episodes of star formation every few million years. In the heart of this heart is a central knot of stars that is so dense it was once thought to be a single star.

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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: nebula - star cluster - LMC - Tarantula Nebula - 30 Doradus - Tumannost' Tarantul - Bol'shoe Magellanovo Oblako - zvezdnoe skoplenie Publikacii so slovami: nebula - star cluster - LMC - Tarantula Nebula - 30 Doradus - Tumannost' Tarantul - Bol'shoe Magellanovo Oblako - zvezdnoe skoplenie
Sm. takzhe: Lisii meh, Konus i Rozhdestvenskaya elka Galaktika Bol'shoe Magellanovo Oblako Molodoe zvezdnoe skoplenie NGC 1333 Raznocvetnye oblaka i zvezdy okolo ρ Zmeenosca Zona Tarantula Tumannosti: ot Chaiki do Kalifornii Zvezdnoe skoplenie IC 348 ot teleskopa "Dzheims Vebb" Vse publikacii na tu zhe temu >>