Ruprecht 85
(VDBH83; FSR 1520; MWSC 1746; OCL 799; vdBergh-Hagen 83; ESO 167 15)
0.94
UTI
0.85
CN
1.0
Cdens
1.0
CC3
0.94
Clit
1.0
Cdup
Nm (P>50%)
373
Core radius and density
1.5 [pc], 8.5 [pc-2]
- CN 0.85 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.94 Very well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 85 is a rich, very dense object of very high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and mass 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 | 150.36 | -55.111 | 0.182 | -4.419 | 3.241 | 23.451 |
| Otto et al. | 2026 | 150.362 | -55.109 | â | -4.44 | 3.24 | 21.8 |
| Almeida et al. | 2025 | 150.352 | -55.111 | â | â | â | â |
| Hunt & Reffert | 2024 | 150.362 | -55.109 | 0.182 | -4.422 | 3.24 | 39.883 |
| Cavallo et al. | 2024 | 150.347 | -55.11 | 0.181 | â | â | â |
| Hunt & Reffert | 2023 | 150.362 | -55.109 | 0.182 | -4.422 | 3.24 | 39.883 |
| Just et al. | 2023 | 150.415 | -55.011 | â | â | â | â |
| Dias et al. | 2021 | 150.352 | -55.111 | 0.172 | -4.422 | 3.243 | 31.488 |
| Spina et al. | 2021 | 150.363 | -55.111 | 0.177 | -4.424 | 3.239 | â |
| Cantat-Gaudin et al. | 2020 | 150.36 | -55.109 | 0.169 | -4.443 | 3.241 | â |
| Cantat-Gaudin & Anders | 2020 | 150.36 | -55.109 | 0.169 | -4.443 | 3.241 | â |
| Soubiran et al. | 2018 | 150.36 | -55.109 | â | â | â | 22.93 |
| Bica et al. | 2019 | 150.356 | -55.115 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 150.36 | -55.109 | 0.169 | -4.443 | 3.241 | â |
| Dias et al. | 2018 | â | â | â | -3.24 | 1.96 | â |
| Dib et al. | 2018 | 150.42 | -55.015 | â | â | â | â |
| Sampedro et al. | 2017 | 150.358 | -55.117 | â | -5.94 | -0.48 | â |
| Joshi et al. | 2016 | 150.42 | -55.015 | â | â | â | â |
| Kharchenko et al. | 2016 | 150.415 | -55.011 | â | â | â | â |
| Dias et al. | 2014 | 150.358 | -55.117 | â | -6.75 | -0.84 | â |
| Kharchenko et al. | 2013 | 150.42 | -55.015 | â | -4.8 | 4.45 | â |
| Bukowiecki et al. | 2011 | 150.35 | -55.107 | â | â | â | â |
| Piskunov et al. | 2008 | 150.381 | -55.013 | â | â | â | â |
| Froebrich et al. | 2007 | 150.367 | -55.117 | â | â | â | â |
| Kharchenko et al. | 2005 | 150.39 | -55.02 | â | -3.68 | 4.78 | â |
| Kharchenko et al. | 2003 | 150.42 | -55.01 | â | -5.05 | 5.57 | â |
| Dias et al. | 2002 | 150.358 | -55.117 | â | -6.75 | -0.84 | â |
| Lynga | 1987 | 150.426 | -55.045 | â | â | â | â |
| van den Bergh & Hagen | 1975 | 149.975 | -54.8 | 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 | 4.305 | 2.24 | 2.42 | 424 | -0.237 | 947 | â | â |
| Otto et al. | 2026 | â | â | â | 204 | -0.240(15) | â | â | â |
| Almeida et al. | 2025 | 4.33 | 3.08 | â | 223 | â | 1638 | â | â |
| Hunt & Reffert | 2024 | 4.84 | 3.31 | 2.42 | 149 | â | 4853(1) | â | â |
| Cavallo et al. | 2024 | 4.49 | 3.53 | â | 182 | -0.120 | â | â | â |
| Hunt & Reffert | 2023 | 4.84 | 3.31 | 2.42 | 149 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 501 | â | 28 | â | â |
| Spina et al. | 2022 | â | â | â | â | -0.237 | â | â | â |
| Dias et al. | 2021 | 4.33 | 3.08 | â | 223 | 0.010 | â | â | â |
| Spina et al. | 2021 | 4.92 | â | â | 204 | -0.238(20) | â | â | â |
| Cantat-Gaudin et al. | 2020 | 4.81 | 2.61 | â | 204 | â | â | â | â |
| Kounkel et al. | 2020 | 4.28 | 2.76 | â | 347 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 5.04 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 5.04 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 5.04 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 1.29 | â | â | 501 | â | â | â | â |
| Joshi et al. | 2016 | 1.29 | 0.53 | â | 501 | â | 112 | â | â |
| Kharchenko et al. | 2016 | 1.29 | 0.53 | â | 501 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.29 | 0.53 | â | 501 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 947 | â | â |
| Bukowiecki et al. | 2011 | 3.70(1) | 2.24 | â | 501 | â | â | â | â |
| Piskunov et al. | 2008 | 1.40 | 0.66 | â | 501 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.40 | 0.66 | â | 501 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.83 | 0.79 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.40 | 0.66 | â | 501 | 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: good fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.85 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.85 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.1444, e_all=0.0737.