Gravitational instability and the formation of planetary systems of solar-type stars | Zendy

Михаил Семенович Легкоступов | Zendy

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Gravitational instability and the formation of planetary systems of solar-type stars

Author(s) -

Михаил Семенович Легкоступов

Publication year - 2021

Publication title -

keldysh institute preprints

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.

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