Open AccessGravitational instability and the formation of planetary systems of solar-type stars
Author(s) -
Михаил Семенович Легкоступов
Publication year - 2021
Publication title -
preprint/preprinty ipm im. m.v. keldyša
Language(s) - English
Resource type - Journals
eISSN - 2071-2901
pISSN - 2071-2898
DOI - 10.20948/prepr-2021-15
Subject(s) - physics , gravitational instability , stars , planetary system , astronomy , solar system , instability , astrobiology , planet , formation and evolution of the solar system , astrophysics , mechanics , galaxy
The fundamental principles of the protoplanetary ring model – the model of formation of planetary systems of stars, which is based on the origin and development of large-scale gravitational instabilities (protoplanetary rings) – are extended to the formation of regular planetary satellites. Based on these principles, a complete model of the formation of planetary systems, including their satellites, (model of gas and dust rings) for solar-type stars is proposed.