Impact-generated hydrothermal systems capable of forming phyllosilicates on Noachian Mars

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Impact-generated hydrothermal systems on Earth and Mars (2013, background): “These observations are particularly important with respect to Mars, where the focus of impact-generated hydrothermal models has exclusively focused on crater interiors (e.g., Rathbun and Squyres, 2002; Abramov and Kring, 2005; Schwenzer and Kring, 2009).”
Subsurface water and clay mineral formation during the early history of Mars (2011, background): “These might produce clays near the hot central peak, beneath an impact melt sheet or in the lower crater wall”
Heterogeneous distribution of H2O in the Martian interior: Implications for the abundance of H2O in depleted and enriched mantle sources (2016, background): “…and Schwenzer 2013; Muttik et al. 2014), models of impact-induced hydrothermal systems (Newsom 1980; Newsom et al. 1996; Osinski et al. 2001; Schwenzer and Kring 2009), and observations of surface features such as recurring slope linea linked to seasonal brine flows and diurnal changes in…”