Mars’ surface reveals a dynamic history shaped by impact cratering, volcanism, and wind-driven (aeolian) processes. Impact craters form from high-velocity collisions, producing shockwaves, ejecta, and distinct simple or complex structures, while also exposing subsurface materials. Unlike the airless Moon rampart and pedestal craters suggest the presence of subsurface ice and highlight interactions between impacts and volatiles. Crater degradation over time reflects climatic and geological changes, and crater counting provides a key method for estimating surface ages. Volcanism has resurfaced much of Mars, forming shield volcanoes, lava plains, and features linked to both effusive and explosive eruptions. Interactions between lava, water, and tectonics—seen in regions like Tharsis and Cerberus Fossae—indicate a complex and possibly still active interior. Aeolian processes, including dunes, ripples, and yardangs, actively reshape the present-day surface, offering insights into both present and past Martian climate conditions.