UPK 502
0.77
UTI
0.57
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Stellar density (N50/rad)
18.5 [N/pc2]
- CN 0.57 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
UPK 502 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close 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 absorption, age, and metallicity parameters (see Parameters). It is well-studied in the literature.
Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 124.363 | -37.774 | 1.429 | -8.079 | 5.666 | 31.897 |
| Li et al. | 2025 | 124.371 | -37.798 | 1.397 | -8.119 | 5.621 | â |
| Almeida et al. | 2025 | 124.341 | -37.816 | â | â | â | â |
| Alfonso et al. | 2024 | 124.287 | -37.81 | 1.405 | -8.053 | 5.706 | â |
| Hunt & Reffert | 2024 | 124.359 | -37.779 | 1.431 | -8.063 | 5.714 | 31.052 |
| Cavallo et al. | 2024 | 124.347 | -37.82 | 1.434 | â | â | â |
| Hunt & Reffert | 2023 | 124.359 | -37.779 | 1.431 | -8.063 | 5.714 | 31.052 |
| Almeida et al. | 2023 | 124.362 | -37.804 | â | â | â | â |
| He et al. | 2022 | 124.326 | -37.792 | 1.433 | -8.09 | 5.665 | â |
| Dias et al. | 2021 | 124.341 | -37.816 | 1.405 | -8.091 | 5.629 | â |
| Cantat-Gaudin et al. | 2020 | 124.371 | -37.798 | 1.397 | -8.119 | 5.621 | â |
| Cantat-Gaudin & Anders | 2020 | 124.362 | -37.788 | 1.405 | -8.085 | 5.65 | â |
| Sim et al. | 2019 | 124.316 | -37.829 | â | -8.08 | 5.61 | 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 | 0.7 | 0.25 | 0.56 | 104 | 0.158 | 87 | 0.66 | â |
| Li et al. | 2025 | 0.67 | 0.04 | â | 374 | 0.230 | â | â | â |
| Almeida et al. | 2025 | 0.69 | 0.28 | â | 196 | â | 87 | â | â |
| Alfonso et al. | 2024 | 0.71 | 0.17 | â | 225 | 0.158 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 71(1) | â | â |
| Cavallo et al. | 2024 | 0.71 | 0.68 | â | 37 | -0.400 | â | â | â |
| Hunt & Reffert | 2023 | 0.66 | 0.25 | 0.56 | 104 | â | â | â | â |
| Almeida et al. | 2023 | 0.68 | 0.18 | â | 287 | 0.045 | 102(1) | 0.66 | â |
| He et al. | 2022 | â | 0.60 | â | 63 | â | â | â | â |
| Tarricq et al. | 2022 | 0.70 | â | â | 78 | â | â | â | â |
| Dias et al. | 2021 | 0.69 | 0.28 | â | 196 | 0.158 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.71 | 0.17 | â | 72 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.70 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.70 | â | â | 71 | 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: good fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.