It's spring in the Northern Hemisphere of Mars (when this image was taken), and this area was recently completely covered by the seasonal frost cap. Here, we see polygonal patterns that are highlighted by carbon dioxide frost that has not entirely sublimed away. These organized patterns are likely caused by differences in the soil (regolith) characteristics such as grain size, density, even grain-shape and orientation in the underlying landforms and geologic materials. Variations in these characteristics strongly influence the strength of the ice-rich permafrost. This gives a preferred orientation to the stress field that produces the polygonal patterns. In this case, there appears to have been a meander in a fluvial channel in which sediments that differ from the native soil were deposited. The physical properties of these sediments probably change near the channel banks where flow rate drops off. Additionally, a high ice content might have resulted from a sediment-rich slurry flow th

It's spring in the Northern Hemisphere of Mars (when this image was taken), and this area was recently completely covered by the seasonal frost cap. Here, we see polygonal patterns that are highlighted by carbon dioxide frost that has not entirely sublimed away. These organized patterns are likely caused by differences in the soil (regolith) characteristics such as grain size, density, even grain-shape and orientation in the underlying landforms and geologic materials. Variations in these characteristics strongly influence the strength of the ice-rich permafrost. This gives a preferred orientation to the stress field that produces the polygonal patterns. In this case, there appears to have been a meander in a fluvial channel in which sediments that differ from the native soil were deposited. The physical properties of these sediments probably change near the channel banks where flow rate drops off. Additionally, a high ice content might have resulted from a sediment-rich slurry flow th
SuperStock offers millions of photos, videos, and stock assets to creatives around the world. This image of It's spring in the Northern Hemisphere of Mars (when this image was taken), and this area was recently completely covered by the seasonal frost cap. Here, we see polygonal patterns that are highlighted by carbon dioxide frost that has not entirely sublimed away. These organized patterns are likely caused by differences in the soil (regolith) characteristics such as grain size, density, even grain-shape and orientation in the underlying landforms and geologic materials. Variations in these characteristics strongly influence the strength of the ice-rich permafrost. This gives a preferred orientation to the stress field that produces the polygonal patterns. In this case, there appears to have been a meander in a fluvial channel in which sediments that differ from the native soil were deposited. The physical properties of these sediments probably change near the channel banks where flow rate drops off. Additionally, a high ice content might have resulted from a sediment-rich slurry flow th by Piemags/PL Photography Limited is available for licensing today.
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Image Number: 6145-45297964Royalty FreeCredit Line:Piemags/PL Photography Limited/SuperStockCollection:PL Photography LimitedStory:Martian Terrain and FossilsContributor:PiemagsModel Release:NoProperty Release:NoResolution:2880×1800