Spectral and geological study of the sulfate-rich region of West Candor Chasma, Mars

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Large-scale spring deposits on Mars? (2008, background): “[47] LTDs in Valles Marineris postdate the canyon formation, and although this has been previously challenged [Catling et al., 2006; Malin and Edgett, 2000; Montgomery and Gillespie, 2005; Schultz, 1998] there are strong evidences of a post-canyon formation of ILDs [Lucchitta et al., 1992; Lucchitta”
A synthesis of Martian aqueous mineralogy after 1 Mars year of observations from the Mars Reconnaissance Orbiter (2009, background): “Higher–spatial resolution data from OMEGA showed that finer-grained, red ferric minerals (possibly oxides) occur in the ILDs and are concentrated, probably by mass wasting, in aprons around the eroded plateaus [Gendrin et al., 2005b; Bibring et al., 2007; Mangold et al., 2008].”
The Sample Analysis at Mars Investigation and Instrument Suite (2012, background): “2009), or (3) recent surficial hydration state ::hanges (Mangold et al. 2008)].”
Multi- and hyperspectral geologic remote sensing: A review (2012, unknown): “, 2008 , Mars and Crowley , 2003 ) .”