FoF 1785

(LP 1785)

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C3
N_50
r_50
DC 16 5.5
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.

Search object in SciX | Simbad

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
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FoF 1785 UCC

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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

Cluster region map