Introduction
Smectitic clay minerals are widespread in the Solar System (Reference Hazen, Sverjensky, Azzolini, Bish, Elmore, Hinnov and MillikenHazen et al., 2013) and can form in many contexts, from alteration settings to magmatic systems, in wide ranges of redox and pH conditions (Reference Fox, Kupper, Ehlmann, Catalano, Razzell-Hollis, Abbey, Schild, Nickerson, Peters, Katz and WhiteFox et al., 2021; Reference MeunierMeunier, 2005; Reference Meunier, Mas, Beaufort, Patrier and DudoignonMeunier et al., 2008; Reference Viennet, Bultel, Riu and WernerViennet et al., 2017, Reference Viennet, Bernard, Le Guillou, Sautter, Schmitt-Kopplin, Beyssac, Pont, Zanda, Hewins and Remusat2020, Reference Viennet, Bernard, Le Guillou, Sautter, Grégoire, Jambon, Pont, Beyssac, Zanda, Hewins and Remusat2021; Reference Zhou and KeelingZhou & Keeling, 2013). These strongly anisotropic minerals carry key information about the geochemistry, oxidation state, and water content of the environments in which they were produced (Reference Ehlmann, Mustard, Clark, Swayze and MurchieEhlmann et al., 2011; Reference Fox, Kupper, Ehlmann, Catalano, Razzell-Hollis, Abbey, Schild, Nickerson, Peters, Katz and WhiteFox et al., 2021), making them good indicators of paleoenvironmental and paleoclimatic conditions. Their intrinsic properties (e.g. adsorption capacity, catalytic properties) confer on them a unique reactivity in the mineral world, explaining their huge number of applications in a variety of domains (e.g. Reference Carniato, Gatti and BisioCarniato et al., 2020; Reference Choy, Choi, Oh and ParkChoy et al., 2007; Reference MurrayMurray, 1991, Reference Murray2000), including medicine (Reference Ghadiri, Chrzanowski and RohanizadehGhadiri et al., 2015; Reference Saadat, Rawtani and ParikhSaadat et al., 2022), pharmaceuticals (Reference Bello, Junior, Freitas, Moreira, da Costa, de Souza, Santos, de Sousa, Castro, Rodrigues and CabralBello et al., 2022; Reference Carretero and PozoCarretero & Pozo, 2009; Reference Corbin, Vulliet, Lanson, Rimola and MignonCorbin et al., 2021), pollution control (Reference Churchman, Gates, Theng, Yuan, Bergaya, Theng and LagalyChurchman et al., 2006; Reference Ewis, Ba-Abbad, Benamor and El-NaasEwis et al., 2022), the petroleum industry (Reference Abdo and HaneefAbdo & Haneef, 2013; Reference Li, Wang, Ma, Huang, Lu and PengLi et al., 2023; Reference Salter, Watson and SephtonSalter et al., 2023), and the construction industry (Reference SinghSingh, 2022). It is the exceptional trapping capabilities of smectites that make possible the geological storage of CO2 or H2 (Reference Abdulelah, Keshavarz, Hoteit, Abid, Goudeli, Ennis-King and IglauerAbdulelah et al., 2023; Reference de Jong, Spiers and Buschde Jong et al., 2014; Reference Ho, Jove-Colon and WangHo et al., 2023; Reference RomanovRomanov, 2013; Reference Rother, Ilton, Wallacher, Hauβ, Schaef, Qafoku, Rosso, Felmy, Krukowski, Stack, Grimm and BodnarRother et al., 2013) and radioactive waste (Reference Delage, Cui and TangDelage et al., 2010; Reference Landais, Dohrmann and KaufholdLandais et al., 2013; Reference Parrotin, Robin, Beaucaire, Descostes and TertreParrotin et al., 2023; Reference Robin, Tertre, Beaucaire, Regnault and DescostesRobin et al., 2017). Smectite-rich rocks are also a major reservoir of Rare Earth Elements (Reference Abbott, Löhr and TrethewyAbbott et al., 2019; Reference Moldoveanu and PapangelakisMoldoveanu & Papangelakis, 2012), and the strong affinities of smectites for organic molecules make them the primary agents for organic carbon sequestration in soils, sediments, and chondrites (Reference Blattmann, Liu, Zhang, Zhao, Haghipour, Montluçon, Plötze and EglintonBlattmann et al., 2019; Reference Kennedy, Pevear and HillKennedy et al., 2002; Reference Viennet, Roskosz, Nakamura, Beck, Baptiste, Lavina, Alp, Hu, Zhao, Gounelle, Brunetto, Yurimoto, Noguchi, Okazaki, Yabuta, Naraoka, Sakamoto, Tachibana, Yada and TsudaViennet et al., 2023) and the probable main actors of the origins of life (Reference Kloprogge and HartmanKloprogge & Hartman, 2022; Reference Viennet, Bernard, Le Guillou, Sautter, Grégoire, Jambon, Pont, Beyssac, Zanda, Hewins and RemusatViennet et al., 2021). Because they are also the main carriers of water in sediments and in the oceanic crust, smectitic rocks play a great role in subduction settings (Reference Hwang, Seoung, Lee, Liu, Liermann, Cynn, Vogt, Kao and MaoHwang et al., 2017; Reference Katayama, Kubo, Sakuma and KawaiKatayama et al., 2015). Their anisotropic nature affects the seismic properties of rocks (Reference Almqvist and MainpriceAlmqvist & Mainprice, 2017), as well as the macroscopic behavior of faults (Reference Ikari, Saffer and MaroneIkari et al., 2009).
Smectites are clay minerals with a 2:1 layer silicate structure, each layer being made of an octahedral sheet sandwiched between two Si(Al,Fe3+)–O tetrahedral sheets and in which stacking creates expandable interlayer spaces capable of storing water, organics, and exchangeable cations (mostly Ca2+, Mg2+, Na+, and K+) balancing the overall charge (Reference Fox, Kupper, Ehlmann, Catalano, Razzell-Hollis, Abbey, Schild, Nickerson, Peters, Katz and WhiteFox et al., 2021; Reference MeunierMeunier, 2005). While trioctahedral smectites (such as hectorite and saponite) have all octahedral sites filled by mostly divalent cations, dioctahedral smectites (such as nontronite, montmorillonite, and beidellite) have only two of their three octahedral sites filled by mostly trivalent cations, the most common octahedral cations being Al, Fe, and Mg. Depending on the pH conditions under which they crystallize, smectites may exhibit tetrahedral substitutions (Al3+, and sometimes Fe3+, can substitute for Si4+ in tetrahedral sites), resulting in an increase in layer charge, thereby impacting their properties, such as their swelling or sorption capacities, catalytic properties, or expansion abilities (Reference Fox, Kupper, Ehlmann, Catalano, Razzell-Hollis, Abbey, Schild, Nickerson, Peters, Katz and WhiteFox et al., 2021; Reference Komadel, Madejová and BujdákKomadel et al., 2005; Reference MeunierMeunier, 2005; Reference MurrayMurray, 2000).
