SAI 47 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a large^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is very well-studied in the literature.

(*): The parallax distance estimate (~5.54 kpc) differs significantly from the median photometric distance (~3.96 kpc).

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	80.995	42.312	0.18	0.016	-0.35	-9.619
Almeida et al.	2025	81.001	42.313	–	–	–	–
Zhang et al.	2024	80.997	42.316	–	–	–	–
Hunt & Reffert	2024	80.997	42.316	0.188	0.06	-0.323	-11.064
Cavallo et al.	2024	80.931	42.322	0.185	–	–	–
Hunt & Reffert	2023	80.997	42.316	0.188	0.06	-0.323	-11.064
Almeida et al.	2023	81.001	42.316	–	–	–	–
Just et al.	2023	80.975	42.323	–	–	–	–
Dias et al.	2021	81.001	42.313	0.187	0.111	-0.311	–
Cantat-Gaudin et al.	2020	81.0	42.315	0.188	0.092	-0.335	–
Sánchez et al.	2020	80.992	42.314	–	0.201	-0.1	–
Cantat-Gaudin & Anders	2020	81.0	42.315	0.188	0.092	-0.335	–
Soubiran et al.	2018	81.0	42.315	–	–	–	-9.46
Bica et al.	2019	80.997	42.317	–	–	–	–
Cantat-Gaudin et al.	2018	81.0	42.315	0.188	0.092	-0.335	–
Kharchenko et al.	2016	80.975	42.323	–	–	–	–
Dias et al.	2014	80.992	42.314	–	-0.7	3.09	–
Kharchenko et al.	2013	80.985	42.323	–	-2.81	-2.58	–
Kharchenko et al.	2012	80.985	42.323	–	-2.81	-2.58	–
Glushkova et al.	2010	80.992	42.314	–	–	–	–
Dias et al.	2002	80.992	42.314	–	-0.7	2.42	–

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