首页> 外文期刊>Journal of Asian earth sciences >Provenance of sediments in the Marwar Supergroup, Rajasthan, India: Implications for basin evolution and Neoproterozoic global events
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Provenance of sediments in the Marwar Supergroup, Rajasthan, India: Implications for basin evolution and Neoproterozoic global events

机译:印度拉贾斯坦邦的Marwar超级群中的沉积物来源:对盆地演化和新元古代全球事件的影响

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The Marwar Supergroup of NW India is one of the largest Neoproterozoic sedimentary successions of India. Deposited in an intracratonic sag basin, the Supergroup contains largely unmetamorphosed and undeformed fluvial and marginal marine siliciclastics, marine carbonates, and minor volcaniclastics which hold clues to the geotectonic evolution of India subsequent to the disintegration of the Rodinia and during the formation of the Gondwanaland. Here, we present age constraints for the initiation of sedimentation and evolution of the basin. The Rb-Sr whole rock isochron of a felsic tuff from the lower part of the Supergroup, yields an age of 703 +/- 40 Ma, which suggests that the sedimentation in the Marwar basin started in the Cryogenian period. The result of Sr isotope stratigraphy suggests a depositional age of similar to 570 Ma (Late Ediacaran) for the carbonate sequences in the middle part of the Supergroup, indicating a depositional hiatus of similar to 100 Ma between the lower and middle Marwars. We speculate that this relapse in the sedimentation could be related to the widespread Pan-African event (Malagasy Orogeny). Provenance analysis using Neodymium (Nd) isotopes and trace elements shows that sediments in the lower Marwars were contributed by the Delhi Supergroup (similar to 1.6 Ga), Banded Gneissic Complex-2 (> 1.8 Ga) and possibly the Erinpura Granites (similar to 850 Ma), whereas the siliciclastics deposited in the middle and upper Marwars were predominantly sourced from the Delhi Supergroup. Interestingly, the contribution from the Malani Igneous Suite (MIS) to the sedimentation is limited only to the basal formation near the basin margin.
机译:印度西北部的马尔瓦尔超群是印度最大的新元古代沉积演替之一。沉积在克拉通凹陷盆地内的超级群主要包含未变质和未变形的河流和边缘海相硅质碎屑岩,海相碳酸盐岩和少量火山碎屑岩,这些线索为罗迪尼亚解体后以及冈瓦纳大陆的形成提供了印度大地构造演化的线索。在这里,我们提出了盆地开始沉积和演化的年龄限制。来自超群下部的长英质凝灰岩的Rb-Sr全岩石等时线的年龄为703 +/- 40 Ma,这表明马尔瓦尔盆地的沉积始于冰冻期。 Sr同位素地层的结果表明,超群中部碳酸盐岩层序的沉积年龄大约为570 Ma(晚期爱迪卡拉岩),表明下,中马尔瓦尔之间的沉积裂隙类似于100 Ma。我们推测沉积物中的这种复发可能与广泛的泛非事件(马尔加斯造山运动)有关。使用钕(Nd)同位素和微量元素进行的物源分析表明,下马尔瓦尔地区的沉积物是由德里超群(类似于1.6 Ga),带状片麻岩复合体2(> 1.8 Ga)以及可能由Erinpura花岗岩(类似于850)贡献的Ma),而沉积在中,上马尔瓦尔地区的硅质碎屑岩主要来自德里超群。有趣的是,Malani火成岩套件(MIS)对沉积的贡献仅限于盆地边缘附近的基底地层。

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