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The "Calamine" of Southwest Sardinia: Geology, Mineralogy, and Stable Isotope Geochemistry of Supergene Zn Mineralization

Maria Boni

Dipartimento di Geofisica and Vulcanologia, Università di Napoli "Federico II," Via Mezzocannone 8, 80134-Napoli, Italy

H. Albert Gilg

Fakultät Chemie, Technische Universität München, Lichtenbergstr. 4, 8574-Garching, Germany

Gaspare Aversa^*

Dipartimento di Geofisica and Vulcanologia, Università di Napoli "Federico II,"Via Mezzocannone 8, 80134-Napoli, Italy

Giuseppina Balassone

Dipartimento di Scienze della Terra, Università di Napoli "Federico II," Via Mezzocannone 8, 80134-Napoli, Italy

Corresponding author: e-mail, boni{at}unina.it

The mining district of southwest Sardinia, Italy, is one of the classic areas where primary carbonate-hosted Zn-Pb sulfide ores are associated with a relatively thick secondary oxidation zone containing Zn (hydroxy-)carbonates and silicates, the so-called "calamine," exploited until the 1970s. The extent of the capping oxidized ore zones, reaching deep below the surface, is generally independent of the present-day water table. The base of the oxidation profile containing nonsulfide Zn minerals in various uplifted blocks in the Iglesiente area can be both elevated above or submerged below the recent water table. The genesis of the ores is therefore considered to be related to fossil, locally reactivated, oxidation phenomena. The mineralogy of the nonsulfide mineralization is generally complex and consists of smithsonite, hydrozincite, and hemimorphite as the main economic minerals, accompanied by iron and manganese oxy-hydroxides and residual clays.

This study places the secondary ores in the context of the tectonostratigraphic and climatic evolution of Sardinia and includes a petrographic and mineralogic study of the most abundant minerals, relating the mineralogy of secondary Zn and Pb carbonates to their stable C and O isotope geochemistry and constraining the origin of the oxidizing fluids and the temperature of mineralization. The ¹⁸O_VSMOW values of smithsonite are homogeneous, regardless of crystal morphology, position, and mine location (avg. 27.4 ± 0.9). This homogeneity points to a relatively uniform isotopic composition of the oxidation fluid and corresponding formation temperatures of 20° to 35°C. Considering the karstic environment of smithsonite formation in southwest Sardinia, this high temperature could be due to heat release during sulfide oxidation. The carbon isotope compositions of secondary Zn carbonates display considerable variations of more than 9 per mil (¹³C_VPDB from –0.6 to –10.4). This large range indicates participation of variable amounts of reduced organic and marine carbonate carbon during sulfide oxidation. The isotopic variation can be related to a variation in crystal morphologies of smithsonite, reflecting different environments of formation with respect to water table oscillations in karstic environments (upper to lower vadose to epiphreatic). The same range in ¹³C isotope values is displayed by the calcite associated with Zn carbonates and by recent speleothems.

The most reliable time span for the deposition of bulk calamine ore in southwest Sardinia ranges from middle Eocene to Plio-Pleistocene, although further multiple reactivation of the weathering profiles, peaking within the warm interglacial periods of the Quaternary, cannot be excluded.

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