Many studies dealing with the synthesis of smectites exist in the literature (Reference Dzene, Brendlé, Limousy, Dutournié, Martin and MichauDzene et al., 2018; Reference KloproggeKloprogge, 1999; Reference Petit, Baron and DecarreauPetit et al., 2017; Reference Ponce and KloproggePonce & Kloprogge, 2020; Reference Zhang, Zhou, Lin, Tong and YuZhang et al., 2010). Although smectites could be synthesized from glasses submitted to high-pressure and high-temperature conditions (Reference Kalo, Möller, Ziadeh, Dolejš and BreuKalo et al., 2010; Reference Nakazawa, Yamada and FujitaNakazawa et al., 1992; Reference TamuraTamura, 2000; Reference YamadaYamada, 1994, Reference Yamada1995), most syntheses are conducted following the sol-gel method, i.e. using gels produced at room temperature before being exposed to hydrothermal conditions. A number of syntheses aimed at producing a suite of smectite samples spanning compositional ranges between Fe(II), Fe(III), Mg, and Al end-member species to document precisely their spectroscopic signatures, was carried out recently by Reference Fox, Kupper, Ehlmann, Catalano, Razzell-Hollis, Abbey, Schild, Nickerson, Peters, Katz and WhiteFox et al. (2021). In parallel, a number of laboratory studies have investigated how conditions (such as temperature and pH) control cation coordination and incorporation into the smectite structure and, in turn, their final crystallochemistry (Reference Andrieux and PetitAndrieux & Petit, 2010; Reference Baron, Petit, Tertre and DecarreauBaron et al., 2016a, Reference Baron, Pushparaj, Fontaine, Sivaiah, Decarreau and Petitb; Reference Blukis, Schindler, Couasnon and BenningBlukis et al., 2022; Reference Grauby, Petit, Decarreau and BaronnetGrauby et al., 1993, Reference Grauby, Petit, Decarreau and Baronnet1994; Reference HarderHarder, 1976; Reference Huertas, Cuadros, Huertas and LinaresHuertas et al., 2000; Reference Petit, Decarreau, Gates, Andrieux and GraubyPetit et al., 2015, Reference Petit, Baron and Decarreau2017). For instance, Reference Blukis, Schindler, Couasnon and BenningBlukis et al. (2022) recently showed that high pH favors a high degree of crystallinity for saponite. However, those studies were dedicated to a given end-member or to a given solid solution (i.e. either the Fe(III)–Mg (nontronite–saponite) or the Fe(III)–Al (nontronite–beidellite) series (Reference Andrieux and PetitAndrieux & Petit, 2010; Reference Grauby, Petit, Decarreau and BaronnetGrauby et al., 1993, Reference Grauby, Petit, Decarreau and Baronnet1994; Reference Petit, Decarreau, Gates, Andrieux and GraubyPetit et al., 2015)).
Because the speciation of Fe, Mg, and Al as a function of pH is different (Reference Millero, Yao and AicherMillero et al., 1995; Reference Perry and ShafranPerry & Shafran, 2001; Reference See, Chapman, Zhu, Wiaderek, Borkiewicz, Barile, Chupas and GewirthSee et al., 2015; Reference Pierrot and MilleroPierrot & Millero, 2017; Reference de Mello Gabriel, Machado Pitombo, Tavares Rosa, AparecidoNavarrete, Botero, do Carmo and Camargo de Oliveirade Mello Gabriel et al., 2021), the optimal pH for the synthesis of saponite, beidellite, and nontronite is anticipated to be different, with pH conditions strongly influencing their production. The sensitivity of different smectites to pH conditions thus remains to be investigated. The purpose of the present study, therefore, was to investigate the influence of pH conditions on the production of smectites, using three different series of hydrothermal syntheses designed to lead (when conditions are optimal) to the crystallization of three smectite end-members containing tetrahedral Al, namely a saponite (Na0.4(Si3.6Al0.4)Mg3O10(OH)2), a beidellite (Na0.4(Si3.6Al0.4)Al2O10(OH)2), and a nontronite (Na0.4(Si3.6Al0.4)Fe3+ 2O10(OH)2).
Experimental
Sample Preparation
The syntheses reported here were conducted via a sol–gel method, i.e. using gels produced at room temperature before being exposed to hydrothermal conditions. To explore the influence of pH conditions, the syntheses reported here used gels produced from solutions at various pH and exposed to hydrothermal conditions within solutions at various pH. The preparation of the gels was done following classic protocols (Reference Baron, Petit, Tertre and DecarreauBaron et al., 2016a; Reference Dzene, Brendlé, Limousy, Dutournié, Martin and MichauDzene et al., 2018; Reference Fox, Kupper, Ehlmann, Catalano, Razzell-Hollis, Abbey, Schild, Nickerson, Peters, Katz and WhiteFox et al., 2021; Reference Petit, Baron and DecarreauPetit et al., 2017). Starting solutions were mixed to obtain gels with the Si:Al:Mg, Si:Al:Al, and Si:Al:Fe molar ratios of pure Al-substituted smectite end-members (i.e. 3.6:0.4:3 for the saponite, 3.6:0.4:2 for the beidellite, and 3.6:0.4:2 for the nontronite). For all gels, the first step was to pour an AlCl3 solution into a Na2SiO3 solution under continuous stirring at room temperature, which led to the instantaneous formation of a white precipitate of amorphous aluminosilicate. Then, a given volume of either a MgCl2, an FeCl3, or an AlCl3 solution was added to provide the exact quantity of cations needed for the octahedral occupancies. Stirring was stopped soon after this step, and the precipitated gel was filtered and rinsed with pure water with a vacuum suction filter device to remove excess salts. Each starting gel was immersed in a solution at a given pH in Teflon acid-digestion bombs which were sealed and placed in an oven for several days (syntheses were conducted in pure water or in solutions at pH values ranging from 12 to 14 for saponites and from 12 to 13 for nontronites and beidellites given the high pH sensitivity of these smectites). The synthesized products were then filtered and rinsed with pure water (resistivity of 18.2 MΩ·cm) to remove any remaining salt. Then, they were dried in an oven at 50°C for 24 h and ground in an agate mortar for characterization using X-ray diffraction (XRD) and Fourier-transform infrared spectroscopy (FTIR) as classically done for smectites (Reference Baron, Petit, Tertre and DecarreauBaron et al., 2016a; Reference Dzene, Brendlé, Limousy, Dutournié, Martin and MichauDzene et al., 2018; Reference Fox, Kupper, Ehlmann, Catalano, Razzell-Hollis, Abbey, Schild, Nickerson, Peters, Katz and WhiteFox et al., 2021; Reference Petit, Baron and DecarreauPetit et al., 2017).
Measurements and Characterization
The pH of each starting solution, i.e. the solution in equilibrium with the gel and the solution in equilibrium with the products of syntheses, was measured using a Fisher Scientific (Hampton, New Hampshire, USA) Accumet XL600 pH/mV/Temp/ISE/DO/Conductivity Meter calibrated with three buffers (pH 7, 10, and 12). The uncertainty for each measurement was estimated to be ± 0.05 pH units. The PhreeqC code associated with the minteq.v4 database was used to determine the major species in the starting solutions used for the production of gels.
