2000
DOI: 10.1144/gsl.sp.2000.170.01.01
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Tectonics of the Nanga Parbat syntaxis and the western Himalaya: an introduction

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Cited by 16 publications
(12 citation statements)
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“…Concerning the two domains evidenced at a regional scale and separated by the Raikhot fault, the different observed stress patterns probably reflect two different stages of the tectonic activity, of different ages. East of the Raikhot fault, most of the Nanga Parbat pop‐up anticline was in the ductile deformation field up to recently, as indicated by 4 to 11 Ma monazite U/Pb ages obtained on the high‐grade migmatitic gneisses [ Smith et al , 1992], 1 to 5 Ma Ar/Ar cooling ages of biotite obtained in these gneisses [ Treloar et al , 2000; Schneider et al , 2001], the intrusion of granites as young as 1 Ma [ Zeitler at al. , 1993], and the shallow (5–6 km) present‐day brittle‐ductile transition as revealed by seismic investigations [ Meltzer et al , 2001].…”
Section: Discussionmentioning
confidence: 99%
“…Concerning the two domains evidenced at a regional scale and separated by the Raikhot fault, the different observed stress patterns probably reflect two different stages of the tectonic activity, of different ages. East of the Raikhot fault, most of the Nanga Parbat pop‐up anticline was in the ductile deformation field up to recently, as indicated by 4 to 11 Ma monazite U/Pb ages obtained on the high‐grade migmatitic gneisses [ Smith et al , 1992], 1 to 5 Ma Ar/Ar cooling ages of biotite obtained in these gneisses [ Treloar et al , 2000; Schneider et al , 2001], the intrusion of granites as young as 1 Ma [ Zeitler at al. , 1993], and the shallow (5–6 km) present‐day brittle‐ductile transition as revealed by seismic investigations [ Meltzer et al , 2001].…”
Section: Discussionmentioning
confidence: 99%
“…There is a rapid drop to “background levels” after circa 470 Ma, falling further to zero by circa 1100 Ma, and a small cluster of ages at circa 1600 Ma (Figure 3a). Ar loss in older grains precludes accurate provenance analysis, but ages are consistent with known tectonothermal events affecting rocks of the Indian plate, including a Pre‐Cambrian metamorphic event, Cambro‐Ordovician and Carboniferous plutonism possibly associated with Pan‐African orogenesis and Neo‐Tethyan rifting, and Jurassic and Early Cretaceous thermal events [ Treloar et al , 1989b; Treloar and Rex , 1990; Gaetani and Garzanti , 1991; Smith et al , 1994; Garzanti et al , 1999; Treloar et al , 2000] (see section 2.2). Some contribution from the Kohistan arc might also be expected.…”
Section: Balakot Formationmentioning
confidence: 75%
“…In the footwall of the MMT, many of the Indian plate rocks attest to a polymetamorphic and deformational pre‐Himalayan history. Granulite facies metamorphism and migmatisation affected the Indian plate basement gneisses at circa 1850 Ma [ Treloar et al , 2000], reflected in the cooling ages of a variety of minerals [ Chamberlain et al , 1989; Zeitler et al , 1989; Treloar et al , 1989b; Treloar and Rex , 1990; Schneider et al , 1999] A mafic dyke intrusion event crosscuts the metamorphic fabric at circa 1600 Ma [ Treloar et al , 2000]. Dating of a series of granitoids suggests a period of magmatism, probably related to the Pan‐African orogeny, in the Cambro‐Ordovician, circa 400–500 Ma, with a cluster of ages at circa 470 Ma [ Le Fort et al , 1979; Zeitler et al , 1989; Chamberlain et al , 1989; Treloar et al , 1991, 2000; Foster et al , 1999; Lombardo et al , 2000].…”
Section: Geological Background Of the Himalayamentioning
confidence: 99%
“…Rapidly evolving terranes and tectonic systems often yield a small range of ages for mineral geochronometers that have very different closure temperatures, including polygenetic Th-and U-bearing accessory minerals formed at or close to peak metamorphic conditions (e.g., Dallmeyer et al, 1986;Dokka et al, 1986;Goodwin and Renne, 1991;Baldwin et al, 1993Baldwin et al, , 2004Brown and Dallmeyer, 1996;Platt et al, 1998;Treloar et al, 2000;Di Vincenzo and Palmeri, 2001;Zeitler et al, 2001;de Jong, 2003;Štípská et al, 2004;Çelik et al, 2006;Schulmann et al, 2008;Pitra et al, 2010;Wilke et al, 2010;Charles et al, 2012;Cubley et al, 2013a,b;Daoudene et al, 2013). Tectonically exhumed terranes generally experienced rapid cooling, whereas exhumation by erosion record slow cooling (e.g., Dallmeyer et al, 1986;Dokka et al, 1986;Baldwin et al, 1993Baldwin et al, , 2004Brown and Dallmeyer, 1996;Platt et al, 1998;Charles et al, 2012;Cubley et al, 2013a,b;Daoudene et al, 2013;Scibiorski et al, 2015), unless erosion was forced by extreme exhumation and became the driving force, as exemplified by the eastern and western Himalayan syntaxes (e.g., Treloar et al, 2000;Zeitler et al, 2001).…”
Section: Tectonically-induced Coolingmentioning
confidence: 99%