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Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
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热疲劳是小小行星上 regolith 的起源
Marco Delbo1, Guy Libourel2, Justin Wilkerson3
1Laboratoire Lagrange, UNS-CNRS, Observatoire de la Côte d'Azur, Boulevard de l'Observatoire-CS 34229, 06304 Nice Cedex 4, France.
Nature
|April 4, 2014
概括
热疲劳,而不是撞击,是小小行星上 regolith的主要来源. 这一由温度变化驱动的过程分解岩石,并可能解释近地小行星的表面.
科学领域:
- 行星科学 行星科学
- 小行星表面的过程.
- 雷戈利特的动力学
背景情况:
- 小小行星被细流层覆盖,这是一个由较小颗粒组成的层.
- 雷戈利特的产生以前被归因于撞击喷射物和微石撞击.
研究的目的:
- 为了确定小小行星上排卵石生成的主导过程.
- 为了研究热疲劳在小行星表面演变中的作用.
主要方法:
- 分析太空任务数据和热红外观测.
- 审查实验室实验和撞击模型对石坑喷射物.
- 作为碎片化机制的热疲劳的理论建模.
主要成果:
- 撞击喷射速度超过小小行星的逃生速度,使它们成为不太可能的岩石的主要来源.
- 热疲劳,由日间温度变化引起,碎片岩石比微型石撞击更快.
- 热碎片是独立于大小的,有助于在所有大小的小行星上形成 regolith.
结论:
- 热疲劳是小型小行星上 regolith 生成的主要过程.
- 这种机制使近地小行星表面再生.
- 热疲劳可能解释了低周日,碳质近地小行星的稀缺性.
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