Magnetic Monopoles and the Origin of the Solar Systyem.docx

This paper attributes the origin of the solar system to the rotation of an electron about a magnetic monopole, generating gravitational waves of increasing wavelength that lead to the accretion of hydrogen and helium from the protoplanetary disk resulting in formation of the Sun, and to the nucleation of dust particles about the rotating electron giving rise to the planets. The initial separation of the protoplanetary disk from the solar nebula 4.6 billion years ago is considered to be a phase separation driven by a magnetic monopole being separated out of the gas and dust particles in the solar nebula.