Tissintite-II in lunar meteorite Northwest Africa 13967: Implications for the high pressure/temperature mineralogy of the lunar regolith

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Axel Wittmann, Christian R. Kroemer, Meenakshi Wadhwa, Thomas G. Sharp, Matthijs Van Soest, Trevor Martin, Tyler Goepfert
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Abstract

We studied lunar regolith breccia meteorite Northwest Africa (NWA) 13967 to explore its mineral and clast inventory with special focus on the ubiquitous occurrence of tissintite-II, a newly recognized, vacancy-rich high-pressure clinopyroxene with a feldspathic, Fe- and Mg-enriched composition. Lithic clasts in NWA 13967 indicate a provenance in the Feldspathic Highlands Terrane on the Moon. Most abundant are cumulate impact melt clasts (“poikilitic granulitic breccias”), granular impact melt rocks, vitric impact melt clasts including impact spherules, and anorthositic clasts, while basalt clasts are rare. The breccia groundmass is mostly fused to flow-textured, vesicular, crystallized impact melt that includes 1 μm corundum crystals and up to 5 μm tissintite-II near the contact with lithic clasts. Rare coesite occurs in moganite clasts entrained in the shock-melted groundmass and rimmed by tissintite-II. Petrographic features of NWA 13967 and its bulk rock chemical composition are most similar to the NWA 8046 clan of lunar meteorites, the largest known lunar meteorite. We discuss mineralogical and petrological characteristics of NWA 13967 to unravel chemical and structural changes of the lunar regolith during shock lithification, which may inform the ongoing exploration of the lunar surface.

西北非洲13967月球陨石中的tissinite - ii:对月球风化层高压/高温矿物学的影响
我们研究了西北非洲(NWA) 13967月球风化角砾岩陨石,以探索其矿物和碎屑储量,特别关注其普遍存在的组织石- ii,这是一种新发现的富含空位的高压斜辉石,具有长石,富含铁和镁的成分。NWA 13967的岩屑表明其来源为月球上的长石高地地质体。最丰富的是堆积性撞击熔体碎屑(“似硅质粒质角砾岩”)、粒状撞击熔体岩、玻璃状撞击熔体碎屑(包括撞击球粒)和斜长岩碎屑,玄武岩碎屑较少。角砾岩地块在与岩屑接触处主要熔融为流织构、水泡状结晶的冲击熔体,其中包括1 μm刚玉晶体和高达5 μm的组织石- ii。罕见的柯石英发生在moganite碎屑在shock-melted携入的基质,tissintite-II形成边缘。NWA 13967的岩石学特征及其整体岩石化学成分与已知最大的月球陨石NWA 8046族最为相似。通过对NWA 13967的矿物学和岩石学特征的研究,揭示了冲击岩化过程中月球风化层的化学和结构变化,为后续的月球表面探测提供了理论依据。
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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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