Development of Simulation Tool for Orbital Motion of Meteoroid Stream Particles

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 Jone...

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Main Author: Bang-Yeop Kim
Format: Article
Language:English
Published: The Korean Space Science Society 2000-06-01
Series:Journal of Astronomy and Space Sciences
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2000/v17n1/OJOOBS_2000_v17n1_107.pdf
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author Bang-Yeop Kim
author_facet Bang-Yeop Kim
author_sort Bang-Yeop Kim
collection DOAJ
description 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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spelling doaj.art-b6eaaaddba354ae0af3b82e7daca09f02024-02-02T17:12:14ZengThe Korean Space Science SocietyJournal of Astronomy and Space Sciences2093-55872093-14092000-06-01171107116Development of Simulation Tool for Orbital Motion of Meteoroid Stream ParticlesBang-Yeop Kim0Koreasat Department, Korea Aerospace Research Institute, Daejeon, 305-606, KoreaThis 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.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2000/v17n1/OJOOBS_2000_v17n1_107.pdf
spellingShingle Bang-Yeop Kim
Development of Simulation Tool for Orbital Motion of Meteoroid Stream Particles
Journal of Astronomy and Space Sciences
title Development of Simulation Tool for Orbital Motion of Meteoroid Stream Particles
title_full Development of Simulation Tool for Orbital Motion of Meteoroid Stream Particles
title_fullStr Development of Simulation Tool for Orbital Motion of Meteoroid Stream Particles
title_full_unstemmed Development of Simulation Tool for Orbital Motion of Meteoroid Stream Particles
title_short Development of Simulation Tool for Orbital Motion of Meteoroid Stream Particles
title_sort development of simulation tool for orbital motion of meteoroid stream particles
url http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2000/v17n1/OJOOBS_2000_v17n1_107.pdf
work_keys_str_mv AT bangyeopkim developmentofsimulationtoolfororbitalmotionofmeteoroidstreamparticles