被冰覆盖的卫星的物理海洋学
Krista M Soderlund1, Marc Rovira-Navarro2, Michael Le Bars3
1Institute for Geophysics, Jackson School of Geosciences, University of Texas at Austin, Austin, Texas, USA;
Annual review of marine science
|September 5, 2023
概括
太阳系外围的巨大的冰月上有地下海洋. 研究人员正在探索独特的海洋学过程,如潮力和电磁,驱动这些外来海洋并影响可居住性.
科学领域:
- 行星科学 行星科学
- 海洋学 海洋学 海洋学
- 天体生物学 天体生物学
背景情况:
- 太阳系外层的许多冰星都有地表下的全球海洋.
- 这些外星海洋为研究物理海洋学提供了独特的环境.
- 它们挑战了关于海洋过程的以地球为中心的假设.
研究的目的:
- 审查冰雪月球上的海洋学驱动机制.
- 探索这些机制与地球的海洋有何不同.
- 评估对冰洋相互作用和可居住性的影响.
主要方法:
- 对行星海洋学现有文献的综述.
- 对冰月相关的物理海洋学过程的分析.
- 地球的海洋动态与外太阳系卫星的海洋动态的比较.
主要成果:
- 确定了诸如浮力驱动的流和潮之类的共同机制.
- 突出了对月球具有重要意义的独特机制: libration, precession 和电磁.
- 确定了这些过程对冰与海洋相互作用的重要性.
结论:
- 了解这些独特的机制对于研究冰冷的月球海洋至关重要.
- 这些力量的相互作用对可居住性有重大影响.
- 未来的任务应该调查这些过程,以测试海洋假设.
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