This article presents an overview of the surface processes thought to be shaping the surface of Mars. Topics include wind and sand dunes, water and drainage channels, and the polar caps. Links to additional information are embedded in the text.
This description of a site outside SERC has not been vetted by SERC staff and may be incomplete or incorrect. If you
have information we can use to flesh out or correct this record let us know.
Subject: Geoscience:Lunar and Planetary Science, Geology, Hydrology Grade Level: High School (9-12), Middle (6-8) Theme: Teach the Earth:Course Topics:Hydrology/Hydrogeology, Planetary Science, Teach the Earth:Teaching Topics:WaterKeywords: Thaumasia Valley, Nirgal Vallis, Chryse Planitia, Kasei Valles, Ares Valles
