N-Body simulations of growth from 1 km planetesimals at 0.4 AU

Icarus

Volumn 203, Issue 2, 2009, Pages 626-643

  Barnes, Rory ^a,b,c   Quinn, Thomas R ^a   Lissauer, Jack J ^d   Richardson, Derek C ^e  

^a UNIVERSITY OF WASHINGTON   (United States)

^b UNIVERSITY OF ARIZONA   (United States)

^c Virtual Planetary Laboratory   (United States)

^d NASA AMES RESEARCH CENTER   (United States)

^e Bldg 142   (United States)

Author keywords

Earth; Origin, Solar system; Planetary formation; Planetesimals

Indexed keywords

EID: 70049111008     PISSN: 00191035     EISSN: 10902643     Source Type: Journal    
DOI: 10.1016/j.icarus.2009.03.042     Document Type: Article

References (52)

1. Aarseth, S., Lecar, M. 1984. The formation of the terrestrial planets from lunar sized planetesimals. In: Brahic, A. (Ed.), Proc. to IAU Colloq. No. 75: Planetary Rings, Cepadues, Toulouse, pp. 661-674.
2. Adachi I., Hayashi C., and Nakazawa K. The gas drag effect on the elliptical motion of a solid body in the primordial solar nebula. PThPh 56 (1976) 1756-1771
3. Agnor C.B., Canup R.M., and Levison H.F. On the character and consequences of large impacts in the late stage of terrestrial planet formation. Icarus 142 (1999) 219-237
4. Barnes J., and Hut P. A hierarchical O(N log N) force-calculation algorithm. Nature 324 (1986) 446-449
5. Binney J., and Tremaine S. Galactic Dynamics (1994), Princeton University Press, Princeton, NJ pp. 120-126
6. Chamberlin T.C. On a possible function of disruptive approach in the formation of meteorites, comets, and nebulae. Astrophys. J. 14 (1901) 17-41
7. Chambers J.E. Making more terrestrial planets. Icarus 152 (2001) 205-224
8. Edgeworth K.E. The origin and evolution of the solar system. MNRAS 109 (1949) 600-609
9. Garaud P., and Lin D.N.C. On the evolution and stability of a protoplanetary disk dust layer. Astrophys. J. 608 (2004) 1050-1075
10. Gehrels N. Confidence limits for small numbers of events in astrophysical data. Astrophys. J. 303 (1986) 336-346
11. Goldreich P., and Ward W.R. The formation of planetesimals. Astrophys. J. 183 (1973) 1051-1062
12. Goldreich P., Lithwick Y., and Sari R. Final stages of planet formation. Astrophys. J. 614 (2004) 497-507
13. Greenberg R., Hartmann W.K., Chapman C.R., and Wacker J.F. Planetesimals to planets - Numerical simulation of collisional evolution. Icarus 35 (1978) 1-26
14. Greenzweig Y., and Lissauer J.J. Accretion rates of protoplanets. Icarus 87 (1990) 40-77
15. Hayashi C. Structure of the solar nebula, growth and decay of magnetic fields and effects of magnetic and turbulent viscosities on the nebula. PThPS 70 (1980) 35-53
16. Hayashi C., Nakazawa K., and Adachi I. Long-term behavior of planetesimals and the formation of the planets. PASJ 29 (1977) 163-196
17. Heggie D.C. Binary evolution in stellar dynamics. Mon. Not. R. Astron. Soc. 173 (1975) 729-787
18. Hill G.W. Researches in the lunar theory. Am. J. Math. 1 (1878) 5-26
19. Johansen A., Oishi J.S., Low M.M., Klahr H., Henning T., and Youdin A. Rapid planetesimal formation in turbulent circumstellar disks. Nature 448 (2007) 1022-1025
20. Kenyon S.J., and Bromeley B.C. Terrestrial planet formation. I. The transition from oligarchic growth to chaotic growth. Astron. J. 131 (2006) 1837-1850
21. Kenyon S.J., and Bromley B.C. Collisional cascades in planetesimal disks. II. Embedded planets. Astron. J. 127 (2004) 513-530
22. Kenyon S.J., and Luu J.X. Accretion in the early kuiper belt. I. Coagulation and velocity evolution. AJ 115 (1998) 2136-2160
23. Kokubo E.S., and Ida S. On runaway growth of planetesimals. Icarus 123 (1996) 180-191
24. Kokubo E.S., and Ida S. Formation of protoplanet systems and diversity of planetary systems. Astrophys. J. 581 (2002) 666-680
25. Kolvoord R.A., and Greenberg R. A critical reanalysis of planetary accretion models. Icarus 98 (1992) 2-19
