Using ChemCam LIBS data to constrain grain size in rocks on Mars: Proof of concept and application to rocks at Yellowknife Bay and Pahrump Hills, Gale crater

Frances Rivera-Hernández (1) , Dawn y Sumner (1) , Nicolas Mangold (2) , Kathryn M Stack (3) , Olivier Forni (4) , Horton Newsom , Amy Williams , Marion Nachon (5) , Jonas L'Haridon (2) , Olivier Gasnault (4) , Roger Wiens (6) , Sylvestre Maurice (4)

1 UC Davis - University of California [Davis]
2 LPG - Laboratoire de Planétologie et Géodynamique [UMR 6112]
3 JPL - Jet Propulsion Laboratory
4 IRAP - Institut de recherche en astrophysique et planétologie
5 CS - UC Davis - Department of Computer Science [Univ California Davis]
6 LANL - Los Alamos National Laboratory

Domaines: Planète et Univers [physics]; Planétologie

Frances Rivera-Hernández, Dawn y Sumner, Nicolas Mangold, Kathryn M Stack, Olivier Forni, et al.. Using ChemCam LIBS data to constrain grain size in rocks on Mars: Proof of concept and application to rocks at Yellowknife Bay and Pahrump Hills, Gale crater. Icarus, 2019, 321, pp.82-98. ⟨10.1016/j.icarus.2018.10.023⟩. ⟨hal-02933737⟩