A model of the SO2 atmosphere and ionosphere of Io

Astronomy and Astrophysics – Astronomy

Scientific paper

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Atmospheric Models, Atmospheric Temperature, Exosphere, Io, Ionospheres, Satellite Atmospheres, Sulfur Dioxides, Absorption Cross Sections, Atmospheric Heating, Chemical Equilibrium, Ionospheric Electron Density, Pioneer 10 Space Probe, Spaceborne Astronomy, Spaceborne Experiments, Ultraviolet Absorption, Voyager Project, Jupiter, Satellites, Io, Ionosphere, Atmosphere, Sulfur Dioxide, Models, Thermal Structure, Exosphere, Temperatures, Pioneer 10, Density, Electrons, Ionization, Ultraviolet, Absorption, Ga

Scientific paper

The calculations of thermal structure for an SO2 atmosphere of Io lead to exospheric temperatures in 800-1200 K range. The Pioneer 10 electron density profiles can be fit with an SO2 surface density of 1.2 x 10 to the 11th per cu cm at 5:30 pm local time and exosphere temperature of 1030 K. Low energy electrons provide the major ionization source but the solar UV absorption dominates the heating of the atmosphere due to the long wavelength absorption threshold of SO2 and large absorption cross sections.

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