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Science 8 March 1996:
Vol. 271. no. 5254, pp. 1387 - 1392
DOI: 10.1126/science.271.5254.1387
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Research Articles

The Exchange of Impact Ejecta Between Terrestrial Planets

Brett J. Gladman, Joseph A. Burns, Martin Duncan, Pascal Lee, Harold F. Levison

Orbital histories of ejecta from the terrestrial planets were numerically integrated to study their transfer to Earth. The properties of the lunar and martian meteorites are consistent with a recurrent ejection of small meteoroids as a result of impacts on their parent bodies. Long-range gravitational effects, especially secular resonances, strongly influence the orbits of many meteoroids, increasing their collision rates with other planets and the sun. These effects and collisional destruction in the asteroid belt result in shortened time scales and higher fluxes than previously believed, especially for martian meteorites. A small flux of mercurian ejecta appears possible; recovery of meteorites from the Earth and Venus is less likely.

B. J. Gladman and P. Lee are in the Department of Astronomy, Cornell University, Ithaca, NY 14853, USA. J. A. Burns is in the Departments of Astronomy and Theoretical and Applied Mechanics, Cornell University, Ithaca, NY 14853, USA. M. Duncan is in the Department of Physics, Queen's University, Kingston, ON K7L 3N6, Canada. H. F. Levison is with Geophysical, Astrophysical, and Planetary Sciences, Southwest Research Institute, 1050 Walnut Street, Suite 429, Boulder, CO 80302, USA.


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