On the issue of gravitational instability of the protoplanetary disk of the Sun. Part I. Formulation of the problem
Abstract:
The paper presents a brief overview of the results of research on the mediums gravitational instability. A physico-mathematical model of the initial stage of the Sun protoplanetary disk evolution is proposed on the base of analysis of the main models of the solar planetary system formation.
Keywords:
protoplanetary disk, gravitational instability, own gravitational field, numerical simulation, dispersion equation, planetary system
