UBC 582
0.74
UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.6
Clit
1.0
Cdup
Stellar density (N50/rad)
10.9 [N/pc2]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
UBC 582 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age 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 | 299.849 | 38.553 | 0.881 | -3.024 | -7.863 | 0.069 |
| Li et al. | 2025 | 299.833 | 38.551 | 0.895 | -3.06 | -7.856 | â |
| Almeida et al. | 2025 | 299.843 | 38.548 | â | â | â | â |
| Hunt & Reffert | 2024 | 299.861 | 38.559 | 0.868 | -2.997 | -7.868 | -0.822 |
| Cavallo et al. | 2024 | 299.848 | 38.558 | 0.879 | â | â | â |
| Hunt & Reffert | 2023 | 299.861 | 38.559 | 0.868 | -2.997 | -7.868 | -0.822 |
| Almeida et al. | 2023 | 299.868 | 38.547 | â | â | â | â |
| He et al. | 2022 | 299.869 | 38.564 | 0.887 | -3.019 | -7.883 | â |
| Tarricq et al. | 2022 | 299.867 | 38.513 | 0.89 | -3.035 | -7.835 | â |
| Dias et al. | 2021 | 299.843 | 38.548 | 0.897 | -3.063 | -7.819 | â |
| Cantat-Gaudin et al. | 2020 | 299.833 | 38.551 | 0.895 | -3.06 | -7.856 | â |
| Castro-Ginard et al. | 2020 | 299.836 | 38.546 | 0.896 | -3.066 | -7.854 | 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 | 1.085 | 0.45 | 0.73 | 18 | -0.047 | 97 | 0.4 | â |
| Li et al. | 2025 | 0.93 | 0.41 | â | 19 | -0.249 | â | â | â |
| Almeida et al. | 2025 | 1.10 | 0.65 | â | 18 | â | 55 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 208(1) | â | â |
| Cavallo et al. | 2024 | 1.08 | 0.48 | â | 10 | -0.080 | â | â | â |
| Hunt & Reffert | 2023 | 1.09 | 0.19 | 0.73 | 9 | â | â | â | â |
| Almeida et al. | 2023 | 1.10 | 0.52 | â | 18 | 0.044 | 97(1) | 0.40 | â |
| He et al. | 2022 | â | 0.30 | â | 11 | â | â | â | â |
| Tarricq et al. | 2022 | 0.99 | â | â | 69 | â | â | â | â |
| Dias et al. | 2021 | 1.10 | 0.65 | â | 18 | -0.014 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.02 | 0.42 | â | 63 | 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.