NGC 6362
| NGC 6362 | |
|---|---|
| Apparent magnitude (V) | +8.3[4] |
| Apparent dimensions (V) | 9' |
| Physical characteristics | |
| Metallicity | = –0.99 Gyr[5] |
| Other designations | GCl 66, C 1726-670[6] |
![{\displaystyle {\begin{smallmatrix}\left[{\ce {Fe}}/{\ce {H}}\right]\end{smallmatrix}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/4c0821bd80891e071c08e7c7ee8e022baedf522c)
NGC 6362 is a
Gallery
-
![Detailed view of NGC 6362 globular cluster.[10]](//upload.wikimedia.org/wikipedia/commons/thumb/c/c6/NGC_6362_globular_cluster_HST.jpg/120px-NGC_6362_globular_cluster_HST.jpg)
Detailed view of NGC 6362 globular cluster.[10]
![Detailed view of NGC 6362 globular cluster.[10]](/File:NGC_6362_globular_cluster_HST.jpg)
References
- Bibcode:1927BHarO.849...11S.
- ^ S2CID 119183070.
- S2CID 120965440.
- ^ ISBN 978-0-00-717223-8.
- ^ S2CID 51825384.
- ^ "NGC 6362". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-19.
- ^ Atkinson, Nancy (2012-10-31). "Beautiful Star Cluster Looks Surprisingly Youthful". University Today. Retrieved 29 November 2012.
- ^ "Dazzling star cluster holds some deceptively young stars". space on NBCnews.com. space.com. Retrieved 29 November 2012.
- ^ "Hubble Sees an Unexpected Population of Young-Looking Stars". Hubble telescope. nasa.gov. Retrieved 29 November 2012.
- ^ "An unexpected population of young-looking stars". ESA/Hubble Picture of the Week. Retrieved 12 November 2012.
External links
Media related to NGC 6362 at Wikimedia Commons
