Textural coarsening as the cause for impact-melt like plagioclase crystal size distributions and subtle layering in high-Al basalt 14053

IF 2.4 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Stu Webb, Clive R. Neal, Bridget Guiza, James M. D. Day
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引用次数: 0

Abstract

High-Al Apollo 14 basalt 14053 has been identified as an endogenous partial melt product from the lunar interior based on geochemical analyses, specifically low abundances of highly siderophile elements, but exhibits textural characteristics similar to those of impact melts. Prior studies of this sample have described mineralogical differences between “interior” and “exterior” portions, which have been attributed to exposure at the lunar surface and subsequent metamorphism through subsolidus reheating within or in proximity to an impact-ejecta blanket. It has been demonstrated that quantitative textural analysis is a useful tool for distinguishing between lunar rocks altered by impact processes and those produced by endogenic magmatic processes. Such an approach is used in this study to analyze multiple thin sections cut from interior and exterior portions of 14053. The textural heterogeneity of plagioclase crystals among thin sections revealed in this study suggests that an impact-ejecta blanket likely impinged on the western side of 14053. This thermal metamorphism coarsened the plagioclase grains within that portion of 14053 so intensely that components diffused to form subtle layering and moderate textural heterogeneity that was quantifiable. These results also support previous conclusions that suggest the differences in reduction textures within this sample are due to the limited penetration depth of solar-wind implanted hydrogen prior to reheating. Thermal metamorphism can produce textural changes in lunar samples even if below the solidus temperature, such that the plagioclase texture of an endogenous basalt is sufficiently altered to that resembling an impact melt. These results highlight the significance of quantitative petrographic observations of lunar samples to reveal important petrogenetic information that has to be placed in proper spatial context to be understood.

Abstract Image

高铝玄武岩14053中冲击熔体样斜长石晶粒尺寸分布和细微分层的织构粗化原因
基于地球化学分析,高铝阿波罗14号玄武岩14053被确定为来自月球内部的内生部分熔融产物,特别是高亲铁元素丰度低,但具有与撞击熔体相似的结构特征。先前对该样品的研究已经描述了“内部”和“外部”部分之间的矿物学差异,这被归因于暴露在月球表面以及随后在撞击喷出物层内或附近通过固体再加热进行的变质作用。研究表明,定量结构分析是区分撞击蚀变月球岩石和内生岩浆作用月球岩石的有效工具。本研究采用这种方法分析了14053的内部和外部的多个薄片。本研究揭示的斜长石晶体薄片的结构不均匀性表明,14053的西侧可能存在撞击-喷射层。这种热变质作用使14053部分的斜长石颗粒变得如此粗糙,以至于成分扩散形成了微妙的层状和中等的质地非均质性,这是可以量化的。这些结果也支持了先前的结论,即样品中还原结构的差异是由于再加热前太阳风注入氢的穿透深度有限。即使低于固相温度,热变质作用也能在月球样品中产生结构变化,从而使内源玄武岩的斜长石结构充分改变为类似于撞击熔体的结构。这些结果强调了对月球样品进行定量岩石学观测的重要性,以揭示重要的岩石成因信息,这些信息必须放在适当的空间背景下才能被理解。
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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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