OC 0282
0.42
UTI
0.29
CN
1.0
Cdens
0.12
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
5.2 [N/pc2]
- CN 0.29 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.12 Very low quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
OC 0282 is a poorly populated, very dense object of very low C3 quality. Its parallax locates it at a relatively close distance, near 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 age parameter (see Parameters). It is poorly studied in the literature.
Note: This object shares a large 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 | 74.97 | 38.683 | 0.54 | 0.02 | -3.575 | -20.206 |
| Hu & Soubiran | 2025 | 74.966 | 38.66 | â | â | â | â |
| Zhang et al. | 2024 | 74.995 | 38.688 | â | â | â | â |
| Hunt & Reffert | 2024 | 74.995 | 38.688 | 0.537 | 0.043 | -3.558 | -20.211 |
| Cavallo et al. | 2024 | 74.967 | 38.66 | 0.537 | â | â | â |
| Hunt & Reffert | 2023 | 74.995 | 38.688 | 0.537 | 0.043 | -3.558 | -20.211 |
| Hao et al. | 2022 | 74.977 | 38.67 | 0.556 | 0.055 | -3.556 | -20.25 |
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 | 1.665 | 1.56 | 0.61 | 174 | -0.108 | 124 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.130(5) | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.106(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 124(1) | â | â |
| Cavallo et al. | 2024 | 1.62 | 1.56 | â | 562 | -0.110 | â | â | â |
| Hunt & Reffert | 2023 | 1.71 | 1.42 | 0.61 | 174 | â | â | â | â |
| Hao et al. | 2022 | â | 3.24 | â | 126 | 0.051 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.