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1 Departamento de Química Agrícola, Geología y Geoquímica, Facultad de Ciencias, Universidad Autónona de Madrid. Cantoblanco s/n 28049 Madrid, Spain
2 UMR 6532 CNRS, Universite de Poitiers, 40, Avenue du Recteur Pineau, 86022 Poitiers Cedex, France
* E-mail address of corresponding author: Jaime.Cuevas{at}uam.es
The chemical and structural properties of Mg smectites in the Vicálvaro sepiolite deposit have been studied in detail. The characterization was performed on different size-fractions of selected smectitic samples (52 µm; 21 µm; 10.5 µm; <0.5 µm and <0.1 µm). The chemical compositions of individual particles (51 µm) and of bulk undifferentiated fine fractions (1 <0.1 µm) were determined by energy dispersive spectroscopy-scanning electron microscopy and interpreted with the aid of X-ray diffraction (XRD) and infrared spectroscopy (IR) methods. The XRD and IR data demonstrate that all of the Mg smectite materials studied are mainly composed of a complex mixture of stevensite, saponite and mica-type minerals. Although the presence or absence of saponite cannot be confirmed absolutely, stevensite is a significant component of these Mg smectites. This is proven by the calculated layer charge reduction after the Hofmann-Klemen effect. The results are in close agreement with the suggested mechanism of topotactic overgrowth of stevensite on pre-existing phyllosilicate templates. This characterizes clay diagenesis in saline-lake systems.
Key Words: Fe-rich Dioctahedral Micas Lacustrine Mg Clays Saponite Stevensite Trioctahedral Smectites Vicálvaro Sepiolite Deposit Spain
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