Berkeley 56
(MWSC 3491; OCL 199; FSR 0269)
0.86
UTI
1.0
CN
1.0
Cdens
0.75
CC3
0.78
Clit
1.0
Cdup
Stellar density (N50/rad)
9.1 [N/pc2]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.78 Well-studied
- Cdup 1.0 Unique
Overview
Berkeley 56 is a very rich, very dense object of high C3 quality. Its parallax locates it at a very large distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an extremely massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 319.401 | 41.824 | 0.07 | -1.911 | -1.843 | -72.787 |
| Hu & Soubiran | 2025 | 319.401 | 41.831 | â | â | â | â |
| Hunt & Reffert | 2024 | 319.385 | 41.828 | 0.095 | -1.895 | -1.865 | -64.266 |
| Cavallo et al. | 2024 | 319.401 | 41.831 | 0.069 | â | â | â |
| Hunt & Reffert | 2023 | 319.385 | 41.828 | 0.095 | -1.895 | -1.865 | -64.266 |
| Just et al. | 2023 | 319.404 | 41.814 | â | â | â | â |
| Perren et al. | 2022 | 319.425 | 41.9 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 319.391 | 41.835 | 0.047 | -1.901 | -1.831 | â |
| Cantat-Gaudin & Anders | 2020 | 319.391 | 41.835 | 0.047 | -1.901 | -1.831 | â |
| Bica et al. | 2019 | 319.413 | 41.848 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 319.391 | 41.835 | 0.047 | -1.901 | -1.831 | â |
| Kharchenko et al. | 2016 | 319.404 | 41.814 | â | â | â | â |
| Dias et al. | 2014 | 319.425 | 41.827 | â | 0.09 | -8.11 | â |
| Kharchenko et al. | 2013 | 319.41 | 41.817 | â | -0.56 | -0.07 | â |
| Dias et al. | 2002 | 319.425 | 41.827 | â | -0.56 | -0.07 | â |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 12.1 | 1.42 | 1.57 | 2732 | -0.340 | 18664 | 0.7 | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.270(5) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 6483(1) | â | â |
| Cavallo et al. | 2024 | 9.64 | 1.63 | â | 5012 | -0.430 | â | â | â |
| Hunt & Reffert | 2023 | 9.05 | 2.06 | 1.57 | 1936 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 2512 | â | 18664 | â | â |
| Perren et al. | 2022 | 11.12 | 1.58 | â | 5248 | -0.340 | 61000 | 0.70 | â |
| Cantat-Gaudin et al. | 2020 | 9.51 | 1.42 | â | 2951 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 13.14 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 13.14 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 13.18 | 0.97 | â | 2512 | â | â | â | â |
| Kharchenko et al. | 2013 | 13.18 | 0.97 | â | 2512 | â | â | â | â |
| Dias et al. | 2002 | 12.10 | 1.24 | â | 3981 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.