Accretion of dust by chondrules in a MHD-turbulent solar nebula

Icarus

Volumn 211, Issue 1, 2011, Pages 876-884

  Carballido, Augusto ^a  

^a UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

Author keywords

Disks; Meteorites; Origin, Solar System; Planetary formation

Indexed keywords

EID: 78650958053     PISSN: 00191035     EISSN: 10902643     Source Type: Journal    
DOI: 10.1016/j.icarus.2010.10.018     Document Type: Article

References (37)

1. Armitage P.J. Astrophysics of Planet Formation 2010, Cambridge Univ. Press, Cambridge, UK.
2. Balbus, S.A., 2009. Magnetohydrodynamics of protostellar disks. arXiv:. arxiv:0906.0854.
3. Balbus S.A., Hawley J.F. Instability, turbulence, and enhanced transport in accretion disks. Rev. Mod. Phys. 1998, 70:1-53.
4. Carballido A., Stone J.M., Turner N.J. Kinematics of solid particles in a turbulent protoplanetary disc. Mon. Not. R. Astron. Soc. 2008, 386:145-154.
5. Carballido A., Cuzzi J.N., Hogan R.C. Relative velocities of solids in a turbulent protoplanetary disc. Mon. Not. R. Astron. Soc. 2010, 405:2339-2344.
6. Ciesla F.J. Two-dimensional transport of solids in viscous protoplanetary disks. Icarus 2009, 200:655-671.
7. Ciesla F.J., Hood L.L., Weidenschilling S.J. Evaluating planetesimal bow shocks as sites for chondrule formation. Meteorit. Planet. Sci. 2004, 39:1809-1821.
8. Cuzzi J.N. Blowing in the wind: III. Accretion of dust rims by chondrule-sized particles in a turbulent protoplanetary nebula. Icarus 2004, 168:484-497.
9. Cuzzi J.N., Alexander C.M.O. Chondrule formation in particle-rich nebular regions at least hundreds of kilometres across. Nature 2006, 441:483-485.
10. Cuzzi J.N., Weidenschilling S.J. Particle-gas dynamics and primary accretion. Meteorites and the Early Solar System II 2006, 353-381. The University of Arizona Press, Tucson. D.S. Lauretta, H.Y. McSween (Eds.).
11. 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.
12. Desch, S.J., Morris, M.A., Connolly Jr., H.C., 2010. A critical examination of the X-wind model for the formation of chondrules and CAIs. Lunar Planet. Sci. XVI, 2200 (abstract).
13. Fleming T., Stone J.M. Local magnetohydrodynamic models of layered accretion disks. Astrophys. J. 2003, 585:908-920.
14. Fromang S., Papaloizou J. Dust settling in local simulations of turbulent protoplanetary disks. Astron. Astrophys. 2006, 452:751-762.
15. Güttler C., Blum J., Zsom A., Ormel C.W., Dullemond C.P. The outcome of protoplanetary dust growth: Pebbles, boulders, or planetesimals? I. Mapping the zoo of laboratory collision experiments. Astron. Astrophys. 2010, 513:A56.
16. Hartmann L., Calvet N., Gullbring E., D'Alessio P. Accretion and the evolution of T Tauri disks. Astrophys. J. 1998, 495:385-400.
17. Hawley J.F., Gammie C.F., Balbus S.A. Local three-dimensional magnetohydrodynamic simulations of accretion disks. Astrophys. J. 1995, 440:742-763.
18. Krot A.N., Nagashima K., Ciesla F.J., Meyer B.S., Hutcheon I.D., Davis A.M., Huss G.R., Scott E.R.D. Oxygen isotopic composition of the Sun and mean oxygen isotopic composition of the protosolar silicate dust: Evidence from refractory inclusions. Astrophys. J. 2010, 713:1159-1166.
19. Leinhardt Z.M., Stewart S.T. Full numerical simulations of catastrophic small body collisions. Icarus 2009, 199:542-559.
20. Metzler K., Bischoff A., Stöffler D. Accretionary dust mantles in CM chondrites: Evidence for solar nebula processes. Geochim. Cosmochim. Acta 1992, 56:2873-2897.
21. Morfill G.E., Durisen R.H., Turner G.W. An accretion rim constraint on chondrule formation theories. Icarus 1998, 134:180-184.
22. Ormel C.W., Cuzzi J.N. Closed-form expressions for particle relative velocities induced by turbulence. Astron. Astrophys. 2007, 466:413-420.
23. 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.
24. Paque, J., Cuzzi, J.N., 1997. Physical characteristics of chondrules and rims, and aerodynamic sorting in the solar nebula. Lunar Planet. Sci. XXVIII, 1189 (abstract).
25. Rubin A.E., Keil K. Size-distributions of chondrule types in the Inman and Allan Hills A77011 L3 chondrites. Meteoritics 1984, 19:135-143.
26. Shakura N.I., Sunyaev R.A. Black holes in binary systems: Observational appearance. Astron. Astrophys. 1973, 24:337-355.
27. Shu F.H., Najita J.R., Shang H., Li Z.-Y. X-winds: Theory and observations. Protostars and Planets IV 2000, 789-813. The University of Arizona Press, Tucson. V. Mannings, A.P. Boss, S.S. Russell (Eds.).
28. Stone J.M., Gardiner T.A. Implementation of the shearing box approximation in ATHENA. Astrophys. J. Suppl. 2010, 189:142-155.
29. Stone J.M., Norman M.L. ZEUS-2D: A radiation magnetohydrodynamics code for astrophysical flows in two space dimensions. I. The hydrodynamic algorithms and tests. Astrophys. J. Suppl. 1992, 80:753-790.
30. Stone J.M., Norman M.L. ZEUS-2D: A radiation magnetohydrodynamics code for astrophysical flows in two space dimensions. II. The magnetohydrodynamic algorithms and tests. Astrophys. J. Suppl. 1992, 80:791-818.
31. Trigo-Rodri{dotless}́guez J.M., Rubin A.E., Wasson J.T. Non-nebular origin of dark mantles around chondrules and inclusions in CM chondrites. Geochim. Cosmochim. Acta 2006, 70:1271-1290.
32. Turner N.J., Sano T., Dziourkevitch N. Turbulent mixing and the dead zone in protostellar disks. Astrophys. J. 2007, 659:729-737.
33. Turner N.J., Carballido A., Sano T. Dust transport in protostellar disks through turbulence and settling. Astrophys. J. 2010, 708:188-201.
34. Wehrstedt, M., Gail, H.-P., 2008. Radial mixing in protoplanetary accretion disks. VII. 2-Dimensional transport of tracers. arXiv:. arxiv:0804.3377.
35. Weidenschilling S.J. Aerodynamics of solid bodies in the solar nebula. Mon. Not. R. Astron. Soc. 1977, 180:57-70.
36. Zsom A., Dullemond C.P. A representative particle approach to coagulation and fragmentation of dust aggregates and fluid droplets. Astron. Astrophys. 2008, 489:931-941.
37. Zsom A., Ormel C.W., Güttler C., Blum J., Dullemond C.P. The outcome of protoplanetary dust growth: Pebbles, boulders, or planetesimals? II. Introducing the bouncing barrier. Astron. Astrophys. 2010, 513:A57.