Planetesimal formation by turbulent concentration

Icarus

Volumn 208, Issue 2, 2010, Pages 505-517

  Chambers, J E ^a  

^a GEOPHYSICAL LABORATORY   (United States)

Author keywords

Origin, Solar System; Planetary formation; Planetesimals; Solar nebula

Indexed keywords

EID: 77955690931     PISSN: 00191035     EISSN: 10902643     Source Type: Journal    
DOI: 10.1016/j.icarus.2010.03.004     Document Type: Article

References (55)

1. Blum J., Wurm G. The growth mechanisms of macroscopic bodies in protoplanetary disks. Annu. Rev. Astron. Astrophys. 2008, 46:21-56.
2. Brauer F., Dullemond C.P., Henning T. Coagulation, fragmentation and radial motion of solid particles in protoplanetary disks. Astron. Astrophys. 2008, 480:859-877.
3. Chambers J.E. Making more terrestrial planets. Icarus 2001, 152:205-224.
4. Chambers J.E. Planetary accretion in the inner Solar System. Earth Planet. Sci. Lett. 2004, 223:241-252.
5. Chambers J.E. Planet formation with migration. Astrophys. J. 2006, 652:L133-L136.
6. Ciesla F.J., Cuzzi J.N. The evolution of the water distribution in a viscous protoplanetary disk. Icarus 2006, 181:178-204.
7. Cuzzi J.N., Weidenschilling S.J. Particle-gas dynamics and primary accretion. Meteorites and the Early Solar System II 2006, 353-381. University of Arizona Press. D.S. Lauretta, H. McSween (Eds.).
8. Cuzzi J.N., Dobrovolskis A.R., Hogan R.C. Turbulence, chondrules, and planetesimals. Chondrules and the Protoplanetary Disk 1996, 35-43. Cambridge University Press. R.H. Hewins, R.H. Jones, E.R.D. Scott (Eds.).
9. Cuzzi J.N., Hogan R.C., Paque J.M., Dobrovolskis A.R. Size-selective concentration of chondrules and other small particles in protoplanetary nebula turbulence. Astrophys. J. 2001, 546:496-508.
10. Cuzzi, J.N., Hogan, R.C., Shariff, K., 2007. Towards a scenario for primary accretion of primitive bodies. Lunar Planet. Sci. 38, 1439 (abstracts).
11. Cuzzi J.N., Hogan R.C., Shariff K. Toward planetesimals: Dense chondrule clumps in the protoplanetary nebula. Astophys. J. 2008, 687:1432-1447.
12. Cuzzi, J.N., Hogan, R.C., Bottke, W., 2009. Primary accretion: The birth population in the asteroid and KBO regions. Lunar Planet. Sci. 40, 2418 (Technical Report, abstracts).
13. D'Alessio P., Calvet N., Hartmann L. Accretion disks around young objects. III. Grain growth. Astrophys. J. 2001, 553:321-334.
14. Fessler J.R., Kulick J.D., Eaton J.K. Preferential concentration of heavy particles in a turbulent channel flow. Phys. Fluids 1994, 6:3742-3749.
15. Garaud P., Lin D.N.C. On the evolution and stability of a protoplanetary disk dust layer. Astrophys. J. 2004, 608:1050-1075.
16. Garaud P., Lin D.N.C. The effect of internal dissipation and surface irradiation on the structure of disks and the location of the snow line around Sun-like stars. Astrophys. J. 2007, 654:606-624.
17. Goldreich P., Ward W.R. The formation of planetesimals. Astrophys. J. 1973, 183:1051-1062.
18. Haghighipour N., Boss A.P. On pressure gradients and rapid migration of solids in a nonuniform solar nebula. Astrophys. J. 2003, 583:996-1003.
19. Haisch K.E., Lada E.A., Lada C.J. Disk frequencies and lifetimes in young clusters. Astrophys. J. 2001, 553:L153-L156.
20. Hartmann L., Calvet N., Gullbring E., D'Alessio P. Accretion and the evolutiion of T Tauri disks. Astrophys. J. 1998, 495:385-400.
21. Hawley J.F., Gammie C.F., Balbus S.A. Local three-dimensional magnetohydrodynamic simulations of accretion disks. Astrophys. J. 1995, 440:742-763.
22. Hogan R.C., Cuzzi J.N. Stokes and Reynolds number dependence of preferential particle concentration in simulated three-dimensional turbulence. Phys. Fluids 2001, 13:2938-2945.
23. Hogan R.C., Cuzzi J.N. Cascade model for particle concentration and enstrophy in fully developed turbulence with mass-loading feedback. Phys. Rev. 2007, 75(5):056305-1-056305-9.
24. Hogan R.C., Cuzzi J.N., Dobrovolskis A.R. Scaling properties of particle density fields formed in simulated turbulent flows. Phys. Rev. 1999, 60:1674-1680.
25. Hubickyj O., Bodenheimer P., Lissauer J.J. Accretion of the gaseous envelope of Jupiter around a 5-10 Earth-mass core. Icarus 2005, 179:415-431.
