Cosmogony of Open Solar System (II): Model of Secondary Planet Formation, Secondary Accretion Disk of the Sun, Formation of Satellites of Giant Planets, Molchanov’s Resonance, Titius–Bode Rule

The chaptere delves into the complex processes involved in the formation of the Solar System, with a particular focus on the secondary accretion disk of the Sun and the subsequent formation of giant planets and their satellites. It introduces two phenomenological models designed to study these processes under the conditions of 'open' systems, where traditional physical theories and celestial mechanics methods are limited. The text explores the integral parameters of the primary and secondary accretion disks, noting their differences in the distribution of average matter density. It also discusses the two-stage formation of giant planets and the intensive formation of regular satellites in the first 100 million years after Phaeton's destruction. The chaptere highlights the role of cyclic bombardments by galactic comets and the formation of satellite 'embryos' from cometoasteroid bodies and the substance of giant planets. Additionally, it examines the phenomenon of parametric resonance in the systems of satellites of giant planets, providing insights into the quantization of their orbits. The text concludes with a discussion on the Titius–Bode rule and its implications for the current configuration of the Solar System.