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The Pipe Dark Nebula
<< Yesterday 21.06.1997 Tomorrow >>
The Pipe Dark Nebula
Credit & Copyright: Jerry Lodriguss
Explanation: The dark nebula predominant at the lower left of the above photograph is known as the Pipe Nebula. The dark clouds, suggestively shaped like smoke rising from a pipe, are caused by absorption of background starlight by dust. These dust clouds can be traced all the way to the Rho Ophiuchi nebular clouds on the right. The brightest star in the field is Antares. Many types of nebula are highlighted here: the red are emission nebula, the blue are reflection nebula, and the dark are absorption nebula. This picture has been digitally enhanced.

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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.

Russkii tekst
Based on Astronomy Picture Of the Day
Publikacii s klyuchevymi slovami: dark nebula - otrazhatel'nye tumannosti - temnaya tumannost' - emissionnaya tumannost'
Publikacii so slovami: dark nebula - otrazhatel'nye tumannosti - temnaya tumannost' - emissionnaya tumannost'
Sm. takzhe:
Vse publikacii na tu zhe temu >>

Ocenka: 3.1 [golosov: 54]
 
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