Explanation: Sculpted by stellar winds and radiation, a magnificent interstellar dust cloud by chance has assumed this recognizable shape. Fittingly named the Horsehead Nebula, it is some 1,500 light-years distant, embedded in the vast Orion cloud complex. About five light-years "tall", the dark cloud is cataloged as Barnard 33 and is visible only because its obscuring dust is silhouetted against the glowing red emission nebula IC 434. Stars are forming within the dark cloud. Contrasting blue reflection nebula NGC 2023, surrounding a hot, young star, is at the lower left. The gorgeous color image combines both narrowband and broadband images recorded using three different telescopes.

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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 - dust - Tumannosti mezhzvezdnye - tumannost' Konskaya Golova - emissionnaya tumannost' - otrazhatel'nye tumannosti Publikacii so slovami: nebula - dust - Tumannosti mezhzvezdnye - tumannost' Konskaya Golova - emissionnaya tumannost' - otrazhatel'nye tumannosti
Sm. takzhe: Slonovii hobot v Cefee Prizraki v Kassiopee Sem' Sester v pyli NGC 6727: tumannost' Buinyi Pavian Temnyi Morskoi konek v Cefee Melott 15 v tumannosti Serdce Tumannost' Oriona i Konskaya Golova Vse publikacii na tu zhe temu >>