Extended Data Fig. 3: Observed distance from the equilibrium for all the simulated scenarios in which planets f and g continue the resonant chain. | Nature

Extended Data Fig. 3: Observed distance from the equilibrium for all the simulated scenarios in which planets f and g continue the resonant chain.

From: A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067

Extended Data Fig. 3: Observed distance from the equilibrium for all the simulated scenarios in which planets f and g continue the resonant chain.

The y axis is converted to the mean peak-to-peak amplitude from the generalized three-body Laplace angle using the following expression: mean \(({\mathcal{A}}({\varPsi }_{i}))=C/4\). Case A2 remains the one that has the potential to be the closest to an equilibrium.

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