Abstract
The results of the computer simulation for the circumsolar gas-dust cloud evolution are presented. The particle dynamics method is used. We show that gas-dust clusters can be formed in ring-shaped structures of protoplanetary disks. It is demonstrated that the clusters are formed as a result of the counteracting of the self-gravitational force of the ring and the gravity of the Sun. This process has a probabilistic nature. The range of the system parameters providing the clusters formation is obtained. Different scenarios of the ring evolution are observed and analyzed. The considered gas-dust clusters can be precursors for the further formation of the planet-satellite systems.
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Murachev, A.S., Tsvetkov, D.V., Galimov, E.M., Krivtsov, A.M. (2018). Numerical Simulation of Circumsolar Ring Evolution. In: dell'Isola, F., Eremeyev, V., Porubov, A. (eds) Advances in Mechanics of Microstructured Media and Structures. Advanced Structured Materials, vol 87. Springer, Cham. https://doi.org/10.1007/978-3-319-73694-5_14
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DOI: https://doi.org/10.1007/978-3-319-73694-5_14
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