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This article is cited in 1 scientific paper (total in 1 paper)
Gravitational instability and the formation of planetary systems of solar-type stars
M. S. Legkostupov
Abstract:
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.
Keywords:
protosolar nebular, gravitational instability, protoplanetary disk,
protoplanetary ring, protosatellite disk, astrophysical observations, planetary system.
Citation:
M. S. Legkostupov, “Gravitational instability and the formation of planetary systems of solar-type stars”, Keldysh Institute preprints, 2021, 015, 32 pp.
Linking options:
https://www.mathnet.ru/eng/ipmp2933 https://www.mathnet.ru/eng/ipmp/y2021/p15
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