Explanation: In the center of nearby star-forming region lies a huge cluster containing some of the largest, hottest, and most massive stars known. These stars, known collectively as star cluster R136, part of the Tarantula Nebula, were captured in the featured image in visible light in 2009 through the Hubble Space Telescope. Gas and dust clouds in the Tarantula Nebula, have been sculpted into elongated shapes by powerful winds and ultraviolet radiation from these hot cluster stars. The Tarantula Nebula lies within a neighboring galaxy known as the Large Magellanic Cloud and is located a mere 170,000 light-years away.

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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: R 136 - LMC - Tumannost' Tarantul - zvezdnoe skoplenie Publikacii so slovami: R 136 - LMC - Tumannost' Tarantul - zvezdnoe skoplenie
Sm. takzhe: Molodoe zvezdnoe skoplenie NGC 1333 Zona Tarantula Zvezdnoe skoplenie IC 348 ot teleskopa "Dzheims Vebb" Bol'shoi Kovsh nad goroi Piramida Bol'shoe Magellanovo Oblako Tri galaktiki i kometa Tumannost' Tarantul ot teleskopa SuperBIT Vse publikacii na tu zhe temu >>