Celestial hemisphere:  Northern  ·  Constellation: Hercules (Her)  ·  Contains:  M 92  ·  NGC 6332  ·  NGC 6341
Getting plate-solving status, please wait...
M92 and a slew of galaxies, riot1013
M92 and a slew of galaxies
Powered byPixInsight

M92 and a slew of galaxies

Getting plate-solving status, please wait...
M92 and a slew of galaxies, riot1013
M92 and a slew of galaxies
Powered byPixInsight

M92 and a slew of galaxies

Equipment

Loading...

Acquisition details

Loading...

Description

Messier 92 (also known as M92, M 92, or NGC 6341) is a globular cluster of stars in the northern constellation of Hercules. It was discovered by Johann Elert Bode in 1777, then published in the Jahrbuch during 1779. It was inadvertently rediscovered by Charles Messier in 1781 and added as the 92nd entry in his catalogue. It is about 26,700 light-years away from the solar system.

It is one of the brighter of its sort in apparent magnitude in the northern hemisphere and in its absolute magnitude in the galaxy, but it is often overlooked by amateur astronomers due to angular proximity to dazzling cluster Messier 13, about 20% closer. It is visible to the naked eye under very good conditions.

It is also one of the galaxy's oldest clusters. It is around 16×103 ly (4.9 kpc) above/below the galactic plane and 33×103 ly (10 kpc) from the Galactic Center. The half-light radius, or radius containing the upper half of its light emission, is 1.09 arcminutes, while the tidal radius, the broadest standard measure, is 15.17′. It appears only slightly flattened: its minor axis is about 89% ± 3% of the major.

Comments