Carbon monoxide in Jupiter's upper atmosphere - an extraplanetary source

Details Carbon monoxide in Jupiter's upper atmosphere - an extraplanetary source Carbon monoxide in Jupiter's upper atmosphere - an extraplanetary source

Aug 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...223.1072p&link_type=abstract

Astrophysical Journal, Part 1, vol. 223, Aug. 1, 1978, p. 1072-1081.

Astronomy and Astrophysics

Astrophysics

19

Atmospheric Chemistry, Atmospheric Models, Carbon Monoxide, Jupiter Atmosphere, Photochemical Reactions, Ablation, Bibliographies, Gas Mixtures, Graphs (Charts), Hydrocarbons, Methane, Micrometeoroids, Photolysis, Pressure Effects, Water, Carbon Dioxide, Carbon Monoxide, Jupiter, Flux, Atmosphere, Temperature, Water, Abundance, Diffusion, Methane, Hydrogen, Concentrations, Models, Spectroscopy, Chemical Composition

Scientific paper

Ablation of meteoroidal material in Jupiter's atmosphere may provide substantial quantities of H2O. Subsequent photochemistry can convert H2O and CH4 to CO and H2. The associated source of CO could account for the observations by Beer, Larson, Fink, and Treffers, and Beer and Taylor, and would explain the relatively low rotational temperatures inferred by Beer and Taylor. Meteoritic debris might also provide spectroscopically detectable concentrations of SiO.

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