Search for HD in Jupiter and Saturn

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Abundance, Deuterium, Hydrogen, Jupiter Atmosphere, Line Spectra, Saturn Atmosphere, Atmospheric Models, Data Acquisition, Fabry-Perot Interferometers, Methane, Nitrogen, Spectrum Analysis, Sulfur

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Upper limits are placed on the D/H ratio in the observed portions of the atmospheres of Jupiter and Saturn from observations at high S/N over the region of the 5-0 R(1) line of HD. The upper limits of 0.00004 and 0.00006 D/H on Jupiter and Saturn, respectively, are not inconsistent with present models for abundance ratios in the primitive solar nebula or with other estimates of this quantity from observations.

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