Conditions for collisional growth of a grain aggregate

Icarus

Volumn 167, Issue 2, 2004, Pages 431-452

  Sirono, Sin Iti ^a  

^a NAGOYA UNIVERSITY   (Japan)

Author keywords

Collisional physics; Planetesimals; Solar nebula

Indexed keywords

EID: 1842480932     PISSN: 00191035     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.icarus.2003.09.018     Document Type: Article

References (48)

1. Arakawa, M., Leliwa-Kopystynski, J., Maeno, N., 2002. Impact experiments on porous icy-silicate cylindrical blocks and the implication for disruption and accumulation of small icy bodies. Icarus 158, 516-531.
2. Benz, W., Asphaug, E., 1994. Impact simulations with fracture. I. Method and tests. Icarus 107, 98-116.
3. Benz, W., Asphaug, E., 1999. Catastrophic disruptions revisited. Icarus 142, 5-20.
4. Berland, B.S., Brown, D.E., Tolbert, M.A., George, S.M., 1995. Refractive index and density of vapor-deposited ice. Geophys. Res. Lett. 22, 3493-3496.
5. Blum, J., Wurm, G., 2000. Experiments on sticking, restructuring, and fragmentation of preplanetary dust aggregates. Icarus 143, 138-146.
6. Bridges, F.G., Supulver, K.D., Lin, D.N.C., Knight, R., Zafra, M., 1996. Energy loss and sticking mechanisms in particle aggregation in planetesimal formation. Icarus 123, 422-435.
7. Chambers, J.E., Wetherill, G.W., 1998. Making the terrestrial planets: N-body integrations of planetary embryos in three dimensions. Icarus 136, 304-327.
8. Chokshi, A., Tielens, A.G.G.M., Hollenbach, D., 1993. Dust coagulation. Astrophys. J. 407, 806-819.
9. Dermott, S.F., Jayaraman, S., Xu, Y.L., Gustafson, B.A.S., Lion, J.C., 1994. A circumsolar ring of asteroidal dust in resonant lock with the Earth. Nature 369, 719-723.
10. Dominik, C., Tielens, A.G.G.M., 1997. The physics of dust coagulation and the structure of dust aggregates in space. Astrophys. J. 480, 647-673.
11. Goldreich, P., Ward, W.R., 1973. The formation of planetesimals. Astrophys. J. 183, 1051-1061.
12. Grady, D.Y., Kipp, M.E., 1980. Continuum modelling of explosive fracture in oil shale. Int. J. Rock Mech. Min. 17, 147-157.
13. Greenberg, J.M., 1982. What are comets made of? A model based on interstellar dust. In: Wilkening, L.L. (Ed.), Comets. Univ. of Arizona Press, Tucson, pp. 131-163.
14. Greenberg, J.M., Mizutani, H., Yamamoto, T., 1995. A new derivation of the tensile strength of cometary nuclei: Application to Comet Shoemaker-Levy 9. Astron. Astrophys. 295, L35-L38.
15. Greenberg, J.M., 1998. Making a comet nucleus. Astron. Astrophys. 330, 375-380.
16. Habing, H.J., Dominik, C., Jourdain de Mulzon, M., Kessler, M.F., Laureijs, R.J., Leech, K., Metcalfe, L., Salama, A., Siebenmorgen, R., Trams, N., 1999. Disappearance of stellar debris disks around main-sequence stars after 400 million years. Nature 401, 456-458.
17. Hayashi, C., Nakazawa, K., Nakagawa, Y., 1985. Formation of the Solar System. In: Black, D.C., Mattews, M.S. (Eds.), Protostars and Planets, vol. 2. Univ. of Arizona Press, Tucson, pp. 1100-1153.
18. Housen, K.R., Holsapple, K.A., Voss, M.E., 1999. Compaction as the origin of the unusual craters on the Asteroid Mathilde. Nature 402, 155-157.
19. Iveson, S.M., Page, N.W., 2001. Tensile bond strength development between liquid-bond pellets during compression. Powder Technol. 117, 113-122.
20. Iveson, S.M., Beathe, J.A., Page, N.W., 2002. The dynamic strength of partially saturated powder compacts: The effect of liquid properties. Powder Technol. 127, 149-161.
21. Johnson, K.L., 1985. Contact Mechanics. Cambridge Univ. Press, Cambridge.
