Preserved in the sedimentary rock record of Mars is an ancient (>3 Ga) history of fluvial activity that persisted long enough to create landforms and layered sequences that suggest both subaerial and subaqueous deposition (Malin & Edgett, 2000, 2003). Geomorphological features observed from orbit provide evidence for extensive fluviolacustrine processes, as evidenced by channelized flow features and delta-like distributary fans (Hynek et al., 2010; Milton, 1973; Sharp & Malin, 1975). On the ground, sedimentological observations by the Curiosity rover include conglomerates, sandstones, and mudstones interpreted to have fluviolacustrine origins (e.g., Grotzinger et al., 2014, 2015). Geochemical and mineralogical investigations of these fluviolacustrine sedimentary rocks have revealed sediment interaction with surface and ground waters in