梅里迪安尼平面和火星的全球水文学
Jeffrey C Andrews-Hanna1, Roger J Phillips, Maria T Zuber
1McDonnell Center for the Space Sciences and the Department of Earth and Planetary Sciences, Washington University, St Louis, Missouri 63130, USA. jhanna@mit.edu
Nature
|March 9, 2007
概括
早期的火星地下水上升和蒸发,而不是封闭的盆地,可能形成了Meridiani Planum.
科学领域:
- 行星科学 行星科学
- 火星的探索火星的探索
- 地质地质地质地质地质地
背景情况:
- 火星探测车在Meridiani Planum发现了富含硫酸盐的沉积物.
- 证据表明,由波动的地下水表引起的基因改变.
- 初级颗粒可能源于平原蒸发物,但形成过程不清楚.
研究的目的:
- 研究Meridiani Planum的蒸发性沉积物的起源.
- 了解导致它们形成的水文过程.
- 探索全球水文学在火星早期环境历史中的作用.
主要方法:
- 早期火星全球水文学的数值模拟.
- 分析由降水和蒸发驱动的地下水流.
- 模拟Tharsis火山上升对含水层系统的影响.
主要成果:
- 预计Meridiani Planum已经经历了大量的地下水上游和蒸发.
- 全球地下水流是由降水引起的充电和蒸发性损失驱动的.
- 由于地下水持续上升而形成的蒸发性沉积物,而不是在封闭的盆地.
结论:
- 持续的地下水上升和蒸发解释了梅里迪亚尼的蒸发性沉积物.
- 蒸发石的形成与火星转向干旱的条件相吻合.
- 根深蒂固的全球水文学显著影响了火星表面早期的演变.
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