Ruprecht 62
Summary
Ruprecht 62 is a poorly populated, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, well above the mid-plane. It is rarely studied in the literature, with no articles listed in the last 13 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 |
|---|---|---|---|---|---|---|
| Kharchenko et al. (2012) | 128.153 | -19.683 | – | -0.93 | 2.29 | – |
| UCC | 128.132 | -19.661 | 0.273 | -3.186 | 1.408 | 98.665 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.396, distance=2160, log_age=8.735 |
Search coordinates in Bayestar19