Ruprecht 80

(NGC 2982; MWSC 1703; OCL 770; ESO 262 01; MWSC 1702)

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0.26 UTI
0.0
CN
0.05
Cdens
0.25
CC3
0.5
Clit
1.0
Cdup
Stellar density (N50/rad) 0.2 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.05 Very loose
  • CC3 0.25 Low quality
  • Clit 0.5 Moderately studied
  • Cdup 1.0 Unique

Overview

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Ruprecht 80 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~3.86 kpc) differs significantly from the median photometric distance (~2.34 kpc).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 145.501 -43.987 0.259 -5.139 2.799 17.974
Just et al. 2023 145.509 -44.017 – – – –
Bica et al. 2019 145.501 -44.02 – – – –
Kharchenko et al. 2016 145.509 -44.017 – – – –
Dias et al. 2014 145.512 -44.017 – -8.79 4.61 –
Kharchenko et al. 2013 145.515 -44.02 – -16.43 6.42 45.8
Piskunov et al. 2008 145.51 -44.012 – – – –
Kharchenko et al. 2005 145.51 -44.02 – -13.73 6.64 –
Kharchenko et al. 2003 145.5 -44.02 – -12.9 5.46 –
Dias et al. 2002 145.512 -44.017 – -8.79 4.61 45.75

💡 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– 2.34 0.93 – 240 -0.373 96 – –
Just et al. 2023 – – – 266 – 96 – –
Kharchenko et al. 2016 2.18 1.22 – 266 – – – –
Kharchenko et al. 2013 2.18 1.22 – 266 -0.373 – – –
Piskunov et al. 2008 2.50 0.93 – 214 – – – –
Kharchenko et al. 2005 2.50 0.93 – 214 – – – –
Kharchenko et al. 2003 1.43 0.16 – – – – – –
Dias et al. 2002 2.50 0.93 – 214 -0.373 – – –

Visualization

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