Ruprecht 130
(VDBH 247; OCL 1034; vdBergh-Hagen 247; ESO 455 41; MWSC 2698; FoF 1205)
0.95
UTI
0.76
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
2.8 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 130 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 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 and mass parameters (see Parameters). It is very well-studied in the literature.
Relatively close
High 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 | β | 266.9 | -30.095 | 0.384 | 0.489 | -1.852 | -0.168 |
| Almeida et al. | 2025 | 266.899 | -30.099 | β | β | β | β |
| Hunt & Reffert | 2024 | 266.895 | -30.098 | 0.382 | 0.492 | -1.872 | 0.841 |
| Cavallo et al. | 2024 | 266.898 | -30.095 | 0.381 | β | β | β |
| Hunt & Reffert | 2023 | 266.895 | -30.098 | 0.382 | 0.492 | -1.872 | 0.841 |
| Jaehnig et al. | 2021 | 266.901 | -30.103 | 0.417 | 0.503 | -1.812 | β |
| Rain et al. | 2021 | 266.9 | -30.098 | 0.389 | 0.477 | -1.795 | β |
| Dias et al. | 2021 | 266.899 | -30.099 | 0.393 | 0.482 | -1.782 | β |
| Cantat-Gaudin et al. | 2020 | 266.9 | -30.098 | 0.389 | 0.477 | -1.795 | β |
| SΓ‘nchez et al. | 2020 | 266.883 | -30.1 | β | 0.539 | -1.732 | β |
| Cantat-Gaudin & Anders | 2020 | 266.9 | -30.098 | 0.389 | 0.477 | -1.795 | β |
| Liu & Pang | 2019 | 266.901 | -30.103 | 0.381 | 0.365 | -1.865 | β |
| Soubiran et al. | 2018 | 266.9 | -30.098 | β | β | β | -41.84 |
| Bica et al. | 2019 | 266.878 | -30.087 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 266.9 | -30.098 | 0.389 | 0.477 | -1.795 | β |
| Dias et al. | 2014 | 266.883 | -30.1 | β | -0.8 | -2.52 | β |
| van den Bergh | 2006 | 266.9 | -30.117 | β | β | β | β |
| Dias et al. | 2002 | 266.883 | -30.1 | β | -0.8 | -2.52 | β |
π‘ 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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 2.01 | 2.89 | β | 403 | β | 292 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1722* | β | β |
| Cavallo et al. | 2024 | 1.78 | 3.66 | β | 60 | -1.050 | β | β | β |
| Hunt & Reffert | 2023 | 2.37 | 3.39 | 1.46 | 106 | β | β | β | β |
| Jaehnig et al. | 2021 | 2.48* | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 2.39 | 3.72 | β | 50 | β | β | β | 0 |
| Dias et al. | 2021 | 2.01 | 2.89 | β | 403 | 0.201 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.34 | 2.76 | β | 398 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.39 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 955 | 0.250 | β | β | β |
| Soubiran et al. | 2018 | 2.39 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.39 | β | β | β | β | β | β | β |
| van den Bergh | 2006 | 2.10 | 3.72 | β | 50 | β | β | β | β |
| Dias et al. | 2002 | 2.10 | 3.72 | β | 50 | 0.030 | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.