PIA03496: Southern Hemisphere Polygonal Patterned Ground
Target Name: Mars
Is a satellite of: Sol (our sun)
Mission: Mars Global Surveyor (MGS)
Spacecraft: Mars Global Surveyor Orbiter
Instrument: Mars Orbiter Camera (MOC)
Product Size: 2235 x 1298 pixels (width x height)
Produced By: Malin Space Science Systems
Producer ID: MOC2-315
Primary Data Set: MGS EDRs
Full-Res TIFF: PIA03496.tif (2.906 MB)
Full-Res JPEG: PIA03496.jpg (915.9 kB)

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Original Caption Released with Image:

On Earth, periglacial is a term that refers to regions and processes where cold climate contributes to the evolution of landforms and landscapes. Common in periglacial environments on Earth, such as the arctic of northern Canada,Siberia, and Alaska, is a phenomenon called patterned ground. The "patterns" in patterned ground often take the form of large polygons, each bounded by either troughs or ridges made up of rock particles different in size from those seen in the interior of the polygon. On Earth, many polygons in periglacial environments are directly linked to water: they typically form from stresses induced by repeated freezing and thawing of water, contraction from stress induced by changing temperatures, and sorting of rocks brought to the surface along polygon boundaries by the freeze-thaw processes. Although not exclusively formed by freezing and thawing of water, that is often the dominant mechanism on Earth.

Polygons similar to those found in Earth's arctic and antarctic regions are also found in the polar regions of Mars. Typically, they occur on crater floors, or on intercrater plains, between about 60 and 80 latitude. The polygons are best seen when bright frost or dark sand has been trapped in the troughs that form the polygon boundaries. Three examples of martian polygons seen by the Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) are shown here. Each is located in the southern hemisphere:

  • (left) Polygon troughs highlighted by frost as the south polar cap retreats during spring. The circular features are the locations of buried craters that were originally formed by meteor impact. This image, E09-00029, is located at 75.1S, 331.3W, and was acquired on 1 October 2001.
  • (center) Summertime view of polygons, highlighted by dark, windblown sand, on the floor of a crater at 71.2S, 282.6W. The image, E12-02319, was obtained on 21January 2002.
  • (right) Polygon troughs highlighted by the retreating south polar frost cap during southern summer near 80.7S, 70.4W. This picture, M11-01795, was taken by MOC on 13 January 2000.
Some Mars researchers assume that polygons on the Red Planet are key indictors that ground ice is present or was present in the recent past. However, whether these polygons actually required water ice to form is, in fact, unknown, since dry processes are also known on Earth for form similar polygons.

Image Credit:
NASA/JPL/MSSS

Image Addition Date:
2002-06-07