{"title":"大陆深俯冲期间壳幔相互作用:来自东昆仑造山带碰撞后基性火成岩轻Mo同位素的证据","authors":"Qing-Chen Yang, Wei Fang, Li-Qun Dai, Li-Tao Ma, Zi-Fu Zhao","doi":"10.1029/2025GC012451","DOIUrl":null,"url":null,"abstract":"<p>It is intriguing whether and how crust-mantle interaction would proceed in continental subduction zones. Here, we report zircon U-Pb ages and Hf isotopes, major and trace elements, and Sr-Nd-Mo isotopes for Late Paleozoic mafic igneous rocks from the East Kunlun orogen (EKO). Zircon U–Pb dating of these rocks yields concordant ages of 384–387 Ma, corresponding to post-collisional magmatism in the EKO. The mafic rocks are characterized by arc-type trace element distribution patterns and slightly enriched Sr-Nd isotopes, indicating their derivation from a fertile mantle source with the involvement of crustal material. Their high Th/La ratios (0.28–0.77) are inconsistent with the recycling of typical oceanic crust but can be related to continental crust-derived melts with residual allanite during crustal anatexis. This is further strengthened by the similarity in Sr-Nd isotopes and zircon Hf isotopes between these mafic rocks and gneiss that represent ancient continental crustal components in the EKO. Notably, the post-collisional mafic rocks have variably low δ<sup>98</sup>Mo values of −0.64‰ to −0.07‰. Combined with the enriched Sr-Nd isotopes and high Th/La features, it is inferred that the light Mo isotopic signatures are inherited from the deeply subducted continental crust. Given that continental crust is generally characterized by high δ<sup>98</sup>Mo values of 0.10–0.40‰, the light Mo isotope compositions of the mafic rocks should be inherited from the previously dehydrated continental crust-derived melts. Our study highlights that the light Mo isotope features can be used to decipher the recycling of continental crust in collisional orogens.</p>","PeriodicalId":50422,"journal":{"name":"Geochemistry Geophysics Geosystems","volume":"26 8","pages":""},"PeriodicalIF":3.0000,"publicationDate":"2025-08-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://agupubs.onlinelibrary.wiley.com/doi/epdf/10.1029/2025GC012451","citationCount":"0","resultStr":"{\"title\":\"Crust-Mantle Interaction During Continental Deep Subduction: Evidence From Light Mo Isotopes in Post-Collisional Mafic Igneous Rocks From the East Kunlun Orogen\",\"authors\":\"Qing-Chen Yang, Wei Fang, Li-Qun Dai, Li-Tao Ma, Zi-Fu Zhao\",\"doi\":\"10.1029/2025GC012451\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>It is intriguing whether and how crust-mantle interaction would proceed in continental subduction zones. Here, we report zircon U-Pb ages and Hf isotopes, major and trace elements, and Sr-Nd-Mo isotopes for Late Paleozoic mafic igneous rocks from the East Kunlun orogen (EKO). Zircon U–Pb dating of these rocks yields concordant ages of 384–387 Ma, corresponding to post-collisional magmatism in the EKO. The mafic rocks are characterized by arc-type trace element distribution patterns and slightly enriched Sr-Nd isotopes, indicating their derivation from a fertile mantle source with the involvement of crustal material. Their high Th/La ratios (0.28–0.77) are inconsistent with the recycling of typical oceanic crust but can be related to continental crust-derived melts with residual allanite during crustal anatexis. This is further strengthened by the similarity in Sr-Nd isotopes and zircon Hf isotopes between these mafic rocks and gneiss that represent ancient continental crustal components in the EKO. Notably, the post-collisional mafic rocks have variably low δ<sup>98</sup>Mo values of −0.64‰ to −0.07‰. Combined with the enriched Sr-Nd isotopes and high Th/La features, it is inferred that the light Mo isotopic signatures are inherited from the deeply subducted continental crust. Given that continental crust is generally characterized by high δ<sup>98</sup>Mo values of 0.10–0.40‰, the light Mo isotope compositions of the mafic rocks should be inherited from the previously dehydrated continental crust-derived melts. Our study highlights that the light Mo isotope features can be used to decipher the recycling of continental crust in collisional orogens.</p>\",\"PeriodicalId\":50422,\"journal\":{\"name\":\"Geochemistry Geophysics Geosystems\",\"volume\":\"26 8\",\"pages\":\"\"},\"PeriodicalIF\":3.0000,\"publicationDate\":\"2025-08-15\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://agupubs.onlinelibrary.wiley.com/doi/epdf/10.1029/2025GC012451\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Geochemistry Geophysics Geosystems\",\"FirstCategoryId\":\"89\",\"ListUrlMain\":\"https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2025GC012451\",\"RegionNum\":2,\"RegionCategory\":\"地球科学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"GEOCHEMISTRY & GEOPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Geochemistry Geophysics Geosystems","FirstCategoryId":"89","ListUrlMain":"https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2025GC012451","RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
Crust-Mantle Interaction During Continental Deep Subduction: Evidence From Light Mo Isotopes in Post-Collisional Mafic Igneous Rocks From the East Kunlun Orogen
It is intriguing whether and how crust-mantle interaction would proceed in continental subduction zones. Here, we report zircon U-Pb ages and Hf isotopes, major and trace elements, and Sr-Nd-Mo isotopes for Late Paleozoic mafic igneous rocks from the East Kunlun orogen (EKO). Zircon U–Pb dating of these rocks yields concordant ages of 384–387 Ma, corresponding to post-collisional magmatism in the EKO. The mafic rocks are characterized by arc-type trace element distribution patterns and slightly enriched Sr-Nd isotopes, indicating their derivation from a fertile mantle source with the involvement of crustal material. Their high Th/La ratios (0.28–0.77) are inconsistent with the recycling of typical oceanic crust but can be related to continental crust-derived melts with residual allanite during crustal anatexis. This is further strengthened by the similarity in Sr-Nd isotopes and zircon Hf isotopes between these mafic rocks and gneiss that represent ancient continental crustal components in the EKO. Notably, the post-collisional mafic rocks have variably low δ98Mo values of −0.64‰ to −0.07‰. Combined with the enriched Sr-Nd isotopes and high Th/La features, it is inferred that the light Mo isotopic signatures are inherited from the deeply subducted continental crust. Given that continental crust is generally characterized by high δ98Mo values of 0.10–0.40‰, the light Mo isotope compositions of the mafic rocks should be inherited from the previously dehydrated continental crust-derived melts. Our study highlights that the light Mo isotope features can be used to decipher the recycling of continental crust in collisional orogens.
期刊介绍:
Geochemistry, Geophysics, Geosystems (G3) publishes research papers on Earth and planetary processes with a focus on understanding the Earth as a system. Observational, experimental, and theoretical investigations of the solid Earth, hydrosphere, atmosphere, biosphere, and solar system at all spatial and temporal scales are welcome. Articles should be of broad interest, and interdisciplinary approaches are encouraged.
Areas of interest for this peer-reviewed journal include, but are not limited to:
The physics and chemistry of the Earth, including its structure, composition, physical properties, dynamics, and evolution
Principles and applications of geochemical proxies to studies of Earth history
The physical properties, composition, and temporal evolution of the Earth''s major reservoirs and the coupling between them
The dynamics of geochemical and biogeochemical cycles at all spatial and temporal scales
Physical and cosmochemical constraints on the composition, origin, and evolution of the Earth and other terrestrial planets
The chemistry and physics of solar system materials that are relevant to the formation, evolution, and current state of the Earth and the planets
Advances in modeling, observation, and experimentation that are of widespread interest in the geosciences.