کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
4715535 1638651 2016 14 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
The syncollisional granitoid magmatism and continental crust growth in the West Kunlun Orogen, China – Evidence from geochronology and geochemistry of the Arkarz pluton
موضوعات مرتبط
مهندسی و علوم پایه علوم زمین و سیارات ژئوشیمی و پترولوژی
پیش نمایش صفحه اول مقاله
The syncollisional granitoid magmatism and continental crust growth in the West Kunlun Orogen, China – Evidence from geochronology and geochemistry of the Arkarz pluton
چکیده انگلیسی


• The Arkarz pluton formed at late Triassic (~ 225 Ma).
• MMEs represent cumulates of common source with the host felsic magmas.
• Melting of remaining oceanic crust during collision produced the Arkarz pluton.
• Paleo-Tethys Ocean may have subducted southward in region of Sanshili to Subashi.

The West Kunlun orogenic belt (WKOB) at the northwest margin of the Greater Tibetan Plateau records seafloor subduction, ocean basin closing and continental collision with abundant syncollisional granitoids in response to the evolution of the Proto- and Paleo-Tethys Oceans from the early-Paleozoic to the Triassic. Here we present a combined study of detailed zircon U-Pb geochronology, whole-rock major and trace elements and Sr-Nd-Hf isotopic geochemistry on the syncollisional Arkarz (AKAZ) pluton with mafic magmatic enclaves (MMEs) exposed north of the Mazha-Kangxiwa suture (MKS) zone. The granitoid host rocks and MMEs of the AKAZ pluton give the same late Triassic age of ~ 225 Ma. The granitoid host rocks are metaluminous granodiorite and monzogranite. They have initial 87Sr/86Sr of 0.70818 to 0.70930, εNd(225 Ma) = − 4.61 to − 3.91 and εHf(225 Ma) = − 3.01 to 0.74. The MMEs are more mafic than the host with varying SiO2 (51.00–63.24 wt.%) and relatively low K2O (1.24–3.02 wt.%), but have similar Sr-Nd-Hf isotope compositions to the host ((87Sr/86Sr)i = 0.70830–0.70955, εNd(225 Ma) = − 4.88 to − 4.29, εHf(225 Ma) = − 2.57 to 0.25). Both the host and MMEs have rare earth element (REE) and trace element patterns resembling those of bulk continental crust (BCC). The MMEs most likely represent cumulate formed from common magmas parental to the granitoid host. The granitoid magmatism is best explained as resulting from melting of amphibolite of MORB protolith during continental collision, which produces andesitic melts with a remarkable compositional similarity to the BCC and the inherited mantle-like isotopic compositions. Simple isotopic mixing calculations suggest that ~ 80% ocean crust and ~ 20% continental materials contribute to the source of the AKAZ pluton. Thus, the hypothesis “continental collision zones as primary sites for net continental crust growth” is applicable in the WKOB as shown by studies in southern Tibet, East Kunlun and Qilian orogens. In addition, we also propose a new view for the tectonic evolution of the Paleo-Tethys Ocean in geological regions recorded and represented by the MKS.

ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Lithos - Volume 245, 15 February 2016, Pages 191–204
نویسندگان
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