Ruprecht 79

(VDBH 77; MWSC 1701; OCL 787; vdBergh-Hagen 77; ESO 167 11; FSR 1502)

Click to load Aladin Lite
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

â„šī¸
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.

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

Cavallo et al. (2024)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 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 –
Almeida et al. 2025 145.259 -53.847 – – – –
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 – – –
Hunt & Reffert 2023 145.261 -53.834 0.244 -4.588 3.043 31.464
Just et al. 2023 145.224 -53.847 – – – –
Jaehnig et al. 2021 145.266 -53.836 0.256 -4.626 3.001 –
Rain et al. 2021 145.259 -53.846 0.221 -4.631 2.995 –
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 –
Cantat-Gaudin & Anders 2020 145.259 -53.846 0.221 -4.631 2.995 –
Soubiran et al. 2018 145.259 -53.846 – – – 29.05
Bica et al. 2019 145.279 -53.83 – – – –
Cantat-Gaudin et al. 2018 145.259 -53.846 0.221 -4.631 2.995 –
Loktin & Popova 2017 145.245 -53.85 – -8.142 -4.46 34.9
Kharchenko et al. 2016 145.224 -53.847 – – – –
Dias et al. 2014 145.246 -53.85 – -3.66 -0.68 –
Kharchenko et al. 2013 145.23 -53.85 – -7.25 1.75 34.9
Gozha et al. 2012 145.246 -53.85 – – – –
Piskunov et al. 2008 145.233 -53.846 – – – –
Kharchenko et al. 2007 145.24 -53.85 – 0.2 – 34.89
van den Bergh 2006 145.25 -53.85 – – – –
Kharchenko et al. 2005 145.24 -53.85 – -10.35 1.24 34.89
Kharchenko et al. 2003 145.21 -53.84 – -8.63 2.91 –
Dias et al. 2002 145.246 -53.85 – -3.66 -0.68 21.4
Dambis 1999 145.246 -53.85 – – – –

💡 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 99999– 3.47 2.26 2.15 38 0.076 2184 – 0.0
Li et al. 2025 3.47 2.42 – 124 0.053 – – –
Almeida et al. 2025 3.56 2.37 – 38 – 1401 – –
Hunt & Reffert 2024 – – – – – 2966(1) – –
Cavallo et al. 2024 2.98 2.33 – 162 0.100 – – –
Hunt & Reffert 2023 3.67 2.34 2.15 71 – – – –
Just et al. 2023 – – – 18 – 273 – –
Jaehnig et al. 2021 3.94(1) – – – – – – –
Rain et al. 2021 4.00 2.20 – 12 – – – 0
Dias et al. 2021 3.56 2.37 – 38 0.107 – – –
Cantat-Gaudin et al. 2020 3.80 1.98 – 62 – – – –
Cantat-Gaudin & Anders 2020 4.00 – – – – – – –
Soubiran et al. 2018 4.00 – – – – – – –
Cantat-Gaudin et al. 2018 4.00 – – – – – – –
Loktin & Popova 2017 2.01 2.19 – 14 – – – –
Kharchenko et al. 2016 1.99 2.16 – 18 – – – –
Kharchenko et al. 2013 1.99 2.16 – 18 – – – –
Gozha et al. 2012 1.98 – – 12 -0.140 4677 – –
Piskunov et al. 2008 1.98 2.29 – 69 – – – –
van den Bergh 2006 1.98 2.23 – 12 – – – –
Kharchenko et al. 2005 1.98 2.29 – 69 – – – –
Kharchenko et al. 2003 1.98 2.02 – – – – – –
Dias et al. 2002 1.98 2.22 – 12 – – – –
Dambis 1999 3.82 2.48 – 71 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

â„šī¸