UBC 596
0.21
UTI
0.0
CN
0.22
Cdens
0.38
CC3
0.23
Clit
1.0
Cdup
Nm (P>50%)
20
Core radius and density
1.4 [pc], 1.1 [pc-2]
- CN 0.0 Sparse
- Cdens 0.22 Very loose
- CC3 0.38 Low quality
- Clit 0.23 Rarely studied
- Cdup 1.0 Unique
Overview
UBC 596 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 3.385 | 53.833 | 0.513 | -2.199 | -1.044 | â |
| Almeida et al. | 2025 | 3.37 | 53.822 | â | â | â | â |
| Zhang et al. | 2024 | 3.414 | 53.827 | â | â | â | â |
| Hunt & Reffert | 2024 | 3.414 | 53.827 | 0.516 | -2.135 | -1.134 | â |
| Cavallo et al. | 2024 | 3.415 | 53.832 | 0.515 | â | â | â |
| Hunt & Reffert | 2023 | 3.414 | 53.827 | 0.516 | -2.135 | -1.134 | â |
| Dias et al. | 2021 | 3.37 | 53.822 | 0.48 | -2.229 | -1.031 | â |
| Cantat-Gaudin et al. | 2020 | 3.36 | 53.832 | 0.527 | -2.193 | -0.973 | â |
| Castro-Ginard et al. | 2020 | 3.391 | 53.832 | 0.532 | -2.221 | -1.008 | 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 | 1.84 | 0.85 | 0.42 | 104 | -0.216 | 70 | â | â |
| Almeida et al. | 2025 | 1.74 | 0.88 | â | 242 | â | 60 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.216(1) | â | â | â |
| Hunt & Reffert | 2024 | 1.93 | 0.61 | 0.42 | 104 | â | 81(1) | â | â |
| Cavallo et al. | 2024 | 1.80 | 0.85 | â | 76 | -0.240 | â | â | â |
| Hunt & Reffert | 2023 | 1.93 | 0.61 | 0.42 | 104 | â | â | â | â |
| Dias et al. | 2021 | 1.74 | 0.88 | â | 242 | -0.079 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.84 | 0.32 | â | 141 | â | â | â | â |
| Kounkel et al. | 2020 | 1.91 | 1.31 | â | 50 | 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.
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).