UPK 585
0.65
UTI
0.55
CN
1.0
Cdens
0.5
CC3
0.6
Clit
1.0
Cdup
Stellar density (N50/rad)
5.8 [N/pc2]
- CN 0.55 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 585 is a moderately populated, very dense object of intermediate 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, young 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 | 212.543 | -75.904 | 1.377 | -6.871 | -5.551 | -21.823 |
| Li et al. | 2025 | 212.787 | -75.872 | 1.388 | -6.81 | -5.57 | â |
| Almeida et al. | 2025 | 212.864 | -75.768 | â | â | â | â |
| Alfonso et al. | 2024 | 211.898 | -75.922 | 1.33 | -6.899 | -5.241 | â |
| Cavallo et al. | 2024 | 212.95 | -75.745 | 1.395 | â | â | â |
| Hunt & Reffert | 2023 | 212.609 | -75.852 | 1.394 | -6.778 | -5.606 | -22.063 |
| Almeida et al. | 2023 | 212.838 | -75.693 | â | â | â | â |
| Dias et al. | 2021 | 212.864 | -75.768 | 1.416 | -6.766 | -5.532 | â |
| Cantat-Gaudin et al. | 2020 | 212.787 | -75.872 | 1.388 | -6.81 | -5.57 | â |
| Cantat-Gaudin & Anders | 2020 | 212.775 | -75.896 | 1.402 | -6.788 | -5.549 | â |
| Sim et al. | 2019 | 212.72 | -75.871 | â | -6.8 | -5.55 | 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 | 0.4 | 0.39 | 93 | -0.075 | 78 | 0.87 | â |
| Li et al. | 2025 | 0.79 | 0.35 | â | 91 | 0.267 | â | â | â |
| Almeida et al. | 2025 | 0.69 | 0.45 | â | 125 | â | 44 | â | â |
| Alfonso et al. | 2024 | 0.70 | 0.20 | â | 65 | -0.075 | â | â | â |
| Cavallo et al. | 2024 | 0.70 | 0.45 | â | 102 | 0.250 | â | â | â |
| Hunt & Reffert | 2023 | 0.68 | 0.22 | 0.39 | 95 | â | â | â | â |
| Almeida et al. | 2023 | 0.70 | 0.45 | â | 282 | -0.233 | 113(1) | 0.87 | â |
| Tarricq et al. | 2022 | 0.69 | â | â | 81 | â | â | â | â |
| Dias et al. | 2021 | 0.69 | 0.45 | â | 125 | -0.075 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.70 | 0.20 | â | 78 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.70 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.71 | 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: intermediate fit. Isochrone match: good fit.
Hunt & Reffert (2024)
Classified as a moving group.