On the detectability of H2S in Jupiter

Details On the detectability of H2S in Jupiter On the detectability of H2S in Jupiter

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icar...55..259b&link_type=abstract

Icarus (ISSN 0019-1035), vol. 55, Aug. 1983, p. 259-271. Research supported by the Centre National d'Etudes Spatiales and Instit

Physics

33

Atmospheric Chemistry, Hydrogen Sulfide, Jupiter Atmosphere, Brightness Temperature, Infrared Spectra, Microwave Spectra, Radiative Transfer, Troposphere, Vertical Distribution, Jupiter, Hydrogen Sulfide, Atmosphere, Chemistry, Infrared, Wavelengths, Spectra, Distribution, Microwaves, Opacity, Troposphere, Saturation, Physics, Chemistry, Hypotheses, Thermal Properties, Calculations, Flux, Radiative Transfer, Pressure, Temperature, Brightness Temperature, Data, Sulfur, Comparisons, Ammonia, Phosphine, Methan

Scientific paper

The influence of hydrogen sulfide, a still-undetected key molecule for the Jovian atmospheric chemistry in the infrared spectrum, was investigated. Synthetic spectra including various vertical distribution profiles of H2S have been computed and compared with observational data for Jupiter in the 2 to 15 per cm and 1160 to 1200 per cm spectral ranges. No firm conclusion about the presence of H2S can be drawn from the latter spectral region because of large uncertainties in gaseous opacities. In the microwave range, H2S is found to be a possible candidate to explain the measurements. Constraints to its vertical distribution which would imply a significant supersaturation in the troposphere are reviewed. Physical and chemical processes involving H2S in the atmosphere are discussed in the light of this hypothesis.

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