西北非洲16788:已知最大的单个火星陨石——一种新的橄榄石微辉长辉长岩及其对火星岩浆作用的影响

IF 4 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Xhonatan Shehaj, Giovanni Pratesi, Cristian Carli, Riccardo Avanzinelli, Alice Stephant, Annarita Franza, Eleonora Ammannito
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引用次数: 0

摘要

我们对2023年7月在撒哈拉沙漠发现的一颗新的火星陨石西北非洲(NWA) 16788进行了全面研究。这个标本构成了已知的最大的火星陨石,总重量为⁓25公斤。详细的矿物学和地球化学调查表明,NWA 16788为富集橄榄石微辉长岩辉长岩。岩石学分析显示其为毫米级的堆积结构,介于辉长岩和辉长岩之间,主要由辉长岩(⁓61 vol.%)、闪长岩(⁓21 vol.%)和橄榄石(⁓15 vol.%)组成。辉石颗粒表现出独特的分区模式,将NWA 16788放置在一小群火星陨石和月球样本中,这些陨石和月球样本记录了独特的冷却历史,这表明类似的样本在火星火成岩中可能比之前认识到的更普遍。高精度的143Nd/144Nd和87Sr/86Sr同位素组成分析,结合微量元素丰度,表明NWA 16788起源于一个富集的火星地幔源的部分熔融。电子后向散射衍射分析显示橄榄石晶粒取向偏差呈单峰分布,平均为⁓4.6°,与高能单次撞击事件相一致。此外,在NWA 16788上获得的可见光和近红外光谱数据可以帮助确定火星表面类似火成岩的潜在位置。最后,基于火星探测器的数据,本研究提出了对目前火星陨石分类方案的改进,旨在减少分类歧义,改善火星陨石和火星火成岩之间的排列。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Northwest Africa 16788: The Largest Known Individual Martian Meteorite—A New Olivine Microgabbroic Shergottite and Its Implications for Martian Magmatism

Northwest Africa 16788: The Largest Known Individual Martian Meteorite—A New Olivine Microgabbroic Shergottite and Its Implications for Martian Magmatism

Northwest Africa 16788: The Largest Known Individual Martian Meteorite—A New Olivine Microgabbroic Shergottite and Its Implications for Martian Magmatism

Northwest Africa 16788: The Largest Known Individual Martian Meteorite—A New Olivine Microgabbroic Shergottite and Its Implications for Martian Magmatism

Northwest Africa 16788: The Largest Known Individual Martian Meteorite—A New Olivine Microgabbroic Shergottite and Its Implications for Martian Magmatism

We present a comprehensive study of a new Martian meteorite, Northwest Africa (NWA) 16788, found in the Sahara Desert in July 2023. This specimen constitutes the largest known individual meteorite of Martian origin, with a total weight of ⁓25 kg. A detailed mineralogical and geochemical investigation identifies NWA 16788 as an enriched olivine microgabbroic shergottite. Petrographic analysis reveals a millimeter-sized cumulate texture, which is intermediate between poikilitic and gabbroic shergottites, primarily composed of pyroxene (⁓61 vol.%), maskelynite (shocked plagioclase, ⁓21 vol.%), and olivine (⁓15 vol.%). Pyroxene grains exhibit a distinctive zoning pattern, placing NWA 16788 within a small group of Martian meteorites and lunar samples that record unique cooling histories, suggesting that similar samples may be more prevalent within the Martian igneous rocks than previously recognized. High-precision analyses of bulk 143Nd/144Nd and 87Sr/86Sr isotopic composition, combined with trace element abundance, indicate that NWA 16788 originated from the partial melting of an enriched Martian mantle source. Electron backscatter diffraction analysis reveals a unimodal distribution of olivine grain misorientation, averaging ⁓4.6°, consistent with a high-energy single-impact event. Moreover, visible and near-infrared spectroscopy data acquired on NWA 16788 could aid in identifying potential locations of analogous igneous rocks on the Martian surface. Finally, this study proposes refinements to the current classification scheme of Martian meteorites, aiming to reduce taxonomic ambiguity and improve the alignment between Martian meteorites and Martian igneous rocks, based on data from Mars rovers.

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来源期刊
Journal of Geophysical Research: Planets
Journal of Geophysical Research: Planets Earth and Planetary Sciences-Earth and Planetary Sciences (miscellaneous)
CiteScore
8.00
自引率
27.10%
发文量
254
期刊介绍: The Journal of Geophysical Research Planets is dedicated to the publication of new and original research in the broad field of planetary science. Manuscripts concerning planetary geology, geophysics, geochemistry, atmospheres, and dynamics are appropriate for the journal when they increase knowledge about the processes that affect Solar System objects. Manuscripts concerning other planetary systems, exoplanets or Earth are welcome when presented in a comparative planetology perspective. Studies in the field of astrobiology will be considered when they have immediate consequences for the interpretation of planetary data. JGR: Planets does not publish manuscripts that deal with future missions and instrumentation, nor those that are primarily of an engineering interest. Instrument, calibration or data processing papers may be appropriate for the journal, but only when accompanied by scientific analysis and interpretation that increases understanding of the studied object. A manuscript that describes a new method or technique would be acceptable for JGR: Planets if it contained new and relevant scientific results obtained using the method. Review articles are generally not appropriate for JGR: Planets, but they may be considered if they form an integral part of a special issue.
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