UPK 54
0.80
UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
16.5 [arcmin]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
UPK 54 is a rich, very dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is well-studied in the literature.
Close
Moderate 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 | 286.129 | 15.73 | 1.203 | -0.569 | -5.886 | -3.225 |
| Li et al. | 2025 | 286.157 | 15.689 | 1.172 | -0.558 | -5.854 | â |
| Almeida et al. | 2025 | 286.169 | 15.645 | â | â | â | â |
| Alfonso et al. | 2024 | 286.407 | 15.258 | 1.114 | -0.57 | -5.937 | â |
| Hunt & Reffert | 2024 | 286.254 | 15.722 | 1.209 | -0.575 | -5.912 | -4.904 |
| Cavallo et al. | 2024 | 286.192 | 15.714 | 1.214 | â | â | â |
| Hunt & Reffert | 2023 | 286.254 | 15.722 | 1.209 | -0.575 | -5.912 | -4.904 |
| Almeida et al. | 2023 | 286.216 | 15.663 | â | â | â | â |
| He et al. | 2022 | 286.161 | 15.761 | 1.218 | -0.539 | -5.899 | â |
| Tarricq et al. | 2022 | 286.073 | 15.779 | 1.221 | -0.551 | -5.89 | â |
| Dias et al. | 2021 | 286.169 | 15.645 | 1.166 | -0.556 | -5.901 | 36.043 |
| Cantat-Gaudin et al. | 2020 | 286.157 | 15.689 | 1.172 | -0.558 | -5.854 | â |
| Cantat-Gaudin & Anders | 2020 | 286.132 | 15.682 | 1.189 | -0.559 | -5.864 | â |
| Sim et al. | 2019 | 286.112 | 15.681 | â | -0.57 | -5.88 | 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 | 0.83 | 0.99 | â | 142 | 0.359 | â | â | â |
| Almeida et al. | 2025 | 0.81 | 1.07 | â | 171 | â | 341 | â | â |
| Alfonso et al. | 2024 | 0.81 | 0.94 | â | 100 | 0.320 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 256* | â | â |
| Cavallo et al. | 2024 | 0.87 | 1.35 | â | 89 | 0.320 | â | â | â |
| Hunt & Reffert | 2023 | 0.80 | 1.17 | 0.60 | 77 | â | â | â | â |
| Almeida et al. | 2023 | 0.80 | 1.25 | â | 202 | -0.188 | 326* | 0.83 | â |
| He et al. | 2022 | â | 1.40 | â | 79 | â | â | â | â |
| Tarricq et al. | 2022 | 0.79 | â | â | 120 | â | â | â | â |
| Dias et al. | 2021 | 0.81 | 1.07 | â | 171 | 0.321 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.81 | 0.94 | â | 117 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.82 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.83 | â | â | 79 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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