Ruprecht 138
(NGC 6506; MWSC 2771; OCL 16; ESO 521 06)
0.89
UTI
0.79
CN
1.0
Cdens
1.0
CC3
0.84
Clit
1.0
Cdup
Stellar density (N50/rad)
32.4 [N/pc2]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.84 Well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 138 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 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 | 269.996 | -24.664 | 0.382 | 0.264 | -1.137 | 7.775 |
| Almeida et al. | 2025 | 269.983 | -24.668 | â | â | â | â |
| Hunt & Reffert | 2024 | 269.992 | -24.663 | 0.394 | 0.271 | -1.142 | 11.615 |
| Celli et al. | 2024 | 269.984 | -24.665 | â | â | â | â |
| Cavallo et al. | 2024 | 269.987 | -24.657 | 0.394 | â | â | â |
| Hunt & Reffert | 2023 | 269.992 | -24.663 | 0.394 | 0.271 | -1.142 | 11.615 |
| Just et al. | 2023 | 269.982 | -24.699 | â | â | â | â |
| Dias et al. | 2021 | 269.983 | -24.668 | 0.364 | 0.252 | -1.149 | â |
| Cantat-Gaudin et al. | 2020 | 269.984 | -24.665 | 0.369 | 0.248 | -1.147 | â |
| Cantat-Gaudin & Anders | 2020 | 269.984 | -24.665 | 0.369 | 0.248 | -1.147 | â |
| Soubiran et al. | 2018 | 269.984 | -24.665 | â | â | â | -10.54 |
| Bica et al. | 2019 | 269.966 | -24.681 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 269.984 | -24.665 | 0.369 | 0.248 | -1.147 | â |
| Kharchenko et al. | 2016 | 269.982 | -24.699 | â | â | â | â |
| Dias et al. | 2014 | 269.983 | -24.683 | â | -2.25 | -3.91 | â |
| Kharchenko et al. | 2013 | 269.991 | -24.698 | â | -1.43 | -2.67 | â |
| Dias et al. | 2002 | 269.983 | -24.683 | â | -2.25 | -3.91 | 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 | 2.26 | 2.28 | 2.36 | 142 | -0.013 | 856 | â | â |
| Almeida et al. | 2025 | 2.26 | 2.35 | â | 13 | â | 626 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1822(1) | â | â |
| Celli et al. | 2024 | â | â | â | 10 | â | 1087 | â | â |
| Cavallo et al. | 2024 | 1.98 | 2.98 | â | 178 | -0.230 | â | â | â |
| Hunt & Reffert | 2023 | 2.29 | 2.59 | 2.36 | 105 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 794 | â | 17 | â | â |
| Dias et al. | 2021 | 2.26 | 2.35 | â | 13 | 0.203 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.73 | 2.21 | â | 10 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.51 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.51 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.51 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.13 | 2.19 | â | 794 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.13 | 2.19 | â | 794 | â | â | â | â |
| Dias et al. | 2002 | 0.93 | 0.56 | â | 1995 | 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.