Acid-sulfate Weathering of Synthetic Martian Basalt: the Acid Fog Model Revisited
نویسندگان
چکیده
Introduction: One of several models that has been proposed to explain the present chemical and minera-logical nature of the Martian surface is referred to as the " acid-fog " model. This model involves the recent (up to 1Ga), slow and continuous interaction of acidic volatiles, presumably of volcanic origin, with the exposed Martian basaltic crust [1, 2]. As a result of this interaction, mineral dissolution occurs and subsequent evaporation of the fluid results in formation of evaporite salts. Banin et al. [2] have tested the acid-fog model experimentally by interacting terrestrial analog basalt with sulfuric, hydrochloric and nitric acid mixtures and found that upon fluid evaporation, the Ca and Al-sulfate salts gypsum and alunogen precipitated as secondary mineral phases with no other phases detected by X-ray diffraction. The study presented here revisits this model using more relevant Martian basaltic analogs synthesized in the laboratory. Results show that the chemical and mineralogical composition of the basaltic analog material is critical in determining fluid chemistry and the subsequent secondary products that are formed. Different chemical compositions of basaltic analogs are used in this study to provide a thorough evaluation of fluid-rock interaction as a function of host rock composition. Experimental and Analytical Procedures: The compositions of synthetic basaltic analogs used in this study include those most relevant to one of the most important sources of chemical data for the Martian surface-the Mars Pathfinder landing site. As an attempt to encompass the chemical spectrum that the Pathfinder data may reflect, two " end member " compositions are used as analogs. These compositions include a lowS Pathfinder rock composition representative of a basaltic andesite Pathfinder surface rock composition and averaged Martian soil (recalculated on a Sand Cl-free basis), which may represent a typical upper crustal composition. The basaltic analog materials are synthesized following the procedure outlined by Tosca et al. [3] to achieve the desired compositions. The products are then lightly crushed and sieved to constrain the particle size between 700 and 70 µm. The analog material is then ultrasonically rinsed in acetone to remove ultra-fine particles and dried overnight at 120 o C. The dried material is then divided and added to 5 different sulfu-ric/hydrochloric acid mixtures with a S:Cl molar ratio of 4, equal to that observed in the Pathfinder soils. Acid mixture concentrations range from a 1M
منابع مشابه
Laboratory Hydrothermal Alteration of Basaltic Tephra by Acid Sulfate Solutions: an Analog Process for Martian Weathering
Introduction: Sulfur is a major chemical component of the Martian surface materials and is thought to have a volcanic origin. Pathfinder and Viking chemical analyses revealed SO3 compositions of “soils” and dust from about 4 to over 7 wt. % [1,2]. Although we know that S is chemically important, we do not know its speciation. Small amounts of sulfates (e.g., Ca and Mg sulfates) and sulfides (e....
متن کاملChemical Weathering Trends from Tir Spectral Models: Implications for Deriving Weathering Trends from Martian Spectral Data
Introduction: Chemical weathering and petrologic trends of the martian surface have been estimated from thermal infrared (TIR) spectral models from the Thermal Emission Spectrometer (TES) and Mini-TES on the Spirit and Opportunity rovers [1,2]. Interpretations of chemical data from APXS on the MER rovers and TIR data from TES and the Thermal Emission Imaging System (THEMIS) suggest planet-wide ...
متن کاملConstraints on the composition and petrogenesis of the Martian crust
[1] Spectral interpretation that silicic rocks are widespread on Mars implies that Earth’s differentiated crust is not unique. Evaluation of observations bearing on the composition of the Martian crust (Martian meteorite petrology and a possible crustal assimilant, analysis of Mars Pathfinder rocks, composition of Martian fines, interpretation of spacecraft thermal emission spectra, and inferre...
متن کاملTiming of acid weathering on Mars: A kinetic-thermodynamic assessment
[1] Weathering of olivine basalt by H2SO4-HCl aqueous solutions at the conditions of early Mars was investigated through numerical modeling in a system open with respect to CO2 and O2 only. The model includes dissolution rates of primary and secondary minerals and oxidation rate of aqueous Fe, as well as chemical equilibration among solutes, dissolved gases, and precipitates. The results reveal...
متن کاملکانی شناسی سطحی خاکهای سولفاته اسیدی ساحلی، در ناحیه شهری پینجارا، جنوب غربی استرالیا
Acid sulfate soils in Western Australia commonly occur in coastal regions. One of the greatest threats to coastal environment is the disturbance of acid sulfate soils due to urban development which can lead to widespread acidification of lands and streams and subsequent economic losses onsite or in adjacent areas. Surface sampling from different landforms of the study area and analytical result...
متن کامل