The abundance of AsH3 in Jupiter

Computer Science

Scientific paper

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Arsenic Compounds, Atmospheric Composition, Hydrides, Jupiter Atmosphere, Abundance, Atmospheric Models, Planetary Atmospheres, Jupiter, Abundance, Arsenic, Earth-Based Observations, Atmosphere, Aircraft Observations, Spectra, Comparisons, Kao Aircraft, Procedure, Models

Scientific paper

Both ground-based and airborne observations of the AsH3 Q-branch at 2126/cm, in conjunction with newly-analyzed laboratory comparison spectra at AsH3, are employed in the derivation of a new estimate of Jovian As abundance. The mole fraction on AsH3 in the Jovian atmosphere is 0.22 + or - 0.11 ppb; this is merely 0.5 times the solar abundance, and a factor-of-9 less than the mole fraction found in Saturn, duplicating the pattern noted in the relative abundance of P in these two planets and furnishing a useful constraint for models of heavy element incorporation in the outer planets' gaseous envelopes.

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