Ruprecht 163

(MWSC 1886)

Click to load Aladin Lite
0.34 UTI
0.0
CN
0.08
Cdens
0.62
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members) 24.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.08 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.5 Moderately studied
  • Cdup 1.0 Unique

Overview

â„šī¸
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 (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~0.94 kpc) differs significantly from the median photometric distance (~3.02 kpc).

Distant Low extinction Near-solar metallicity Old

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 166.198 -67.922 1.061 -5.848 0.066 13.785
Hu & Soubiran 2025 165.791 -67.617 – – – –
Cavallo et al. 2024 165.791 -67.617 1.043 – – –
Hunt & Reffert 2023 166.172 -67.998 1.042 -5.825 0.139 16.195
Just et al. 2023 166.215 -67.939 – – – –
Kharchenko et al. 2016 166.215 -67.939 – – – –
Dias et al. 2014 166.212 -67.95 – -6.94 3.5 –
Kharchenko et al. 2013 166.222 -67.943 – -12.26 6.7 –
Dias et al. 2002 166.213 -67.95 – -12.26 6.7 –

💡 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
Hu & Soubiran 2025 – – – – -0.080* – – –
Cavallo et al. 2024 0.96 0.39 – 617 0.130 – – –
Hunt & Reffert 2023 0.91 0.38 0.82 374 – – – –
Just et al. 2023 – – – 2317 – 462 – –
Kharchenko et al. 2016 3.02 0.97 – 2317 – – – –
Kharchenko et al. 2013 3.02 0.97 – 2317 – – – –
Dias et al. 2002 3.02 0.97 – 2317 – – – –

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

Visualization

â„šī¸