The XRD data reported here were collected on unoriented powders at room temperature with a step size of 0.033°2θ over the 4–75°2θ CoKα1,2 (40 mA, 45 kV) angular range and a counting time of 300 ms per step using an X’Pert Pro instrument from Malvern PANalytical (Malvern, UK), operating at the Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie (IMPMC, Paris, France).
The FTIR data shown here were collected on unoriented powders in attenuated total reflection mode (ATR) with a diamond internal reflexion element with a 4 cm–1 resolution in the mid-infrared (MIR) range (4000–400 cm–1) using a Fisher Scientific (Hampton, New Hampshire, USA) Nicolet 6700 FTIR spectrometer equipped with a KBr beamsplitter and DTGS-KBr detector and operating at the Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie (IMPMC, Paris, France).
Starting Solutions
Dilute solutions (0.2 M) of Na2SiO3 (>95%), AlCl3 (99%), MgCl2 (>99%), and FeCl3 (>99%) were prepared using pure water (milliQ—18.2 MΩ-cm) for the syntheses reported here, leading to a Na2SiO3 solution at pH 13.1, a MgCl2 solution at pH 5.4, an FeCl3 solution at pH 1.8, and an AlCl3 solution at pH 3.4 (Table 1). Some NaOH was added to the AlCl3 and FeCl3 solutions to obtain an additional FeCl3 solution at pH 2.1 and four additional AlCl3 solutions at pH 3.9, 5.3, 8.0, and 10.6 (Table 1). These additional solutions were used to test the influence of the pH of the starting solutions on the synthesis of nontronite and beidellite. All chemicals were obtained from Sigma Aldrich (St. Louis, Missouri, USA)..
Detailed Protocols
Saponite syntheses
Four different syntheses were conducted from the gel of saponite composition for the present study. The starting gels were prepared by pouring 556 µL of the AlCl3 solution at pH 3.4 into 5 mL of the Na2SiO3 solution, before being mixed with 4.17 mL of the MgCl2 solution, to produce, theoretically, ~100 mg of a gel stoichiometrically identical to a pure saponite with 0.4 Al in each tetrahedron (Na0.4 (Si3.6Al0.4)Mg3O10(OH)2). The pH of the solution in equilibrium with the gel was ~10. After filtration, the gel produced was placed into 23 mL Teflon reactors before drying and immersed in 16.5 mL of pure water at pH 5.5 (i.e. pure water in equilibrium with atmospheric CO2) or in 16.5 mL of a solution composed of pure water in which was added NaOH to reach a pH of 12, 13, or 14 (cf Table 2). All reactors were then put in an oven at 230°C (~28 bar) for 4 days, following the recommendations of Reference Zhang, Petit, He, Villiéras, Razafitianamaharavo, Baron, Tao and ZhuZhang et al. (2020) for the synthesis of pure saponites. During syntheses above 200°C, saponite particles grow faster during the first 3 days than during the subsequent 10 (Reference Zhang, Petit, He, Villiéras, Razafitianamaharavo, Baron, Tao and ZhuZhang et al., 2020). Of note, although saponites can be produced at low temperature (i.e. 90°C; Reference Meyer, Bennici, Vaulot, Rigolet and DzeneMeyer et al., 2020; Reference Ponce and KloproggePonce & Kloprogge, 2020), high temperature conditions inhibit the incorporation of Al into octahedral sheets, while enhancing [4]Al3+ for [4]Si4+ tetrahedral substitutions, as reported by Reference Kloprogge and PonceKloprogge and Ponce (2021).
Beidellite Syntheses
Four different syntheses were conducted from the gel of beidellite composition for the present study. The starting gels were prepared by pouring 2.833 mL of the AlCl3 solution at pH 3.9 into 4.25 mL of the Na2SiO3 solution to produce theoretically ~80 mg of a gel stoichiometrically identical to a pure beidellite with 0.4 Al in each tetrahedron (Na0.4(Si3.6Al0.4)Al2O10(OH)2). The pH of the solution at room temperature in equilibrium with the gel was ~4.5. After filtration, the produced gel was kept hydrated and placed into 23 mL Teflon reactors and immersed into 12.5 mL of pure water at pH 5.5 (i.e. pure water in equilibrium with atmospheric CO2) or into 12.5 mL of a solution composed of pure water to which was added NaOH to reach a pH of 12, 12.5, or 13 (cf Table 2). Only 12.5 mL of pure water or solution at pH 12, 12.5, or 13 was used rather than 16.5 mL to prevent overpressure related to the swelling of the gel containing a lot of highly hydrated Al3+. All reactors were then placed in an oven at 230°C (~28 bar) for 9 days, previous successful syntheses having been conducted over 8 to 10 days from 175–200°C (Reference De KimpeDe Kimpe, 1976; Reference Kloprogge, van der Eerden, Jansen, Geus and SchuilingKloprogge et al., 1993) to well above 300°C (Reference Kloprogge, Jansen and GeusKloprogge et al., 1990; Reference Lantenois, Muller, Bény, Mahiaoui and ChampallierLantenois et al., 2008).
Nontronite Syntheses
Three different series of syntheses were conducted from four different gels of nontronite composition for the present study. A first series of four syntheses was conducted with a gel produced using the AlCl3 solution at pH 3.4, a second series of four syntheses was conducted with a gel produced using the AlCl3 solution at pH 10.6, and a third series of two syntheses was conducted with either a gel produced using the AlCl3 solution at pH 5.3 or a gel produced using the AlCl3 solution at pH 8. Each starting gel was prepared by pouring 833 µL of the AlCl3 solution into 7.5 mL of the Na2SiO3 solution, before being mixed with 4.17 mL of the FeCl3 solution, to produce, theoretically, ~165 mg of a gel stoichiometrically identical to a pure nontronite with 0.4 Al in each tetrahedron (Na0.4(Si3.6Al0.4)Fe(III)2O10(OH)2). The pH of the solution in equilibrium with the gel prepared with the AlCl3 solution at pH 3.4 was ~4, while that formed with the AlCl3 solution at pH 10.6 reached a pH of 9. After filtration, all the gels produced were kept hydrated and placed in 23 mL Teflon reactors. The gels produced using either the AlCl3 solution at pH 3.4 or the AlCl3 solution at pH 10.6 were immersed in 16.5 mL of pure water at pH 5.5 (i.e. pure water in equilibrium with atmospheric CO2) or in 16.5 mL of a solution composed of pure water to which was added NaOH to reach a pH of 12, 12.5, or 13, while the two gels produced using either the AlCl3 solution at pH 5.3 or the AlCl3 solution at pH 8 were immersed only in 16.5 mL of a solution composed of pure water to which was added NaOH to reach a pH of 12.5 (cf Table 2). All reactors were then placed in an oven at 150°C (4.75 bar) for 2.5 days, following the recommendations of Reference Andrieux and PetitAndrieux and Petit (2010), Reference Baron, Petit, Tertre and DecarreauBaron et al. (2016a), and Reference Dzene, Dutournie, Brendle, Limousy, Le Meins, Michelin, Vidal, Gree, Abdelmoula, Martin and MichauDzene et al. (2022). In fact, higher temperatures (>200°C) may favor the formation of kaolinite, hematite (akaganeite), or aegirine (Reference Andrieux and PetitAndrieux & Petit, 2010; Reference Decarreau, Petit, Martin, Farges, Vieillard and JousseinDecarreau et al., 2008; Reference Delvaux, Mestdagh, Vielvoye and HerbillonDelvaux et al., 1989).
