| Messier 69 | |
| Class: | V |
| Dist Ly: | 8.8order=flipNaNorder=flip |
| Appmag V: | 7.6[1] |
| Size V: | 10.8 |
| Radius Ly: | 45 ly[2] |
| Radius Tidal Ly: | 28.17abbr=onNaNabbr=on. |
| Metal Fe: | –0.78 |
| Names: | GCl 96, M69, NGC 6637 |
Messier 69 or M69, also known NGC 6637, is a globular cluster in the southern constellation of Sagittarius. It can be found 2.5° to the northeast of the star Epsilon Sagittarii and is dimly visible in 50 mm aperture binoculars. The cluster was discovered by Charles Messier on August 31, 1780, the same night he discovered M70. At the time, he was searching for an object described by Nicolas-Louis de Lacaille in 1751 - 2 and thought he had rediscovered it, but it is unclear if Lacaille actually described M69.
This cluster is about 28,700 light-years away from Earth and 1.6kpc from the Galactic Center, with a spatial radius of 45 light-years.[2] It is a relatively metal-rich globular cluster that is a likely member of the galactic bulge population. It has a mass of with a half-mass radius of 3.56abbr=onNaNabbr=on, a core radius of 8.94abbr=onNaNabbr=on, and a tidal radius of 28.17abbr=onNaNabbr=on. Its center has a bright luminosity density of ·pc−3 (meaning per cubic parsec). It is a close neighbor of its analog M70 - possibly only 1,800 light-years separates the two.