Ruprecht 162
Summary
Ruprecht 162 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, 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) | 163.225 | -62.317 | – | -1.7 | -0.2 | -0.3 |
| Kharchenko et al. (2012) | 163.208 | -62.305 | – | -2.44 | 4.78 | – |
| UCC | 163.157 | -62.293 | 0.166 | -6.812 | 3.046 | 33.711 |
Estimated members
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Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.312, Dist=3019.0, Age=8.385 |
| Kharchenko et al. (2012) | e_bv=0.312, distance=3019, log_age=8.385 |
Search coordinates in Bayestar19