Computer Science
Scientific paper
Feb 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993icar..101..293k&link_type=abstract
Icarus (ISSN 0019-1035), vol. 101, no. 2, p. 293-312.
Computer Science
21
Mercury Atmosphere, Planetary Composition, Planetary Crusts, Sodium, Mercury Surface, Planetology, Regolith, Mercury (Planet), Sodium, Atmosphere, Origin, Source, Crust, Ions, Abundance, Gas Phase, Diffusion, Surface, Exosphere, Regolith, Flow, Structure, Composition, Temperature, Silicates, Calculations, Flux, Porosity, Fissures, Vents, Potassium, Vaporization, Impact Effects, Sputtering, Desorption, Photons, Environment, Megaregolith
Scientific paper
The possible sources of the Na atmosphere of Mercury are calculatively studied. The likely structure, composition, and temperature of the planet's upper crust is examined along with the probable flux of Na from depth by grain boundary diffusion and by Knudsen flow. The creation of fresh regolith is considered along with mechanisms for supplying Na from the surface to the exosphere. The implications of the calculations for the probable abundances in the regolith are discussed.
Killen Rosemary Margaret
Morgan Thomas H.
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