Downloaded from http://sp.lyellcollection.org/ at Kingston University on January 3, 2020 Introduction to Himalayan tectonics: a modern synthesis MICHAEL P. SEARLE1* & PETER J. TRELOAR2 1Department of Earth Sciences, University of Oxford, Oxford OX1 3AN, UK 2School of the Natural and Built Environment, Kingston University, Penrhyn Road, Kingston-upon-Thames, Surrey KT1 2EE, UK MPS, 0000-0001-6904-6398 *Correspondence:
[email protected] The Himalaya resulted from collision of the Indian widespread migmatization and mid-crustal melting plate with Asia and are well known as the highest, during the Oligocene–Mid-Miocene. The age of the youngest and one of the best studied continental col- abundant leucogranite sills and dykes along the top lision orogenic belts. They are frequently used as the of the GHS, beneath the STD, is concomitant with type example of a continental collision orogenic belt the sillimanite-grade metamorphic event. The GHS in studies of older Phanerozoic orogenic belts. The metamorphism is all part of one continuum of crustal beauty of the Himalaya is that, on a broad scale they thickening and shortening, increasing pressure and form a relatively simple orogenic belt. The major temperature following a standard clockwise Pressure- structural divisions, the Indus–(Yarlung Tsangpo) Temperature-Time (PTt) path. Decompression suture zone, the Tethyan Himalaya sedimentary melting peaked with widespread partial melting and units, Greater Himalaya Sequence (GHS) metamor- formation of migmatites and leucogranites along the phic rocks, the Lesser Himalaya fold-and-thrust highest peaks of the Himalaya. Structural mapping belt and the Sub-Himalaya Siwalik molasse basin and timing constraints suggest the large-scale are present along the entire 2000 km length of the southward extrusion of a partially melted layer of Himalaya (Figs 1 & 2).