UBC 533
0.76
UTI
0.66
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
5.5 [arcmin]
- CN 0.66 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UBC 533 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close 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 and metallicity parameters (see Parameters). It is moderately studied in the literature.
Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.
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 | 230.308 | -53.179 | 0.826 | -1.751 | -1.325 | -15.368 |
| Li et al. | 2025 | 230.274 | -53.179 | 0.791 | -1.69 | -1.345 | â |
| Hu & Soubiran | 2025 | 230.326 | -53.187 | â | â | â | â |
| Almeida et al. | 2025 | 230.31 | -53.18 | â | â | â | â |
| Hunt & Reffert | 2024 | 230.328 | -53.172 | 0.815 | -1.759 | -1.298 | -10.153 |
| Cavallo et al. | 2024 | 230.326 | -53.187 | 0.819 | â | â | â |
| Hunt & Reffert | 2023 | 230.328 | -53.172 | 0.815 | -1.759 | -1.298 | -10.153 |
| Almeida et al. | 2023 | 230.315 | -53.17 | â | â | â | â |
| He et al. | 2022 | 230.327 | -53.166 | 0.843 | -1.757 | -1.313 | â |
| Dias et al. | 2021 | 230.31 | -53.18 | 0.796 | -1.693 | -1.344 | â |
| Cantat-Gaudin et al. | 2020 | 230.274 | -53.179 | 0.791 | -1.69 | -1.345 | â |
| Castro-Ginard et al. | 2020 | 230.299 | -53.175 | 0.795 | -1.703 | -1.334 | 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 | 1.14 | 0.72 | â | 324 | -0.048 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.260* | â | â | â |
| Almeida et al. | 2025 | 1.21 | 0.86 | â | 213 | â | 125 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 270* | â | â |
| Cavallo et al. | 2024 | 1.34 | 0.59 | â | 501 | 0.500 | â | â | â |
| Hunt & Reffert | 2023 | 1.16 | 0.70 | 0.79 | 264 | â | â | â | â |
| Almeida et al. | 2023 | 1.23 | 0.88 | â | 239 | 0.018 | 81* | 0.43 | â |
| He et al. | 2022 | â | 0.90 | â | 89 | â | â | â | â |
| Tarricq et al. | 2022 | 1.19 | â | â | 93 | â | â | â | â |
| Dias et al. | 2021 | 1.21 | 0.86 | â | 213 | 0.189 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.22 | 0.75 | â | 89 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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