1991
DOI: 10.1086/629553
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U-Pb Ages of Zircon and Sphene for Two Gneiss Terranes Adjacent to the Kolar Schist Belt, South India: Evidence for Separate Crustal Evolution Histories

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Cited by 120 publications
(69 citation statements)
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“…They are formed on the base of migmatites, granite gneiss and granites ranging in composition from granodiorite to tonalite and intruded younger dolerites. These abundant granitoid rocks are of calc-alkaline nature (Balakrishnan et al 1990;1999;Krogstad et al 1991). Sanukitioids, a high Mg, high Ni granitoids are also present and monoclinic series of amphiboles tremolite, actinolite comprising Ca, Mg and halogens (F, Cl) occur as intrusive with the PGCs.…”
Section: Geology and Hydrogeologymentioning
confidence: 99%
“…They are formed on the base of migmatites, granite gneiss and granites ranging in composition from granodiorite to tonalite and intruded younger dolerites. These abundant granitoid rocks are of calc-alkaline nature (Balakrishnan et al 1990;1999;Krogstad et al 1991). Sanukitioids, a high Mg, high Ni granitoids are also present and monoclinic series of amphiboles tremolite, actinolite comprising Ca, Mg and halogens (F, Cl) occur as intrusive with the PGCs.…”
Section: Geology and Hydrogeologymentioning
confidence: 99%
“…The U-Pb titanite and zircon ages determined on the granitoid rocks of the Kolar belt by Krogstad et al (1989Krogstad et al ( , 1991 and in the Ramagiri areas by Balakrishnan et al (1999), are shown in table 1. In the Kolar area, the Patna granitoid has yielded identical titanite and zircon U-Pb ages of 2552 ± 1 and 2551 ± 2.5 Ma respectively, whereas, in the Dod gneiss the zircon age of 2631 ± 6.5 Ma is about 80 million years older than the titanite U-Pb age of 2551 ± 2 Ma.…”
Section: Kolar Schist Beltmentioning
confidence: 99%
“…Thus Sm-Nd isotope study on titanites, hornblende or biotite crystallized at the same time along with the whole rock can provide meaningful age information. Two samples, a granodiorite and a quartz monzodiorite surrounding Kolar and Ramagiri schist belts respectively, whose ages were precisely determined by U-Pb titanite and zircon geochronology (Krogstad et al 1991;Balakrishnan et al 1999), were chosen for this exercise.…”
Section: Introductionmentioning
confidence: 99%
“…The absence of mafic end-member (that could be the result of magma fractionation hidden at depth) within the TTGs of the study area thus indicates the possibility of fractional crystallization . Thus, to constrain the potential sources of the parent magma of TTGs, different petrogenetic models have been reviewed for both global occurrence (Condie, 1981;Martin,1986;Smithies, 2000;Martin and Moyen, 2002;Smithies et al 2003; as well as for EDC (Balakrishnan and Rajamani, 1987;Krogstad et al 1991Krogstad et al , 1995Jayananda et al 2000Jayananda et al , 2006Moyen et al 2003b). Different possibilities such as (1) reworking of older crust to direct melting of mantle and slab melting at different depths in subduction setting have been tried for the TTGs of the present study.…”
Section: Ttgsmentioning
confidence: 99%
“…Older basement gneisses are present as huge enclaves (within younger TTG gneisses) in the southeastern part of the EDC (Jayananda et al 2000(Jayananda et al , 2003Chardon et al 2002), whereas the younger TTG gneisses occupy vast areas, especially in the northern parts and are accreted during 2.7 -2.55 Ga (Krogstad et al 1991;Peucat et al1993;Jayananda et al 2000Jayananda et al , 2003Chardon et al 2002). The juvenile continental accretion during 2.55-2.51 Ga has led to emplacement of large magmatic bodies like Closepet granite and other related granite intrusions during a tectono-metamorphic event that affected the craton at the close of the Archaean (Peucat et al 1993;Krogstad et al 1991;Jayananda et al 1995Jayananda et al , 2000Chardon et al 2002;Moyen et al 2003a, b). This accretion event was immediately followed by reworking of newly formed crust and granulite event close to 2.51 Ga (Peucat et al 1993;Mahabaleswar et al 1995) that affected the entire Archaean continental crust of the Dharwar craton.…”
Section: Introductionmentioning
confidence: 99%