2010
DOI: 10.1007/s12594-010-0046-4
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Magnetic susceptibility mapping of felsic magmatic lithounits in the central part of Bundelkhand Massif, central India

Abstract: Late Archaean to Palaeoproterozoic felsic magmatic lithounits exposed in the central part of the Bundelkhand massif have been mapped and their redox series (magnetite vs ilmenite series) evaluated based on magnetic susceptibility (MS) data. The central part of Bundelkhand massif comprises of multiple felsic magmatic pulses (~2600-2200 Ma), commonly represented by coarse grained granite (CGG-grey granite, CPG-pink granite), medium grained pink granite (MPG), fine grained pink granite (FPG) , grey and pink rhyol… Show more

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Cited by 29 publications
(24 citation statements)
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(14 reference statements)
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“…The NeoArchaean acidic magmatism was a part of major geological process when the granite production occurred on a large scale and subsequently the Bundelkhand craton acquired thermal equilibrium of the stable geotherm. The signature of this event is marked by the emplacement of different types of granitoids that are available throughout the craton in time and space (Basu 2010;Mondal et al 2002;Kumar et al 2010). The successive events of granitoid magmatism occurred within a very short span of time in this craton (~50 Ma, Mondal et al 2002).…”
Section: Geological Backgroundmentioning
confidence: 99%
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“…The NeoArchaean acidic magmatism was a part of major geological process when the granite production occurred on a large scale and subsequently the Bundelkhand craton acquired thermal equilibrium of the stable geotherm. The signature of this event is marked by the emplacement of different types of granitoids that are available throughout the craton in time and space (Basu 2010;Mondal et al 2002;Kumar et al 2010). The successive events of granitoid magmatism occurred within a very short span of time in this craton (~50 Ma, Mondal et al 2002).…”
Section: Geological Backgroundmentioning
confidence: 99%
“…The variation in the REE data is in agreement with the concentration of radiogenic elements in different varieties of rocks. The geochemical studies based on redox potentiality (Kumar et al 2010) suggest that grey granitoid is dominated by magnetite series (oxidizing environment), while most of the pink granitoid is related to ilmenite series (reducing environment). The low oxidation (strongly reducing conditions) estimates, high K 2 O and SiO 2 content and high radiogenic elemental abundances suggest the dominance of crustal source materials (pelitic) for fine-grained pink granite compared to that of mantle component for grey granitoid in their genesis.…”
Section: Granitoidsmentioning
confidence: 99%
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“…2.56–2.51 Ga; Jayananda, Peucat, et al, ; Jayananda, Tsutsumi, et al, ). Widespread granitic magmatism in the adjoining Bundelkhand Craton and the Bastar Craton (Meert et al, ) occurred at a similar time frame producing the vast batholithic bodies of the Bundelkhand Granite and the Dongargarh‐Kanker‐Malanjkhand Granites, respectively (Kumar et al, ; Meert et al, ; Mondal, Goswami, Deomurari, & Sharma, ). Thus, the southern and central Indian crustal blocks characterized by amalgamated proto‐continents, mostly formed and stabilized by large‐scale granite magmatism in the end Neoarchaean (ca.…”
Section: Discussionmentioning
confidence: 99%
“…All these lithologies are intruded by NE–SW trending quartz reefs and NW–SE trending dolerite dike swarms during the crustal‐scale shearing (Basu, ; Basu, ; Bhattacharya & Singh, ; Mondal et al, ; Singh, Singh, Srivastava, & Basu, ). Geochronological studies carried out by several workers in the Bundelkhand Craton (Joshi et al, ; Kaur, Zeh, Chaudhri, & Eliyas, ; Kumar, Raju, Pathak, & Pandey, ; Mondal et al, ; Mondal, Sharma, Rahman, & Goswami, ; Saha et al, ; Sarkar, ; Verma, Verma, Oliveira, Singh, & Moreno, ) suggest that accretion of tonalite‐trondhjemite‐granodiorite (TTG) occurred in three phases from 3,500 to 3,200 Ma (Kaur et al, ). Ultramafic–mafic and basalt‐andesite‐rhyolite‐dacite magmatism (plume‐arc type) in the Mauranipur–Babina greenstone belt accreted at approximately 2,700 to 2,545 Ma (Singh et al, ).…”
Section: Geologymentioning
confidence: 99%