Ruprecht 128
(VDBH 243; MWSC 2672; vdBergh-Hagen 243; OCL 1020; ESO 393 17; FoF 716)
0.89
UTI
0.82
CN
1.0
Cdens
1.0
CC3
0.81
Clit
1.0
Cdup
Nm (P>50%)
284
Core radius and density
0.9 [pc], 21 [pc-2]
- CN 0.82 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.81 Well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 128 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (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 | 266.064 | -34.878 | 0.504 | 1.887 | -1.285 | -39.482 |
| Otto et al. | 2026 | 266.066 | -34.877 | â | 1.89 | -1.26 | -39.8 |
| Li et al. | 2025 | 266.063 | -34.879 | 0.498 | 1.889 | -1.262 | â |
| Hu & Soubiran | 2025 | 266.061 | -34.871 | â | â | â | â |
| Wei et al. | 2025 | 266.069 | -34.88 | 0.516 | 1.895 | -1.278 | â |
| Almeida et al. | 2025 | 266.056 | -34.873 | â | â | â | â |
| Hunt & Reffert | 2024 | 266.066 | -34.877 | 0.494 | 1.88 | -1.281 | -23.391 |
| Cavallo et al. | 2024 | 266.061 | -34.871 | 0.496 | â | â | â |
| Hunt & Reffert | 2023 | 266.066 | -34.877 | 0.494 | 1.88 | -1.281 | -23.391 |
| Almeida et al. | 2023 | 266.059 | -34.872 | â | â | â | â |
| Just et al. | 2023 | 266.06 | -34.885 | â | â | â | â |
| Jadhav & Subramaniam | 2021 | 266.063 | -34.879 | â | â | â | â |
| Dias et al. | 2021 | 266.056 | -34.873 | 0.499 | 1.883 | -1.264 | -39.563 |
| Cantat-Gaudin et al. | 2020 | 266.063 | -34.879 | 0.498 | 1.889 | -1.262 | â |
| Cantat-Gaudin & Anders | 2020 | 266.063 | -34.879 | 0.498 | 1.889 | -1.262 | â |
| Liu & Pang | 2019 | 266.054 | -34.874 | 0.493 | 1.843 | -1.285 | â |
| Soubiran et al. | 2018 | 266.063 | -34.879 | â | â | â | -39.79 |
| Bica et al. | 2019 | 266.106 | -34.931 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 266.063 | -34.879 | 0.498 | 1.889 | -1.262 | â |
| Dias et al. | 2018 | â | â | â | 2.0 | -0.31 | â |
| Sampedro et al. | 2017 | 266.075 | -34.883 | â | 1.92 | -1.22 | â |
| Kharchenko et al. | 2016 | 266.06 | -34.885 | â | â | â | â |
| Dias et al. | 2014 | 266.075 | -34.883 | â | 1.03 | -1.12 | â |
| Kharchenko et al. | 2013 | 266.07 | -34.885 | â | -4.15 | 1.43 | â |
| Dias et al. | 2002 | 266.075 | -34.883 | â | 1.03 | -1.12 | â |
| Lynga | 1987 | 266.062 | -34.875 | â | â | â | â |
| van den Bergh & Hagen | 1975 | 265.225 | -34.85 | 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 | 1.86 | 3.01 | 2.53 | 955 | -0.102 | 1118 | 0.69 | 0 |
| Otto et al. | 2026 | â | â | â | 955 | 0.130(15) | â | â | â |
| Li et al. | 2025 | 1.59 | 2.85 | â | 842 | -0.055 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.150(5) | â | â | â |
| Wei et al. | 2025 | 2.95 | 3.00 | â | 1510 | -0.750 | 1189 | 0.69 | â |
| Almeida et al. | 2025 | 1.56 | 2.49 | â | 845 | â | 1046 | â | â |
| Hunt & Reffert | 2024 | 1.86 | 3.03 | 2.53 | 251 | â | 3939(1) | â | â |
| Cavallo et al. | 2024 | 1.21 | 3.62 | â | 676 | -0.960 | â | â | â |
| Hunt & Reffert | 2023 | 1.86 | 3.02 | 2.53 | 251 | â | â | â | â |
| Almeida et al. | 2023 | 1.70 | 2.76 | â | 520 | 0.134 | 846(1) | 0.69 | â |
| Just et al. | 2023 | â | â | â | 1585 | â | 115 | â | â |
| Jadhav & Subramaniam | 2021 | 1.77 | 1.92 | â | 955 | â | 1412 | â | 0(1) |
| Dias et al. | 2021 | 1.56 | 2.49 | â | 845 | 0.144 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.77 | 1.92 | â | 955 | â | â | â | â |
| Kounkel et al. | 2020 | 2.17 | 3.82 | â | 1000 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.90 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 1410 | -0.500 | â | â | â |
| Soubiran et al. | 2018 | 1.90 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.90 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.49 | 5.12 | â | 1585 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.49 | 5.12 | â | 1585 | â | â | â | â |
| Dias et al. | 2002 | 2.49 | 5.12 | â | 1585 | 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: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.37 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.37 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.1371, e_all=0.0031.
Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010).