Extended Data Fig. 2: Generalized three-body Laplace angles for known systems in resonant chains.
From: A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067

Included are the Galilean satellites Kepler-60 (refs. 12,115), Kepler-80 (ref. 159), K2-138 (ref. 112), Kepler-223 (ref. 110), TRAPPIST-1 (ref. 13) and TOI-178 (ref. 10). Measurements belonging to the same system are marked with the same colour. The line marks the observed distance to the theorized equilibrium (marked with a circle). The distances are estimated at the zeroth order in eccentricity110,111. For most systems, a single estimation of the generalized Laplace angle is made, whereas ref. 110 made an estimation for each Kepler quarter.