了解印度特提斯喜马拉雅斯皮蒂地区三叠纪沉积岩的物源和沉积条件

IF 1.7 Q3 GEOSCIENCES, MULTIDISCIPLINARY Journal of Asian Earth Sciences: X Pub Date : 2023-06-01 DOI:10.1016/j.jaesx.2023.100154
Javid A. Ganai , Shaik A. Rashid , Abdul Samad Siddiqui , Nurul Absar , Heena , Ghulam Jeelani
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引用次数: 0

摘要

斯皮蒂地区被誉为印度地质博物馆,是一个世界著名的沉积序列,包含从新元古代到白垩纪的良好暴露序列。采用地球化学和同位素方法,以理朗超群的三叠纪硅质碎屑沉积岩为研究对象,了解其风化史、物源、古气候和沉积条件。与PAAS(澳大利亚后太古宙页岩)相比,三叠纪页岩显示出或多或少相似的成分,CaO大量富集,这可能归因于该地区与石灰岩的结合。然而,砂岩显示出微量元素浓度的显著减少,这表明石英稀释的影响。在页岩的微量元素蜘蛛图中可以注意到流动元素(Rb、Ba)相对于不动元素(Zr、Nb、Hf)的相对损耗。三叠纪沉积岩具有富集的LREE和贫化的HREE模式,具有明显的负Eu异常。蚀变化学指数(CIA;56-86)表明源区化学风化程度低至强烈。地层向上剖面中CIA和其他风化指数的异常下降归因于三叠纪沉积物沉积期间气候和环境条件的变化。解开这些特征对于理解大灭绝危机至关重要,尤其是缺氧在这些事件中的作用。在氧化还原敏感元素二元图中,三叠纪黑色页岩代表了低氧到缺氧的沉积条件。本研究的碳同位素数据得到了总有机碳(TOC)的有力支持,该数据推断海洋生物系统试图从生物生命的枯竭中恢复。εNd和87Sr/86Sr系统学记录了三叠纪早期至晚期烃源地形的变化。与晚三叠世沉积物(TDM=1.76–1.91 Ga)相比,早三叠世样品显示出更古老的贫化地幔模型年龄(TDM=1.94–1.98 Ga)。Th/Sc比率(从~6到~0.05)和(La/Yb)N比率(从~32到~5)可以得出类似的解释,记录了从早三叠世到晚三叠世Spiti沉积岩的这些比率的增加。总的来说,Spiti地区三叠纪岩石的微量元素比率和放射成因同位素特征指向泛非花岗岩起源,而幼年富含镁铁质的源岩(如Panjal Traps、非洲克拉通和阿拉伯-努比亚地盾)则留下了少量印记。
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Understanding the provenance and depositional conditions of Triassic sedimentary rocks from the Spiti region, Tethys Himalaya, India

The Spiti region, renowned as the Museum of Indian Geology, is a world-famous sedimentary succession containing well-exposed sequences from Neoproterozoic to Cretaceous age. In this study, Triassic siliciclastic sedimentary rocks of the Lilang Supergroup were chosen to understand weathering history, provenance, paleoclimate, and depositional conditions using a geochemical and isotopic approach. Triassic shales show more or less similar compositions with substantial enrichment in CaO compared to PAAS (Post Archean shales from Australia), which may be attributed to the association with limestones in the region. However, the sandstones display significant depletion in the trace element concentrations signifying the effect of quartz dilution. The relative depletion of mobile elements (Rb, Ba) as against immobile elements (Zr, Nb, Hf) can be noticed in the trace element spider diagram of the shales. The Triassic sedimentary rocks are characterized by enriched LREE and depleted HREE patterns with pronounced negative Eu anomalies. The Chemical Index of Alteration (CIA; 56–86) indicates low to intense chemical weathering in the source area. The unusual decrease in CIA and other weathering indices in the stratigraphically up section is attributed to changes in climate and environmental conditions during the deposition of sediments in the Triassic period. Detangling the signatures is crucial to understanding the mass extinction crisis, particularly the role of anoxia in these events. Triassic black shales represent suboxic to anoxic depositional conditions in the redox-sensitive elemental binary diagrams. The carbon isotope data of the present study is very well supported by the Total Organic Carbon (TOC), which infers that the oceanic biological system tried to recover from the depletion of biological life. The εNd and 87Sr/86Sr systematics record a shift in source terrains from the Early to Late Triassic period. The Early Triassic samples show much older depleted mantle model ages (TDM = 1.94–1.98 Ga) compared to Late Triassic sediments (TDM = 1.76–1.91 Ga). Similar interpretations can be drawn from Th/Sc ratios (from ∼ 6 to ∼ 0.05) and (La/Yb) N ratios (from ∼ 32 to ∼ 5), which record an increase in these ratios from Early Triassic to Late Triassic formations of the Spiti sedimentary rocks. Overall, trace elemental ratios and radiogenic isotopic signatures of the Triassic rocks of the Spiti region point towards Pan African granitic origin with minor impressions from the juvenile mafic-rich sources, such as Panjal Traps, the African craton, and Arabian-Nubian shield.

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来源期刊
Journal of Asian Earth Sciences: X
Journal of Asian Earth Sciences: X Earth and Planetary Sciences-Earth-Surface Processes
CiteScore
3.40
自引率
0.00%
发文量
53
审稿时长
28 weeks
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