FoF 1692
(LP 1692)
Summary
FoF 1692 is a poorly populated, very dense object of high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is poorly studied in the literature.
This object shares a large percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2021) | 289.171 | 14.156 | 0.244 | -2.169 | -5.371 | 31.952 |
| He et al. (2023) | 289.182 | 14.164 | 0.204 | -2.156 | -5.51 | 58.43 |
| Almeida et al. (2025) | 289.171 | 14.156 | – | – | – | – |
| UCC | 289.178 | 14.153 | 0.218 | -2.148 | -5.452 | 58.432 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2021) | Av=2.911, Dist=3926, logage=6.904, [Fe/H]=0.269 |
| He et al. (2023) | A0=3.5, m-M=12.85, logA=7.0 |
| Almeida et al. (2025) | AV=2.911, Dist=3926, logAge=6.904, MassRk=1578.9 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 407 | 100.0 | 289.19 | 14.16 | 0.21 | -2.16 | -5.5 | 46.67 | 0.44 |