FSR 1782
Summary
FSR 1782 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, well 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 |
|---|---|---|---|---|---|---|
| Froebrich et al. (2007) | 279.583 | -37.544 | – | – | – | – |
| Kharchenko et al. (2012) | 279.57 | -37.56 | – | -4.22 | -1.4 | – |
| UCC | 279.558 | -37.554 | 0.262 | -4.879 | -2.937 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.416, distance=2650, log_age=9.175 |
Search coordinates in Bayestar19