Explanation: A faint, dusty rose of the northern sky, emission nebula IC 410 lies about 12,000 light-years away in the constellation Auriga. The cloud of glowing hydrogen gas is over 100 light-years across, sculpted by stellar winds and radiation from embedded open star cluster NGC 1893. Formed in the interstellar cloud a mere 4 million years ago, the bright cluster stars are seen just below the prominent dark dust cloud near picture center. Notable near the 7 o'clock position in this wide, detailed view are two relatively dense streamers of material trailing away from the nebula's central regions. Potentially sites of ongoing star formation, these cosmic tadpole shapes are about 10 light-years long.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
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NASA Official: Jay Norris. Specific rights apply.
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& Michigan Tech. U.

Publikacii s klyuchevymi slovami: emission nebula - star cluster - zvezdnoe skoplenie - emissionnaya tumannost' - zvezdoobrazovanie Publikacii so slovami: emission nebula - star cluster - zvezdnoe skoplenie - emissionnaya tumannost' - zvezdoobrazovanie
Sm. takzhe: Slonovii hobot v Cefee IC 348 i Barnard 3 Prizraki v Kassiopee M16: stolpy sozidaniya Melott 15 v tumannosti Serdce Molodoe zvezdnoe skoplenie NGC 1333 Tumannost' Tyul'pan i chernaya dyra Lebed' X-1 Vse publikacii na tu zhe temu >>