Add to ORKGThe weathering history of Mars can be deduced largely from the mineralogy and distribution of ferric oxide/oxyhydroxide phases. As discussed, some insights can be gained through spectrophotometric remote sensing, but absolute determinations must depend on direct laboratory analysis of returned Martian samples
organic matter on Mars, and both the Viking Labeled Release and Gas Exchange experiments indicated a...
International audienceVarious iron-bearing primary phases and rocks have been weathered experimental...
As the nearest planetary neighbor with potential earlier habitable conditions, Mars is replete with ...
We are performing oxidation and reduction reactions on hydrated ferric oxide minerals in order to in...
Transmission spectra of three ferric oxides (two alpha-Fe2O3 samples and one gamma-Fe2O3 sample) and...
The density and composition of the Martian atmosphere allow solar ultraviolet photons with wavelengt...
Bright regions on Mars are interpreted as 'soil' derived by chemical alteration of crustal rocks, wh...
The element iron plays a crucial role in the study of the evolution of matter from an interstellar c...
A mineralogical model for the Mars fine soil that includes as major components smectite clays absorb...
International audienceThe origin of iron bearing phases in the Martian regolith is usually interpret...
The reddened oxidized surface of Mars is indicative of temporal interactions between the Martian atm...
International audienceThe mineralogical composition of the Martian surface is constrained by analyzi...
Large areas of Mars' surface are covered by oxidative weathering products containing ferric and sulf...
[1] The most plausible models for the origin and evolution of a unique geologic unit in 7 Meridiani ...
The Mossbauer (MB) spectrometers on the Mars Exploration Rovers (MER) Spirit (Gusev crater) and Oppo...
organic matter on Mars, and both the Viking Labeled Release and Gas Exchange experiments indicated a...
International audienceVarious iron-bearing primary phases and rocks have been weathered experimental...
As the nearest planetary neighbor with potential earlier habitable conditions, Mars is replete with ...
We are performing oxidation and reduction reactions on hydrated ferric oxide minerals in order to in...
Transmission spectra of three ferric oxides (two alpha-Fe2O3 samples and one gamma-Fe2O3 sample) and...
The density and composition of the Martian atmosphere allow solar ultraviolet photons with wavelengt...
Bright regions on Mars are interpreted as 'soil' derived by chemical alteration of crustal rocks, wh...
The element iron plays a crucial role in the study of the evolution of matter from an interstellar c...
A mineralogical model for the Mars fine soil that includes as major components smectite clays absorb...
International audienceThe origin of iron bearing phases in the Martian regolith is usually interpret...
The reddened oxidized surface of Mars is indicative of temporal interactions between the Martian atm...
International audienceThe mineralogical composition of the Martian surface is constrained by analyzi...
Large areas of Mars' surface are covered by oxidative weathering products containing ferric and sulf...
[1] The most plausible models for the origin and evolution of a unique geologic unit in 7 Meridiani ...
The Mossbauer (MB) spectrometers on the Mars Exploration Rovers (MER) Spirit (Gusev crater) and Oppo...
organic matter on Mars, and both the Viking Labeled Release and Gas Exchange experiments indicated a...
International audienceVarious iron-bearing primary phases and rocks have been weathered experimental...
As the nearest planetary neighbor with potential earlier habitable conditions, Mars is replete with ...