Ruprecht 33
(MWSC 1332)
0.82
UTI
0.76
CN
0.88
Cdens
0.75
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
7.7 [arcmin]
- CN 0.76 Rich
- Cdens 0.88 Dense
- CC3 0.75 High quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 33 is a rich, dense object of high 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, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is well-studied in the literature.
Relatively close
Low extinction
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 | 116.439 | -21.916 | 0.419 | -1.39 | 0.065 | 48.266 |
| Hu & Soubiran | 2025 | 116.442 | -21.91 | â | â | â | â |
| Almeida et al. | 2025 | 116.461 | -21.91 | â | â | â | â |
| Hunt & Reffert | 2024 | 116.445 | -21.917 | 0.415 | -1.384 | 0.065 | 51.219 |
| Cavallo et al. | 2024 | 116.442 | -21.91 | 0.418 | â | â | â |
| He et al. | 2023 | 116.36 | -21.999 | 0.289 | -2.19 | 2.961 | â |
| Hunt & Reffert | 2023 | 116.445 | -21.917 | 0.415 | -1.384 | 0.065 | 51.219 |
| Just et al. | 2023 | 116.477 | -21.918 | â | â | â | â |
| Dias et al. | 2021 | 116.461 | -21.91 | 0.411 | -1.388 | 0.067 | â |
| Cantat-Gaudin et al. | 2020 | 116.445 | -21.915 | 0.417 | -1.384 | 0.058 | â |
| Cantat-Gaudin & Anders | 2020 | 116.445 | -21.915 | 0.417 | -1.384 | 0.058 | â |
| Soubiran et al. | 2018 | 116.445 | -21.915 | â | â | â | 48.1 |
| Cantat-Gaudin et al. | 2018 | 116.445 | -21.915 | 0.417 | -1.384 | 0.058 | â |
| Loktin & Popova | 2017 | 116.475 | -21.92 | â | -5.714 | 1.823 | â |
| Kharchenko et al. | 2016 | 116.477 | -21.918 | â | â | â | â |
| Dias et al. | 2014 | 116.492 | -21.95 | â | -3.67 | -1.15 | â |
| Kharchenko et al. | 2013 | 116.482 | -21.92 | â | -4.34 | 2.35 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.150* | â | â | â |
| Almeida et al. | 2025 | 1.96 | 1.13 | â | 286 | â | 276 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 558* | â | â |
| Cavallo et al. | 2024 | 2.06 | 0.87 | â | 537 | 0.230 | â | â | â |
| He et al. | 2023 | 3.09 | 1.35 | â | 25 | â | â | â | â |
| Hunt & Reffert | 2023 | 2.18 | 0.94 | 0.90 | 308 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 646 | â | 42 | â | â |
| Dias et al. | 2021 | 1.96 | 1.13 | â | 286 | -0.078 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.37 | 0.82 | â | 269 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.24 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.24 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.24 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.99 | 0.86 | â | 170 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.56 | 0.36 | â | 646 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.56 | 0.36 | â | 646 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.