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Oceanography on Saturn's moon, Titan

机译:土星月亮的海洋学,泰坦

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Saturn's frigid moon Titan was long suspected to have seas of liquid methane and ethane: the existence and extent of these seas has been determined by the Cassini spacecraft, and sea state, depth and the physical properties of the liquid are being learned. Titan's meteorology leads to concentration of liquid in the polar regions: two major northern seas, Kraken and Ligeia, and one shallow lake in the south, Ontario Lacus, are particularly well-studied to date. Titan serves as a new laboratory for physical oceanography, with familiar processes occurring under very alien conditions.
机译:土星的寒冷月亮泰坦长期怀疑有液体甲烷和乙烷的海洋:这些海洋的存在和程度已经由Cassini航天器确定,海区,深度和液体的物理性质正在学习。泰坦的气象导致极地地区的液体集中:两个主要的北部海洋,克拉伦和灯塔,以及南部的一个浅湖,迄今为止尤其研究。泰坦作为物理海洋学的新实验室,熟悉的过程在非常外国条件下发生。

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