Petrology and U–Pb geochronology of zircon in a suite of charnockitic gneisses from parts of the Chotanagpur Granite Gneiss Complex (CGGC): evidence for the reworking of a Mesoproterozoic basement during the formation of the Rodinia supercontinent
Abstract:Understanding the evolution of the Chotanagpur Granite Gneiss Complex (CGGC) of the East Indian Shield is crucial to decipher the role of the Indian Shield in the formation of the Rodinia supercontinent. The area around Deoghar–Dumka exposes a suite of granulite-facies orthogneisses (variably retrogressed to amphibole–biotite gneiss) that enclose remnants of Palaeoproterozoic metasedimentary and meta-igneous rocks. Results from mineral chemistry, laser ablation inductively coupled plasma mass spectrometry (LA … Show more
“…The Mesoproterozoic overprint is synchronous with the emplacement of A‐type felsic orthogneisses ( c . 1.45 Ga) in the Deoghar–Dumka area in the eastern part of the gneiss complex (Mukherjee et al., ). The early Neoproterozoic 1.03–0.96 Ga ages can be correlated with the Grenville‐age high‐grade metamorphism accompanied by regional deformation and granite magmatism that pervasively affected a large part of the CGC (Acharyya, ; Chatterjee et al., ; Maji et al., ; Rekha et al., ; Sanyal & Sengupta, ; Sanyal et al., ).…”
Section: Discussionmentioning
confidence: 99%
“…922 Ma. The closure of the rift basin due to compressional tectonics during continent–continent collision between 900 and 780 Ma formed the regional S 3 fabric at amphibolite facies condition (Chatterjee et al., ; Karmakar et al., ; Maji et al., ; Mukherjee et al., ; Sanyal & Sengupta, ; Sanyal et al., ).…”
Section: Regional Geological Settingmentioning
confidence: 99%
“…The terrane has a polychronous evolutionary history involving granitic and charno‐enderbitic magmatism at 1.70–1.64 Ga and c . 45 Ga respectively (Mukherjee et al., ; Saikia et al., ), granulite facies metamorphism and partial melting at c . 1.65 and c .…”
Section: Introductionmentioning
confidence: 99%
“…1.65 and c . 1.0 Ga (Chatterjee, Crowley, & Ghose, ; Chatterjee & Ghose, ; Dey et al., ; Karmakar et al., ; Maji et al., ; Mukherjee et al., ; Rekha et al., ; Sanyal & Sengupta, ; Sanyal et al., ), anorthosite emplacement at c . 1.55 Ga (Chatterjee et al., ), nepheline syenite intrusion at c .…”
Section: Introductionmentioning
confidence: 99%
“…1.55 Ga (Chatterjee et al., ), nepheline syenite intrusion at c . 0.92 Ga, and amphibolite facies metamorphism/deformation between 900 and 780 Ma (Chatterjee, Banerjee, Bhattacharya, & Maji, ; Karmakar et al., ; Maji et al., ; Mukherjee et al., ; Sanyal & Sengupta, ; Sanyal et al., ). The North Singhbhum Mobile Belt is dominated by a volcanosedimentary succession of interlayered quartzite, schist, and phyllite intercalated with ultramafic, mafic, and felsic volcanic and plutonic rocks.…”
The Central Indian Tectonic Zone (CITZ) is a Proterozoic suture along which the Northern and Southern Indian Blocks are inferred to have amalgamated forming the Greater Indian Landmass. In this study, we use the metamorphic and geochronological evolution of the Gangpur Schist Belt (GSB) and neighbouring crustal units to constrain crustal accretion processes associated with the amalgamation of the Northern and Southern Indian Blocks. The GSB sandwiched between the Bonai Granite pluton of the Singhbhum craton and granite gneisses of the Chhotanagpur Gneiss Complex (CGC) links the CITZ and the North Singhbhum Mobile Belt. New zircon age data constrain the emplacement of the Bonai Granite at 3,370 ± 10 Ma, while the magmatic protoliths of the Chhotanagpur gneisses were emplaced at c. 1.65 Ga. The sediments in the southern part of the Gangpur basin were derived from the Singhbhum craton, whereas those in the northern part were derived dominantly from the CGC. Sedimentation is estimated to have taken place between c. 1.65 and c. 1.45 Ga. The Upper Bonai/Darjing Group rocks of the basin underwent major metamorphic episodes at c. 1.56 and c. 1.45 Ga, while the Gangpur Group of rocks were metamorphosed at c. 1.45 and c. 0.97 Ga. Based on thermobarometric studies and zircon–monazite geochronology, we infer that the geological history of the GSB is similar to that of the North Singhbhum Mobile Belt with the Upper Bonai/Darjing and the Gangpur Groups being the westward extensions of the southern and northern domains of the North Singhbhum Mobile Belt respectively. We propose a three‐stage model of crustal accretion across the Singhbhum craton—GSB/North Singhbhum Mobile Belt—CGC contact. The magmatic protoliths of the Chhotanagpur Gneisses were emplaced at c. 1.65 Ga in an arc setting. The earliest accretion event at c. 1.56 Ga involved northward subduction and amalgamation of the Upper Bonai Group with the Singhbhum craton followed by accretion of the Gangpur Group with the Singhbhum craton–Upper Bonai Group composite at c. 1.45 Ga. Finally, continent–continent collision at c. 0.96 Ga led to the accretion of the CGC with the Singhbhum craton–Upper Bonai Group–Gangpur Group crustal units, synchronous with emplacement of pegmatitic granites. The geological events recorded in the GSB and other units of the CITZ only partially overlap with those in the Trans North China Orogen and the Capricorn Orogen of Western Australia, indicating that these suture zones are not correlatable.