Results
Saponite Syntheses
Each of the four syntheses produced a translucid, gelatinous solid residue immersed in a transparent solution at a pH close to that of the solutions in which the starting gels were immersed (i.e. 7.5 for the synthesis conducted in pure water, 10.4 in the solution at pH 12, 12.9 in the solution at pH 13, and 13.7 in the solution at pH 14; cf Table 2). These residues turned white upon drying.
Whatever the pH of the solution used for the syntheses, the XRD patterns of the synthetic products exhibited peaks typical of the hkl reflections of 2:1 trioctahedral saponites (Reference Grauby, Petit, Decarreau and BaronnetGrauby et al., 1994), i.e. peaks at ~12.7 Å (001), 4.55 Å (02,11), ~3.10 Å (004), 2.60 Å (13,20), 1.73 Å (15,24,31), and ~1.53 Å (06,33) (Fig. 1). The 06,33 reflection of these saponites confirmed their trioctahedral nature (>1.51 Å; Reference Brown, Brindley, Brindley and BrownBrown & Brindley, 1980; Reference Decarreau, Grauby and PetitDecarreau et al., 1992; Reference Grauby, Petit, Decarreau and BaronnetGrauby et al., 1994), and the position of the 00l reflections indicated that they were mainly monohydrated (Reference Brown, Brindley, Brindley and BrownBrown & Brindley, 1980; Reference Ferrage, Lanson, Sakharov and DritsFerrage et al., 2005, Reference Ferrage, Lanson, Sakharov, Geoffroy, Jacquot and Drits2007). Under vacuum, the d 001 of the saponite synthesized in pure water collapsed to 10.45 Å (Fig. S1). The 02,11 and 06,33 reflections of the saponite synthesized in solution at pH 14 shifted to lower angles compared to saponites synthesized in solutions at lower pH (4.58 to 4.55 Å and 1.533 to 1.526 Å).
All synthetic products had a FTIR spectrum exhibiting a broad band near 3420 cm–1 typical of the ѵOH vibrations of the water adsorbed within the interlayer spaces of smectites (Fig. 2; Reference Madejová, Gates and PetitMadejová et al., 2017). In addition, the FTIR spectra of all synthetic products showed the characteristic bands of saponite, i.e. ѵMg3OH and δMg3OH vibrations at 3680 and 655 cm–1, respectively; ѵSi–O vibration near 1000–950 cm–1; [4]Al–O out of plane near 800 cm–1; perpendicular Si–O–Mg vibrations at 692 and 532 cm–1; and δSi–O–Si vibrations near 500 and 455 cm–1 (Reference Kloprogge and PonceKloprogge & Ponce, 2021; Reference Madejová, Gates and PetitMadejová et al., 2017). Bands corresponding to ѵMg3OH and δMg3OH vibrations in the FTIR spectra of the saponite synthesized in solution at pH 14 shifted toward higher and lower wavenumbers compared to FTIR spectra of saponites synthesized in solutions at lower pH. The band near 3612–3634 cm–1 is related to the stretching vibration of interlayer water molecules (Fig. S2). In this case, the two OH groups of the molecule are not equivalent and this signal is assigned to the OH group weakly bonded to the surface oxygens (Reference FarmerFarmer, 1974).
Beidellite Syntheses
Each of the four syntheses produced solid residues immersed in a colorless transparent solution at a pH close to that of the solutions in which the starting gels were immersed (i.e. 7.2 for the synthesis conducted in pure water at pH 5.5, 9.4 in the solution at pH 12, 11 in the solution at pH 12.5, and 12 for the synthesis at pH 13; Table 2).
The synthesis conducted in pure water produced a white and pasty solid residue which became very soft upon drying, showing an XRD pattern typical of kaolins, with peaks at 7.17 Å (001), 4.43 Å (020), 4.34 Å (110), 4.41 Å (111), 3.57 Å (002), 3.39 Å (111), 2.55 Å (201), 2.35 Å (003), 1.79 Å (004), and 1.486 Å (060) (Fig. 3; Reference CarrollCarroll, 1970). The bands at 3621 and 3692 cm–1 in the FTIR spectrum of this solid confirms the presence of kaolins (Fig. 4; Reference KodamaKodama, 1962; Reference Zhang, Zhou, Lin, Tong and YuZhang et al., 2010; Reference Madejová, Gates and PetitMadejová et al., 2017).
The synthesis conducted in the solution at pH 12 produced a translucid, gelatinous solid residue that turned white, with a paper texture, upon drying. The XRD pattern of this synthetic product revealed the presence of reflections typical of smectitic clay minerals, with peaks at 12.17 Å (001), 6.12 Å (002), 4.43 Å (02,11), 3.09 Å (004), 2.53 Å (13,20), 2.04 Å (006), 1.68 Å (15,24,31), and 1.488 Å (06,33) (Fig. 3). In addition, the basal spacing of the d(06,33) is typical of dioctahedral Al-rich smectites such as beidellite (1.48–1.50 Å Reference Grauby, Petit, Decarreau and BaronnetGrauby et al., 1994; Reference Petit, Decarreau, Gates, Andrieux and GraubyPetit et al., 2015). Its presence was suggested also by the FTIR spectrum exhibiting characteristic bands of Al-rich smectites, i.e. the bands at 3670 cm–1 (ѵAl2OH), 3626 cm–1 (ѵAl2OH), 1000–950 cm–1 (ѵSi–O), 914 cm–1 (δAl2OH), 815 cm–1 ([4]Al–O out of plane), 694 cm–1 ([6]Al–Oap), 520 cm–1 (δSi–O–[6]Al), and 455 cm–1 (δSi–O–Si) (Fig. 4; Reference Farmer and RussellFarmer & Russell, 1964; Reference Kloprogge, Jansen and GeusKloprogge et al., 1990; Reference Lantenois, Muller, Bény, Mahiaoui and ChampallierLantenois et al., 2008; Reference Zviagina, McCarty, Środonón and DritsZviagina et al., 2004). Under vacuum, the d 001 of the beidellite synthesized in the solution at pH 12 collapsed to 9.78 Å (Fig. S1).
