Messier 12
![Sky map](http://upload.wikimedia.org/wikipedia/commons/thumb/e/e4/Jupiter_and_moon.png/20px-Jupiter_and_moon.png)
Messier 12 | |
---|---|
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 Gyr[3] |
Other designations | NGC 6218[7] |
Messier 12 or M 12 (also designated NGC 6218) is a
M12 is roughly 3°
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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Messier 12 core by HST
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The Central Part of Messier 12. Credit:ESO
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Map showing the location of M12
See also
- List of Messier objects
Notes
- ^ distance × sin( diameter_angle / 2 ) = 37.2 ly radius
References
- ^ Bibcode:1927BHarO.849...11S.
- ^ S2CID 119183070.
- ^ .
- ^ "Messier 12". SEDS Messier Catalog. Archived from the original on 1 July 2022. Retrieved 27 April 2022.
- S2CID 118652005. Mass is from MPD on Table 1.
- S2CID 51825384.
- ^ "M 12". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2006-11-15.
- ^ ISBN 978-0596526856.
- ^ ISBN 978-1441968500.
- ^ ISBN 978-0521553322.
- ^ "Messier 12: Gumball Globular | Messier Objects". www.messier-objects.com. 11 March 2015. Retrieved 2015-08-17.
- ESO, February 7, 2006, archived from the originalon February 8, 2007.
External links
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