Ruprecht 79
(VDBH 77; MWSC 1701; OCL 787; vdBergh-Hagen 77; ESO 167 11; FSR 1502)
0.97
UTI
0.83
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
29.9 [N/pc2]
- CN 0.83 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 79 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, young 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 | 145.263 | -53.845 | 0.243 | -4.599 | 3.028 | 31.004 |
| Li et al. | 2025 | 145.259 | -53.846 | 0.221 | -4.631 | 2.995 | â |
| Almeida et al. | 2025 | 145.259 | -53.847 | â | â | â | â |
| Hunt & Reffert | 2024 | 145.261 | -53.834 | 0.244 | -4.588 | 3.043 | 31.464 |
| Cavallo et al. | 2024 | 145.268 | -53.845 | 0.244 | â | â | â |
| Hunt & Reffert | 2023 | 145.261 | -53.834 | 0.244 | -4.588 | 3.043 | 31.464 |
| Just et al. | 2023 | 145.224 | -53.847 | â | â | â | â |
| Jaehnig et al. | 2021 | 145.266 | -53.836 | 0.256 | -4.626 | 3.001 | â |
| Rain et al. | 2021 | 145.259 | -53.846 | 0.221 | -4.631 | 2.995 | â |
| Dias et al. | 2021 | 145.259 | -53.847 | 0.225 | -4.632 | 2.98 | 29.715 |
| Cantat-Gaudin et al. | 2020 | 145.259 | -53.846 | 0.221 | -4.631 | 2.995 | â |
| Cantat-Gaudin & Anders | 2020 | 145.259 | -53.846 | 0.221 | -4.631 | 2.995 | â |
| Soubiran et al. | 2018 | 145.259 | -53.846 | â | â | â | 29.05 |
| Bica et al. | 2019 | 145.279 | -53.83 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 145.259 | -53.846 | 0.221 | -4.631 | 2.995 | â |
| Loktin & Popova | 2017 | 145.245 | -53.85 | â | -8.142 | -4.46 | 34.9 |
| Kharchenko et al. | 2016 | 145.224 | -53.847 | â | â | â | â |
| Dias et al. | 2014 | 145.246 | -53.85 | â | -3.66 | -0.68 | â |
| Kharchenko et al. | 2013 | 145.23 | -53.85 | â | -7.25 | 1.75 | 34.9 |
| Gozha et al. | 2012 | 145.246 | -53.85 | â | â | â | â |
| Piskunov et al. | 2008 | 145.233 | -53.846 | â | â | â | â |
| Kharchenko et al. | 2007 | 145.24 | -53.85 | â | 0.2 | â | 34.89 |
| van den Bergh | 2006 | 145.25 | -53.85 | â | â | â | â |
| Kharchenko et al. | 2005 | 145.24 | -53.85 | â | -10.35 | 1.24 | 34.89 |
| Kharchenko et al. | 2003 | 145.21 | -53.84 | â | -8.63 | 2.91 | â |
| Dias et al. | 2002 | 145.246 | -53.85 | â | -3.66 | -0.68 | 21.4 |
| Dambis | 1999 | 145.246 | -53.85 | 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 | 3.47 | 2.26 | 2.15 | 38 | 0.076 | 2184 | â | 0.0 |
| Li et al. | 2025 | 3.47 | 2.42 | â | 124 | 0.053 | â | â | â |
| Almeida et al. | 2025 | 3.56 | 2.37 | â | 38 | â | 1401 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2966(1) | â | â |
| Cavallo et al. | 2024 | 2.98 | 2.33 | â | 162 | 0.100 | â | â | â |
| Hunt & Reffert | 2023 | 3.67 | 2.34 | 2.15 | 71 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 18 | â | 273 | â | â |
| Jaehnig et al. | 2021 | 3.94(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 4.00 | 2.20 | â | 12 | â | â | â | 0 |
| Dias et al. | 2021 | 3.56 | 2.37 | â | 38 | 0.107 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.80 | 1.98 | â | 62 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.00 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 4.00 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.00 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.01 | 2.19 | â | 14 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.99 | 2.16 | â | 18 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.99 | 2.16 | â | 18 | â | â | â | â |
| Gozha et al. | 2012 | 1.98 | â | â | 12 | -0.140 | 4677 | â | â |
| Piskunov et al. | 2008 | 1.98 | 2.29 | â | 69 | â | â | â | â |
| van den Bergh | 2006 | 1.98 | 2.23 | â | 12 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.98 | 2.29 | â | 69 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.98 | 2.02 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.98 | 2.22 | â | 12 | â | â | â | â |
| Dambis | 1999 | 3.82 | 2.48 | â | 71 | 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.