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Fig. 3

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Expected gravitational force due to system gravity and external perturbers, as a function of satellite distance for Pulcova (upper panel) and Emma (lower panel). The shaded regions around planetary forces indicate the range of the force between the objects closest and farthest approach to the asteroid. At the positions of both Pulcamoon and Emmoon (marked with a dashed line), the contribution of external perturbers is negligible.

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