Quick
Search: 
 
advanced search
 GSW Home    GeoRef Home    My GSW Alerts    Contact GSW    About GSW    Journals List    Help 
Clays and Clay Minerals Signup for GSW Email News
JOURNAL HOME HELP CONTACT PUBLISHER SUBSCRIBE ARCHIVE SEARCH TABLE OF CONTENTS

Clays and Clay Minerals; August 2004; v. 52; no. 4; p. 473-483; DOI: 10.1346/CCMN.2004.0520408
© 2004 Clay Minerals Society
This Article
Right arrow Figures Only
Right arrow Full Text
Right arrow Full Text (PDF)
Right arrow Alert me when this article is cited
Right arrow Alert me if a correction is posted
Right arrow Citation Map
Services
Right arrow Email this article to a friend
Right arrow Similar articles in this journal
Right arrow Similar articles in ISI Web of Science
Right arrow Alert me to new issues of the journal
Right arrow Download to citation manager
Right arrow reprints & permissions
Citing Articles
Right arrow Citing Articles via Google Scholar
Google Scholar
Right arrow Articles by Vingiani, S.
Right arrow Articles by Terribile, F.
Right arrow Search for Related Content
GeoRef
Right arrow GeoRef Citation

MIXED-LAYER KAOLINITE-SMECTITE MINERALS IN A RED-BLACK SOIL SEQUENCE FROM BASALT IN SARDINIA (ITALY)

Simona Vingiani1, Dominique Righi2,*, Sabine Petit2 and Fabio Terribile1

1 DISSPA, Università di Napoli Federico II, Facoltà di Agraria, Via Università 100, 80055 Portici (NA), Italy
2 UMR-CNRS 6532 "HydrASA", Faculté des Sciences, 86022 Poitiers Cedex, France

* E-mail address of corresponding author: dominique.righi{at}hydrasa.univ-poitiers.fr

Clay minerals from soils of a red-black soil complex developed from basaltic parent material in Sardinia are formed along a short toposequence (200 m). At the foot of the sequence, a clay-rich, black Vertisol forms, whereas at the summit, the soil is a dark reddish-brown Inceptisol. X-ray diffraction, infrared spectroscopy (FTIR), cation exchange capacity (CEC) and permanent and variable charges analyses were used, and the data show that clay minerals varied according to soil horizon and topographic position of the soil. Clay minerals in the Inceptisol are dominated by kaolinite and mixed-layer kaolinite-smectite (K-S, K:S >0.5), whereas the Vertisol contains smectites and K-S with K:S proportions <0.5. In the Vertisol, the proportion of kaolinitic layers in the K-S increases from the C horizon (K:S ~0.35–0.40) to the Ap horizon (K:S ~0.40–0.45). This soil clay-mineral distribution, in relation to topography, is similar to that reported for other (kaolinitic) red-black (smectitic) soil associations in subtropical and tropical areas. The sequence forms by downward drainage on summits and slopes, and buildup of ions in ‘lows’ produces smectites. Fourier transform infrared spectra indicate that two types of smectite are formed in the C horizon of the Vertisol; one is more ferric (Fe-beidellite, nontronite), the other more aluminous. Mineralogical evolution in the soil profile (from C to Ap horizon) shows a decreasing proportion of ferric smectite layers (compared to the more aluminous smectite layers). This would indicate that ferric smectite layers are preferentially transformed (or dissolved) to give kaolinite layers, with Fe precipitating as oxides and/or oxy-hydroxides or retained partly in kaolinite layers. Because the surface properties of clay minerals are related to mineralogy, the CEC (33–41 cmol kg–1) in the brown Inceptisol is ~50% pH-dependent charge while in the Vertisol up to ~75% of the CEC (48–61 cmol kg–1) comes from accessible permanent charges.

Key Words: Basalt (weathering) • Fe-beidellite • Italy • Mixed-layer Kaolinite-smectite • Nontronite • Red-black Soil Sequence • Sardinia • Vertisol







JOURNAL HOME HELP CONTACT PUBLISHER SUBSCRIBE ARCHIVE SEARCH TABLE OF CONTENTS
Copyright © 2008 by Clay Minerals Society