Abstract
The distribution of heavy metals in typical Terra Rossa soils and their partitioning in specific soil phases are estimated on the basis of the comparative evaluation of bulk contents, results from sequential chemical extraction procedure (SEP) and scanning electron microscopy/energy dispersive X-ray analysis (SEMEDX). A general natural enrichment of heavy metals with respect to average soil is observed. Cadmium proves to be remarkably high (up to 2.4 ppm). Large amounts of Fe, Cr, Cu, Ni, Pb, and Zn occur in the ‘residual’ fraction. The results indicate selective accumulation of the heavy metals in Fe oxides, present as hematite, goethite and maghemite. There is good evidence that Mn and Cd are subjected to similar influences, both elements mainly occurring in the ‘easily reducible’ fraction. The affinity of Cd for poorly crystallized Mn oxides governs its behaviour and mobility, which may significantly increase in moderate reducing conditions in relation to Mn phases stability.
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