1993
DOI: 10.1016/0301-9268(93)90097-l
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Early Archean crust in Bastar Craton, Central India—a geochemical and isotopic study

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Cited by 181 publications
(60 citation statements)
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“…1). The Archean crust was consolidated by 2.5 Ga (Sarkar et al 1993;Chadwick et al 2000;Kovach et al 2001), whereas Nd-model ages from different lithologies of the Eastern Ghats Province imply that its crust formed in Proterozoic time . Lithological similarities (Katz 1989), a similar crustal evolution (Mezger and Cosca 1999;Rickers et al 2001), and combined tectonic and petrologic studies at the contact with the Bhandara craton (Gupta et al 2000) strongly suggest that the Eastern Ghats Province and East Antarctica formed one crustal terrane that collided with proto-India during the global Grenvillian orogeny (Mezger and Cosca 1999;Gupta et al 2000).…”
Section: Geological Settingmentioning
confidence: 98%
“…1). The Archean crust was consolidated by 2.5 Ga (Sarkar et al 1993;Chadwick et al 2000;Kovach et al 2001), whereas Nd-model ages from different lithologies of the Eastern Ghats Province imply that its crust formed in Proterozoic time . Lithological similarities (Katz 1989), a similar crustal evolution (Mezger and Cosca 1999;Rickers et al 2001), and combined tectonic and petrologic studies at the contact with the Bhandara craton (Gupta et al 2000) strongly suggest that the Eastern Ghats Province and East Antarctica formed one crustal terrane that collided with proto-India during the global Grenvillian orogeny (Mezger and Cosca 1999;Gupta et al 2000).…”
Section: Geological Settingmentioning
confidence: 98%
“…The EGMB is juxtaposed against the Archean cratons, namely the Dharwar, Bhandara-Bastar and Singhbhum Cratons (Figure 1b), which are dominantly comprised of tonalite-trondhjemite gneisses (circa 3.5 Ga) and greenstone belts. Several K-rich granite plutons [circa 2.5 Ga, Sarkar et al, 1993], and dolerite, rhyolite and trachyte dykes [circa 1.4 Ga, Mallikarjuna Rao et al, 1995;Nanda et al, 1998] have intruded the cratons during different geological periods. The cratons are unconformably overlain by the platform sequences of rocks known as the Purana Group [> circa 1.1 Ga; Chatterjee et al, 1995], in several sedimentary basins (Chhatishgarh, Khariar and Cuddapah) surrounding the EGMB front (Figure 1c).…”
Section: Lithologymentioning
confidence: 99%
“…None of the other mafic dykes have been radiometrically dated. However, on the basis of field relationships, the ages of granitoid rocks, and stratigraphic relationship between different rock units (Ramakrishnan, 1990;Sarkar et al, 1993;Srivastava et al, 1996;Singh, 2003b, 2004;Srivastava, 2006a), their approximate emplacement ages may be inferred. It is proposed that the BD1 swarm was emplaced in the Mesoarchaean and BD2 swarm in the Paleoproterozoic (1.88 Ga).…”
Section: Geological Settingmentioning
confidence: 99%