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Henstock, Timothy J.ORCID iD iconorcid.org/0000-0002-2132-2514
Publications (2 of 2) Show all publications
Pickering, K. T., Pouderoux, H., McNeill, L. C., Backman, J., Chemale, F., Kutterolf, S., . . . Dugan, B. (2020). Sedimentology, stratigraphy and architecture of the Nicobar Fan (Bengal-Nicobar Fan System), Indian Ocean: Results from International Ocean Discovery Program Expedition 362. Sedimentology, 67(5), 2248-2281
Open this publication in new window or tab >>Sedimentology, stratigraphy and architecture of the Nicobar Fan (Bengal-Nicobar Fan System), Indian Ocean: Results from International Ocean Discovery Program Expedition 362
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2020 (English)In: Sedimentology, ISSN 0037-0746, E-ISSN 1365-3091, Vol. 67, no 5, p. 2248-2281Article in journal (Refereed) Published
Abstract [en]

Drill sites in the southern Bay of Bengal at 3 degrees N 91 degrees E (International Ocean Discovery Program Expedition 362) have sampled for the first time a complete section of the Nicobar Fan and below to the oceanic crust. This generally overlooked part of the Bengal-Nicobar Fan System may provide new insights into uplift and denudation rates of the Himalayas and Tibetan Plateau. The Nicobar Fan comprises sediment gravity-flow deposits, mostly turbidites, that alternate with hemipelagite drapes and pelagite intervals of varying thicknesses. The decimetre-thick to metre-thick oldest pre-fan sediments (limestones/chalks) dated at 69 Ma are overlain by volcanic material and slowly accumulated pelagites (0.5 g cm(-2) kyr(-1)). At Expedition 362 Site U1480, terrigenous input began in the early Miocene at ca 22.5 Ma as muds, overlain by very thin-bedded and thin-bedded muddy turbidites at ca 19.5 Ma. From 9.5 Ma, sand content and sediment supply sharply increase (from 1-5 to 10-50 g cm(-2) kyr(-1)). Despite the abundant normal faulting in the Nicobar Fan compared with the Bengal Fan, it offers a better-preserved and more homogeneous sedimentary record with fewer unconformities. The persistent connection between the two fans ceased at 0.28 Ma when the Nicobar Fan became inactive. The Nicobar Fan is a major sink for Himalaya-derived material. This study presents integrated results of International Ocean Discovery Program Expedition 362 with older Deep Sea Drilling Project/Ocean Drilling Program/International Ocean Discovery Program sites that show that the Bengal-Nicobar Fan System experienced successive large-scale avulsion processes that switched sediment supply between the Bengal Fan (middle Miocene and late Pleistocene) and the Nicobar Fan (late Miocene to early Pleistocene). A quantitative analysis of the submarine channels of the Nicobar Fan is also presented, including their stratigraphic frequency, showing that channel size/area and abundance peaked at ca 2 to 3 Ma, but with a distinct low at 3 to 7 Ma: the intervening stratigraphic unit was a time of reduced sediment accumulation rates.

Keywords
Bengal Fan, Indian Ocean, IODP Expedition 362, Nicobar Fan, sediment gravity flow, submarine fan, Sunda Subduction Zone
National Category
Earth and Related Environmental Sciences
Identifiers
urn:nbn:se:su:diva-180386 (URN)10.1111/sed.12701 (DOI)000515102100001 ()
Available from: 2020-04-01 Created: 2020-04-01 Last updated: 2025-02-07Bibliographically approved
McNeill, L. C., Dugan, B., Backman, J., Pickering, K. T., Pouderoux, H. F. A., Henstock, T. J., . . . Thomas, E. (2017). Understanding Himalayan erosion and the significance of the Nicobar Fan. Earth and Planetary Science Letters, 475, 134-142
Open this publication in new window or tab >>Understanding Himalayan erosion and the significance of the Nicobar Fan
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2017 (English)In: Earth and Planetary Science Letters, ISSN 0012-821X, E-ISSN 1385-013X, Vol. 475, p. 134-142Article in journal (Refereed) Published
Abstract [en]

A holistic view of the Bengal-Nicobar Fan system requires sampling the full sedimentary section of the Nicobar Fan, which was achieved for the first time by International Ocean Discovery Program (IODP) Expedition 362 west of North Sumatra. We identified a distinct rise in sediment accumulation rate (SAR) beginning similar to 9.5 Ma and reaching 250-350 m/Myr in the 9.5-2 Ma interval, which equal or far exceed rates on the Bengal Fan at similar latitudes. This marked rise in SAR and a constant Himalayan-derived provenance necessitates a major restructuring of sediment routing in the Bengal-Nicobar submarine fan. This coincides with the inversion of the Eastern Himalayan Shillong Plateau and encroachment of the west-propagating Indo-Burmese wedge, which reduced continental accommodation space and increased sediment supply directly to the fan. Our results challenge a commonly held view that changes in sediment flux seen in the Bengal-Nicobar submarine fan were caused by discrete tectonic or climatic events acting on the Himalayan-Tibetan Plateau. Instead, an interplay of tectonic and climatic processes caused the fan system to develop by punctuated changes rather than gradual progradation.

Keywords
Bengal-Nicobar Fan, submarine fan, Himalayan tectonics, Asian monsoon, Indian Ocean
National Category
Earth and Related Environmental Sciences
Identifiers
urn:nbn:se:su:diva-147858 (URN)10.1016/j.epsl.2017.07.019 (DOI)000411167800012 ()
Available from: 2017-10-27 Created: 2017-10-27 Last updated: 2025-02-07Bibliographically approved
Identifiers
ORCID iD: ORCID iD iconorcid.org/0000-0002-2132-2514

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