相关实验视频
Updated: May 11, 2026

06:14
Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
月球面膜盆的起源
H J Melosh1, Andrew M Freed, Brandon C Johnson
1Department of Earth, Atmospheric, and Planetary Sciences, Purdue University, 550 Stadium Mall Drive, West Lafayette, IN 47907, USA. jmelosh@purdue.edu
概括
月球质量度 (mascons) 是由撞击盆地挖掘,崩和静平调整产生的. 重力恢复和内部实验室 (GRAIL) 的数据揭示了与这些过程和融化池冷却相关的牛眼重力模式.
科学领域:
- 行星科学 行星科学
- 地质物理学 地质物理学
- 月球地质学 月球地质学
背景情况:
- 月球质量度 (mascons) 是月球上正重力异常的区域.
- 以前的研究表明,mascons起源于撞击过程,但缺乏详细的解释.
- 重力恢复和内部实验室 (GRAIL) 任务提供了高分辨率的重力数据.
研究的目的:
- 用GRAIL引力数据澄清月球巨星的起源.
- 为了解释与冲击盆相关的特征性的目标重力异常模式.
- 为了建模负责mascon形成的地质物理过程.
主要方法:
- 来自GRAIL的高分辨率自由空气重力异常的分析.
- 使用水解码建模模拟撞击盆地形成的模拟.
- 使用有限元素分析对随后的粘弹性放松和冷却进行建模.
主要成果:
- 在月球撞击盆地上观测到牛眼重力模式 (中央阳性,负项圈,外部阳性圆环).
- 证明这些模式源于撞击挖掘,崩和静平调整.
- 确定了冷却和收缩的大型池在塑造重力特征中的作用.
结论:
- 月球巨石是大撞击事件的直接后果,其次是地质放松和冷却.
- 影响mascon重力特征的关键参数包括撞击器能量,月球热梯度,地厚度和火山填充.
- 该研究提供了一个全面的mascon形成的地质物理模型,通过GRAIL数据验证.
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