1999
DOI: 10.1086/314331
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U‐Pb Ages for Zircon and Titanite from the Ramagiri Area, Southern India: Evidence for Accretionary Origin of the Eastern Dharwar Craton during the Late Archean

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Cited by 149 publications
(78 citation statements)
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“…Combinations of these two end-member models are suggested by a number of workers like [9] that included initial subduction fol- Kolar greenstone belt consists of komatiites, tholeiites, and dacites. Whereas, the Hutti is madeup of tholeiitic basalts, dacites, and rhyolite with rare occurrence of ultramafic rocks [16] [17]. The field observations, Rb-Sr and Sm-Nd isotope studies, geochemical studies are indicating the rocks are classified as basalt, basaltic andesite, andesite, dacite, and rhyolite [17].…”
Section: Geology Of the Dharwar Cratonmentioning
confidence: 99%
“…Combinations of these two end-member models are suggested by a number of workers like [9] that included initial subduction fol- Kolar greenstone belt consists of komatiites, tholeiites, and dacites. Whereas, the Hutti is madeup of tholeiitic basalts, dacites, and rhyolite with rare occurrence of ultramafic rocks [16] [17]. The field observations, Rb-Sr and Sm-Nd isotope studies, geochemical studies are indicating the rocks are classified as basalt, basaltic andesite, andesite, dacite, and rhyolite [17].…”
Section: Geology Of the Dharwar Cratonmentioning
confidence: 99%
“…In the WDC, TTG basement rocks (also known as Peninsular Gneiss) are abundant and accreted mainly during Mesoarchean time (Peucat et al, 1993) with some late Archean (~2.6 Ga) potassic plutons (Taylor et al, 1984;Nutman et al, 1996;Jayananda et al, 2006). The EDC is dominated by late Archean TTG gneisses and calc-alkaline to potassic granitoids (Balakrishnan et al, 1999;Nutman et al, 1996;Jayananda et al, 2000). The greenstone belts in the WDC are thick, widely distributed and dominated by sedimentary sequences compared to the greenstone belts in the EDC.…”
Section: Geological Settingmentioning
confidence: 99%
“…The uniformitarians proposed that the EDC formed as a result of accretion of a series of island arcs (e.g., Balakrishnan et al, 1999;Manikyamba et al, 2005;Naqvi et al, 2006) to the WDC through transpression. Chadwick et al (2000) suggests that the accretion of already formed island arcs and granitic plutons constituted a single landmass (i.e., Dharwar batholith) to the WDC, causing sin- Chardon et al, 2008) showing the locations and ages of Mesoarchean and Neoarchean granitoids referred to in the text.…”
Section: Geological Settingmentioning
confidence: 99%
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