在火星上形成水热碳酸盐的地球化学模型
1Department of Earth and Planetary Sciences, McDonnell Center for the Space Sciences, Washington University, St. Louis, Missouri 63130, USA.
Nature
|October 5, 1995
概括
火星可能已经失去了大量的二氧化碳和水. 水热碳酸盐为火星表面下这些挥发性物质的隔离提供了一个合理的解释.
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:
- 大量的二氧化碳和水从火星大气层,极地盖和冰岩中消失了.
- 大气逃逸和表面沉积物不能完全解释这些挥发物质的不足.
- 以前的模型表明,火星的长期地表水或降雨不太可能发生.
研究的目的:
- 为了研究水热系统在火星上隔离二氧化碳的潜力.
- 为了建模火星水热环境中碳酸盐的形成.
主要方法:
- 利用冰岛作为陆地热水过程的类似物.
- 使用地质化学建模.
- 推断来自火星石的宿主岩石组成.
主要成果:
- 热水碳酸盐的形成是一个可行的机制,用于隔离大量的二氧化碳.
- 模型表明,潜在的地下储备相当于大气中至少一二氧化碳.
- 火星过去广泛的热水活动可以解释失踪的挥发性物质.
结论:
- 水热碳酸盐为火星的挥发性赤字提供了一个令人信服的解决方案.
- 通过热水活动的地下封存提供了对表面储存解释的替代方案.
- 这种机制突显了过去的热水过程在火星地质历史中的重要性.
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