OCSN 52
Summary
OCSN 52 is a poorly populated, very dense object of very high C3 quality. It is located at a very close distance from the Sun, near the mid-plane. It was recently reported in the literature.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 |
|---|---|---|---|---|---|---|
| Qin et al. (2023) | 69.21 | 23.91 | 7.55 | 6.68 | -21.1 | 9.27 |
| UCC | 68.731 | 24.35 | 7.744 | 6.999 | -21.169 | 14.636 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Qin et al. (2023) | E(B-V)=0.18, m-M=6.14, logt=6.6 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 7 | 100.0 | 68.63 | 24.72 | 7.68 | 6.71 | -21.2 | 13.0 | 0.21 |
| Taurus | 2.1 | 65.78 | 27.29 | 7.72 | 8.8 | -25.91 | 14.81 | 0.38 |