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Collisional Simulations of Cometary Nuclei

Published online by Cambridge University Press:  30 March 2016

Sin-iti Sirono
Sin-iti Sirono*
Affiliation:
Earth and Environmental Sciences, Nagoya University, Building E, Nagoya 464-8602, Japan

Abstract

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Collisional simulations of cometary nuclei (icy dust aggregates) are conducted. Conditions for sticking are determined as a function of the impact velocity and mechanical properties of nuclei. Possible collisional outcomes in three evolutionary stages of icy-dust aggregates are discussed.

Type
I. Joint Discussions
Information
Highlights of Astronomy , Volume 13 , 2005 , pp. 528 - 530
Copyright
Copyright © Astronomical Society of Pacific 2005

References

Benz, W., & Asphaug, E. 1994, Icarus, 107, 98 CrossRefGoogle Scholar
Greenberg, J. M. 1982, in Comets, ed. Wilkening, L. L., 131 Google Scholar
Stern, S. A., & Colwell, J. E. 1997, AJ, 114, 841 CrossRefGoogle Scholar
Stern, S. A., & Weissman, P. R. 2001, Nature, 409, 589 CrossRefGoogle Scholar
Sirono, S. 2004, Icarus, 167, 431 CrossRefGoogle Scholar
Sirono, S. & Greenberg, J. M. 2000, Icarus, 145, 230 CrossRefGoogle Scholar