M. Chaussidon, Z. Deng, J. Villeneuve, J. Moureau, B. Watson, F. Richter, F. Moynier
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引用次数: 16
Abstract
Isotopic variation for traditional elements (H, C, N, O and S) has been widely used in the past 40 years in Earth and planetary sciences to study many processes with an emphasis on environments where fluids are present (e.g., Valley and Cole 2011). More recent developments have allowed high-precision measurements of isotope ratios of what has been called non-traditional elements (i.e., Mg, Si, Fe, Zn, Cu, Mo), which are usually less fractionated than traditional elements by at least an order of magnitude (see this volume). These non-traditional stable isotopes can give insights on processes where fluids are not present (e.g., metal–silicate fractionation, e.g., Georg et al. 2007 and review by Poitrasson et al. 2017, this volume), evaporation processes during planetary formation (e.g., Paniello et al. 2012, Wang and Jacobsen 2016, and review by Moynier et al. 2017 this volume), igneous differentiation (e.g., Williams et al. 2009; Sossi et al. 2012; and review by Dauphas et al. 2017, this volume), and on biological processes (e.g., Walczyk and von Blanckenburg 2002, and review by Albarede et al. 2017 this volume). Among all these non-traditional isotopic systems, Mg isotopes are of major importance because (i) Mg is a major constituent of the silicate portion of planetary bodies, (ii) Mg has more than two isotopes (24Mg, 25Mg and 26Mg) allowing to study processes leading to various types of mass fractionation (Young et al. 2002; Young and Galy 2004; Davis et al. 2015) and (iii) 26Mg excesses produced by the radioactive decay of short-lived 26Al (T1/2=0.73 Ma) (Lee et al. 1976) are a key tool for early Solar system chronology (see reviews by Dauphas and Chaussidon 2011; Chaussidon and Liu 2015). Note that in addition, significant Mg isotopic …
过去40年来,传统元素(氢、碳、氮、氧和硫)的同位素变化在地球和行星科学中被广泛用于研究许多过程,重点是流体存在的环境(例如,Valley和Cole, 2011年)。最近的发展已经允许对所谓的非传统元素(即Mg、Si、Fe、Zn、Cu、Mo)的同位素比率进行高精度测量,这些元素通常比传统元素的分异程度至少低一个数量级(见本卷)。这些非传统稳定同位素可以深入了解流体不存在的过程(例如,金属硅酸盐分选,例如,Georg等人,2007年和Poitrasson等人,2017年,本卷),行星形成过程中的蒸发过程(例如,Paniello等人,2012年,Wang和Jacobsen 2016年,Moynier等人,2017年,本卷),火成岩分异(例如,Williams等人,2009;Sossi et al. 2012;并由Dauphas等人审查。2017年,本卷),以及生物过程(例如,Walczyk和von Blanckenburg 2002年,以及Albarede等人审查。2017年,本卷)。在所有这些非传统同位素系统中,Mg同位素非常重要,因为(i) Mg是行星体硅酸盐部分的主要成分,(ii) Mg有两种以上的同位素(24Mg, 25Mg和26Mg),允许研究导致各种类型质量分拣的过程(Young等人,2002;Young and Galy 2004;Davis et al. 2015)和(iii)由短寿命26Al的放射性衰变产生的26Mg过量(T1/2=0.73 Ma) (Lee et al. 1976)是早期太阳系年代学的关键工具(见Dauphas和Chaussidon 2011年的评论;Chaussidon and Liu 2015)。注意,另外,显著的Mg同位素…
期刊介绍:
RiMG is a series of multi-authored, soft-bound volumes containing concise reviews of the literature and advances in theoretical and/or applied mineralogy, crystallography, petrology, and geochemistry. The content of each volume consists of fully developed text which can be used for self-study, research, or as a text-book for graduate-level courses. RiMG volumes are typically produced in conjunction with a short course but can also be published without a short course. The series is jointly published by the Mineralogical Society of America (MSA) and the Geochemical Society.