NGC 6717 (also known as Palomar 9) is a globular cluster in the constellation Sagittarius, and is a member of the Palomar Globular Clusters group. Palomar 9 was discovered by William Herschel on August 7, 1784. It is located about 7,300 parsecs away from Earth.[2]
| NGC 6717 | |
|---|---|
 Hubble Space Telescope image of NGC 6717 | |
| Observation data (J2000 epoch) | |
| Constellation | Sagittarius |
| Right ascension | 18h 55m 06.04s[1] |
| Declination | −22° 42′ 05.3″[1] |
| Distance | 23.8 ± 1.6 kly (7.3 ± 0.5 kpc)[2] |
| Apparent magnitude (V) | +9.28[3] |
| Physical characteristics | |
| Other designations | NGC 6717, Cr 395, ESO 523-14, GCl 105[1] |
The globular cluster, which has an apparent magnitude of 9.28 and diameter of 9.9 arcminutes, is located just south of the star ν2 Sagittarii. The bright star region on the north-eastern edge has the separate designation IC 4802.
References
edit- ^ a b c "NGC 6717". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 30 December 2016.
- ^ a b Oliveira, R. A. P.; Ortolani, S.; Barbuy, B.; Kerber, L. O.; Maia, F. F. S.; Bica, E.; Cassisi, S.; Souza, S. O.; Pérez-Villegas, A. (2022). "Precise distances from OGLE-IV member RR Lyrae stars in six bulge globular clusters". Astronomy & Astrophysics. 657: A123. arXiv:2110.13943. Bibcode:2022A&A...657A.123O. doi:10.1051/0004-6361/202141596. S2CID 239998638.
- ^ Frommert, Hartmut. "NGC 6717, Palomar 9". seds.org. Retrieved 30 December 2016.
External links
edit
 | This star cluster–related article is a stub. You can help Wikipedia by expanding it. |