Vapor Condensates on the Most Pristine Black Beads From a Clod in Apollo Drive Tube 73001: Discovery of Lunar NaCl Nanocrystals

IF 3.9 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Yang Liu, Chi Ma
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Abstract

Identification of the mineral species of vapor condensates on the surface of lunar pyroclastic beads, formed during the flights of beads in the lunar volcanic plume, helps to constrain the physical and chemical conditions of the lunar volcanic plume. We conducted nanomineralogy studies of vapor condensates on the surface of pristine black beads from a clod that was extracted from the recently opened Apollo drive tube 73001. This drive tube had been sealed under vacuum since its collection on the Moon and thus represents the most pristine sample in allocatable Apollo collection. Vapor condensates observed on the surface include patches made of ZnS nanocrystals and possible rare scattered NaCl nanocrystals. ZnS nanocrystals were previously found on Apollo 15 green and yellow beads, but NaCl nanocrystals are unique to black beads. Both ZnS and NaCl nanocrystals are absent in Apollo 17 74220 orange beads. Although orange and black beads are of similar chemistry, black beads in the clod 73001, 226 could form from a different environment.

阿波罗驱动管 73001 中泥块上最纯净的黑色珠子上的蒸汽冷凝物:发现月球氯化钠纳米晶体
对月球火山羽流中的珠粒在飞行过程中形成的月球火成碎屑珠粒表面蒸汽冷凝物的矿物种类进行鉴定,有助于确定月球火山羽流的物理和化学条件。我们对从最近打开的阿波罗第 73001 号驱动管中提取的原始黑色珠块表面的蒸汽冷凝物进行了纳米矿物学研究。该驱动管自在月球上采集以来一直密封在真空中,因此是可分配的阿波罗采集物中最原始的样本。在表面观察到的蒸汽冷凝物包括由 ZnS 纳米晶体和可能罕见的零散 NaCl 纳米晶体组成的斑块。之前曾在阿波罗 15 号的绿色和黄色珠子上发现过 ZnS 纳米晶体,但 NaCl 纳米晶体是黑色珠子上独有的。阿波罗 17 号 74220 橙色珠子中没有锌盐和氯化钠纳米晶体。虽然橙色珠子和黑色珠子的化学性质相似,但泥块 73001 226 中的黑色珠子可能是在不同的环境中形成的。
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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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