According to new research published in the journal Nature, lava flows possibly originating from the Jezero Mons on Mars could have shaped the geology of the Jezero crater’s floor. According to the findings, the analysis of NASA's Perseverance rover samples could also reveal clues about ancient Mars when it was still geologically active.

The study was led by Sara C. Cuevas-Quiñones, a Ph.D. Planetary Science student from Georgia Tech’s School of Earth and Atmospheric Sciences (EAS) and Brown University. The research team also included EAS Professor James Wray and EAS Assistant Professor Frances Rivera-Hernández. 

As Cuevas-Quiñones and her colleagues note in their paper, the detection of clay and carbonate minerals on Jezero crater's floor supports the conclusion that the sedimentary deposits on the crater's western edge are the result of aqueous activity that took place roughly 3.8 to 3.5 billion years ago. In addition, satellite observations have revealed a set of non-sedimentary geologic materials that cover most of the Jezero crater's floor.