“…The similar ionic radii of Ra 2+ and Ba 2+ , electronegativities, electronic configuration and the identical crystallographic structure of pure RaSO 4 and barite (Curti, 1999;Zhu, 2004) make barite an almost ideal host mineral for Ra. However, the precipitation of Ra with other minerals such as gypsum (CaSO 4 Á2H 2 O), anhydrite (CaSO 4 ), calcite (CaCO 3 ) and aragonite (CaCO 3 ) was also studied (Langmuir and Riese, 1985;Chan and Chung, 1987;Gnanapragasam and Lewis, 1995;Yoshida et al, 2009). Field observations indicate that Ra partitioning occurs preferentially with barite (e.g., Paytan et al, 1996;van Beek et al, 2004;Ř anda et al, 2010) but also with other minerals such as Mn and Fe hydrous oxides (Kronfeld et al, 1991), alunite (KAl 3 (SO 4 ) 2 (OH) 6 ) and jarosite (KFe(III) 3 (OH) 6 (SO 4 ) 2 ) (Dickson and Herczeg, 1992).…”