Abstract
The Indus Suture Zone, with many ophiolite occurrences, represents the northern limit of the Tethyan Himalaya. The volcanic rocks of the Dras ophiolite zone exhibit low TiO 2, K 2O, P 2O 5, SiO 2, Pb, Rb, Ba, Sr and Zr concentrations and lower La Yb ratios than the intraplate tholeiites. Intercalation of marine sediments, presence of pillow lavas, low K 2O, low to moderate TiO 2, high MgO, CaO TiO 2 and Al 2O 3 TiO 2 , flat REE patterns with lower La N Sm N ratios and increase of SiO 2, FeO (T) and TiO 2 with the fractionation indicate that they are island-arc tholeiites similar to lavas of late Cretaceous age in Cyprus and Oman. These volcanics are postulated to have been derived from a tholeiitic magma generated by a high degree of partial melting and fractionation of mafic phases prior to the crystallization of plagioclase. The island-arc tholeiitic volcanism, the lack of major CA volcanic activity and the reported blueschist metamorphism of the Indus ophiolites suggest a palaeo-island arc development along the Indus Suture Zone along which the Tethys oceanic crust was consumed.
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