Understanding the cycle of sediments to become sedimentary rocks that might preserve organic compounds and biosignatures, and how these rocks then become exposed at the surface for study and sampling, is essential to guide rover exploration. The Curiosity rover benefitted from this knowledge in its discovery of preserved organics (Eigenbrode et al., 2018;Freissinet et al., 2015). The study of sedimentary rocks and processes on Mars, as on Earth, must necessarily involve analysis of the characteristic attributes of strata as well as their bounding surfaces, which in all cases represent some degree of temporal discontinuity (Sadler, 1981). Early studies of Martian strata showed that sedimentation was discontinuous, as revealed, for example, by the break in accumulation implied Abstract Sedimentary rocks record the ancient climate of Mars through changes between subaqueous and eolian depositional environments, recognized by their stratal geometries and suites of sedimentary structures. Orbiter-and rover-image-based geologic mapping show a dynamic evolution of the 5-km-thick sedimentary sequence exposed along the flanks of Aeolis Mons (informally, Mt. Sharp) in Gale crater, Mars, by deposition of subaqueous strata followed by exhumation via eolian erosion and then deposition of overlying, onlapping strata of inferred eolian origin. This interpretation suggests that a significant unconformity should occur at the base of the onlapping strata, thus predicting lateral variations in elevation along the contact between the underlying Mt. Sharp group and overlying Stimson formation. Curiosity rover and high-resolution orbital image data quantify paleotopographic variability associated with the contact; ∼140 m of net elevation change and a slope closely aligned with the modern topography is expressed along the regional contact. These results support the interpretation of an erosional unconformity between these strata and that it was likely formed as a result of eolian erosion within the crater, indicative of a transition from wet to dry climate and providing insight into the stratigraphic context, geologic history, and habitability within Gale crater.
Plain Language SummaryThe discovery of sedimentary rocks on Mars is relatively recent. On a planet that apparently lacked plate tectonics, one important question is whether or not there is a rock cycle in which sediments become rocks that then are exhumed and recycled back into the crust through renewed burial. Rover missions have confirmed the existence of the first part of this cycle-erosion, transport, deposition, and burial. However, the second half of the cycle, which begins with exhumation, is poorly constrained. The work presented here demonstrates the presence of ancient surfaces of erosion-unconformities-that mark past exhumation events at Gale crater. Furthermore, the ancient erosion surface is then overlain by a younger series of sedimentary rocks, which demonstrates burial of that unconformity surface and the completion of the rock cycle. On Earth, exhumation is dri...