Sehsah Haytham, Furnes Harald, Pham Luan Thanh, Eldosouky Ahmed M
Geology Department, Faculty of Science, Damietta University, New Damietta, Damietta, 34517, Egypt.
Department of Earth Science, University of Bergen, Allegt. 41, 5007, Bergen, Norway.
Sci Rep. 2022 Aug 3;12(1):13349. doi: 10.1038/s41598-022-16981-y.
The debatable timing of India-Eurasia collision is based on geologic, stratigraphic, kinematic, and tectonic evidence. However, the collision event disturbed persistent processes, and the timing of disturbance in such processes could determine the onset of India-Eurasia collision precisely. We use the longevity of Southeast Indian Ridge (SEIR)-Kerguelen mantle plume (KMP) interaction cycles along the Ninetyeast ridge (NER) as a proxy to determine the commencement of India-Eurasia collision. The geochemical signature of the KMP tail along the NER is predominantly that of long-term coupling cycles, that was perturbed once by a short-term decoupling cycle. The long-term coupling cycles are mainly of enriched mid-ocean ridge basalts (E-MORBs). The short-term decoupling cycle is mostly derived from two distinct sources, MOR and plume separately, whereas the KMP is still being on-axis. The onset of India-Eurasia collision led to continental materials recycling into the mantle; hence the abrupt enrichment in incompatible elements at ca. 55 Ma, the MOR-plume on-axis decoupling, and the abrupt slowdown in the northward drift of the Indian plate was induced by the onset of India-Eurasia collision, thereafter MOR-plume recoupled.
印度与欧亚大陆碰撞时间存在争议,其依据是地质、地层、运动学和构造学证据。然而,碰撞事件扰乱了持续的过程,而这些过程中干扰的时间可以精确确定印度与欧亚大陆碰撞的开始时间。我们利用沿着东经九十度海岭(NER)的东南印度海岭(SEIR)-凯尔盖朗地幔柱(KMP)相互作用周期的持续时间作为代理,来确定印度与欧亚大陆碰撞的开始。沿着NER的KMP尾部的地球化学特征主要是长期耦合周期的特征,该特征曾被一个短期解耦周期扰动过。长期耦合周期主要是富集型大洋中脊玄武岩(E-MORB)。短期解耦周期大多分别来自两个不同的源,即大洋中脊和地幔柱,而KMP仍位于轴线上。印度与欧亚大陆碰撞的开始导致大陆物质再循环进入地幔;因此,约5500万年前不相容元素的突然富集、大洋中脊-地幔柱在轴线上的解耦以及印度板块向北漂移的突然减缓是由印度与欧亚大陆碰撞的开始引起的,此后大洋中脊-地幔柱重新耦合。