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The Synthetic Aperture Radar (SAR) instrumentation on board the Cassini orbiter has identified large hydrocarbon liquid deposits on the surface of Titan [e.g. 1], distributed mainly around its northern polar regions. Recent studies  suggest that the rims of these structures display seasonal changes, where the lakes appear to be shrinking. However, the precise depth, evolution and composition of these lake-like features are still unknown. The physical and chemical characteristics of the Titan lakes will be one of the major objectives of a future space mission to Titan [e.g. 3, 4]. We propose here the application of Micro-Electro-Mechanical Systems (MEMS) as part of a science surface properties package aboard a future Lake Lander. MEMS devices offer a low cost and reduced size of instrumentation in order to accomplish the 3-D sounding of the liquid deposit and detect the presence of any biomarkers in a broader area.