FSR 0090 is a sparse, loose object of low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~2.49 kpc) differs significantly from the median photometric distance (~1.39 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	–	282.603	-3.611	0.402	-3.724	-4.313	-40.421
Bica et al.	2019	282.587	-3.581	–	–	–	–
Dias et al.	2014	282.583	-3.578	–	-0.61	-1.33	–
Froebrich et al.	2007	282.583	-3.578	–	–	–	–
Dias et al.	2002	282.583	-3.578	–	-0.29	-3.68	–

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