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The 1:2,500,000-scale global tectonic map of the Moon 被引量:2
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作者 Tianqi Lu Kai Zhu +11 位作者 Shengbo Chen Jianzhong Liu Zongcheng Ling Xiaozhong Ding Kunying Han Jianping Chen Weiming Cheng Danhong Lei yongling mu Anzhen Li Jian Chen Ziyuan Ouyang 《Science Bulletin》 SCIE EI CAS CSCD 2022年第19期1962-1966,共5页
The tectonic evolution of the Moon is driven by both endogenic(e.g.,magmatism)and exogenic(e.g.,meteorite impact)forces.A tectonic map of the Moon provides key information about the spatiotemporal distribution of stru... The tectonic evolution of the Moon is driven by both endogenic(e.g.,magmatism)and exogenic(e.g.,meteorite impact)forces.A tectonic map of the Moon provides key information about the spatiotemporal distribution of structures and tectonic units.Although the Moon has no plate tectonics,its surface can be divided into different terranes due to the uneven evolution[1].We define these terranes as tectonic units.Structures,such as craters and faults,are the basic elements of the tectonic units.As a synthesis of current knowledge on lunar tectonics and evolutionary history,lunar tectonic maps are a fundamental resource for scientific research,exploration planning,and landing site selection[2]. 展开更多
关键词 外动力地质作用 地理信息平台 构造图 环形构造 工程数据 动力学机制 线性构造 构造单元
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