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The orbital evolution of meteor streams at the 2/1 resonance with Jupiter
Published online by Cambridge University Press: 12 April 2016
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We investigated the orbital evolution of Quadrantid-like meteor streams situated in the vicinity of the 2/1 resonance with Jupiter. For the starting orbital elements we took the values of the orbital elements of the Quadrantid meteor stream except for the semi-major axis which was varied between a = 3.22 and a = 3.34 AU. We considered these meteor streams as a ring and we investigated the resonant effect on the dispersion of this ring over a period of 13 000 years. Only gravitational forces due to the Sun and due to Jupiter were taken into account.
- Type
- Section III. Meteor Streams and Interrelations with Minor Planets
- Information
- International Astronomical Union Colloquium , Volume 83: Dynamics of Comets: Their Origin and Evolution , 1985 , pp. 179 - 180
- Copyright
- Copyright © Cambridge University Press 1985
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