Explanation: One of the most identifiable nebulae in the sky, the Horsehead Nebula in Orion, is part of a large, dark, molecular cloud. Also known as Barnard 33, the unusual shape was first discovered on a photographic plate in the late 1800s. The red glow originates from hydrogen gas predominantly behind the nebula, ionized by the nearby bright star Sigma Orionis. The darkness of the Horsehead is caused mostly by thick dust, although the lower part of the Horsehead's neck casts a shadow to the left. Streams of gas leaving the nebula are funneled by a strong magnetic field. Bright spots in the Horsehead Nebula's base are young stars just in the process of forming. Light takes about 1500 years to reach us from the Horsehead Nebula. The above image was taken with the 0.9-meter telescope at Kitt Peak National Observatory.

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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: Horsehead Nebula - Konskaya golova - Molekulyarnye oblaka Publikacii so slovami: Horsehead Nebula - Konskaya golova - Molekulyarnye oblaka
Sm. takzhe: Ruka pomoshi v Kassiopee Temnyi Morskoi konek v Cefee Tumannost' Oriona i Konskaya Golova Tumannost' "Temnaya shtuchka" Temnaya tumannost' Lindsa LDN 1251 NGC 6188: drakony v Zhertvennike Molekulyarnoe oblako Hameleon-I Vse publikacii na tu zhe temu >>