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Some Features of Evolution of Meteor Streams

Published online by Cambridge University Press:  30 March 2016

P.B. Babadzhanov  and
Yu.V. Obrubov
P.B. Babadzhanov
Affiliation:
Astrophysical Institute, Dushanbe, 734670, USSR
Yu.V. Obrubov
Affiliation:
Astrophysical Institute, Dushanbe, 734670, USSR

Abstract

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It is shown that a number of features of meteor showers such as the correlation of orbital semimajor axes and longitudes of the ascending nodes with meteor magnitudes, the restriction of visibility periods and the displacement of maximum activity dates is explained by the joint influence of planetary perturbations, the Poynting-Robertson effect and its corpuscular analogue, light pressure and ejection velocities of different mass meteoroids from cometary nuclei.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 6 , 1983 , pp. 411 - 419
Copyright
Copyright © Reidel 1983

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