The secular influence of solar mass-loss on the orbital elements of meteor streams

Details The secular influence of solar mass-loss on the orbital elements of meteor streams The secular influence of solar mass-loss on the orbital elements of meteor streams

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005pnaoc...2..194l&link_type=abstract

Astronomical Research and Technology. Publications of National Astronomical Observatories of China (ISSN 1672-7673), Vol. 2, No.

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Solar Mass-Loss, Meteor Streams Orbit, Secular Influence

Scientific paper

The secular influence of solar mass-loss on the orbital elements of meteor streams is examined by using the method of celestial mechanics of variable mass in this paper. The mass-loss includes the light radiation and solar wind. The numerical computation for the secular variable of the semi-major axis, solar distance at perihelion, orbital periods and longitude of perihelion has been made for fifteen meteor streams by using the solution of Gylden-Meshcherckii equations. The results show that the solar mass-loss extends the semi-major axis, the distance at perihelion and orbital periods of the meteor streams, especially, the extensive influence on the semi-major axis is not overlooked, but this influence on other orbital elements may be neglected.

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