UPK 90
0.72
UTI
0.43
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
8.1 [arcmin]
- CN 0.43 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 90 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a close distance, near 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.
Close
Low extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 299.773 | 28.418 | 1.233 | -0.835 | -5.747 | -14.868 |
| Li et al. | 2025 | 299.777 | 28.422 | 1.228 | -0.824 | -5.705 | â |
| Almeida et al. | 2025 | 299.741 | 28.424 | â | â | â | â |
| Alfonso et al. | 2024 | 299.734 | 28.418 | 1.2 | -0.871 | -5.646 | â |
| Hunt & Reffert | 2024 | 299.726 | 28.434 | 1.227 | -0.837 | -5.698 | -13.589 |
| Cavallo et al. | 2024 | 299.769 | 28.437 | 1.236 | â | â | â |
| Hunt & Reffert | 2023 | 299.726 | 28.434 | 1.227 | -0.837 | -5.698 | -13.589 |
| He et al. | 2022 | 299.76 | 28.437 | 1.244 | -0.806 | -5.734 | â |
| Tarricq et al. | 2022 | 299.765 | 28.457 | 1.242 | -0.85 | -5.752 | â |
| Dias et al. | 2021 | 299.741 | 28.424 | 1.236 | -0.825 | -5.728 | â |
| Cantat-Gaudin et al. | 2020 | 299.777 | 28.422 | 1.228 | -0.824 | -5.705 | â |
| Cantat-Gaudin & Anders | 2020 | 299.773 | 28.419 | 1.231 | -0.837 | -5.719 | â |
| Sim et al. | 2019 | 299.787 | 28.408 | â | -0.83 | -5.72 | 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 | 0.92 | 1.07 | â | 179 | 0.144 | â | â | â |
| Almeida et al. | 2025 | 0.79 | 0.96 | â | 385 | â | 123 | â | â |
| Alfonso et al. | 2024 | 0.79 | 0.85 | â | 101 | 0.075 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 110* | â | â |
| Cavallo et al. | 2024 | 0.83 | 1.07 | â | 49 | -0.070 | â | â | â |
| Hunt & Reffert | 2023 | 0.78 | 0.80 | 0.80 | 122 | â | â | â | â |
| He et al. | 2022 | â | 1.25 | â | 50 | â | â | â | â |
| Tarricq et al. | 2022 | 0.78 | â | â | 55 | â | â | â | â |
| Dias et al. | 2021 | 0.79 | 0.96 | â | 385 | 0.076 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.79 | 0.85 | â | 49 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.79 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.79 | â | â | 45 | 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.