Cosmogenic10Be‐ and21Ne‐based model exposure ages of desert pavements in the 
Thar Desert, India

Kaushal, Rahul K.; Parida, Sukumar; Kumar, Pavitra V.; Kumar, Pankaj; Niedermann, Samuel; Wasson, Robert J.; Dhir, Ram P.; Chopra, Sundeep; Mishra, Sheila; Pappu, Shanti; Singhvi, Ashok K.

doi:10.1002/esp.5999

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Cosmogenic10Be‐ and21Ne‐based model exposure ages of desert pavements in the Thar Desert, India

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Kaushal, Rahul K.
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Parida, Sukumar
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Kumar, Pavitra V.
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Kumar, Pankaj
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Niedermann, Samuel
3.1 Inorganic and Isotope Geochemistry, 3.0 Geochemistry, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum;

Wasson, Robert J.
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Dhir, Ram P.
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Chopra, Sundeep
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Mishra, Sheila
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Pappu, Shanti
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Singhvi, Ashok K.
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Kaushal, R. K., Parida, S., Kumar, P. V., Kumar, P., Niedermann, S., Wasson, R. J., Dhir, R. P., Chopra, S., Mishra, S., Pappu, S., Singhvi, A. K. (2024): Cosmogenic10Be‐ and21Ne‐based model exposure ages of desert pavements in the Thar Desert, India. - Earth Surface Processes and Landforms, 49, 14, 4808-4822.
https://doi.org/10.1002/esp.5999

Cite as: https://gfzpublic.gfz-potsdam.de/pubman/item/item_5028648

Abstract

The Thar Desert, India has desert pavements comprising angular-subangular to well-rounded gravels at marginally higher elevations than the surrounding terrain. Sedimentological and geomorphic analyses suggest that the pavements are lags of weathered Mesozoic and older bedrock. The presence of Palaeolithic artefacts on the pavement surfaces and occasionally within their matrix was used to infer their antiquity and landscape stability. This study presents the first surface exposure ages based on cosmic-ray-produced 10Be and 21Ne for pavements at four sites in the Thar Desert, viz. Bhojka, Hamira, Solanki and Jayal. The computation of model exposure ages assumed that (a) the gravels were derived from cemented conglomerates, uplifted by tectonics and thereafter disintegrated by climate, and (b) cosmogenic nuclide production in the gravels began when the conglomerates approached the surface and, continued during their disintegration, gravity sliding of individual gravels and storage, until the present. Assuming an average burial depth of 50 cm, 21Ne and 10Be data provide ages ranging from 1.30 to 2.92 Ma and 1.11 to 5.4 Ma, respectively, for the two nuclides. Published electron spin resonance ages of Thar calcretes suggest the presence of water and extreme seasonality since 1.54 Ma. Such conditions facilitated the mobilization and precipitation of carbonates. The pavement ages and the minimum age of the conglomerate at 2.51 Ma extend the time of such desertic conditions to > 2.51 Ma and suggest that the initiation of desertic conditions in the Thar was possibly linked to global aridity beginning around 3.6 Ma. Depending on assumptions, cosmic ray surface exposure (10Be) ages at Jayal range between 0.76 and 2.43 Ma. In the context of the Indian Palaeolithic, the presence of tools on the gravel surfaces and within dunes, suggests frequent occupation of this region from at least 0.76 Ma and, parallels Early to Middle Pleistocene Acheulian assemblages from Southern India.