Revisiting dynamics of Sun center relative to barycenter of Solar system
Sergey V. Ershkov, Dmytro Leshchenko

TL;DR
This paper revisits the Sun's motion relative to the Solar system barycenter, proposing a model based on the Sun's self-resulting photo-gravitational force and suggesting a method for stellar navigation using this force.
Contribution
It introduces a novel approach to Solar system dynamics by emphasizing the Sun's self-resulting photo-gravitational force and proposes an algorithm for star navigation based on this force.
Findings
Hierarchical Solar system configuration remains stable during outward motion at high velocity.
Proposed algorithm for moving towards stars using the Sun's photo-gravitational force.
Solar system size may increase over time due to angular momentum loss.
Abstract
We introduce here in the current research the revisiting of approach to the dynamics of Sun center relative to barycenter of Solar system by using self-resulting photo-gravitational force of the Sun as the main reason of such motion. In case of slowly moving in the direction outwards with respect to the initial position of barycenter of Solar system (together with the current position of Solar system barycenter, of course) with average established velocity not less than 1050 Km/day, we should especially note that hierarchical configuration of Solar system will be preferably the same during this motion. As the main findings, we have suggested algorithm how to move towards stars using Solar self-resulting photo-gravitational force. The obvious physically reasonable assumption is that the Solar system will have been increasing its size during the evolution in a future (due to losses of the…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Earth Systems and Cosmic Evolution · Fluid dynamics and aerodynamics studies
