Mineralogical and geochemical studies were carried out in chromitites belonging to the mafic–ultramafic bodies of Niquelaˆndia, Luanga, and Campo Formoso, which are, respectively, included in the Goia´s Massif and the Amazon and Sa˜o Francisco cratons. The main platinum-group minerals (PGM) included or associated with chromite grains are laurite in Niquelaˆndia and Campo Formoso and sperrylite and braggite in Luanga. The most common primary base metal sulfides (BMS) are pentlandite, chalcopyrite, and minor pyrrhotite. Also present are base metal alloys (BMA), such as awaruite, and the BMS millerite, pyrite, and copper as secondary mineral phases linked to later alteration process. The Luanga chromites display the lowest Cr2O3/Al2O3 and Cr2O3/FeOt ratios. The chondrite-normalized profiles are strongly enriched in the platinum PGE subgroup (PPGE, Pt, Pd, Rh). The average Pd/Ir ratio (24.2) and 187Os/188Os values (0.17869–0.18584) are very high. Niquelaˆndia chromites have higher Cr2O3/Al2O3 and Cr2O3/FeOt ratios than Luanga. Its PGE contents are low and chondrite-normalized profiles depleted, mainly in the PPGE subgroup. The average Pd/Ir ratio (0.45) and 187Os/188Os values (0.12598–0.12777) are low. Campo Formoso chromites have the highest Cr2O3/Al2O3 and Cr2O3/FeOt ratios; its average Pd/Ir ratio (0.72) and chondrite-normalized profiles (except the pronounced Ru spike) are closer to those of Niquelaˆndia. The remarkable differences in terms of chromite bulk-composition, PGE contents and patterns, Pd/Ir ratios, and 187Os/188Os values associated with probable distinctions in the inferred geochemical compositions of the respective parental magmas indicate that the Luanga and Niquelaˆndia complexes originated from distinct parental sources. Geochemical and isotopic features indicate that Luanga chromitites and associated rocks are consistent with a parental magma, either originated from an enriched mantle reservoir or strongly contaminated, whereas Niquelaˆndia derives from a depleted mantle source, which displays a slightly positive Os anomaly.

A comparison of selected Precambrian Brazilian chromitites: chromite, PGE-PGM, Re/Os as parental source indicators.

Diella V
2006

Abstract

Mineralogical and geochemical studies were carried out in chromitites belonging to the mafic–ultramafic bodies of Niquelaˆndia, Luanga, and Campo Formoso, which are, respectively, included in the Goia´s Massif and the Amazon and Sa˜o Francisco cratons. The main platinum-group minerals (PGM) included or associated with chromite grains are laurite in Niquelaˆndia and Campo Formoso and sperrylite and braggite in Luanga. The most common primary base metal sulfides (BMS) are pentlandite, chalcopyrite, and minor pyrrhotite. Also present are base metal alloys (BMA), such as awaruite, and the BMS millerite, pyrite, and copper as secondary mineral phases linked to later alteration process. The Luanga chromites display the lowest Cr2O3/Al2O3 and Cr2O3/FeOt ratios. The chondrite-normalized profiles are strongly enriched in the platinum PGE subgroup (PPGE, Pt, Pd, Rh). The average Pd/Ir ratio (24.2) and 187Os/188Os values (0.17869–0.18584) are very high. Niquelaˆndia chromites have higher Cr2O3/Al2O3 and Cr2O3/FeOt ratios than Luanga. Its PGE contents are low and chondrite-normalized profiles depleted, mainly in the PPGE subgroup. The average Pd/Ir ratio (0.45) and 187Os/188Os values (0.12598–0.12777) are low. Campo Formoso chromites have the highest Cr2O3/Al2O3 and Cr2O3/FeOt ratios; its average Pd/Ir ratio (0.72) and chondrite-normalized profiles (except the pronounced Ru spike) are closer to those of Niquelaˆndia. The remarkable differences in terms of chromite bulk-composition, PGE contents and patterns, Pd/Ir ratios, and 187Os/188Os values associated with probable distinctions in the inferred geochemical compositions of the respective parental magmas indicate that the Luanga and Niquelaˆndia complexes originated from distinct parental sources. Geochemical and isotopic features indicate that Luanga chromitites and associated rocks are consistent with a parental magma, either originated from an enriched mantle reservoir or strongly contaminated, whereas Niquelaˆndia derives from a depleted mantle source, which displays a slightly positive Os anomaly.
2006
Istituto per la Dinamica dei Processi Ambientali - IDPA - Sede Venezia
Istituto di Geologia Ambientale e Geoingegneria - IGAG
Chromitite
Niquelaˆndia
Luanga
Campo Formoso
Mantle
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/48079
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