| NGC 6325 | |
|---|---|
 NGC 6325 as seen through the
Hubble Space Telescope | |
| Observation data ( J2000 epoch) | |
| Class | IV [1] |
| Constellation | Ophiuchus |
| Right ascension | 17h 17m 59.27s [2] |
| Declination | −23° 45′ 57.7″ [2] |
| Distance | 25,400 ly (7,800 pc) [1] |
| Apparent magnitude (V) | 10.33 [3] |
| Apparent dimensions (V) | 4.3′ × 4.3′ [1] |
| Physical characteristics | |
| Metallicity | = -1.25 [3] dex |
| Other designations | GCl 58, ESO 519-11 [2] |
![{\displaystyle {\begin{smallmatrix}\left[{\ce {Fe}}/{\ce {H}}\right]\end{smallmatrix}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/4c0821bd80891e071c08e7c7ee8e022baedf522c)
NGC 6325 is a globular cluster located in the constellation Ophiuchus. Its Shapley-Sawyer Concentration Class is IV, meaning that it has "intermediate rich concentration"; it was discovered by the British astronomer John Herschel on 24 May 1835. It is at a distance of about 25,000 light years away from Earth. [4]
See also
References
- ^ a b c Hartmut Frommert. "NGC 6325 - Hartmut Frommert - SEDS". SEDS. Retrieved 6 February 2017.
- ^ a b c "NGC 6325". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 8 February 2017.
- ^ a b William E. Harris. "Catalog of Parameters for Milky Way Globular Clusters". Retrieved 3 February 2017.
- ^ "NGC 6325 (= GCL 58)". cseligman. Retrieved 8 February 2017.
External links
-
Media related to
NGC 6325 at Wikimedia Commons
 | This star cluster–related article is a stub. You can help Wikipedia by expanding it. |