Morphometry of Great Basin pluvial shore landforms: Implications for paleolake basins on Mars

Many basins with relict contributing valley networks and outlet valleys in the Martian highlands indicate past flowing and ponded water on the surface. These likely paleolakes motivate an investigation of pluvial shore landforms in the Great Basin region of the western United States, as confident identification of strandlines on Mars would facilitate analyses of its past hydrology and climate. The purpose of this study is to characterize the scale of Late Pleistocene erosional and depositional shore landforms in an endorheic setting, determine the preservation potential of similar forms from multiple epochs in early Martian history, and identify the data products that would be necessary to detect them. We use Differential Global Positioning System field surveys to measure the dimensions and elevations of shore landforms; compare shore platform widths to theoretical maxima; and note the minimum scale of landforms that have survived since the Late Noachian and Early Hesperian Epochs on Mars. We find that due to impact gardening and aeolian erosion, Martian highland paleolakes like those in the pluvial Great Basin would likely not have well-preserved shore landforms, unless they were unusually large and formed in the Late Hesperian or later. Individual strandlines are often not equally well expressed around an entire basin, so correlating shore landforms in plan view imaging and using their consistency in elevation as a hypothesis test for paleolakes can be challenging. Detection of younger shore landforms like those examined here would require meter-resolution imaging and topography such as stereo digital elevation models.