FoF 1992
(LP 1992)
Summary
FoF 1992 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) | 148.008 | -50.394 | 0.223 | -4.993 | 3.269 | – |
| Almeida et al. (2025) | 148.008 | -50.394 | – | – | – | – |
| UCC | 147.963 | -50.481 | 0.225 | -4.965 | 3.295 | 14.823 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2021) | Av=1.555, Dist=4010, logage=8.771, [Fe/H]=0.074 |
| Almeida et al. (2025) | AV=1.555, Dist=4010, logAge=8.771, MassRk=656.6 |
Search coordinates in Bayestar19