FSR 1417
Summary
FSR 1417 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well 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) | 143.079 | -35.977 | – | – | – | – |
| Kharchenko et al. (2012) | 143.093 | -35.98 | – | -10.42 | 0.14 | – |
| UCC | 143.093 | -35.987 | 0.155 | -3.197 | 2.987 | 77.214 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.833, distance=2210, log_age=8.51 |
Search coordinates in Bayestar19