月球形成大碰撞理论的数值模拟研究进展
Adevances of The Research on Numerical Simulation for the Moon-Forming Giant Impact Theory
查看参考文献72篇
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文摘
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月球的起源是一个长期具有争议的重大科学问题。大碰撞理论自1974年提出以后,由于它能较好的解释地月系统间的一系列观测事实和数据,而逐渐成为月球起源的各种理论中最被广为接受的一种。自2001年第一个模拟大碰撞的标准模型 (canonical)建立以后,一系列新的数值模型和相关理论不断出现。本文全面回顾了大碰撞理论迄今的发展历程及研究现状,介绍了现行最主要的数值模型及其存在的缺点、相关理论的发展现状,以及近年来在地月系统间一些基本特性的全新认识。然而这些新的模型理论和认识均存在各自的疑点,尚未对现行的数值模型产生根本的影响。月球的形成问题远未解决,需要获取更多的探测与实验数据,并更加深入的探讨数值模型的约束条件与过程机理。 |
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其他语种文摘
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The origin of the moon is an important long-term controversial scientific question. The giant impact theory was proposed in 1974. Since then,it has gradually become the most popular theory among various theories of the Moon formation because it can more reasonably explain a series of observed facts and acquired data for the system between the earth and the moon than other theories. Since the establishment of the first standard model (Canonical) for simulating the giant impact in 2001,a series of new numerical models and theories have been continuously proposed. This paper has comprehensively reviewed the progress and research status of the giant impact theory since its establishment,has introduced some currently popular numerical models and their disadvantages,the development status of some related theories,and some new viewpoints on some basic features of the earth-moon system proposed in recent years. However,these new numerical models and theories have their own respective doubtful points,thus they have not significantly influenced on the standard numerical model. The problem of the moon formation is far from resolved,as much more detection and experimental data need to be acquired in order to furtherly discuss constraint conditions and process mechanisms of the numerical model. |
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来源
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矿物岩石地球化学通报
,2017,36(4):673-686 【核心库】
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DOI
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10.3969/j.issn.1007-2802.2017.04.020
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关键词
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大碰撞理论
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月球形成
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数值模拟
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地址
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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, 贵阳, 550081
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语种
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中文 |
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文献类型
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综述型 |
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ISSN
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1007-2802 |
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学科
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地质学 |
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基金
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国家自然科学基金重大项目
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中国科学院专项B
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文献收藏号
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CSCD:6057116
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参考文献 共
72
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