Ruprecht 93
(NGC 3519; MWSC 1885; OCL 844; ESO 128 30; FoF 1062)
0.91
UTI
0.8
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
23.9 [N/pc2]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 93 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is very well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 166.042 | -61.375 | 0.447 | -6.426 | 3.132 | -27.77 |
| Li et al. | 2025 | 166.037 | -61.372 | 0.436 | -6.411 | 3.104 | â |
| Almeida et al. | 2025 | 166.043 | -61.375 | â | â | â | â |
| Hunt & Reffert | 2024 | 166.05 | -61.377 | 0.447 | -6.427 | 3.131 | -27.73 |
| Cavallo et al. | 2024 | 166.028 | -61.377 | 0.447 | â | â | â |
| Hunt & Reffert | 2023 | 166.05 | -61.377 | 0.447 | -6.427 | 3.131 | -27.73 |
| Almeida et al. | 2023 | 166.047 | -61.372 | â | â | â | â |
| Just et al. | 2023 | 166.042 | -61.366 | â | â | â | â |
| Dias et al. | 2021 | 166.043 | -61.375 | 0.437 | -6.422 | 3.115 | -24.55 |
| Cantat-Gaudin et al. | 2020 | 166.037 | -61.372 | 0.436 | -6.411 | 3.104 | â |
| Cantat-Gaudin & Anders | 2020 | 166.037 | -61.372 | 0.436 | -6.411 | 3.104 | â |
| Liu & Pang | 2019 | 166.072 | -61.397 | 0.447 | -6.462 | 2.843 | â |
| Bossini et al. | 2019 | 166.037 | -61.372 | â | â | â | â |
| Soubiran et al. | 2018 | 166.037 | -61.372 | â | â | â | -24.4 |
| Bica et al. | 2019 | 166.018 | -61.358 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 166.037 | -61.372 | 0.436 | -6.411 | 3.104 | â |
| Loktin & Popova | 2017 | 166.05 | -61.373 | â | -3.191 | -2.615 | 5.1 |
| Kharchenko et al. | 2016 | 166.042 | -61.366 | â | â | â | â |
| Kharchenko et al. | 2013 | 166.05 | -61.37 | â | -5.08 | 0.85 | 5.1 |
| Piskunov et al. | 2008 | 166.084 | -61.361 | â | â | â | â |
| van den Bergh | 2006 | 166.1 | -61.367 | â | â | â | â |
| Kharchenko et al. | 2005 | 166.09 | -61.37 | â | -3.89 | 0.39 | â |
| Kharchenko et al. | 2003 | 166.08 | -61.36 | â | -3.05 | -0.02 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.945 | 0.71 | 0.47 | 384 | 0.019 | 418 | 0.52 | â |
| Li et al. | 2025 | 1.87 | 0.67 | â | 511 | -0.155 | â | â | â |
| Almeida et al. | 2025 | 2.00 | 0.90 | â | 281 | â | 335 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1209(1) | â | â |
| Cavallo et al. | 2024 | 1.89 | 1.05 | â | 316 | -0.100 | â | â | â |
| Hunt & Reffert | 2023 | 2.05 | 0.38 | 0.47 | 480 | â | â | â | â |
| Almeida et al. | 2023 | 2.02 | 0.89 | â | 318 | 0.019 | 502(1) | 0.52 | â |
| Just et al. | 2023 | â | â | â | 569 | â | 110 | â | â |
| Dias et al. | 2021 | 2.00 | 0.90 | â | 281 | 0.028 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.15 | 0.70 | â | 245 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.15 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 562 | 0.250 | â | â | â |
| Bossini et al. | 2019 | 2.16 | 0.64 | â | 330 | 0.010 | â | â | â |
| Soubiran et al. | 2018 | 2.15 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.15 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.46 | 0.70 | â | 160 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.62 | 0.52 | â | 569 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.62 | 0.52 | â | 569 | 0.153 | â | â | â |
| Piskunov et al. | 2008 | 1.44 | 0.71 | â | 437 | â | â | â | â |
| van den Bergh | 2006 | 1.44 | 0.71 | â | 155 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.44 | 0.71 | â | 437 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.43 | 0.71 | â | â | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: worst fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.
Dias et al. (2002)
Spiral arm (Cheon, S. et al. 2010, JKAS, arXiv:1007.2686)