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Fig. 3

image

Orbital evolution of Kepler-47 B and Kepler-47 b. In each plot, we compare the simulated values to their present day observed values. We can also see how the critical semi-major axis affects and raises the amplitude of the CBP’s semi-major axis and eccentricity as the planet approaches the dynamic stability limit. The approximate runtime was 90 min. github.com: cbp_dynamic_stability/kepler47b/

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