火星水库的演变来自大气和地中的D/H比率
1Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor 48109, USA.
Nature
|March 30, 1995
概括
根据新的石数据,古老的火星拥有巨大的水库,可能有数百米的深度. 这支持地质证据,一个曾经是潮湿的星球,解决大气中的气逃脱差异.
科学领域:
- 行星科学 行星科学
- 地质化学 地质化学
- 天体生物学 天体生物学
背景情况:
- 古老的火星上有河流网络,这表明超过30亿年前的温暖,潮湿的过去.
- 地质证据表明,近期,火星地中数百米深的全行星水库.
- 大气中的气逃逸率和同位素分数表明过去和现在的地水体积小得多 (0.5-6米).
研究的目的:
- 为了协调地质水估计和火星大气中的气数据之间的差异.
- 利用来自SNC石的新与比测量来限制火星水库的演化.
主要方法:
- 在SNC石 (火星起源) 中的含水矿物中分析与的比率.
- 基于同位素组成和大气逃逸率的地水库大小的建模.
主要成果:
- 新的石数据需要大规模的现代火星地水库 (至少几米深).
- 火星大气中的丰富表明,古老的地水库深达数百米.
- 这些发现与火星上大量古代水的地质证据一致.
结论:
- 在SNC石中与的比率为火星水的历史提供了关键的限制.
- 现在,地质和同位素证据都一致指出,古火星上存在着大量的水库.
- 了解火星水的演变是评估其过去可居住性的关键.
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