Ruprecht 97
(VDBH 124; MWSC 1987; OCL 867; vdBergh-Hagen 124; ESO 130 03)
0.88
UTI
0.76
CN
0.91
Cdens
1.0
CC3
0.87
Clit
1.0
Cdup
Nm (P>50%)
121
Core radius and density
1.8 [pc], 4.5 [pc-2]
- CN 0.76 Rich
- Cdens 0.91 Very dense
- CC3 1.0 Very high quality
- Clit 0.87 Well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 97 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 near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is 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 | 179.373 | -62.71 | 0.252 | -6.503 | 0.489 | -11.456 |
| Otto et al. | 2026 | 179.366 | -62.71 | â | -6.49 | 0.43 | 0.2 |
| Almeida et al. | 2025 | 179.369 | -62.708 | â | â | â | â |
| Hunt & Reffert | 2024 | 179.366 | -62.71 | 0.259 | -6.511 | 0.526 | 5.362 |
| Cavallo et al. | 2024 | 179.372 | -62.704 | 0.259 | â | â | â |
| Hunt & Reffert | 2023 | 179.366 | -62.71 | 0.259 | -6.511 | 0.526 | 5.362 |
| Just et al. | 2023 | 179.338 | -62.707 | â | â | â | â |
| Dias et al. | 2021 | 179.369 | -62.708 | 0.197 | -6.49 | 0.434 | â |
| Spina et al. | 2021 | 179.373 | -62.707 | 0.193 | -6.495 | 0.443 | â |
| Cantat-Gaudin et al. | 2020 | 179.369 | -62.708 | 0.199 | -6.486 | 0.435 | â |
| Cantat-Gaudin & Anders | 2020 | 179.369 | -62.708 | 0.199 | -6.486 | 0.435 | â |
| Soubiran et al. | 2018 | 179.369 | -62.708 | â | â | â | 5.36 |
| Bica et al. | 2019 | 179.367 | -62.706 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 179.369 | -62.708 | 0.199 | -6.486 | 0.435 | â |
| Dias et al. | 2018 | â | â | â | -6.69 | -0.02 | â |
| Dib et al. | 2018 | 179.347 | -62.71 | â | â | â | â |
| Loktin & Popova | 2017 | 179.37 | -62.717 | â | -3.792 | -5.751 | -14.9 |
| Sampedro et al. | 2017 | 179.367 | -62.717 | â | -3.79 | -0.97 | â |
| Joshi et al. | 2016 | 179.347 | -62.71 | â | â | â | â |
| Kharchenko et al. | 2016 | 179.338 | -62.707 | â | â | â | â |
| Dias et al. | 2014 | 179.367 | -62.717 | â | -3.89 | -1.11 | â |
| Kharchenko et al. | 2013 | 179.347 | -62.71 | â | -3.89 | -2.47 | -14.9 |
| Gozha et al. | 2012 | 179.367 | -62.717 | â | â | â | â |
| van den Bergh | 2006 | 179.325 | -62.65 | â | â | â | â |
| Dias et al. | 2002 | 179.367 | -62.717 | â | -3.89 | -1.11 | -14.9 |
| Lynga | 1987 | 179.33 | -62.641 | â | â | â | â |
| van den Bergh & Hagen | 1975 | 178.8 | -62.417 | 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 | 3.21 | 1.065 | 0.75 | 220 | -0.030 | 207 | â | â |
| Otto et al. | 2026 | â | â | â | 178 | 0.080(15) | â | â | â |
| Almeida et al. | 2025 | 3.21 | 1.71 | â | 171 | â | 207 | â | â |
| Hunt & Reffert | 2024 | 3.57 | 1.42 | 0.75 | 166 | â | 688(1) | â | â |
| Cavallo et al. | 2024 | 3.18 | 1.89 | â | 204 | -0.150 | â | â | â |
| Hunt & Reffert | 2023 | 3.57 | 1.43 | 0.75 | 166 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 447 | â | 53 | â | â |
| Spina et al. | 2022 | â | â | â | â | 0.102 | â | â | â |
| Dias et al. | 2021 | 3.21 | 1.71 | â | 171 | 0.011 | â | â | â |
| Spina et al. | 2021 | 4.99 | â | â | 178 | 0.097(20) | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.89 | 1.40 | â | 178 | â | â | â | â |
| Kounkel et al. | 2020 | 4.09 | 1.40 | â | 417 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.40 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 4.40 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.40 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 1.54 | â | â | 447 | â | â | â | â |
| Loktin & Popova | 2017 | 1.33 | 0.71 | â | 228 | â | â | â | â |
| Joshi et al. | 2016 | 1.54 | 0.66 | â | 447 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.54 | 0.66 | â | 447 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.54 | 0.66 | â | 447 | -0.590 | â | â | â |
| Gozha et al. | 2012 | 1.36 | â | â | 220 | -0.220 | â | â | â |
| Paunzen et al. | 2010 | â | â | â | â | -0.220 | â | â | â |
| van den Bergh | 2006 | 1.36 | 0.73 | â | 219 | â | â | â | â |
| Dias et al. | 2002 | 1.36 | 0.72 | â | 220 | -0.030 | â | â | â |
| Lynga | 1987 | 4.00 | 0.63 | â | 1000 | 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: intermediate fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.0937, e_all=0.0969.