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Averaged changes in the orbital elements of meteoroids due to Yarkovsky-Radzievskij force

Published online by Cambridge University Press:  05 January 2015

Galina O. Ryabova*
Affiliation:
Tomsk State University, 634050 Tomsk, Russian Federation email: ryabova@niipmm.tsu.ru
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Abstract

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Yarkovsky-Radzievskij effect exceeds the Poynting-Robertson effect in the perturbing action on particles larger than 100 μm. We obtained formulae for averaged changes in a meteoroid's Keplerian orbital elements and used them to estimate dispersion in the Geminid meteoroid stream. It was found that dispersion in semi-major axis of the model shower increased nearly three times on condition that meteoroids rotation is fast, and the rotation axis is stable.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2014 

References

Burns, J. A. 1979, Am. J. Phys., 44, 944Google Scholar
Burns, J. A., Lamy, P. L., & Soter, S. 1979, Icarus, 40, 1Google Scholar
Fox, K., Williams, I. P. & Hughes, D. W. 1983, MNRAS, 205, 1155Google Scholar
Olsson-Steel, D. 1987, MNRAS, 226, 1Google Scholar
Ryabova, G. O. 1990, Sol. Syst. Res., 24, 169Google Scholar
Ryabova, G. O. 2007, MNRAS, 375, 1371Google Scholar