Ruprecht 164
(VDBH 119; MWSC 1951; OCL 858; vdBergh-Hagen 119; ESO 129 23; FSR 1588)
0.89
UTI
0.78
CN
1.0
Cdens
1.0
CC3
0.84
Clit
1.0
Cdup
Nm (P>50%)
190
Core radius and density
1.3 [pc], 7.3 [pc-2]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.84 Well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 164 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low 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.
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 172.608 | -60.75 | 0.209 | -6.854 | 1.35 | 0.76 |
| Li et al. | 2025 | 172.616 | -60.752 | 0.194 | -6.83 | 1.321 | â |
| Hu & Soubiran | 2025 | 172.624 | -60.753 | â | â | â | â |
| Almeida et al. | 2025 | 172.644 | -60.754 | â | â | â | â |
| Hunt & Reffert | 2024 | 172.606 | -60.746 | 0.207 | -6.856 | 1.38 | -0.689 |
| Cavallo et al. | 2024 | 172.624 | -60.753 | 0.209 | â | â | â |
| Hunt & Reffert | 2023 | 172.606 | -60.746 | 0.207 | -6.856 | 1.38 | -0.689 |
| Just et al. | 2023 | 172.703 | -60.746 | â | â | â | â |
| Jadhav & Subramaniam | 2021 | 172.616 | -60.752 | â | â | â | â |
| Dias et al. | 2021 | 172.644 | -60.754 | 0.194 | -6.829 | 1.317 | â |
| Cantat-Gaudin et al. | 2020 | 172.616 | -60.752 | 0.194 | -6.83 | 1.321 | â |
| Cantat-Gaudin & Anders | 2020 | 172.616 | -60.752 | 0.194 | -6.83 | 1.321 | â |
| Soubiran et al. | 2018 | 172.616 | -60.752 | â | â | â | 7.91 |
| Bica et al. | 2019 | 172.632 | -60.734 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 172.616 | -60.752 | 0.194 | -6.83 | 1.321 | â |
| Dias et al. | 2018 | â | â | â | -6.91 | 0.71 | â |
| Dib et al. | 2018 | 172.71 | -60.75 | â | â | â | â |
| Sampedro et al. | 2017 | 172.604 | -60.753 | â | -5.84 | -1.58 | â |
| Joshi et al. | 2016 | 172.71 | -60.75 | â | â | â | â |
| Kharchenko et al. | 2016 | 172.703 | -60.746 | â | â | â | â |
| Dias et al. | 2014 | 172.713 | -60.733 | â | -5.22 | -1.66 | â |
| Kharchenko et al. | 2013 | 172.71 | -60.75 | â | -5.12 | 1.95 | -3.0 |
| Piskunov et al. | 2008 | 172.702 | -60.724 | â | â | â | â |
| Kharchenko et al. | 2005 | 172.71 | -60.73 | â | -2.05 | 6.05 | â |
| Kharchenko et al. | 2003 | 172.72 | -60.75 | â | -0.89 | 5.03 | â |
| Dias et al. | 2002 | 172.713 | -60.733 | â | -0.89 | 5.03 | â |
| Lynga | 1987 | 172.776 | -60.809 | â | â | â | â |
| van den Bergh & Hagen | 1975 | 172.2 | -60.533 | 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 | 3.91 | 0.86 | 1.85 | 950 | -0.150 | 987 | â | 2 |
| Li et al. | 2025 | 4.58 | 1.62 | â | 950 | -0.060 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.240(5) | â | â | â |
| Almeida et al. | 2025 | 3.91 | 1.33 | â | 1256 | â | 987 | â | â |
| Hunt & Reffert | 2024 | 4.25 | 1.65 | 1.85 | 408 | â | 2221(1) | â | â |
| Cavallo et al. | 2024 | 2.61 | 1.75 | â | 1585 | -0.380 | â | â | â |
| Hunt & Reffert | 2023 | 4.25 | 1.65 | 1.85 | 407 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 50 | â | 97 | â | â |
| Jadhav & Subramaniam | 2021 | 3.91 | 0.86 | â | 1698 | â | 1677 | â | 2(1) |
| Dias et al. | 2021 | 3.91 | 1.33 | â | 1256 | 0.099 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.91 | 0.86 | â | 1698 | â | â | â | â |
| Kounkel et al. | 2020 | 4.22 | 1.58 | â | 389 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.48 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 4.48 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.48 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 1.30 | â | â | 50 | â | â | â | â |
| Joshi et al. | 2016 | 1.30 | 0.35 | â | 50 | â | 42 | â | â |
| Kharchenko et al. | 2016 | 1.30 | 0.35 | â | 50 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.30 | 0.35 | â | 50 | â | â | â | â |
| Piskunov et al. | 2008 | 0.78 | 0.35 | â | 1000 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.78 | 0.35 | â | 1000 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.00 | 0.32 | â | â | â | â | â | â |
| Dias et al. | 2002 | 0.78 | 0.35 | 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: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.81 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.81 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.0979, e_all=0.1433.