Gas-solid carbonation as a possible source of carbonates in cold planetary environments

Planetary and Space Science

Volumn 76, Issue 1, 2013, Pages 28-41

  Garenne, A ^a   Montes Hernandez, G ^a   Beck, P ^a   Schmitt, B ^a   Brissaud, O ^a   Pommerol, A ^b  

^a OBSERVATOIRE DE GRENOBLE   (France)

^b UNIVERSITY OF BERN   (Switzerland)

Author keywords

Ca and Mg hydroxides; Carbonates; Gas solid carbonation; Infrared microscopy; Low temperature; Mars

Indexed keywords

ALTERNATIVE PROCESS; AQUEOUS ALTERATION; AQUEOUS CONDITION; CARBONATE FORMATIONS; CARBONATION PROCESS; EXTRATERRESTRIAL ENVIRONMENTS; FORMATION MECHANISM; GAS-SOLID CARBONATIONS; HUMID ENVIRONMENT; INFRARED MICROSCOPE; INFRARED MICROSCOPY; LIQUID WATER; LOW TEMPERATURES; MARS; MARTIAN ATMOSPHERES; MINERAL GRAINS; MINERAL MATERIALS; MINERAL PRECURSOR; MINERAL SURFACES; NEGATIVE TEMPERATURES; ORBITALS; PHOENIX MISSION; PLANETARY ENVIRONMENTS; REACTION CELLS; REACTION UNDER; REDUCED CO; ROVER MISSIONS; SHAHEEN; SMALL CONCENTRATION; SUB-SURFACES; SURFACE PROCESS; TERRESTRIAL ENVIRONMENTS;

ATMOSPHERIC HUMIDITY; CALCIUM; CALCIUM CARBONATE; CARBON DIOXIDE; CARBONATE MINERALS; CARBONATES; CARBONATION; DUST; HYDRATION; ICE; PORE PRESSURE; SILICATES; SURFACES; TEMPERATURE;

PHASE INTERFACES;

EID: 84874112051     PISSN: 00320633     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.pss.2012.11.005     Document Type: Article

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