月球经历了比我们目前在其表面看到的更大的撞击

IF 12.9 1区物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS

Nature Astronomy Pub Date : 2025-01-13 DOI:10.1038/s41550-024-02445-y

引用次数: 0

摘要

行星形成的尾端吸积假说认为，早期月球经历了严重的撞击。粘性松弛抹去了月球岩浆海洋凝固后不久形成的月球撞击盆地，从而解释了月球上目前存在的盆地数量较少的原因。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

Moon experienced more large impacts than we currently see on its surface

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Moon experienced more large impacts than we currently see on its surface

The tail-end accretion hypothesis of planet formation posits that the early Moon underwent heavy impacts. Viscous relaxation erased lunar impact basins that formed shortly after the solidification of the lunar magma ocean, explaining the low number of basins currently present on the Moon.

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来源期刊

Nature Astronomy Physics and Astronomy-Astronomy and Astrophysics

CiteScore

19.50

自引率

2.80%

发文量

252

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