Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-27T15:42:04.183Z Has data issue: false hasContentIssue false
  • English
  • Français

N-body Simulations of Planet Formation

Published online by Cambridge University Press:  26 May 2016

Shigeru Ida ,
Eiichiro Kokubo  and
Junko Kominami
Shigeru Ida
Affiliation:
Tokyo Institute of Technology, Meguro-ku, Tokyo 158-5881, Japan
Eiichiro Kokubo
Affiliation:
National Astronomical Observatory, Mitaka-shi, Tokyo 181-8588, Japan
Junko Kominami
Affiliation:
Tokyo Institute of Technology, Meguro-ku, Tokyo 158-5881, Japan

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Accretion from many small planetesimals to planets is reviewed. Solid protoplanets accrete through runaway and oligarchic growth until they become isolated. The isolation mass of protoplanets in terrestrial planet region is about 0.1-0.2 Earth mass, which suggests giant impacts among the protoplanets in the final stage of terrestrial planet formation. On the other hand, the isolation mass in Jupiter's and Saturn's orbits is about a few to 5 Earth masses, which may be massive enough to trigger gas accretion onto the cores. The isolation mass in Uranus and Neptune's orbits is as large as their present cores. Extending the above arguments to extrasolar planetary systems that are formed from disks with various initial masses, we also discuss diversity of extrasolar planetary systems.

Type
Planetary Formation
Information
Symposium - International Astronomical Union , Volume 208: Astrophysical Supercomputing using Particle Simulations , 2003 , pp. 25 - 35
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Adachi, I., Hayashi, C., & Nakazawa, K. 1976, Prog. Theor. Phys., 56, 1756 CrossRefGoogle Scholar
Agnor, C. B., Canup, R. M., & Levison, H. F. 1999, Icarus, 142, 219 CrossRefGoogle Scholar
Beckwith, S. V. W. & Sargent, A. I. 1993, in Protostars and Planets III, ed. Levy, E. H. & Lunine, J. I. (Tuscon: Univ. of Arizona Press), 521; 1996, Nature, 383, 139 Google Scholar
Bodenheimer, P. & Pollack, J. B. 1986, Icarus, 67, 391 Google Scholar
Chambers, J. E. & Wetherill, G. W. 1998, Icarus, 136, 30 Google Scholar
Chambers, J. E., Wetherill, G. W., & Boss, A. P. 1996, Icarus, 119, 261 CrossRefGoogle Scholar
Hayashi, C. 1981, Prog. Theor. Phys. Suppl., 70, 35 CrossRefGoogle Scholar
Hayashi, C., Nakazawa, K., & Nakagawa, Y. 1985 in Protostars and Planets II, ed. Black, D. C. & Matthews, M. S. (Tuscon: Univ. of Arizona Press), 1100 Google Scholar
Ida, S. & Kokubo, E. 2001, in ASP Conf. Series, Planetary Systems in the Universe: Observation, Formation and Evolution, eds. Penny, A.J., Artymowicz, P., Lagrange, A.-M., and Russell, S.S. (San Francisco, ASP), in press Google Scholar
Ida, S. & Makino, J. 1992, Icarus, 96, 107; 1993, Icarus, 106, 210 Google Scholar
Ikoma, M., Nakazawa, K., & Emori, H. 2000, ApJ, 537, 1013 CrossRefGoogle Scholar
Ito, T. & Tanikawa, K. 1999, Icarus, 139, 336 Google Scholar
Iwasaki, K, Tanaka, H., Nakazawa, K., & Emori, H. 2001a, PASJ, 53, 321; 2001b, submitted to PASJ Google Scholar
Kokubo, E. & Ida, S 1995, Icarus, 114, 247; 1996, Icarus, 123, 180; 1998, Icarus, 131, 171; 2000, Icarus, 143, 15 CrossRefGoogle Scholar
Lin, D. N. C. & Ida, S. 1997, ApJ, 477, 781 CrossRefGoogle Scholar
Lin, D. N. C., Bodenheimer, P., & Richardson, D. 1996, Nature, 380, 606 CrossRefGoogle Scholar
Lin, D. N. C. & Papaloizou, J. C. B. 1993, in Protostars and Planets III, ed. Levy, E. H. & Lunine, J. I. (Tuscon: Univ. of Arizona Press), 749 Google Scholar
Mizuno, H. 1981, Prog. Theor. Phys., 64, 544 CrossRefGoogle Scholar
Nagasawa, M, Tanaka, H. & Ida, S. 2000, AJ, 119, 1480 CrossRefGoogle Scholar
Safronov, V. 1969, Evolution of the protoplanetary cloud and formation of the earth and planets (Moscow: Nauka Press)Google Scholar
Stewart, G. R. & Wetherill, G. W. 1988, Icarus, 74, 542 CrossRefGoogle Scholar
Strom, S. E., Edwards, S., & Skrutski, M. F. 1993, in Protostars and Planets III eds. Levy, E.H. & Lunine, J.I. (Tucson: Univ. of Arizona Press), 837 Google Scholar
Ward, W. R. 1986, Icarus, 67, 164; 1993, Icarus, 106, 274; 1997 Icarus, 126, 261 Google Scholar
Weidenschilling, S. J. 1984, Icarus, 60, 553 CrossRefGoogle Scholar
Weidenschilling, S. J. & Marzari, F. 1996, Nature, 384, 619 CrossRefGoogle Scholar
Wetherill, G. W. 1980, ARA&A, 18, 77 Google Scholar
Wetherill, G. W. & Stewart, G. R. 1989, Icarus, 77, 330 Google Scholar
Zuckerman, B., Forveille, T. & Kastner, J. H. 1995, Nature, 373, 494 Google Scholar