FSR 1082
Summary
FSR 1082 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 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) | 100.042 | -1.72 | – | – | – | – |
| Kharchenko et al. (2012) | 100.028 | -1.745 | – | 2.42 | 1.83 | – |
| UCC | 100.038 | -1.737 | 0.218 | -0.48 | 0.101 | 59.383 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.833, distance=4040, log_age=8.84 |
Search coordinates in Bayestar19