基于 10Be 和 21Ne 宇宙生成物的印度塔尔沙漠路面模型暴露年龄

IF 2.8 3区 地球科学 Q2 GEOGRAPHY, PHYSICAL
Rahul K. Kaushal, Sukumar Parida, Pavitra V. Kumar, Pankaj Kumar, Samuel Niedermann, Robert J. Wasson, Ram P. Dhir, Sundeep Chopra, Sheila Mishra, Shanti Pappu, Ashok K. Singhvi
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引用次数: 0

摘要

印度塔尔沙漠的沙漠路面由角状、长方形到圆形砾石组成,海拔略高于周围地形。沉积学和地貌学分析表明,这些路面是中生代和更古老的基岩风化而成的岩层。本研究首次根据宇宙射线产生的 10Be 和 21Ne 对塔尔沙漠四个地点(即 Bhojka、Hamira、Solanki 和 Jayal)的路面进行了地表暴露年龄分析。在计算模型暴露年龄时假定:(a)砾石来源于胶结砾岩,因构造作用而隆起,随后因气候作用而解体;(b)砾石中的宇宙成因核素产生于砾岩接近地表时,并在其解体、单个砾石的重力滑动和储存过程中持续至今。假设平均埋藏深度为 50 厘米,21Ne 和 10Be 数据分别提供了 1.30 至 2.92 Ma 和 1.11 至 5.4 Ma 的两种核素年龄。这些条件有利于碳酸盐的移动和沉淀。路面年龄和砾岩的最小年龄(2.51Ma)将这种沙漠化条件的时间延长到 > 2.51Ma,并表明塔尔沙漠化条件的开始可能与大约 3.6Ma 开始的全球干旱有关。在印度旧石器时代的背景下,砾石表面和沙丘内出现的工具表明,至少从公元前 0.76 年开始,该地区就被频繁占据,并与印度南部早更新世至中更新世的 Acheulian 组合相似。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Cosmogenic 10Be- and 21Ne-based model exposure ages of desert pavements in the Thar Desert, India

Cosmogenic 10Be- and 21Ne-based model exposure ages of desert pavements in the Thar Desert, India

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.

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来源期刊
Earth Surface Processes and Landforms
Earth Surface Processes and Landforms 地学-地球科学综合
CiteScore
6.40
自引率
12.10%
发文量
215
审稿时长
4 months
期刊介绍: Earth Surface Processes and Landforms is an interdisciplinary international journal concerned with: the interactions between surface processes and landforms and landscapes; that lead to physical, chemical and biological changes; and which in turn create; current landscapes and the geological record of past landscapes. Its focus is core to both physical geographical and geological communities, and also the wider geosciences
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