Ryu 912
Summary
Ryu 912 is a poorly populated, very dense object of high C3 quality. It is located at a large 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 is a unique object, which shares a very small percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Bica et al. (2019) | 281.323 | -2.799 | – | – | – | – |
| UCC | 281.323 | -2.801 | 0.189 | -1.536 | -3.856 | – |
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 |
|---|---|---|---|---|---|---|---|---|
| CWNU 3930 | 100.0 | 281.31 | -2.8 | 0.21 | -1.52 | -3.85 | 47.3 | 0.17 |
| BDSB 125 | 3.8 | 281.46 | -2.73 | 0.24 | -1.17 | -3.72 | 28.11 | 0.19 |