Petrogenesis of early Paleozoic syn-collisional granitoids and enclaves in Western Kunlun, Northwest China: Implications for the growth of continental crust

The Western Kunlun Orogenic Belt (WKOB), along the northwestern margin of the Qinghai–Xizang Plateau, was formed by the collision of Gondwana-derived terranes to the south and the Tarim Block to the north and was closely associated with closure of the Proto-Tethys Ocean during the late Neoproterozoic to early Paleozoic. We present a combined zircon U Pb geochronology , whole-rock composition, and Sr–Nd–Hf isotopic study of syn-collisional granitoid plutons and mafic microgranular enclaves (MMEs) in the region. Zircon U Pb dating yields ages of 443.8 ± 4.4, 451.9 ± 4.2, 462.9 ± 3.5, and 456 ± 4.2 Ma for the Tongayoupuagezi, Shanjie, and Pishigai plutons and MMEs from the Pishigai pluton, respectively. The granitoids are metaluminous to weakly peraluminous (A/CNK = 1.00–1.17) and belong to the high-K calc-alkaline series. They have ( 87 Sr/ 86 Sr) i ratios of 0.7058–0.7154, ε Nd (t) values of −8.78 to −0.93, and ε Hf (t) values of −19.72 to +6.87. The MMEs have variable SiO 2 contents (45.7–60.2 wt%) and are more mafic than the host granitoids, but have similar Sr–Nd–Hf isotopic compositions to the host granitoids [( 87 Sr/ 86 Sr) i = 0.7102–0.7110; ε Nd (t) = −6.57 to −3.56; ε Hf (t) = −7.17 to −1.81]. The MMEs are fragments of cumulates formed during the early stages of magma evolution . The granitoids were produced by the partial melting of a mélange source. The new data support the view that the Middle–Late Ordovician syn-collisional granitoids with MMEs distributed along the WKOB represent a magmatic response to terrane collision. This suggests that juvenile crustal growth in older orogenic systems, which occurs by arc addition, also involves some vertical addition during the final stage of orogenic collision. Our study suggests that mélange diaper melting is a key mechanism of crustal growth during the syn-collision stage in continental collision zones, associated with slab breakoff. • The MMEs are the fragments of cumulate formed in the early stage of magma evolution. • The granitoids were produced by the partial melting of mélange source. • The mélange diaper melting may have acted as a leading mechanism for crustal growth.

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Publication Details

Journal
Lithos
Published
2024-10-24
DOI
https://doi.org/10.1016/j.lithos.2024.107844
Citations
2
Primary Topic
Geological and Geochemical Analysis
Type
article
Field-Weighted Citation Impact
1.07
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article

Petrogenesis of early Paleozoic syn-collisional granitoids and enclaves in Western Kunlun, Northwest China: Implications for the growth of continental crust

Xin Wang, Qichao Zhang, Yu Zhang
2 citations
Lithos
Geological and Geochemical Analysis
1.07
article

Petrogenesis of early Paleozoic syn-collisional granitoids and enclaves in Western Kunlun, Northwest China: Implications for the growth of continental crust

Xin Wang, Qichao Zhang, Yu Zhang
article en
2 citations

Abstract

The Western Kunlun Orogenic Belt (WKOB), along the northwestern margin of the Qinghai–Xizang Plateau, was formed by the collision of Gondwana-derived terranes to the south and the Tarim Block to the north and was closely associated with closure of the Proto-Tethys Ocean during the late Neoproterozoic to early Paleozoic. We present a combined zircon U Pb geochronology , whole-rock composition, and Sr–Nd–Hf isotopic study of syn-collisional granitoid plutons and mafic microgranular enclaves (MMEs) in the region. Zircon U Pb dating yields ages of 443.8 ± 4.4, 451.9 ± 4.2, 462.9 ± 3.5, and 456 ± 4.2 Ma for the Tongayoupuagezi, Shanjie, and Pishigai plutons and MMEs from the Pishigai pluton, respectively. The granitoids are metaluminous to weakly peraluminous (A/CNK = 1.00–1.17) and belong to the high-K calc-alkaline series. They have ( 87 Sr/ 86 Sr) i ratios of 0.7058–0.7154, ε Nd (t) values of −8.78 to −0.93, and ε Hf (t) values of −19.72 to +6.87. The MMEs have variable SiO 2 contents (45.7–60.2 wt%) and are more mafic than the host granitoids, but have similar Sr–Nd–Hf isotopic compositions to the host granitoids [( 87 Sr/ 86 Sr) i = 0.7102–0.7110; ε Nd (t) = −6.57 to −3.56; ε Hf (t) = −7.17 to −1.81]. The MMEs are fragments of cumulates formed during the early stages of magma evolution . The granitoids were produced by the partial melting of a mélange source. The new data support the view that the Middle–Late Ordovician syn-collisional granitoids with MMEs distributed along the WKOB represent a magmatic response to terrane collision. This suggests that juvenile crustal growth in older orogenic systems, which occurs by arc addition, also involves some vertical addition during the final stage of orogenic collision. Our study suggests that mélange diaper melting is a key mechanism of crustal growth during the syn-collision stage in continental collision zones, associated with slab breakoff. • The MMEs are the fragments of cumulate formed in the early stage of magma evolution. • The granitoids were produced by the partial melting of mélange source. • The mélange diaper melting may have acted as a leading mechanism for crustal growth.

LithosVol. 488-489
Guangxi University (CN), Chinese Academy of Geological Sciences (CN)
Openalex Percentile: Top 24%
Geological and Geochemical Analysis
1.07
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