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岩浆洋分异与月壳
Differentiation of the lunar magma ocean and formation of the lunar crust

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朱丹 1 *   王世杰 2   朱成明 3  
文摘 回顾了岩浆洋概念最初的由来,具体阐述了月浆洋冷却结晶形成斜长岩月壳的过程.根据行星演化、核一幔分异及地球化学方面等方面提供的证据,论证了岩浆洋是行星早期演化必然经历的一个阶段.已有的岩浆洋结晶模型都认为岩浆洋中的岩浆在成分上是均一的.根据目前实验火成岩石学方面的进展,认为这个前提不存在,提出了月浆洋Soret分异的一个新假说.此模型为今后研究岩浆洋分异提供了一个新思路,并指出了今后的研究方向.
其他语种文摘 We review the original idea of the magma ocean in this paper,and describe in more detail how the anorthositic lunar crust formed through crystallization of the lunar magma ocean during cooling.The magma ocean hypothesis is consistent with several lines of evidence including planet formation,core-mantle differentiation and geochemical observations,and it is proved as an inevitable stage in the early evolution of planets.The magma ocean is assumed to be homogeneous in previous models during crystallization.Based on the recent advance in experimental igneous petrology,we question this assumption,and propose that an gabbrotic melt,from which the anorthositic lunar crust crystallized,can be produced by Soret effect,rather than by magma fractionation.This novel hypothesis supplies with a different view for the future researches.
来源 地球化学 ,2010,39(1):63-72 【核心库】
关键词 岩浆洋 ; 核幔分异 ; W同位素 ; Soret效应
地址

1. 中国科学院地球化学研究所, 矿床地球化学国家重点实验室, 贵州, 贵阳, 550002  

2. 中国科学院地球化学研究所,天体地球化学研究组, 贵州, 贵阳, 550002  

3. 中国科学院地球化学研究所地球深部物质与流体作用地球化学研究室, 贵州, 贵阳, 550002

语种 中文
文献类型 研究性论文
ISSN 0379-1726
学科 天文学
基金 国家自然科学基金 ;  中国科学院知识创新工程重要方向项目
文献收藏号 CSCD:3856256

参考文献 共 87 共5页

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引证文献 3

1 许英奎 存在初始“传导盖层”的月球岩浆洋演化与月壳成因 岩石学报,2016,32(1):1-9
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2 刘耘 国内理论及计算地球化学十年进展 矿物岩石地球化学通报,2013,32(5):531-543
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