Abstract
Various approaches have been used to estimate when and how long liquid water was present at the surface of Mars. The olivine dissolution-lifetime application suggested by Stopar et al. (2006) and Olsen and Rimstidt (2007) is here adapted and tested at the scale of individual etch-pits using published data from an experimental system in which the volume of mineral removed and the duration of the mineralremoval episode are known. Different assumptions about the specific geometry of etch-pits on olivine result in surface-area estimates that vary by less than a factor of two from the simple hemispherical pit used in the calculations. Given that other sources of uncertainty in mass-time relationships of silicatemineral dissolution during natural weathering can be up to four orders of magnitude, the effects of differing geometric assumptions about the shapes and surface areas of the etch-pits are negligible.
Using compiled experimentally determined forsterite dissolution rates and the imaged etch-pit sizes from experiments recovers the duration of the experiment that produced the imaged etch-pits to within less than a factor of two. This suggests that extensively etched olivine surfaces imply a dominance of the etch-pit walls over the bulk surface between the etch-pits during olivine corrosion. The approach adopted here recovers the timescales of experimental etch-pit production on olivine at STP and extreme undersaturation of the solution with respect to olivine in experiments where pH is known. Continued progress in understanding the fundamentals of olivine dissolution kinetics will narrow the ranges of uncertainty in mineral-lifetime estimates at Mars’ surface in support of constraining the compositions and duration of potentially habitable aqueous solutions on Mars
© 2014 by Walter de Gruyter Berlin/Boston
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- Data-driven abductive discovery in mineralogy
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- Experimental study of phlogopite reaction rim formation on olivine in phonolite melts: Kinetics, reaction rates, and residence times
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- Determining hematite content from NUV/Vis/NIR spectra: Limits of detection
- The role of water in generation of group II kimberlite magmas: Constraints from multiple saturation experiments
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Articles in the same Issue
- Highlights and Breakthroughs Merrillite and apatite as recorders of planetary magmatic processes
- Highlights and Breakthroughs Comparing clays from Mars and Earth: Implications for martian habitability
- Data-driven abductive discovery in mineralogy
- Thermal expansion of fluorapatite-hydroxylapatite crystalline solutions
- Synthesis and structure of carbonated barium and lead fluorapatites: Effect of cation size on A-type carbonate substitution
- Optical absorption spectroscopy study of the causes for color variations in natural Fe-bearing gahnite: Insights from iron valency and site distribution data
- Si-magnetite nano-precipitates in silician magnetite from banded iron formation: Z-contrast imaging and ab initio study
- Ordering kinetics in synthetic Mg(Al,Fe3+)2O4 spinels: Quantitative elucidation of the whole Al-Mg-Fe partitioning, rate constants, activation energies
- Experimental study of phlogopite reaction rim formation on olivine in phonolite melts: Kinetics, reaction rates, and residence times
- Etch-pit size, dissolution rate, and time in the experimental dissolution of olivine: Implications for estimating olivine lifetime at the surface of Mars
- Ferrian saponite from the Santa Monica Mountains (California, U.S.A., Earth): Characterization as an analog for clay minerals on Mars with application to Yellowknife Bay in Gale Crater
- A large spectral survey of small lunar craters: Implications for the composition of the lunar mantle
- In-situ characterization of oxalic acid breakdown at elevated P and T: Implications for organic C-O-H fluid sources in petrologic experiments
- Slawsonite-celsian-hyalophane assemblage from a picrite sill (Prague Basin, Czech Republic)
- Determining hematite content from NUV/Vis/NIR spectra: Limits of detection
- The role of water in generation of group II kimberlite magmas: Constraints from multiple saturation experiments
- Quantum mechanical modeling of hydrolysis and H2O-exchange in Mg-, Ca-, and Nisilicate clusters: Implications for dissolution mechanisms of olivine minerals
- Redox-driven exsolution of iron-titanium oxides in magnetite in Miller Range (MIL) 03346 nakhlite: Evidence for post crystallization oxidation in the nakhlite cumulate pile?
- Energetics of lanthanide-doped calcium phosphate apatite
- Thermal conductivity of molten and glassy NaAlSi3O8, CaMgSi2O6, and Mg2SiO4 by non-equilibrium molecular dynamics at elevated temperature and pressure
- Energetics of heterometal substitution in ε-Keggin [MO4Al12(OH)24(OH2)12]6/7/8+ ions
- Ab initio calculations of elastic constants of plagioclase feldspars
- Diagenetic formation of interlayer-deficient fluorophlogopite as a clay mineral in Early Cambrian phosphorite (Lesser Himalaya, India): The trioctahedral analog of illite
- Natural sepiolite: Enthalpies of dehydration, dehydroxylation, and formation derived from thermochemical studies
- A new interpretation of decomposition products of serpentine under shock compression
- model for calculating the viscosity of natural iron-bearing silicate melts over a wide range of temperatures, pressures, oxygen fugacites, and compositions
- The replacement of chalcopyrite by bornite under hydrothermal conditions
- Characterization of porosity in sulfide ore minerals: A USANS/SANS study
- Synthesis of a quenchable high-pressure form of magnetite (h-Fe3O4) with composition Fel(Fe2+0.75Mg0.26)Fe2(Fe3+ 0.70Cr0.15Al0.11Si0.04)2O4
- High-pressure elasticity of sodium majorite garnet, Na2MgSi5O12
- Armstrongite from Khan Bogdo (Mongolia): Crystal structure determination and implications for zeolite-like cation exchange properties
- Steinhardtite, a new body-centered-cubic allotropic form of aluminum from the Khatyrka CV3 carbonaceous chondrite
- New Mineral Names
- Book Review