NH4-Smectite, a Potential Source of N Compounds (NO) in SAM Analyses

Andrejkovičová, S ; McAdam, A C ; Stern, J C ; Knudson, C A ; Navarro-González, R ; Millan, M ; Wieman, S T ; Sebree, J A ; Bishop, N M ; Rampe, E B(NASA Johnson Space Center, Houston, TX, United States)

关键词: AMMONIA;    MONTMORILLONITE;    NITROGEN OXIDES;    CURIOSITY ROVER;    MARS SURFACE SAMPLES;    NASA SPACE PROGRAMS;   

RP-ID  :  LPI Contrib. No. 2083-1998,JSC-E-DAA-TN53574

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来源: NASA Technical Reports Server

【 摘 要 】

Recent detection of nitrate by Curiosity's Sample Analysis at Mars (SAM) instrument suite in Gale Crater sediments on Mars at abundances up to ~600 mg/kg indicates that nitrogen fixation processes occurred in early Martian history. But little is known about other possible N reservoirs on Mars, including those that may contain reduced forms of fixed N (i.e., NH3, NH4+) in the mantle, crust and sediments. Specifically, fixed nitrogen (i.e. NH3, NH4+, NOx or N that is chemically bound to either inorganic or organic molecules and can be released by hydrolysis to form NH3 or NH4+) is useful to terrestrial living organisms Therefore, understanding whether reduced N compounds such as NH4+ are present in surface materials is important to assess habitability in the Martian environment. While these species generally have short photochemical lifetimes, nitrogen in this form may be sequestered and stabilized in the soil by inclusion of NH4+ in certain phyllosilicates.