The physicochemical mechanisms of the formation of planetary systems

Details The physicochemical mechanisms of the formation of planetary systems The physicochemical mechanisms of the formation of planetary systems

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978m%26p....18..217g&link_type=abstract

Moon and the Planets, vol. 18, Apr. 1978, p. 217-221.

Physics

Condensed Matter

4

Astronomical Models, Physical Chemistry, Planetary Evolution, Planetary Systems, Solar System, Cosmic Dust, Diffusion Theory, Interplanetary Gas, Stellar Evolution, Stellar Mass Ejection, Stellar Rotation

Scientific paper

A diffusion hypothesis is put forward, according to which the regular structure of planetary systems can be quantitatively explained as a consequence of spatially periodic condensation of gaseous matter during the formation of the central body. This theory is applied to the solar system. It enables one to calculate the time of formation of primary rings of condensed matter and the ages of the planets and solar system as a whole. The results of the theory are in harmony with the Titius-Bode rule.

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