Ruprecht 116
Summary
Ruprecht 116 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is poorly 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) | 245.833 | -52.0 | – | -1.1 | -5.97 | – |
| Piskunov et al. (2008) | 245.823 | -52.002 | – | – | – | – |
| Kharchenko et al. (2012) | 245.85 | -52.0 | – | -3.23 | -3.95 | – |
| UCC | 245.851 | -52.027 | 0.248 | -1.964 | -1.484 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.1, Dist=900.0, Age=8.95 |
| Piskunov et al. (2008) | E(B-V)=0.1, Dist=900, logt=8.95, logMA=1.364 |
| Kharchenko et al. (2012) | e_bv=0.135, distance=895, log_age=8.95 |
Search coordinates in Bayestar19