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Fig. 6

image

Digitally filtered time series from the output of a numerical experiment for 100 Myr, with initial conditions equal to those of (31) but for osculating a = 3.165 au, and a Yarkovsky model such that the secular drift should be da/dt = −2 × 10−4 au/Myr.Top panel: filtered semimajor axis (au). Bottom panel: filtered eccentricity, showing much larger oscillations after the entry into the secular resonance gg6 at about + 50 Myr.

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