Ruprecht 80
(NGC 2982; MWSC 1703; OCL 770; ESO 262 01; MWSC 1702)
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
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
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 145.501 | -43.987 | 0.259 | -5.139 | 2.799 | 17.974 |
| Just et al. | 2023 | 145.509 | -44.017 | â | â | â | â |
| Bica et al. | 2019 | 145.501 | -44.02 | â | â | â | â |
| Kharchenko et al. | 2016 | 145.509 | -44.017 | â | â | â | â |
| Dias et al. | 2014 | 145.512 | -44.017 | â | -8.79 | 4.61 | â |
| Kharchenko et al. | 2013 | 145.515 | -44.02 | â | -16.43 | 6.42 | 45.8 |
| Piskunov et al. | 2008 | 145.51 | -44.012 | â | â | â | â |
| Kharchenko et al. | 2005 | 145.51 | -44.02 | â | -13.73 | 6.64 | â |
| Kharchenko et al. | 2003 | 145.5 | -44.02 | â | -12.9 | 5.46 | â |
| Dias et al. | 2002 | 145.512 | -44.017 | â | -8.79 | 4.61 | 45.75 |
đĄ 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 | 99999â | 2.34 | 0.93 | â | 240 | -0.373 | 96 | â | â |
| Just et al. | 2023 | â | â | â | 266 | â | 96 | â | â |
| Kharchenko et al. | 2016 | 2.18 | 1.22 | â | 266 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.18 | 1.22 | â | 266 | -0.373 | â | â | â |
| Piskunov et al. | 2008 | 2.50 | 0.93 | â | 214 | â | â | â | â |
| Kharchenko et al. | 2005 | 2.50 | 0.93 | â | 214 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.43 | 0.16 | â | â | â | â | â | â |
| Dias et al. | 2002 | 2.50 | 0.93 | â | 214 | -0.373 | â | â | â |
MOCA
