Overview of the results for the sample of simulations for asteroids disturbed by Jupiter. In this plot, we consider only the data concerning the asteroids with short Lyapunov time (of just a few hundred years). This figure is divided by the light blue line into two parts, in the vertical axis: (1) positive values indicate the final orbital radius of the asteroid (pink), in units of Jupiter’s orbital radius, and (2) negative values indicate the logarithm of Lyapunov characteristic exponent of the asteroid, where (i) the complete LCE, given by γ, is in red; (ii) the contribution of the radial component, given by γ_rad, is in green; and (iii) the LCE without the radial contribution, given by γ_∗, is in blue. The horizontal axis indicates the initial semi-major axis of the asteroid.