Martian Surface

The Martian surface is a rocky, dusty terrain marked by vast plains, towering volcanoes like Olympus Mons, and deep canyon systems like Valles Marineris. It features a thin atmosphere mainly of carbon dioxide, with signs of past water flows in dried riverbeds and mineral deposits. The landscape includes dust storms that can engulf the planet and seasonal polar ice caps composed of frozen water and carbon dioxide. Overall, Mars' surface is a harsh, geologically diverse environment shaped by volcanic activity, erosion, and limited liquid water, offering insights into its ancient climate and potential habitability.