Celestial hemisphere:  Northern  ·  Constellation: Hercules (Her)  ·  Contains:  M 92  ·  NGC 6341
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M92, jrtb
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M92

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M92, jrtb
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M92

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Description

Messier 92 (M92) is a globular cluster located in the constellation Hercules. Here are some key facts about Messier 92:
  1. Discovery: Johann Elert Bode discovered M92 in 1777, and it was later independently rediscovered by Charles Messier in 1781. As a result, it was included as the 92nd entry in Messier's catalog of non-stellar objects.
  2. Location: Messier 92 is situated in the northern celestial hemisphere, within the constellation Hercules. It is relatively close to another globular cluster, Messier 13 (M13), which is more famous and easier to observe due to its brightness.
  3. Physical Characteristics: M92 is one of the older globular clusters, estimated to be around 14 billion years old. It is composed of a large number of stars densely packed together in a roughly spherical shape. The cluster contains a significant population of variable stars, including RR Lyrae variables.
  4. Distance: The estimated distance to Messier 92 from Earth is approximately 26,700 light-years.
  5. Apparent Magnitude: M92 has an apparent magnitude of about 6.3, making it visible to the naked eye under dark skies. However, it is best observed with binoculars or a telescope, where individual stars within the cluster become discernible.
  6. Observation: Messier 92 is a popular target for amateur astronomers. It is often compared to Messier 13, another globular cluster in Hercules, for its interesting features and differences in appearance.
  7. Globular Cluster Characteristics: Globular clusters like M92 are dense, spherical collections of stars that orbit the galactic core as satellites. They are composed of hundreds of thousands to millions of stars bound together by gravity. Globular clusters are typically found in the halos of galaxies.

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M92, jrtb