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Updated: Oct 22, 2025

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Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
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来自InSight地震数据的火星地的厚度和结构
Brigitte Knapmeyer-Endrun1, Mark P Panning2, Felix Bissig3
1Bensberg Observatory, University of Cologne, Vinzenz-Pallotti-Str. 26, 51429 Bergisch Gladbach, Germany. bknapmey@uni-koeln.de.
概括
科学家使用InSight着陆器的地震数据测量了火星地的厚度. 据估计,火星的地平均厚度在24至72公里之间.
科学领域:
- 星球科学
- 地震学
- 地质学
背景情况:
- 它记录了行星的形成和演变.
- 在这项研究之前,火星缺乏绝对地厚度的测量.
研究的目的:
- 在火星上的InSight着陆站下面的地厚度.
- 提供火星地厚度的第一个绝对测量.
主要方法:
- 在地下界面反射和转换的地震相的分析.
- 使用火星地震记录和环境波场.
- 使用全球重力和地形图进行点测量的推断.
主要成果:
- 地震数据显示至少有两个,可能有三个地下接口.
- 地厚度估计在20 ± 5公里 (第二个接口) 到39 ± 8公里 (第三个接口) 之间.
- 平均火星地厚度估计在24至72公里之间.
结论:
- 这些发现为了解火星地质演变提供了至关重要的数据.
- 地力学和组成限制有利于在深度集中热生成元素的较厚的地模型.
- 这项研究为火星地研究奠定了新的基础.
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