FoF 1888

(LP 1888)

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C3
N_50
r_50
CC 13 9.7
Summary

FoF 1888 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is poorly studied in the literature.

This object shares a small percentage of members with a later reported entry.

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
Liu & Pang (2019) 14.513 63.25 0.356 -2.21 -0.265
Dias et al. (2021) 14.626 63.276 0.345 -2.275 -0.381
Almeida et al. (2025) 14.626 63.276
           
UCC 14.525 63.291 0.335 -2.227 -0.33 -55.202
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FoF 1888 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Liu & Pang (2019) Age=0.537, Z=0.5
Dias et al. (2021) Av=1.706, Dist=2487, logage=7.375, [Fe/H]=0.15
Almeida et al. (2025) AV=1.706, Dist=2487, logAge=7.375, MassRk=1350.7

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 10481 12.0 15.26 63.27 0.34 -2.19 -0.41 -112.34 0.06