Martian Eolian Dust Analyzed by ChemCam

J. Lasue*, A. Cousin, P. Y. Meslin, N. Mangold, R. C. Wiens, G. Berger, E. Dehouck, O. Forni, W. Goetz, O. Gasnault, W. Rapin, S. Schröder, A. Ollila, J. Johnson, S. Le Mouélic, S. Maurice, R. Anderson, D. Blaney, B. Clark, S. M. CleggC. d'Uston, C. Fabre, N. Lanza, M. B. Madsen, J. Martin-Torres, N. Melikechi, H. Newsom, V. Sautter, M. P. Zorzano

*Corresponding author for this work

Research output: Contribution to conferencePaper

Abstract

The martian eolian dust chemical composition is homogeneous at the sub- mm scale. It is different from the Aeolis Palus soils and Bagnold sands with a larger content of FeO, TiO2 and lower hydration.
Original languageEnglish
Number of pages2
Publication statusPublished - Jul 2019
EventNinth International Conference on Mars, held 22-25 July, 2019 in Pasadena, California - California Institute of Technology , Pasadena , United States
Duration: 22 Jul 201925 Jul 2019
Conference number: 31488-19
https://www.hou.usra.edu/meetings/ninthmars2019/

Conference

ConferenceNinth International Conference on Mars, held 22-25 July, 2019 in Pasadena, California
CountryUnited States
CityPasadena
Period22/07/1925/07/19
Internet address

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