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Pipe Nebula
The Pipe Nebula (also known as Barnard 59, 65–67, and 78) is a dark nebula in the Ophiuchus constellation and a part of the Dark Horse Nebula. It is a large but readily apparent pipe shaped dust lane that obscures the Milky Way star clouds behind it. Clearly visible to the naked eye in the Southern United States under clear dark skies, but it is best viewed with 7x binoculars.
The nebula has two main parts: the Pipe Stem with an opacity of 6 which is composed of Barnard 59, 65, 66, and 67 (also known as LDN 1773) 300′ x 60′ RA: 17h 21m Dec: −27° 23′; and the Bowl of the Pipe with an opacity of 5 which is composed of Barnard 78 (also known as LDN 42) 200′ x 140′ RA: 17h 33m Dec: −26° 30′.
==Gallery==
File:Guisard - Milky Way.jpg|The Milky Way between Sagittarius and Scorpius: the Pipe Nebula is visible slightly above and left of center.
File:Laser Towards Milky Ways Centre.jpg|View of the Milky Way and the Great Rift from ESO's Very Large Telescope in Cerro Paranal, Chile. The laser beam points almost directly toward the Pipe Nebula.
抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』
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