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Fig. B.2
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Four angles (σ1,σ2,ς1,ς2) of the 5:1 MMR for the annex simulation presented in Fig. B.1. At time t = 650 years, the significant increase in the inclination of the outer submoon corresponds to the moment when the angle ς2, conjugated to the inclination of the outer submoon, starts to librate.
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