FSR 0930 is a poorly populated, loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.29 kpc) differs significantly from the median photometric distance (~2.04 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	–	85.059	11.49	0.304	0.14	0.848	–
Just et al.	2023	85.023	11.46	–	–	–	–
Bica et al.	2019	85.048	11.459	–	–	–	–
Kharchenko et al.	2016	85.023	11.46	–	–	–	–
Kharchenko et al.	2013	85.03	11.46	–	0.69	0.69	–
Froebrich et al.	2007	85.042	11.457	–	–	–	–

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