FSR 0656 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature, with no articles listed in the last 6 years.

(*): The parallax distance estimate (~4.82 kpc) differs significantly from the median photometric distance (~1.40 kpc).

⚠️ 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	–	59.723	53.629	0.207	0.03	-0.599	-36.55
Donor et al.	2020	59.715	53.64	–	1.7	-0.6	-43.6
Bica et al.	2019	59.717	53.631	–	–	–	–
Dias et al.	2014	59.721	53.632	–	-0.04	-1.53	–
Froebrich et al.	2007	59.721	53.632	–	–	–	–
Dias et al.	2002	59.721	53.632	–	-0.1	-1.84	–

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