温奇库姆地区tochilinite(碳酸盐和磁铁矿)同位素分析:CM母体早期水蚀变的温度约束

IF 2.4 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
M. D. Suttle, R. Findlay, I. A. Franchi, C. Biagioni, X. Zhao, F. A. J. Abernethy, L. Riches, L. Folco
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引用次数: 0

摘要

本文报道了CM球粒陨石(Winchcombe,岩性C [CM2.2/2.3])中tochilinite的首次氧同位素测量结果(δ17O: 11.0±2.1‰,δ18O: 23.5±4.0‰和Δ17O:−1.1±1.2‰)。我们分析了由假晶替代卡玛石而形成的i型透辉石-透辉石共生体(tci)。这些次级相与T1和T2方解石和磁铁矿一起在δ17O-δ18O同位素空间中定义了一条线性趋势线,斜率为0.50,略低于质量相关斜率(0.52)。这表明,除了主要的质量依赖分馏(由矿物特异性和温度依赖的平衡过程控制)外,富含16o的无水硅酸盐和缺乏16o的水之间的质量独立混合影响了蚀变流体Δ17O组成的演化。岩石学证据表明,tochilinite和T1方解石形成较早,在蚀变序列中关系密切。假设这些相之间的同位素平衡,我们估计地层温度约为135℃,δ18Owater值为28‰。这些发现与以前的热液合成实验相一致,强调了多相同位素测量对重建球粒质母体流体历史的价值。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Isotopic analysis of tochilinite (carbonate and magnetite) in Winchcombe: Temperature constraints on early-stage aqueous alteration in the CM parent body

Isotopic analysis of tochilinite (carbonate and magnetite) in Winchcombe: Temperature constraints on early-stage aqueous alteration in the CM parent body

We report the first oxygen isotope measurements of tochilinite (δ17O: 11.0 ± 2.1‰, δ18O: 23.5 ± 4.0‰ and Δ17O: −1.1 ± 1.2‰) in a CM chondrite (Winchcombe, lithology C [CM2.2/2.3]). We analyzed type-I tochilinite-cronstedtite intergrowths (TCIs)—formed by pseudomorphic replacement of kamacite. Alongside T1 and T2 calcite and magnetite, these secondary phases define a linear trendline in δ17O-δ18O isotope space with a slope of 0.50, slightly shallower than the mass-dependent slope (0.52). This demonstrates that, in addition to dominant mass-dependent fractionation (controlled by mineral-specific and temperature-dependent equilibrium processes), mass-independent mixing between 16O-rich anhydrous silicates, and 16O-poor water influenced the evolving Δ17O composition of alteration fluids. Petrographic evidence shows tochilinite and T1 calcite formed early and are closely associated in the alteration sequence. Assuming isotopic equilibrium between these phases, we estimate formation temperatures of approximately 135°C and a δ18Owater value of 28‰. These findings align with previous hydrothermal synthesis experiments and underscore the value of multi-phase isotopic measurements for reconstructing the fluid history of chondritic parent bodies.

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来源期刊
Meteoritics & Planetary Science
Meteoritics & Planetary Science 地学天文-地球化学与地球物理
CiteScore
3.90
自引率
31.80%
发文量
121
审稿时长
3 months
期刊介绍: First issued in 1953, the journal publishes research articles describing the latest results of new studies, invited reviews of major topics in planetary science, editorials on issues of current interest in the field, and book reviews. The publications are original, not considered for publication elsewhere, and undergo peer-review. The topics include the origin and history of the solar system, planets and natural satellites, interplanetary dust and interstellar medium, lunar samples, meteors, and meteorites, asteroids, comets, craters, and tektites. Our authors and editors are professional scientists representing numerous disciplines, including astronomy, astrophysics, physics, geophysics, chemistry, isotope geochemistry, mineralogy, earth science, geology, and biology. MAPS has subscribers in over 40 countries. Fifty percent of MAPS'' readers are based outside the USA. The journal is available in hard copy and online.
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