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This image in the Utopia Planitia region is marked by large somewhat circular pits roughly tens of meters (yards) deep, with scalloped edges. The presence of these pits has lead to hypotheses of the removal of subsurface material, possibly ice by sublimation (evaporation) since no channels are observed to imply melting. Close up, the upper surface is arrayed with a polygonal pattern of fractures in a variety of regular and irregular orientations. These fractures indicated that a competent or cohesive surface layer is present that has undergone stress, in much the same way paint cracks as it dries and shrinks. Although, in this geologic context of the middle latitudes of Mars, stress might be caused by subsidence, desiccation, or thermal contraction. The scalloped walls and some of the floor area of these pits are peppered with smaller polygonal patterns only 10 meters (yards) across. The change in crack pattern may indicate a change in the strength of subsurface material, a change in the forces inducing stress, or both. Other areas of the of the floors of these pits are hummocky with scattered rocks.
Image TRA_000856_2265 was taken by the High Resolution Imaging Science Experiment (HiRISE) camera onboard the Mars Reconnaissance Orbiter spacecraft on October 2, 2006. The complete image is centered at 46.0 degrees latitude, 92.0 degrees East longitude. The range to the target site was 301 km (188 miles). At this distance the image scale is 30 cm/pixel (with 1 x 1 binning) so objects ~90 cm across are resolved. The full image (shown at top) has been map-projected to 25 cm/pixel and north is up. The image was taken at a local Mars time of 3:17 PM and the scene is illuminated from the west with a solar incidence angle of 45.9 degrees, thus the sun was about 44.1 degrees above the horizon. At a solar longitude of 114.7 degrees, the season on Mars is Northern Summer / Southern Winter. |