UPK 402
(OCSN 309)
0.76
UTI
0.49
CN
1.0
Cdens
1.0
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
10.1 [arcmin]
- CN 0.49 Poorly populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 402 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption 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.
Very close
Moderate extinction
Low mass
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 87.516 | 2.822 | 2.472 | -1.112 | -1.822 | 23.075 |
| Li et al. | 2025 | 87.515 | 2.822 | 2.385 | -1.112 | -1.917 | â |
| Alfonso et al. | 2024 | 87.517 | 2.812 | 2.431 | -1.137 | -1.805 | â |
| Hunt & Reffert | 2024 | 87.515 | 2.9 | 2.471 | -1.105 | -1.785 | 14.811 |
| Celli et al. | 2024 | 87.515 | 2.822 | â | â | â | â |
| Cavallo et al. | 2024 | 87.522 | 2.76 | 2.466 | â | â | â |
| Hunt & Reffert | 2023 | 87.515 | 2.9 | 2.471 | -1.105 | -1.785 | 14.811 |
| Qin et al. | 2023 | 87.5 | 2.91 | 2.46 | -1.05 | -1.66 | 30.19 |
| He et al. | 2022 | 87.509 | 2.819 | 2.47 | -1.096 | -1.809 | â |
| Cantat-Gaudin et al. | 2020 | 87.515 | 2.822 | 2.385 | -1.112 | -1.917 | â |
| Cantat-Gaudin & Anders | 2020 | 87.515 | 2.822 | 2.417 | -1.154 | -1.961 | â |
| Sim et al. | 2019 | 87.507 | 2.806 | â | -1.15 | -1.96 | 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 | 0.35 | 0.69 | â | 7 | -0.145 | â | â | â |
| Alfonso et al. | 2024 | 0.43 | 1.26 | â | 12 | 0.009 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 42* | â | â |
| Celli et al. | 2024 | â | â | â | 7 | â | 28 | â | â |
| Cavallo et al. | 2024 | 0.45 | 1.61 | â | 6 | 0.160 | â | â | â |
| Hunt & Reffert | 2023 | 0.39 | 1.12 | 1.50 | 5 | â | â | â | â |
| Qin et al. | 2023 | 0.49 | 0.46 | â | 6 | â | â | â | â |
| He et al. | 2022 | â | 0.15 | â | 3 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.43 | 1.26 | â | 7 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.41 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.43 | â | â | 7 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.