UBC 424
0.51
UTI
0.57
CN
0.56
Cdens
0.75
CC3
0.32
Clit
1.0
Cdup
Nm (P>50%)
65
Core radius and density
1.2 [pc], 2.8 [pc-2]
- CN 0.57 Moderately populated
- Cdens 0.56 Moderately dense
- CC3 0.75 High quality
- Clit 0.32 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 424 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate 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 poorly studied in the literature.
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 50.968 | 51.239 | 0.435 | 0.006 | -1.694 | -40.764 |
| Li et al. | 2025 | 50.967 | 51.237 | 0.413 | 0.073 | -1.67 | â |
| Almeida et al. | 2025 | 50.992 | 51.261 | â | â | â | â |
| Zhang et al. | 2024 | 50.959 | 51.238 | â | â | â | â |
| Hunt & Reffert | 2024 | 50.958 | 51.238 | 0.443 | 0.001 | -1.68 | -40.765 |
| Cavallo et al. | 2024 | 50.972 | 51.262 | 0.443 | â | â | â |
| Hunt & Reffert | 2023 | 50.958 | 51.238 | 0.443 | 0.001 | -1.68 | -40.765 |
| Almeida et al. | 2023 | 50.998 | 51.268 | â | â | â | â |
| Jadhav & Subramaniam | 2021 | 50.967 | 51.237 | â | â | â | â |
| Dias et al. | 2021 | 50.992 | 51.261 | 0.396 | 0.088 | -1.607 | â |
| Cantat-Gaudin et al. | 2020 | 50.967 | 51.237 | 0.413 | 0.073 | -1.67 | â |
| Castro-Ginard et al. | 2020 | 50.976 | 51.258 | 0.42 | 0.067 | -1.646 | 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 | 2.08 | 1.725 | 1.25 | 432 | -0.137 | 344 | 0.62 | 0 |
| Li et al. | 2025 | 1.78 | 1.65 | â | 744 | -0.137 | â | â | â |
| Almeida et al. | 2025 | 2.08 | 1.91 | â | 430 | â | 422 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.168(1) | â | â | â |
| Hunt & Reffert | 2024 | 2.06 | 1.58 | 1.25 | 434 | â | 375(1) | â | â |
| Cavallo et al. | 2024 | 2.12 | 1.77 | â | 372 | 0.330 | â | â | â |
| Hunt & Reffert | 2023 | 2.06 | 1.58 | 1.25 | 435 | â | â | â | â |
| Almeida et al. | 2023 | 1.96 | 1.97 | â | 493 | -0.139 | 303(1) | 0.62 | â |
| Jadhav & Subramaniam | 2021 | 2.25 | 1.68 | â | 389 | â | 314 | â | 0(1) |
| Dias et al. | 2021 | 2.08 | 1.91 | â | 430 | -0.074 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.25 | 1.68 | â | 389 | â | â | â | â |
| Kounkel et al. | 2020 | 2.17 | 2.38 | â | 437 | 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: good fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).