Formation and Evolution of the Multi-Stage Peace Vallis Alluvial Fan System, Gale Crater, Mars

Z. G. Gallegos , H. E. Newsom (1) , L. A. Scuderi , R. C. Wiens (2) , J. A. Grant , O. Gasnault (3) , S. Le Mouélic (4) , S. E. Johnstone , K. Escarcega , E. Edge

1 IOM - Institute of Meteoritics [Albuquerque]
2 LANL - Los Alamos National Laboratory
3 IRAP - Institut de recherche en astrophysique et planétologie
4 LPG - Laboratoire de Planétologie et Géodynamique [UMR 6112]

The Peace Vallis alluvial fan is now recognized through this study as a complex, multi-stage system (Hesperian-Amazonian) with the investigation of rover-based ChemCam RMI imagery and orbital data.

Domaines: Planétologie

Z. G. Gallegos, H. E. Newsom, L. A. Scuderi, R. C. Wiens, J. A. Grant, et al.. Formation and Evolution of the Multi-Stage Peace Vallis Alluvial Fan System, Gale Crater, Mars. Ninth International Conference on Mars, Jul 2019, Pasadena, United States. ⟨hal-02411329⟩