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Science 8 May 1998:
Vol. 280. no. 5365, pp. 874 - 876
DOI: 10.1126/science.280.5365.874

Reports

A 100,000-Year Periodicity in the Accretion Rate of Interplanetary Dust

Stephen J. Kortenkamp, * Stanley F. Dermott

Numerical modeling of the orbital evolution of interplanetary dust particles revealed that, over the past 1.2 million years, the rate of accretion of dust by Earth has varied by a factor of 2 to 3. These variations display a 100,000-year periodicity and are anticorrelated with Earth's changing orbital eccentricity. Extraterrestrial helium-3 concentrations in a deep-sea sediment core display a similar periodicity but are 50,000 years out of phase with the predicted variations. Also, because collisions between large bodies in the asteroid belt are inevitable, it is expected that large-amplitude stochastic variations on 107- to 108-year time scales would be superimposed on the 105-year periodic variations.

S. J. Kortenkamp, Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road NW, Washington, DC 20015, USA. E-mail: kortenka{at}dtm.ciw.edu
S. F. Dermott, Department of Astronomy, University of Florida, 211 Space Sciences Building, Gainesville, FL 32611-2055, USA. E-mail: dermott{at}astro.ufl.edu
*   To whom correspondence should be addressed.


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