UBC 212
0.01
UTI
0.68
CN
1.0
Cdens
0.75
CC3
0.31
Clit
0.01
Cdup
Radius (P>50% members)
2.5 [arcmin]
- CN 0.68 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.31 Poorly studied
- Cdup 0.01 Very likely duplicate
Overview
UBC 212 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
â ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.
Relatively close
Low extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 100.966 | -0.885 | 0.34 | -0.648 | 0.673 | 64.633 |
| Hu & Soubiran | 2025 | 100.966 | -0.879 | â | â | â | â |
| Cavallo et al. | 2024 | 100.966 | -0.879 | 0.33 | â | â | â |
| Hunt & Reffert | 2023 | 100.97 | -0.884 | 0.326 | -0.616 | 0.655 | 64.112 |
| Cantat-Gaudin et al. | 2020 | 100.957 | -0.886 | 0.335 | -0.618 | 0.659 | â |
| Castro-Ginard et al. | 2020 | 100.945 | -0.878 | 0.34 | -0.604 | 0.652 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.270* | â | â | â |
| Cavallo et al. | 2024 | 2.73 | 0.93 | â | 1047 | 0.490 | â | â | â |
| Hunt & Reffert | 2023 | 2.64 | 0.89 | 0.66 | 701 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.81 | 0.90 | â | 1072 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.