description Pipe Nebula (Barnard 78) Overview
The Pipe Nebula is a large, prominent dark cloud complex located in the constellation Ophiuchus, consisting of dense clouds of interstellar dust that obscure the light of background stars. Cataloged by astronomer Edward Emerson Barnard, the complex is recognized for its distinct silhouette, which is divided into two main sections: the bowl and the stem, with the latter officially designated as Barnard 78.
help Pipe Nebula (Barnard 78) FAQ
Where is the Pipe Nebula located in the sky?
The Pipe Nebula is a large dark cloud complex situated in the constellation Ophiuchus. Its dense clouds of interstellar dust effectively obscure the light of background stars, making it a prominent feature against the Milky Way.
Who cataloged the Pipe Nebula?
The nebula complex was cataloged by the pioneering astronomer Edward Emerson Barnard in the early 20th century. His extensive photographic surveys of dark nebulae remain foundational to modern astronomy.
What is Barnard 78 specifically?
Barnard 78 refers specifically to the bowl of the Pipe Nebula. The entire pipe shape is actually made up of multiple dark nebulae, with B78 being the densest part of the interstellar dust cloud.
Can the Pipe Nebula be seen with the naked eye?
Because it is a dark nebula, it is only visible as a silhouette blocking the starlight behind it, requiring very dark skies. It is best observed photographically or with large binoculars under ideal conditions in Ophiuchus.
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