Ruprecht 176

(MWSC 2373)

Click to load Aladin Lite
0.92 UTI
0.86
CN
1.0
Cdens
1.0
CC3
0.87
Clit
1.0
Cdup
Stellar density (N50/rad) 24.0 [N/pc2]
  • CN 0.86 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.87 Well-studied
  • Cdup 1.0 Unique

Overview

ℹ️
Ruprecht 176 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 and metallicity parameters (see Parameters). It is well-studied in the literature.

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

Cavallo et al. (2024)
Gold sample.

Data

ℹ️
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 243.675 -51.333 0.357 -2.684 -2.992 -52.249
Li et al. 2025 243.676 -51.332 0.335 -2.644 -2.984 –
Almeida et al. 2025 243.681 -51.333 – – – –
Hunt & Reffert 2024 243.671 -51.333 0.365 -2.703 -2.991 -52.27
Cavallo et al. 2024 243.679 -51.339 0.363 – – –
Hunt & Reffert 2023 243.671 -51.333 0.365 -2.703 -2.991 -52.27
Just et al. 2023 243.649 -51.332 – – – –
Dias et al. 2021 243.681 -51.333 0.338 -2.677 -2.99 -52.246
Cantat-Gaudin et al. 2020 243.676 -51.332 0.335 -2.644 -2.984 –
SΓ‘nchez et al. 2020 243.7 -51.333 – -2.627 -2.963 –
Cantat-Gaudin & Anders 2020 243.676 -51.332 0.335 -2.644 -2.984 –
Bossini et al. 2019 243.676 -51.332 – – – –
Soubiran et al. 2018 243.676 -51.332 – – – -52.19
Cantat-Gaudin et al. 2018 243.676 -51.332 0.335 -2.644 -2.984 –
Kharchenko et al. 2016 243.649 -51.332 – – – –
Dias et al. 2014 243.7 -51.333 – -2.54 -2.86 –
Kharchenko et al. 2013 243.66 -51.333 – -4.3 -3.01 –
Dias et al. 2002 243.7 -51.333 – -2.99 -2.9 –

πŸ’‘ 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 99999– 2.62 1.715 1.47 162 0.089 739 – –
Li et al. 2025 2.39 1.87 – 118 0.246 – – –
Almeida et al. 2025 2.22 1.86 – 130 – 739 – –
Hunt & Reffert 2024 – – – – – 1616(1) – –
Cavallo et al. 2024 1.71 2.38 – 162 -0.900 – – –
Hunt & Reffert 2023 2.45 1.75 1.47 215 – – – –
Just et al. 2023 – – – 575 – 611 – –
Dias et al. 2021 2.22 1.86 – 130 0.179 – – –
Cantat-Gaudin et al. 2020 2.62 1.66 – 120 – – – –
Cantat-Gaudin & Anders 2020 2.75 – – – – – – –
Bossini et al. 2019 2.58 1.68 – 147 0.000 – – –
Soubiran et al. 2018 2.75 – – – – – – –
Cantat-Gaudin et al. 2018 2.75 – – – – – – –
Kharchenko et al. 2016 2.69 1.48 – 575 – – – –
Kharchenko et al. 2013 2.69 1.48 – 575 – – – –
Dias et al. 2002 2.69 1.48 – 575 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

ℹ️