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SPAZIO CLIL The Alpine-Himalayan Orogeny EUROPE T ASIA Alps Caucasus Tien Shan Atlas AFRICA Tibetan plateau Zagros Himalayas Saudi Arabia China India Figure 1 The Alpine-Himalayan belt showing the chains of high mountains built by the ongoing collision of the African, Arabian, and Indian plates with the Eurasian Plate. 60 Ma Indian plate Eurasian plate (Tibet) The Indian Plate moved northward, carrying the Indian subcontinent. As it subducted under the Eurasian Plate, an accretionary wedge accumulated from the sediments and oceanic crust scraped off the descending plate. Rising magma from the descending plate thickened the Eurasian Plate crust. Oceanic crust Continental crust 30÷50 Ma The Indian subcontinent collided with Tibet, but India was too buoyant to be subducted into the mantle, so India broke along the Main Central Thrust fault. Main central trust Eroded uplifted material 20÷30 Ma As the collision continued, the motion was taken up along the thrust fault, and a slice of Indian crust and shelf sediments stacked onto the oncoming subcontinent. 10÷20 Ma A second thrust fault, the Main Boundary Fault, developed, stacking a second slice of crust onto India and lifting the first slice. Thus two overthrust slices make up the bulk of the Himalayas. Main boundary fault Main central trust Ganges plain Himalayas Tibetan Plateau Main boundary fault Main central trust Figure 2 Cross sections showing the sequence of events that have caused the Himalayan orogeny, simplified and vertically exaggerated. (After P. Molnar, The Structure of Mountain Ranges. Scientific American, July 1986, p. 70) Fantini, Monesi, Piazzini - Elementi o see orogeny in action, we look to the great chains of high mountains that stretch from Europe through the Middle East and across Asia, known collectively as the Alpine-Himalayan belt (see figure 1) The breakup of the ancient supercontinent Pangaea sent the continental crust of Africa, Arabia, and India northward, causing the ancient Tethys Ocean to close as its lithosphere was subducted beneath Eurasia. These former pieces of Gondwanaland (the southern part of Pangaea) collided with Eurasia in a complex se quence, beginning in the western part of Eurasia during the Cretaceous period and continuing eastward through the Cenozoic, raising the Alps in central Europe, the Caucasus and Zagros mountains in the Middle East, and the Himalayas and other high mountain chains across central Asia. The Himalayas, the world’s highest mountains, are the most spectacular result of this modern episode of continent-continent collision. About 50 million years ago, the Indian subcontinent, riding on the subducting Indian Plate, first encountered the island arcs and continental volcanic belts that then bounded the Eurasian Plate (see figure 2). As the landmasses of India and Eurasia merged, the Tethys Ocean disappeared through subduction. Pieces of the oceanic crust were trapped along the suture zone between the converging continents and can be seen today as ophiolites along the Indus and Tsangpo river valleys that separate the high Himalayas from Tibet. The collision slowed India’s advance, but the plate continued to drive northward. So far, India has penetrated over 2 000 km into Eurasia, causing the largest and most intense orogeny of the Cenozoic era. The Himalayas were formed from overthrust slices of the old northern portion of India, stacked one atop the other. This process took up some of the compression. Horizontal compression also thickened the crust north of India, causing uplift of the huge Tibetan Plateau, which now has a crustal thickness of 60 to 70 km (almost twice the thickness of normal continental crust) and stands nearly 5 km above sea level. These and other zones of compression account for perhaps half of India’s penetration into Eurasia. The other half has been accommodated by pushing China and Mongolia eastward, out of India’s way, like toothpaste squeezed from a tube. The mountains, plateaus, faults, and great earthquakes of Asia, thousands of kilometers from the Indian-Eurasian suture, are thus affected by the Himalayan orogeny, which continues as India ploughs into Asia at a rate of 40 to 50 mm/year. di Scienze della Terra • Italo Bovolenta editore - 2013 1