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Timescale for oceans in the past of Titan

✍ Scribed by Larsson, Richard; McKay, Christopher P.

Book ID
121410548
Publisher
Elsevier Science
Year
2013
Tongue
English
Weight
327 KB
Volume
78
Category
Article
ISSN
0032-0633

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We have developed a coupled atmosphere and ocean model of Titan's surface. The atmospheric model is a 1-D spectrally-resolved radiative-convective model. The ocean thermodynamics are based upon solution theory. The ocean, initially composed of CH4, becomes progressively enriched in ethane over time.