Titan's Dichotomy in Lake Distribution and its Astronomical Evolution

Mathematics – Logic

Scientific paper

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Scientific paper

Titan's hydrocarbon lakes exhibit a dramatic hemispheric asymmetry in their distribution. Liquid filled and empty lakes cover significant area fractions of the northern high latitudes, while the same southern latitudes are now known to be largely devoid of such features. Recently acquired SAR images in the southern hemisphere confirm early suggestions that, with approximately equal coverage of area sampled (>50%), a dichotomy is present in all lake types: filled lakes represent about 10% of the coverage area in the north compared with <0.1% in the south. Empty and granular lakes are each a factor of >5 more abundant in the north than in the south.
Here we propose that the observed difference in lake distribution may be caused by an asymmetry in Titan's seasons due to Saturn's orbital configuration, discuss quantitatively the feasibility of this new idea for Titan, and its predictable time dependence. The effect is modulated by, and reverses with, dynamical variations in the orbit. In this picture, much like in Earth's climate cycles, the resulting vigorous hydrologic cycle has a period of tens of thousands of years and leads to active geologic surface modification in the polar latitudes with that timescale. We discuss the possibility in light of the new data, new global circulation models, as well as the implications of possible hydrocarbon liquid level changes for this idea.

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