Concentration of H, Si, Cl, K, Fe, and Th in the low- and mid-latitude regions of Mars

By W. Boynton, G. Taylor, L. Evans, R. Reedy, R. Starr, D. Janes, K. Kerry, D. Drake, K. Kim, R. M. E. Williams and 18 more. 2007

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Mapping the methane on Mars (2010, background): “The northern and northeastern regions of Arabia Terrae have been instead associated with an extensive subsurface deposit of permafrost (Boynton et al. 2007), while the corresponding surface is enriched in hydrated silicates (Mustard et al. 2008) and other water-related minerals such as carbonates…”
Emplacement of the youngest flood lava on Mars: A short, turbulent story (2010, background): “…(GRS) onboard the Mars Odyssey spacecraft provides abundances for select elements (Boynton et al., 1992); however, the instrument has an effective field of view of 500 km, and published maps are smoothed with a 900 km boxcar filter (Boynton et al., 2007), so the signal from Aav is not isolated.”
The composition of Mars (2019, unknown): “Taylor et al. (2010) used GRS data for Cl/K observed a ratio of 1.3 ± 0.2, comparable to the CI value (1.28), and yielded 0.5 wt% Cl in the BSM.”
Heterogeneous distribution of H2O in the Martian interior: Implications for the abundance of H2O in depleted and enriched mantle sources (2016, background): “FMM, PS, and JF acknowledge support from NASA’s Mars Fundamental Research Program through grant NNX13AG44G awarded to FMM and grant NNX13AG35G awarded to JF.”