首页> 外文期刊>Earth and Planetary Science Letters: A Letter Journal Devoted to the Development in Time of the Earth and Planetary System >U-Pb age and Hf isotopic constraints of detrital zircons from the Himalayan foreland Subathu sub-basin on the Tertiary palaeogeography of the Himalaya
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U-Pb age and Hf isotopic constraints of detrital zircons from the Himalayan foreland Subathu sub-basin on the Tertiary palaeogeography of the Himalaya

机译:喜马拉雅第三纪古地理上喜马拉雅前陆苏巴图亚盆地碎屑锆石的U-Pb年龄和Hf同位素约束

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摘要

The Subhimalaya of NW India exposes a well developed marine to continental foreland sequence preserving sediments shed from the tectonically evolving Cenozoic Himalayan orogen. Detrital zircon U-Pb ages and their Hf isotopic compositions, of seven samples, were analyzed from the Subathu sub-basin foreland formations to constrain sediment provenance. The detrital zircon U-Pb age spectra yielded a similar pattern, for all foreland formations, with major peaks clustered at ~. 500-650. Ma, 900-1000. Ma and ~. 2500. Ma, corresponding to (indistinguishable) Tethyan Himalaya and Higher Himalayan Crystalline sources and those at ~. 1800-1900. Ma corresponding to lower a Lesser Himalayan arc source. Comparison of the foreland detrital zircon U-Pb age spectra with Himalayan lithotectonic source units, in conjunction with their Hf isotopes and previously determined sediment petrography and age constraints, suggest that the sediments to the flysch marine Subathu Formation (~65 to >41. Ma) were sourced from a positive-relief area of the Tethyan Himalaya mixed with detritus from lower Lesser Himalaya and additional cratonic northern Indian Precambrian rocks. No Cretaceous to Eocene-aged detrital zircons, contributed by eroding Ladakh batholith north of the Indus Tsangpo suture zone, were recorded in the Palaeogene-aged foreland samples. The younger synorogenic continental Dagshai Formation (<30 to <22. Ma) sediments were sourced from the very low-grade Tethyan Himalaya, whereas the alluvial-facies Kasauli Formation (<22 to 13. Ma) began to receive sediments additionally from erosion of the medium-grade metamorphic rocks of the Higher Himalayan Crystalline and the lower Lesser Himalaya. The Lower Siwalik Formation sediments (~13-11.5. Ma) were derived from the low-grade rocks of the Tethyan Himalaya, both the upper and lower Lesser Himalaya and additionally from the eroding high-grade migmatitic gneisses of the Higher Himalayan Crystalline. Thus, from the similar detrital zircon age spectra of the foreland formations, we infer that differences in the continental sediment detritus into the foreland basin reflect a straightforward sediment mixture of variable proportions from fixed Himalayan lithotectonic sources which progressively shifted towards the foreland with development of the orogen.
机译:印度西北部的喜马拉雅山将发育良好的海洋到大陆前陆序列暴露出来,并保留了构造演化的新生代喜马拉雅造山带中沉积的沉积物。从Subathu次盆地前陆地层中分析了七个样品的碎屑锆石U-Pb年龄及其Hf同位素组成,以限制沉积物来源。碎屑锆石的U-Pb年龄谱对于所有前陆形成都产生相似的模式,主要峰聚集在〜处。 500-650。马900-1000麻〜。 2500. Ma,对应于(不可区分的)特提斯喜马拉雅山和更高的喜马拉雅结晶源以及〜处的那些。 1800-1900。 Ma对应于降低小喜马拉雅弧源。将前陆碎屑锆石U-Pb年龄谱与喜马拉雅岩性构造源单元及其Hf同位素和先前确定的沉积物岩相学和年龄限制进行比较,表明该沉积物为复理海苏巴图组(〜65至> 41。Ma )来源于特提斯喜马拉雅山的正浮雕地区,混合有来自小喜马拉雅山下游的碎屑和其他克拉通北部印度前寒武纪岩石。在古近纪年龄的前陆样品中,没有记录到由始祖印度洋缝合线以北的拉达克岩床侵蚀造成的白垩纪至始新世的碎屑锆石。较年轻的同生成陆大陆Dagshai组(<30至<22。Ma)沉积物来自极低品位的特提斯喜马拉雅山,而冲积相Kasauli组(<22至13. Ma)也开始从泥沙的侵蚀中获得沉积物。喜马拉雅山高结晶带和小喜马拉雅山下带的中级变质岩。下西瓦里克组沉积物(〜13-11.5。Ma)来自特提斯喜马拉雅山脉的低品位岩石,小喜马拉雅山脉的上,下,以及喜马拉雅山脉高品位的侵蚀性高品位片麻岩。因此,从前陆地层的类似碎屑锆石年龄谱中,我们推断进入前陆盆地的大陆沉积物碎屑的差异反映了固定比例的喜马拉雅岩性构造源的直接不同比例的沉积物混合物,随着沉积物的发展逐渐向前陆转移。造山带。

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