UBC 366
0.70
UTI
0.52
CN
1.0
Cdens
0.75
CC3
0.6
Clit
1.0
Cdup
Radius (P>50% members)
5.3 [arcmin]
- CN 0.52 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
UBC 366 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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.
Relatively close
Low extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 299.853 | 37.213 | 0.53 | -1.209 | -2.241 | -4.146 |
| Li et al. | 2025 | 299.841 | 37.204 | 0.529 | -1.204 | -2.233 | â |
| Hu & Soubiran | 2025 | 299.856 | 37.205 | â | â | â | â |
| Almeida et al. | 2025 | 299.849 | 37.211 | â | â | â | â |
| Hunt & Reffert | 2024 | 299.865 | 37.205 | 0.523 | -1.197 | -2.256 | -20.727 |
| Cavallo et al. | 2024 | 299.857 | 37.205 | 0.526 | â | â | â |
| Hunt & Reffert | 2023 | 299.865 | 37.205 | 0.523 | -1.197 | -2.256 | -20.727 |
| Almeida et al. | 2023 | 299.846 | 37.222 | â | â | â | â |
| Dias et al. | 2021 | 299.849 | 37.211 | 0.527 | -1.199 | -2.23 | -1.879 |
| Cantat-Gaudin et al. | 2020 | 299.841 | 37.204 | 0.529 | -1.204 | -2.233 | â |
| Castro-Ginard et al. | 2020 | 299.835 | 37.21 | 0.527 | -1.187 | -2.234 | 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 | 1.59 | 0.83 | â | 548 | -0.036 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.050* | â | â | â |
| Almeida et al. | 2025 | 1.81 | 1.02 | â | 305 | â | 129 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 273* | â | â |
| Cavallo et al. | 2024 | 1.74 | 0.68 | â | 589 | 0.400 | â | â | â |
| Hunt & Reffert | 2023 | 1.79 | 0.82 | 0.64 | 362 | â | â | â | â |
| Almeida et al. | 2023 | 1.73 | 0.97 | â | 448 | 0.053 | 164* | 0.54 | â |
| Dias et al. | 2021 | 1.81 | 1.02 | â | 305 | 0.154 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.79 | 0.83 | â | 380 | 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.
Cavallo et al. (2024)
Gold sample.