月球早期岩石圈温度应力的评估

IF 0.6 4区 物理与天体物理 Q4 MECHANICS
S. A. Voropaev, A. P. Krivenko
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引用次数: 0

摘要

在月球形成的早期阶段,其不断增长的岩石圈经历了复杂的时变温度和重力应力。尽管随后表面发生了强烈的撞击转变,但在GRAIL太空任务的重力研究中,发现了古代深部侵入体的存在。对线性引力异常的分析表明,由于温度应力超过引力压缩,月球外层刚性层在其演化的早期阶段会膨胀。获得岩石圈膨胀的时间间隔对许多无量纲热导率参数的依赖性,将有可能完善现有的月球早期热演化和地球化学演化模型。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Assessment of Temperature Stresses in the Lithosphere of the Early Moon

Assessment of Temperature Stresses in the Lithosphere of the Early Moon

In the early stages of the Moon’s formation, its growing lithosphere experienced complex time-varying temperature and gravitational stresses. Despite the subsequent intense impact transformation of the surface, during the gravimetric study of the GRAIL space mission, the presence of ancient deep intrusions was detected. The analysis of linear gravitational anomalies shows the expansion of the outer rigid layer of the Moon at a certain early stage of its evolution due to the excess of temperature stresses over gravitational compression. Obtaining the dependence of the time interval of the lithosphere expansion on a number of dimensionless thermal conductivity parameters will make it possible to refine the existing models of the thermal and geochemical evolution of the early Moon.

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来源期刊
Doklady Physics
Doklady Physics 物理-力学
CiteScore
1.40
自引率
12.50%
发文量
12
审稿时长
4-8 weeks
期刊介绍: Doklady Physics is a journal that publishes new research in physics of great significance. Initially the journal was a forum of the Russian Academy of Science and published only best contributions from Russia in the form of short articles. Now the journal welcomes submissions from any country in the English or Russian language. Every manuscript must be recommended by Russian or foreign members of the Russian Academy of Sciences.
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