The distribution of ferric iron (Fe 3+ ) between the octahedral and tetrahedral sheets of smectites is still an active problem due to the difficulty of identifying and quantifying the tetrahedral ferric iron ( [4] Fe 3+ ). Mossbauer spectroscopy has often been used to address this problem, with the spectra being fitted by a sum of doublets, but the empirical attribution of each doublet has failed to yield a uniform interpretation of the spectra of natural reference Fe 3+ -rich smectites, especially with regard to [4] Fe 3+ , because little consensus exists as to the [4] Fe 3+ content of natural samples. In an effort to resolve this problem, the current study was undertaken using a series of synthetic nontronites [Si 4–x [4] Fe x 3+ ] [6] Fe 2 3+ O 10 (OH) 2 Na x with x ranging from 0.51 to 1.3. Mossbauer spectra were obtained at 298, 77, and 4 K. Statistically acceptable deconvolutions of the Mossbauer spectra at 298 and 77 K were used to develop a model of the distribution of tetrahedral substitutions, taking into account: (1) the [4] Fe 3+ content; (2) the three possible tetrahedral cationic environments around [6] Fe 3+ , i.e., [4Si]-(3 [6] Fe 3+ ), [3Si [4] Fe 3+ ]-(3 [6] Fe 3+ ), and [2Si 2 [4] Fe 3+ ]-(3 [6] Fe 3+ ); and (3) the local environment around a [4] Fe 3+ , i.e., [3Si]-(2 [6] Fe 3+ ) respecting Lowenstein’s Rule. This approach allowed the range of Mossbauer parameters for [6] Fe 3+ and [4] Fe 3+ to be determined and then applied to spectra of natural Fe 3+ -rich smectites. Results revealed the necessity of taking into account the distribution of tetrahedral cations ( [4] R 3+ ) around [6] Fe 3+ cations to deconvolute the Mossbauer spectra, and also highlighted the influence of sample crystallinity on Mossbauer parameters.
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