Ruprecht 160
Summary
Ruprecht 160 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, above 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) | 149.092 | -47.033 | – | -0.86 | 3.3 | – |
| Kharchenko et al. (2012) | 149.085 | -47.03 | – | -6.03 | 4.99 | – |
| UCC | 149.028 | -47.019 | 0.31 | -6.614 | 4.298 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.625, Dist=2187.0, Age=8.62 |
| Kharchenko et al. (2012) | e_bv=0.625, distance=2187, log_age=8.62 |
Search coordinates in Bayestar19