Explanation: East of Antares, dark markings sprawl through crowded star fields toward the center of our Milky Way Galaxy. Cataloged in the early 20th century by astronomer E. E. Barnard, the obscuring interstellar dust clouds include B59, B72, B77 and B78, seen in silhouette against the starry background. Here, their combined shape suggests a pipe stem and bowl, and so the dark nebula's popular name is the Pipe Nebula. The deep and expansive view was represents nearly 24 hours of exposure time recorded in very dark skies of the Chilean Atacama desert. It covers a full 10 by 10 degree field in the pronounceable constellation Ophiuchus. The Pipe Nebula is part of the Ophiuchus dark cloud complex located at a distance of about 450 light-years. Dense cores of gas and dust within the Pipe Nebula are collapsing to form stars.

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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: dark nebula - Pipe Nebula - temnaya tumannost' Publikacii so slovami: dark nebula - Pipe Nebula - temnaya tumannost'
Sm. takzhe: IC 348 i Barnard 3 LDN 43: tumannost' Kosmicheskaya Letuchaya Mysh' Temnaya bashnya v Skorpione Temnye tumannosti v Hameleone Tumannost' "Temnaya shtuchka" LBN 86: tumannost' Skat-orlyak Tumannost' Konskaya Golova Vse publikacii na tu zhe temu >>