HIGHLIGHTS
SUMMARY
Salts have been detected on the surface of Mars and are widely distributed (Clark and Kounaves, 2016; Gasda et_al, 2017; Gendrin, 2005; Hecht et_al, 2009; Rivera-Valentín et_al, 2020; Thomas et_al, 2019). This incorporation widens the domain of liquid stability of the solution, therefore brines would be more stable than pure water on the surface of Mars (Brass, 1980; Davila et_al, 2010; Fischer et_al, 2016; RiveraValentín et_al, 2020). In this context, several experimental studies have reported on sediment transport by water under Martian conditions (Massé et_al, 2016; Raack et_al, 2017; Herny et_al . . .
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