Cassini Data Unveils Complex Dynamics of Titan's Hydrocarbon Seas

New analysis reveals surface composition, wave activity, and currents in Titan's methane and ethane seas.

Cornell-led research used bistatic radar data from Cassini to study Titan's polar seas.
Hydrocarbon seas show varying compositions, with pure methane rivers mixing into ethane-rich seas.
Surface waves were generally small, but coastal areas showed higher roughness indicating tidal currents.
The study provides insights into Titan's meteorological models, suggesting methane-dominated precipitation.
Ongoing analysis of Cassini's data aims to uncover further details about Titan's unique environment.