FSR 1057
Summary
FSR 1057 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, near 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 |
|---|---|---|---|---|---|---|
| Froebrich et al. (2007) | 101.783 | 1.962 | – | – | – | – |
| Kharchenko et al. (2012) | 101.79 | 1.965 | – | -1.89 | -2.21 | – |
| UCC | 101.815 | 1.969 | 0.269 | -1.04 | -0.035 | 79.274 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.562, distance=2910, log_age=9.065 |
Search coordinates in Bayestar19