26. Hueso R., Guillot T. Evolution of protoplanetary disks: Constraints from DM Tauri and GM Aurigae. Astron. Astrophys. 2005, 442:703-725.
27. Ikoma M., Nakazawa K., Emori H. Formation of giant planets: Dependences on core accretion rate and grain opacity. Astrophys. J. 2000, 537:1013-1025.
28. Inaba S., Wetherill G.W., Ikoma M. Formation of gas giant planets: Core accretion models with fragmentation and planetary envelope. Icarus 2003, 166:46-62.
29. Johansen A., Oishi J.S., Low M.-M.M., Klahr H., Henning T., Youdin A. Rapid planetesimal formation in turbulent circumstellar disks. Nature 2007, 448:1022-1025.
30. Kenyon S.J., Bromley B.C. Terrestrial planet formation. I. The transition from oligarchic growth to chaotic growth. Astron. J. 2006, 131:1837-1850.
31. Kokubo E., Ida S. Oligarchic growth of protoplanets. Icarus 1998, 131:171-178.
32. Lissauer J.J. Timescales for planetary accretion and the structure of the protoplanetary disk. Icarus 1987, 69:249-265.
33. Lissauer J.J., Stevenson D.J. Formation of giant planets. Protostars and Planets V 2007, 591-606. University of Arizona Press. B. Reipurth, D. Jewitt, K. Keil (Eds.).
34. Lodders K. Solar System abundances and condensation temperatures of the elements. Astrophys. J. 2003, 591:1220-1247.
35. Matsumura S., Pudritz R.E. Dead zones and extrasolar planetary properties. Mon. Not. R. Astron. Soc. 2006, 365:572-584.
36. Meneveau C., Sreenivasan K.R. The multifractal nature of turbulent energy dissipation. J. Fluid Mech. 1991, 224:429-484.
37. Morfill G.E. Some cosmochemical consequences of a turbulent protoplanetary cloud. Icarus 1983, 53:41-54.
38. Nelson R.P. On the orbital evolution of low mass protoplanets in turbulent, magnetised disks. Astron. Astrophys. 2005, 443:1067-1085.
39. O'Brien D.P., Morbidelli A., Levison H.F. Terrestrial planet formation with strong dynamical friction. Icarus 2006, 184:39-58.
40. Ormel C.W., Cuzzi J.N., Tielens A.G.G.M. Co-accretion of chondrules and dust in the solar nebula. Astrophys. J. 2008, 679:1588-1610.
41. Pollack J.B., Hubickyj O., Bodenheimer P., Lissauer J.J., Podolak M., Greenzweig Y. Formation of the giant planets by concurrent accretion of solids and gas. Icarus 1996, 124:62-85.
42. Rafikov R.R. Fast accretion of small planetesimals by protoplanetary cores. Astron. J. 2004, 128:1348-1363.
43. Raymond S.N., Quinn T., Lunine J.I. High-resolution simulations of the final assembly of Earth-like planets. I. Terrestrial accretion and dynamics. Icarus 2006, 183:265-282.
44. Safronov V.S. Evolution of the Protoplanetary Cloud and Formation of the Earth and Planets 1969, Nauka Press, Moscow, English Translation: NASA TTF-677.
45. Sekiya M. Gravitational instabilities in a dust-gas layer and formation of planetesimals in the solar nebula. Prog. Theor. Phys. 1983, 69:1116-1130.
46. Shakura N.I., Sunyaev R.A. Black holes in binary systems. Observational appearance. Astron. Astrophys. 1973, 24:337-355.
47. Squires K.D., Eaton J.K. Preferential concentration of particles by turbulence. Phys. Fluids A 1991, 3:1169-1178.
48. Sreenivasan K.R., Stolovitzky G. Turbulent cascades. J. Stat. Phys. 1995, 78:311-333.
49. Thommes E.W., Duncan M.J., Levison H.F. Oligarchic growth of giant planets. Icarus 2003, 161:431-455.
50. Weidenschilling S.J. Aerodynamics of solid bodies in the solar nebula. Mon. Not. R. Astron. Soc. 1977, 180:57-70.
51. Weidenschilling S.J. The distribution of mass in the planetary system and solar nebula. Astrophys. Space Sci. 1977, 51:153-158.
52. Weidenschilling S.J. Dust to planetesimals - Settling and coagulation in the solar nebula. Icarus 1980, 44:172-189.
53. Wetherill G.W., Stewart G.R. Formation of planetary embryos - Effects of fragmentation, low relative velocity, and independent variation of eccentricity and inclination. Icarus 1993, 106:190-209.
54. Youdin A.N., Lithwick Y. Particle stirring in turbulent gas disks: Including orbital oscillations. Icarus 2007, 192:588-604.
55. Youdin A.N., Shu F.H. Planetesimal formation by gravitational instability. Astrophys. J. 2002, 580:494-505.