1. Going With the Flow: Sedimentary Evolution of the Jezero Western Fan, Mars
- Author
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S Gupta, K Stack Morgan, N Mangold, L R W Ives, S Gwizd, R M E Williams, N Randazzo, A J Williams, P Russell, B H N Horgan, K L Siebach, M M Tice, J Hurowitz, R Barnes, C Tate, J I Núñez, S Sholes, L C Kah, M E Minitti, G Dromart, J F Bell, III, J Maki, G Paar, A Annex, B P Weiss, O Beyssac, J Frydenvang, M Nachon, R Kronyak, V Sun, A J Jones, D L Shuster, J I Simon, M P Lamb, J P Grotzinger, S Le Mouélic, O Gasnault, R C Wiens, S Maurice, and K A Farley
- Subjects
Lunar and Planetary Science and Exploration - Abstract
Sedimentary fans developed at the mouths of Martian valleys have been interpreted as the deposits of sustained surface water flow on early Mars building either fluvial fan systems or deltas into standing bodies of water. Whilst much insight has been gleaned from orbital observations, it is only possible to constrain the character, relative timing and persistence of ancient aqueous activity on Mars through detailed on-the-ground interrogation of sedimentary successions built during fan growth. A prominent sedimentary fan deposit at the western margin of Jezero crater – the Western fan – has been interpreted from orbital data/observations to be a river delta that prograded into an ancient lake basin during the Late Noachian-Early Hesperian epochs on Mars (~3.6-3.8 Ga). The Western fan deposit forms a point-sourced depositional system developed at the mouth of Neretva Vallis, a valley system that is incised across the crater rim and has an extensive extra-crater catchment draining over diverse ancient geological units in Nili Planum. The mechanism of crater rim breaching remains unconstrained. Between 2022 and 2023, the Mars 2020 Perseverance rover explored the Western fan, with the objective of characterizing its paleoenvironmental context and collecting a diverse suite of sedimentary rock samples for return to Earth via the Mars Sample Return mission. Perseverance has now completed her traverse across the Western fan having commenced in the distal downstream sectors exposed at the erosional front of the fan and then crossing across its upper exposed surface toward the fan apex region near the mouth of Neretva Vallis. This transect provides a unique window into a Martian sediment routing system at a time when climate conditions permitted the flow of surface water. In this contribution, we review the overall sedimentary architecture of the fan and develop a model for its evolution based on detailed mapping of lithofacies changes across the fan. A first-order synoptic overview is presented.
- Published
- 2024