Iron XANES measurements of carbonates and phyllosilicates in CM chondrites: A record of redox conditions during aqueous alteration

IF 2.4 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Elizabeth Bailey, Myriam Telus, Phoebe J. Lam, Samuel M. Webb
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Abstract

Multiple generations of calcite and dolomite precipitated in CM chondrites during ice melting events that led to episodes of liquid water. Models and laboratory analysis have suggested a long-term transition from oxidizing to reducing conditions during aqueous alteration on the CM parent body. We found that synchrotron X-ray absorption near edge spectroscopy (XANES) can detect relative differences in the oxidation state of trace iron within these carbonates. In CM chondrites, previous work interpreted Mn abundance in calcite as an indicator of relatively early or late formation, and dolomite is understood to form relatively late. In the CM1 chondrite Meteorite Hills 01070, XANES maps reveal that Mn-poor calcite contains more oxidized iron relative to Mn-rich calcite. While these measurements of carbonates support increasing iron reduction with progressive aqueous alteration in MET 01070, comparison among different CM chondrites suggests a complex picture of redox evolution. In addition to carbonates, we performed XANES measurements of the phyllosilicate-rich matrix of Allan Hills 83,100. Pre-edge centroid analysis indicates that this CM1/2 has an oxidation state similar to typical CM2 chondrites. While additional measurements are warranted to confirm the full span of redox trends in CM carbonates, our data do not support a correlation between redox state and petrologic type.

Abstract Image

CM球粒陨石中碳酸盐和层状硅酸盐的铁XANES测量:水蚀变期间氧化还原条件的记录
在导致液态水出现的冰融化事件中,多代方解石和白云石沉淀在CM球粒陨石中。模型和实验室分析表明,CM母体在含水蚀变过程中经历了从氧化到还原的长期转变。我们发现同步加速器x射线吸收近边光谱(XANES)可以检测到这些碳酸盐中微量铁氧化态的相对差异。在CM球粒陨石中,先前的工作将方解石中的Mn丰度解释为形成相对早或晚的指标,而白云岩则被认为形成相对晚。在CM1球粒陨石山01070中,XANES地图显示贫锰方解石比富锰方解石含有更多的氧化铁。虽然这些碳酸盐的测量结果支持MET 01070中随着水蚀变而增加的铁还原,但不同CM球粒陨石之间的比较表明了氧化还原演化的复杂图景。除了碳酸盐外,我们还对Allan Hills 83,100富含层状硅酸盐的基质进行了XANES测量。前边缘质心分析表明,CM2 /2具有与典型CM2球粒相似的氧化态。虽然需要额外的测量来确认CM碳酸盐的氧化还原趋势,但我们的数据并不支持氧化还原状态与岩石学类型之间的相关性。
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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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