Liquid Elevations and Topographic Constraints of Titan's Lacustrine Basins at the end of Cassini: Hydrology and Formation

The topographic information provided by Cassini RADAR Altimetry, SAR Topography, and stereo photogrammetry has opened new doors for Titan research by allowing the quantitative analysis of morphologic form as well as relative measurements of liquid elevation. Herein, we investigate the relative elevation of liquid bodies and the three-dimensional morphology of Titan's lacustrine basins in order to provide observables that will constrain connectivity and plausible formation mechanisms. Using delay-Dopler processed altimetry measurements we show that the liquid elevations of Titan's Mare are the same to within measurement error, consistent with an equipotential surface. The liquid elevation of several smaller lakes, however, are found to be several hundreds above this sea level, suggesting that they exist in isolated or perched basins. Within a given topographic basin, the floor elevations of empty lakes are typically higher than the local liquid elevation, suggesting either the presence of an impermeable boundary or local subsurface connectivity. Basins with floors closer to the local phreatic surface appear brighter to both nadir and off-nadir microwave observations than those that are more elevated, indicating a potential change in composition. The majority of Titan's lakes reside in sharp edged depressions whose planform curvature suggests expansion through uniform scarp retreat. Many, but not all, of these basins exhibit flat floors and hundred-meter scale steep-sided raised rims that present a challenge to formation models. Raised rims are found on 57% of all the lakes in our study, including for all lakes >500 km2 in area. With super-resolution altimetry profiles, the raised rims can also be correlated directly with SAR image data, allowing for the identification of raised rims on other lakes, even when they lack topographic data coverage.. The basins are often topographically closed with no evidence for inflow or flow channels at the 300 m resolution of Cassini SAR images. The implications of these observations will be discussed in the context of common basin formation models. We conclude that sublimation and dissolution mechanisms can best match the observed constraints, but that challenges still exist in their implementation.