Berkeley 85
(MWSC 3311; Dolidze 41; OCL 160; OCL 163; FSR 0208; MWSC 3309)
0.96
UTI
1.0
CN
1.0
Cdens
1.0
CC3
0.9
Clit
1.0
Cdup
Nm (P>50%)
687
Core radius and density
2.4 [pc], 9.7 [pc-2]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.9 Very well-studied
- Cdup 1.0 Unique
Overview
Berkeley 85 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the absorption, age, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 304.697 | 37.744 | 0.243 | -2.937 | -4.678 | -34.091 |
| Otto et al. | 2026 | 304.699 | 37.731 | â | -2.94 | -4.68 | -34.2 |
| Almeida et al. | 2025 | 304.694 | 37.75 | â | â | â | â |
| Hunt & Reffert | 2024 | 304.699 | 37.731 | 0.249 | -2.953 | -4.673 | -26.033 |
| Cavallo et al. | 2024 | 304.701 | 37.746 | 0.244 | â | â | â |
| Hunt & Reffert | 2023 | 304.699 | 37.731 | 0.249 | -2.953 | -4.673 | -26.033 |
| Just et al. | 2023 | 304.682 | 37.727 | â | â | â | â |
| Jadhav & Subramaniam | 2021 | 304.692 | 37.744 | â | â | â | â |
| Dias et al. | 2021 | 304.694 | 37.75 | 0.216 | -2.947 | -4.677 | -33.478 |
| Cantat-Gaudin et al. | 2020 | 304.692 | 37.744 | 0.22 | -2.94 | -4.677 | â |
| Zhong et al. | 2020 | 304.692 | 37.744 | â | -2.94 | -4.677 | -35.612 |
| Cantat-Gaudin & Anders | 2020 | 304.692 | 37.744 | 0.22 | -2.94 | -4.677 | â |
| Monteiro & Dias | 2019 | 304.704 | 37.75 | â | -2.934 | -4.678 | 2.322 |
| Soubiran et al. | 2018 | 304.692 | 37.744 | â | â | â | -33.72 |
| Bica et al. | 2019 | 304.712 | 37.737 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 304.692 | 37.744 | 0.22 | -2.94 | -4.677 | â |
| Dias et al. | 2018 | â | â | â | -2.91 | -5.33 | â |
| Dib et al. | 2018 | 304.687 | 37.73 | â | â | â | â |
| Loktin & Popova | 2017 | 304.725 | 37.758 | â | -0.945 | -0.945 | -1.0 |
| Sampedro et al. | 2017 | 304.729 | 37.759 | â | -0.36 | -0.32 | â |
| Joshi et al. | 2016 | 304.687 | 37.73 | â | â | â | â |
| Kharchenko et al. | 2016 | 304.682 | 37.727 | â | â | â | â |
| Tadross | 2014 | 304.704 | 37.75 | â | â | â | â |
| Dias et al. | 2014 | 304.729 | 37.759 | â | -1.45 | -1.52 | â |
| Kharchenko et al. | 2013 | 304.687 | 37.73 | â | -3.52 | -2.78 | â |
| Bukowiecki et al. | 2011 | 304.688 | 37.721 | â | â | â | â |
| Dias et al. | 2002 | 304.729 | 37.759 | â | -1.45 | -1.52 | â |
| Lynga | 1987 | 304.719 | 37.709 | â | â | â | 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 | 3.3 | 2.77 | 2.48 | 417 | 0.060 | 3237 | â | 1 |
| Otto et al. | 2026 | â | â | â | 417 | 0.060(15) | â | â | â |
| Liu et al. | 2025 | 9.38 | 1.11 | â | 224 | â | â | â | â |
| Almeida et al. | 2025 | 3.00 | 3.07 | â | 242 | â | 3237 | â | â |
| Hunt & Reffert | 2024 | 3.71 | 3.83 | 2.48 | 80 | â | 8390(1) | â | â |
| Cavallo et al. | 2024 | 3.24 | 3.75 | â | 182 | 0.240 | â | â | â |
| Hunt & Reffert | 2023 | 3.71 | 3.83 | 2.48 | 80 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1161 | â | 2234 | â | â |
| Jadhav & Subramaniam | 2021 | 3.53 | 2.77 | â | 417 | â | 5086 | â | 1(1) |
| Dias et al. | 2021 | 3.00 | 3.07 | â | 242 | 0.424 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.53 | 2.77 | â | 417 | â | â | â | â |
| Kounkel et al. | 2020 | 3.57 | 3.14 | â | 219 | â | â | â | â |
| Zhong et al. | 2020 | 4.02(1) | 2.43 | â | 9065 | 0.000 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.02 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 3.36 | 3.38 | â | 335 | 0.013 | â | â | â |
| Soubiran et al. | 2018 | 4.02 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.02 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 1.76 | â | â | 1161 | â | â | â | â |
| Loktin & Popova | 2017 | 3.07 | 2.63 | â | 759 | â | â | â | â |
| Joshi et al. | 2016 | 1.76 | 2.43 | â | 1161 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.76 | 2.43 | â | 1161 | â | â | â | â |
| Tadross | 2014 | 1.76 | 1.67 | â | 400 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.76 | 2.43 | â | 1161 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 3155 | â | â |
| Bukowiecki et al. | 2011 | 2.18(1) | 3.00 | â | 355 | â | â | â | â |
| Dias et al. | 2002 | 1.76 | 2.43 | â | 1000 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as hyperbolic encounter pair 34 along with Gulliver_23.
Palma et al. (2025)
Part of multiple system G94, along with UBC_1100 and Gulliver_23.
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.80 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.80 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.1392, e_all=0.1208.
Bica et al. (2019)
Analysis of Dolidze objects by M. Kronberger reported in DAML02.