Berkeley 63
(MWSC 177; OCL 346)
0.89
UTI
0.68
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
13.8 [N/pc2]
- CN 0.68 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Berkeley 63 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is very 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 | 34.858 | 63.717 | 0.186 | -1.006 | 0.16 | â |
| Almeida et al. | 2025 | 34.86 | 63.72 | â | â | â | â |
| Hunt & Reffert | 2024 | 34.851 | 63.719 | 0.189 | -1.002 | 0.15 | -44.943 |
| Celli et al. | 2024 | 34.858 | 63.718 | â | â | â | â |
| Cavallo et al. | 2024 | 34.866 | 63.715 | 0.189 | â | â | â |
| Hunt & Reffert | 2023 | 34.851 | 63.719 | 0.189 | -1.002 | 0.15 | -44.943 |
| Just et al. | 2023 | 34.886 | 63.727 | â | â | â | â |
| Dias et al. | 2021 | 34.86 | 63.72 | 0.168 | -0.952 | 0.195 | â |
| Cantat-Gaudin et al. | 2020 | 34.858 | 63.718 | 0.172 | -0.958 | 0.203 | â |
| Cantat-Gaudin & Anders | 2020 | 34.858 | 63.718 | 0.172 | -0.958 | 0.203 | â |
| Soubiran et al. | 2018 | 34.858 | 63.718 | â | â | â | -49.26 |
| Bica et al. | 2019 | 34.875 | 63.704 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 34.858 | 63.718 | 0.172 | -0.958 | 0.203 | â |
| Loktin & Popova | 2017 | 34.905 | 63.717 | â | -2.092 | 2.164 | â |
| Kharchenko et al. | 2016 | 34.886 | 63.727 | â | â | â | â |
| Dias et al. | 2014 | 34.9 | 63.717 | â | -0.06 | 2.83 | â |
| Kharchenko et al. | 2013 | 34.899 | 63.73 | â | -2.6 | 2.98 | â |
| Kharchenko et al. | 2012 | 34.899 | 63.73 | â | -2.6 | 2.98 | â |
| Dias et al. | 2002 | 34.9 | 63.717 | â | -0.06 | 2.83 | 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 | 4.66 | 2.635 | 1.76 | 32 | 0.328 | 587 | â | â |
| Almeida et al. | 2025 | 4.57 | 2.63 | â | 10 | â | 339 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1085(1) | â | â |
| Celli et al. | 2024 | â | â | â | 18 | â | 622 | â | â |
| Cavallo et al. | 2024 | 4.94 | 2.37 | â | 141 | 0.850 | â | â | â |
| Hunt & Reffert | 2023 | 4.66 | 2.64 | 1.76 | 33 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 794 | â | 552 | â | â |
| Dias et al. | 2021 | 4.57 | 2.63 | â | 10 | -0.194 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 5.42 | 2.52 | â | 18 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.97 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 4.97 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.97 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.47 | 2.08 | â | 25 | â | â | â | â |
| Kharchenko et al. | 2016 | 3.99 | 2.84 | â | 794 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.99 | 2.84 | â | 794 | â | â | â | â |
| Kharchenko et al. | 2012 | 3.99 | 2.84 | â | 794 | â | â | â | â |
| Dias et al. | 2002 | 5.70 | 2.98 | â | 30 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.