Abstract
In the present paper, the early evolution of the Solar System with regard to the process of the formation and mass growth of small bodies in protoplanetary rings is considered. This process is modeled with the use of the results that were obtained in the analysis of the libration motions of asteroids. It has been shown that libration centers could occur prior to the formation of the bodies, when the redistribution of gaseous-dust grains occurred in protoplanetary rings. The distribution density of gaseous-dust grains could be similar or equal to that in the Gaussian ring or its analogs for long-period librations. In this case, the bodies can be initially formed and grow in stable libration centers.
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References
T. R. Abdul’myanov and R. V. Zagretdinov, Kinematika i Fiz. Nebesnykh Tel 11, no. 4, 34 (1994).
T. R. Abdul’myanov, Solar Syst. Res. 35, no. 5, 408 (2001).
T. R. Abdulmyanov, Proc. Eur. Planetary Sci. Congress, EPSC2012-75, Madrid, Spain, 2012, vol. 7.
T. R. Abdulmyanov, Proc. Eur. Planetary Sci. Congress. EPSC2013-720, London, 2013, vol. 8.
T. R. Abdulmyanov, Proc. Eur. Planetary Sci. Congress. EPSC2013-722, London, 2013, vol. 8.
Y. Alibert, C. Broeg, W. Benz, G. Wuchterl, O. Grasset, C. Sotin, C. Eiroa, T. Henning, T. Herbst, L. Kaltenegger, A. Léger, R. Liseau, H. Lammer, Ch. Beichman, W. Danchi, M. Fridlund, J. Lunine, F. Paresce, A. Pen- ny, A. Quirrenbach, H. Röttgering, F. Selsis, J. Schneider, D. Stam, G. Tinetti, and G. J. White, Astrobiology 10, no. 1, 19 (2010).
P. J. Armitage, Lecture Notes on the Formation and Early Evolution of Planetary Systems, (Astrophys. Planet Formation, Cambridge University, 2010).
E. M. Galimov, A. M. Krivtsov, A. V. Zabrodin, Yu. I. Sidorov, M. S. Legkostupov, and T. M. Eneev, Geochem. Int. 43, no. 11, 1045 (2005).
B. Garfinkel, Astron. J. 82, 368 (1977).
K. F. Gauss, Werke 3, 333–355 (1866).
L. E. Gurevich and A. I. Lebedinskii, Izv. Akad. Nauk SSSR, Ser. Fiz. 14, no. 6, 765 (1950).
A. Johansen, J. Oishi, M. MacLow, H. Klahr, Th. Henning, and A. Youdin, Nature 448, 1022 (2007).
A. V. Zabrodin, E. A. Zabrodina, M. S. Legkostupov, K. V. Manukovsky, and L. A. Pliner, Some models of description protoplanetary Soleil disk on the beginning stage of its evolution, Preprint Inst. Appl. Mathem. Russ. Acad. Sci., 2006, no. 070, p. 44.
B. P. Kondrat’ev, Theory of Potential. New Methods and Problems with Solutions(Moscow, 2007) [in Russian].
B. P. Kondrat’ev, Solar Syst. Res. 46, no. 5, 241 (2012).
K. Murray and S. Dermott, Solar System Dynamics (Oxford: Oxford Univ., 1999; Moscow, 2009).
V. S. Safronov, The Evolution of the Protoplanetary Cloud and the Formation of the Earth and the Planets (Moscow: Nauka, 1969).
M. F. Subbotin, Introduction in Theoretic Astronomy (Moscow, 1968) [in Russian].
T. M. Eneev and N. N. Kozlov, Astron. Vestn. 15, no. 2, 80 (1981).
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Original Russian Text © T.R. Abdul’myanov, 2014, published in Vestnik Moskovskogo Universiteta. Fizika, 2014, No. 6, pp. 115–121.
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Abdul’myanov, T.R. On the mechanism of the formation and mass growth of solar system bodies at the early stages of evolution. Moscow Univ. Phys. 69, 558–564 (2014). https://doi.org/10.3103/S0027134914060022
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DOI: https://doi.org/10.3103/S0027134914060022