An Etymological Dictionary of Astronomy and Astrophysics

English-French-Persian

فرهنگ ریشه‌شناختی اخترشناسی-اخترفیزیک



Pipe Nebula
  میغ ِ پیپ  
miq-e pip
Fr.: Nébuleuse de la Pipe  

An extended complex of → molecular clouds in the constellation → Ophiuchus, apparently shaped like a smoker’s pipe, about 5° in size and located about 5° away from the → Galactic center. It has a mass of 104 solar masses, lies at a distance of about 130 pc, and is among the closest molecular clouds to Earth. The Pipe Nebula includes a number of → dark nebulae, including Barnard 59, 65, 66, 67, 77, 244, and 256. It is of particular interest because of the almost complete lack of
star formation within it. This cloud is an extremely rare example of a relatively massive molecular cloud that may be in a state of evolution prior to the onset of significant star-forming activity.

See also:pipe; → nebula.