Predicted chemistry of the deep atmosphere of Uranus before the Voyager 2 encounter

Details Predicted chemistry of the deep atmosphere of Uranus before the Voyager 2 encounter Predicted chemistry of the deep atmosphere of Uranus before the Voyager 2 encounter

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985natur.318...48f&link_type=abstract

Nature (ISSN 0028-0836), vol. 318, Nov. 7, 1985, p. 48-50.

Astronomy and Astrophysics

Astronomy

8

Atmospheric Chemistry, Planetary Composition, Spaceborne Astronomy, Uranus Atmosphere, Vertical Distribution, Abundance, Atmospheric Models, Chemical Equilibrium, Infrared Interferometers, Infrared Spectrometers, Nonequilibrium Conditions, Reaction Kinetics, Voyager 2 Spacecraft, Uranus, Voyager 2, Chemistry, Atmosphere, Iris, Gases, Source, Depth, Infrared Interferometer Spectrometer, Phosphine, Germanium Tetraethly, Mixing, Models, Thermochemistry, Kinetics, Calculations, Nitrogen

Scientific paper

The authors describe the results of comprehensive thermochemical equilibrium and chemical kinetic calculations for the Uranus atmosphere. It is predicted that the most abundant non-equilibrium trace gas derived from the deep atmosphere of Uranus is N2; other important non-equilibrium species include HCl, HF, GeH4, C2H6, PH3, H2Se, CH3SH, CO, CH3NH2, CH3OH, and CO2. Some of these species are detectable potentially by the Voyager instruments during the January 1986 encounter.

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