UPK 654
(OCSN 323)
0.78
UTI
0.64
CN
1.0
Cdens
1.0
CC3
0.62
Clit
1.0
Cdup
Stellar density (N50/rad)
10.9 [N/pc2]
- CN 0.64 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.62 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 654 is a moderately populated, very 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, young cluster, but with a large variance across recent sources for the age parameter (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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 277.301 | -34.542 | 1.968 | 1.189 | -8.667 | 0.649 |
| Li et al. | 2025 | 277.329 | -34.528 | 1.97 | 1.165 | -8.67 | â |
| Almeida et al. | 2025 | 277.283 | -34.527 | â | â | â | â |
| Alfonso et al. | 2024 | 277.22 | -34.52 | 1.925 | 1.172 | -8.656 | â |
| Almeida et al. | 2023 | 277.208 | -34.473 | â | â | â | â |
| Qin et al. | 2023 | 277.35 | -34.52 | 1.95 | 1.19 | -8.71 | 0.97 |
| He et al. | 2022 | 277.308 | -34.502 | 1.964 | 1.205 | -8.721 | â |
| Tarricq et al. | 2022 | 277.348 | -34.451 | 1.978 | 1.181 | -8.643 | â |
| Dias et al. | 2021 | 277.283 | -34.527 | 1.96 | 1.157 | -8.652 | 5.384 |
| Cantat-Gaudin et al. | 2020 | 277.329 | -34.528 | 1.97 | 1.165 | -8.67 | â |
| Cantat-Gaudin & Anders | 2020 | 277.32 | -34.528 | 1.967 | 1.206 | -8.621 | â |
| Sim et al. | 2019 | 277.359 | -34.49 | â | 1.13 | -8.65 | 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 | 0.505 | 0.505 | â | 98 | -0.046 | 108 | 0.5 | â |
| Li et al. | 2025 | 0.52 | 0.50 | â | 95 | 0.057 | â | â | â |
| Almeida et al. | 2025 | 0.50 | 0.51 | â | 133 | â | 112 | â | â |
| Alfonso et al. | 2024 | 0.52 | 0.16 | â | 68 | -0.046 | â | â | â |
| Almeida et al. | 2023 | 0.50 | 0.46 | â | 329 | -0.048 | 105(1) | 0.50 | â |
| Qin et al. | 2023 | 0.69 | 0.78 | â | 251 | â | â | â | â |
| He et al. | 2022 | â | 0.60 | â | 71 | â | â | â | â |
| Tarricq et al. | 2022 | 0.51 | â | â | 83 | â | â | â | â |
| Dias et al. | 2021 | 0.50 | 0.51 | â | 133 | -0.047 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.52 | 0.16 | â | 79 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.50 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.50 | â | â | 100 | 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. Silver sample.