UBC 415
0.69
UTI
0.41
CN
1.0
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Stellar density (N50/rad)
9.9 [N/pc2]
- CN 0.41 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
UBC 415 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 absorption and age parameters (see Parameters). It is moderately studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 42.55 | 72.914 | 1.113 | -1.333 | -1.678 | -22.877 |
| Liu et al. | 2025 | 42.51 | 72.9 | 1.12 | -1.3 | -1.69 | -26.06 |
| Li et al. | 2025 | 42.54 | 72.914 | 1.096 | -1.301 | -1.626 | â |
| Almeida et al. | 2025 | 42.555 | 72.901 | â | â | â | â |
| Alfonso et al. | 2024 | 44.901 | 72.026 | 0.879 | 0.1 | -1.529 | â |
| Hunt & Reffert | 2024 | 42.509 | 72.897 | 1.12 | -1.301 | -1.686 | -26.062 |
| Celli et al. | 2024 | 42.54 | 72.914 | â | â | â | â |
| Cavallo et al. | 2024 | 42.841 | 72.903 | 1.126 | â | â | â |
| Hunt & Reffert | 2023 | 42.509 | 72.897 | 1.12 | -1.301 | -1.686 | -26.062 |
| He et al. | 2022 | 42.659 | 72.898 | 1.124 | -1.331 | -1.68 | â |
| Dias et al. | 2021 | 42.555 | 72.901 | 1.08 | -1.309 | -1.607 | â |
| Cantat-Gaudin et al. | 2020 | 42.54 | 72.914 | 1.096 | -1.301 | -1.626 | â |
| Castro-Ginard et al. | 2020 | 42.531 | 72.895 | 1.092 | -1.279 | -1.613 | 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 | 0.89 | 1.26 | 0.86 | 17 | -0.067 | 87 | â | â |
| Liu et al. | 2025 | 1.08 | 0.36 | â | 29 | â | â | â | â |
| Li et al. | 2025 | 1.01 | 1.26 | â | 13 | -0.055 | â | â | â |
| Almeida et al. | 2025 | 0.89 | 1.58 | â | 17 | â | 87 | â | â |
| Alfonso et al. | 2024 | 0.83 | 1.06 | â | 80 | -0.078 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 91(1) | â | â |
| Celli et al. | 2024 | â | â | â | 23 | â | 57 | â | â |
| Cavallo et al. | 2024 | 0.95 | 1.33 | â | 14 | 0.190 | â | â | â |
| Hunt & Reffert | 2023 | 0.86 | 1.03 | 0.86 | 10 | â | â | â | â |
| He et al. | 2022 | â | 1.30 | â | 11 | â | â | â | â |
| Dias et al. | 2021 | 0.89 | 1.58 | â | 17 | -0.078 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.83 | 1.06 | â | 23 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 144 along with FSR_0569, and as primordial binary cluster 182 along with HSC_1082, and of multiple system 22 along with CWNU_77, FSR_0569 and HSC_1082.
Palma et al. (2025)
Part of multiple system G85, along with HSC_1052, HSC_1082, CWNU_77 and FSR_0569.
Cavallo et al. (2024)
Gold sample.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.