FSR 0655 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by high 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 16 years.

(*): The parallax distance estimate (~3.90 kpc) differs significantly from the median photometric distance (~1.74 kpc).

Note: This object shares a small percentage of members with at least one entry reported in the same catalogue. 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	–	59.032	53.892	0.256	-0.084	-0.585	-20.556
Glushkova et al.	2010	59.049	53.869	–	–	–	–
Froebrich et al.	2007	59.058	53.865	–	–	–	–
Dias et al.	2002	59.058	53.865	–	1.21	-2.24	–

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