UPK 82
0.87
UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.78
Clit
1.0
Cdup
Stellar density (N50/rad)
7.3 [N/pc2]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.78 Well-studied
- Cdup 1.0 Unique
Overview
UPK 82 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is well-studied in the literature.
Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 298.354 | 26.412 | 1.838 | 2.297 | -2.152 | -17.006 |
| Li et al. | 2025 | 298.285 | 26.379 | 1.842 | 2.358 | -2.138 | â |
| Almeida et al. | 2025 | 298.264 | 26.397 | â | â | â | â |
| Alfonso et al. | 2024 | 298.102 | 26.438 | 1.777 | 2.12 | -2.206 | â |
| Zhang et al. | 2024 | 298.464 | 26.202 | â | â | â | â |
| Hunt & Reffert | 2024 | 298.464 | 26.202 | 1.822 | 2.278 | -2.169 | -16.125 |
| Cavallo et al. | 2024 | 298.243 | 26.412 | 1.828 | â | â | â |
| Hunt & Reffert | 2023 | 298.464 | 26.202 | 1.822 | 2.278 | -2.169 | -16.125 |
| Almeida et al. | 2023 | 298.214 | 26.464 | â | â | â | â |
| He et al. | 2022 | 298.378 | 26.385 | 1.845 | 2.319 | -2.153 | â |
| Tarricq et al. | 2022 | 298.15 | 26.172 | 1.825 | 2.292 | -2.135 | â |
| Dias et al. | 2021 | 298.264 | 26.397 | 1.836 | 2.37 | -2.139 | -12.417 |
| Cantat-Gaudin et al. | 2020 | 298.285 | 26.379 | 1.842 | 2.358 | -2.138 | â |
| Cantat-Gaudin & Anders | 2020 | 298.285 | 26.39 | 1.842 | 2.375 | -2.135 | â |
| Sim et al. | 2019 | 298.291 | 26.394 | â | 2.34 | -2.13 | 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 | 0.53 | 0.38 | 0.7 | 83 | 0.021 | 156 | 0.62 | â |
| Li et al. | 2025 | 0.53 | 0.35 | â | 87 | 0.043 | â | â | â |
| Almeida et al. | 2025 | 0.53 | 0.41 | â | 150 | â | 156 | â | â |
| Alfonso et al. | 2024 | 0.55 | 0.38 | â | 83 | 0.034 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.009(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 153(1) | â | â |
| Cavallo et al. | 2024 | 0.55 | 0.84 | â | 38 | -0.200 | â | â | â |
| Hunt & Reffert | 2023 | 0.53 | 0.18 | 0.70 | 78 | â | â | â | â |
| Almeida et al. | 2023 | 0.50 | 0.38 | â | 132 | -0.051 | 212(1) | 0.62 | â |
| He et al. | 2022 | â | 0.70 | â | 63 | â | â | â | â |
| Tarricq et al. | 2022 | 0.55 | â | â | 85 | â | â | â | â |
| Dias et al. | 2021 | 0.53 | 0.41 | â | 150 | 0.034 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.55 | 0.38 | â | 81 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.53 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.54 | â | â | 79 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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