UPK 66
0.75
UTI
0.66
CN
0.92
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
21.4 [arcmin]
- CN 0.66 Moderately populated
- Cdens 0.92 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 66 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
Close
Low 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 | 305.356 | 13.447 | 1.471 | 0.453 | -10.003 | -7.024 |
| Li et al. | 2025 | 305.39 | 13.509 | 1.459 | 0.496 | -9.95 | â |
| Almeida et al. | 2025 | 305.392 | 13.464 | â | â | â | â |
| Alfonso et al. | 2024 | 305.416 | 13.453 | 1.447 | 0.44 | -10.004 | â |
| Hunt & Reffert | 2024 | 305.283 | 13.343 | 1.472 | 0.428 | -10.053 | -5.494 |
| Cavallo et al. | 2024 | 305.375 | 13.332 | 1.48 | â | â | â |
| Hunt & Reffert | 2023 | 305.283 | 13.343 | 1.472 | 0.428 | -10.053 | -5.494 |
| He et al. | 2022 | 305.468 | 13.499 | 1.499 | 0.43 | -10.005 | â |
| Tarricq et al. | 2022 | 305.335 | 13.423 | 1.468 | 0.466 | -10.011 | â |
| Dias et al. | 2021 | 305.392 | 13.464 | 1.463 | 0.481 | -9.962 | -7.154 |
| Cantat-Gaudin et al. | 2020 | 305.39 | 13.509 | 1.459 | 0.496 | -9.95 | â |
| Cantat-Gaudin & Anders | 2020 | 305.37 | 13.468 | 1.453 | 0.533 | -9.976 | â |
| Sim et al. | 2019 | 305.337 | 13.478 | â | 0.51 | -9.93 | 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 | 0.69 | 0.15 | â | 165 | 0.168 | â | â | â |
| Almeida et al. | 2025 | 0.67 | 0.26 | â | 183 | â | 81 | â | â |
| Alfonso et al. | 2024 | 0.67 | 0.26 | â | 138 | -0.012 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 98* | â | â |
| Cavallo et al. | 2024 | 0.68 | 0.56 | â | 107 | 0.130 | â | â | â |
| Hunt & Reffert | 2023 | 0.65 | 0.15 | 0.50 | 236 | â | â | â | â |
| He et al. | 2022 | â | 0.65 | â | 126 | â | â | â | â |
| Tarricq et al. | 2022 | 0.65 | â | â | 155 | â | â | â | â |
| Dias et al. | 2021 | 0.67 | 0.26 | â | 183 | -0.012 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.67 | 0.26 | â | 148 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.67 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.67 | â | â | 126 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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