1994
DOI: 10.1016/0301-9268(94)90071-x
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RbSr ages of Late Archean metavolcanics and granites, Dharwar craton, South India and evidence for Early Proterozoic thermotectonic event(s)—reply

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Cited by 10 publications
(7 citation statements)
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“…More recently, Ishwar Kumar et al (2013) have reported U-Pb SHRIMP ages of ∼2.57 Ga for quartzo-feldspathic gneisses from the Dharwar block. Similar ages (2.6-2.5 Ga, CHIME-monazite) were obtained by Rekha et al (2013) Pb whole-rock isochron age of 2565 5 28 Ma (Taylor et al 1984) and an Rb-Sr isochron age of 2520 5 62 Ma (Bhaskar Rao et al 1992 Pb whole-rock isochron age of 2605 5 18 Ma (Taylor et al 1984) and a U-Pb zircon age of 2614 5 10 Ma (Jayananda et al 2006). Felsic volcanism and granitic intrusion in the Gadag greenstone belt has been dated at 2588 5 10 and 2570 5 10 Ma, respectively (U-Pb zircon; Sarma et al 2011).…”
Section: Discussionsupporting
confidence: 50%
“…More recently, Ishwar Kumar et al (2013) have reported U-Pb SHRIMP ages of ∼2.57 Ga for quartzo-feldspathic gneisses from the Dharwar block. Similar ages (2.6-2.5 Ga, CHIME-monazite) were obtained by Rekha et al (2013) Pb whole-rock isochron age of 2565 5 28 Ma (Taylor et al 1984) and an Rb-Sr isochron age of 2520 5 62 Ma (Bhaskar Rao et al 1992 Pb whole-rock isochron age of 2605 5 18 Ma (Taylor et al 1984) and a U-Pb zircon age of 2614 5 10 Ma (Jayananda et al 2006). Felsic volcanism and granitic intrusion in the Gadag greenstone belt has been dated at 2588 5 10 and 2570 5 10 Ma, respectively (U-Pb zircon; Sarma et al 2011).…”
Section: Discussionsupporting
confidence: 50%
“…Based on the tectono‐thermal and magmatic history, crustal thickness, structure and age, the Dharwar Craton has been divided into the WDC and the Eastern Dharwar Craton (EDC) (Bhaskar Rao et al, 1992; Chardon & Jayananda, 2008; Gupta et al, 2003; Sundar Raju et al, 2014; Swami Nath et al, 1976), while Naha et al (1986, 1990), based on structural similarity negate suturing of the EDC and WDC. Maibam et al (2017) and Singh et al (2021) also arrived at similar inferences based on geochronological data.…”
Section: Geological Backgroundmentioning
confidence: 99%
“…Subsequently, these rocks were metamorphosed and intruded by acidic magmas around 3.13–2.96 Ga, which formed the protoliths of the Peninsular Gneiss Complex (PGC) (Peucat et al, 1993; Ramakrishnan & Swaminatha, 1976). The PGC is a polyphase gneiss complex that was formed by dynamo‐thermal metamorphism of the older pre‐Dharwar sedimentary‐volcanic sequence and partial melting of mafic crust (Bhaskar Rao et al, 1992; Gupta et al, 2003; Jayananda et al, 2015, 2018; Maibam et al, 2011, 2016). Formation of the PGC and its stabilization lasted for almost 0.5 billion years, beginning with polyphase gneisses and emplacement of tonalite‐trondhjemite‐granodiorite (TTG) suites and ending with late‐stage voluminous granite plutons from 3.2 to 2.5 Ga (Chadwick et al, 1981; Corfu & Hegde, 2020; Jayananda et al, 2015; Figure 1b).…”
Section: Geological Backgroundmentioning
confidence: 99%
“…The WDC comprises TTG-type gneisses and greenstone belts, which are separated into the older Sargur Group and the younger Dharwar Supergroup (Chadwick et al, 2000;Jayananda et al, 2006, 2015, andreferences therein). The Peninsular Gneisses (TTG) resulted from accretion in several stages between 3.36 and 3.2 Ga (Meen et al, 1992;Bhaskar Rao et al, 1992;Peucat et al, 1993;Jayananda et al, 2015Jayananda et al, , 2018Santosh et al, 2015). The Sargur Group greenstone belt comprises predominantly komatiite and basalt, constrained by a Sm-Nd whole rock isochron age of 3352 ± 110 Ma (Jayananda et al, 2008), while a more precise U-Pb zircon age of 3298 ± 7 Ma has been obtained on the subordinate felsic volcanic rocks (Peucat et al, 1995).…”
Section: Geological Outline Of the Dharwar Cratonmentioning
confidence: 99%