Large variations in the lithospheric thickness of northwestern India: Imprints of collisional and thermal reworking

IF 2.4 3区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Niraj Kumar, Om Prakash, V.M. Tiwari, A.P. Singh
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Abstract

The fold belts, which border the cratons, are the building blocks for understanding the origin and modification of older continents. The Aravalli-Delhi Fold Belt (ADFB) in northwestern India provides evidence of crustal block accretion due to continental collision, whereas Malani Igneous Suite (MIS) modified with widespread magmatism. Imaging of upper mantle structure and lithospheric modifications, if any, of such regions has been intricate owing to reworking by subsequent superimposed tectono-magmatic processes. We applied a 2D modelling approach to model the lithospheric architecture along a 1000-km long WNW-SSE geotransect across northwestern India, which has been deformed in the past. Our modelling technique combines terrestrial gravity anomaly, heat flow data, satellite-based geoid, and topographic datasets using the basic premise of thermal steady-state and local isostasy. The overall 38 to 40 km thick crustal geometry underneath the Marwar Block had the maximum lithological heterogeneity. The region surrounding the MIS is characterised by 8–10 km thick high-density (2.78 g/cm3) sills deposited in the upper crust down to 9 km depth and another 10–15 km thick high-density (3.05 g/cm3) mafic mantle material near the Moho. About 42 km thick crust, including an 8 to 10-km thick high-density (3.05 g/cm3) underplated layer at its bottom, characterises the high-relief ADFB. The Vindhyan region of Bundelkhand craton is defined by a ∼ 1 km thick trap, having Moho extending at a depth of ∼40 km. The lithospheric thickness varies substantially from ∼143–168 km underneath the Marwar block, which thins to ∼135 km under the ADFB and thickens gradually to ∼150–165 km beneath the Vindhyan region. Substantial crustal density differences in distinct crustal domains, when integrated with the thin lithosphere, reinforce the concept that tectono-magmatic processes might have modified the lithosphere in NW India.

Abstract Image

印度西北部岩石圈厚度的巨大变化:碰撞和热再加工的印记
褶皱带与陆块交界,是了解旧大陆起源和改造的基础。印度西北部的阿拉瓦利-德里褶皱带(Aravalli-Delhi Fold Belt,ADFB)提供了大陆碰撞导致地壳块体增生的证据,而马拉尼火成岩组(Malani Igneous Suite,MIS)则通过广泛的岩浆活动进行了改造。这些地区的上地幔结构和岩石圈的变化(如果有的话)由于随后叠加的构造-岩浆过程的再加工而变得错综复杂。我们采用二维建模方法,沿印度西北部 1000 公里长的 WNW-SSE 地质断面对岩石圈结构进行建模,该断面在过去曾发生过变形。我们的建模技术结合了陆地重力异常、热流数据、卫星大地水准面和地形数据集,以热稳态和局部等稳态为基本前提。马尔瓦地块下 38 至 40 千米厚的地壳几何形状具有最大的岩性异质性。MIS周围区域的特点是,上地壳有8-10千米厚的高密度(2.78克/立方厘米)岩屑沉积至9千米深处,莫霍附近还有10-15千米厚的高密度(3.05克/立方厘米)岩浆地幔物质。约42千米厚的地壳,包括其底部8至10千米厚的高密度(3.05克/立方厘米)下伏层,是高起伏ADFB的特征。邦德尔康德克拉通的文迪安地区由厚达 1 千米的陷落层所界定,莫霍面延伸至 40 千米深处。岩石圈厚度变化很大,在马尔瓦地块下为 143-168 千米,在 ADFB 下减薄至 135 千米,在 Vindhyan 地区下逐渐增厚至 150-165 千米。不同地壳域的巨大地壳密度差异与薄岩石圈相结合,强化了构造-岩浆过程可能改变了印度西北部岩石圈的概念。
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来源期刊
Physics of the Earth and Planetary Interiors
Physics of the Earth and Planetary Interiors 地学天文-地球化学与地球物理
CiteScore
5.00
自引率
4.30%
发文量
78
审稿时长
18.5 weeks
期刊介绍: Launched in 1968 to fill the need for an international journal in the field of planetary physics, geodesy and geophysics, Physics of the Earth and Planetary Interiors has now grown to become important reading matter for all geophysicists. It is the only journal to be entirely devoted to the physical and chemical processes of planetary interiors. Original research papers, review articles, short communications and book reviews are all published on a regular basis; and from time to time special issues of the journal are devoted to the publication of the proceedings of symposia and congresses which the editors feel will be of particular interest to the reader.
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