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Encyclopedia > Messier 27
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Messier Object 27, the Dumbbell Nebula

The Dumbbell Nebula (also known as Messier Object 27, M27, or NGC 6853) is a planetary nebula in the Vulpecula constellation, at a distance of about 1250 light years.


This object was the first planetary to be discovered; by Charles Messier in 1764. At its brightness of visual magnitude 7.4 and its diameter of about 8 arcminutes, it is easily visible in binoculars, and a great observing target in amateur telescopes.


It is estimated that the Dumbbell Nebula is 3,000 to 4,000 years old.


Related topics

External links

  • SEDS Messier page on M27 (http://www.seds.org/messier/m/m027.html)

  Results from FactBites:
 
Sea and Sky's Astronomy Resources: Messier Objects M101 - M110 (898 words)
M104 is characterized by a dark dust lane that spans the length of the galaxy's disk.
It was discovered by Messier's colleague, Pierre Mechain, in 1782 and was not included in the original publication of the catalog.
M110 was discovered by Messier in 1783 when he discovered M31, but it was not included in his catalog at the time.
M27, Messier 27, Dumbell Nebula (363 words)
Messier 27 is considered by many to be the finest planetary nebula in the sky.
Messier 27 is estimated to be approximately 1.5 light years wide [easily encompassing our entire solar system].
The visible part of Messier 27 is an expanding shell of stellar material that is set aglow by the central star which has since become a very strong source of ultraviolet radiation.
  More results at FactBites »


 

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