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Evolution of Meteoroid Orbits Over Millenia

Published online by Cambridge University Press:  14 August 2015

I. V. Galibina  and
A. K. Terentjeva
I. V. Galibina
Affiliation:
Leningrad College for Finance and Economics
A. K. Terentjeva
Affiliation:
Astronomical Council, USSR Academy of Sciences

Extract

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The evolution of meteorid orbits over long time periods has been studied using the Gauss-Halphen-Gorjatschew method taking into account perturbations from the outer four planets (Galibina 1970). As initial elements, 15 different meteor orbits were taken from photographic observations (McCrosky 1968). Calculations were carried out from the modern epoch back in time for intervals of 10000 to 100000 years. Initial elements and the time intervals are given in Table 1.

Type
II: Meteors and Meteorites
Information
Symposium - International Astronomical Union , Volume 90: Solid Particles in the Solar System , 1980 , pp. 145 - 148
Copyright
Copyright © Reidel 1980 

References

Galibina, I.V.: 1970, Bull. Inst. Theor. Astron., Leningrad, 12, p. 261.Google Scholar
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McCrosky, R.E.: 1968, in Kresák, LK. and Millman, P.M. (eds.), “Physics and Dynamics of Meteors”, IAU Symp. 33, p. 265.Google Scholar
Terentjeva, A.K.: 1966, Rezultaty Issled. MGP - Issled. Meteorov, Moskva, No. 1, 62.Google Scholar
Terentjeva, A.K.: 1968, in Kresák, LK. and Millman, P.M. (eds.), “Physics and Dynamics of Meteors”, IAU Symp. 33, p. 408.Google Scholar