The Process of Formation of a Single Star System for Gravitational Compression of a Gas-dust Cloud in Outer Space

Abstract

In this paper it is shown that in the process of formation of a single star system favorable conditions are created for the appearance of the planetary system due to the collision of the oppositely moving condensed dust zones from the newly born star and falling onto it from the periphery. A hypothetical version of the possible structure of the core of a single star born in a rarefied gas-dust cloud, explaining the cause of the mismatch of the axis of rotation of the star and the dipole magnetic field, is proposed. An assumption is made about the causes of the appearance of a directed orbital motion of planets that are not related to external perturbations of the initial gas-dust cloud.