![Indian plate](https://www.english.nina.az/wikipedia/image/aHR0cHM6Ly91cGxvYWQud2lraW1lZGlhLm9yZy93aWtpcGVkaWEvY29tbW9ucy90aHVtYi9iL2JiL0luZGlhblBsYXRlLnBuZy8xNjAwcHgtSW5kaWFuUGxhdGUucG5n.png )
The Indian plate (or India plate) is 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 100 million years ago and began moving north, carrying Insular India with it. It was once fused with the adjacent Australian plate to form a single Indo-Australian plate; recent studies suggest that India and Australia have been separate plates for at least 3 million years. 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, and extending up to but not including Ladakh, Kohistan, and Balochistan in Pakistan.
Indian plate | |
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Type | Minor |
Approximate area | 11,900,000 km2 (4,600,000 sq mi) |
Movement1 | North-east |
Speed1 | 26–36 mm/a (1.0–1.4 in/year)[citation needed] |
Features | Indian subcontinent, Indian Ocean, Arabian Sea, Himalayas |
1Relative to the African plate |
Plate movements
![image](https://www.english.nina.az/wikipedia/image/aHR0cHM6Ly93d3cuZW5nbGlzaC5uaW5hLmF6L3dpa2lwZWRpYS9pbWFnZS9hSFIwY0hNNkx5OTFjR3h2WVdRdWQybHJhVzFsWkdsaExtOXlaeTkzYVd0cGNHVmthV0V2WTI5dGJXOXVjeTkwYUhWdFlpOHlMekptTDBocGJXRnNZWGxoTFdadmNtMWhkR2x2Ymk1bmFXWXZNVGN3Y0hndFNHbHRZV3hoZVdFdFptOXliV0YwYVc5dUxtZHBaZz09LmdpZg==.gif)
Until roughly 140 million years ago, 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; a process which led to the opening of the Indian Ocean.
In the late Cretaceous approximately 100 million years ago, 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 20 cm (7.9 in) per year, and is believed to have begun colliding with Asia as early as 55 million years ago, in the Eocene epoch of the Cenozoic. However, some authors suggest the collision between India and Eurasia occurred much later, around 35 million years ago. If the collision occurred between 55 and 50 Mya, the Indian plate would have covered a distance of 3,000 to 2,000 km (1,900–1,200 mi), 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 (~1,300 km or 800 mi) and the amount of convergence between India and Asia (~3,600 km or 2,200 mi). 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.
In 2007, German geologists suggested the reason the Indian plate moved so quickly is that it is only half as thick (100 km or 62 mi) as the other plates 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. The remains of this plume today form the (Prince Edward Islands), the Kerguelen hotspot, and the Réunion hotspots. 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. 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.
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.
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 five cm (2.0 in) per year, while the Eurasian plate is moving north at only two cm (0.79 in) per year. This is causing the Eurasian plate to deform, and the Indian plate to compress at a rate of four mm (0.16 in) per year.[citation needed]
Geography
The westerly side of the Indian plate is a transform boundary with the Arabian plate called the Owen fracture zone, and a divergent boundary with the African plate called the Central Indian Ridge (CIR). The northerly side of the plate is a convergent boundary with the Eurasian plate forming the Himalaya and Hindu Kush mountains, called the Main Himalayan Thrust.[citation needed]
See also
- Historical geology
- List of tectonic plate interactions
- List of tectonic plates
- Palaeogeography
- Seychelles microcontinent
Notes
- "Sizes of Tectonic or Lithospheric Plates". Geology.about.com. 2014-03-05. Archived from the original on 2016-06-05. Retrieved 2016-01-13.
- Oskin, Becky (2013-07-05). "New Look at Gondwana's Breakup". Livescience.com. Retrieved 2016-01-13.
- Stein, Seth; Sella, Giovanni F.; Okai, Emile A. (2002). "The January 26, 2001 Bhuj Earthquake and the Diffuse Western Boundary of the Indian Plate". Plate Boundary Zones (PDF). Geodynamics Series. American Geophysical Union. pp. 243–254. doi:10.1029/GD030p0243. ISBN 9781118670446. Retrieved 2015-12-25.
