FoF 1785
(LP 1785)
Summary
FoF 1785 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is rarely studied in the literature.
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 |
|---|---|---|---|---|---|---|
| Dias et al. (2021) | 316.149 | 49.301 | 0.25 | -3.078 | -3.896 | -65.351 |
| Almeida et al. (2025) | 316.149 | 49.301 | – | – | – | – |
| UCC | 316.194 | 49.308 | 0.238 | -3.099 | -3.863 | -62.172 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2021) | Av=2.937, Dist=4167, logage=8.794, [Fe/H]=0.04 |
| Almeida et al. (2025) | AV=2.937, Dist=4167, logAge=8.794, MassRk=2034.8 |
Search coordinates in Bayestar19