Ferrero 10 is a poorly populated, 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 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 (~2.28 kpc) differs significantly from the median photometric distance (~4.85 kpc).

Note: This object shares a moderate 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	–	105.194	-3.051	0.438	-1.286	0.638	83.927
Bica et al.	2019	105.113	-3.012	–	–	–	–
Loktin & Popova	2017	105.12	-3.009	–	-0.422	0.191	–
Dias et al.	2014	105.112	-3.01	–	0.22	5.57	–
Dias et al.	2002	105.112	-3.01	–	0.22	5.57	–

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