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Oceanography on Saturn's moon, Titan

机译:土星卫星泰坦上的海洋学

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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:长期以来,人们一直怀疑土星的寒冷卫星土卫六拥有甲烷和乙烷的液态海洋:卡西尼号航天器确定了这些海洋的存在和程度,并正在研究液态的海洋状态,深度和物理性质。土卫六的气象学导致两极地区的液体集中:迄今为止,对两个主要的北部海域海怪和利吉亚以及南部的一个浅湖安大略安大略湖进行了深入研究。泰坦是物理海洋学的新实验室,在非常陌生的条件下会发生熟悉的过程。

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