OC 0417
Summary
OC 0417 is a poorly populated, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It was recently reported in the literature.
Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Hao et al. (2022) | 117.588 | -25.464 | 0.268 | -2.771 | 3.02 | – |
| UCC | 117.582 | -25.456 | 0.281 | -2.748 | 3.03 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hao et al. (2022) | AG=0.44, age=7.5, Z=0.028 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Haffner 16 | 100.0 | 117.58 | -25.46 | 0.29 | -2.79 | 3.03 | 76.45 | 0.95 |
| FSR 1308 | 25.7 | 117.57 | -25.46 | 0.31 | -2.83 | 3.05 | – | 0.11 |
| CWNU 2123 | 8.6 | 117.48 | -25.37 | 0.32 | -2.7 | 2.89 | – | 0.08 |