UPK 169
0.78
UTI
0.64
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
13.6 [arcmin]
- CN 0.64 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
UPK 169 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is well-studied in the literature.
Close
Moderate extinction
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 | 326.698 | 59.778 | 1.169 | -1.997 | -2.464 | -14.553 |
| Li et al. | 2025 | 326.718 | 59.915 | 1.155 | -2.004 | -2.4 | â |
| Almeida et al. | 2025 | 326.752 | 59.796 | â | â | â | â |
| Alfonso et al. | 2024 | 326.695 | 59.77 | 1.142 | -1.981 | -2.507 | â |
| Hunt & Reffert | 2024 | 326.741 | 59.722 | 1.154 | -2.001 | -2.518 | -15.695 |
| Celli et al. | 2024 | 326.718 | 59.915 | â | â | â | â |
| Cavallo et al. | 2024 | 326.596 | 59.871 | 1.173 | â | â | â |
| Hunt & Reffert | 2023 | 326.741 | 59.722 | 1.154 | -2.001 | -2.518 | -15.695 |
| Almeida et al. | 2023 | 326.818 | 59.705 | â | â | â | â |
| He et al. | 2022 | 326.758 | 59.754 | 1.169 | -1.956 | -2.535 | â |
| Dias et al. | 2021 | 326.752 | 59.796 | 1.158 | -2.009 | -2.378 | â |
| Cantat-Gaudin et al. | 2020 | 326.718 | 59.915 | 1.155 | -2.004 | -2.4 | â |
| Cantat-Gaudin & Anders | 2020 | 326.794 | 59.803 | 1.158 | -2.007 | -2.398 | â |
| Sim et al. | 2019 | 326.749 | 59.848 | â | -1.95 | -2.36 | 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 | 0.68 | 2.25 | â | 16 | -0.163 | â | â | â |
| Almeida et al. | 2025 | 0.82 | 1.78 | â | 12 | â | 105 | â | â |
| Alfonso et al. | 2024 | 0.90 | 1.47 | â | 11 | -0.024 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 319* | â | â |
| Celli et al. | 2024 | â | â | â | 14 | â | 255 | â | â |
| Cavallo et al. | 2024 | 0.92 | 2.23 | â | 11 | 0.600 | â | â | â |
| Hunt & Reffert | 2023 | 0.82 | 2.52 | 2.49 | 7 | â | â | â | â |
| Almeida et al. | 2023 | 0.83 | 2.44 | â | 15 | -0.286 | 358* | 0.65 | â |
| He et al. | 2022 | â | 2.40 | â | 9 | â | â | â | â |
| Dias et al. | 2021 | 0.82 | 1.78 | â | 12 | -0.024 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.90 | 1.47 | â | 14 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.84 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.84 | â | â | 13 | 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. Silver sample.
Cavallo et al. (2024)
Gold sample.