UBC 482
0.22
UTI
0.0
CN
0.08
Cdens
0.5
CC3
0.26
Clit
1.0
Cdup
Nm (P>50%)
23
Core radius and density
2.6 [pc], 0.4 [pc-2]
- CN 0.0 Sparse
- Cdens 0.08 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.26 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 482 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a moderate percentage of members with 3 later reported entries. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 131.054 | -45.93 | 0.457 | -5.137 | 5.03 | â |
| Li et al. | 2025 | 131.14 | -45.951 | 0.446 | -5.155 | 4.977 | â |
| Almeida et al. | 2025 | 131.155 | -45.972 | â | â | â | â |
| Hunt & Reffert | 2024 | 130.941 | -45.876 | 0.456 | -5.091 | 5.011 | 29.639 |
| Celli et al. | 2024 | 131.14 | -45.951 | â | â | â | â |
| Cavallo et al. | 2024 | 131.164 | -46.006 | 0.456 | â | â | â |
| Hunt & Reffert | 2023 | 130.941 | -45.876 | 0.456 | -5.091 | 5.011 | 29.639 |
| Dias et al. | 2021 | 131.155 | -45.972 | 0.445 | -5.169 | 4.966 | 29.322 |
| Cantat-Gaudin et al. | 2020 | 131.14 | -45.951 | 0.446 | -5.155 | 4.977 | â |
| Castro-Ginard et al. | 2020 | 131.154 | -45.961 | 0.45 | -5.164 | 4.972 | 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 | 2.0 | 1.09 | 2.52 | 27 | -0.007 | 499 | â | â |
| Li et al. | 2025 | 1.97 | 0.96 | â | 24 | -0.050 | â | â | â |
| Almeida et al. | 2025 | 2.00 | 1.14 | â | 21 | â | 1048 | â | â |
| Hunt & Reffert | 2024 | 2.00 | 1.06 | 2.52 | 51 | â | 409(1) | â | â |
| Celli et al. | 2024 | â | â | â | 27 | â | 499 | â | â |
| Cavallo et al. | 2024 | 1.97 | 1.12 | â | 98 | 0.130 | â | â | â |
| Hunt & Reffert | 2023 | 2.00 | 1.06 | 2.52 | 51 | â | â | â | â |
| Dias et al. | 2021 | 2.00 | 1.14 | â | 21 | -0.007 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.25 | 0.88 | â | 27 | â | â | â | â |
| Kounkel et al. | 2020 | 2.11 | 1.40 | â | 28 | 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)
Classified as optical pair P366, along with CWNU_2907.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.99 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.99 (50th percentile).