26. Leinhardt Z.M., and Richardson D.C. Planetesimals to protoplanets. I. Effect of fragmentation on terrestrial planet formation. Icarus 625 (2005) 427-440
27. Leinhardt, Z.M., Richardson, D.C., Lufkin, G., Haseltine, J., 2009. Planetesimals to protoplanets. II: Effect of debris on terrestrial planet formation. MNRAS 396, 718-728.
28. Lissauer J.J. Timescales for planetary accretion and the structure of the protoplanetary disk. Icarus 69 (1987) 249-265
29. Lissauer J.J. Urey prize lecture: On the diversity of plausible planetary systems. Icarus 14 (1995) 217-236
30. Lissauer, J.J., Slartibartfast, 2008. How extreme can planets be? In: Fischer, D.A., Rasio, F.A., Thorsett, S.E., Wolszczan, A. (Eds.), Extreme Solar Systems, ASP Conference Series, pp. 491-498.
31. Lissauer, J.J., Stewart, G.R. 1993. Growth of planets from planetesimals. In: Lissauer, J.J., Stewart, G.R. (Eds.), Protostars and Planets III, pp. 1061-1088.
32. Moore B., Governato F., Quinn T., Stadel J., and Lake G. Resolving the structure of cold dark matter halos. Astrophys. J. 499 (1998) L5-L8
33. Morishima R., Schmidt M.W., Stadel J., and Moore B. Formation and accretion history of terrestrial planets from runaway growth through to late time: implications for orbital eccentricity. Astrophys. J. 685 (2008) 1247-1261
34. O'Brien D.P., Morbidelli A., and Levison H.F. Terrestrial planet formation with strong dynamical friction. Icarus 184 (2006) 39-58
35. Press W.H., Teukolsky S.A., Vetterling W.T., and Flannery B.P. Numerical Recipes in C: The Art of Scientific Computing (1996), Cambridge University Press, Cambridge pp. 657-661
36. Rafikov R.R. Fast accretion of small planetesimals by protoplanetary cores. Astron. J. 128 (2004) 1348-1363
37. Raymond S.N., Barnes R., and Kaib N. Predicting new planets in known extra-solar planetary systems. III: Terrestrial planet formation. Astrophys. J. 644 (2006) 1223-1231
38. Richardson D.C., Quinn T., Stadel J., and Lake G. Direct large-scale N-body simulations of planetesimal dynamics. Icarus 143 (2000) 45-59
39. Safronov V.S. On the gravitational instability in flattened systems with axial symmetry and non-uniform rotation. Ann. Astrophys. 23 (1960) 979-982
40. Safronov, V.S., 1969. Evolution of the protoplanetary cloud and formation of the Earth and the planets (NASA Tech. Trans. F-677, Nauka Press, Moscow).
41. Saha P., and Tremaine S. Symplectic integrators for solar system dynamics. Astron. J. 104 (1992) 1633-1640
42. Stadel, J.G., 2001. Cosmological N-body simulations and their analysis. Ph.D. Thesis, University of Washington.
43. Stewart G.R., and Wetherill G.W. Evolution of planetesimal velocities. Icarus 74 (1988) 542-553
44. Wadsley J.W., Stadel J., and Quinn T. Gasoline: A flexible, parallel implementation of TreeSPH. New Astron. 9 (2004) 137-158
45. Weidenschilling S.J. Aerodynamics of solid bodies in the solar nebula. Mon. Not. R. Astron. Soc. 180 (1977) 57-70
46. Weidenschilling S.J. Can gravitational instability form planetesimals?. Icarus 116 (1995) 433-435
47. Weidenschilling, S.J., Cuzzi, J.N., 1993. Formation of planetesimals in the solar nebula. Protostars and Planets III, pp. 1031-1060.
48. Weidenschilling S.J., Spaute D., Davis D.R., Marzari F., and Ohtsuki K. Accretional evolution of a planetesimal swarm. Icarus 128 (1997) 429-455
49. Wetherill G.W. Comparison of analytical and physical modeling of planetesimal accumulation. Icarus 88 (1990) 336-354
50. Wetherill G.W., and Stewart G.R. Accumulation of a swarm of small planetesimals. Icarus 77 (1989) 330-357
51. Wisdom J., and Tremaine S. Local simulations of planetary rings. Astron. J. 95 (1988) 925-940
52. Youdin A.N., and Shu F. Planetesimal formation by gravitational instability. Astrophys. J. 580 (2002) 494-505