“…Instead, Ra 2+ co-precipitates with a phase that can reach saturation (henceforth referred to as the host mineral phase). Minerals considered to be appropriate hosts for Ra or that have been found to contain Ra include rock-forming minerals such as gypsum (CaSO 4 Á2H 2 O), anhydrite (CaSO 4 ), calcite (CaCO 3 ) and aragonite (CaCO 3 ) (Langmuir and Riese, 1985;Chan and Chung, 1987;Gnanapragasam and Lewis, 1995;Yoshida et al, 2009) and minor and trace minerals such as barite (BaSO 4 ) (e.g., Doerner and Hoskins, 1925;Gordon, 1955;Gordon and Rowley, 1957), celestine (SrSO 4 ) (Langmuir and Melchior, 1985), 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, 1992a).…”