UPK 93
0.77
UTI
0.53
CN
1.0
Cdens
0.75
CC3
0.78
Clit
1.0
Cdup
Stellar density (N50/rad)
5.9 [N/pc2]
- CN 0.53 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.78 Well-studied
- Cdup 1.0 Unique
Overview
UPK 93 is a moderately populated, very dense object of 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, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 300.312 | 29.97 | 1.422 | -0.841 | -8.249 | 13.871 |
| Li et al. | 2025 | 300.324 | 29.971 | 1.414 | -0.863 | -8.206 | â |
| Almeida et al. | 2025 | 300.314 | 29.949 | â | â | â | â |
| Alfonso et al. | 2024 | 300.337 | 30.052 | 1.35 | -0.853 | -8.172 | â |
| Zhang et al. | 2024 | 300.315 | 29.945 | â | â | â | â |
| Hunt & Reffert | 2024 | 300.315 | 29.945 | 1.376 | -0.888 | -8.14 | 16.017 |
| Cavallo et al. | 2024 | 300.437 | 30.134 | 1.377 | â | â | â |
| Hunt & Reffert | 2023 | 300.315 | 29.945 | 1.376 | -0.888 | -8.14 | 16.017 |
| Almeida et al. | 2023 | 300.177 | 30.031 | â | â | â | â |
| He et al. | 2022 | 300.324 | 29.972 | 1.423 | -0.83 | -8.308 | â |
| Dias et al. | 2021 | 300.314 | 29.949 | 1.411 | -0.867 | -8.166 | 14.051 |
| Cantat-Gaudin et al. | 2020 | 300.324 | 29.971 | 1.414 | -0.863 | -8.206 | â |
| Cantat-Gaudin & Anders | 2020 | 300.312 | 29.971 | 1.4 | -0.882 | -8.153 | â |
| Sim et al. | 2019 | 300.309 | 29.96 | â | -0.85 | -8.28 | 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 | 0.69 | 0.36 | 0.44 | 564 | -0.094 | 121 | 0.79 | â |
| Li et al. | 2025 | 0.75 | 0.58 | â | 476 | -0.347 | â | â | â |
| Almeida et al. | 2025 | 0.68 | 0.36 | â | 575 | â | 110 | â | â |
| Alfonso et al. | 2024 | 0.69 | 0.32 | â | 676 | -0.094 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.070(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 121(1) | â | â |
| Cavallo et al. | 2024 | 0.76 | 0.54 | â | 309 | 0.450 | â | â | â |
| Hunt & Reffert | 2023 | 0.68 | 0.17 | 0.44 | 564 | â | â | â | â |
| Almeida et al. | 2023 | 0.64 | 0.41 | â | 583 | -0.228 | 166(1) | 0.79 | â |
| He et al. | 2022 | â | 0.30 | â | 794 | â | â | â | â |
| Tarricq et al. | 2022 | 0.68 | â | â | 550 | â | â | â | â |
| Dias et al. | 2021 | 0.68 | 0.36 | â | 575 | -0.094 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.69 | 0.32 | â | 513 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.70 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.69 | â | â | 398 | 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.