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

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Diskussion der Untersuchungsergebnisse,ns in the abundance have been found with both position and time. The total two-way transmission has varied from less than 5 to 77 . of water vapor. Comparisons will be made between the water vapor abundances, presence of UV features, and the CO. abundances determined from near simultaneous observati

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The Escape of Planetary Atmospheresbegan to take form whether or not the Moon possessed an atmosphere. And this idea was gradually extended to other planets..The lunar observers of the late eighteenth century set out to ascertain whether the Moon indeed showed visible traces of an atmosphere. In 1792, Schroter recorded what he interp

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Modern Research in High Resolution Infrared Spectroscopy and Its Importance to Planetary Physicserg done in the early 50’s are not summarized in this paper because they are all consolidated in three previous publications. On the other hand, more recent measurements on CO. are scattered in several publications and, therefore, an attempt has been made to collect them together in this article. Th

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Ground-Based Observations of Mars and Venus Water Vapor during 1972 and 1973e Mariner 9 IRIS and Mars 3 observations made during the same period..During the second period (..= 124° to 266°) observations were made to follow the seasonal latitudinal and diurnal changes in the water vapor abundance in the Martian atmosphere. The water vapor abundance declines from a maximum of

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