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 1,500 years to reach us from the Horsehead Nebula. The featured image was taken with the large 3.6-m Canada-France-Hawaii Telescope in Hawaii, USA.

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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: tumannost' Konskaya Golova - Horsehead Nebula Publikacii so slovami: tumannost' Konskaya Golova - Horsehead Nebula
Sm. takzhe: Tumannost' Konskaya Golova Tumannost' Oriona i Konskaya Golova Konskaya Golova i Plamya Tumannost' Konskaya Golova v infrakrasnom svete ot teleskopa imeni Habbla Okrestnosti tumannosti Konskaya Golova bez zvezd Tumannosti Konskaya Golova i Plamya Tumannosti Oriona i Konskaya Golova Vse publikacii na tu zhe temu >>