OC 0490
Summary
OC 0490 is a sparse, very dense object of intermediate C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It was recently reported in the literature.
This object shares a large percentage of members with a later reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Hao et al. (2022) | 137.368 | -43.311 | 0.395 | -4.414 | 4.992 | – |
| UCC | 137.36 | -43.318 | 0.396 | -4.439 | 4.988 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hao et al. (2022) | AG=4.04, age=7.1, Z=0.018 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 8106 | 92.0 | 137.36 | -43.32 | 0.39 | -4.44 | 4.98 | – | 0.04 |