Ruprecht 169
Summary
Ruprecht 169 is a poorly populated, loose object of very 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 23 years.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 269.842 | -24.767 | – | -1.34 | -2.6 | – |
| UCC | 269.857 | -24.792 | 0.355 | -1.32 | -2.553 | 25.592 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.66, Dist=1390.0, Age=9.0 |
Search coordinates in Bayestar19