Physics
Scientific paper
Apr 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aps..apr.r9016z&link_type=abstract
American Physical Society, April Meeting, 2003, April 5-8, 2003 Philadelphia, Pennsylvania, MEETING ID: APR03, abstract #R9.016
Physics
Scientific paper
Radiation mechanics provides an understanding of origin of our solar system and a proof of why the planets must revolve in a common orbital plane. The solar system was formed by successive condensations of the atomic gas in the nucleus of a primary solar nebula into Jovian planets along the rim of the nebular nucleus which was surrounded by an electron ring. Origin of the solar system is due to condensations of the four Jovian planets: Neptune, Uranus, Saturn and Jupiter in succession, along the rim of the nucleus lens of the primary solar nebula. As the Jovian planets grew up to the critical sizes, they started to trap electrons in their rings, broke off from the nucleus and wiped out the nebular plane in the spiral orbits. Terrestrial planets were formed by aggregation of the remaining debris of condensed materials in the region that was the previous nebular nucleus. As all the planets are magnets, the observed orbital motion of the planets in a common orbit plane is a necessity. Rational mechanics also explains why the planets must have rotation, and demonstrate the factors that influence the rotation rates and the mechanism that leads to the diversity of orientations of spin axes of the planets.
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