FSR 0232 is a sparse, moderately dense object of very low C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~2.47 kpc) differs significantly from the median photometric distance (~1.55 kpc).

Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	304.519	42.64	0.405	-2.919	-4.658	–
Bica et al.	2019	304.557	42.636	–	–	–	–
Froebrich et al.	2007	304.558	42.631	–	–	–	–
Dias et al.	2002	304.558	42.631	–	0.81	-3.47	–

💡 Note: The UCC values are estimated from its identified members.