Titlebook: Exploration of the Planetary System; A. Woszczyk,C. Iwaniszewska Book 1974 International Astronomical Union 1974 Planet.Planetary system.S

Mucosa

Nature of the Venus Clouds as Derived from Their Polarization particle properties deduced from the polarization eliminate all but one of the cloud compositions which have been proposed for Venus. A concentrated solution of sulfuric acid (H.SO.-H.O) provides good agreement with the polarization data.

cinder

Water Vapor in Venus Determined by Airborne Observations of the 8200 ? Bandlution groundbased studies..These results establish that the average value over the entire disk is quite low but allows that locally larger values may exist as reported by Barker. A more complete description of this work appeared in . . (1974), 213.

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Book 1974 of his birth, came during the XIV General Assembly of IAU in Brighton. The Executive Committee has approved it in the program of the Extraordinary (Copernicus) General Assembly ofIAU in Poland in 1973. The IAU Symposium No 65 (Copernicus Symposium IV) on the ‘Exploration of the Planetary System‘ wa

大都市

Status of Molecular Opacities of Interest in the Modeling of a Proto-Solar Nebulans of a mixture of atoms, molecules, and their ionic species in the gaseous phase, condensation into grains with refractory cores and mantles of volatile compounds, and the ‘optical’ properties of the grain-gas medium. A summary of available and still needed basic (input) data and some currently available results are presented.

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amplitude

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intuition

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Robert W. Baloh,Robert E. BartholomewWe have searched for molecular lines in planetary atmospheres using the PEPSIOS spectrometer with an instrumental width about equal to that of the expected absorption line, and in the case of Jupiter, with the additional feature of Doppler compensation over the planetary disc.