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    中国百强科技报刊

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    Volume 39 Issue 2
    Feb.  2014
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    Article Contents
    Zhou Qunjun, Xu Wenliang, Wang Qinghai, Yang Debin, Pei Fuping, Yu Yang, 2014. Petrogenesis of Olivine-Bearing Clinopyroxenite Xenolith in Early Cretaceous Adakitic Rocks from Xuhuai Area in Eastern China and Its Petrologic Implication. Earth Science, 39(2): 141-154. doi: 10.3799/dqkx.2014.014
    Citation: Zhou Qunjun, Xu Wenliang, Wang Qinghai, Yang Debin, Pei Fuping, Yu Yang, 2014. Petrogenesis of Olivine-Bearing Clinopyroxenite Xenolith in Early Cretaceous Adakitic Rocks from Xuhuai Area in Eastern China and Its Petrologic Implication. Earth Science, 39(2): 141-154. doi: 10.3799/dqkx.2014.014

    Petrogenesis of Olivine-Bearing Clinopyroxenite Xenolith in Early Cretaceous Adakitic Rocks from Xuhuai Area in Eastern China and Its Petrologic Implication

    doi: 10.3799/dqkx.2014.014
    • Received Date: 2013-04-28
    • Publish Date: 2014-02-01
    • The petrography and mineral chemical data of olivine-bearing clinopyroxenite xenolith entrained by the Early Cretaceous adakitic rocks in Xuhuai area, eastern China are reported in this paper. Olivine-bearing clinopyroxenite consists of clinopyroxene (~80%), orthopyroxene (~5%), olivine (~5%), and hornblende (~10%) and displays cumulate texture and massive structure. The orthopyroxene reaction rim can be found around olivine. The hornblendes occur among pyroxenes, and display poikilitic texture. The mineral chemical data indicate that olivines have forsterite (Fo)=77.7-79.3 and Ni=623×10-6-773×10-6, that orthopyroxenes have Mg#=75.6-80.2, Cr=161×10-6-684 ×10-6, and Ni=79×10-6-708×10-6, and that clinopyroxenes have Mg#=84.5-86.4, CaO=21.59%-23.13%, Al2O3=1.72%-2.44%. Chemically, these minerals are similar to the olivine, orthopyroxene, and clinopyroxene phenocrysts from the Mesozoic and Cenozoic basalts and those from the pyroxenites with cumulate origin. Additionally, the clinopyroxenes from the xenolith are characterized by convex upward rare earth element (REE) distribution patterns, low REE contents (∑REE=10.14×10-6-12.71×10-6), and no Eu anomalies (δEu=0.90-1.16), similar to the clinopyroxene phenocrysts in the Cenozoic basalts. Hornblendes in this xenolith have Mg#=74.0-80.4, SiO2=43.2%-44.5%, Na2O=2.04%-2.29%, and display flat REE patterns and depletion in high field strength elements (HFSEs, Nb, Ta, Zr and Hf) and Th as well as enrichment in Sr, Rb and Ba, different from those hornblende xenocrysts from Cenozoic basalts. Combined with its poikilitic texture, it is suggested that these hornblendes could be formed by injection of the host magma. Taken together, we conclude that the olivine-bearing clinopyroxenite xenolith could be formed by the high-pressure accumulation of basaltic melt. Combined with Early Cretaceous bimodal magmatism in eastern China, it is suggested that the olivine-bearing clinopyroxenite could be generated by the underplating of mantle-derived basaltic magma.

       

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