Ryu 212
Summary
Ryu 212 is a poorly populated, very dense object of low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.
This object shares a small percentage of members with 2 later reported entries.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Bica et al. (2019) | 274.224 | -16.312 | – | – | – | – |
| UCC | 274.212 | -16.306 | 0.328 | -0.356 | -2.386 | -0.921 |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 1756 | 13.3 | 274.02 | -16.4 | 0.31 | -0.5 | -2.12 | 14.97 | 0.51 |
| CWNU 2798 | 3.3 | 274.01 | -16.47 | 0.32 | -0.77 | -2.55 | 30.15 | 0.44 |