Chao Wang , Siji Sanlang , Xiaohua Tong , Kaihan Xu , Lu Han , Huan Xie , Yongjiu Feng , Xiong Xu , Yanmin Jin
{"title":"基于“嫦娥五号”样本和遥感影像的高保真月球风化模拟研究","authors":"Chao Wang , Siji Sanlang , Xiaohua Tong , Kaihan Xu , Lu Han , Huan Xie , Yongjiu Feng , Xiong Xu , Yanmin Jin","doi":"10.1016/j.icarus.2025.116764","DOIUrl":null,"url":null,"abstract":"<div><div>The Chang'E-5 (CE-5) mission, China's pioneering endeavor to retrieve lunar samples, brings back approximately 1.7 kg of Moon samples. These CE-5 samples provide valuable material for investigating the properties of lunar regolith and help to understand the geological evolution of the Moon. In this study, we propose a framework for developing a lunar regolith simulant that closely resembles the regolith at the CE-5 landing site. Firstly, the in-situ internal friction angle of the lunar regolith where CE-5 touched down was determined based on the impact depth of the lander footpad and the lunar regolith properties, yielding an estimated range from 29.2° to 43.0°. Secondly, two CE-5 lunar samples, CE5C0300YJFM002GP and CE5C1000YJFM002GP, were analyzed using scanning electron microscopy, micro-computed tomography, and stereoscopic microscopy to investigate particle morphology and size distribution. Thirdly, according to the statistical data from the samples, a new lunar regolith simulant named Tongji University-CE5 (TJ-CE5) was developed through a process involving drying, grinding, sieving, and blending by controlling the bulk density and size distribution. Subsequently, a series of tests were conducted to characterize the properties of the TJ-CE5 simulant. The internal friction angle of TJ-CE5 was measured as 36.9°, which is consistent with the predicted in-situ value. Ultimately, the derived TJ-CE5 simulant is equivalent to the CE-5 lunar regolith in terms of density, particle morphology, particle size distribution, internal friction angle, and chemical composition. Therefore, the framework of this study can be applied to the preparation of other lunar regolith simulants with different properties specific to various landing sites. This research established a methodology for developing a simulant that replicates the characteristics of lunar regolith and provided material for ground experiments supporting lunar exploration and construction missions.</div></div>","PeriodicalId":13199,"journal":{"name":"Icarus","volume":"442 ","pages":"Article 116764"},"PeriodicalIF":3.0000,"publicationDate":"2025-07-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Developing a high-fidelity lunar regolith simulant based on Chang'E-5 samples and remote sensing images\",\"authors\":\"Chao Wang , Siji Sanlang , Xiaohua Tong , Kaihan Xu , Lu Han , Huan Xie , Yongjiu Feng , Xiong Xu , Yanmin Jin\",\"doi\":\"10.1016/j.icarus.2025.116764\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div>The Chang'E-5 (CE-5) mission, China's pioneering endeavor to retrieve lunar samples, brings back approximately 1.7 kg of Moon samples. These CE-5 samples provide valuable material for investigating the properties of lunar regolith and help to understand the geological evolution of the Moon. In this study, we propose a framework for developing a lunar regolith simulant that closely resembles the regolith at the CE-5 landing site. Firstly, the in-situ internal friction angle of the lunar regolith where CE-5 touched down was determined based on the impact depth of the lander footpad and the lunar regolith properties, yielding an estimated range from 29.2° to 43.0°. Secondly, two CE-5 lunar samples, CE5C0300YJFM002GP and CE5C1000YJFM002GP, were analyzed using scanning electron microscopy, micro-computed tomography, and stereoscopic microscopy to investigate particle morphology and size distribution. Thirdly, according to the statistical data from the samples, a new lunar regolith simulant named Tongji University-CE5 (TJ-CE5) was developed through a process involving drying, grinding, sieving, and blending by controlling the bulk density and size distribution. Subsequently, a series of tests were conducted to characterize the properties of the TJ-CE5 simulant. The internal friction angle of TJ-CE5 was measured as 36.9°, which is consistent with the predicted in-situ value. Ultimately, the derived TJ-CE5 simulant is equivalent to the CE-5 lunar regolith in terms of density, particle morphology, particle size distribution, internal friction angle, and chemical composition. Therefore, the framework of this study can be applied to the preparation of other lunar regolith simulants with different properties specific to various landing sites. This research established a methodology for developing a simulant that replicates the characteristics of lunar regolith and provided material for ground experiments supporting lunar exploration and construction missions.</div></div>\",\"PeriodicalId\":13199,\"journal\":{\"name\":\"Icarus\",\"volume\":\"442 \",\"pages\":\"Article 116764\"},\"PeriodicalIF\":3.0000,\"publicationDate\":\"2025-07-28\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Icarus\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S0019103525003124\",\"RegionNum\":2,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Icarus","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0019103525003124","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
Developing a high-fidelity lunar regolith simulant based on Chang'E-5 samples and remote sensing images
The Chang'E-5 (CE-5) mission, China's pioneering endeavor to retrieve lunar samples, brings back approximately 1.7 kg of Moon samples. These CE-5 samples provide valuable material for investigating the properties of lunar regolith and help to understand the geological evolution of the Moon. In this study, we propose a framework for developing a lunar regolith simulant that closely resembles the regolith at the CE-5 landing site. Firstly, the in-situ internal friction angle of the lunar regolith where CE-5 touched down was determined based on the impact depth of the lander footpad and the lunar regolith properties, yielding an estimated range from 29.2° to 43.0°. Secondly, two CE-5 lunar samples, CE5C0300YJFM002GP and CE5C1000YJFM002GP, were analyzed using scanning electron microscopy, micro-computed tomography, and stereoscopic microscopy to investigate particle morphology and size distribution. Thirdly, according to the statistical data from the samples, a new lunar regolith simulant named Tongji University-CE5 (TJ-CE5) was developed through a process involving drying, grinding, sieving, and blending by controlling the bulk density and size distribution. Subsequently, a series of tests were conducted to characterize the properties of the TJ-CE5 simulant. The internal friction angle of TJ-CE5 was measured as 36.9°, which is consistent with the predicted in-situ value. Ultimately, the derived TJ-CE5 simulant is equivalent to the CE-5 lunar regolith in terms of density, particle morphology, particle size distribution, internal friction angle, and chemical composition. Therefore, the framework of this study can be applied to the preparation of other lunar regolith simulants with different properties specific to various landing sites. This research established a methodology for developing a simulant that replicates the characteristics of lunar regolith and provided material for ground experiments supporting lunar exploration and construction missions.
期刊介绍:
Icarus is devoted to the publication of original contributions in the field of Solar System studies. Manuscripts reporting the results of new research - observational, experimental, or theoretical - concerning the astronomy, geology, meteorology, physics, chemistry, biology, and other scientific aspects of our Solar System or extrasolar systems are welcome. The journal generally does not publish papers devoted exclusively to the Sun, the Earth, celestial mechanics, meteoritics, or astrophysics. Icarus does not publish papers that provide "improved" versions of Bode''s law, or other numerical relations, without a sound physical basis. Icarus does not publish meeting announcements or general notices. Reviews, historical papers, and manuscripts describing spacecraft instrumentation may be considered, but only with prior approval of the editor. An entire issue of the journal is occasionally devoted to a single subject, usually arising from a conference on the same topic. The language of publication is English. American or British usage is accepted, but not a mixture of these.