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Collision probabilities of migrating small bodies and dust particles with planets

Published online by Cambridge University Press:  06 April 2010

Sergei I. Ipatov
Sergei I. Ipatov*
Affiliation:
Catholic University of America, Washington DC, USA email: siipatov@hotmail.com Space Research Institute, Moscow, Russia
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Abstract

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Probabilities of collisions of migrating small bodies and dust particles produced by these bodies with planets were studied. Various Jupiter-family comets, Halley-type comets, long-period comets, trans-Neptunian objects, and asteroids were considered. The total probability of collisions of any considered body or particle with all planets did not exceed 0.2. The amount of water delivered from outside of Jupiter's orbit to the Earth during the formation of the giant planets could exceed the amount of water in Earth's oceans. The ratio of the mass of water delivered to a planet by Jupiter-family comets or Halley-type comets to the mass of the planet can be greater for Mars, Venus, and Mercury, than that for Earth.

Keywords

Minor planetsasteroidscomets: generalsolar system: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S263: Icy Bodies of the Solar System , August 2009 , pp. 41 - 44
Copyright
Copyright © International Astronomical Union 2010

References

Drake, M. & Campins, H. 2006, in: Lazzaro, D., Ferraz-Mello, S. & Fernandez, J. A. (eds), Asteroids, Comets, & Meteors, IAU Symp. 229 (Cambridge: Cambridge Univ. Press), p. 381Google Scholar
Genda, H. & Icoma, M. 2008, Icarus, 194, 42Google Scholar
Ipatov, S. I. 1987, Earth, Moon, & Planets, 39, 101Google Scholar
Ipatov, S. I. 1988, Sov. Astron., 65, 1075Google Scholar
Ipatov, S. I. 1993, Solar System Res., 27, 65Google Scholar
Ipatov, S. I. 2001, Adv. Space Res., 28, 1107Google Scholar
Ipatov, S. I. & Mather, J. C. 2003, Earth, Moon, & Planets, 92, 89Google Scholar
Ipatov, S. I. & Mather, J. C. 2004a, Ann. New York Acad. Sci., 1017, 46Google Scholar
Ipatov, S. I. & Mather, J. C. 2004b, Adv. Space Res., 33, 1524Google Scholar
Ipatov, S. I. & Mather, J. C. 2006, Adv. Space Res., 37, 126Google Scholar
Ipatov, S. I. & Mather, J. C. 2007, in: IAUS 236 Near-Earth Objects, Our Celestial Neighbors: Opportunity and Risk, p. 55Google Scholar
Ipatov, S. I., Mather, J. C., & Taylor, P. A. 2004, Ann. New York Acad. Sci., 1017, 66Google Scholar
Levison, H. F. & Duncan, M. J. 1994, Icarus, 108, 18CrossRefGoogle Scholar
Levison, H. F., et al. 2001, Icarus, 151, 286Google Scholar
Lunine, J. I., Chambers, J., Morbidelli, A., & Leshin, L. A. 2003, Icarus, 165, 1CrossRefGoogle Scholar
Marov, M. Ya. & Ipatov, S. I. 2006, Solar Syst. Res., 39, 374Google Scholar
Morbidelli, A., Chambers, J., Lunine, J. I., Petit, J. M., Robert, F., Valsecchi, G. B., & Cyr, K. E. 2000, Meteoritics & Planet. Sci., 35, 1309CrossRefGoogle Scholar
Petit, J.-M., Morbidelli, A., & Chambers, J. 2001, Icarus, 153, 338CrossRefGoogle Scholar