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NASA NTRS ยท 20030111592

H2O-Silicate Microphysics in Ascending Volcanic Plumes on Mars

Abstract

We begin this study with a simple investigation of the role of the particle size frequency distribution on adsorptive scavenging in the ascending cloud. We define a parcel of silicates and H2O, and allow that parcel to cool, monitoring the total H2O remaining in the vapor phase. In this case, we have defined 10(exp 7) kg of silicates in the test volume, with a log-normal size-frequency distribution, a mean grain size of 10(exp -5) m, and a minimum of 10(exp -6) square meters per particle. This is based on observations of terrestrial ash particles that reveal enormous internal surface area. We assume 10(exp 5) kg of H2O (approximately equal to 1 wt%). The results of this study show significant dependence of the H2O sequestered in the adsorbed phase.

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BibTeXRIS

Zent, A. P.. 2003-01-01. H2O-Silicate Microphysics in Ascending Volcanic Plumes on Mars. https://ntrs.nasa.gov/citations/20030111592

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