Ontario Lacus

Smooth lines parallel to the current shoreline could be formed by low waves over time, which were likely driven by winds sweeping in from the west or southwest.

[3] Infrared observations show that the southwest shoreline of the lake receded 9–11 km over four years (2005-2009), evidently due to evaporation during the dry southern hemisphere autumn.

[6] Hydrological runoff models have found evidence for an extensive basin catchment area for the lake, suggesting seasonal rainfall may be responsible for filling liquids in the local depression.

[7] Any waves on the lake are also far smaller than those that would be on a sizable body of liquid water on Earth; their estimated maximum height was less than 3 mm during observations of a radar specular reflection during Cassini's T49 flyover of July 2009.

[5][8] In any case, the apparent presence of a wave-generated beach on the lake's northeast shore suggests that at times considerably higher waves form.

Infrared image of Titan's south polar region. Ontario Lacus is the dark feature at centre-left.
Radar image of Titan's south polar region, showing Ontario Lacus and surroundings. In the annotated version, the putative shoreline of a proposed former south polar sea of Titan is outlined.
The left and right images show the large catchment areas of Lake Eyre (dark grey region) and Ontario Lacus (red outline) respectively. In both cases, the lake area (blue, dashed ovals) is much smaller than the catchment area.