A Case Study on the Effects of the Solar Wind and Solar CNO
Cycle on the Formation of Jovian Planets and Comets
By:
Akbar Mohammadzade
Iran university of science and technology
akbarmohammadzade@yahoo.com
Abstract: Rotation period of planets and moons vary, and do not obey the distance
calculations of the main gravity field, or the planet's mass, or other regular gravity field properties.
Spins are synchronous for some and faster for others. The reason for the fast rotational spins of
Jovian planets has not been studied. Here, we study the formation process and some secondary
noticeable currents in the system. The solar wind and its carried particles effects on system are
assessed, together with solar CNO cycle-produced particles. Our work resulted in different
properties for the outer part of the Heliosphere at 5-100 AU which can cause mass increases of the
Jovian planets according to a snow ball model, and can produce further angular momentum for
planets through any method of arithmetic progress.
Keywords: cosmogony, CNO cycle, snow ball model, solar wind, planetary system