低温水性变化对氏体的变化
Martin R Lee1, Conel M O'D Alexander2, Addi Bischoff3
1School of Geographical & Earth Sciences, University of Glasgow, Glasgow, G12 8QQ UK.
概括
早期的太阳系小行星体经历了液态水的改变,正如体石所证明的那样. 本综述研究了这些低温水性变化反应的过程,产品和时间.
科学领域:
- 太空化学 太空化学
- 行星科学 行星科学
- 地质地质地质地质地质地
背景情况:
- 体石为早期在小物体上的液态水相互作用提供了关键证据.
- 了解水的变化是解读早期太阳系条件的关键.
研究的目的:
- 审查各种地石和小行星中低温水性变化的过程,产物和时间.
- 综合了解变化条件,流体特性和反应时间表的见解.
主要方法:
- 对地质石质,矿物学和岩石学的分析.
- 物理化学建模和热水实验.
- 液体包容分析和同位素地质化学 (Mn-Cr,I-Xe).
主要成果:
- 详细描述矿学和岩石学在水合的地石和黑暗的石块.
- 洞察水性流体的性质及其与母体材料的反应.
- 使用放射测年法对水性变化事件的时间约束.
结论:
- 水的变化是太阳系早期的一个重要过程,它塑造了小天体的组成.
- 本综述巩固了关于这些关键早期过程的条件,演变和时间的当前知识.
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