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    Volume 36 Issue 3
    May  2011
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    Article Contents
    WANG Chun-guang, XU Wen-liang, WANG Feng, YANG De-bin, 2011. Petrogenesis of the Early Cretaceous Xi'anli Hornblende-Gabbros from the Southern Taihang Mountains: Evidence from Zircon U-Pb Geochronology, Hf Isotope and Whole-Rock Geochemistry. Earth Science, 36(3): 471-482. doi: 10.3799/dqkx.2011.049
    Citation: WANG Chun-guang, XU Wen-liang, WANG Feng, YANG De-bin, 2011. Petrogenesis of the Early Cretaceous Xi'anli Hornblende-Gabbros from the Southern Taihang Mountains: Evidence from Zircon U-Pb Geochronology, Hf Isotope and Whole-Rock Geochemistry. Earth Science, 36(3): 471-482. doi: 10.3799/dqkx.2011.049

    Petrogenesis of the Early Cretaceous Xi'anli Hornblende-Gabbros from the Southern Taihang Mountains: Evidence from Zircon U-Pb Geochronology, Hf Isotope and Whole-Rock Geochemistry

    doi: 10.3799/dqkx.2011.049
    • Received Date: 2010-12-18
    • Publish Date: 2011-05-01
    • This paper reports zircon U-Pb geochronology, Hf isotope, and whole-rock geochemical data, aimed at constraining the petrogenesis of the hornblende (Hb)-gabbros from the Xi'anli intrusion in the southern Taihang Mountains (Mts.). The intrusion is composed mainly of olivine-bearing Hb-gabbro, Hb-diorite, and diorite. Zircons from the Hb-gabbros display euhedral shape and zonal homogeneous absorption on CL images, and have high Th/U ratio (1.44-2.85), suggesting a magmatic origin. Their 206Pb/238U ages range from 135 to 127 Ma, yielding a mean age of 131±1 Ma (MSWD=6.5, n=15), which suggests that the Xi'anli Hb-gabbros were formed in the Early Cretaceous. The εHf(t) values of selected zircons range from -23.5 to -19.2. The Xi'anli Hb-gabbros have SiO2 = 50.27%-50.89%, Mg# =0.76-0.78, and Na2O/K2O= 2.18-2.37, and are enriched in transitional elements such as Sc (19.2-20.3)×10-6, Cr (939-1 050)×10-6, Co (54.6-58.2)×10-6, and Ni (645-718)×10-6. Moreover, these gabbros are characterized by relative enrichment in large ion lithophile elements (LILEs, such as Cs, Ba, Sr) and light rare earth elements (LREEs), and intensive depletion in high field strength elements (HFSEs, such as Nb, Ta, Zr, Hf) and heavy rare earth elements (HREEs). Combined with the mineralogical and geochemical study of the dunite xenolith and the olivine xenocrysts hosted in the Hb-gabbros, we propose that the Xi'anli Hb-gabbros may have been produced by the reaction of the delaminated lower continental crust-derived melt and mantle peridotite.

       

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