- Sinvhal, Understanding Earthquake Disasters, p. 52, Tata McGraw-Hill Education, 2010, ISBN 978-0-07-014456-9
- Kumar, M. Ravi; Bhatia, S. C. (1999). "A new seismic hazard map for the Indian plate region under the global seismic hazard assessment programme". Current Science. 77 (3): 447. JSTOR 24102967.
- M. Asif Khan, Tectonics of the Nanga Parbat syntaxis and the Western Himalaya, p. 375, Geological Society of London, 2000, ISBN 978-1-86239-061-4
- Srikrishna Prapnnachari, Concepts in Frame Design, page 152, Srikrishna Prapnnachari, ISBN 978-99929-52-21-4
- A.M. Celâl Şengör (1989). Tectonic evolution of the Tethyan Region, Springer ISBN 978-0-7923-0067-0
- Kind 2007
- Kumar et al. 2007
- Scotese 2001
- Aitchison, Ali & Davis 2007
- van Hinsbergen, D.; Lippert, P.; Dupont-Nivet, G.; McQuarrie, N.; Doubrivine, P.; Spakman, W.; Torsvik, T. (2012). "Greater India Basin hypothesis and a two-stage Cenozoic collision between India and Asia". Proceedings of the National Academy of Sciences. 109 (20): 7659–7664. Bibcode:2012PNAS..109.7659V. doi:10.1073/pnas.1117262109. PMC 3356651. PMID 22547792.
- Qin, Shi-Xin; Li, Yong-Xiang; Li, Xiang-Hui; Xu, Bo; Luo, Hui (2019-01-17). "Paleomagnetic results of Cretaceous cherts from Zhongba, southern Tibet: New constraints on the India-Asia collision". Journal of Asian Earth Sciences. 173: 42–53. Bibcode:2019JAESc.173...42Q. doi:10.1016/j.jseaes.2019.01.012. ISSN 1367-9120. S2CID 134469511.
- The lithospheric roots in South Africa, Australia, and Antarctica are 300 to 180 km (190 to 110 mi) thick. (Kumar et al. 2007) See also Kumar et al. 2007, figure 1
- Meert, J.G.; Tamrat, Endale (2006). "Paleomagnetic evidence for a stationary Marion hotspot: Additional paleomagnetic data from Madagascar". Gondwana Research. 10 (3–4): 340–348. Bibcode:2006GondR..10..340M. doi:10.1016/j.gr.2006.04.008.
- Schulte, Peter; et al. (5 March 2010). "The Chicxulub Asteroid Impact and Mass Extinction at the Cretaceous-Paleogene Boundary" (PDF). Science. 327 (5970). AAAS: 1214–1218. Bibcode:2010Sci...327.1214S. doi:10.1126/science.1177265. ISSN 1095-9203. PMID 20203042. S2CID 2659741.
- Pérez-Díaz, L.; Eagles, G.; Sigloch, K. (2020). "Indo-Atlantic plate accelerations around the Cretaceous-Paleogene boundary: A time-scale error, not a plume-push signal". Geology. 48 (12): 1169–1173. Bibcode:2020Geo....48.1169P. doi:10.1130/G47859.1.
- Andrews, Robin George (14 April 2021). "The New Historian of the Smash That Made the Himalayas". Quanta Magazine. Retrieved 15 April 2021.
References
- Aitchison, Jonathan C.; Ali, Jason R.; Davis, Aileen M. (2007). "When and where did India and Asia collide?". Journal of Geophysical Research. 112 (B5): B05423. Bibcode:2007JGRB..112.5423A. CiteSeerX 10.1.1.1008.2522. doi:10.1029/2006JB004706. hdl:10722/72794. ISSN 0148-0227. Retrieved January 12, 2016.
