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Erosive Hit-and-Run Impact Events: Debris Unbound

Published online by Cambridge University Press:  01 March 2016

Gal Sarid ,
Sarah T. Stewart  and
Zoë M. Leinhardt
Gal Sarid
Affiliation:
Florida Space Institute, University of Central Florida, Partnership 1 Building, 12354 Research Parkway, Suite 214, Orlando, FL, USA32826-0650 email: [email protected]
Sarah T. Stewart
Affiliation:
Department of Earth and Planetary Sciences, University of California Davis, One Shields Avenue, Davis, CAUSA95618 email: [email protected]
Zoë M. Leinhardt
Affiliation:
School of Physics, University of Bristol, H.H. Wills Physics Laboratory, Tyndall Avenue, Bristol, BS8 1TL, UK email: [email protected]
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Abstract

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Erosive collisions among planetary embryos in the inner solar system can lead to multiple remnant bodies, varied in mass, composition and residual velocity. Some of the smaller, unbound debris may become available to seed the main asteroid belt. The makeup of these collisionally produced bodies is different from the canonical chondritic composition, in terms of rock/iron ratio and may contain further shock-processed material. Having some of the material in the asteroid belt owe its origin from collisions of larger planetary bodies may help in explaining some of the diversity and oddities in composition of different asteroid groups.

Keywords

asteroidsminor planetssolar system: formationmethods: numerical
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S318: Asteroids: New Observations, New Models , August 2015 , pp. 9 - 15
Copyright
Copyright © International Astronomical Union 2016 

References

Agnor, C. B., Canup, R. M., & Levison, H. F. 1999, Icarus, 142, 219Google Scholar
Asphaug, E. 2010, Chemie der Erde / Geochemistry, 70, 199CrossRefGoogle Scholar
Benz, W., Anic, A., Horner, J., & Whitby, J. A. 2007, Sp. Sci. Rev., 132, 189CrossRefGoogle Scholar
Bottke, W. F., Nesvorný, D., Grimm, R. E., Morbidelli, A. & O'Brien, D. P. 2006, Nature, 439, 821CrossRefGoogle Scholar
Burbine, T. H., McCoy, T. J., Meibom, A., Gladman, B., & Keil, K. 2002, Asteroids III, (University of Arizona Press, Tucson), p. 653Google Scholar
Canup, R. M. 2012, Science, 338, 1052CrossRefGoogle Scholar
Chambers, J. E. 2013, Icarus, 224, 43Google Scholar
Consolmagno, G. J., Golabek, G. J., Turrini, D., et al. 2015, Icarus, 254, 190Google Scholar
Cuk, M. & Stewart, S. T. 2012, Science, 338, 1047Google Scholar
Davis, D. R., Chapman, C. R., Weidenschilling, S. J., & Greenberg, R. 1985, icarus, 62, 30Google Scholar
Davis, D. R., Farinella, P., & Marzari, F. 1999, Icarus, 137, 140CrossRefGoogle Scholar
DeMeo, F. E. & Carry, B. 2013, Icarus, 226, 723Google Scholar
Genda, H. & Abe, Y. 2003, Icarus, 164, 149Google Scholar
Goldstein, J. I., Scott, E. R. D., & Chabot, N. L. 2009, Chemie der Erde / Geochemistry, 69, 293Google Scholar
Leinhardt, Z. M., Marcus, R. A., & Stewart, S. T. 2010, ApJ, 714, 1789Google Scholar
Leinhardt, Z. M. & Stewart, S. T. 2012, ApJ, 745, 79CrossRefGoogle Scholar
Lissauer, J. J. 1993, ARA&A, 31, 129Google Scholar
Marcus, R. A., Stewart, S. T., Sasselov, D., & Hernquist, L. 2009, ApJL, 700, L118Google Scholar
Margot, J.-L. 2015, arXiv:1507.06300Google Scholar
Marinova, M. M., Aharonson, O., & Asphaug, E. 2008, Nature, 453, 1216Google Scholar
Raymond, S. N., O'Brien, D. P., Morbidelli, A., & Kaib, N. A. 2009, Icarus, 203, 644Google Scholar
Sarid, G., Stewart, S. T., & Leinhardt, Z. M. 2014, LPI Cont., 45, 2723Google Scholar
Sarid, G., Stewart, S. T., & Leinhardt, Z. M. In preparationGoogle Scholar
Springel, V. 2005, MNRAS, 364, 1105CrossRefGoogle Scholar
Stewart, S. T. & Leinhardt, Z. M. 2012, ApJ, 751, 32Google Scholar
Stewart, S. T., Lock, S. J., & Mukhopadhyay, S. 2014, LPI Cont., 45, 2869Google Scholar
Tarduno, J. A., Cottrell, R. D., Nimmo, F., et al. 2012, Science, 338, 939CrossRefGoogle Scholar
Walsh, K. J., Morbidelli, A., Raymond, S. N., O'Brien, D. P., & Mandell, A. M. 2011, Nature, 475, 206CrossRefGoogle Scholar
Yang, J., Goldstein, J. I., & Scott, E. R. D. 2010, Geochim. Cosmochim. Acta., 74, 4471Google Scholar