Ruprecht 163
(MWSC 1886)
0.32
UTI
0.0
CN
0.08
Cdens
0.62
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad)
0.4 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.08 Very loose
- CC3 0.62 Intermediate quality
- Clit 0.45 Poorly studied
- Cdup 1.0 Unique
Overview
Ruprecht 163 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close* distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~0.94 kpc) differs significantly from the median photometric distance (~3.02 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 166.198 | -67.922 | 1.061 | -5.848 | 0.066 | 13.785 |
| Hu & Soubiran | 2025 | 165.791 | -67.617 | â | â | â | â |
| Cavallo et al. | 2024 | 165.791 | -67.617 | 1.043 | â | â | â |
| Hunt & Reffert | 2023 | 166.172 | -67.998 | 1.042 | -5.825 | 0.139 | 16.195 |
| Just et al. | 2023 | 166.215 | -67.939 | â | â | â | â |
| Kharchenko et al. | 2016 | 166.215 | -67.939 | â | â | â | â |
| Dias et al. | 2014 | 166.212 | -67.95 | â | -6.94 | 3.5 | â |
| Kharchenko et al. | 2013 | 166.222 | -67.943 | â | -12.26 | 6.7 | â |
| Dias et al. | 2002 | 166.213 | -67.95 | â | -12.26 | 6.7 | 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 | 3.02 | 0.97 | 0.82 | 2317 | 0.025 | 462 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.080(5) | â | â | â |
| Cavallo et al. | 2024 | 0.96 | 0.39 | â | 617 | 0.130 | â | â | â |
| Hunt & Reffert | 2023 | 0.91 | 0.38 | 0.82 | 374 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 2317 | â | 462 | â | â |
| Kharchenko et al. | 2016 | 3.02 | 0.97 | â | 2317 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.02 | 0.97 | â | 2317 | â | â | â | â |
| Dias et al. | 2002 | 3.02 | 0.97 | â | 2317 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.