22. Kendall, K., Alford, N.McN., Birchall, J.D., 1987. A new method for measuring the surface energy of solids. Nature 325, 794-796.
23. h: An effective pair, central force potential model of the static interaction. J. Chem. Phys. 67, 3206-3213.
24. Kokubo, E., Ida, S., 1998. Oligarchic growth of protoplanets. Icarus 131, 171-178.
25. Kouchi, A., Kudo, T., Nakano, H., Arakawa, M., Watanabe, N., Sirono, S., Higa, M., Maeno, N., 2002. Rapid growth of asteroids owing to very sticky interstellar organic grains. Astrophys. J. 566, L121-L125.
26. Lawn, B.R., Wilshaw, T.R., 1975. Fracture of Brittle Solids. Cambridge Univ. Press, New York.
27. Mellor, M., 1975. A review of basic snow mechanics. IAHS-AISH Pub. 114, 251-291.
28. Monaghan, J.J., 1992. Smooth particle hydrodynamics. Annu. Rev. Astron. Astr. 30, 543-574.
29. Nichols, F.A., Mullins, W.W., 1965. Morphological changes of a surface of revolution due to capillarity-induced surface diffusion. J. Appl. Phys. 36, 1826-1835.
30. Petrenko, V.F., Whitworth, R.W., 1999. Physics of Ice. Oxford Univ. Press, Oxford.
31. Poppe, T., Blum, J., Henning, T., 2000. Analogous experiments on the stickiness of micron-sized preplanetary dust. Astrophys. J. 533, 454-471.
32. Poppe, T., 2003. Sintering of highly porous silica-particle samples: Analogues of early Solar-System aggregates. Icarus 164, 139-148.
33. Schweiger, A., Zimmermann, I., 1999. A new approach for the measurement of the tensile strength of powders. Powder Technol. 101, 7-15.
34. Sekanina, Z., 1993. Disintegration phenomena expected during collision of Comet Shoemaker-Levy 9 with Jupiter. Science 262, 382-387.
35. Selhammar, M., 1997. Modified artificial viscosity in smooth particle hydrodynamics. Astron. Astrophys. 325, 857-865.
36. Sirono, S., 1999. Effects by sintering on the energy dissipation efficiency in collisions of grain aggregates. Astron. Astrophys. 347, 720-723.
37. Sirono, S., Greenberg, J.M., 2000. Do cometesimal collisions lead to bound rubble piles or to aggregates held together by gravity? Icarus 145, 230-238.
38. Stern, S.A., Colwell, J.E., 1997. Accretion in the Edgewordi-Kuiper belt: Forming 100-1000 km radius bodies at 30 AU and beyond. Astron. J. 114, 841-849.
39. Supulver, K.D., Bridges, F.G., Tiscareno, S., Lievore, J., Lin, D.N.C., 1997. The sticking properties of water frost produced under various ambient conditions. Icarus 129, 539-554.
40. Valverde, J.M., Ramos, A., Castellanos, A., Watson, P.K., 1998. The tensile strength of cohesive powders and its relationship to consolidation, free volume and cohesivity. Powder Technol. 97, 237-245.
41. Veverka, J., 16 colleagues, 1997. NEAR's flyby of 253 Mathilde: Images of a C asteroid. Science 278, 2109-2112.
42. Weidenschilling, S.J., 1980. Dust to planetesimals: Settling and coagulation in the solar nebula. Icarus 44, 172-189.
43. Weidenschilling, S.J., 1984. Evolution of grains in a turbulent solar nebula. Icarus 60, 555-567.
44. Weidenschilling, S.J., Cuzzi, J.N., 1993. Formation of planetesimals in the solar nebula. In: Levy, E.H., Lunine, J.I. (Eds.), Protostars and Planets, vol. 3. Univ. Arizona Press, Tucson, pp. 1031-1060.
45. Weidenschilling, S.J., 1997. The origin of comets in the solar nebula: A unified model. Icarus 127, 290-306.
46. Wetherill, G.W., Stewart, G.R., 1989. Accumulation of a swarm of small planetesimals. Icarus 77, 330-357.
47. Wilkins, M.L., 1999. Computer Simulation of Dynamic Phenomena. Springer, Berlin, p. 149.
48. Youdin, A.M., Shu, F.H., 2002. Planetesimal formation by gravitational instability. Astrophys. J. 580, 494-505.