“…The formation of phyllosilicates in the Fe-Si-O-H system has been reported in various geological and engineering settings: on meteorites (Elmaleh et al, 2015;Lauretta et al, 2000;Muller et al, 1979;Zolensky et al, 1993;Zolotov, 2014), on Mars (Bishop et al, 2008;Ehlmann et al, 2011), in deep-sea sediments (Badaut et al, 1985(Badaut et al, , 1992Baldermann et al, 2015;Marcus & Lam, 2014), in iron-banded formations (Eugster & Chou, 1973;Grubb, 1971), in ore deposits (Inoué & Kogure, 2016;Rasmussen et al, 1998;Rivas-Sanchez et al, 2006), at iron-clay (Lanson et al, 2012;Le Pape et al, 2015;Pignatelli et al, 2014) and steel-glass interfaces (Carriere et al, 2017(Carriere et al, , 2021Schlegel et al, 2016), and as a scale deposit in brinehandling equipment (Manceau et al, 1995). Thermodynamic modeling for some of these settings has been performed with the intention of estimating the physicochemical conditions which led to the formation of these minerals in the past (Chevrier et al, 2007;Fritz & Toth, 1997;Zolotov, 2014), or of estimating the evolution of physicochemical conditions for a given mineralogical composition with time (Ngo et al, 2015;Wilson et al, 2015).…”