Ruprecht 5
Summary
Ruprecht 5 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, well below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 13 years.
Warning: contains less than 25 stars with P>0.5 estimated.
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) | 103.808 | -18.6 | – | 1.37 | 1.45 | – |
| Kharchenko et al. (2012) | 103.809 | -18.6 | – | 1.37 | 1.45 | – |
| UCC | 103.809 | -18.554 | 0.163 | -0.262 | 0.671 | 70.904 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.416, Dist=4712.0, Age=9.15 |
| Kharchenko et al. (2012) | e_bv=0.416, distance=4712, log_age=9.15 |
Search coordinates in Bayestar19