Fig. 1

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Eccentricities (left side) and inclinations (right side) over the invariant plane J2000 (see Appendix D.2) of the inner planets over 250 000 yr in the future. The solid black line stands for the full (i.e. non-filtered) direct integration LaX13b, while the red line is the solution of our forced model in Eq. (16). The secular integration La90 is represented by the dashed blue line. The maximum relative root mean square of our model residuals is 2% for the eccentricities and 0.7% for theinclinations.
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