UPK 84
0.30
UTI
0.77
CN
0.86
Cdens
1.0
CC3
0.6
Clit
0.4
Cdup
Radius (P>50% members)
21.8 [arcmin]
- CN 0.77 Rich
- Cdens 0.86 Dense
- CC3 1.0 Very high quality
- Clit 0.6 Moderately studied
- Cdup 0.4 Possibly duplicate
Overview
UPK 84 is a rich, dense object of very 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, old cluster (see Parameters). It is moderately studied in the literature.
â ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.
Close
Low extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 310.224 | 20.21 | 1.078 | -6.295 | -9.294 | 24.191 |
| Li et al. | 2025 | 310.245 | 20.212 | 1.08 | -6.258 | -9.248 | â |
| Almeida et al. | 2025 | 310.255 | 20.17 | â | â | â | â |
| Alfonso et al. | 2024 | 310.231 | 20.191 | 1.049 | -6.293 | -9.297 | â |
| Almeida et al. | 2023 | 310.236 | 20.186 | â | â | â | â |
| He et al. | 2022 | 310.201 | 20.115 | 1.074 | -6.286 | -9.3 | â |
| Tarricq et al. | 2022 | 310.191 | 20.082 | 1.097 | -6.287 | -9.303 | â |
| Dias et al. | 2021 | 310.255 | 20.17 | 1.097 | -6.298 | -9.272 | 24.598 |
| Cantat-Gaudin et al. | 2020 | 310.245 | 20.212 | 1.08 | -6.258 | -9.248 | â |
| Cantat-Gaudin & Anders | 2020 | 310.247 | 20.191 | 1.083 | -6.283 | -9.281 | â |
| Sim et al. | 2019 | 310.219 | 20.175 | â | -6.25 | -9.25 | 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 | 0.87 | 0.30 | â | 1243 | -0.147 | â | â | â |
| Almeida et al. | 2025 | 0.87 | 0.27 | â | 1183 | â | 147 | â | â |
| Alfonso et al. | 2024 | 0.95 | 0.31 | â | 954 | -0.059 | â | â | â |
| Almeida et al. | 2023 | 0.90 | 0.23 | â | 1138 | -0.011 | 242* | 0.53 | â |
| He et al. | 2022 | â | 0.30 | â | 1122 | â | â | â | â |
| Tarricq et al. | 2022 | 0.92 | â | â | 1023 | â | â | â | â |
| Dias et al. | 2021 | 0.87 | 0.27 | â | 1183 | -0.059 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.95 | 0.31 | â | 1000 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.90 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.90 | â | â | 562 | 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.