Origin of the Site U1504 alkaline basalts in the South China Sea continental margin: Insights on deep mantle diversity and subduction dynamics under continental arcs

Liheng Sun, Yunying Zhang, Zhen Sun, Xiuquan Miao, Ruilong Li, Wanfeng Zhang
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Abstract

Alkaline basalts produced in continental arcs should contain information different from the arc tholeiite-calc-alkaline-series magmas, and their origin could provide unique constraints on deep mantle composition and material cycling. However, due to their sparse occurrence, alkaline basalts in continental arcs have not been studied thoroughly, which hinders our understanding of the mantle diversity and subduction dynamics under continental arcs. In this study, we present new 40Ar/39Ar ages, major and trace elements, and Sr-Nd-Hf isotopic data for the International Ocean Discovery Program Site U1504 alkaline basalts in the continental arc developed on the South China Block (SCB). These alkaline basalts were generated at ca. 121 Ma and display typical oceanic-island basalt geochemical characteristics. Their relatively high εNd(t) (3.5−3.7) and low (87Sr/86Sr)i (0.7034−0.7040) and La/Nb (0.5−1.0) values suggest that they were mainly derived from an asthenosphere mantle source. Compared to alkaline basalts in the SCB inland, U1504 alkaline basalts exhibit lower K2O/Na2O, Zr/Sm, Zr/Y, εNd(t), and εHf(t) values, indicating the addition of minor sub-continental lithospheric mantle. The enrichment of Nb, Ta, light rare earth elements, and slight depletion of Zr, Hf, and Ti, as well as elevated Fe/Mn and Sm/Yb and low CaO, indicate that their mantle lithology was mainly garnet pyroxenite. Based upon these findings and previous studies, the garnet pyroxenite was probably formed by the interaction of upwelling asthenosphere with slab edges in the scenario of break-off of the Paleo-Pacific Plate, and such interaction diversified the mantle chemistry beneath continental arcs. In conjunction with other reported alkaline basalt data, it is proposed that the enriched asthenosphere mantle beneath the SCB had formed sequentially from inland to coastal since the late Mesozoic, and this may be related to lateral and vertical flow in the deep asthenosphere controlled by the break-off of subducted plates.
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中国南海大陆边缘U1504地块碱性玄武岩的起源:对大陆弧下深部地幔多样性和俯冲动力学的启示
大陆弧中产生的碱性玄武岩应该包含有别于弧内透辉石-钙-碱性系列岩浆的信息,它们的起源可以为深部地幔成分和物质循环提供独特的约束。然而,由于大陆弧中的碱性玄武岩分布稀少,对它们的研究并不深入,这阻碍了我们对大陆弧下地幔多样性和俯冲动力学的了解。本研究提供了国际大洋发现计划U1504站点碱性玄武岩的40Ar/39Ar年龄、主要元素、痕量元素和Sr-Nd-Hf同位素数据。121Ma,具有典型的大洋岛弧玄武岩地球化学特征。它们相对较高的εNd(t) (3.5-3.7)和较低的(87Sr/86Sr)i (0.7034-0.7040)和La/Nb (0.5-1.0)值表明它们主要来源于星体地幔。与SCB内陆地区的碱性玄武岩相比,U1504碱性玄武岩的K2O/Na2O、Zr/Sm、Zr/Y、εNd(t)和εHf(t)值均较低,表明其中含有少量次大陆岩石圈地幔。Nb、Ta和轻稀土元素的富集,Zr、Hf和Ti的轻微贫化,以及Fe/Mn和Sm/Yb的升高和CaO的降低,表明它们的地幔岩性主要是石榴石辉石。根据这些发现和以往的研究,石榴石辉石可能是在古太平洋板块断裂的情况下,上涌的星体层与板块边缘相互作用形成的,这种相互作用使大陆弧下的地幔化学成分多样化。结合其他报道的碱性玄武岩数据,提出南中生代晚期以来,南中生界下的富集星体层地幔是由内陆向沿岸依次形成的,这可能与俯冲板块断裂控制的深部星体层横向和纵向流动有关。
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