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This image shows the rock Yogi and tracks from the Rover.
Click on image for full size
Courtesy of NASA

Weathering processes on Mars

Unlike the rocks of Earth, where there are many things which cause erosion, there are only two main weathering agents on Mars: wind and acid fog. Acid fog is very important, but because there is not a lot of water, the action of sand and wind is the most important thing to cause changes to the planet's surface.

Wind erosion of Mars was examined in the Mars Pathfinder mission. Rocks examined by the Pathfinder's Rover found evidence of the following erosion features:

A wind tail is shown in the lee of the rock "Yogi" in the picture to the left.

Sand and dust from the surface is whipped up by the winds of Mars and distributed around the globe in global dust storms. The force of winds during these storms pounds sand into the rock formations, contributing toward the breakdown and recycling of the Martian surface.

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Windows to the Universe, a project of the National Earth Science Teachers Association, is sponsored in part is sponsored in part through grants from federal agencies (NASA and NOAA), and partnerships with affiliated organizations, including the American Geophysical Union, the Howard Hughes Medical Institute, the Earth System Information Partnership, the American Meteorological Society, the National Center for Science Education, and TERC. The American Geophysical Union and the American Geosciences Institute are Windows to the Universe Founding Partners. NESTA welcomes new Institutional Affiliates in support of our ongoing programs, as well as collaborations on new projects. Contact NESTA for more information. NASA ESIP NCSE HHMI AGU AGI AMS NOAA