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Solar Sail Equilibrium Orbits in the Circular Restricted Three Body Problem with Oblateness

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Figure

Figure 1. Schematic geometry of the circular re-stricted three-body problem.
Figure 2. A flat solar sail model.
Figure 3. Positions of L1, L2, L3 vary with the variations of A and β.
Figure 5. (a) Position modification derived from the solar sail about the L1 point; (b) Velocity change as time increases in case A
+3

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