Planum Australe

The geology of this region was to be explored by the failed NASA mission Mars Polar Lander, which lost contact on entry into the Martian atmosphere.

[1][2][3][4] Planum Australe is partially covered by a permanent polar ice cap composed of frozen water and carbon dioxide about 3 km thick.

[9][10][11] In 1966, Leighton and Murray proposed that the Martian polar caps provided a store of CO2 much larger than the atmospheric reservoir.

[17] Then, sublimed CO2 (and probably water) increase pressure in their interior, producing geyser-like eruptions of cold fluids often mixed with dark basaltic sand or mud.

[18][19][20][21] This process is rapid, observed happening in the space of a few days, weeks or months, a growth rate rather unusual in geology – especially for Mars.

[22][23] In September 2020, scientists confirmed the existence of several large saltwater lakes under the ice in the south polar region of the planet Mars.

Site of south polar subglacial water body (reported July 2018)
Elevation map of the south pole. Note how Planum Australe rises above the surrounding cratered terrain. Click to enlarge and for more info.
Depiction of erupting south polar sand-laden jets ( Ron Miller )
Close up of "dark dune spots" created by geyser-like systems