• We perform simulations of the solar system with various initial conditions of the giant planets and the terrestrial planets (see next section) for 265 Myr with a time step of 0.01 yr (3.6525 days). The **data** is output every 1000 yr. We use the 2nd order MVS integrator of Laskar & Robutel (2001), implemented (Brož et al., 2005) in the SWIFT integration package (Levison & Duncan, 1994). The code includes digital filtering of the orbital elements using Kaiser windows (Kaiser, 1966), based on the method of Quinn et al. (1991). Any signal with a period shorter than 667 yr is suppressed. To mimic the effect of general relativity we added a correction term as described in Nobili & Will (1986).