The synthesis conducted in the solution at pH 12.5 produced a solid residue with an XRD pattern exhibiting peaks at 10.96 Å (001), 4.42 Å (02,11), 2.52 Å (13,20), and 1.481 Å (06,33), probably indicating the presence of beidellite (i.e. the d(06,33) diffracts between 1.48 and 1.50 Å; Fig. 3). The weak and broad peak of the (001) reflection indicates its poorly crystalline and dehydrated state (Reference Ferrage, Lanson, Sakharov, Geoffroy, Jacquot and DritsFerrage et al., 2007). This beidellite cohabits with two zeolites (which are the main phases of the residue): analcime (diffraction peaks at 5.58, 4.83, 3.65, 3.42, 2.91, 2.42, 2.22, 2.15, 1.90, 1.86, 1.74, 1.71, and 1.59 Å) and a Na-garronite-like zeolite (diffraction peaks at 7.04, 5.75, 5.02, 4.91, 4.08, 3.51, 3.32, 3.18, 3.12, 3.03, 2.68, 2.65, 2.04, 1.97, 1.96, and 1.78 Å; Reference Oleksiak, Ghorbanpour, Conato, McGrail, Grabow, Motkuri and RimerOleksiak et al., 2016; Reference Tayraukham, Jantarit, Osakoo and WittayakunTayraukham et al., 2020).
The synthesis conducted in the solution at pH 13 produced a grainy solid residue with an XRD pattern typical of analcime, with peaks at 6.20 Å, 5.62 Å (011), 4.86 Å (020), 3.79 Å, 3.67 Å (021), 3.41 Å (222), 3.24 Å, 2.91 Å (112), 2.80 Å (022), 2.69 Å (130), 2.51 Å (231), 2.43 Å (040), 2.23 Å (032), 2.17 Å (032), 2.12 Å, 2.02 Å, 1.94 Å, 1.90 Å (151), 1.87 Å (141), 1.83 Å, 1.74 Å (051), 1.71 Å (444), 1.69 Å (223), 1.66 Å, 1.62 Å, 1.59 Å (043), and 1.50 Å and 1.48 (233) (Fig. 3). Peaks at 2.08 and 1.81 Å (also present in the XRD pattern of the saponite produced in the solution at pH 14; Fig. 1) were attributed to an austenitic steel from a spatula used during preparation for XRD. The FTIR spectrum (Fig. 4) shows two bands at 735 and 664 cm–1 corresponding to ѵSi–O–Si and ѵSi–O–Al vibrations, and a band at 613 cm–1 attributed to 4-membered rings vibrations of analcime (Reference Mozgawa, Krol and BarczykMozgawa et al., 2011).
Nontronite Syntheses
Each of the syntheses conducted in solutions at pH of <13 produced red solid residues, with the exception of the syntheses conducted with the AlCl3 solution at pH 10.6 and the syntheses conducted in solutions at pH 12.5 using the gels obtained with the AlCl3 solutions above pH 5.4. The latter produced gelatinous solid residues that were green on top and orange below. In contrast, the syntheses conducted in solutions at pH 13 produced gelatinous solid residues green on top and yellow below.
Syntheses from the Gels Obtained using the AlCl3 Solution at pH 3.4
Each of the four syntheses produced solid residues immersed in a reddish solution at a pH lower than that of the solution in which the starting gel was immersed (i.e. 4.7 for the synthesis conducted in pure water, 8.3 in the solution at pH 12, 10.7 at pH 12.5, and 12.7 at pH 13; Table 2). The XRD patterns of the synthetic products are very different from one another (Fig. 5). The solid produced in pure water exhibited XRD peaks at 8.96 Å (001), 4.50 Å (02,11), 3.52 Å (002), 2.54 Å (20,13), 2.32 Å (04,22), 2.15 Å, 1.91 Å, 1.53 Å (06,33), and 1.50 Å, probably corresponding to hisingerite (i.e. a precursor of nontronite containing no Al, nontronite-like phase; Reference EggletonEggleton, 1998; Reference Farmer, McHardy, Elsass and RobertFarmer et al., 1994; Reference KohyamaKohyama, 1975), while the solid produced in the solution at pH 12 exhibited only two broad bands near 3.58 and 1.93 Å, maybe indicating the presence of a semi-amorphous hisingerite). The solid produced in the solution at pH 12.5 showed a broad peak at ~12.3 Å (001) and weak peaks at 4.52 Å (02,11), 3.14 Å (004), 2.59 Å (13,20), 1.72 Å (15,24,31), and 1.524 Å (06,33) corresponding to nontronite (Reference Baron, Petit, Tertre and DecarreauBaron et al., 2016a). The solid produced in the solution at pH 13 contained sharper, rather crystalline nontronite (XRD peaks at 12.18 Å (001), 4.54 Å (02,11), 3.09 Å (004), 2.61 Å (13,21), and 1.530 Å (06,33); Fig. 5) mixed with analcime (XRD peaks at 5.55, 4.81, 3.67, 3.41, 2.91, 2.68, 2.49, 2.41, 2.22, 1.89, 1.86, 1.73, 1.71, and 1.68 Å; Fig. 5). Note that the 06,33 reflection of this nontronite was shifted toward lower angles (greater d spacings) possibly indicating [4]Fe3+ for [4]Si4+ tetrahedral substitutions and, thus, an increase of its charge (Reference Baron, Petit, Tertre and DecarreauBaron et al., 2016a). The FTIR data (Fig. 6) confirmed the interpretations of the XRD patterns; the bands typical of nontronite (i.e. ѵFe2 3+–OH at ~3560 cm–1, δFe2 3+–OH at 815 cm–1, the 855 cm–1 (not assigned), [4]Fe–O at 707 cm–1, and [6]Fe3+–Oap ~ 667 cm–1; Reference Baron, Petit, Tertre and DecarreauBaron et al., 2016a; Reference Dzene, Dutournie, Brendle, Limousy, Le Meins, Michelin, Vidal, Gree, Abdelmoula, Martin and MichauDzene et al., 2022; Reference Goodman, Russell, Fraser and WoodhamsGoodman et al., 1976) were stronger in the FTIR spectrum of the solid produced in the solution at pH 13 than in the FTIR spectrum of the solid produced in the solution at pH 12.5, indicating that the nontronite produced at pH 12.5 was poorly crystallized. No band typical of nontronite was observed in the FTIR spectra of the solids produced in solutions at pH <12.5 (Fig. 6).
