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Prog. Theor. Phys. Supplement No.96 (1988) pp. 274-280
Chapter 23. Gas Capture by Proto-Jupiter and Proto-Saturn
Minoru Sekiya,
Shoken M. Miyama* and
Chushiro Hayashi**
Department of Applied Physics, Tokyo Institute of Technology, Tokyo 152
*Department of Physics, Kyoto University, Kyoto 606
**Momoyama Yogoro-cho 1, Fushimi-ku, Kyoto 612
(Received October 28, 1988)
Abstract:
The interaction of proto-giant-planets and the solar nebula in the stage after the occurrence of Mizuno's instability of the proto-giant-planets is reviewed. When the mass of proto-Jupiter reaches the present Jovian value by accreting the gases of the solar nebula, proto-Jupiter begins to push the gases away from its orbit and form a gap around the orbit. It is considered that this process determined the present Jovian mass. On the other hand, Saturn would have stopped growing owing to the dissipation of the nebular gas.
URL :
http://ptp.ipap.jp/link?PTPS/96/274/
DOI : 10.1143/PTPS.96.274
References:
- Bodenheimer, P., in Protostars and Planets II, ed. D. C. Black and M. S. Matthews (Univ. Arizona Press, Tucson, 1985), p. 873.
Bodenheimer, P., Grossman, A. S., De Campli, W. M., Marcy, G. and Pollack, J. B., Icarus 41 (1980), 293.
Goldreich, P. and Tremaine, S., Astrophys. J. 241 (1980), 425[CrossRef].
Grossman, A. S., Pollack, J. B., Reynolds, R. T., Summers, A. L. and Graboske, H. C., Jr., Icarus 42 (1980), 358.
Hayashi, C., Prog. Theor. Phys. Suppl. No. 70 (1981), 35[IPAP].
Lin, D. N. C. and Papaloizou, J., Astrophys. J. 307 (1986), 395.
Miyama, S. M., Hayashi, C. and Narita, S., Astrophys. J. 279 (1984), 621[CrossRef].
Mizuno, H., Prog. Theor. Phys. 64 (1980), 544[IPAP].
Papaloizou, J. and Lin, D. N. C., Astrophys. J. 285 (1984), 818.
Sekiya, M. and Miyama, S. M., (1988) in preparation.
Sekiya, M., Miyama, S. M. and Hayashi, C., Earth Moon Planets 39 (1987), 1.
Stevenson, D. J., Ann. Rev. Earth Planet. Sci. 10 (1982), 257.
