Stimulated Radiative Molecular Association in the Early Solar System. II. Orbital Radii of the Planets and Other Satellites of the Sun
James C. Lombardi Sr

TL;DR
This paper proposes a model linking the orbital radii of planets and satellites to photon energies in hydrogen spectra, explaining their formation and distribution in the early solar system.
Contribution
It extends a previous model to the Sun's planetary system, relating orbital positions to SRMA reactions and photon energies, and offers explanations for belts and planetary features.
Findings
Orbital radii correlate with hydrogen photon energies.
Protosun's surface temperature was higher than T Tauri stars.
A primordial belt likely existed near Neptune.
Abstract
In a previous investigation, the orbital radii of regular satellites of Uranus, Jupiter, Neptune, and Saturn are shown to be directly related to photon energies in the spectra of atomic and molecular hydrogen. To explain these observations a model was developed involving stimulated radiative molecular association (SRMA) reactions among photons and atoms in the protosatellite disks of the planets. In the present investigation, the previously developed model is applied to the planets and important satellites of the Sun. A key component of the model involves resonance associated with SRMA. Through this resonance, thermal energy is extracted from the protosun's protoplanetary disk at specific distances from the protosun wherever there is a match between the local thermal energy of the disk and the energy of photons impinging on the disk. Orbital radii of the planets and satellites are…
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Taxonomy
TopicsAstro and Planetary Science · Astrophysics and Star Formation Studies · Atmospheric Ozone and Climate
