UBC 178
0.72
UTI
0.47
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
7.8 [arcmin]
- CN 0.47 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UBC 178 is a poorly 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 and mass parameters (see Parameters). It is moderately studied in the literature.
Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.
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 | 346.168 | 63.361 | 1.163 | -1.223 | -1.839 | -14.65 |
| Li et al. | 2025 | 346.201 | 63.36 | 1.148 | -1.235 | -1.823 | â |
| Almeida et al. | 2025 | 346.212 | 63.326 | â | â | â | â |
| Alfonso et al. | 2024 | -14.273 | 63.157 | 1.142 | -1.149 | -2.05 | â |
| Hunt & Reffert | 2024 | 346.148 | 63.355 | 1.176 | -1.127 | -1.896 | 0.73 |
| Celli et al. | 2024 | 346.201 | 63.36 | â | â | â | â |
| Cavallo et al. | 2024 | 346.281 | 63.321 | 1.174 | â | â | â |
| Hunt & Reffert | 2023 | 346.148 | 63.355 | 1.176 | -1.127 | -1.896 | 0.73 |
| Almeida et al. | 2023 | 346.201 | 63.325 | â | â | â | â |
| He et al. | 2022 | 344.226 | 62.745 | 1.187 | -1.16 | -2.364 | â |
| Dias et al. | 2021 | 346.212 | 63.326 | 1.146 | -1.2 | -1.834 | â |
| Cantat-Gaudin et al. | 2020 | 346.201 | 63.36 | 1.148 | -1.235 | -1.823 | â |
| Castro-Ginard et al. | 2020 | 346.228 | 63.357 | 1.148 | -1.228 | -1.803 | 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 | 0.64 | 2.28 | â | 8 | -0.353 | â | â | â |
| Almeida et al. | 2025 | 0.87 | 1.98 | â | 11 | â | 522 | â | â |
| Alfonso et al. | 2024 | 0.94 | 1.58 | â | 10 | 0.244 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 106* | â | â |
| Celli et al. | 2024 | â | â | â | 10 | â | 308 | â | â |
| Cavallo et al. | 2024 | 0.82 | 2.05 | â | 6 | -0.030 | â | â | â |
| Hunt & Reffert | 2023 | 0.82 | 1.95 | 1.30 | 4 | â | â | â | â |
| Almeida et al. | 2023 | 0.83 | 2.11 | â | 8 | -0.047 | 576* | 0.61 | â |
| He et al. | 2022 | â | 2.80 | â | 3 | â | â | â | â |
| Dias et al. | 2021 | 0.87 | 1.98 | â | 11 | 0.245 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.95 | 1.58 | â | 10 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.