Paleolatitudes of the Tibetan Himalaya from primary and secondary magnetizations of Jurassic to Lower Cretaceous sedimentary rocks

Publication date

2015-01-15

Authors

Huang, WentaoISNI 0000000449452454
van Hinsbergen, Douwe J.J.ORCID 0000-0003-3410-0344ISNI 0000000065827851
Dekkers, Mark J.ISNI 0000000138306804
Garzanti, Eduardo
Dupont-Nivet, GuillaumeISNI 0000000388630324
Lippert, Peter C.
Li, Xiaochun
Maffione, MarcoISNI 0000000506825991
Langereis, CorORCID 0000-0001-9232-2178ISNI 0000000032917519
Hu, Xiumian

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Abstract

The Tibetan Himalaya represents the northernmost continental unit of the Indian plate that collided with Asia in the Cenozoic. Paleomagnetic studies on the Tibetan Himalaya can help constrain the dimension and paleogeography of "Greater India," the Indian plate lithosphere that subducted and underthrusted below Asia after initial collision. Here we present a paleomagnetic investigation of a Jurassic (limestones) and Lower Cretaceous (volcaniclastic sandstones) section of the Tibetan Himalaya. The limestones yielded positive fold test, showing a prefolding origin of the isolated remanent magnetizations. Detailed paleomagnetic analyses, rock magnetic tests, end-member modeling of acquisition curves of isothermal remanent magnetization, and petrographic investigation reveal that the magnetic carrier of the Jurassic limestones is authigenic magnetite, whereas the dominant magnetic carrier of the Lower Cretaceous volcaniclastic sandstones is detrital magnetite. Our observations lead us to conclude that the Jurassic limestones record a prefolding remagnetization, whereas the Lower Cretaceous volcaniclastic sandstones retain a primary remanence. The volcaniclastic sandstones yield an Early Cretaceous paleolatitude of 55.5°S [52.5°S, 58.6°S] for the Tibetan Himalaya, suggesting it was part of the Indian continent at that time. The size of "Greater India" during Jurassic time cannot be estimated from these limestones. Instead, a paleolatitude of the Tibetan Himalaya of 23.8°S [21.8°S, 26.1°S] during the remagnetization process is suggested. It is likely that the remagnetization, caused by the oxidation of early diagenetic pyrite to magnetite, was induced during 103-83 or 77-67 Ma. The inferred paleolatitudes at these two time intervals imply very different tectonic consequences for the Tibetan Himalaya.

Keywords

Paleolatitude, Remagnetization, Tibetan Himalaya, Geochemistry and Petrology, Geophysics

Citation

Huang, W, van Hinsbergen, D J J, Dekkers, M J, Garzanti, E, Dupont-Nivet, G, Lippert, P C, Li, X, Maffione, M, Langereis, C G, Hu, X, Guo, Z & Kapp, P 2015, 'Paleolatitudes of the Tibetan Himalaya from primary and secondary magnetizations of Jurassic to Lower Cretaceous sedimentary rocks', Geochemistry, Geophysics, Geosystems, vol. 16, no. 1, pp. 77-100. https://doi.org/10.1002/2014GC005624