在岩石小行星上检测到的热疲劳导致的快速岩石断裂
A Lucchetti1, S Cambioni2, R Nakano3,4
1INAF-Astronomical Observatory of Padova, Vic. Osservatorio 5, 35122, Padova, Italy. alice.lucchetti@inaf.it.
Nature communications
|July 30, 2024
概括
小行星Dimorphos上的断裂,是S复合体的一部分,可能是由于热疲劳而形成的. 这个过程可能会通过改变喷射的质量和动量来影响小行星偏移任务.
科学领域:
- 行星科学 行星科学
- 小行星地质学
- 太空飞船的观测空间飞船的观测.
背景情况:
- 碳化小行星显示热应力断裂.
- 像Dimorphos这样的S复合小行星上的断裂是不太了解的.
- 迪莫尔福斯是小行星迪迪莫斯的月球,是NASADART任务的目标.
研究的目的:
- 在Dimorphos岩石上调查断裂形成.
- 确定骨折是否是由于热疲劳造成的.
- 评估对小行星偏移的影响.
主要方法:
- 太空飞船对Dimorphos岩石的观测. 太空飞船对Dimorphos岩石的观察.
- 骨折大小频率分布和方向的分析.
- 由于热疲劳造成的断裂传播的建模.
主要成果:
- 在Dimorphos岩石上的断裂模式与热疲劳是一致的.
- 断裂可能在Dimorphos的位置上形成,而不是从Didymos转移.
- 浅,水平断裂的形成速度比垂直断裂 (Myrs) 快 (100 kyr).
结论:
- 热疲劳是塑造S型小行星表面的重要过程.
- 小行星上的断裂模式可以使用热疲劳来建模.
- 小行星表面破裂可能会增加在动力冲击器任务期间喷射的质量和动量.
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