在木星内部条件下发现与不混合的证据
S Brygoo1, P Loubeyre2, M Millot3
1Commissariat à l'Énergie Atomique, DAM/DIF, Bruyères-le-Châtel, France. stephanie.brygoo@cea.fr.
Nature
|May 27, 2021
概括
研究人员在极端条件下研究与的混合物, 他们发现了相隔区域, 影响了木星和土星内部的模型.
科学领域:
- 星球科学
- 在极端条件下的材料科学
- 计算物理
背景情况:
- - (H-He) 混合物的相位行为对于理解木星和土星等气体巨星的内部结构和演变至关重要.
- 在行星条件下的H-He相行为之前的研究由于实验和计算挑战而受到限制.
研究的目的:
- 在模拟木星和土星内部条件下实验地探测H-He混合物的相位行为.
- 限制与行星演化模型相关的H-He混合性差距.
主要方法:
- 使用激光驱动的冲击压缩预压缩的H2-He样品在钻石细胞中.
- 在极端温度和压力下 (高达150 GPa和10,200 K) 测试样品的性能,包括反射率.
主要成果:
- 在H-He混合物中确定了Hugoniot曲线的不混合区域.
- 在特定的压力-温度点上观察到不连续的反射变化,表明不混合区域的边界.
- 限制H-He相分离在10,200K时发生在150GPa以上,在4,700K时发生在93GPa以上.
结论:
- 关于H-He不混合性的实验限制支持木星内层模型.
- 据估计,H-He的相位分离会影响木星半径的15%.
- 这些发现为解释朱诺和利略任务的观测提供了微物理支持.
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