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Messier 69

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Messier 69

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Also known as M69

Globular cluster

Key facts

Class
V
Constellation
Sagittarius
Right ascension
18 31 23.10
Declination
−32 ° 20 ′ 53.1 ″
Distance
29 kly (8.8 kpc)
Apparent dimensions v
10.8 ′
Mass
2.0 × 10 M ☉ M ☉
Radius
45 ly
Tidal radius
91.9 ly.
Metallicity
[ Fe/H ] = –0.78 dex
Estimated age
13.06 Gyr
Other designations
GCl 96, M69, NGC 6637, NGC 6634

via Wikipedia infobox

Wikidata facts

Distance from Earth
28700
Radius
25
Image
Messier 69 Hubble WikiSky.jpg
Show 13 more facts
Commons category
Messier 69
catalog code
[KPS2012] MWSC 2936
apparent magnitude
7.306
Commons gallery
Messier 69
time of discovery or invention
1780-08-31
radial velocity
39.1
absolute magnitude
-7.64
metallicity
-0.78
spectral class
XI
right ascension
277.846250
declination
-32.348083
right ascension component of proper motion
1.59
declination component of proper motion
-2.27
Sources (2)

via Wikidata · CC0

~1 min read

Article

Messier 69 or M69, also known NGC 6637, and NGC 6634, 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 5,200 ly from the Galactic Center, with a spatial radius of 45 light-years. It is a relatively metal-rich globular cluster that is a likely member of the galactic bulge population. It has a mass of 200000 M☉ with a half-mass radius of 11.6 ly, a core radius of 29.2 ly, and a tidal radius of 91.9 ly. Its center has a bright luminosity density of 6,460 L☉·pc (meaning per cubic parsec). It is a close neighbor of its analog M70 – possibly only 1,800 light-years separates the two.

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