Development of Simulation Tool for Orbital Motion of Meteoroid Stream Particles

Details Development of Simulation Tool for Orbital Motion of Meteoroid Stream Particles Development of Simulation Tool for Orbital Motion of Meteoroid Stream Particles

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000jass...17..107k&link_type=abstract

Journal of Astronomy and Space Sciences, vol. 17, no. 1, p. 107-116.

Astronomy and Astrophysics

Astronomy

Scientific paper

This paper presents the preliminary survey and simulation results of the prediction of Leonid stream's orbital motion. Based on the model survey on eject velocity and perturbation of meteoroid particles, a simulation program was developed and applied to orbital motion of Leonid stream. The Jones ejection distribution model was used to describe the particle's eject velocity and the orbital dynamics model includes perturbations of major planet's gravity. DE405 ephemeris file generated by Solar System Dynamics Group at Jet Propulsion Laboratory in NASA was used for the planet's ephemeris calculations. Solar radiation pressure were also considered in the simulation and 8th order Runge-Kutta algorithm was used as a numerical integration method.

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