Release 7.11 ("Paola")

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Your query: M 12

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Parameters
Positional Parameters
clusterNGC 6218
nameM 12
RA16 47 14.
Declination-01 56 52
Galactic longitude15.72
Galactic latitude26.31
R sun4.9
R gc4.5
X4.2
Y1.2
Z2.2
Photometric Parameters
E (B-V)0.19
V HB14.6
(m-M)14.02
Vt6.7
MVt-7.32
(U-B)0.2
(B-V)0.83
(V-R)0.56
(V-I)1.14
S_RR0
HBR0.97
hbt1
Structural Parameters
[Fe / H]-1.48
SpT F8
v_r-42.2
err0.5
v_LSR-26.4
c1.39
r_c0.72
r_h2.16
r_t17.6
lg(tc)8.1
lg(th)9.02
mu_V18.17
rho_v3.23
Color-magnitude diagrams
authorSato, Takashi; Richer, Harvey B.; Fahlman, Gregory G.
titleDeep CCD photometry in globular clusters. VIII - M12
journalAstronomical Journal, vol. 98, Oct. 1989, p. 1335-1353
CM diagram
Description of NGC 6218

Messier 12 (also known as M12, Globular Cluster M12 or NGC 6218) is a globular cluster in the constellation Ophiuchus. It was discovered by Charles Messier on May 30, 1764.

Located roughly 3 degrees from the cluster M10, M12 is about 16,000 light-years distant and has a spatial diameter of ~75 light-years. The brightest stars of M12 are of 12th magnitude. It is rather loosely packed for a globular and M12 was once thought to be a tightly concentrated open cluster. Thirteen variable stars have been recorded in this cluster.

Source: Wikipedia | Notify inaccuracies

DSS image

Image of the cluster from the Digital Sky Survey

Other Resources
for NGC 6218
Globular Clusters Blog
ADS "Object Search"
C. Clement variables data
SEDS data
Google Sky
Web Links for this cluster
(1 link in the database at the moment)
Users comments for this cluster
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Selected biblio
Paper n. 1
Sato, Takashi; Richer, Harvey B.; Fahlman, Gregory G.
Deep CCD photometry in globular clusters. VIII - M12
Astronomical Journal, vol. 98, Oct. 1989, p. 1335-1353
(NGC 6218 cmd )
See all items (1 paper)

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