FSR 1690
Summary
FSR 1690 is a sparse, very loose object of 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 |
|---|---|---|---|---|---|---|
| Froebrich et al. (2007) | 218.083 | -53.699 | – | – | – | – |
| Kharchenko et al. (2012) | 218.083 | -53.7 | – | -8.2 | 0.64 | – |
| UCC | 218.12 | -53.687 | 0.346 | -6.448 | -1.821 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.666, distance=1850, log_age=9.135 |
Search coordinates in Bayestar19