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The study of Martian geology provides valuable insights into Earth's past. Firstly, the similarities between the two planets' surface features suggest they underwent comparable geological processes in their early histories. For instance, the presence of ancient riverbeds and lake basins on Mars indicates it once had a warmer, wetter climate capable of sustaining liquid water on its surface, much like early Earth. [1] Secondly, the absence of active plate tectonics on Mars today can help us understand how Earth's surface evolved before the onset of plate tectonics. The predominance of impact craters and volcanic features on Mars resembles the early stages of Earth's geological evolution before plate tectonics began to reshape the planet's surface. P. Geo. Ricardo A Valls, M. Sc. and Geo Gadfly Valls Geoconsultant ORCID ID- https://orcid.org/0000-0002-5421-0914 Scopus Author ID: 7003369619/35335510700 ResearcherID: S-6604-2018 If you like this content, please "buy me a coffee" https://www.buymeacoffee.com/goldendroplets