Ruprecht 119

(MWSC 2413; OCL 963; ESO 226 10)

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0.95 UTI
0.75
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
C3 classification AA
Number of members (P>50%) 108
Radius (P>50% members) 4.4 [arcmin]
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique
πŸ“₯ Members πŸ“Š Colab πŸ”¬ Bayestar19 πŸ” CDS πŸ” Simbad πŸ” CDS (Ξ±, Ξ΄) πŸ” Simbad (Ξ±, Ξ΄)

Overview
ℹ️
Ruprecht 119 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, young cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.

(*): The parallax distance estimate (~2.21 kpc) differs significantly from the median photometric distance (~1.40 kpc).

Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

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

Cavallo et al. (2024)
Gold sample.

Data
πŸ” Search references for Ruprecht 119 in: SciX Simbad
ℹ️
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 247.012 -51.495 0.452 -1.349 -3.416 -46.702
Li et al. 2025 247.039 -51.5 0.433 -1.3 -3.413 –
Almeida et al. 2025 247.042 -51.504 – – – –
Hunt & Reffert 2024 247.003 -51.496 0.455 -1.407 -3.416 -45.258
Cavallo et al. 2024 247.02 -51.485 0.455 – – –
Hunt & Reffert 2023 247.003 -51.496 0.455 -1.407 -3.416 -45.258
Almeida et al. 2023 247.038 -51.504 – – – –
Just et al. 2023 247.039 -51.509 – – – –
Jaehnig et al. 2021 247.037 -51.497 0.469 -1.298 -3.426 –
Rain et al. 2021 247.039 -51.5 0.433 -1.3 -3.413 –
Dias et al. 2021 247.042 -51.504 0.439 -1.314 -3.424 –
Cantat-Gaudin et al. 2020 247.039 -51.5 0.433 -1.3 -3.413 –
SΓ‘nchez et al. 2020 247.062 -51.5 – -1.392 -3.512 –
Cantat-Gaudin & Anders 2020 247.039 -51.5 0.433 -1.3 -3.413 –
Soubiran et al. 2018 247.039 -51.5 – – – -39.38
Bica et al. 2019 247.034 -51.505 – – – –
Cantat-Gaudin et al. 2018 247.039 -51.5 0.433 -1.3 -3.413 –
Loktin & Popova 2017 247.065 -51.501 – -3.809 -8.03 -11.2
Kharchenko et al. 2016 247.039 -51.509 – – – –
Dias et al. 2014 247.063 -51.5 – -2.13 -3.42 –
Kharchenko et al. 2013 247.05 -51.51 – -2.11 -0.56 -11.2
Gozha et al. 2012 247.062 -51.5 – – – –
Piskunov et al. 2008 247.057 -51.505 – – – –
van den Bergh 2006 247.05 -51.5 – – – –
Kharchenko et al. 2005 247.06 -51.5 – -2.17 -0.35 –
Kharchenko et al. 2003 247.03 -51.52 – -2.42 -0.96 –
Dias et al. 2002 247.062 -51.5 – -2.13 -3.42 -11.21
Dambis 1999 247.062 -51.5 – – – –

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] Bfr BSS
Li et al. 2025 1.07 0.84 – 1287 -0.333 – – –
Almeida et al. 2025 1.90 1.86 – 101 – 369 – –
Hunt & Reffert 2024 – – – – – 1231* – –
Cavallo et al. 2024 1.69 1.87 – 263 0.220 – – –
Hunt & Reffert 2023 1.99 1.91 2.15 48 – – – –
Almeida et al. 2023 1.88 1.97 – 99 0.180 874* 0.61 –
Just et al. 2023 – – – 272 – 72 – –
Jaehnig et al. 2021 2.13* – – – – – – –
Rain et al. 2021 2.16 1.77 – 7 – – – 0
Dias et al. 2021 1.90 1.86 – 101 0.183 – – –
Cantat-Gaudin et al. 2020 2.23 1.49 – 48 – – – –
Cantat-Gaudin & Anders 2020 2.16 – – – – – – –
Soubiran et al. 2018 2.16 – – – – – – –
Cantat-Gaudin et al. 2018 2.16 – – – – – – –
Loktin & Popova 2017 1.00 1.71 – 10 – – – –
Kharchenko et al. 2016 1.10 1.77 – 272 – – – –
Kharchenko et al. 2013 1.10 1.77 – 272 – – – –
Gozha et al. 2012 0.96 – – 7 – 54 – –
Piskunov et al. 2008 0.96 1.77 – 27 – – – –
van den Bergh 2006 0.96 1.77 – 7 – – – –
Kharchenko et al. 2005 0.96 1.77 – 27 – – – –
Kharchenko et al. 2003 0.96 1.55 – – – – – –
Dias et al. 2002 0.96 1.77 – 7 – – – –
Dambis 1999 0.95 1.73 – 45 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0655 22.2 247.0 -51.5 0.48 -1.4 -3.45 -66.85 0.02

πŸ’‘ Note: The % column shows the percentage of members that Ruprecht 119 shares with each listed object.

Visualization
ℹ️
Ruprecht 119 UCC
Ruprecht 119 HUNT23
Ruprecht 119 CANTAT20
Galactocentric position diagram