UBC 177
0.53
UTI
0.56
CN
0.56
Cdens
0.75
CC3
0.4
Clit
1.0
Cdup
Stellar density (N50/rad)
2.8 [N/pc2]
- CN 0.56 Moderately populated
- Cdens 0.56 Moderately dense
- CC3 0.75 High quality
- Clit 0.4 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 177 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively 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 parameter (see Parameters). It is poorly studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 339.717 | 67.055 | 0.861 | -1.935 | -1.038 | -194.993 |
| Almeida et al. | 2025 | 339.647 | 67.057 | â | â | â | â |
| Celli et al. | 2024 | 339.659 | 67.044 | â | â | â | â |
| Almeida et al. | 2023 | 339.721 | 67.063 | â | â | â | â |
| He et al. | 2022 | 339.726 | 67.043 | 0.871 | -1.931 | -1.054 | â |
| Dias et al. | 2021 | 339.647 | 67.057 | 0.857 | -1.945 | -0.994 | â |
| Cantat-Gaudin et al. | 2020 | 339.659 | 67.044 | 0.855 | -1.973 | -0.973 | â |
| Castro-Ginard et al. | 2020 | 339.611 | 67.036 | 0.854 | -1.938 | -0.974 | 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 | 1.15 | 2.04 | â | 26 | 0.177 | 191 | 0.72 | â |
| Almeida et al. | 2025 | 1.15 | 2.04 | â | 21 | â | 262 | â | â |
| Celli et al. | 2024 | â | â | â | 28 | â | 184 | â | â |
| Almeida et al. | 2023 | 1.08 | 2.22 | â | 126 | 0.103 | 191(1) | 0.72 | â |
| He et al. | 2022 | â | 2.65 | â | 25 | â | â | â | â |
| Dias et al. | 2021 | 1.15 | 2.04 | â | 21 | 0.252 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.15 | 1.99 | â | 28 | 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: good fit.