Ruprecht 174
(MWSC 3405; OCL 176; C 2041+368; FSR 0216; FoF 70)
0.83
UTI
0.77
CN
0.84
Cdens
1.0
CC3
0.77
Clit
1.0
Cdup
Nm (P>50%)
157
Core radius and density
1.8 [pc], 4.2 [pc-2]
- CN 0.77 Rich
- Cdens 0.84 Dense
- CC3 1.0 Very high quality
- Clit 0.77 Well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 174 is a rich, dense object of very high C3 quality. Its parallax locates it at a moderate distance, below 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 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 | 310.848 | 37.029 | 0.391 | -3.153 | -4.716 | -5.918 |
| Li et al. | 2025 | 310.856 | 37.031 | 0.398 | -3.154 | -4.675 | â |
| Almeida et al. | 2025 | 310.858 | 37.023 | â | â | â | â |
| Zhang et al. | 2024 | 310.861 | 37.031 | â | â | â | â |
| Hunt & Reffert | 2024 | 310.861 | 37.031 | 0.39 | -3.145 | -4.705 | 40.831 |
| Cavallo et al. | 2024 | 310.854 | 37.021 | 0.395 | â | â | â |
| Hunt & Reffert | 2023 | 310.861 | 37.031 | 0.39 | -3.145 | -4.705 | 40.831 |
| Just et al. | 2023 | 310.851 | 37.009 | â | â | â | â |
| Jadhav & Subramaniam | 2021 | 310.856 | 37.031 | â | â | â | â |
| Dias et al. | 2021 | 310.858 | 37.023 | 0.405 | -3.152 | -4.672 | â |
| Cantat-Gaudin et al. | 2020 | 310.856 | 37.031 | 0.398 | -3.154 | -4.675 | â |
| Zhong et al. | 2020 | 310.856 | 37.031 | â | -3.154 | -4.675 | -4.545 |
| Cantat-Gaudin & Anders | 2020 | 310.856 | 37.031 | 0.398 | -3.154 | -4.675 | â |
| Liu & Pang | 2019 | 310.855 | 37.016 | 0.397 | -3.152 | -4.677 | â |
| Soubiran et al. | 2018 | 310.856 | 37.031 | â | â | â | -12.89 |
| Bica et al. | 2019 | 310.871 | 36.879 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 310.856 | 37.031 | 0.398 | -3.154 | -4.675 | â |
| Dias et al. | 2018 | â | â | â | -3.2 | -5.33 | â |
| Dib et al. | 2018 | 310.855 | 37.012 | â | â | â | â |
| Loktin & Popova | 2017 | 310.875 | 37.024 | â | -2.73 | -4.49 | â |
| Sampedro et al. | 2017 | 310.879 | 37.024 | â | -1.96 | -2.91 | â |
| Kharchenko et al. | 2016 | 310.851 | 37.009 | â | â | â | â |
| Dias et al. | 2014 | 310.879 | 37.024 | â | -2.73 | -4.49 | â |
| Kharchenko et al. | 2013 | 310.855 | 37.012 | â | -2.3 | -2.66 | â |
| Dias et al. | 2002 | 310.879 | 37.024 | â | -2.73 | -4.49 | â |
| Lynga | 1987 | 310.881 | 37.051 | 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 | 2.34 | 1.66 | 1.27 | 479 | 0.110 | 586 | â | 0 |
| Li et al. | 2025 | 2.00 | 1.89 | â | 410 | -0.141 | â | â | â |
| Almeida et al. | 2025 | 2.07 | 1.96 | â | 323 | â | 522 | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.239(1) | â | â | â |
| Hunt & Reffert | 2024 | 2.36 | 1.89 | 1.27 | 253 | â | 1078(1) | â | â |
| Cavallo et al. | 2024 | 2.24 | 2.12 | â | 240 | 0.220 | â | â | â |
| Hunt & Reffert | 2023 | 2.36 | 1.89 | 1.27 | 254 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 794 | â | 125 | â | â |
| Jadhav & Subramaniam | 2021 | 2.37 | 1.43 | â | 479 | â | 649 | â | 0(1) |
| Dias et al. | 2021 | 2.07 | 1.96 | â | 323 | -0.031 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.37 | 1.43 | â | 479 | â | â | â | â |
| Kounkel et al. | 2020 | 2.60 | 2.18 | â | 372 | â | â | â | â |
| Zhong et al. | 2020 | 2.34(1) | 1.01 | â | 8900 | 0.000 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.34 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 692 | 0.250 | â | â | â |
| Soubiran et al. | 2018 | 2.34 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.34 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 1.82 | â | â | 794 | â | â | â | â |
| Loktin & Popova | 2017 | 2.60 | 1.37 | â | 676 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.82 | 1.01 | â | 794 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.82 | 1.01 | â | 794 | â | â | â | â |
| Dias et al. | 2002 | 2.11 | 1.01 | â | 794 | 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: good fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.0455, e_all=0.0781.