WHAT DEPOSITIONAL PROCESSES AND PALEOENVIRONMENTS FORMED THE LAYERED SULFATE UNIT IN GALE CRATER, MARS ? : INSIGHTS FROM MARKER BAND VALLEY - Archive ouverte HAL
Communication Dans Un Congrès Année : 2023

WHAT DEPOSITIONAL PROCESSES AND PALEOENVIRONMENTS FORMED THE LAYERED SULFATE UNIT IN GALE CRATER, MARS ? : INSIGHTS FROM MARKER BAND VALLEY

Joel M Davis
Edwin Kite
Patrick J Gasda

Résumé

The stratigraphy of Aeolis Mons, Gale crater, is considered to provide a record of the possible ‘drying out’ of Mars with a temporal evolu-tion from clay-bearing mudstones, to sulfate-bearing rocks, to anhydrous minerals [1]. The Mars Science Laboratory Curiosity rover is investigating the deposi-tional environments of the layered sulfate-bearing unit considered to be from a ‘drier’ period than the underly-ing clay-bearing strata [1, 2, 3]. On sol 3560, Curiosity commenced exploration of the informally named Marker Band Valley (Figure 1) where the sulfate-bearing strata are exposed in local buttes. One of the overarching questions is what depositional environ-ments do the sulfate-bearing-units record. Here, we characterize the stratigraphic relations visible in these scarps and reconstruct processes of deposition of the sedimentary strata and their paleoenvironments.
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Dates et versions

hal-04052600 , version 1 (30-03-2023)

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Amelie L. Roberts, Sanjeev Gupta, William E. Dietrich, Lauren A. Edgar, William Rapin, et al.. WHAT DEPOSITIONAL PROCESSES AND PALEOENVIRONMENTS FORMED THE LAYERED SULFATE UNIT IN GALE CRATER, MARS ? : INSIGHTS FROM MARKER BAND VALLEY. 54th Lunar and Planetary Science Conference, Lunar and Planetary Institute, Mar 2023, The Woodlands (Texas), United States. pp.2945. ⟨hal-04052600⟩
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