{"title":"Analyzing the Mechanical Heterogeneity of the Chang'e-5 Lunar Breccia Clast: Implications for the Elastic Modulus of Lunar Rock","authors":"Jiayan Nie, Siqiao Wang, Yifei Cui, Zhijun Wu, Jian He, Guodong Wang, Xiaojia Zeng","doi":"10.1029/2024JE008849","DOIUrl":null,"url":null,"abstract":"<p>Understanding the mechanical properties (e.g., Young's modulus and hardness) of lunar regolith materials, especially their heterogeneity, is of great significance to planetary science. For the first time, we applied grid nanoindentation tests on the Chang'e-5 lunar breccia clast to analyze its mechanical heterogeneity along with a micromorphology analysis of representative indentation spots. A novel Bayesian deconvolution method was proposed to identify the dominating components and statistical characteristics of their mechanical properties, which were further employed to estimate the elastic properties of lunar rocks. Research has shown that lunar breccia clasts exhibit high mechanical heterogeneity due to their polymineral compositions, well-developed micro-pores, micro-cracks, and complex surface fabrics. Moreover, compared with the asteroid 25,143 Itokawa regolith particles, and the Chelyabinsk and NWA6013 meteorites, the Chang'e-5 lunar breccia clast, and the lunar DHOFAR 1084, JAH 838 and NWA 11444 meteorites have larger average plastic indices, indicating that the lunar regolith materials may be characterized by better cushion energy absorption and ductility properties than asteroids. In addition, two dominant components with similar hardness but different relative weights were identified for two representative measurement regions within the lunar breccia clast. On the basis of the deconvolved mechanical information, we finally estimated the elastic modulus range of lunar rocks (i.e., 38∼56 GPa) through effective medium theory. This study provides important implications for understanding the influence of planetary surface processes on the mechanical properties of extraterrestrial regolith materials and for predicting the engineering properties of lunar rocks from dimensionally limited lunar samples.</p>","PeriodicalId":16101,"journal":{"name":"Journal of Geophysical Research: Planets","volume":"130 6","pages":""},"PeriodicalIF":3.9000,"publicationDate":"2025-05-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Geophysical Research: Planets","FirstCategoryId":"89","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1029/2024JE008849","RegionNum":1,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
Understanding the mechanical properties (e.g., Young's modulus and hardness) of lunar regolith materials, especially their heterogeneity, is of great significance to planetary science. For the first time, we applied grid nanoindentation tests on the Chang'e-5 lunar breccia clast to analyze its mechanical heterogeneity along with a micromorphology analysis of representative indentation spots. A novel Bayesian deconvolution method was proposed to identify the dominating components and statistical characteristics of their mechanical properties, which were further employed to estimate the elastic properties of lunar rocks. Research has shown that lunar breccia clasts exhibit high mechanical heterogeneity due to their polymineral compositions, well-developed micro-pores, micro-cracks, and complex surface fabrics. Moreover, compared with the asteroid 25,143 Itokawa regolith particles, and the Chelyabinsk and NWA6013 meteorites, the Chang'e-5 lunar breccia clast, and the lunar DHOFAR 1084, JAH 838 and NWA 11444 meteorites have larger average plastic indices, indicating that the lunar regolith materials may be characterized by better cushion energy absorption and ductility properties than asteroids. In addition, two dominant components with similar hardness but different relative weights were identified for two representative measurement regions within the lunar breccia clast. On the basis of the deconvolved mechanical information, we finally estimated the elastic modulus range of lunar rocks (i.e., 38∼56 GPa) through effective medium theory. This study provides important implications for understanding the influence of planetary surface processes on the mechanical properties of extraterrestrial regolith materials and for predicting the engineering properties of lunar rocks from dimensionally limited lunar samples.
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.