CWNU 2285
Summary
CWNU 2285 is a poorly populated, moderately dense object of high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.
This object shares a large percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 229.76 | -60.024 | 0.314 | -3.8 | -3.001 | -38.88 |
| UCC | 229.732 | -60.013 | 0.306 | -3.815 | -3.001 | -45.533 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.05, m-M=12.2, logAge=7.9 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 3114 | 79.3 | 229.73 | -60.0 | 0.3 | -3.8 | -2.99 | -45.53 | 0.03 |