Investigation of the sources of volatile elements in fine-grained regolith on Mars
Year: 2026
Type: conference-abstract
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 (
DOI: 10.5194/epsc2026-99
Institutions: Centre National de la Recherche Scientifique, Institut de Recherche en Astrophysique et Planétologie, Lyon 1 Université, École Normale Supérieure de Lyon, Laboratoire de Géologie de Lyon : Terre, Planètes et Environnement, Université Jean Monnet, Observatoire de Paris, LIRA - Laboratoire d'instrumentation et de recherche en astrophysique, Purdue University West Lafayette
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: gold
OpenAlex ID: W4404750918
