UBC 54
0.76
UTI
0.83
CN
1.0
Cdens
0.75
CC3
0.6
Clit
1.0
Cdup
Stellar density (N50/rad)
16.2 [N/pc2]
- CN 0.83 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
UBC 54 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near 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 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 | 64.706 | 46.453 | 0.903 | 3.265 | -3.808 | -18.994 |
| Li et al. | 2025 | 64.747 | 46.453 | 0.879 | 3.32 | -3.758 | â |
| Wei et al. | 2025 | 64.751 | 46.445 | 0.91 | 3.259 | -3.813 | â |
| Zhang et al. | 2024 | 64.725 | 46.415 | â | â | â | â |
| Hunt & Reffert | 2024 | 64.725 | 46.415 | 0.908 | 3.275 | -3.809 | -20.361 |
| Cavallo et al. | 2024 | 64.714 | 46.453 | 0.908 | â | â | â |
| Hunt & Reffert | 2023 | 64.725 | 46.415 | 0.908 | 3.275 | -3.809 | -20.361 |
| He et al. | 2022 | 64.72 | 46.438 | 0.914 | 3.269 | -3.8 | â |
| Tarricq et al. | 2022 | 64.807 | 46.443 | 0.907 | 3.264 | -3.809 | â |
| Cantat-Gaudin et al. | 2020 | 64.747 | 46.453 | 0.879 | 3.32 | -3.758 | â |
| Cantat-Gaudin & Anders | 2020 | 64.747 | 46.453 | 0.879 | 3.32 | -3.758 | â |
| Castro-Ginard et al. | 2019 | 64.721 | 46.439 | 0.878 | 3.325 | -3.79 | 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 | 1.1 | 1.095 | 0.82 | 288 | 0.097 | 694 | 0.36 | â |
| Li et al. | 2025 | 1.00 | 1.05 | â | 413 | -0.056 | â | â | â |
| Wei et al. | 2025 | 1.76 | 1.23 | â | 288 | 0.250 | 430 | 0.36 | â |
| Zhang et al. | 2024 | â | â | â | â | -0.132(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 957(1) | â | â |
| Cavallo et al. | 2024 | 1.15 | 1.14 | â | 372 | 0.320 | â | â | â |
| Hunt & Reffert | 2023 | 1.04 | 0.97 | 0.82 | 280 | â | â | â | â |
| He et al. | 2022 | â | 1.25 | â | 224 | â | â | â | â |
| Tarricq et al. | 2022 | 1.07 | â | â | 295 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.11 | 0.98 | â | 251 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.10 | â | â | â | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Part of multiple system G74, along with LP_2139 and HSC_1255.
Cavallo et al. (2024)
Gold sample.