Fig. 4
Orbital evolution of one clone still locked in the 5:2 resonance at the end of 200 000 years backward numerical integration: Δ ϖ = ϖJ − ϖast, difference in the longitudes of perihelion of Jupiter and clone (first panel), critical argument σ5:2J = 5λJ − 2λast − 3ϖast (second panel), semimajor axis and eccentricity (third and fourth panels).
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