Magnesium and oxygen isotopes in Roberts Victor eclogites

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• 作者：Jin-Xiang Huang^a ; ^b ; ^{jinxiang.huang@mq.edu.au" class="auth_mail" title="E-mail the corresponding author} ; YuanXin Xiang^a ; Yajun An^c ; William L. Griffin^b ; Yoann Gré ; au^b ; Liewen Xie^a ; Norman J. Pearson^b ; Huimin Yu^c ; Suzanne Y. O'Reilly^b
• 关键词：Mg isotopes ; O isotopes ; Mantle metasomatism ; Eclogites ; Kaapvaal Craton
• 刊名：Chemical Geology
• 出版年：2016
• 出版时间：2 November 2016
• 年：2016
• 卷：438
• 期：Complete
• 页码：73-83
• 全文大小：1290 K

文摘

Magnesium and oxygen are critical elements in the solid Earth and hydrosphere. A better understanding of the combined behavior of Mg and O isotopes will refine their use as a tracer of geochemical processes and Earth evolution. In this study, the Mg-isotope compositions of garnet and omphacite separated from well-characterized xenolithic eclogites from the Roberts Victor kimberlite pipe (South Africa) have been measured by solution multi-collector ICP-MS. The reconstructed whole-rock δ²⁶Mg values of Type I (metasomatized) eclogites range from − 0.61‰ to − 0.20‰ (Type IA) and from − 0.60‰ to − 0.30‰ (Type IB) (mean − 0.43‰ ± 0.12‰), while δ²⁶Mg of Type IIA (fresh, least metasomatized) eclogites ranges from − 1.09‰ to − 0.17‰ (mean − 0.69‰ ± 0.41‰); a Type IIB (fresh, least metasomatized) has δ²⁶Mg of − 0.37‰. Oxygen-isotope compositions of garnet were analyzed in situ by SIMS (CAMECA 1280) and cross-checked by laser fluorination. Garnets have δ¹⁸O of 6.53‰ to 9.08‰ in Type IA, 6.14‰ to 6.65‰ in Type IB, and 2.34‰ to 2.91‰ in Type IIB. The variation of δ²⁶Mg and δ¹⁸O in Type IA and IB eclogites is consistent with the previously proposed model for the evolution of these samples, based on major and trace elements and radiogenic isotopes. In this model, the protoliths (Type II eclogites) were metasomatized by carbonatitic to kimberlitic melts/fluids to produce first Type IA eclogites and then Type IB. Metasomatism has changed the O-isotope compositions, but the Mg-isotope compositions of Type IA are mainly controlled by the protoliths; those of Type IB eclogites reflect mixing between the protoliths and the kimberlitic melt/fluid. The combination of a large range of δ²⁶Mg and low δ¹⁸O in Type II eclogites cannot be explained easily by seawater alteration of oceanic crust, interaction of carbonate/silicate sediments with oceanic crust, or partial melting of mafic rocks.