在火星上的Meridiani Planum的岩基基质生成的火山环境
Thomas M McCollom1, Brian M Hynek
1Center for Astrobiology, University of Colorado, Boulder, Colorado 80309, USA. mccollom@lasp.colorado.edu
Nature
|December 24, 2005
概括
梅里迪亚尼平原的基石很可能是由火山灰与烟蒸气反应而形成的,而不是来自浅水. 这种新模型表明,古代火星环境的宜居性比以前想象的要低.
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:
- 梅里迪亚尼平面岩基岩显示了诸如血和硫酸盐之类的矿物质.
- 以前的解释表明,沉积在盐水中以蒸发或酸性矿井排水般的气候变化.
- 这些模型并不完全符合观察到的岩石化学.
研究的目的:
- 为梅里迪安尼平面 (Meridiani Planum) 基石提出一个替代的基因模型.
- 在不需要大量地表水的情况下解释观察到的矿物学和化学.
- 重新评估在Meridiani Planum的古代火星环境的可居住性.
主要方法:
- 从Meridiani Planum基岩中分析化学和矿物学证据.
- 开发一种涉及火山灰和烟雾蒸汽的基因模型.
- 拟议模型与以前的解释进行比较.
主要成果:
- 化学成分与浅水或酸性矿井排水模型不一致.
- 提出了一个涉及火山灰与二氧化硫和含水的烟雾蒸汽发生反应的替代模型.
- 这个过程可以在高温下发生,不需要长时间的地表水相互作用.
结论:
- 梅里迪亚尼平原 (Meridiani Planum) 的基石很可能是通过火山灰由烟雾气体形成的.
- 这种形成场景表明,过去生物活动的环境不如以前推断的那么有利.
- 修订了我们对水岩相互作用和早期火星可居住性的理解.
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