Berkeley 55
(MWSC 3490)
0.90
UTI
0.82
CN
1.0
Cdens
1.0
CC3
0.84
Clit
1.0
Cdup
Stellar density (N50/rad)
88.3 [N/pc2]
- CN 0.82 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.84 Well-studied
- Cdup 1.0 Unique
Overview
Berkeley 55 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (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 | 99999β | 319.236 | 51.765 | 0.312 | -4.085 | -4.653 | -45.45 |
| Almeida et al. | 2025 | 319.227 | 51.763 | β | β | β | β |
| Hunt & Reffert | 2024 | 319.235 | 51.761 | 0.325 | -4.086 | -4.68 | -32.001 |
| Cavallo et al. | 2024 | 319.23 | 51.764 | 0.325 | β | β | β |
| Hunt & Reffert | 2023 | 319.235 | 51.761 | 0.325 | -4.086 | -4.68 | -32.001 |
| Just et al. | 2023 | 319.245 | 51.761 | β | β | β | β |
| Dias et al. | 2021 | 319.227 | 51.763 | 0.304 | -4.026 | -4.627 | -42.456 |
| Cantat-Gaudin et al. | 2020 | 319.232 | 51.762 | 0.309 | -4.05 | -4.618 | β |
| SΓ‘nchez et al. | 2020 | 319.242 | 51.759 | β | -3.976 | -4.546 | β |
| Cantat-Gaudin & Anders | 2020 | 319.232 | 51.762 | 0.309 | -4.05 | -4.618 | β |
| Soubiran et al. | 2018 | 319.232 | 51.762 | β | β | β | -43.58 |
| Cantat-Gaudin et al. | 2018 | 319.232 | 51.762 | 0.309 | -4.05 | -4.618 | β |
| Loktin & Popova | 2017 | 319.245 | 51.761 | β | -1.135 | -2.297 | β |
| Kharchenko et al. | 2016 | 319.245 | 51.761 | β | β | β | β |
| Kharchenko et al. | 2013 | 319.249 | 51.765 | β | -3.02 | -7.83 | β |
| Kharchenko et al. | 2012 | 319.249 | 51.765 | β | -3.02 | -7.83 | β |
| Dias et al. | 2002 | 319.242 | 51.759 | β | -5.93 | -12.57 | β |
π‘ 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 | 99999β | 2.85 | 4.96 | 3.07 | 200 | 0.175 | 863 | β | β |
| Almeida et al. | 2025 | 2.58 | 4.16 | β | 130 | β | 863 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 3609(1) | β | β |
| Cavallo et al. | 2024 | 2.96 | 5.17 | β | 47 | 0.010 | β | β | β |
| Hunt & Reffert | 2023 | 2.85 | 5.56 | 3.07 | 63 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 372 | β | 10 | β | β |
| Dias et al. | 2021 | 2.58 | 4.16 | β | 130 | 0.341 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.75 | 4.80 | β | 200 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.96 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 2.96 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.96 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 3.66 | 4.39 | β | 380 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.70 | 4.96 | β | 372 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.70 | 4.96 | β | 372 | β | β | β | β |
| Kharchenko et al. | 2012 | 1.70 | 4.96 | β | 372 | β | β | β | β |
| Dias et al. | 2002 | 3.98 | 5.74 | β | 50 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Silver sample.