Computer Science
Scientific paper
Sep 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987icar...71..472p&link_type=abstract
(The Planet Mercury Conference, Tucson, AZ, Aug. 6-9, 1986) Icarus (ISSN 0019-1035), vol. 71, Sept. 1987, p. 472-477.
Computer Science
46
Mercury (Planet), Mercury Atmosphere, Planetary Composition, Radiation Pressure, Sodium Vapor, Solar Radiation, Elastic Scattering, Emission Spectra, High Resolution, High Temperature, Mercury Surface, Radial Velocity, Mercury (Planet), Sodium, Solar Radiation, Pressure, Atmosphere, Models, Acceleration, Velocity, Abundance, Temperature, Emissions, Density, Earth-Based Observations, Telescope Methods, Data, Spectra, Analysis
Scientific paper
Sodiums atoms in the atmosphere of Mercury can be accelerated by solar radiation pressure, and several authors have suggested that radiation pressure could sweep sodium off the planet. As a consequence, the sodium abundance might be expected to decrease as the radiation pressure increases. The authors have measured the average sodium abundance over a range of solar radiation pressures and found that the sodium abundance does decrease with increasing radiation pressure. Possible explanations for the observed variation are (1) that radiation pressure sweeps away transient high-velocity sodium atoms generated upon meteoric material impacts, thus reducing the supply rate of sodium, or (2) that the accommodation coefficient of sodium for surface interactions is less than unity, so that radiation pressure can effectively push sodium to the dark side of the planet, where it cannot be detected by scattered sunlight.
Morgan Thomas H.
Potter Andrew E.
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