- Chen, Ji (January 4, 2005). "Magnitude 9.0 off W coast of northern Sumatra Sunday, December 26, 2004 at 00:58:49 UTC: Preliminary rupture model". United States Geological Survey. Archived from the original on March 5, 2005. Retrieved 28 December 2004.
- Kind, Rainer (17 October 2007). "The fastest continent: India's truncated lithospheric roots" (Press release). Helmholtz Association of German Research Centres. Retrieved 2 October 2019.
- Kumar, Prakash; Yuan, Xiaohui; Kumar, M. Ravi; Kind, Rainer; Li, Xueqing; Chadha, R. K. (18 October 2007). "The rapid drift of the Indian tectonic plate". Nature. 449 (7164): 894–897. Bibcode:2007Natur.449..894K. doi:10.1038/nature06214. ISSN 0028-0836. PMID 17943128. S2CID 4339656.
- Scotese, Christopher R. (January 2001). "The collision of India and Asia (90 mya – present)". Paleomap Project. Retrieved 28 December 2004.
External links
Media related to Indian tectonic plate at Wikimedia Commons
The Indian plate or India plate is 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 100 million years ago and began moving north carrying Insular India with it It was once fused with the adjacent Australian plate to form a single Indo Australian plate recent studies suggest that India and Australia have been separate plates for at least 3 million years 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 and extending up to but not including Ladakh Kohistan and Balochistan in Pakistan Indian plateTypeMinorApproximate area11 900 000 km2 4 600 000 sq mi Movement1North eastSpeed126 36 mm a 1 0 1 4 in year citation needed FeaturesIndian subcontinent Indian Ocean Arabian Sea Himalayas1Relative to the African platePlate movementsDue 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 140 million years ago 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 a process which led to the opening of the Indian Ocean In the late Cretaceous approximately 100 million years ago 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 20 cm 7 9 in per year and is believed to have begun colliding with Asia as early as 55 million years ago in the Eocene epoch of the Cenozoic However some authors suggest the collision between India and Eurasia occurred much later around 35 million years ago If the collision occurred between 55 and 50 Mya the Indian plate would have covered a distance of 3 000 to 2 000 km 1 900 1 200 mi 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 1 300 km or 800 mi and the amount of convergence between India and Asia 3 600 km or 2 200 mi 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 In 2007 German geologists suggested the reason the Indian plate moved so quickly is that it is only half as thick 100 km or 62 mi as the other plates 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 The remains of this plume today form the Prince Edward Islands the Kerguelen hotspot and the Reunion hotspots 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 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 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 Perez Diaz 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 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 five cm 2 0 in per year while the Eurasian plate is moving north at only two cm 0 79 in per year This is causing the Eurasian plate to deform and the Indian plate to compress at a rate of four mm 0 16 in per year citation needed GeographyThe westerly side of the Indian plate is a transform boundary with the Arabian plate called the Owen fracture zone and a divergent boundary with the African plate called the Central Indian Ridge CIR The northerly side of the plate is a convergent boundary with the Eurasian plate forming the Himalaya and Hindu Kush mountains called the Main Himalayan Thrust citation needed See alsoGeology portalIndia portalHistorical geology List of tectonic plate interactions List of tectonic plates Palaeogeography Seychelles microcontinentNotes Sizes