Volume 45 Issue 10
Nov.  2020
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Lu Huan, Wang Qingbin, Niu Chengmin, Du Xiaofeng, Song Zhangqiang, Feng Chong, 2020. Meteoric Leaching Evidences, Diagenetic Model and Its Geology Significance in Mixed Rock of Steep Slope Zone of Shijiutuo Uplift. Earth Science, 45(10): 3721-3730. doi: 10.3799/dqkx.2020.175
Citation: Lu Huan, Wang Qingbin, Niu Chengmin, Du Xiaofeng, Song Zhangqiang, Feng Chong, 2020. Meteoric Leaching Evidences, Diagenetic Model and Its Geology Significance in Mixed Rock of Steep Slope Zone of Shijiutuo Uplift. Earth Science, 45(10): 3721-3730. doi: 10.3799/dqkx.2020.175

Meteoric Leaching Evidences, Diagenetic Model and Its Geology Significance in Mixed Rock of Steep Slope Zone of Shijiutuo Uplift

doi: 10.3799/dqkx.2020.175
  • Received Date: 2020-04-10
  • Publish Date: 2020-11-17
  • QHD29-2E and Q36 structure is so far the largest fan delta siliciclastic and lacustrine carbonate mixed deposits in the first and second members of Shahejie Formation in Paleogene system of Bohai Bay area,which breaks record of maximum reserve scale of siliclastic-carbonate mixed reservoir,the maximum thickness of single oil-bearing layer,and the highest tested productivity in Bohai Sea area. In our recent research,based on comprehensive analysis of rock core,rock slice observation,carbon and oxygen isotope analysis and trace element analysis,it is found that meteoric water leaching diagenesis is the major factor for high reservoir quality forming in the mixing deposition of steep slope zone of Shijiutuo uplift. Petrographical and geochemical evidences of meteoric waters process are identified. It includes 2 processes:dissolution pores,integranular fissures,terrigenous kaolinite in conglomerates during syndepositional process,and vertical karst fissures,geopetal structure in carbonates during subaerial exposure. The meteoric leaching process could be divided into 3 stages,including provenance,transportation and beach bar periods. Finally,the meteoric diagenetic model of mixed deposits in the slope zone is established. Meteoric diagenesis takes place primarily in two formation zones:the vadose zone and the phreatic zone. The diagenetic feature and evolution model of each zone are also concluded.

     

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