Mikhail V. Mironenko

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[1] Theoretical geochemical modeling has been used to evaluate the formation conditions of amorphous silica during aqueous alteration of typical Martian igneous rocks at 0 C. The models show that some silica can form during low-temperature alteration of mafic to ultramafic rocks over a large range of pH and water/rock ratios. Silica-dominated deposits, like(More)
FOR A FERRAR DOLERITE COMPOSITION. A. C. McAdam, M. Yu. Zolotov, M. V. Mironenko, L. A. Leshin, and T. G. Sharp, Dept. of Geological Sciences, Arizona State University, Box 871404, Tempe, AZ 85287-1404, amcadam@asu.edu, 2 Vernadsky Institute of Geochemistry and Analytical Chemistry, Russian Academy of Sciences, 19 Kosygin Str., Moscow 119991, Russia,(More)
CHEMICAL EQUILIBRIUM CONSTRAINTS. A. C. McAdam, M. Yu. Zolotov, M. V. Mironenko, and T. G. Sharp, Atmospheric Experiments Laboratory, Code 699, Goddard Space Flight Center, Greenbelt, MD 20771, Amy.McAdam-1@nasa.gov, School of Earth & Space Exploration, Arizona State University, Tempe, AZ 852871404, Amy.McAdam-1@nasa.gov, Vernadsky Institute of Geochemistry(More)
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