The geology of India is a product of its great age and diverse geologic settings.

Plate Tectonics

The Indian craton was once part of the Supercontinent of Pangaea. At that time, it was attached to Madagascar and southern Africa on the south west coast, and Australia along the east coast. 160 million years ago during the Jurassic Period, rifting caused Pangaea to break apart into two supercontinents: (Gondwana to the south and Laurasia to the north). The Indian craton remained attached to Gondwana, until the supercontinent began to rift apart about in the early Cretaceous, about 125 million years ago. The Indian Plate then drifted northward toward the Eurasian Plate, at a pace that is the fastest movement of any known plate. About 90 million years ago, the Indian plate separated from Madagascar. The Indian Plate began collided with the Eurasian Plate about 50 million years ago. This orogeny, which is continuing today, is related to closure of the Teyths ocean. The closure of this ocean which created the Alps in Europe, and the Caucasus range in western Asia, created Himalaya Mountains and the Tibetan Plateau in South Asia. The current orogenic event is causing parts of the Asian continent to deform westward and eastward on either side of the orogeny. Concurrently with this collision, the Indian Plate sutured on to the adjacent Australian Plate, forming a new larger plate, the Indo-Australian Plate.

The Deccan Traps

During its journey northward after breaking off from the rest of Gondwana, the Indian Plate passed over a geologic hotspot, the Réunion hotspot, which caused extensive melting underneath the Indian craton. The melting broke through the surface of the craton in a massive flood basalt event, creating what is known as the Deccan Traps. It is also thought that the Reunion hotspot caused the separation of Madagascar and India.

Tectonic Evolution

The earliest phase of tectonic evolution was marked by the cooling and solidification of the upper crust of the earth surface in the Archaean era (prior to 2.5 billion years)which is represented by the exposure of gneisses and granites especially on the Peninsula. These form the core of the Indian craton. The Aravali Range is the remanent of an early Proterozoic orogen called the Aravali-Delhi orogen that joined the two older segments that make up the Indian craton. It extends approximately 500 km (310 miles) from its northern end to isolated hills and rocky ridges into Haryana, ending near Delhi.

Minor igneous intrusions, deformation(folding and faulting) and subsequent metamorphism of the Aravali Mountains represent the main phase of orogenesis . The erosion of the mountains, and further deformation of the sediments of the Dharwaian group (Bijawars) marks the second phase. The volcanic activities and intrusions, associated with this second phase are recorded in composition of these sediments.

Early to Late Proterozoic calcareous and arenaceous deposits, which correspond to humid and semi-arid climatic regimes, were deposited the Cuddapah and Vindhyan basins. These basins which border or lie within the existing crystalline basement, were uplifted during the Cambrian (500 million years ago. The sediments are generally undeformed and have in many places preserved their original horizontal stratification. The Vindhyans are believed to have been deposited between ~1700 and 650 million years ago (Ray, J.S., Journal of Earth System Science, February, 2006).

Early Paleozoic rocks are found in the Himalayas and consist of southerly derived sediments eroded from the crystalline craton and deposited on the Indian platform.

In the Late Paleozoic, Permo-Carboniferous glaciations left extensive glacio-fluvial deposits across central India, in new basins created by sag/normal faulting. These tillites and glacially derived sediments are designated the Gondwanas series. The sediments are overlain by rocks resulting from a Permain marine transgression (270 million years ago).

The late Paleozoic coincided with the deformation and drift of the Gondwana supercontinent. To this drift, the uplift of the Vindhyan sediments and the deposition of northern peripheral sediments in the Himalayan Sea, can be attributed.

At the close of the Mesozoic one of the greatest volcanic eruptions in earths history occurred, the Deccan lava flows. Covering more than 500,000 km² area, these mark the final break from Gondwana.

In the early Tertiary, the first phase of the Himalayan orogeny, the Karakoram phase occurred. The Himalayan orogeny has continued to the present day.

Main rock groups

Precambrian

A considerable area of peninsular India consists of Archean gneisses and schists, which are the oldest rocks found in India. The Pre-Cambrian rocks of India have been classified into two systems, namely the Dharwar system and the Archaean system.

The rocks of the Dharwar system are mainly sedimentary in origin, and occur in narrow elongated synclines resting on the gneisses found in Bellary district, Mysore and the Aravalis of Rajputana. These rocks are enriched in Manganese and Iron ore which represents a significant resource of these metals. They are also extensively mineralized with gold most notably the Kolar gold mines located in Mysore. In the north and west of India, the Vaikrita system, which occurs in Hundes, Kumaon and Spiti areas, the Dailing series in Sikkim and the Shillong series in Assam are believed to be of the same age as the Dharwar system.

The metamorphic basement consists of gneisses which are further classified into the Bengal gneiss, the Bundelkhand gneiss and the Nilgiri gneiss. The Nilgiri system comprises of Charnockites ranging from granites to gabbros. Also the earliest possible trace fossils of multicellular life ^{[citation needed]} (apart from 2-billion-year-old tracks from Texas and a multicelluar red alga called Bangomorphia pubecenis which was found in Ectasian (Mesoproterozoic, 1.2 bya) strata).

