NAOC Open IR
月球的地体构造与起源模式
张福勤1; 李春来2; 邹永廖2; 刘建忠2; 欧阳自远2
2009
Source Publication岩石学报
ISSN1000-0569
Volume000Issue:008Pages:2011
Abstract按照月球表面物质成分分布的特点,月壳可以划分为三个主要的化学地体:1)风暴洋克里普地体(PKT);2)斜长质高地地体(FHT);3)南极爱特肯地体(SPAT),综合对比天体化学和固体地球科学研究的前缘和热点,本文建立了月球地体构造及其起源的星子堆积模式,对月球化学分布的不均匀性的起因给出了较为简单和合理的解释. Abstract: According to the composition distributon on the lunar surface, lunar crust can he divided into three main chemical terranes: 1) Procellarum KREEP Terrane (PKT); 2) Feldspathic Highland Terrane (FHT); 3) South Pole Aitken Terrane (SPAT). Through research the frontier and focus of cosmochemistry and solid earth science, we found lunar terranes structure and planetesimal accumulation model of lunar origin, giving an simply and reasonable explanation of inhomogeneity chemical distribution on the Moon.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/37519
Collection中国科学院国家天文台
Affiliation1.中国科学院地质与地球物理研究所
2.中国科学院国家天文台
Recommended Citation
GB/T 7714
张福勤,李春来,邹永廖,等. 月球的地体构造与起源模式[J]. 岩石学报,2009,000(008):2011.
APA 张福勤,李春来,邹永廖,刘建忠,&欧阳自远.(2009).月球的地体构造与起源模式.岩石学报,000(008),2011.
MLA 张福勤,et al."月球的地体构造与起源模式".岩石学报 000.008(2009):2011.
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