Syntheses from the Gels Obtained using the AlCl3 Solution at pH 10.6
Each of the four syntheses produced solid residues immersed in solutions ranging from reddish to colorless; the lower the pH of the solution in which the synthesis was conducted, the more reddish the solution at the end of the synthesis (Table 2). With the exception of the final solution of the synthesis conducted in pure water at pH which ended at pH 9.7, the final solutions had pH values close to those of the solutions in which the starting gels were immersed (Table 2). The XRD patterns of all the solids show the presence of nontronite, i.e. XRD peaks at 12.43–13.07 Å (001), 4.53–4.56 Å (02,11), 3.10–3.14 Å (004), 2.58–2.62 Å (13,20), 1.73 Å (13,24,31), and 1.522–1.537 Å (06,33) (Reference Baron, Petit, Tertre and DecarreauBaron et al., 2016a; Fig. 5). The increase of the 06,33 reflection position may indicate increasing [4]Fe3+ for [4]Si4 tetrahedral substitutions with increasing pH (Reference Baron, Petit, Tertre and DecarreauBaron et al., 2016a). The additional presence of bayerite (Al(OH)3) can be inferred from the solid produced in pure water, as well as from the solid produced in the solution at pH 12 (although in lower abundance), from the XRD peaks at 4.68, 4.35, 3.18, 2.21, 1.71, and 1.59 Å (Reference Lefevre and FedoroffLefevre & Fedoroff, 2002; Reference MilliganMilligan, 1951) and the FTIR bands at 3651, 3545, 3461, and 3418 cm–1 (Reference Phambu, Humbert and BurneauPhambu et al., 2002 – Figs. 5 and 6). FTIR spectra of all solid residues showed bands typical of nontronite (i.e. bands at ~3560 cm–1 (ѵFe2OH), ~950 cm–1 (ѵSi–O), ~815 cm–1 (δFe3+ 2OH), ~667 cm–1 ([6]Fe3+–Oap), 585 cm–1 (δSi–O) and ~480 cm–1 ([6]Fe–O–Si) (Reference Baron, Petit, Tertre and DecarreauBaron et al., 2016a; Reference Goodman, Russell, Fraser and WoodhamsGoodman et al., 1976). The bands at 850 and 707 cm–1 are present commonly in nontronite with large [6]Fe occupancy, but the band at 707 cm–1 is present only in the FTIR spectrum of the nontronite produced in the solution at pH 13. Of note, the weak band at ~3635 cm–1 observed in the FTIR spectra of the solids produced in the solutions at pH 12 and 12.5 corresponds to OH vibrations from water (cf Fig. S2). Under vacuum, the d 001 of the nontronite synthesized in the solution at pH 12 with the gel produced using the AlCl3 solution at pH 10.6 collapsed to 10.06 Å (Fig. S1).
Syntheses from the Gels Obtained using the AlCl3 Solutions at pH 5.3 and pH 8
Both syntheses conducted in the solution at pH 12.5 produced nontronite as revealed by XRD (peaks at ~12.7 Å, 4.55 Å / 4.54 Å, 3.1 Å, 2.6 Å, 1.73 Å, 1.528 Å / 1.527 Å; Reference Baron, Petit, Tertre and DecarreauBaron et al., 2016a) and FTIR (bands at 3564, 812, 855, 707, and 665 cm–1; Reference Baron, Petit, Tertre and DecarreauBaron et al., 2016a; Reference Goodman, Russell, Fraser and WoodhamsGoodman et al., 1976; Figs. 5 and 6). However, a band at 707 cm–1, corresponding to [4]Fe–O vibrations, is present in both FTIR spectra, probably indicating [4]Fe3+ for [4]Si4+ tetrahedral substitutions.
Discussion
The results show that the conditions required for the syntheses of pure (i.e. with no other mineral) Al-substituted smectite end-members (saponite, beidellite, and nontronite) are very different, even though these smectites differ only by the cation present at their octahedral sites. In this article the sensitivity to pH conditions of the production of pure saponite, beidellite, and nontronite is discussed and the various protocols leading to their successful syntheses are summarized.
Influence of pH
The results reported here show that the synthesis of pure saponite does not depend heavily on the pH of the solution in which the gels of saponite composition are immersed (saponite was obtained in solutions at pH ranging from 5.5 to 14). This can be due to the stability of the starting gel of trioctahedral smectites, as previously observed by Reference Huertas, Cuadros, Huertas and LinaresHuertas et al. (2000). Of note, the saponites produced in the present study contain tetrahedral Al and no octahedral Al. In fact, the ATR-FTIR spectra of the saponites produced were very similar to the ATR-FTIR spectrum of saponite presented by Reference Kloprogge and PonceKloprogge and Ponce (2021), with a feature at 800–815 cm–1 attributed to δAl–O of tetrahedral Al (absent from the ATR-FTIR spectrum of talc which contains no tetrahedral Al; Reference Kloprogge and PonceKloprogge & Ponce, 2021). Plus, the absence of the FTIR band attributed to vMg2-Al–OH at 3625 cm–1 is consistent with the absence of octahedral Al (Reference Kloprogge and PonceKloprogge & Ponce, 2021).
The XRD pattern of the saponite synthesized in solutions at pH 14 exhibited narrower 001 reflections than those of the saponites synthesized in solutions at lower pH. Such a decrease in width indicates a decrease in the d 001 distance and can be interpreted as an increase in crystallinity (Reference Zhang, Fu, Wang and LingZhang et al., 2022). Consistently, high-pH conditions during syntheses have been reported to improve both the crystallinity and crystallization rate of saponites (Reference Blukis, Schindler, Couasnon and BenningBlukis et al., 2022), as is the case for high-temperature conditions (Reference Kloprogge and FrostKloprogge & Frost, 2000; Reference Kloprogge and PonceKloprogge & Ponce, 2021). Still, such a decrease in width may also indicate an increase in the permanent charge, i.e. a higher degree of [4]Al3+ for [4]Si4+ tetrahedral substitutions. Consistently, with increasing pH (from 5.5 to 14), the ѵSi–O–Si and δAl–O absorption bands shifted from 960 to 944 cm–1 and from 800 to 815 cm–1, respectively, while the ѵMg3OH and δMg3OH absorption bands of the synthesized saponites shifted from 3674 to 3685 cm–1 and from 655 to 640 cm–1, respectively (Fig. 2), such shifts having been interpreted previously as an increase in the permanent charge (Reference Meyer, Bennici, Vaulot, Rigolet and DzeneMeyer et al., 2020; Reference Pelletier, Michot, Humbert, Barrès, de la Caillerie and RobertPelletier et al., 2003). Note that the production of saponites with a higher charge should leave available Si and Mg in the system, possibly leading to the production of other phases such as brucite (Mg(OH)2), serpentine (Mg3Si2O5(OH)4), or talc (Si4Mg3O10(OH)2), i.e. an assemblage similar to what is obtained with a gel produced using Na2SiO3 and AlCl3 solutions at pH 14 (Fig. S3). The absence of these minerals in the final residue (only saponite is present according to XRD and FTIR data; Figs. 1 and 2) suggests either that both Si and Mg in excess have been leached during filtration or that some Mg has replaced Na as the interlayer cation. Additional data (such as elemental or nuclear magnetic resonance – NMR data) would be required to determine if the saponite produced by immersing the gel in a solution at pH 14 has exactly the same composition as those produced at lower pH.
