2001
DOI: 10.1016/s0375-6742(01)00161-3
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Regional oxygen isotope systematics of felsic volcanics; a potential exploration tool for volcanogenic massive sulphide deposits in the Iberian Pyrite Belt

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Cited by 6 publications
(5 citation statements)
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“…Whilst, lack of exposure of bedrock in the area prevented this hypothesis from being tested, the main mineralisation orientation is W-E at Tharsis and Ríotinto (Figs. 2 and 3;Carvalho 1998;Saez et al 1999;Lerouge et al 2001;Lunar et al 2002;Solomon et al 2004). If trace element concentrations were to reflect parent material, high values would be expected in W-E bands which is not the case (Figs.…”
Section: Discussionmentioning
confidence: 99%
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“…Whilst, lack of exposure of bedrock in the area prevented this hypothesis from being tested, the main mineralisation orientation is W-E at Tharsis and Ríotinto (Figs. 2 and 3;Carvalho 1998;Saez et al 1999;Lerouge et al 2001;Lunar et al 2002;Solomon et al 2004). If trace element concentrations were to reflect parent material, high values would be expected in W-E bands which is not the case (Figs.…”
Section: Discussionmentioning
confidence: 99%
“…Parent materials at Tharsis and Ríotinto consist mostly of submarine felsic to mafic volcanic rocks intercalated with marine sediments (slate, quartzite, greywacke, limestone, chert) (Saez et al 1999;Lerouge et al 2001;Lunar et al 2002;Solomon et al 2004) of Middle Famennian-Upper Visean age (Oliveira 1983). These rocks host the sulphide mineralisation of the Iberian Pyrite Belt (Kase et al 1990;Saez et al 1999;Lerouge et al 2001;Lunar et al 2002;Solomon et al 2004). The sand-type geological formations of the Huelva area have been dated as Upper Miocene-Lower Pliocene (Muniz and Mayoral 2001).…”
Section: Study Areamentioning
confidence: 99%
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“…Oliver et al (1998) advocated a 500 m zone of locally depleted whole-rock oxygen isotope values (δ 18 O = +6.4 to +9.3‰, relative to V-SMOW) within and adjacent to the Kanmantoo deposit that formed as a result of localized fluid flow derived from a crystallizing magma. However, Marshall and Spry (2000) suggested the isotopic anomaly could just as easily result from hydrothermal fluid flow related to the formation of massive sulfide deposits via syn-sedimentary hydrothermal exhalations (e.g., Nesbitt, 1996;Brauhart et al, 2000;Lerouge et al, 2001).…”
Section: Stable Isotopesmentioning
confidence: 99%