UPK 645
0.78
UTI
0.5
CN
1.0
Cdens
1.0
CC3
0.69
Clit
1.0
Cdup
Stellar density (N50/rad)
15.8 [N/pc2]
- CN 0.5 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.69 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 645 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a close distance, below 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 270.129 | -42.787 | 1.427 | 2.746 | -2.887 | -3.256 |
| Li et al. | 2025 | 270.167 | -42.783 | 1.43 | 2.797 | -2.844 | â |
| Almeida et al. | 2025 | 270.129 | -42.708 | â | â | â | â |
| Alfonso et al. | 2024 | 270.179 | -42.767 | 1.38 | 2.735 | -2.888 | â |
| Hunt & Reffert | 2024 | 270.14 | -42.84 | 1.41 | 2.76 | -2.893 | -0.245 |
| Cavallo et al. | 2024 | 270.146 | -42.69 | 1.41 | â | â | â |
| Hunt & Reffert | 2023 | 270.14 | -42.84 | 1.41 | 2.76 | -2.893 | -0.245 |
| He et al. | 2022 | 270.175 | -42.785 | 1.403 | 2.751 | -2.924 | â |
| Tarricq et al. | 2022 | 270.182 | -42.794 | 1.442 | 2.771 | -2.887 | â |
| Dias et al. | 2021 | 270.129 | -42.708 | 1.432 | 2.772 | -2.847 | 2.807 |
| Cantat-Gaudin et al. | 2020 | 270.167 | -42.783 | 1.43 | 2.797 | -2.844 | â |
| Cantat-Gaudin & Anders | 2020 | 270.167 | -42.739 | 1.426 | 2.773 | -2.843 | â |
| Sim et al. | 2019 | 270.177 | -42.733 | â | 2.76 | -2.85 | 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 | 0.69 | 0.335 | 0.63 | 138 | -0.007 | 138 | â | â |
| Li et al. | 2025 | 0.71 | 0.17 | â | 501 | 0.131 | â | â | â |
| Almeida et al. | 2025 | 0.69 | 0.32 | â | 466 | â | 136 | â | â |
| Alfonso et al. | 2024 | 0.70 | 0.35 | â | 365 | -0.007 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 140(1) | â | â |
| Cavallo et al. | 2024 | 0.67 | 0.71 | â | 105 | -0.290 | â | â | â |
| Hunt & Reffert | 2023 | 0.67 | 0.19 | 0.63 | 160 | â | â | â | â |
| He et al. | 2022 | â | 0.60 | â | 50 | â | â | â | â |
| Tarricq et al. | 2022 | 0.68 | â | â | 115 | â | â | â | â |
| Dias et al. | 2021 | 0.69 | 0.32 | â | 466 | -0.007 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.70 | 0.35 | â | 105 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.69 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.68 | â | â | 89 | 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: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.