New insights into deep carbon recycling and formation of nepheline-bearing alkaline rocks from Sr-Nd-Mg isotope compositions

GSA Bulletin Pub Date : 2022-10-19 DOI:10.1130/b36555.1
Weiliang Kong, Zhaochong Zhang, Dongyang Zhang, Changhong Wang, M. Santosh, Bingxiang Liu, Bowen Wei
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Abstract

Magnesium isotopes are widely used to trace recycled carbonates in the mantle source. We recently recognized extremely light Mg isotope values (δ26Mg = −0.50 to −0.62‰) in nepheline syenites in the Tarim large igneous province (TLIP), NW China. To evaluate the significance of the light Mg isotopes, we conducted petrological, mineral chemical, zircon U-Pb ages, and geochemical and isotopes (Sr-Nd-Mg) analyses on the nepheline syenite to understand its petrogenesis. Laser ablation−inductively coupled plasma−mass spectrometry zircon U-Pb dating yields an age of 272.5 ± 1.4 Ma for the nepheline syenite. Petrographic and geochemical studies show that the nepheline syenite and nephelinite in the TLIP display similar mineral assemblages, clinopyroxene Sr isotope compositions and bulk-rock Sr and Nd isotope compositions (87Sr/86Sr(i) = 0.70364−0.70399, εNd(t) = +3.51 to +4.49 versus 87Sr/86Sr(i) = 0.70348−0.70371, εNd(t) = +3.28 to +3.88 for nepheline syenite and nephelinite, respectively), indicating they are possibly co-magmatic. Rhyolite-MELTS modeling shows that the nepheline syenite formed from nephelinite by fractional crystallization of spinel, olivine, clinopyroxene, apatite, and biotite. In combination with information from previous studies, we correlated the extremely light magnesium isotopes of nepheline syenite to “genetic genes” of nephelinite (δ26Mg = −0.35 to −0.55‰) which were produced by the reaction between peridotite and carbonated silicate melt derived from the carbonated eclogite. We invoke a three-stage model for the genesis of the nepheline syenite in the TLIP. Initially, the subduction of oceanic crust delivered the sedimentary carbonate rocks into the deep mantle and formed carbonated eclogite. The carbonated silicate melt derived by the melting of the carbonated eclogite reacted with ambient peridotite to form primary nephelinitic magma. Finally, fractional crystallization of nephelinitic melt during ascent produced the nepheline syenite. Our study provides insights into the implication of light magnesium isotopes for deep carbon recycling in the origin of alkaline rocks.
Sr-Nd-Mg同位素组成对含石榴石碱性岩深部碳循环和形成的新认识
镁同位素被广泛用于追踪地幔源中的再生碳酸盐。最近在塔里木大火成岩省(TLIP)的霞石正长岩中发现了极轻的Mg同位素值(δ26Mg = - 0.50 ~ - 0.62‰)。为了评价轻Mg同位素的意义,我们对霞石正长岩进行了岩石学、矿物化学、锆石U-Pb年龄、地球化学和同位素(Sr-Nd-Mg)分析,以了解其岩石成因。激光烧蚀-电感耦合等离子体-质谱法锆石U-Pb测年结果显示霞石正长岩的年龄为272.5±1.4 Ma。岩石学和地球化学研究表明,该区霞石正长岩和闪辉岩具有相似的矿物组合,斜辉石Sr同位素组成和块状岩石Sr和Nd同位素组成(87Sr/86Sr(i) = 0.70364 ~ 0.70399, εNd(t) = +3.51 ~ +4.49,而霞石正长岩和闪辉岩的εNd(t)分别= 0.70348 ~ 0.70371,εNd(t) = +3.28 ~ +3.88),表明两者可能为共岩浆作用。流纹石-熔体模拟表明,由尖晶石、橄榄石、斜辉石、磷灰石和黑云母分馏结晶而成的霞石正长岩。结合前人研究资料,将霞石正长岩极轻镁同位素与霞石岩的“成因基因”(δ26Mg = - 0.35‰~ - 0.55‰)进行了关联,这些基因是由碳酸化榴辉岩中的橄榄岩与碳酸化硅酸盐熔体反应产生的。我们提出了一个三阶段模型来解释该区霞石正长岩的成因。最初,洋壳的俯冲作用使沉积碳酸盐岩进入深部地幔,形成碳酸榴辉岩。碳酸化榴辉岩熔融后产生的碳酸化硅酸盐熔体与周围的橄榄岩反应形成原生辉石岩浆。最后,上升过程中霞石熔体的分离结晶形成霞石正长岩。我们的研究揭示了轻镁同位素对碱性岩石深部碳循环的意义。
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