冲击压缩液态的温度测量:对木星内部的影响
W J Nellis1, M Ross, N C Holmes
1Lawrence Livermore National Laboratory, University of California, Institute of Geophysics and Planetary Physics and H Division, Livermore 94550, USA.
概括
冲击压缩实验显示,由于分离相位过渡,在高压下气温度低于预测. 这一发现影响了我们对木星内部结构和温度变化的理解.
科学领域:
- 高压物理学的高压物理
- 星球科学 星球科学
- 材料科学是一种材料科学.
背景情况:
- 了解在极端条件下的行为对于行星科学至关重要.
- 之前的模型预测,在千兆帕斯卡压力下,的温度会更高.
研究的目的:
- 在极端压力下实验测量的冲击温度.
- 调查预测和测量温度之间的差异的原因.
- 将这些发现应用于行星内部模型,特别是木星.
主要方法:
- 对高达5200K的冲击温度进行光学测量.
- 使用冲击压缩,达到高达83千兆帕斯卡尔 (830千瓦) 的压力.
- 分析冲击压缩中的热平衡.
主要成果:
- 在最高压力下测量的温度明显低于理论预测.
- 确定了20千兆帕斯卡尔以上的中的连续解离相过渡是原因.
- 木星的分子外可能比以前认为的温度变化较小,更冷.
结论:
- 中的分离相过渡挑战了木星分子地幔和金属核心之间的尖界限的概念.
- 在木星的分子区域内可能存在一个静止的边界层.
- 冲击数据为行星内部的修订理论提供了基础.
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