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The Geology of Mars:
Seepage Channels?

Newton Crater
Newton Crater

Photographs taken might show evidence of relatively recent water erosion on Mars.  It was thought that all of the planet's water was locked up in the polar icecaps and in deep permafrost layers in the soil. However, images from about 120 sites show us features that may be evidence of recently flowing water.    
South Polar Pitted Walls
Nirgal Vallis
South Polar Pitted Walls   Nirgal Vallis

The features are landforms that appear to be gullies racing down cliff walls in canyons and canyons.  Each is composed of a deep channel with a collapsed region at the top (called an alcove) and at the other end an area of accumulated debris (called an apron).  The material at the apron appears to have been transported down the slope. This may be the result of liquid water, soil, rock and ice that has cut through the cliff face.

An area that is near a cliff face (canyon or crater wall) may experience some initial seepage (the cause is still unknown).  As the water evaporates, it cools the ground, freezing the water behind it, forming an ice barrier.  Pressure then builds up behind the 'ice dam' and eventually the dam bursts sending forth floods of water mixed with soil, ice and rocks forming a landslide. Since liquid water exposed to the Martian atmosphere would immediately begin to boil, scientists think that this boiling could be explosive and violent.  The sudden outbursts of water and debris might then be similar to flash floods on the Earth.

Gorgonum Chaos

 

 

 

 

 

 

 

Gorgonum Chaos

A different hypothesis is that the sublimation of ground ice - a change from solid to gas - loosened the landslide material, which then moved downslope.  This hypothesis does not include the presence of liquid water, merely the presence of underground ice deposits.

Martian Crater/Earth Volcano

 

 

 

 

 

 

Martian Crater/Earth Volcano

Interestingly these features are seen mostly in very cold areas. They are found in shadowed sides of crater and canyon walls, the sides that see less sunlight, and in latitudes higher than 30 degrees.  The reason is because frozen water escaping on the sunny side would instantly boil and evaporate into vapor because of the low atmospheric pressure on Mars, about 100 times less than it is at sea level on the Earth. 

Noachis Crater

 

 

 

 

 

 

Noachis Crater

The gullies look similar to gully washes seen in the American West.  The eruptions all seem to appear at approximately the same depth, about 100-500 meters down from the surface.  The gullies overlay all other features implying that they are, geologically speaking, relatively young.  Each flow that came down a gully may have had a volume of water of approximately 2,500 cubic meters (~90,000 cubic feet) or enough to supply 100 households for a month!

The presence of possible liquid water on Mars today has important implications for the question "Does Mars have life?"  If life did develop on Mars and has survived into the present, these landforms may be a good place to look.  In addition, if water is available in substantial amounts in other areas besides the polar caps then human crews could access and use it (for drinking, air to breath, and to create rocket fuel by extracting the oxygen and hydrogen).

Questions to think about: 

  • As an engineer or scientist on Earth, what types of robotic spacecraft and experiments could you devise to test out the hypothesis that liquid water was responsible for these gullies?
  • As an explorer on the surface of Mars, what types of vehicles or equipment would you need to explore these regions?
  • If water does exist on Mars at this depth and is near the surface in these regions, how would you recommend extracting it for use by humans?

Next... The Geology of Mars: Ice Caps (pg. 10 of 13)


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