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Featured researches published by V. M. Tu.


American Mineralogist | 2014

Dissolution rates of amorphous Al- and Fe-phosphates and their relevance to phosphate mobility on Mars

V. M. Tu; Elisabeth M. Hausrath; Oliver Tschauner; Valentin Iota; Gerald W. Egeland

Abstract Phosphate is an essential nutrient for life on Earth, and therefore if life exists or ever existed on Mars it may have required phosphate. Amorphous Al- and Fe-phosphates rapidly precipitate from acidic solutions and amorphous Al-phosphates likely control phosphate concentrations in some natural waters on Earth. The amorphous fraction of martian soils has also been shown to be enriched in P, and amorphous phosphates are therefore also likely important in the phosphate cycle on Mars. Despite this importance, however, few dissolution rates exist for amorphous Al- and Fe-phosphates. In this study, dissolution rates of amorphous Al- and Fe-phosphates were measured in flow-through reactors from steady state concentrations of Al, Fe, and P. A pH-dependent rate law, log R = log k - npH was determined from the dissolution rates, where R is the dissolution rate, k is the intrinsic rate constant, and n is the reaction order with respect to H+. For amorphous Al-phosphate, log k = -6.539 ± 1.529 and n = 2.391 ± 0.493. For amorphous Fe-phosphate, log k = -13.031 ± 0.558 and n = 1.376 ± 0.221. The amorphous Al-phosphate dissolves stoichiometrically under all experimental conditions measured, and the amorphous Fe-phosphate dissolves non-stoichiometrically, approaching stoichiometric dissolution as pH decreases, due potentially to Fe oxyhydroxides precipitating and armoring grain surfaces. Perhaps due to these effects, amorphous Al-phosphate dissolution rates are approximately three orders of magnitude faster than the amorphous Fe-phosphate dissolution rates measured under these experimental conditions. Amorphous Al-phosphate dissolution rates measured in this study are also faster than published dissolution rates for the crystalline Al-phosphate variscite. The rapid dissolution rates measured in this study therefore suggest that, if these phases are present on Mars, phosphate would be rapidly released into acidic environments.


Archive | 2014

Experimental evidence suggests significant aqueous alteration of abundant phosphorus release on Mars

Elisabeth M. Hausrath; C. T. Adcock; S. R. Gainey; M. H. Steiner; V. M. Tu


Archive | 2013

Dissolution of amorphous Al- and Fe-phosphates: Implications for phosphate mobility on Mars

V. M. Tu; Elisabeth M. Hausrath


Archive | 2012

Dissolution rates of amorphous Al-and Fe-phosphates and their relevance to Mars

V. M. Tu; Elisabeth M. Hausrath


Archive | 2012

Interpreting phosphate mobility on Mars and the implications for habitability

Elisabeth M. Hausrath; C. T. Adcock; V. M. Tu


Archive | 2012

Phosphate records environmental conditions important to habitability in soils and rocks on Mars

Elisabeth M. Hausrath; C. T. Adcock; V. M. Tu


Archive | 2011

Serpentinite Weathering and Implications for Mars

V. M. Tu; Julie L. Baumeister; Rodney V. Metcalf; Amanda A. Olsen; Elisabeth M. Hausrath


Archive | 2011

Reactive transport modeling of phosphate mobility under Mars-like conditions

Elisabeth M Hausrath; V. M. Tu


Archive | 2011

Chemical Weathering of Serpentinites in the Klamath Mountains, California

Julie L. Baumeister; V. M. Tu; Mary H. Evert; Rodney V. Metcalf; Amanda A. Olsen; Elisabeth M. Hausrath


Archive | 2010

Chemical weathering of serpentinite rocks and implications for atmospheric CO2 carbonation

V. M. Tu; Julie L. Baumeister; Elisabeth M. Hausrath

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