概括
表面氧化在火星上显著耗尽水 (H2O),比以前想象的更快地去除它. 这一过程可能影响了火星土壤和冰盖在地质时间上的水的可用性.
科学领域:
- 行星科学 行星科学
- 天体生物学 天体生物学
- 地质化学 地质化学
背景情况:
- 外层逃逸被认为是火星不可逆转的水损失的主要机制.
- 以前的估计表明,每平方厘米每秒的水损失率约为108个分子.
研究的目的:
- 为了量化火星大气层因表面氧化而流失水的速度.
- 为了比较这种损失率与外层逃逸,并评估其对火星水历史的意义.
主要方法:
- 对火星大气组成和表面过程的分析.
- 参与表面氧化和水损失的化学反应的建模.
主要成果:
- 表面氧化以每平方厘米每秒10~8~10~11个分子的速度从火星大气中去除氧气和气.
- 这相当于在地质时间内净损失10~25~10~28 H2O分子 (10~2~10~5) g/cm2,假设损失均.
- 通过表面氧化计算的损失率明显超过了外层逃逸的损失率.
结论:
- 表面氧化是火星大气中的水的主要,以前被低估的,不可逆转的沉没点.
- 这一过程可能在塑造地球的水库中发挥了比外层逃逸更重要的作用.
- 表面氧化可能影响了火星细流体和极地冰盖中的水的可用性.
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