“…The Mesoproterozoic overprint is synchronous with the emplacement of A‐type felsic orthogneisses ( c . 1.45 Ga) in the Deoghar–Dumka area in the eastern part of the gneiss complex (Mukherjee et al., ). The early Neoproterozoic 1.03–0.96 Ga ages can be correlated with the Grenville‐age high‐grade metamorphism accompanied by regional deformation and granite magmatism that pervasively affected a large part of the CGC (Acharyya, ; Chatterjee et al., ; Maji et al., ; Rekha et al., ; Sanyal & Sengupta, ; Sanyal et al., ).…”
Section: Discussionmentioning
confidence: 99%
“…922 Ma. The closure of the rift basin due to compressional tectonics during continent–continent collision between 900 and 780 Ma formed the regional S 3 fabric at amphibolite facies condition (Chatterjee et al., ; Karmakar et al., ; Maji et al., ; Mukherjee et al., ; Sanyal & Sengupta, ; Sanyal et al., ).…”
Section: Regional Geological Settingmentioning
confidence: 99%
“…The terrane has a polychronous evolutionary history involving granitic and charno‐enderbitic magmatism at 1.70–1.64 Ga and c . 45 Ga respectively (Mukherjee et al., ; Saikia et al., ), granulite facies metamorphism and partial melting at c . 1.65 and c .…”
Section: Introductionmentioning
confidence: 99%
“…1.65 and c . 1.0 Ga (Chatterjee, Crowley, & Ghose, ; Chatterjee & Ghose, ; Dey et al., ; Karmakar et al., ; Maji et al., ; Mukherjee et al., ; Rekha et al., ; Sanyal & Sengupta, ; Sanyal et al., ), anorthosite emplacement at c . 1.55 Ga (Chatterjee et al., ), nepheline syenite intrusion at c .…”
Section: Introductionmentioning
confidence: 99%
“…1.55 Ga (Chatterjee et al., ), nepheline syenite intrusion at c . 0.92 Ga, and amphibolite facies metamorphism/deformation between 900 and 780 Ma (Chatterjee, Banerjee, Bhattacharya, & Maji, ; Karmakar et al., ; Maji et al., ; Mukherjee et al., ; Sanyal & Sengupta, ; Sanyal et al., ). The North Singhbhum Mobile Belt is dominated by a volcanosedimentary succession of interlayered quartzite, schist, and phyllite intercalated with ultramafic, mafic, and felsic volcanic and plutonic rocks.…”
The Central Indian Tectonic Zone (CITZ) is a Proterozoic suture along which the Northern and Southern Indian Blocks are inferred to have amalgamated forming the Greater Indian Landmass. In this study, we use the metamorphic and geochronological evolution of the Gangpur Schist Belt (GSB) and neighbouring crustal units to constrain crustal accretion processes associated with the amalgamation of the Northern and Southern Indian Blocks. The GSB sandwiched between the Bonai Granite pluton of the Singhbhum craton and granite gneisses of the Chhotanagpur Gneiss Complex (CGC) links the CITZ and the North Singhbhum Mobile Belt. New zircon age data constrain the emplacement of the Bonai Granite at 3,370 ± 10 Ma, while the magmatic protoliths of the Chhotanagpur gneisses were emplaced at c. 1.65 Ga. The sediments in the southern part of the Gangpur basin were derived from the Singhbhum craton, whereas those in the northern part were derived dominantly from the CGC. Sedimentation is estimated to have taken place between c. 1.65 and c. 1.45 Ga. The Upper Bonai/Darjing Group rocks of the basin underwent major metamorphic episodes at c. 1.56 and c. 1.45 Ga, while the Gangpur Group of rocks were metamorphosed at c. 1.45 and c. 0.97 Ga. Based on thermobarometric studies and zircon–monazite geochronology, we infer that the geological history of the GSB is similar to that of the North Singhbhum Mobile Belt with the Upper Bonai/Darjing and the Gangpur Groups being the westward extensions of the southern and northern domains of the North Singhbhum Mobile Belt respectively. We propose a three‐stage model of crustal accretion across the Singhbhum craton—GSB/North Singhbhum Mobile Belt—CGC contact. The magmatic protoliths of the Chhotanagpur Gneisses were emplaced at c. 1.65 Ga in an arc setting. The earliest accretion event at c. 1.56 Ga involved