在Candor Chasma,火星的骨折控制的古流体流
Chris H Okubo1, Alfred S McEwen
1Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA. chriso@lpl.arizona.edu
概括
在火星的Candor Chasma的关节沿线发现了局部流体改变区域. 这表明过去的地下液体通过裂流动,突出突破沉积物是研究火星地质水历史的关键地点.
科学领域:
- 行星科学 行星科学
- 地质地质地质地质地质地
- 天体生物学 天体生物学
背景情况:
- 火星的Candor Chasma中的分层沉积物保存了该星球地质过去的记录.
- 了解流体岩石相互作用对于破译火星水文历史至关重要.
研究的目的:
- 为了调查在西坎多尔沙斯马的分层沉积物中过去流体变化的证据.
- 为了确定断裂在火星地下流体迁移中的作用.
主要方法:
- 来自火星侦察轨道器 (MRO) 上的高分辨率成像科学实验 (HiRISE) 的色彩观测分析.
- 在分层沉积物中的接头沿着局部化和漂白区域的识别.
主要成果:
- 沿关节观察到局部流体变化的区域,包括凝固和漂白.
- 这些变化区域表明过去的地下流体迁移和凝固.
- 随后的侵蚀暴露了这些表面的地下变化特征.
结论:
- 沿断裂的流体流动是这些火星层层沉积物中地下流体迁移的重要机制.
- 分裂层层沉积物被确定为未来对火星水的地质历史调查的有希望的目标.
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