Indian plate

Template:Short description Template:About Template:Distinguish Template:Infobox tectonic plate

The Indian plate (or India plate) is or was a minor tectonic plate straddling the equator in the Eastern Hemisphere. Originally a part of the ancient continent of Gondwana, the Indian plate broke away from the other fragments of Gondwana Template:Mya and began moving north, carrying Insular India with it.<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> It was once fused with the adjacent Australian plate to form a single Indo-Australian plate, but recent studies suggest that India and Australia may have been separate plates for at least 3 million years.<ref>Template:Cite book</ref> The Indian plate includes most of modern South Asia (the Indian subcontinent) and a portion of the basin under the Indian Ocean, including parts of South China, western Indonesia,<ref>Sinvhal, Understanding Earthquake Disasters, p. 52, Tata McGraw-Hill Education, 2010, Template:ISBN</ref><ref>Template:Cite journal</ref> and extending up to but not including Ladakh, Kohistan, and Balochistan in Pakistan.<ref>M. Asif Khan, Tectonics of the Nanga Parbat syntaxis and the Western Himalaya, p. 375, Geological Society of London, 2000, Template:ISBN</ref><ref>Srikrishna Prapnnachari, Concepts in Frame Design, page 152, Srikrishna Prapnnachari, Template:ISBN</ref><ref>A.M. Celâl Şengör (1989). Tectonic evolution of the Tethyan Region, Springer Template:ISBN</ref>

Plate movementsEdit

File:Himalaya-formation.gif

Due to plate tectonics, Insular India, situated over the Indian plate, split from Madagascar and collided (c. 55 Mya) with the Eurasian plate, resulting in the formation of the Himalayas.

Until roughly Template:Mya, the Indian plate formed part of the supercontinent, Gondwana, together with modern Africa, Australia, Antarctica, and South America. Gondwana fragmented as these continents drifted apart at different velocities;<ref name="second">Template:Harvnb</ref> a process which led to the opening of the Indian Ocean.<ref name="Kumar-etal">Template:Harvnb</ref>

In the late Cretaceous approximately Template:Mya, and subsequent to the splitting from Gondwana of conjoined Madagascar and India, the Indian plate split from Madagascar and formed Insular India. It began moving north, at about Template:Cvt per year,<ref name="second" /> and is believed to have begun colliding with Asia as early as Template:Mya,<ref name="Scotese">Template:Harvnb</ref> in the Eocene epoch of the Cenozoic. However, some authors suggest the collision between India and Eurasia occurred much later, around Template:Mya.<ref name="fast">Template:Harvnb</ref> If the collision occurred between 55 and 50 Mya, the Indian plate would have covered a distance of Template:Cvt, moving more quickly than any other known plate. In 2012, paleomagnetic data from the Greater Himalaya was used to propose two collisions to reconcile the discrepancy between the amount of crustal shortening in the Himalaya (~Template:Cvt) and the amount of convergence between India and Asia (~Template:Cvt).<ref>Template:Cite journal</ref> These authors propose a continental fragment of northern Gondwana rifted from India, traveled northward, and initiated the "soft collision" between the Greater Himalaya and Asia at ~50 Mya. This was followed by the "hard collision" between India and Asia occurred at ~25 Mya. Subduction of the resulting ocean basin that formed between the Greater Himalayan fragment and India explains the apparent discrepancy between the crustal shortening estimates in the Himalaya and paleomagnetic data from India and Asia. However, the proposed ocean basin was not constrained by paleomagnetic data from the key time interval of ~120 Mya to ~60 Mya. New paleomagnetic results of this critical time interval from southern Tibet do not support this Greater Indian Ocean basin hypothesis and the associated dual collision model.<ref>Template:Cite journal</ref>

In 2007, German geologists<ref name="second" /> suggested the reason the Indian plate moved so quickly is that it is only half as thick (Template:Cvt) as the other plates<ref>The lithospheric roots in South Africa, Australia, and Antarctica are Template:Cvt thick. (Template:Harvnb) See also Template:Harvnb</ref> which formerly constituted Gondwana. The mantle plume that once broke up Gondwana might also have melted the lower part of the Indian subcontinent, which allowed it to move both more quickly and farther than the other parts.<ref name="second" /> The remains of this plume today form the Marion hotspot (Prince Edward Islands), the Kerguelen hotspot, and the Réunion hotspots.<ref name="Kumar-etal" /><ref name="Gondwana Research, vol 10 3-4">Template:Cite journal</ref> As India moved north, it is possible the thickness of the Indian plate degenerated further as it passed over the hotspots and magmatic extrusions associated with the Deccan and Rajmahal Traps.<ref name="Kumar-etal" /> The massive amounts of volcanic gases released during the passage of the Indian plate over the hotspots have been theorised to have played a role in the Cretaceous–Paleogene extinction event, generally held to be due to a large asteroid impact.<ref name="schulte">Template:Cite journal</ref>

In 2020, however, geologists at the University of Oxford and the Alfred Wegener Institute found that new plate-motion models displayed increased movement speeds in all mid-ocean ridges during the late Cretaceous, a result irreconcilable to current theories of plate tectonics and a refutation of the plume-push hypothesis. Pérez-Díaz concludes that the accelerated movement of the Indian plate is an illusion wrought by large errors in geomagnetic reversal timing around the Cretaceous–Paleogene boundary, and that a recalibration of the time scale shows no such acceleration exists.<ref>Template:Cite journal</ref><ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref>

The collision with the Eurasian plate along the boundary between India and Nepal formed the orogenic belt that created the Tibetan Plateau and the Himalaya Mountains, as sediment bunched up like earth before a plow.

The Indian plate is currently moving north-east at Template:Cvt per year, while the Eurasian plate is moving north at only Template:Cvt per year. This is causing the Eurasian plate to deform, and the Indian plate to compress at a rate of Template:Cvt per year.Template:Citation needed