Space Weathering Properties of Chang’e-6 Soils and Implication for Regolith Evolution of Young Lunar Maria

Xuejin Lu, Jian Chen, Haijun Cao, Changqing Liu, Ziyi Jia, Chengxiang Yin, Tianwei Wang, Xiaohui Fu, Le Qiao, Xiaojia Zeng, Jiang Zhang and Zongcheng Ling
{"title":"Space Weathering Properties of Chang’e-6 Soils and Implication for Regolith Evolution of Young Lunar Maria","authors":"Xuejin Lu, Jian Chen, Haijun Cao, Changqing Liu, Ziyi Jia, Chengxiang Yin, Tianwei Wang, Xiaohui Fu, Le Qiao, Xiaojia Zeng, Jiang Zhang and Zongcheng Ling","doi":"10.3847/2041-8213/adbffc","DOIUrl":null,"url":null,"abstract":"Lunar soil samples from young maria (formed <3.0 billion years ago (Ga)) preserve key records of recent space weathering history in the Earth–Moon system. China’s Chang’e-6 mission returned the first farside soil samples from a young mare (∼2.8 Ga) at the northeastern South Pole–Aitken basin. We present preliminary results on the space weathering properties of the Chang’e-6 soils. The glassy agglutinate content in the Chang’e-6 soils is approximately 30%, significantly lower than the 50%–70% observed in the mature Apollo soils from older maria (>3.0 Ga) and higher than the ∼21% found in the Chang’e-5 soils from younger mare (∼2.0 Ga). However, our spectroscopic study reveals that the Chang’e-6 soils are well developed, with high maturity, weak absorption, and a red-sloped continuum, similar to the characteristics of the mature soils from the Apollo and Chang’e-5 landing sites. Orbital observations indicate more mature surface than in the returned samples from young mare regions, likely due to the destruction of an optically mature veneer by spacecraft. The optically mature veneer reveals deficiencies in remote sensing and emphasizes the importance of sample return missions. The thinner optically mature veneer and lower abundance of glassy agglutinate in younger maria suggest reduced gardening cycles and changes in impactor properties (such as rate and size) after 3.0 Ga. This is important for understanding how the relative contributions of space weathering agents change over time and the evolution of impactors in the inner solar system.","PeriodicalId":501814,"journal":{"name":"The Astrophysical Journal Letters","volume":"23 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2025-04-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"The Astrophysical Journal Letters","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.3847/2041-8213/adbffc","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0

Abstract

Lunar soil samples from young maria (formed <3.0 billion years ago (Ga)) preserve key records of recent space weathering history in the Earth–Moon system. China’s Chang’e-6 mission returned the first farside soil samples from a young mare (∼2.8 Ga) at the northeastern South Pole–Aitken basin. We present preliminary results on the space weathering properties of the Chang’e-6 soils. The glassy agglutinate content in the Chang’e-6 soils is approximately 30%, significantly lower than the 50%–70% observed in the mature Apollo soils from older maria (>3.0 Ga) and higher than the ∼21% found in the Chang’e-5 soils from younger mare (∼2.0 Ga). However, our spectroscopic study reveals that the Chang’e-6 soils are well developed, with high maturity, weak absorption, and a red-sloped continuum, similar to the characteristics of the mature soils from the Apollo and Chang’e-5 landing sites. Orbital observations indicate more mature surface than in the returned samples from young mare regions, likely due to the destruction of an optically mature veneer by spacecraft. The optically mature veneer reveals deficiencies in remote sensing and emphasizes the importance of sample return missions. The thinner optically mature veneer and lower abundance of glassy agglutinate in younger maria suggest reduced gardening cycles and changes in impactor properties (such as rate and size) after 3.0 Ga. This is important for understanding how the relative contributions of space weathering agents change over time and the evolution of impactors in the inner solar system.
求助全文
约1分钟内获得全文 求助全文
来源期刊
自引率
0.00%
发文量
0
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信