Explanation: Dusty emission nebula IC 410 lies about 12,000 light-years away in the northern constellation Auriga. The cloud of glowing 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, bright cluster stars are seen just below the prominent dark dust cloud near picture center. Notable near the 7 o'clock position 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. Emission from sulfur atoms is shown in red, hydrogen atoms in green, and oxygen in blue hues in this false-color, narrow band composite image.

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

Publikacii s klyuchevymi slovami: emission nebula - star cluster - narrow band filter - emissionnaya tumannost' - Rasseyannoe skoplenie - zvezdoobrazovanie Publikacii so slovami: emission nebula - star cluster - narrow band filter - emissionnaya tumannost' - Rasseyannoe skoplenie - zvezdoobrazovanie
Sm. takzhe: Slonovii hobot v Cefee IC 348 i Barnard 3 NGC 602: zvezdy protiv stolbov Prizraki v Kassiopee M16: stolpy sozidaniya Melott 15 v tumannosti Serdce Molodoe zvezdnoe skoplenie NGC 1333 Vse publikacii na tu zhe temu >>