of Tectonic or Lithospheric Plates Geology about com 2014 03 05 Archived from the original on 2016 06 05 Retrieved 2016 01 13 Oskin Becky 2013 07 05 New Look at Gondwana s Breakup Livescience com Retrieved 2016 01 13 Stein Seth Sella Giovanni F Okai Emile A 2002 The January 26 2001 Bhuj Earthquake and the Diffuse Western Boundary of the Indian Plate Plate Boundary Zones PDF Geodynamics Series American Geophysical Union pp 243 254 doi 10 1029 GD030p0243 ISBN 9781118670446 Retrieved 2015 12 25 Sinvhal Understanding Earthquake Disasters p 52 Tata McGraw Hill Education 2010 ISBN 978 0 07 014456 9 Kumar M Ravi Bhatia S C 1999 A new seismic hazard map for the Indian plate region under the global seismic hazard assessment programme Current Science 77 3 447 JSTOR 24102967 M Asif Khan Tectonics of the Nanga Parbat syntaxis and the Western Himalaya p 375 Geological Society of London 2000 ISBN 978 1 86239 061 4 Srikrishna Prapnnachari Concepts in Frame Design page 152 Srikrishna Prapnnachari ISBN 978 99929 52 21 4 A M Celal Sengor 1989 Tectonic evolution of the Tethyan Region Springer ISBN 978 0 7923 0067 0 Kind 2007 Kumar et al 2007 Scotese 2001 Aitchison Ali amp Davis 2007 van Hinsbergen D Lippert P Dupont Nivet G McQuarrie N Doubrivine P Spakman W Torsvik T 2012 Greater India Basin hypothesis and a two stage Cenozoic collision between India and Asia Proceedings of the National Academy of Sciences 109 20 7659 7664 Bibcode 2012PNAS 109 7659V doi 10 1073 pnas 1117262109 PMC 3356651 PMID 22547792 Qin Shi Xin Li Yong Xiang Li Xiang Hui Xu Bo Luo Hui 2019 01 17 Paleomagnetic results of Cretaceous cherts from Zhongba southern Tibet New constraints on the India Asia collision Journal of Asian Earth Sciences 173 42 53 Bibcode 2019JAESc 173 42Q doi 10 1016 j jseaes 2019 01 012 ISSN 1367 9120 S2CID 134469511 The lithospheric roots in South Africa Australia and Antarctica are 300 to 180 km 190 to 110 mi thick Kumar et al 2007 See also Kumar et al 2007 figure 1 Meert J G Tamrat Endale 2006 Paleomagnetic evidence for a stationary Marion hotspot Additional paleomagnetic data from Madagascar Gondwana Research 10 3 4 340 348 Bibcode 2006GondR 10 340M doi 10 1016 j gr 2006 04 008 Schulte Peter et al 5 March 2010 The Chicxulub Asteroid Impact and Mass Extinction at the Cretaceous Paleogene Boundary PDF Science 327 5970 AAAS 1214 1218 Bibcode 2010Sci 327 1214S doi 10 1126 science 1177265 ISSN 1095 9203 PMID 20203042 S2CID 2659741 Perez Diaz L Eagles G Sigloch K 2020 Indo Atlantic plate accelerations around the Cretaceous Paleogene boundary A time scale error not a plume push signal Geology 48 12 1169 1173 Bibcode 2020Geo 48 1169P doi 10 1130 G47859 1 Andrews Robin George 14 April 2021 The New Historian of the Smash That Made the Himalayas Quanta Magazine Retrieved 15 April 2021 ReferencesAitchison Jonathan C Ali Jason R Davis Aileen M 2007 When and where did India and Asia collide Journal of Geophysical Research 112 B5 B05423 Bibcode 2007JGRB 112 5423A CiteSeerX 10 1 1 1008 2522 doi 10 1029 2006JB004706 hdl 10722 72794 ISSN 0148 0227 Retrieved January 12 2016 Chen Ji January 4 2005 Magnitude 9 0 off W coast of northern Sumatra Sunday December 26 2004 at 00 58 49 UTC Preliminary rupture model United States Geological Survey Archived from the original on March 5 2005 Retrieved 28 December 2004 Kind Rainer 17 October 2007 The fastest continent India s truncated lithospheric roots Press release Helmholtz Association of German Research Centres Retrieved 2 October 2019 Kumar Prakash Yuan Xiaohui Kumar M Ravi Kind Rainer Li Xueqing Chadha R K 18 October 2007 The rapid drift of the Indian tectonic plate Nature 449 7164 894 897 Bibcode 2007Natur 449 894K doi 10 1038 nature06214 ISSN 0028 0836 PMID 17943128 S2CID 4339656 Scotese Christopher R January 2001 The collision of India and Asia 90 mya present Paleomap Project Retrieved 28 December 2004 External linksMedia related to Indian tectonic plate at Wikimedia Commons