Surficial units on titan: equatorial dunes and polar lakes and seas... These lacustrine features cover more than 13% and 1% of the northern and southern polar regions, respectively....
Martian surface/near-surface water inventory: sources, sinks, and changes with time... Our estimate of approximately 24m near-surface water in the Late Noachian is insufficient to support an ocean at that time also and favors episodic melting of an icy highlands to produce the fluvial and lacustrine features....
Sediment transport and aqueous alteration in a mars-analog glacial system... Moreover, climatic models have suggested that the early Martian climate was not warm and wet, but cold and icy, with some of the apparent fluvial and lacustrine features attributable to transient melting of ice sheets as opposed to persistent surface water....
The climate history of early mars: insights from the antarctic mcmurdo dry valleys hydrologic system... We review a series of MDV fluvial and lacustrine features to guide investigators in the analysis of the geomorphology of early Mars and we outline a new model for the nature and evolution of a “cold and icy ” Late...
