Ruprecht 83
(VDBH80; FSR 1508; MWSC 1718; OCL 791; vdBergh-Hagen 80; ESO 167 07)
0.96
UTI
0.81
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
2.4 [arcmin]
- CN 0.81 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 83 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near 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 age and metallicity parameters (see Parameters). It is very well-studied in the literature.
Note: This object shares a small percentage of members with 4 later reported entries. See table with shared members information.
Distant
Moderate extinction
Massive
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 147.315 | -54.608 | 0.253 | -4.607 | 2.892 | 25.151 |
| Li et al. | 2025 | 147.307 | -54.611 | 0.217 | -4.639 | 2.897 | â |
| Almeida et al. | 2025 | 147.31 | -54.609 | â | â | â | â |
| Hunt & Reffert | 2024 | 147.325 | -54.606 | 0.259 | -4.613 | 2.886 | 24.314 |
| Cavallo et al. | 2024 | 147.314 | -54.596 | 0.252 | â | â | â |
| Hunt & Reffert | 2023 | 147.325 | -54.606 | 0.259 | -4.613 | 2.886 | 24.314 |
| Just et al. | 2023 | 147.325 | -54.608 | â | â | â | â |
| Dias et al. | 2021 | 147.31 | -54.609 | 0.219 | -4.633 | 2.923 | 24.615 |
| Cantat-Gaudin et al. | 2020 | 147.307 | -54.611 | 0.217 | -4.639 | 2.897 | â |
| Cantat-Gaudin & Anders | 2020 | 147.307 | -54.611 | 0.217 | -4.639 | 2.897 | â |
| Soubiran et al. | 2018 | 147.307 | -54.611 | â | â | â | 24.75 |
| Bica et al. | 2019 | 147.316 | -54.59 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 147.307 | -54.611 | 0.217 | -4.639 | 2.897 | â |
| Loktin & Popova | 2017 | 147.315 | -54.6 | â | -9.655 | 0.943 | â |
| Kharchenko et al. | 2016 | 147.325 | -54.608 | â | â | â | â |
| Dias et al. | 2014 | 147.312 | -54.6 | â | -5.1 | -1.4 | â |
| Kharchenko et al. | 2013 | 147.33 | -54.612 | â | -8.44 | 3.27 | â |
| Froebrich et al. | 2007 | 147.317 | -54.606 | â | â | â | â |
| van den Bergh | 2006 | 147.278 | -54.569 | â | â | â | â |
| Dias et al. | 2002 | 147.312 | -54.6 | â | -5.1 | -1.4 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 3.05 | 2.61 | â | 725 | -0.145 | â | â | â |
| Almeida et al. | 2025 | 3.11 | 2.58 | â | 153 | â | 792 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2079* | â | â |
| Cavallo et al. | 2024 | 3.47 | 2.84 | â | 251 | 0.490 | â | â | â |
| Hunt & Reffert | 2023 | 3.54 | 2.98 | 2.20 | 102 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 3 | â | 1607 | â | â |
| Dias et al. | 2021 | 3.11 | 2.58 | â | 153 | 0.151 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.70 | 2.38 | â | 112 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.06 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 4.06 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.06 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.54 | 1.44 | â | 290 | â | â | â | â |
| Kharchenko et al. | 2016 | 6.02 | 3.87 | â | 3 | â | â | â | â |
| Kharchenko et al. | 2013 | 6.02 | 3.87 | â | 3 | â | â | â | â |
| van den Bergh | 2006 | 2.46 | 1.40 | â | 282 | â | â | â | â |
| Dias et al. | 2002 | 2.46 | 1.40 | â | 282 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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