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Fig. 6

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Plot of ⟨ Δr ⟩ / ⟨ r ⟩ versus for different local perturbations of the asteroid Apollo. Only one facet group of the asteroid is perturbed at a time, and only this section defines ⟨ Δr ⟩ / ⟨ r ⟩. With local perturbations less than 10%, the relative change in mostly remains below 10%. Therefore, we can conclude that the asteroid Apollo is locally YORP-stable.

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