火星中层地中的液态水
Vashan Wright1, Matthias Morzfeld1, Michael Manga2
1Scripps Institution of Oceanography, University of California San Diego, La Jolla, CA 92093.
概括
液态水可能和了火星.
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:
- 证据表明,早期的火星表面有大量的液态水.
- 这种水的命运 (地下封存或丢失到太空) 仍在争论中.
研究的目的:
- 为了调查火星地中部水的存在和状态.
- 将地震和重力数据与行星进化模型相协调.
主要方法:
- 使用了岩石物理模型.
- 应用贝叶斯反转技术.
- 使用来自InSight着陆器的地震速度和重力数据的受约束模型.
主要成果:
- 识别了石质,水和度,多孔度和孔隙形状,与火星中层地数据一致.
- 一个被液态水和的碎裂岩石的中间地最适合观测.
- 在约11.5至20公里之间的受限的中层地深度.
结论:
- 液态水可能存在于火星地下.
- 这些发现影响了对火星水循环和可居住性的理解.
- 结果将为未来的资源利用和寻找生命的任务提供信息.
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