Explanation: Cosmic clouds seem to form fantastic shapes in the central regions of emission nebula IC 1805. Of course, the clouds are sculpted by stellar winds and radiation from massive hot stars in the nebula's newborn star cluster, Melotte 15. About 1.5 million years young, the cluster stars are toward the right in this colorful skyscape, along with dark dust clouds in silhouette against glowing atomic gas. A composite of narrow and broad band telescopic images, the view spans about 30 light-years and includes emission from hydrogen in green, sulfur in red, and oxygen in blue hues. Wider field images reveal that IC 1805's simpler, overall outline suggests its popular name - The Heart Nebula. IC 1805 is located about 7,500 light years away toward the constellation Cassiopeia.

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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 formation - tumannost' - zvezdnoe skoplenie - pyl' Publikacii so slovami: emission nebula - star formation - tumannost' - zvezdnoe skoplenie - pyl'
Sm. takzhe: Lisii meh, Konus i Rozhdestvenskaya elka Okolo tumannosti Serdce Slonovii hobot v Cefee Prizraki v Kassiopee M16: stolpy sozidaniya Temnyi Morskoi konek v Cefee Molodoe zvezdnoe skoplenie NGC 1333 Vse publikacii na tu zhe temu >>