月球的起源

Robin M. Canup, Kevin Righter, Nicolas Dauphas, Kaveh Pahlevan, Matija Ćuk, Simon J. Lock, Sarah T. Stewart, Julien Salmon, Raluca Rufu, Miki Nakajima, Tomáš Magna
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引用次数: 0

摘要

地月系统在几个方面都不同寻常。月球的半径大约是地球的 1/4--卫星与行星的尺寸比冥王星的卡戎以外的所有已知卫星都要大。月球的内核很小,可能只占其质量的 ~1%,而地球的内核则占其质量的近 30%。地月系统的总角动量很大,这意味着月球形成时地球正在快速旋转。此外,早期的月球温度很高,至少部分熔融,有很深的岩浆海洋。确定一个月球起源模型可以令人满意地...
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Origin of the Moon
The Earth–Moon system is unusual in several respects. The Moon is roughly ¼ the radius of the Earth—a larger satellite-to-planet size ratio than all known satellites other than Pluto’s Charon. The Moon has a tiny core, perhaps with only ~1% of its mass, in contrast to Earth whose core contains nearly 30% of its mass. The Earth–Moon system has a high total angular momentum, implying a rapidly spinning Earth when the Moon formed. In addition, the early Moon was hot and at least partially molten with a deep magma ocean. Identification of a model for lunar origin that can satisfactorily...
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