We investigate a new mechanism for producing oxidants, especially hydrogen peroxide (H2O2), on Mars. Large-scale electrostatic fields generated by charged sand and dust in the martian dust devils and storms, as well as during normal saltation, can induce chemical changes near and above the surface of Mars. The most dramatic effect is found in the pro-duction of H2O2 whose atmospheric abundance in the “vapor ” phase can exceed 200 times that produced by photochemistry alone. With large electric fields, H2O2 abundance gets large enough for condensation to occur, followed by precipitation out of the atmosphere. Large quantities of H2O2 would then be adsorbed into the regolith, either as solid H2O2 “dust ” or as re-evaporated vapor if the solid...
The factors governing the amounts of CO, O_2, and O_3 in the martian atmosphere are investigated usi...
Until recently, the chemistry of the atmosphere of Mars was believed to be straightforward, driven p...
Because H2 reacts efficiently with O+, CO2 +, CO+, and N2 +, the molecular hydrogen abundance assume...
Hydrogen peroxide (H2O2) has been suggested as a possible oxidizer of the martian surface. Photochem...
International audienceEver since the Viking mass spectrometer failed to detect organics on the surfa...
International audienceIn 1976, the Viking probes did not provide any results demonstrating the prese...
Laboratory studies, numerical simulations, and desert field tests indicate that aeolian dust transpo...
Freshly ground basaltic minerals produce sufficient quantities of hydrogen peroxide (H2O2) when imme...
The oxidation state of the Earth's surface is one of the most obvious indications of the effect of l...
HOx radicals are produced in the martian atmosphere by the photolysis of water vapor and subsequentl...
Internal reportAlready since the 1970s, hydrogen peroxide (H2O2) has been suggested as a possible ox...
The existence of methane in the Martian atmosphere is well established today. Several mechanisms hav...
International audienceDust storms on Mars play a role in transporting water from its lower to upper ...
While hydrogen peroxide (H2O2) has been detected in the martian atmosphere, it has not been detected...
The factors governing the amounts of CO, O_2, and O_3 in the martian atmosphere are investigated usi...
Until recently, the chemistry of the atmosphere of Mars was believed to be straightforward, driven p...
Because H2 reacts efficiently with O+, CO2 +, CO+, and N2 +, the molecular hydrogen abundance assume...
Hydrogen peroxide (H2O2) has been suggested as a possible oxidizer of the martian surface. Photochem...
International audienceEver since the Viking mass spectrometer failed to detect organics on the surfa...
International audienceIn 1976, the Viking probes did not provide any results demonstrating the prese...
Laboratory studies, numerical simulations, and desert field tests indicate that aeolian dust transpo...
Freshly ground basaltic minerals produce sufficient quantities of hydrogen peroxide (H2O2) when imme...
The oxidation state of the Earth's surface is one of the most obvious indications of the effect of l...
HOx radicals are produced in the martian atmosphere by the photolysis of water vapor and subsequentl...
Internal reportAlready since the 1970s, hydrogen peroxide (H2O2) has been suggested as a possible ox...
The existence of methane in the Martian atmosphere is well established today. Several mechanisms hav...
International audienceDust storms on Mars play a role in transporting water from its lower to upper ...
While hydrogen peroxide (H2O2) has been detected in the martian atmosphere, it has not been detected...
The factors governing the amounts of CO, O_2, and O_3 in the martian atmosphere are investigated usi...
Until recently, the chemistry of the atmosphere of Mars was believed to be straightforward, driven p...
Because H2 reacts efficiently with O+, CO2 +, CO+, and N2 +, the molecular hydrogen abundance assume...