摘要
人类对月表物质成分的科学认识始于20世纪60~70年代.大量的无人和载人月球探测获得了珍贵的历史数据.利用这些数据资料,美国地质勘探局编制了最早的一批月球地质图,但由于当时缺乏全面的月表物质成分探测数据,早期的月表地质单元划分多以形貌特征为依据而缺少成分约束. 20世纪90年代以来,新一轮的月球探测任务获取了全月球表面的物质成分探测数据,为开展月表物质成分编图提供了第一手资料.通过对月表物质成分分布信息的研究,本研究建立了月球内动力地质作用形成的岩石类型分类体系.基于GIS平台编制完成的1:250万月球岩石类型分布图及建立的月球物质成分数据库,为开展月球数字地质图编研和月球地质综合研究以及未来其他天体的编图工作奠定了基础.
Scientific knowledge of lunar lithologies was first acquired in the 1960s-1970s.The space race between the United States(U.S.)and Soviet Union has promoted numerous manned and robotic lunar exploration missions.Utilizing datasets from these missions,the first series of lunar geologic maps was prepared and published by the U.S.Geological Survey(USGS)The definition of lunar geological features in these maps was mostly based on morphological characteristics but lacked lithological constraints owing to the incompleteness of the compositional datasets avail-able.After two decades of silence,a new era of lunar exploration began in the 1990s when the Galileo spacecraft flew by the Moon during its gravity-assisted maneuvers.The very successful orbital missions,the Clementine and Lunar Prospector(LP),provided the first global geochemical and mineralogical(multispectral,gamma ray,neutron,etc.)datasets of the lunar surface.
作者
陈剑
凌宗成
刘建忠
陈圣波
丁孝忠
陈建平
程维明
李勃
张江
孙灵芝
刘长卿
曹海军
毕向宇
刘莉
万晟
齐晓彬
赵紫旭
郭弟均
籍进柱
刘敬稳
王俊涛
张珂
张敬宜
孙鹏举
朱凯
陆天启
吴聪哲
韩坤英
许可娟
金铭
王颖
张诚
邓佳音
宋杨
欧阳自远
Jian Chen;Zongcheng Ling;Jianzhong Liu;Shengbo Chen;Xiaozhong Ding;Jianping Chen;Weiming Cheng;Bo Li;Jiang Zhang;Lingzhi Sun;Changqing Liu;Haijun Cao;Xiangyu Bi;Li Liu;Sheng Wan;Xiaobin Qi;Zixu Zhao;Dijun Guo;Jinzhu Ji;Jingwen Liu;Juntao Wang;Ke Zhang;Jingyi Zhang;Pengju Sun;Kai Zhu;Tianqi Lu;Congzhe Wu;Kunying Han;Kejuan Xu;Ming Jin;Ying Wang;Cheng Zhang;Jiayin Deng;Yang Song;Ziyuan Ouyang(Shandong Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment,Institute of Space Sciences,School of Space Science and Physics,Shandong University,Weihai 264209,China;Center for Excellence in Comparative Planetology,Chinese Academy of Sciences,Hefei 230026,China;Center for Lunar and Planetary Science,Institute of Geochemistry,Chinese Academy of Sciences,Guiyang 550081,China;College of Geoexploration Science and Technology,Jilin University,Changchun 130000,China;Institute of Geology,Chinese Academy of Geological Sciences,Beijing 100037,China;School of Earth Sciences and Resources,China University of Geosciences,Beijing 100083,China;Institute of Geographic Sciences and Natural Resources Research,Chinese Academy of Sciences,Beijing 100101,China;Hawai’i Institute of Geophysics and Planetology,Department of Earth Sciences,University of Hawai’i at Manoa,Honolulu HI 96826,USA;National Space Science Center,Chinese Academy of Sciences,Beijing 100190,China;School of Mining,Inner Mongolia University of Technology,Hohhot 010051,China;University of Chinese Academy of Sciencess,Beijing 100049,China)
基金
supported by the National Science and Technology Infrastructure Work Projects(2015FY210500)
Key Research Program of Frontier Sciences,Chinese Academy of Sciences(QYZDY-SSW-DQC028)
Strategic Priority Program of Chinese Academy of Sciences(XDB41000000)
the National Natural Science Foundation of China(42102280,41972322,and 11941001)
the Natural Science Foundation of Shandong Province(ZR2021QD016)
the China Postdoctoral Science Foundation(2020M682164)
the State Scholarship Fund(201706220310)
。