A dynamical equivalent to the equilatera
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Carles Dรญez; รngel Jorba; Carles Simรณ
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Article
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1991
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Springer Netherlands
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English
โ 707 KB
Consider the Earth-Moon-particle system as a Restricted Three Body Problem. There are two equilateral libration points. In the actual world system, those points are no longer relative equilibrium points mainly due to the effect of the Sun and to the noncircular motion of the Moon around the Earth. I