Palaeozoic

• Lower Paleozoic

Rocks of the earleist Cambrian period are found in the Salt range in Punjab and the Spiti are in central Himalayas and consist of a thick sequence of fossiliferous sediments. In the Salt range, the stratigraphy starts with the Salt Pseudomorph zone, which has a thickness of 450 ft and consists of dolomites and sandstones. It is overlain by magnesian sandstones with a thickness of 250 ft, similar to the underlying dolomites. These sandstones have very few fossils. Overlying the sandstones is the Neobolus Shale, which is composed of dark shales with a thickness of 100 ft. Finally there is a zone consisting of red or purple sandstones having a thickness of 250 to 400 ft called the Purple Sandstone. These are unfossiliferous and show sun-cracks and worm burrows which is typical of subaerial weathering . The deposits in Spiti are known as Haimanta system and they consist of Slates, micaceous quartzite and dolomitic limestones.

The Ordovician rocks comprise flaggy shales, limestones, red quartzites, quartzites, sandstones and conglomerates. Siliceous limestones belonging to the Silurian overlie the Ordovician rocks. These limestones are in turn overlain by white quartzite and this is known as Muth quartzite. Silurian rocks which contain typical Silurian fauna are also found in the Vihi district of Kashmir.

• Upper Paleozoic

Devonian fossils and corals are found in grey limestone in the central Himalayas and in black limestone in the Chitral area.

The Carboniferous is composed of two distinct sequences, the upper carboniferous Po, and the lower carbonferous Lipak. Fossils of Brachiopods and some Trilobites are found in the calcareous and sandy rocks of the Lipak series. The Syringothyris limestone in Kashmir also belongs to the Lipak. The Po series overlays the Lipak series, and the Fenestella shales are interbedded within a sequence of quartzites and dark shales. In many places Carboniferous strata are overlaid by grey agglomeratic slates, believed to be of volcanic origin.

Many genera of Productus are found in the limestones of the Permo - Triassic, which has led to these rocks being referred to as "productus limestone". This limestone is of marine origin and is divided into three distinct litho-stratigraphic units based on the productus chronology. The Late Permian Chideru, which contains many ammonites, the Late - Middle Permain Virgal, and the Middle Permian Amb unit.

Mesozoic

In the Triassic the Ceratite beds, named after the ammonite ceratite, consist of arenaceous limestones, calcerous sandstones and marls.

The Jurassic consists of two distinct units. The Kioto limestone, extends from the lower the middle Jurassic with a thickness 2000 to 3000 ft. The upper Jurassic is represented by the Spiti black shales, and stretches from the Karakoram to Sikkim.

Cretaceous rocks are cover an extensive area in India. In south India, the sedimentary rocks are divided into four stages; the Niniyur , the Ariyalur, the Trichinopoly, and the Utatur stages. In the Utatur stage the rocks host phosphatic nodules, which constitute an important source of phosphates in the country. In the central provinces, the well developed beds of Lameta contain fossil records which are helpful in estimating the age of the Deccan Traps. This sequence of basaltic rocks was formed near the end of the Cretaceous period due to volcanic activity. These lava flows occupy an area of 200,000 square miles. These rocks are a source of high quality building stone and also provide a very fertile clayey loam, particularly suited to cotton cultivation.

Cenozoic

• Tertiary

In this period the Himalayan orogeny began, and the volcanism associated with the Deccan Traps continued. The rocks of this era have valuable deposits of petroleum and coal. Sandstones of Eocene age are found in Punjab, which grade into chalky limestones with oil seepages. Further north the rocks found in the Simla area are divided into three series, the Sabathu series consisting of grey and red shales, the Dagshai series comprising bright red clays and the Kasauli series comprising sandstones. Towards the east in Assam, Nummulitic limestone is found in the Khasi hills. Oil is associated with these rocks of the Oligo-Miocene age. Along the foothills of the Himilayas the Siwalik molasse is composed of sandstones, conglomerates and shales with thicknesses of 16000 to 20000 ft and ranging from Eocene to Pliocene. These rocks are famous for their rich fossil vertebrate fauna including many fossil hominoids.

• Quaternary

The alluvium which is found in the Indo-Gangetic plain belongs to this era. It was eroded from the Himalayas by the rivers and the monsoons. These alluvial deposits consist of clay, loam, silt etc. and are divided into the older alluvium and the newer alluvium. The older alluvium is called Bhangar and is present in the ground above the flood level of the rivers. Khaddar or newer alluvium is confined to the river channels and their flood plains. This region has some of the most fertile soil found in the country as new silt is continually laid down by the rivers every year.

See also

• Indian Plate

Notes

1. ^ "Volcanic push to Barren tourism". Times of India. Retrieved June 8. {{cite web}}: Check date values in: |accessdate= (help); Unknown parameter |accessyear= ignored (|access-date= suggested) (help)