Aravalli A-type granites (ca. 1.72 Ga), NW India: Petrogenesis, geodynamic evolution, and global implications for late Paleoproterozoic crustal reworking
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Abstract
The geochemical and isotopic data for ca. 1.72 Ga A-type granites in the central Aravalli orogen, NW India, remain limited, hindering a detailed evaluation of their petrogenesis and tectonic setting. New results of combined zircon U-Pb-Hf isotope analyses and whole-rock geochemical data reveal that the A-type granites are characterised by high liquidus temperatures (≥850 °C), enrichment in rare earth elements and incompatible elements, and oxidised in nature. They were generated through partial melting of a silica-poor dioritic source within a post-collisional extensional setting. This A-type magmatism is synchronous with the emplacement of charnockites and granulite-facies metamorphism in the region. The coeval formation of A-type and charnockite magmas is attributed to partial melting of evolved Neoarchean crust (εHft = -12.5 to −5.2 and TDM2 = 3.02 to 2.68 Ga) at moderate depth (20–25 km), triggered by upwelling of asthenospheric mantle following a slab break-off at ca. 1730 Ma. This process induced lithospheric extension and granulite-facies metamorphism in the lower crust. A global compilation of zircon Hf isotope and whole-rock Nd isotope data for late Paleoproterozoic A-type granites suggests that these rocks primarily formed by large-scale reworking of existing crustal sources, with only limited melt contributions from depleted mantle sources, thereby having a negligible impact on crustal growth over time. On the contrary, the Phanerozoic A-type granites largely represent addition of new crust.
期刊介绍:
Precambrian Research publishes studies on all aspects of the early stages of the composition, structure and evolution of the Earth and its planetary neighbours. With a focus on process-oriented and comparative studies, it covers, but is not restricted to, subjects such as:
(1) Chemical, biological, biochemical and cosmochemical evolution; the origin of life; the evolution of the oceans and atmosphere; the early fossil record; palaeobiology;
(2) Geochronology and isotope and elemental geochemistry;
(3) Precambrian mineral deposits;
(4) Geophysical aspects of the early Earth and Precambrian terrains;
(5) Nature, formation and evolution of the Precambrian lithosphere and mantle including magmatic, depositional, metamorphic and tectonic processes.
In addition, the editors particularly welcome integrated process-oriented studies that involve a combination of the above fields and comparative studies that demonstrate the effect of Precambrian evolution on Phanerozoic earth system processes.
Regional and localised studies of Precambrian phenomena are considered appropriate only when the detail and quality allow illustration of a wider process, or when significant gaps in basic knowledge of a particular area can be filled.