Investigation of the sources of volatile elements in fine-grained regolith on Mars

2026 Open access

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Authors: A. Cousin, W. Rapin, P.Y. Meslin, E. Dehouck, O. Forni, G. David, P. Pilleri, R. C. Wiens, Olivier Gasnault
DOI: 10.5194/epsc2026-99
Cited by: 0

Abstract

Introduction: Martian regolith [1] is constituted with different mineral phases of various grain sizes that could originate from local, regional or global sources [2,3]. It corresponds to the ultimate stage of various erosion and weathering processes. Dust (

Fields of Study & Subjects

Planetary Science and Exploration

Publication details

Publication date
2 July 2026
Language
EN