Other
Scientific paper
Mar 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982icar...49..416d&link_type=abstract
Icarus, vol. 49, Mar. 1982, p. 416-426.
Other
58
Abundance, Atmospheric Composition, Jupiter Atmosphere, Phosphines, Planetary Composition, Deuterium, Germanium Compounds, Hydrogen, Iris Satellites, Molecular Spectra, Voyager 1 Spacecraft
Scientific paper
No evidence is found for large scale phosphine abundance variations over Jovian latitudes between -30 and +30 deg, in PH3, CH3D, and GeH4 abundances derived from the 2100-2250/cm region of the Voyager 1 IRIS spectra. The PH3/H2 value of (4.5 + or - 1.5) X 10 to the -7th derived from atmospheric regions corresponding to 170-200 K is 0.75 + or - 0.25 times the solar value, and suggests that the PH3/H2 ratio on Jupiter decreases with atmospheric pressure upon comparison with other PH3 determinations at 10 microns. In the 200-250 K region, CH3D/H2 and GeH4/H2 ratios of 2.0 X 10 to the -7th and 1.0 X 10 to the -9th, respectively, are derived within a factor of 2.0. Assuming a C/H value of 0.001, as derived from Voyager, the CH3D/H2 ratio obtained in this study implies a D/H ratio of 0.000018. This is in agreement with the interstellar medium value.
Combes Michel
Drossart Pierre
Encrenaz Th.
Hanel Rudolf
Kunde Virgil
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