Messier 12 | |
---|---|
Observation data (J2000 epoch) | |
Class | IX[1] |
Constellation | Ophiuchus |
Right ascension | 16h 47m 14.18s[2] |
Declination | –01° 56′ 54.7″[2] |
Distance | 16.44 ± 0.16 kly (5.04 ± 0.05 kpc)[3] |
Apparent magnitude (V) | 6.7[4] |
Apparent dimensions (V) | 16.0′ |
Physical characteristics | |
Mass | 8.7×104[5] M☉ |
Radius | 37.2 ly[NB 1] |
Metallicity | = –1.14[6] dex |
Estimated age | 13.8 ± 1.1 Gyr[3] |
Other designations | NGC 6218[7] |
Messier 12 or M 12 (also designated NGC 6218) is a globular cluster in the constellation of Ophiuchus. It was discovered by the French astronomer Charles Messier on May 30, 1764, who described it as a "nebula without stars".[8] In dark conditions this cluster can be faintly seen with a pair of binoculars. Resolving the stellar components requires a telescope with an aperture of 8 in (20 cm) or greater.[9] In a 10 in (25 cm) scope, the granular core shows a diameter of 3′ (arcminutes) surrounded by a 10′ halo of stars.[8]
M12 is roughly 3°[9] northwest from the cluster M10 and 5.6° east southeast from star Lambda Ophiuchi. It is also located near the 6th magnitude 12 Ophiuchi.[10] The cluster is about 16,400 light-years (5,000 parsecs)[3] from Earth and has a spatial diameter of about 75 light-years. The brightest stars of M12 are of 12th magnitude. M10 and M12 are only a few thousand light-years away from each other and each cluster would appear at about magnitude 4.5 from the other.[10] With a Shapley-Sawyer rating of IX,[1] it is rather loosely packed for a globular and was once thought to be a tightly concentrated open cluster. Thirteen variable stars have been recorded in this cluster. M12 is approaching us at a velocity of 16 km/s.[11]
A study published in 2006 concluded that this cluster has an unusually low number of low-mass stars. The authors surmise that they were stripped from the cluster by passage through the relatively matter-rich plane of the Milky Way.[12]
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