In the first place, we need to test the dynamics of the planets in relation to the available solar energy. I did that by calculating the energy that an atom, ion or gas molecule would get by the Sun’s temperature. Then, I equated this energy to the kinetic energy of that particle, which equation contains the average velocity of the gas. Then, I could relate that velocity to the Sun’s temperature and find this velocity, because the temperature and the velocity were the sole variables in the equations. All other parts were constants and natural constants.