Hydrogen Spectra, Molecular Association and Orbital Radii in the Solar System
| dc.creator | Lombardi Sr., James C. | |
| dc.date | 2003-07-24 | |
| dc.date.accessioned | 2026-07-07T06:27:54Z | |
| dc.date.available | 2026-07-07T06:27:54Z | |
| dc.description | A relationship between the average orbital radii of the planets and their satellites in the solar system and the spectra of atomic and molecular hydrogen is identified and investigated. In this model, stimulated radiative association resonances develop early on in the disk of the protosun that cause the disk to cool at only certain radii, with each radius depending on a specific photon energy in the atomic hydrogen spectrum. The planets then evolve from the relatively cool rings that are formed. Similar activity occurs in the formation of the satellite systems of the giant planets. The present investigation deals with the mechanism that generates rings from which the planets are formed. It does not deal with the evolution of the rings into planets. Many characteristics of the solar system are explained including the sizes of the orbital radii of the planets and their satellites, the tilt of Uranus's axis, the positions of the asteroid and Kuiper belts, the source of the scattered Kuiper belt objects, the positions of Saturn's main rings and the rings of Uranus, Jupiter, and Neptune. It also shows that a commonality exists in the structures of the solar system and the planetary systems that can be attributed to the common process that initiated their evolution. | |
| dc.description | 44 pages including 8 tables and 8 figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0307421 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0307421 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/97552 | |
| dc.subject | Astrophysics | |
| dc.title | Hydrogen Spectra, Molecular Association and Orbital Radii in the Solar System | |
| dc.type | text |