Ruprecht 174

(MWSC 3405; OCL 176; C 2041+368; FSR 0216; FoF 70)

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0.95 UTI
0.77
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members) 3.7 [arcmin]
  • CN 0.77 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique

Overview

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Ruprecht 174 is a rich, very 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 very well-studied in the literature.
Relatively close Moderate extinction Near-solar metallicity Intermediate age

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 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 –
Almeida et al. 2025 310.858 37.023 – – – –
Zhang et al. 2024 310.861 37.031 – – – –
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 – – –
Hunt & Reffert 2023 310.861 37.031 0.39 -3.145 -4.705 40.831
Just et al. 2023 310.851 37.009 – – – –
Dias et al. 2021 310.858 37.023 0.405 -3.152 -4.672 –
Cantat-Gaudin et al. 2020 310.856 37.031 0.398 -3.154 -4.675 –
Cantat-Gaudin & Anders 2020 310.856 37.031 0.398 -3.154 -4.675 –
Liu & Pang 2019 310.855 37.016 0.397 -3.152 -4.677 –
Soubiran et al. 2018 310.856 37.031 – – – -12.89
Bica et al. 2019 310.871 36.879 – – – –
Cantat-Gaudin et al. 2018 310.856 37.031 0.398 -3.154 -4.675 –
Loktin & Popova 2017 310.875 37.024 – -2.73 -4.49 –
Kharchenko et al. 2016 310.851 37.009 – – – –
Dias et al. 2014 310.879 37.024 – -2.73 -4.49 –
Kharchenko et al. 2013 310.855 37.012 – -2.3 -2.66 –
Dias et al. 2002 310.879 37.024 – -2.73 -4.49 –

💡 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
Li et al. 2025 2.00 1.89 – 410 -0.141 – – –
Almeida et al. 2025 2.07 1.96 – 323 – 522 – –
Zhang et al. 2024 – – – – 0.239* – – –
Hunt & Reffert 2024 – – – – – 1078* – –
Cavallo et al. 2024 2.24 2.12 – 240 0.220 – – –
Hunt & Reffert 2023 2.36 1.89 1.27 254 – – – –
Just et al. 2023 – – – 794 – 125 – –
Dias et al. 2021 2.07 1.96 – 323 -0.031 – – –
Cantat-Gaudin et al. 2020 2.37 1.43 – 479 – – – –
Cantat-Gaudin & Anders 2020 2.34 – – – – – – –
Liu & Pang 2019 – – – 692 0.250 – – –
Soubiran et al. 2018 2.34 – – – – – – –
Cantat-Gaudin et al. 2018 2.34 – – – – – – –
Loktin & Popova 2017 2.60 1.35 – 676 – – – –
Kharchenko et al. 2016 1.82 1.00 – 794 – – – –
Kharchenko et al. 2013 1.82 1.00 – 794 – – – –
Dias et al. 2002 2.11 0.99 – 794 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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