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Encyclopedia > Globular Cluster M92

Globular Cluster M92 (also known as Messier Object 92, Messier 92, M92, or NGC 6341) is a globular cluster in the Hercules constellation. It was discovered by Johann Elert Bode in 1777 and independently rediscovered by Charles Messier on March 18, 1781. M92 is at a distance of about 26,000 light-years away from Earth.


External links

  • Globular Cluster M92 @ SEDS Messier pages (http://www.seds.org/messier/m/m092.html)

  Results from FactBites:
 
Star Clusters - Globular (1802 words)
Globular clusters are not formed within the galaxy structure, but usually large numbers of them form a halo around the main galactic structure.
Globular clusters usually require a larger telescope and higher magnification to observe to best effect, although the larger and closer ones can be spectacular in small instruments.
Stellar concentration is average for a globular cluster and it is one of the metal-richest globulars.
Messier 92 - Wikipedia, the free encyclopedia (143 words)
Messier 92 (also known as M92 or NGC 6341) is a globular cluster in the Hercules constellation.
M92 is at a distance of about 26,000 light-years away from Earth.
M92 is one of the brighter globular clusters in the northern hemisphere, but it is often overlooked by astronomers because of its proximity to the even more spectacular M13.
  More results at FactBites »


 
 

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