Possible microwave absorption by H2S gas in Uranus' and Neptune's atmospheres

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摘要：

We present new VLA observations of Neptune at 3.55 and 20.1 cm. The disk-averaged brightness temperatures are 191.2 ± 6 K at 3.55 cm, and 276.4 ± 10 K at 20.1 cm. These values are consistent with thermal spectra of the planet. We further present a comparison between Uranus and Neptune's spectrum, using improved atmospheric models for both planets. We improved the old models by including microwave absorption by H 2 S. The rotational lines of this gas, which are all at (sub)millimeter wavelengths, are pressure broadened to such an extent that considerable opacity at centimeter wavelengths is expected. We estimate from our calculations that the H 2 S mixing ratio on Uranus and Neptune is likely enhanced by a factor of 10–30 above the solar sulfur elemental ratio, and that the S/N ratio must exceed 5 × the solar ratio. Our calculations suggest the width of the H 2 S line to be similar to or less than that of water. There is more microwave opacity in Neptune's atmosphere than in that of Uranus, which may be caused by the presence of some NH 3 gas above the NH 4 SH cloud layer. From a comparison with the radio occultation data, we suggest that NH 3 is likely supersaturated in Neptune's atmosphere at levels where T 210–225 K, or P 20–25 bar.

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classical and quantum mechanics, general physics neptune planet planetary atmospheres uranus planet absorption atmospheric circulation brightness chemical composition comparative evaluations element abundance