UPK 31
0.67
UTI
0.56
CN
1.0
Cdens
0.5
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
19.7 [arcmin]
- CN 0.56 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 31 is a moderately populated, very dense object of intermediate 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 (see Parameters). It is moderately studied in the literature.
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
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 | 285.919 | -8.458 | 1.841 | -0.289 | 1.169 | -16.336 |
| Li et al. | 2025 | 285.913 | -8.51 | 1.823 | -0.28 | 1.216 | â |
| Almeida et al. | 2025 | 285.908 | -8.574 | â | â | â | â |
| Alfonso et al. | 2024 | 285.957 | -8.458 | 1.795 | -0.294 | 1.169 | â |
| Hunt & Reffert | 2024 | 285.922 | -8.483 | 1.822 | -0.278 | 1.176 | -17.605 |
| Cavallo et al. | 2024 | 285.936 | -8.38 | 1.828 | â | â | â |
| Hunt & Reffert | 2023 | 285.922 | -8.483 | 1.822 | -0.278 | 1.176 | -17.605 |
| Tarricq et al. | 2022 | 285.876 | -8.442 | 1.858 | -0.292 | 1.118 | â |
| Dias et al. | 2021 | 285.908 | -8.574 | 1.827 | -0.281 | 1.203 | -16.265 |
| Cantat-Gaudin et al. | 2020 | 285.913 | -8.51 | 1.823 | -0.28 | 1.216 | â |
| Cantat-Gaudin & Anders | 2020 | 285.924 | -8.532 | 1.83 | -0.299 | 1.198 | â |
| Sim et al. | 2019 | 285.952 | -8.484 | â | -0.32 | 1.21 | 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 | 0.60 | 0.78 | â | 581 | 0.126 | â | â | â |
| Almeida et al. | 2025 | 0.54 | 0.83 | â | 618 | â | 81 | â | â |
| Alfonso et al. | 2024 | 0.54 | 0.61 | â | 657 | 0.006 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 103* | â | â |
| Cavallo et al. | 2024 | 0.55 | 1.05 | â | 339 | 0.130 | â | â | â |
| Hunt & Reffert | 2023 | 0.52 | 0.64 | 1.10 | 426 | â | â | â | â |
| Tarricq et al. | 2022 | 0.53 | â | â | 501 | â | â | â | â |
| Dias et al. | 2021 | 0.54 | 0.83 | â | 618 | 0.006 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.54 | 0.61 | â | 501 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.54 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.54 | â | â | 35 | 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. Silver sample.
Cavallo et al. (2024)
Gold sample.