UPK 94
0.65
UTI
0.44
CN
0.67
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
12.9 [arcmin]
- CN 0.44 Poorly populated
- Cdens 0.67 Moderately dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 94 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is moderately studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Close
Moderate 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 | 304.788 | 27.606 | 1.036 | 2.104 | 1.03 | -11.423 |
| Li et al. | 2025 | 304.778 | 27.618 | 1.026 | 2.128 | 1.073 | â |
| Almeida et al. | 2025 | 304.765 | 27.592 | â | â | â | â |
| Alfonso et al. | 2024 | 304.722 | 27.623 | 1.008 | 2.139 | 1.012 | â |
| Hunt & Reffert | 2024 | 304.851 | 27.628 | 1.031 | 2.108 | 1.046 | -12.329 |
| Cavallo et al. | 2024 | 304.789 | 27.593 | 1.033 | â | â | â |
| Hunt & Reffert | 2023 | 304.851 | 27.628 | 1.031 | 2.108 | 1.046 | -12.329 |
| Almeida et al. | 2023 | 304.767 | 27.589 | â | â | â | â |
| Dias et al. | 2021 | 304.765 | 27.592 | 1.033 | 2.118 | 1.082 | â |
| Cantat-Gaudin et al. | 2020 | 304.778 | 27.618 | 1.026 | 2.128 | 1.073 | â |
| Cantat-Gaudin & Anders | 2020 | 304.778 | 27.618 | 1.028 | 2.124 | 1.121 | â |
| Sim et al. | 2019 | 304.754 | 27.623 | â | 2.12 | 1.06 | 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 | 0.82 | 0.87 | â | 794 | -0.241 | â | â | â |
| Almeida et al. | 2025 | 0.93 | 1.16 | â | 318 | â | 126 | â | â |
| Alfonso et al. | 2024 | 0.95 | 0.98 | â | 69 | 0.109 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 109* | â | â |
| Cavallo et al. | 2024 | 1.00 | 1.30 | â | 331 | -0.180 | â | â | â |
| Hunt & Reffert | 2023 | 0.93 | 0.96 | 0.50 | 272 | â | â | â | â |
| Almeida et al. | 2023 | 0.93 | 1.21 | â | 423 | -0.040 | 147* | 0.66 | â |
| Tarricq et al. | 2022 | 0.93 | â | â | 135 | â | â | â | â |
| Dias et al. | 2021 | 0.93 | 1.16 | â | 318 | 0.109 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.95 | 0.98 | â | 135 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.95 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.94 | â | â | 79 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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