Petrography, geochemistry and petrogenesis of calc-alkaline granitoids from the Mercara Shear Zone (MSZ), southwest of West Dharwar Craton, India: Indication of continental arc magmatism and deep-crustal melting
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引用次数: 0
Abstract
The Mercara Shear Zone (MSZ) is an intensely deformed, curvilinear, mylonitised zone juxtaposed between the Western Dharwar Craton (WDC) and the Coorg Block (CB). In the vicinity of Madikeri town, the MSZ exposes many bands and enclaves of granulite-grade meta-supracrustals and mafic granulites hosted within charnockite or felsic orthogneiss (retrogressed charnockite). Subsequently, the area is intruded by a suite of granitoids along the mid-axis of the shear zone, showing no signature of metamorphism. Views on the origin and timing of the formation of the granulite-grade rocks of the MSZ are not streamlined, and the unmetamorphosed suite of granitoids has not been studied in detail in light of the evolution of the terrain. The field relationship, petrography and bulk rock geochemistry of the suite of unmetamorphosed granitoids from the MSZ were carried out to address this issue. Petrological and geochemical data indicate an I-type affinity of the granitoids. Trace and rare earth element (REE) patterns suggest a magmatic arc setting. The rocks are calc-alkaline, and the REE pattern is fractionated, enriched in Ba, Sr, and depleted in high field strength elements like Nb, Ta, and Ti with almost no significant negative Eu anomaly. These characteristics indicate the dominance of crustal involvement over the mantle in the generation of melt. Studied samples show ‘adakite-like’ geochemical characteristics (high Sr/Y, La/Yb) but are not the product of typical slab melting. The present study indicates that the granitoids were derived from a thick crustal source by partial melting in an oxidized condition (fO2 between NNO and HM buffer) at 941–985°C and 10–12.5 kbar pressure (corresponding to 30–40 km depth).
期刊介绍:
The Journal of Earth System Science, an International Journal, was earlier a part of the Proceedings of the Indian Academy of Sciences – Section A begun in 1934, and later split in 1978 into theme journals. This journal was published as Proceedings – Earth and Planetary Sciences since 1978, and in 2005 was renamed ‘Journal of Earth System Science’.
The journal is highly inter-disciplinary and publishes scholarly research – new data, ideas, and conceptual advances – in Earth System Science. The focus is on the evolution of the Earth as a system: manuscripts describing changes of anthropogenic origin in a limited region are not considered unless they go beyond describing the changes to include an analysis of earth-system processes. The journal''s scope includes the solid earth (geosphere), the atmosphere, the hydrosphere (including cryosphere), and the biosphere; it also addresses related aspects of planetary and space sciences. Contributions pertaining to the Indian sub- continent and the surrounding Indian-Ocean region are particularly welcome. Given that a large number of manuscripts report either observations or model results for a limited domain, manuscripts intended for publication in JESS are expected to fulfill at least one of the following three criteria.
The data should be of relevance and should be of statistically significant size and from a region from where such data are sparse. If the data are from a well-sampled region, the data size should be considerable and advance our knowledge of the region.
A model study is carried out to explain observations reported either in the same manuscript or in the literature.
The analysis, whether of data or with models, is novel and the inferences advance the current knowledge.