In contrast to that of saponite, the synthesis of beidellite is highly sensitive to the pH of the AlCl3 solution and the pH of the solution in which gels are immersed. A gel of beidellite composition produced using an AlCl3 solution at pH 3.4 seems to be very unstable and does not lead to the formation of pure beidellite, irrespective of the pH of the solution used for the synthesis (cf Fig. S4). In contrast, a gel of beidellite composition produced using an AlCl3 solution at pH 10.6 will lead systematically to the formation of boehmite (cf Fig. S4). Syntheses using gels of beidellite composition immersed in pure water will lead to the formation of kaolins, while only zeolites form in solutions at high pH, as also reported by Reference De KimpeDe Kimpe (1976) and Reference Huertas, Cuadros, Huertas and LinaresHuertas et al. (2000). The cause resides in the (pH-dependent) form of Si and Al species. In pure water, H4SiO4, Al(OH)2 +, and Al(OH)2+ prevail, and Si and Al ions form tetrahedral and octahedral complexes, respectively, while at high pH (> 13), H2SiO4 – and Al(OH)4 – prevail, leading to the formation of only tetrahedral complexes (Table 1). Thus, the successful synthesis of pure beidellite occurs only at a very specific pH (i.e. 12), where fourfold and sixfold coordinated Al species exist, as previously suggested (Reference De KimpeDe Kimpe, 1976).
The synthesis of [4]Al-nontronite is also very sensitive to the pH of solutions, as is the case for [4]Fe-nontronite as acknowledged earlier (Reference Andrieux and PetitAndrieux & Petit, 2010; Reference Boumaiza, Dutournié, Le Meins, Limousy, Brendlé, Martin, Michau and DzeneBoumaiza et al., 2020; Reference Dzene, Dutournie, Brendle, Limousy, Le Meins, Michelin, Vidal, Gree, Abdelmoula, Martin and MichauDzene et al., 2022). Only the gel produced using an AlCl3 solution at pH 10.6 and immersed in a solution at pH 12.5 leads to pure [4]Al-nontronite. The syntheses conducted at pH <12.5 from the gels of nontronite composition produced using an AlCl3 solution at pH 10.6 led to the production of nontronite together with bayerite. Gels produced using an AlCl3 solution at pH 10.6 and immersed in solutions at pH 13 crystallized into pure nontronite, but these are [4]Fe-nontronites as indicated by the shift of the 06,33 reflection to lower angles and the shift of the ѵSi–O to lower wavelengths (Reference Baron, Petit, Tertre and DecarreauBaron et al., 2016a). A high pH, thus, seems to favor [4]Fe3+ for [4]Si4+ tetrahedral substitutions, as historically suggested by Reference GrubbGrubb (1969). The use of gels produced using an AlCl3 solution at pH 3.4 did not lead to the production of pure, well crystallized [4]Al-nontronite (only poorly crystalline nontronite is obtained at pH 12.5). The immersion of such gels in solutions at lower pH leads to the production of hisingerite (i.e. a precursor of nontronite containing no Al; Reference KohyamaKohyama, 1975; Reference Farmer, McHardy, Elsass and RobertFarmer et al., 1994; Reference EggletonEggleton, 1998; Reference Milliken and BishMilliken & Bish, 2014), while their immersion in solutions at higher pH leads to the production of a zeolite (analcime) together with [4]Fe-nontronite.
Mechanistic Considerations
This section concerns the reactions that have probably occurred during the syntheses of saponite, beidellite, and nontronite. Please note that the equations presented below refer to the theoretical products of the syntheses carried out in the present study.
Pure saponite can be synthesized following various protocols, at various temperatures (Reference Kloprogge and FrostKloprogge & Frost, 2000; Reference Meyer, Bennici, Vaulot, Rigolet and DzeneMeyer et al., 2020) and for different durations (Reference Zhang, Petit, He, Villiéras, Razafitianamaharavo, Baron, Tao and ZhuZhang et al., 2020), whatever the pH (Reference Blukis, Schindler, Couasnon and BenningBlukis et al., 2022). Here, saponite was obtained by immersing gels in solutions at pH ranging from 5.5 to 14, probably because the rather large Mg2+ ions did not compete with Al species for tetrahedral substitutions. The major species in the Na2SiO3 solution at 0.2 M at pH 13.1 are H2SiO4 2– and H3SiO4 – (Table 1). Although Al was present mainly as Al3+ in the AlCl3 solution, it converted to Al(OH)4 – when this solution was poured into the Na2SiO3 solution, leading to the polymerization of an aluminosilicate network (i.e. tetrahedral complexes) at high pH (as suggested by Reference Besselink, Stawski, Freeman, Hövelmann and ToBesselink et al., 2020). The subsequent addition of the MgCl2 solution was responsible for a slight decrease in the pH (down to 10 – Table 2), probably converting the remaining H2SiO4 2– ions into H3SiO4 –, thereby leading to the polymerization of Mg-rich octahedral complexes. The gel produced crystallized into saponite whatever the pH of the solution into which it will be immersed, following the overall simplified reaction, written with respect to the main species present in each starting solution at 20°C (cf Table 1).
Pure beidellite cannot be synthesized over a large range of pH. The pH of the solution in which the gel is immersed for crystallization has to be controlled precisely. Although the formation of tetrahedral complexes occurred as for saponite when pouring the AlCl3 solution at pH 3.9 into the Na2SiO3 solution at 0.2 M at pH 13.1, the subsequent addition of the second AlCl3 solution was responsible for a large decrease in the pH (down to 4.5 – Table 2), destabilizing the tetrahedral complexes already formed and converting the H2SiO4 2– ions into H4SiO4 and the Al(OH)4 – ions into Al(OH)2 +, Al(OH)2+, and Al3+. The gel obtained with the starting AlCl3 solution at pH 3.9 will crystallize into pure beidellite only if immersed in solutions at pH 12 (allowing the conversion of Al species into Al(OH)4 –, and thus the incorporation of tetrahedral Al) followed the overall simplified reaction, written with respect to the main species present in each starting solution at 20°C (cf Table 1):
If the gel is immersed in a solution at pH <12, only kaolins will be produced following Eq. 3, while if the gel is immersed in a solution at pH >12, only zeolites will be produced following Eq. 4 (together with SiO2 or Al(OH)3, respectively, which are probably leached during filtration). Note that a starting AlCl3 solution at pH >8, which would contain Al(OH)4 – ions, cannot be used to produce a gel because of the inevitable precipitation of AlOOH or Al(OH)3 (Fig. S4).
