Messier 12

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Messier 12
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
Mass8.7×104[5] M
Radius37.2 ly[NB 1]
Metallicity = –1.14
Gyr[3]
Other designationsNGC 6218[7]
See also: Globular cluster, List of globular clusters

Messier 12 or M 12 (also designated NGC 6218) is a

arcminutes) surrounded by a 10 halo of stars.[8]

M12 is roughly 3°

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]

  • Messier 12 core by HST
    Messier 12 core by HST
  • The Central Part of Messier 12. Credit: ESO
    The Central Part of Messier 12. Credit:
    ESO
  • Map showing the location of M12
    Map showing the location of M12

See also

  • List of Messier objects

Notes

  1. ^ distance × sin( diameter_angle / 2 ) = 37.2 ly radius

References

External links