Spatial resolution and the geologic interpretation of Martian morphology - Implications for subsurface volatiles

Details Spatial resolution and the geologic interpretation of Martian morphology - Implications for subsurface volatiles Spatial resolution and the geologic interpretation of Martian morphology - Implications for subsurface volatiles

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987icar...71..257z&link_type=abstract

(NASA, Lunar and Planetary Institute, and National Air and Space Museum, MECA Conference on Mars: The Evolution of Its Climate a

Mathematics

Logic

30

Mars Surface, Planetary Geology, Remote Sensing, Spatial Resolution, Viking Mars Program, Dunes, High Resolution, Morphology, Stereophotography, Tectonics, Mars, Morphology, Subsurface, Volatiles, Spacecraft Observations, Viking Missions, Orbiters, Imagery, Analysis, Image Processing, Maps, Dunes, Acheron Fossae, Hypotheses, Terrain, Topography, Photographs

Scientific paper

Viking Orbiter images with a spatial resolution >50 m/pixel provide valuable information about the tectonic and stratigraphic relationships of surface terrain units, but this resolution cannot provide strong constraints on the relative importance of geologic processes that have acted upon the surface. Images with a spatial resolution <10 m/pixel reveal the presence of features, such as small mounds interpreted to be aeolian dunes, that are significant to a complete evaluation of the surface history but which may be invisible at >50 m/pixel resolution. Landforms proposed as indicators of subsurface volatiles will only be as useful as the degree to which their geologic history can be assessed from the available image resolution.

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