{"title":"Zinc partitioning between mantle minerals and basaltic melts: Application to revisit the Zn/FeT redox proxy","authors":"Zhongxing Sun , Mingdi Gao , Xiaolin Xiong","doi":"10.1016/j.gca.2024.09.010","DOIUrl":null,"url":null,"abstract":"<div><div>Zn/Fe<sup>T</sup> (Fe<sup>T</sup>=Fe<sup>2+</sup> + Fe<sup>3+</sup>) ratios in primitive melts have been proposed as a redox proxy to assess the redox states of the upper mantle. However, to effectively use the melt Zn/Fe<sup>T</sup> ratio as a redox proxy, it is necessary to compare variations of melt Zn/Fe<sup>T</sup> ratios induced by changes in oxygen fugacity (<em>f</em>O<sub>2</sub>) with variations due to changes in Zn-Fe contents and mineralogy of the sources. Here we show that the melt Zn/Fe<sup>T</sup> ratio variation caused by <em>f</em>O<sub>2</sub> change can be expressed as Δ(Zn<sub>m</sub>/<span><math><msubsup><mtext>Fe</mtext><mrow><mtext>m</mtext></mrow><mtext>T</mtext></msubsup></math></span>) = (Zn<sub>per</sub>/<span><math><msubsup><mtext>Fe</mtext><mrow><mtext>per</mtext></mrow><mtext>T</mtext></msubsup></math></span>)* <span><math><mrow><mi>Δ</mi><mo>(</mo><msubsup><mrow><mi>F</mi><mi>e</mi></mrow><mrow><mi>m</mi></mrow><mrow><mn>2</mn><mo>+</mo></mrow></msubsup><mo>/</mo><msubsup><mrow><mi>F</mi><mi>e</mi></mrow><mrow><mi>m</mi></mrow><mi>T</mi></msubsup><mo>)</mo></mrow></math></span>/(<span><math><msubsup><mtext>D</mtext><mrow><mtext>Zn</mtext></mrow><mtext>per/m</mtext></msubsup></math></span>/<span><math><msubsup><mtext>D</mtext><mrow><msup><mrow><mtext>Fe</mtext></mrow><mtext>2+</mtext></msup></mrow><mtext>per/m</mtext></msubsup></math></span>). Zn/Fe<sup>T</sup> ratios in most arc and MORB peridotites (Zn<sub>per</sub>/<span><math><msubsup><mtext>Fe</mtext><mrow><mtext>per</mtext></mrow><mtext>T</mtext></msubsup></math></span>) are 9.0 ± 1.0*10<sup>−4</sup>, and melt Fe<sup>2+</sup>/Fe<sup>T</sup> ratio variation resulted from <em>f</em>O<sub>2</sub> change [<span><math><mrow><mi>Δ</mi><mo>(</mo><msubsup><mrow><mi>F</mi><mi>e</mi></mrow><mrow><mi>m</mi></mrow><mrow><mn>2</mn><mo>+</mo></mrow></msubsup><mo>/</mo><msubsup><mrow><mi>F</mi><mi>e</mi></mrow><mrow><mi>m</mi></mrow><mi>T</mi></msubsup><mo>)</mo></mrow></math></span>] can be easily obtained by the existing model. Hence, if the Zn and Fe<sup>2+</sup> partition coefficients (<span><math><msubsup><mtext>D</mtext><mrow><mtext>Zn</mtext></mrow><mtext>per/m</mtext></msubsup></math></span> and <span><math><msubsup><mtext>D</mtext><mrow><msup><mrow><mtext>Fe</mtext></mrow><mtext>2+</mtext></msup></mrow><mtext>per/m</mtext></msubsup></math></span>) between melt and peridotite are known, the melt Zn/Fe<sup>T</sup> ratio variation resulting from <em>f</em>O<sub>2</sub> change can be estimated. In this study, we determined D<sub>Zn</sub> between olivine, orthopyroxene, clinopyroxene and basaltic melts at 0.75–2.5 GPa and 1250–1450 ℃. Our data show that melt composition (expressed as MgO content) dominantly controls the mineral-melt Zn partitioning under peridotite melting conditions. These data, along with published mineral-melt <span><math><msub><mtext>D</mtext><msup><mrow><mtext>Fe</mtext></mrow><mtext>2+</mtext></msup></msub></math></span> data, enable us to calculate appropriate <span><math><msubsup><mtext>D</mtext><mrow><mtext>Zn</mtext></mrow><mtext>per/m</mtext></msubsup></math></span>/<span><math><msubsup><mtext>D</mtext><mrow><msup><mrow><mtext>Fe</mtext></mrow><mtext>2+</mtext></msup></mrow><mtext>per/m</mtext></msubsup></math></span>, which is 0.78 ± 0.02 under arc and MORB spinel peridotite melting conditions. Based on these parameters, the calculated average melt Zn/Fe<sup>T</sup> ratio variation caused by per log unity <em>f</em>O<sub>2</sub> change in typical <em>f</em>O<sub>2</sub> span of arc and MORB mantles is only ∼ 0.69 ± 0.20*10<sup>−4</sup>. Alternatively, melt Zn/Fe<sup>T</sup> ratio variations caused by changes in Zn-Fe contents and