UPK 562
0.65
UTI
0.52
CN
0.8
Cdens
0.75
CC3
0.6
Clit
1.0
Cdup
Stellar density (N50/rad)
4.0 [N/pc2]
- CN 0.52 Moderately populated
- Cdens 0.8 Dense
- CC3 0.75 High quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 562 is a moderately populated, dense object of high C3 quality. Its parallax locates it at a 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 165.875 | -56.99 | 1.225 | -11.702 | 4.875 | -6.011 |
| Almeida et al. | 2025 | 165.957 | -56.964 | â | â | â | â |
| Alfonso et al. | 2024 | 166.12 | -56.973 | 1.18 | -11.671 | 4.77 | â |
| Hunt & Reffert | 2024 | 165.955 | -57.024 | 1.199 | -11.667 | 4.836 | -3.501 |
| Cavallo et al. | 2024 | 166.082 | -57.025 | 1.211 | â | â | â |
| Hunt & Reffert | 2023 | 165.955 | -57.024 | 1.199 | -11.667 | 4.836 | -3.501 |
| Almeida et al. | 2023 | 165.985 | -57.025 | â | â | â | â |
| Tarricq et al. | 2022 | 165.815 | -56.96 | 1.253 | -11.723 | 4.846 | â |
| Dias et al. | 2021 | 165.957 | -56.964 | 1.207 | -11.641 | 4.864 | 26.676 |
| Cantat-Gaudin et al. | 2020 | 165.861 | -56.978 | 1.199 | -11.688 | 4.876 | â |
| Cantat-Gaudin & Anders | 2020 | 165.875 | -56.967 | 1.214 | -11.668 | 4.847 | â |
| Sim et al. | 2019 | 165.861 | -56.952 | â | -11.67 | 4.85 | 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 | 0.8 | 0.31 | 0.63 | 222 | -0.033 | 189 | 0.7 | â |
| Almeida et al. | 2025 | 0.79 | 0.26 | â | 222 | â | 189 | â | â |
| Alfonso et al. | 2024 | 0.80 | 0.37 | â | 90 | -0.033 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 80(1) | â | â |
| Cavallo et al. | 2024 | 0.81 | 0.33 | â | 269 | 0.360 | â | â | â |
| Hunt & Reffert | 2023 | 0.77 | 0.13 | 0.63 | 506 | â | â | â | â |
| Almeida et al. | 2023 | 0.85 | 0.31 | â | 233 | -0.069 | 330(1) | 0.70 | â |
| Tarricq et al. | 2022 | 0.79 | â | â | 102 | â | â | â | â |
| Dias et al. | 2021 | 0.79 | 0.26 | â | 222 | -0.032 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.80 | 0.37 | â | 98 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.80 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.82 | â | â | 79 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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