首页> 外文期刊>Journal of Petrology >Immiscible Transition from Carbonate-rich to Silicate-rich Melts in the 3 GPa Melting Interval of Eclogite + CO2 and Genesis of Silica-undersaturated Ocean Island Lavas
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Immiscible Transition from Carbonate-rich to Silicate-rich Melts in the 3 GPa Melting Interval of Eclogite + CO2 and Genesis of Silica-undersaturated Ocean Island Lavas

机译:榴辉岩和CO 2 3 GPa熔融区间从富碳酸盐熔体到富硅酸盐熔体的不混溶过渡和硅欠饱和海洋岛熔岩的成因

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摘要

We explore the partial melting behavior of a carbonated silica-deficient eclogite (SLEC1; 5 wt % CO2) from experiments at 3 GPa and compare the compositions of partial melts with those of alkalic and highly alkalic oceanic island basalts (OIBs). The solidus is located at 1050–1075 °C and the liquidus at ∼1415 °C. The sub-solidus assemblage consists of clinopyroxene, garnet, ilmenite, and calcio-dolomitic solid solution and the near solidus melt is carbonatitic (<2 wt % SiO2, <1 wt % Al2O3, and <0·1 wt % TiO2). Beginning at 1225 °C, a strongly silica-undersaturated silicate melt (∼34–43 wt % SiO2) with high TiO2 (up to 19 wt %) coexists with carbonate-rich melt (<5 wt % SiO2). The first appearance of carbonated silicate melt is ∼100 °C cooler than the expected solidus of CO2-free eclogite. In contrast to the continuous transition from carbonate to silicate melts observed experimentally in peridotite + CO2 systems, carbonate and silicate melt coexist over a wide temperature interval for partial melting of SLEC1 carbonated eclogite at 3 GPa. Silicate melts generated from SLEC1, especially at high melt fraction (>20 wt %), may be plausible sources or contributing components to melilitites and melilititic nephelinites from oceanic provinces, as they have strong compositional similarities including their SiO2, FeO*, MgO, CaO, TiO2 and Na2O contents, and CaO/Al2O3 ratios. Carbonated silicate partial melts from eclogite may also contribute to less extreme alkalic OIB, as these lavas have a number of compositional attributes, such as high TiO2 and FeO* and low Al2O3, that have not been observed from partial melting of peridotite ± CO2. In upwelling mantle, formation of carbonatite and silicate melts from eclogite and peridotite source lithologies occurs over a wide range of depths, producing significant opportunities for metasomatic transfer and implantation of melts.
机译:通过在3 GPa的实验中,我们探索了碳酸盐缺硅榴辉岩(SLEC1; 5 wt%CO 2 )的部分熔融行为,并比较了部分熔融物与碱度和强碱度海洋岛的成分玄武岩(OIBs)。固相线位于1050–1075°C,液相线位于〜1415°C。亚固相线组合由斜辉石,石榴石,钛铁矿和钙-白云岩固溶体组成,近固相线熔体是碳酸盐岩(<2 wt%SiO 2 ,<1 wt%Al 2 O 3 和<0·1 wt%TiO 2 )。从1225°C开始,与高TiO 2 (最高19 wt%)的强烈二氧化硅不足饱和的硅酸盐熔体(〜34–43 wt%SiO 2 )与富含碳酸盐的熔体(<5 wt%SiO 2 )。碳酸硅酸盐熔体的首次出现比不含CO 2 的榴辉石的预期固相线低约100°C。与在橄榄岩+ CO 2 系统中实验观察到的从碳酸盐到硅酸盐熔体的连续过渡相反,碳酸盐和硅酸盐熔体在3 GPa的部分熔融SLEC1碳酸榴辉岩的宽温度范围内共存。从SLEC1产生的硅酸盐熔体,特别是高熔体分数(> 20 wt%)时,可能是来自海洋省的硅镁土和银云母辉石的合理来源或贡献成分,因为它们具有强烈的成分相似性,包括SiO 2 ,FeO * ,MgO,CaO,TiO 2 和Na 2 O含量以及CaO / Al 2 O 3 比。榴辉岩中碳酸化的硅酸盐部分熔体也可能导致较弱的碱性OIB,因为这些熔岩具有许多组成属性,例如高TiO 2 和FeO * 和低Al橄榄岩±CO 2 的部分熔融尚未发现 2 O 3 。在地幔上升流中,由榴辉岩和橄榄岩源岩性形成的碳酸盐岩和硅酸盐熔岩在很宽的深度范围内发生,为熔体的交代转移和注入提供了重要机会。

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