Himalayas

Geologic history

   Over the past 65 million years, powerful global plate-tectonic forces have moved the Earth’s crust to form the band of Eurasian mountain ranges—including the Himalayas—that stretch from the Alps to the mountains of Southeast Asia.

    During the Jurassic Period (about 200 to 145 million years ago), a deep crustal downwarp—the Tethys Ocean—bordered the entire southern fringe of Eurasia, then excluding the Arabian Peninsula and the Indian subcontinent. About 180 million years ago, the old supercontinent of Gondwana (or Gondwanaland) began to break up. One of Gondwana’s fragments, the lithospheric plate that included the Indian subcontinent, pursued a northward collision course toward the Eurasian Plate during the ensuing 130 million years. This Indian-Australian Plate gradually confined the Tethys trench within a giant pincer between itself and the Eurasian Plate. As the Tethys trench narrowed, increasing compressive forces bent the layers of rock beneath it and created interlacing faults in its marine sediments. Masses of granites and basalts intruded from the depth of the mantle into this weakened sedimentary crust. About 50 million years ago, the Indian subcontinent finally collided with Eurasia. The plate containing India was sheared downward, or subducted, beneath the Tethys trench at an ever-increasing pitch.

     During the next 30 million years, shallow parts of the Tethys Ocean gradually drained as its sea bottom was pushed up by the plunging Indian-Australian Plate; this formed the Plateau of Tibet. On the plateau’s southern edge, marginal mountains—the Trans-Himalayan ranges of today—became the region’s first major watershed and rose high enough to become a climatic barrier. As heavier rains fell on the steepening southern slopes, the major southern rivers eroded northward toward the headwaters with increasing force along old transverse faults and captured the streams flowing onto the plateau, thus laying the foundation for today’s drainage patterns. To the south the northern reaches of the Arabian Sea and the Bay of Bengal rapidly filled with debris carried down by the ancestral Indus, Ganges (Ganga), and Brahmaputra rivers. The extensive erosion and deposition continue even now as these rivers carry immense quantities of material every day.

     Once the Great Himalayas had risen high enough, they became a climatic barrier: the marginal mountains to the north were deprived of rain and became as parched as the Plateau of Tibet. In contrast, on the wet southern flanks the rivers surged with such erosive energy that they forced the crest line to migrate slowly northward. Simultaneously, the great transverse rivers breaching the Himalayas continued their downcutting in pace with the uplift. Changes in the landscape, however, compelled all but these major rivers to reroute their lower courses because, as the northern crests rose, so also did the southern edge of the extensive nappes. The formations of the Siwalik Series were overthrust and folded, and in between the Lesser Himalayas downwarped to shape the midlands. Now barred from flowing due south, most minor rivers ran east or west through structural weaknesses in the midlands until they could break through the new southern barrier or join a major torrent.

   In some valleys, such as the Vale of Kashmir and the Kathmandu Valley of Nepal, lakes formed temporarily and then filled with Pleistocene deposits. After drying up some 200,000 years ago, the Kathmandu Valley rose at least 650 feet (200 metres), an indication of localized uplift within the Lesser Himalayas.