Mars may not serve as a pre-tectonic model for Earth due to its distinct geological features. The planet exhibits a dichotomy between its southern and northern hemispheres, characterized by a thick, heavily cratered crust in the south and a younger, thinner crust in the north. Evidence of strong residual magnetism and early spreading ridges suggests past tectonic activity, while features like the Tharsis bulge and Olympus Mons indicate a history of volcanism rather than a primitive state. Mars is considered post-tectonic, likely influenced by its smaller mass, which affects the thermal dynamics of its core and mantle. The discussion raises questions about the definition of tectonic activity, suggesting that volcanic activity may be a more appropriate term for Mars, despite evidence of tectonic processes in its history.