Sun Density

Audio File   The mass of our sun is slightly greater than the estimate of our physicists, who have reckoned it as about two octillion (2 x 10 to the 27th power) tons.  It now exists about halfway between the most dense and the most diffuse stars, having about one and one-half times the density … Continue reading Sun Density

The Origin of Space Bodies

Audio File        The bulk of the mass contained in the suns and planets of a superuniverse originates in the nebular wheels; very little of superuniverse mass is organized by the direct action of the power directors (as in the construction of the headquarters’ architectural spheres), although a constantly varying quantity of matter originates … Continue reading The Origin of Space Bodies

Solar — Energy Reactions

Audio File   In those suns which are encircuited in the space-energy channels, solar energy is liberated by various complex nuclear-reaction chains, the most common of which is the hydrogen - carbon - helium reaction.  In this metamorphosis, carbon acts as an energy catalyst since it is in no way actually changed by this process … Continue reading Solar — Energy Reactions

Sun Stability

Audio File   The larger suns maintain such a gravity control over their electrons that light escapes only with the aid of the powerful X-rays.  These helper rays penetrate all space and are concerned in the maintenance of the basic ultimatonic associations of energy.  The great energy losses in the early days of a sun … Continue reading Sun Stability