The C/H ratio in Jupiter from the Voyager infrared investigation

Details The C/H ratio in Jupiter from the Voyager infrared investigation The C/H ratio in Jupiter from the Voyager infrared investigation

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...257..901g&link_type=abstract

Astrophysical Journal, Part 1, vol. 257, June 15, 1982, p. 901-912.

Astronomy and Astrophysics

Astronomy

71

Abundance, Infrared Astronomy, Jupiter Atmosphere, Planetary Composition, Voyager 1 Spacecraft, Atmospheric Temperature, Brightness Temperature, Error Analysis, Hydrogen, Methane, Opacity, Planetary Evolution, Radiative Transfer, Jupiter, Voyager, Element Ratios, Hydrogen, Infrared, Wavelengths, Spectra, Iris, Atmosphere, Abundance, Formation, Evolution, Analysis, Opacity, Procedure, Radiative Transfer, Gases, Brightness Temperature, Data, Methane

Scientific paper

From a selection Voyager IRIS spectra corresponding to cloud-free areas of Jupiter, the CH4/H2 volume ratio in the atmosphere of this planet has been determined to be equal to 0.00195 + or - 0.00022, which corresponds to 2.07 + or - 0.24 times the solar value of Lambert (C/H = 0.00047). The estimate of errors includes both instrument noise and systematic uncertainties. Implications of this result for the formation and evolution of Jupiter are discussed.

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