Abstract:This work investigates the dynamical behavior of the resonant curves in the motion of the Earth-Moon system under the influence of resistive force. In this study, the resonance arises in this motion due to the rate of change of Earth’s equatorial ellipticity (EEE) (˙ γ), the Moon’s angular velocity (˙ θmo) around the Earth, and angular velocity of barycenter (˙ α0) around the Sun, including the coefficient of resistive force (b). The configuration and equations of motion are expressed in a spherical coordinate… Show more
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