火星石ALH84001中碳酸盐的可能高温起源
1Department of Geological Sciences, Case Western Reserve University, Cleveland, Ohio 44106-7216, USA. rph@po.cwtu.edu
Nature
|July 4, 1996
概括
火星石艾伦·希尔斯 84001碳酸盐可能是在撞击事件中由热,富含二氧化碳的液体形成的,而不是低温水. 这种冲击性体化解释了它们的组成和矿物分区.
科学领域:
- 行星科学 行星科学
- 地质化学 地质化学
- 矿物学是什么?矿物学是什么?
背景情况:
- 艾伦·希尔斯 (ALH) 84001石,火星起源,含有独特的区域,地球前碳酸盐矿物质.
- 以前的氧同位素研究表明,火星地中的低温 (0-80°C) 水性流体沉.
研究的目的:
- 分析ALH 84001碳酸盐的主要元素组成.
- 为了独立地限制碳酸盐形成的流体的组成和温度.
- 为了评估观察到的碳酸盐特征的替代形成机制.
主要方法:
- 在ALH 84001石中分析碳酸盐矿物的主要元素组成.
- 观察到的组成与各种地质模型的预测进行比较.
主要成果:
- 碳酸盐成分与低温水性流体沉不一致.
- 观察到的矿物学和区分最好通过热 (>650°C),富含二氧化碳的流体和宿主岩石之间的反应来解释.
- 缺少并存的含水矿物质支持一个高温,冲击驱动的形成场景.
结论:
- 在ALH 84001中的碳酸盐很可能是在高温事件中通过冲击元体形成的.
- 冲击过程提供了一个合理的机制来产生所需的热,富含二氧化碳的流体和流体通路.
- 这种形成模型协调了碳酸盐中观察到的氧同位素不平衡,矿物序列和分区模式.
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