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KIAM Preprint  15, Moscow, 2021
Authors: Legkostupov M.S.
Gravitational instability and the formation of planetary systems of solar-type stars
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.
protosolar nebular, gravitational instability, protoplanetary disk, protoplanetary ring, protosatellite disk, astrophysical observations, planetary system
Publication language: russian,  pages: 32
Research direction:
Theoretical and applied problems of mechanics
Russian source text:
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About authors:
  • Legkostupov Mikhail Semenovich, RAS