Motion of a Meteoroid Released from an Asteroid

Statistics – Applications

Scientific paper

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Asteroid, Meteoroid Release, Tidal Force, Itokawa, Interplanetary Dust Particles

Scientific paper

Evidence of asteroid surface features as regolith grains and larger boulders implies resurfacing possibility due to external forces such as gravitational tidal force during close planet encounters. Motion of a meteoroid released from an asteroid in the gravitational fields of the asteroid and the Earth is modeled. We are interested mainly in a distance between the meteoroid and the asteroid as a function of the time. Applications to Itokawa and some close approaching NEAs are presented.

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