UPK 220
0.84
UTI
0.83
CN
1.0
Cdens
1.0
CC3
0.69
Clit
1.0
Cdup
Stellar density (N50/rad)
22.2 [N/pc2]
- CN 0.83 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.69 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 220 is a rich, very dense object of very 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, young cluster, but with a large variance across recent sources for the age 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 350.954 | 66.505 | 1.03 | -2.4 | -2.649 | -6.177 |
| Almeida et al. | 2025 | 350.988 | 66.509 | â | â | â | â |
| Alfonso et al. | 2024 | -9.063 | 66.483 | 1.003 | -2.407 | -2.626 | â |
| Hunt & Reffert | 2024 | 350.954 | 66.462 | 1.032 | -2.391 | -2.655 | -2.191 |
| Cavallo et al. | 2024 | 350.932 | 66.503 | 1.03 | â | â | â |
| Hunt & Reffert | 2023 | 350.954 | 66.462 | 1.032 | -2.391 | -2.655 | -2.191 |
| Almeida et al. | 2023 | 350.88 | 66.452 | â | â | â | â |
| He et al. | 2022 | 350.996 | 66.517 | 1.033 | -2.419 | -2.644 | â |
| Tarricq et al. | 2022 | 350.961 | 66.487 | 1.023 | -2.388 | -2.685 | â |
| Dias et al. | 2021 | 350.988 | 66.509 | 1.008 | -2.414 | -2.592 | -7.194 |
| Cantat-Gaudin et al. | 2020 | 350.955 | 66.505 | 1.009 | -2.416 | -2.584 | â |
| Cantat-Gaudin & Anders | 2020 | 350.942 | 66.505 | 1.012 | -2.42 | -2.582 | â |
| Sim et al. | 2019 | 350.973 | 66.502 | â | -2.41 | -2.59 | 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 | 0.96 | 2.755 | 2.76 | 70 | 0.029 | 922 | 0.6 | â |
| Almeida et al. | 2025 | 0.95 | 2.73 | â | 20 | â | 591 | â | â |
| Alfonso et al. | 2024 | 0.99 | 2.16 | â | 53 | 0.029 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1284(1) | â | â |
| Cavallo et al. | 2024 | 1.08 | 2.96 | â | 85 | 0.630 | â | â | â |
| Hunt & Reffert | 2023 | 0.94 | 2.96 | 2.76 | 56 | â | â | â | â |
| Almeida et al. | 2023 | 0.94 | 2.78 | â | 30 | 0.025 | 922(1) | 0.60 | â |
| He et al. | 2022 | â | 3.30 | â | 112 | â | â | â | â |
| Tarricq et al. | 2022 | 0.96 | â | â | 120 | â | â | â | â |
| Dias et al. | 2021 | 0.95 | 2.73 | â | 20 | 0.029 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.99 | 2.16 | â | 110 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.96 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.97 | â | â | 562 | 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: intermediate fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.