- Source: Palomar 6
Palomar 6 is a loose globular cluster in the constellation Ophiuchus that belongs to the Milky Way galaxy. It is a member of the Palomar Globular Clusters group. It is located about 25,000 light-years (7,700 parsecs) away from the Sun. It formed in what would become the bulge of the Milky Way. It is similar to other old-bulge globular clusters such as Messier 62, NGC 6522, NGC 6558, and Haute-Provence 1.
First discovered on the National Geographic Society – Palomar Observatory Sky Survey plates by Robert G. Harrington and Fritz Zwicky,
it was catalogued as a globular cluster, and is one of four globulars known to contain a planetary nebula.
References
External links
Media related to Palomar 6 at Wikimedia Commons
Simbad reference data
SEDS: Palomar 6, Capricornus Dwarf
Palomar 6 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
NASA Astronomy Picture of the Day: Palomar 6: Globular Star Cluster (19 October 2021)
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