High-resolution observations of the 6815-A band of methane in the major planets

Details High-resolution observations of the 6815-A band of methane in the major planets High-resolution observations of the 6815-A band of methane in the major planets

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icar...56..534b&link_type=abstract

Icarus (ISSN 0019-1035), vol. 56, Dec. 1983, p. 534-542.

Mathematics

14

Abundance, Gas Giant Planets, Methane, Molecular Absorption, Planetary Atmospheres, Planetary Composition, Aerosols, Atmospheric Scattering, Molecular Spectra, Planetary Evolution, Solar System, Uranus Atmosphere

Scientific paper

High-resolution (0.1-A) spectra of the 6815-A band of methane are presented for Jupiter, Saturn, Uranus, and Neptune. Spectra for Uranus, Neptune, and the equatorial region of Saturn were acquired with the SPIFI (Smith, Hicks, and Born (1978) at the 2.2-m telescope of the Mauna-Kea Observatory during May and June 1980. Additional spectra were obtained for Jupiter and the northern temperate and polar regions of Saturn in December 1980 and January 1981 from Kitt Peak National Obsevatory's McMath Solar Telescope. The spectra show a dichotomy in strength of methane absorption between Jupiter-Saturn and Uranus-Neptune. A simple model analysis, based on homogeneous scattering models, is unable to resolve whether this dichotomy is due to an actual increase in the methane mixing ratio with solar distance or to the temperature dependence of line strengths and absorption pathlengths in these atmospheres. If the rotational quantum number for the prominent 6818.9-A feature is J less than 4, then significant aerosol extinction must exist within the visibly accessible portion of Uranus' atmosphere for the methane mixing ratio to be greater than the solar value.

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