Yiming Diao , Honglei Lin , Juan Li , Shouding Li , Changyi Xu , Zhaobin Zhang , Zongyu Yue , Bo Zheng , Xiukuo Sun , Tao Xu , Xinshuo Chen , Yanfang Wu , Xiao Li
{"title":"UPRS-1:模拟火星乌托邦平原的风化层","authors":"Yiming Diao , Honglei Lin , Juan Li , Shouding Li , Changyi Xu , Zhaobin Zhang , Zongyu Yue , Bo Zheng , Xiukuo Sun , Tao Xu , Xinshuo Chen , Yanfang Wu , Xiao Li","doi":"10.1016/j.icarus.2025.116692","DOIUrl":null,"url":null,"abstract":"<div><div>Understanding the composition and properties of Martian soils is crucial for scientific research and engineering tests for payloads and landers, which is why simulants are utilized in diverse applications in the absence of Martian samples returned to Earth. Existing simulants are predominantly based on the global Martian surface materials and some regions in the southern highlands of Mars, neglecting the northern lowlands such as Utopia Planitia. The Zhurong rover of the Chinese Tianwen-1 mission explored Utopia Planitia, collecting extensive physical and chemical data from surface materials and facilitating the development of a new Mars simulant representing the northern lowlands. Thus, we developed Utopia Planitia Regolith Simulant-1 (UPRS-1) to replicate the soil properties of Utopia Planitia and proposed a quantitative evaluation to assess the high similarity of UPRS-1. The overall similarity parameter of UPRS-1 is 86.1 % via quantitative evaluation. Additionally, its composition is adaptable to specific research requirements, enabling its application in diverse fields, including geotechnical experiments, in-situ resource utilization (ISRU) technology, ground tests for exploration missions, and astrobiology.</div></div>","PeriodicalId":13199,"journal":{"name":"Icarus","volume":"441 ","pages":"Article 116692"},"PeriodicalIF":2.5000,"publicationDate":"2025-06-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"UPRS-1: A regolith simulant of Utopia Planitia, Mars\",\"authors\":\"Yiming Diao , Honglei Lin , Juan Li , Shouding Li , Changyi Xu , Zhaobin Zhang , Zongyu Yue , Bo Zheng , Xiukuo Sun , Tao Xu , Xinshuo Chen , Yanfang Wu , Xiao Li\",\"doi\":\"10.1016/j.icarus.2025.116692\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div>Understanding the composition and properties of Martian soils is crucial for scientific research and engineering tests for payloads and landers, which is why simulants are utilized in diverse applications in the absence of Martian samples returned to Earth. Existing simulants are predominantly based on the global Martian surface materials and some regions in the southern highlands of Mars, neglecting the northern lowlands such as Utopia Planitia. The Zhurong rover of the Chinese Tianwen-1 mission explored Utopia Planitia, collecting extensive physical and chemical data from surface materials and facilitating the development of a new Mars simulant representing the northern lowlands. Thus, we developed Utopia Planitia Regolith Simulant-1 (UPRS-1) to replicate the soil properties of Utopia Planitia and proposed a quantitative evaluation to assess the high similarity of UPRS-1. The overall similarity parameter of UPRS-1 is 86.1 % via quantitative evaluation. Additionally, its composition is adaptable to specific research requirements, enabling its application in diverse fields, including geotechnical experiments, in-situ resource utilization (ISRU) technology, ground tests for exploration missions, and astrobiology.</div></div>\",\"PeriodicalId\":13199,\"journal\":{\"name\":\"Icarus\",\"volume\":\"441 \",\"pages\":\"Article 116692\"},\"PeriodicalIF\":2.5000,\"publicationDate\":\"2025-06-06\",\"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/S0019103525002398\",\"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/S0019103525002398","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}
UPRS-1: A regolith simulant of Utopia Planitia, Mars
Understanding the composition and properties of Martian soils is crucial for scientific research and engineering tests for payloads and landers, which is why simulants are utilized in diverse applications in the absence of Martian samples returned to Earth. Existing simulants are predominantly based on the global Martian surface materials and some regions in the southern highlands of Mars, neglecting the northern lowlands such as Utopia Planitia. The Zhurong rover of the Chinese Tianwen-1 mission explored Utopia Planitia, collecting extensive physical and chemical data from surface materials and facilitating the development of a new Mars simulant representing the northern lowlands. Thus, we developed Utopia Planitia Regolith Simulant-1 (UPRS-1) to replicate the soil properties of Utopia Planitia and proposed a quantitative evaluation to assess the high similarity of UPRS-1. The overall similarity parameter of UPRS-1 is 86.1 % via quantitative evaluation. Additionally, its composition is adaptable to specific research requirements, enabling its application in diverse fields, including geotechnical experiments, in-situ resource utilization (ISRU) technology, ground tests for exploration missions, and astrobiology.
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.