- Source: Palomar 5
5.180.24.3/info/palomar" target="_blank">Palomar 5 is a globular cluster and a member of the 5.180.24.3/info/palomar" target="_blank">Palomar Globular Clusters group. It was discovered by Walter Baade in 1950, and independently found again by Albert George Wilson in 1955. After the initial name of Serpens, it was subsequently catalogued as 5.180.24.3/info/palomar" target="_blank">Palomar 5.
There is a process of disruption acting on this cluster because of the gravitation of the Milky Way – in fact there are many stars leaving this cluster in the form of a stellar stream. The stream has a mass of 5000 solar masses and is 30,000 light years long. The cluster is currently 60.6 kly (18.6 kpc) from the Galactic Center. It shows a noticeable amount of flattening, with an aspect ratio of 0.62 ± 0.23 between its semimajor axis and semiminor axis.
See also
List of globular clusters
List of stellar streams
References
External links
SEDS 5.180.24.3/info/palomar" target="_blank">Palomar 5
5.180.24.3/info/palomar" target="_blank">Palomar 5 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
Gieles, Mark; Erkal, Denis; Antonini, Fabio; Balbinot, Eduardo; Peñarrubia, Jorge (2021), N-body simulation of the Galactic globular cluster 5.180.24.3/info/palomar" target="_blank">Palomar 5 and its stream, arXiv:2102.11348, doi:10.1038/s41550-021-01392-2, S2CID 256703405, archived from the original on 2021-12-18, retrieved 2021-07-08
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