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306   CHAPTER 10



           strong (Fig. 10.12e), the foreland displays a simple shear   The Himalayan–Tibetan orogen (Fig. 10.13) is one
           thin-skinned mode of deformation. Underthrusting of   of the best places to study a large-scale continent–
           the shield is accompanied by the eastward propagation   continent collision that followed the closure of a major
           of the thin-skinned thrust belt above a shallow décolle-  ocean basin and formed an orogenic plateau. The active
           ment at 8–14 km depth and drives deformation in the   tectonics, diverse structure, and relatively well-known
           lower crust beneath the plateau. This style conforms   plate boundary history of this belt allow many tectonic
           well to observations east of the Altiplano and north of   relationships to be measured directly and provide
           23°S. It also simulates the conditions of the Himalayan   important constraints on the driving mechanisms of
           fold-thrust belt south of the Tibetan Plateau (Section   deformation and the manner in which deformation is
           10.4.4). In the case where the Paleozoic sediments are   accommodated (Yin & Harrison, 2000). In addition,
           weak and the foreland warm and weak (Fig. 10.12c),   the immense size and high elevations of this orogen
           deformation in the foreland is thick-skinned with a deep   illustrate how mountain building and global climate
           décollement at ∼25 km depth (Fig. 10.12f). This latter   are interrelated. These interactions form important
           style conforms well to observations east of the Puna   elements of orogenesis in most, if not all, tectonic
           and south of 23°S and results because the foreland is   settings.
           weak enough to deform by buckling.             This section provides a discussion of four main
             These observations and experiments illustrate that   aspects of the Himalayan–Tibetan orogen: (i) the rela-
           variations in lithospheric strength and rheology play an   tive motion of Indian and Eurasia and their tectonic
           important role in controlling the tectonic evolution of   history prior to collision; (ii) the nature of post-colli-
           compressional basins and fold-thrust belts. These effects   sional convergent deformation as revealed by seismicity
           are prominent at scales ranging from individual thrust   and geodetic data; (iii) the geologic history of the Hima-
           sheets to the entire lithosphere.            laya and the Tibetan Plateau; and (iv) the deep structure
                                                        of the orogen. Section 10.4.6 provides a discussion of
                                                        the main factors controlling the mechanical evolution
                                                        of the orogen.
           10.4 CONTINENT–
           CONTINENT                                    10.4.2 Relative plate motions

           COLLISION                                    and collisional history


                                                        The Himalayan–Tibetan orogen was created mainly by
                                                        the collision between India and Eurasia over the past
           10.4.1 Introduction                          70–50 Myr (Yin & Harrison, 2000). The orogen is part
                                                        of the greater Himalayan–Alpine system, which extends
           Collisional mountain ranges form some of the most   from the Mediterranean Sea in the west to the Sumatra
           spectacular and dominant features on the surface of the   arc of Indonesia in the east over a distance of >7000 km.
           Earth. Examples include the Himalayan–Tibetan   This composite belt has evolved since the Paleozoic as
           orogen, the Appalachians, the Caledonides, the Euro-  the Tethyan oceans (e.g. Fig. 11.27) closed between two
           pean Alps, the Urals (Section 11.5.5), the Southern Alps   great converging landmasses: Laurasia in the north and
           of New Zealand (Sections 8.3.3, 8.6.3), and many of the   Gondwana in the south (Sengör & Natal’in, 1996).
                                                                             S
           Proterozoic orogens (e.g. Section 11.4.3). The anatomy   Tethys may have been only a few hundred kilometers
           of these belts is highly diverse, in part due to differences   wide in the west but opened to the east to form an
           in the size, shape, and mechanical strength of the col-  ocean that was at least several thousands of kilometers
           liding plates, and the effects of different precollisional   wide.
           tectonic histories. In addition, continental collision can   The India–Eurasia collision was brought about by
           range from being highly oblique, such as occurs on the   the rifting of India from Africa and East Antarctica
           South Island of New Zealand, to nearly orthogonal.   during the Mesozoic (Section 11.5.5) and by its migra-
           These differences greatly influence the mechanisms of   tion northward as the intervening oceanic lithosphere

           collisional orogenesis (Section 10.4.6).     was subducted beneath the Eurasian Plate. Magnetic
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