Ruprecht 43
(MWSC 1401; OCL 684; ESO 430 06; Turner-Majaess 1)
0.67
UTI
0.58
CN
0.5
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
2.8 [arcmin]
- CN 0.58 Moderately populated
- Cdens 0.5 Moderately dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 43 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~6.34 kpc) differs significantly from the median photometric distance (~1.30 kpc).
Relatively close
Low extinction
Low mass
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 119.682 | -28.816 | 0.158 | -2.199 | 3.048 | 114.157 |
| Li et al. | 2025 | 119.697 | -28.805 | 0.105 | -2.23 | 3.041 | â |
| Just et al. | 2023 | 119.814 | -28.867 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 119.697 | -28.805 | 0.105 | -2.23 | 3.041 | â |
| Cantat-Gaudin & Anders | 2020 | 119.697 | -28.805 | 0.105 | -2.23 | 3.041 | â |
| Soubiran et al. | 2018 | 119.697 | -28.805 | â | â | â | 103.56 |
| Bica et al. | 2019 | 119.818 | -28.966 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 119.697 | -28.805 | 0.105 | -2.23 | 3.041 | â |
| Kharchenko et al. | 2016 | 119.814 | -28.867 | â | â | â | â |
| Dias et al. | 2014 | 119.692 | -28.811 | â | -1.82 | 0.4 | 113.37 |
| Kharchenko et al. | 2013 | 119.82 | -28.87 | â | -1.03 | 1.18 | 113.4 |
| Piskunov et al. | 2008 | 119.811 | -28.899 | â | â | â | â |
| Kharchenko et al. | 2005 | 119.82 | -28.9 | â | -3.57 | -0.08 | â |
| Kharchenko et al. | 2003 | 119.67 | -28.87 | â | -4.63 | -1.9 | â |
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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 5.11 | 1.32 | â | 612 | 0.060 | â | â | â |
| Just et al. | 2023 | â | â | â | 251 | â | 48 | â | â |
| Cantat-Gaudin & Anders | 2020 | 7.46 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 7.46 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 7.46 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 0.97 | 0.64 | â | 251 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.97 | 0.64 | â | 251 | â | â | â | â |
| Piskunov et al. | 2008 | 1.30 | 0.84 | â | 295 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.30 | 0.84 | â | 295 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.00 | 0.16 | â | â | â | â | â | â |