Pure nontronite cannot be synthesized over a large pH range. As for beidellite, the pH of the solution in which the gel is immersed for crystallization has to be controlled precisely, even though the pH of the starting AlCl3 solution does not seem to be critical, given that pure [4]Fe-nontronite or [4]Al-nontronite were produced here from AlCl3 solutions at either pH 3.4 or 10.6. However, here, only the use of an AlCl3 solution at pH 10.6 led to the production of [4]Al-Nontronite. As for saponite and beidellite, the formation of tetrahedral complexes occurred when pouring the AlCl3 solution into the 0.2 M Na2SiO3 solution at pH 13.1. The subsequent addition of the FeCl3 solution was responsible for only a slight decrease in the pH (down to 9; Table 2), leading to the production of Fe-rich octahedral complexes forming a gel which would crystallize into pure [4]Al-nontronite only if immersed in solutions at pH 12.5 following the overall simplified reaction, written with respect to the main species present in each starting solution at 20°C (cf Table 1):
At high pH, the major species in solution were H3SiO4 –, H2SiO4 2–, Al(OH)4 –, and Fe(OH)4 – (Reference Guan, Dong, Ma and JiangGuan et al., 2009; Reference Perry and ShafranPerry & Shafran, 2001), with Al(OH)4 – competing with Fe(OH)4 – for tetrahedral substitutions (Reference Decarreau and PetitDecarreau & Petit, 2014). According to the present results, if the gel is immersed in a solution at pH 12.5, Al(OH)4 – is preferentially incorporated into tetrahedral sites over Fe(OH)4 –, leading eventually to the production of [4]Al-nontronite. In contrast, if the gel is immersed in a solution at pH >12.5, Fe(OH)4 – is incorporated preferentially into tetrahedral sites over Al(OH)4 –, eventually leading to the production of [4]Fe-nontronite rather than [4]Al-nontronite (cf Fig. 6). At pH <12.5, Al seems to be incorporated neither in tetrahedral nor octahedral sites and bayerite is produced together with [4]Fe-nontronite (Fig. 6).
Concluding Remarks
Optimal pH for the Synthesis of Saponite, Beidellite, and Nontronite
The successful synthesis of saponite was achieved by exposing the starting gels to a temperature of 230°C for 4 days in solutions at pH ranging from 5.5 to 14, confirming the pH non-sensitivity of saponite production (Reference Blukis, Schindler, Couasnon and BenningBlukis et al., 2022). Of note, the gel-to-solution ratio is an important parameter. Here, a mass of ~100 mg of gel was immersed in 16.5 mL of solution. In a similar volume of solution, a smaller (50 mg) or a larger (200 mg) mass of gel led to the formation of less crystalline saponites (data not shown here).
The successful synthesis of beidellite was achieved by exposing the gel obtained using the AlCl3 solution at pH 3.9 to 230°C for 9 days in a solution at pH 12. The gel-to-solution ratio is also an important parameter. Here, a mass of about 80 mg of gel was immersed into 12.5 mL of solution at pH 12. In a similar volume of solution, a lower mass of gel (60 mg) led to the formation of zeolites, while a larger mass of gel (100 mg) led to the formation of kaolins and aluminum hydroxides (data not shown here).
The successful synthesis of nontronite was achieved by exposing the starting gels to 150°C for 2.5 days in solutions at pH between 12.5 and 13. Pure nontronite was obtained by immersing gels prepared with an AlCl3 solution at a pH above 5 in solutions at pH 12.5 (confirming the results of Reference Andrieux and PetitAndrieux & Petit, 2010). Here, a mass of ~165 mg of gel was immersed in 16.5 mL of solution. Of note, changing this ratio will influence the pH and may lead to the additional production of either analcime or aluminum hydroxides (data not shown here).
Implications for Natural Systems
Smectites carry key information on the geochemistry, oxidation state, and water content of the environments in which they were produced (Reference Ehlmann, Mustard, Clark, Swayze and MurchieEhlmann et al., 2011; Reference Fox, Kupper, Ehlmann, Catalano, Razzell-Hollis, Abbey, Schild, Nickerson, Peters, Katz and WhiteFox et al., 2021), making them good indicators of paleoenvironmental and paleoclimatic conditions. Although further characterization (such as elemental or NMR analyses) would be required to ascertain the exact structure and composition of the various products more precisely, the present study shows that the optimal pH for the synthesis of saponite, beidellite, or nontronite is different; pH conditions influence strongly the purity and the final crystallochemistry of the smectites produced. Although extrapolating experimental results to natural settings remains complicated, the present results suggest that the crystallochemistry of natural smectites could also be used (a priori) as a paleo-pH proxy. However, smectitic clay minerals are rarely pure in natural settings, and most often exist in a complicated assemblage of various (more or less interstratified) clay mineral phases. Plus, natural clay minerals, either terrestrial or extraterrestrial, have usually experienced a complex history, including possible transport, mixing, reworking, and alteration, without mentioning interactions with organic compounds which may influence the crystallization and the final crystallochemistry of clay minerals (Reference Jacquemot, Viennet, Bernard, Le Guillou, Rigaud, Delbes, Georgelin and JaberJacquemot et al., 2019; Reference Viennet, Bernard, Le Guillou, Jacquemot, Balan, Delbes, Rigaud, Georgelin and JaberViennet et al., 2019, Reference Viennet, Le Guillou, Baron, Balan, Criouet, Delbes, Blanchenet, Laurent, Remusat and Bernard2022). Finally, the precise estimation of an age is fundamental for a proxy to be useful, and it remains very difficult to date smectitic clay minerals other than relying on certain impurities (transition ions) and point defects (radicals) which may be probed using electron paramagnetic resonance spectroscopy (Reference Allard, Balan, Calas, Fourdrin, Morichon and SorieulAllard et al., 2012; Reference Balan, Allard, Morin, Fritsch, Calas and BertrandBalan et al., 2020). Still, there is no doubt that the results of the present study will be of great help to constrain better the geochemical conditions existing or having existed on extraterrestrial planetary bodies such as Mars, on which the production of clay minerals has been intense (Reference Carter, Poulet, Bibring, Mangold and MurchieCarter et al., 2013; Reference Ehlmann and EdwardsEhlmann & Edwards, 2014), or on rocky and/or icy small bodies such as Ceres, Enceladus, or Europa on which the production of (probably smectitic) clay minerals have recently been reported (Reference Marchi, Raponi, Prettyman, Sanctis, Castillo-Rogez, Raymond, Ammannito, Bowling, Ciarniello, Kaplan, Palomba, Russell, Vinogradoff and YamashitaMarchi et al., 2019; Reference Nordheim, Hand and ParanicasNordheim et al., 2018; Reference Waite, Glein, Perryman, Teolis, Magee, Miller, Grimes, Perry, Miller, Bouquet, Lunine, Brockwell and BoltonWaite et al., 2017).
Acknowledgements
The authors acknowledge the spectroscopic and X-ray diffraction facilities of the Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie (IMPMC) and Elisabeth Malassis for administrative support.
Authors’ Contributions
IC, JCV, and SB designed the present study. IC and JCV performed the FTIR and the XRD analyses, with the help of LD and MG. All authors contributed to the interpretation of the data and discussed their implications. IC, JCV, and SB wrote the present manuscript, with critical inputs from FB, AB, and EB.
Funding
This work was mode possible thanks to financial support from the ATM program at MNHN (Project BioMars; PI: S. Bernard), from the Institut des Matériaux of Sorbonne Université (IMat) (Project Ageing on Mars; PI: S. Bernard) and from the European Research Council (ERC Consolidator Grant No. 819587: HYDROMA; PI: L. Remusat).
Data Availability
All data are available at https://drive.google.com/drive/folders/1prbEh1-XBEL-Qcb8NxvS1qzrygQ873yZ?usp=sharing
Declarations
Conflicts of Interest
The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this article.
Supplementary Information
The online version contains supplementary material available at https://doi.org/10.1007/s42860-023-00255-3.