Timing, quantification and tectonic modelling of Pliocene–Quaternary movements in the NW Himalaya: evidence from fission track dating
Introduction
Northern parts of the extensively remobilized Himalayan Metamorphic Belt (HMB) due to continental collision tectonics between the northerly moving Indian Plate and the Eurasian Plate since Early Cenozoic (∼55 Ma) constitute the highest uplifted and fastest eroded terrain of the Himalaya [1], [2], [3], [4], [5]. It has been modelled to have evolved within a 15–20 km thick, northeast-dipping intracontinental ductile shear zone due to intense crustal shortening [3], [6], [7], and has been thrust southwestward over the Lesser Himalayan sedimentary sequence along the Main Central Thrust (MCT) and its various splays, e.g. the Jutogh/Vaikrita thrusts (Fig. 1).
Geochronological data from the NW Himalaya during the past two decades have demonstrated that the Higher Himalayan Crystallines (HHC) have undergone fastest and episodic exhumation during the Cenozoic after the collision tectonics; the main Neo-Himalayan phase (∼25–18 Ma) has caused rapid uplift, tectonic denudation and deposition of colossal molassic sediments in the Sub-Himalayan foreland basin and the maga fans within the Indian Ocean [8]. Another major uplift phase during the Late Pliocene–Quaternary appears to be mainly responsible for the present-day Himalayan relief [9], and links the ongoing crustal deformation of the Himalaya with the Early Cenozoic geodynamics.
Fission track dating of zircon and apatite has recently been applied to numerous geological problems covering low-temperature tectonothermal evolution, and calculation of variable cooling and exhumation rates across numerous fault zones, e.g. Tectonic Median Line [10], the Insubric fault line in Alps [11], the Main Mantle Thrust [12], [13], and many others. However, the application of FT technique to calculate the amount of displacement along such fault zones is limited [14]. The main objective of this paper is to document and interpret accelerated exhumation of the HHC from the FT ages along the Sutlej Valley, Himachal Pradesh as well as to estimate the displacements along the thrust zone, and to provide tectonothermal models for similar phenomena elsewhere in the NW Himalaya.
Section snippets
Geological framework
In the NW Himalayan segment of Himachal Pradesh along the Sutlej–Baspa–Beas Valleys, the outermost and frontal para-autochthonous Lesser Himalayan Krol–Shali Belt of the Proterozoic quartzite–dolomite–slate–volcanic sequence is thrust southwestward and imbricated with the Sub-Himalayan Cenozoic belt of the Punjab re-entrant along the Main Boundary Thrust (Fig. 1) [15], [16]. Overriding the frontal tectonic units, the HMB is thrust southwestward along the Jutogh Thrust as the Jutogh nappe. This
Sample preparation and analytical procedure
Conventional crushing, magnetic and heavy liquid separation techniques were used to recover apatite and zircon fractions from the rock samples. Apatite crop was available in all the samples, while zircons could only be recovered in sufficient quantity from five samples on the hanging wall of the Chaura thrust and one sample from within the Vaikrita Thrust zone. Araldite epoxy was used for fixing the apatite grains at room temperature, while zircon grains were fixed in PFA teflon at 320°C. The
Zeta values
The ages, reported in the present work, were determined by two analysts using two different reactors. Hence, it will be apposite to mention about the zeta values employed to calculate the ages. For the CIRUS reactor, a zeta value of 110.6±1.3 (1 σ) against CN1 glass was determined by A.K. through multiple irradiations of age standards consisting of two apatites (Fish Canyon Tuff and Mt. Dromedery Complex), three zircons (Fish Canyon Tuff, Buluk Member and Mt. Warning Complex) and one sphene
Cooling and exhumation rates
The HHC are characterized by numerous intensely deformed bodies of granite gneiss, which appear to have been emplaced as granitoids like the WGC. U–Pb dates on zircons, extracted from the undeformed portions of this body, are 2066±9 Ma from the lower parts of the hanging wall of MCT and 1866±10 Ma from the main body above the Chaura thrust [21]. This is supported by a 12-point Rb–Sr whole rock isochron age of 1895±64 Ma from the Wangtu body [20]. These ages strongly suggest the involvement of
Tectonic exhumation of the NW Himalaya
Systematic isotopic data from a few segments of the HHC from the NW Himalaya reveal accelerated exhumation pulses after the initial India–Asia collision ∼55 Ma, which has caused regional overthickening of the continental crust, its deformation and regional metamorphism. Tectonically, these appear to be controlled by (i) large-scale domes and/or windows, which have been active either independently or in combination with (ii) major thrusts as well as extensional normal faults, which have caused
Acknowledgements
The present investigations were undertaken as a part of the Thrust Area Programme of the Department of Science and Technology (DST) entitled ‘Evolution of the Metamorphic Belts in Phanerozoic Collision Boundary’. N.L. thanks Gunther Wagner for fruitful discussion during the early stage of this work. Constructive criticism on a version of the paper by Anthony Hurford and three anonymous reviewers, and by Maurice Pagel at various stages substantially improved the manuscript. J.W.H. Schreurs is
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