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Updated: Jul 11, 2026

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Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
火星的南极层层沉积物的密度
Maria T Zuber1, Roger J Phillips, Jeffrey C Andrews-Hanna
1Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139-4307, USA. zuber@mit.edu
概括
火星南极层层沉积物的密度是使用轨道数据计算的. 结果表明这些火星冰盖主要是含有一些灰尘的水冰,完善了我们对火星水的理解.
科学领域:
- 行星科学 行星科学
- 地质物理学 地质物理学
- 天体生物学 天体生物学
背景情况:
- 火星有极地冰盖,这些冰盖是由层层的沉积物组成的.
- 了解这些沉积物的组成对于行星科学和天体生物学至关重要.
研究的目的:
- 为了确定火星南极层层沉积物的密度.
- 为了推断火星冰盖的组成和纯度.
主要方法:
- 来自火星侦察轨道器 (MRO) 的综合重力场数据.
- 来自火星轨道器激光高度计 (MOLA) 的综合表面地形.
- 利用来自火星地下和离子层探测 (MARSIS) 先进雷达的基础地形数据.
主要成果:
- 计算出南极层层沉积物最适合的密度为1220kg/m3.
- 这种密度与含有约15%混合尘埃的水冰相一致.
- 这些发现表明,这些沉积物主要由相对清洁的水冰组成.
结论:
- 南极的分层沉积物很可能由相对纯净的水冰组成.
- 这项研究改进了对火星表面水库存的估计.
- 提供了洞察火星的地质历史和潜在的可居住性.
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