Extensive valley glacier deposits in the northern mid-latitudes of Mars: Evidence for Late Amazonian obliquity-driven climate change

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Radar evidence for ice in lobate debris aprons in the mid‐northern latitudes of Mars (2009, background): “…related to the presence of subsurface ice in the LDAs of this region and in LDAs elsewhere on Mars [e.g., Carr and Schaber, 1977; Squyres, 1978, 1979; Mangold and Allemand, 2001; Mangold, 2003; Pierce and Crown, 2003; Chuang and Crown, 2005; Head et al., 2005, 2006a, 2006b; Chuang and Crown, 2009].”
Geologic history of Mars (2010, background): “Indeed, Fassett and Head (2008a) mapped more than 210 open-basin lakes, including some that are the size of Lake Baikal or the Caspian Sea on Earth, and others that form continuous interconnected chains that extend across the surface toward the northern lowlands for distances typically of ∼1000 km, ”
SHARAD detection and characterization of subsurface water ice deposits in Utopia Planitia, Mars (2016, background): “It is hypothesized that much of the water ice deposited at high obliquity remains in the midlatitude subsurface and that this water ice is slowly being removed by sublimation [Clifford et al., 2010; Head et al., 2003, 2005, 2006; Madeleine et al., 2009; Mustard et al., 2001].”