稳定的甲水合物高于2GPa,也是泰坦大气中的甲来源
J S Loveday1, R J Nelmes, M Guthrie
1Department of Physics and Astronomy, University of Edinburgh, Mayfield Road, Edinburgh EH9 3JZ, UK. J.Loveday@ed.ac.uk
Nature
|April 5, 2001
概括
与之前的假设不同,甲水合物在泰坦内部的高压下保持稳定. 这种稳定性解释了月球大气中的甲,这表明月球冰层内有一层酸盐.
科学领域:
- 行星科学 行星科学
- 地质化学 地质化学
- 材料科学 材料科学 材料科学
背景情况:
- 甲水合物对于了解外行星及其卫星的形成至关重要.
- 之前的模型假定甲水合物在1-2 GPa的解离,这给泰坦大气中的甲带来了挑战.
- 泰坦大气层中甲的存在需要在其内部有一个稳定的来源.
研究的目的:
- 调查甲水合物在高压下与行星形成相关的热力学行为.
- 为了确定在泰坦内部的条件下甲水合物相的稳定性.
- 为了使观测到的泰坦大气中的甲与其形成历史相协调.
主要方法:
- 中子衍射研究.
- 同步射线X射线衍射研究.
- 在高达10 GPa的温度下对甲水合物的热力学分析.
主要成果:
- 甲水合物在大约1和2GPa时经历结构转变.
- 新的水合物相在高达至少10 GPa的压力下是稳定的.
- 这些发现与甲水合物的假设分离压力相矛盾.
结论:
- 泰坦核心的原始甲在分化过程中可能保持在稳定的水合物阶段.
- 大约100公里厚的甲酸盐层可能存在于泰坦的冰层中.
- 这种稳定的酸盐层为泰坦大气中的甲补充提供了一个合理的来源.
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