Juchert 12 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a young cluster (see Parameters). It is poorly studied in the literature, with no articles listed in the last 6 years.

(*): The parallax distance estimate (~8.34 kpc) differs significantly from the median photometric distance (~2.13 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	–	110.24	-22.849	0.12	-1.063	2.119	–
Sánchez et al.	2020	110.237	-22.867	–	-0.482	1.102	–
Bica et al.	2019	110.239	-22.864	–	–	–	–
Dias et al.	2014	110.237	-22.867	–	-3.46	0.52	–
Kronberger et al.	2006	110.236	-22.867	–	–	–	–
Dias et al.	2002	110.237	-22.867	–	–	–	–

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