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Martian Gullies
Discovered in Mars Global Surveyor images in 2000, gullies excited scientists because their formation probably involved the action of recent, liquid water.
Gullies are found on steep slopes and have a broad alcove at the top, deep V-shaped channels, and an apron at the base. The lack of many craters on and around them reveal their youth. The older a surface, the more craters it contains. On Mars everything gets quickly covered in bright dust. Since the gullies are often dark and dust-free, they could be just weeks old.
When first described, scientists believed they were due to aquifers--water bearing layers of rock. As more images poured in, other theories for their formation arose. One of the first alternative ideas was that gullies resulted from melting under a snow pack. The melting could occur from the pressure from the wieght of the snow and/or from heat flow from the planet. Some areas of Mars have what appear to be snowfields--they seem to cover the terrain, making it appear to be smooth.
Some researchers noticed the similarity between Martian gullies and debris flows in Greenland. The theory goes that when frozen soil on a steep slope melts, it will tend to move downhill and produce features that look identical to the gullies.
There are other ideas to explain these strange features, but at present , the cause or causes remain a tantalizing mystery. Because many of the explanations involve recent, liquid water, the gullies hold the focus of scientists.
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