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

微生物

erythema

Book 1974 of the Polish Acade- my of Sciences made possible the participation of several young astronomers in this meeting. We are very grateful to Professor P. Swings, the Director of the Astrophysical Institute of the University of Liege, Belgium, for accepting the task of chairing this symposium. His expe

infringe

1743-9213 rofessor P. Swings, the Director of the Astrophysical Institute of the University of Liege, Belgium, for accepting the task of chairing this symposium. His expe978-90-277-0450-4978-94-010-2206-4Series ISSN 1743-9213 Series E-ISSN 2352-2186

使長胖

Status of Molecular Opacities of Interest in the Modeling of a Proto-Solar Nebulaas models for the solar nebula during planet formation and for the atmospheres of some planets. Specifically considered are the equilibrium compositions of a mixture of atoms, molecules, and their ionic species in the gaseous phase, condensation into grains with refractory cores and mantles of volat

現(xiàn)實

On the Growth Mechanism of Grains in a Primordial Stage of the Solar Nebula and electromagnetic mechanisms between grains. The velocity distribution function has been investigated for grains embedded in a turbulent gaseous medium. Results have been obtained for protoplanetary nebula densities ranging from 10. to 10. g cm.. Considering interactions between two grains, photo

無彈性

The Escape of Planetary Atmospheresthe Earth’s atmosphere as a medium extending to infinity, with a stationary Earth imbedded at the center. Indeed, it was this concept that led Ptolemy, among many others, to conclude that the Earth could not be moving, for otherwise it would be subject to a gale-force wind caused by its own motion.

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Infrared Spectra of Venuspectroscopically forty years ago, and minor constituents (CO, HF, HCl) have been found more recently. The infrared spectra also provide a means of studying the motions of her cloudy atmosphere. The composition of the clouds has been sought in the reflection spectrum of Venus, and some of the evidenc