northward subduction and amalgamation of the Upper Bonai Group with the Singhbhum craton followed by accretion of the Gangpur Group with the Singhbhum craton–Upper Bonai Group composite at c. 1.45 Ga. Finally, continent–continent collision at c. 0.96 Ga led to the accretion of the CGC with the Singhbhum craton–Upper Bonai Group–Gangpur Group crustal units, synchronous with emplacement of pegmatitic granites. The geological events recorded in the GSB and other units of the CITZ only partially overlap with those in the Trans North China Orogen and the Capricorn Orogen of Western Australia, indicating that these suture zones are not correlatable.
The Central Indian Tectonic Zone, because of its critical position in the tectonic framework of East Gondwanaland, holds insights into our understanding of the assembly and dispersal of Columbia and Rodinia supercontinents through the growth of the Greater Indian Landmass. The tectonic zone, which is now a collage of different supracrustal and granulite‐gneiss belts, bears testimony to a multistage orogenic evolution from Late Palaeoproterozoic to Early Neoproterozoic time. In this contribution, the current status of orogenic evolution in the Central Indian Tectonic Zone has been reviewed using petrological and geochronological constraints from the Sausar Mobile Belt, its southernmost constituent. It reveals a three‐stage evolution leading to the growth of the Greater Indian Landmass: (a) c. 1.6–1.5‐Ga accretionary orogenesis produced the first nucleus of Greater India through the assembly of arc, back arc, and continental margins; (b) a phase of Middle Proterzoic extension led to the disintegration of the Proto‐Greater India; and (c) classical Himalayan‐style continental collision between 1.06 and 0.93 Ga finally stitched the North and South India blocks to produce the final configuration of the Greater Indian Landmass. It is argued that the Late Palaeoproterozoic to Early Mesoproterozoic orogenesis in India and former Gondwanaland and Laurentian fragments is a globally significant amalgamation event separate from the Columbia Supercontinent assembly.
The north‐eastern part of the Chotanagpur Granite Gneiss Complex (CGGC) in the East Indian shield contains enclaves of migmatitic pelitic granulites (PG) within felsic orthogneiss (FOG). Field observations, petrology and geochronology (LA–MC–ICP–MS U–Pb dating of zircon and EPMA Th–U–total‐Pb dating of monazite) of the PG suggest two distinct metamorphic events. The earliest event M1, which is characterized by high‐temperature (>850°C) granulite facies metamorphism, occurred in the timespan of ~1680–1580 Ma. Extensive dehydration melting of biotite + sillimanite + quartz‐rich protoliths led to stabilization of the restitic assemblage (garnet + alkali‐feldspar + quartz + sillimanite + ferrian‐ilmenite) together with large volumes of felsic melts (leucosomes). Collisional tectonics followed by delamination and asthenospheric upwelling could have triggered the M1 event. Subsequently, at ~1470–1400 Ma, the igneous protolith of the host FOG intruded and hydrated the PG. Thereafter, a second metamorphic event, M2, accompanied by compressional structures, affected both the rock types. A clockwise P–T path that culminated at ≥10 kbar ~760–850°C and is followed by a steeply decompressive retrograde path characterizes this event. The P–T path and the inferred geothermal gradient (<27°C/km) are compatible with a continent–continent collisional setting. Geochronological findings suggest a protracted orogeny for the M2 event with its major pulse during ~970–950 Ma. When combined with the published information, this study supports the view that a large (if not the entire) portion of the Indian shield and the granulite terranes of east Antarctica share similar tectonothermal events that led to the formation of two supercontinents, Columbia and Rodinia.
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