通过 MarSCoDe LIBS 在火星祝融着陆点观测到的碱痕量元素:定量分析及其地质学意义

IF 3.9 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Yuxuan Luo, Jianjun Liu, Zhaopeng Chen, Yizhong Zhang, Xing Wang, Xin Ren, Xiangfeng Liu, Zhenqiang Zhang, Weiming Xu, Rong Shu
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引用次数: 0

摘要

火星表面成分探测仪(MarSCoDe)是中国首次火星探测任务 "天文一号 "中 "祝融号 "探测器携带的重要有效载荷之一。MarSCoDe的激光诱导击穿光谱(LIBS)仪器主要用于探测火星表面的主要元素和痕量元素。锂(Li)、锶(Sr)和铷(Rb)等碱痕量元素的定量分析对揭示祝融着陆点的地质演化具有重要意义。本研究的重点是利用在地面实验室测试的 84 个样品的 MarSCoDe LIBS 光谱建立单变量校准模型。随后,通过对 12 个搭载的 MarSCoDe 校准靶(MCCTs)进行分析,验证了这些模型的准确性,准确度在百万分之一(ppm)以内。利用这些模型,确定了在最初的 300 Sols(火星天)穿越期间地表目标中的锂、锶和铷浓度。这些浓度分别为 6 至 18、106-628 和 22-87 ppm。我们的结果表明,锂、锶和铷主要与祝融着陆点岩石和土壤中的火成岩成分有关。MarSCoDe 科学目标中的主要次生矿物可能是少量硫酸盐,似乎是由近期地表盐水酸性风化形成的。科学目标中的粘土矿物可能不存在或非常稀少。着陆点的地表火成岩材料可能来自亚马逊纪的最近熔岩流。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Alkali Trace Elements Observed by MarSCoDe LIBS at Zhurong Landing Site on Mars: Quantitative Analysis and Its Geological Implications

Mars Surface Composition Detector (MarSCoDe) is one of the important payloads carried by the Zhurong rover, China's first Mars exploration mission Tianwen-1. The laser-induced breakdown spectroscopy (LIBS) instrument of MarSCoDe is mainly used to detect major and trace elements on the surface of Mars. The quantitative analysis of alkali trace elements, namely lithium (Li), strontium (Sr), and rubidium (Rb), holds significance in unraveling the geological evolution of the Zhurong landing site. This study focuses on establishing univariate calibration models using MarSCoDe LIBS spectra from 84 samples tested in the ground laboratory. The accuracy of these models, within a few parts per million (ppm), was subsequently validated through the analysis of 12 onboard MarSCoDe Calibration Targets (MCCTs). With these models, Li, Sr, and Rb concentrations in the surface targets during the initial 300 sols (Martian days) traverse were determined. These concentrations ranged from 6 to 18, 106–628, and 22–87 ppm, respectively. Our results suggest that Li, Sr, and Rb are mainly related to the igneous rock components in the rocks and soils at the Zhurong landing site. The major secondary minerals in MarSCoDe scientific targets are likely small amounts of sulfates, which appear to have formed from the acidic weathering of recent surface brine. Clay minerals are likely either absent or very sparse in the scientific targets. The surface igneous materials at the landing site likely have originated from the most recent lava flow during the Amazonian epoch.

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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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