mineralogy of peridotites are ±1.10*10<sup>−4</sup>. These findings indicate that melt Zn/Fe<sup>T</sup> ratio variation induced by one log units <em>f</em>O<sub>2</sub> change is on the same order of magnitude as those caused by changes in Zn-Fe contents and mineralogy of peridotites. Therefore, unless the precise chemical and mineralogical compositions of the mantle sources can be determined independently, the melt Zn/Fe<sup>T</sup> redox proxy is unsuitable for tracing the mantle <em>f</em>O<sub>2</sub>. Our study, combined with recent works on melt Cu and V/Sc redox proxies, suggests that these redox proxies, previously considered as the strongest evidence for a reduced arc mantle, might not support the idea of a reduced arc mantle.</div></div>","PeriodicalId":327,"journal":{"name":"Geochimica et Cosmochimica Acta","volume":"385 ","pages":"Pages 141-155"},"PeriodicalIF":4.5000,"publicationDate":"2024-09-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Geochimica et Cosmochimica Acta","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0016703724004915","RegionNum":1,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
Zn/FeT (FeT=Fe2+ + Fe3+) ratios in primitive melts have been proposed as a redox proxy to assess the redox states of the upper mantle. However, to effectively use the melt Zn/FeT ratio as a redox proxy, it is necessary to compare variations of melt Zn/FeT ratios induced by changes in oxygen fugacity (fO2) with variations due to changes in Zn-Fe contents and mineralogy of the sources. Here we show that the melt Zn/FeT ratio variation caused by fO2 change can be expressed as Δ(Znm/) = (Znper/)* /(/). Zn/FeT ratios in most arc and MORB peridotites (Znper/) are 9.0 ± 1.0*10−4, and melt Fe2+/FeT ratio variation resulted from fO2 change [] can be easily obtained by the existing model. Hence, if the Zn and Fe2+ partition coefficients ( and ) between melt and peridotite are known, the melt Zn/FeT ratio variation resulting from fO2 change can be estimated. In this study, we determined DZn between olivine, orthopyroxene, clinopyroxene and basaltic melts at 0.75–2.5 GPa and 1250–1450 ℃. Our data show that melt composition (expressed as MgO content) dominantly controls the mineral-melt Zn partitioning under peridotite melting conditions. These data, along with published mineral-melt data, enable us to calculate appropriate /, which is 0.78 ± 0.02 under arc and MORB spinel peridotite melting conditions. Based on these parameters, the calculated average melt Zn/FeT ratio variation caused by per log unity fO2 change in typical fO2 span of arc and MORB mantles is only ∼ 0.69 ± 0.20*10−4. Alternatively, melt Zn/FeT ratio variations caused by changes in Zn-Fe contents and mineralogy of peridotites are ±1.10*10−4. These findings indicate that melt Zn/FeT ratio variation induced by one log units fO2 change is on the same order of magnitude as those caused by changes in Zn-Fe contents and mineralogy of peridotites. Therefore, unless the precise chemical and mineralogical compositions of the mantle sources can be determined independently, the melt Zn/FeT redox proxy is unsuitable for tracing the mantle fO2. Our study, combined with recent works on melt Cu and V/Sc redox proxies, suggests that these redox proxies, previously considered as the strongest evidence for a reduced arc mantle, might not support the idea of a reduced arc mantle.
期刊介绍:
Geochimica et Cosmochimica Acta publishes research papers in a wide range of subjects in terrestrial geochemistry, meteoritics, and planetary geochemistry. The scope of the journal includes:
1). Physical chemistry of gases, aqueous solutions, glasses, and crystalline solids
2). Igneous and metamorphic petrology
3). Chemical processes in the atmosphere, hydrosphere, biosphere, and lithosphere of the Earth
4). Organic geochemistry
5). Isotope geochemistry
6). Meteoritics and meteorite impacts
7). Lunar science; and
8). Planetary geochemistry.