Same as the right column of Figure 4, but for a disk lifetime of 5 × 10³ yr (left column) and 5 × 10⁴ yr (right column). The top row shows the evolution of the orbital distance of the satellites and the bottom row shows the evolution of their eccentricities. For the left column, the final semimajor axis of the planet is 0.125 AU and for the right column, it is 0.035 AU. This difference can be visualized thanks to the gray dashed lines corresponding to one-half of the Hill radius of the planet, which comes much closer to the planet when the τ_disk = 5 × 10⁴ yr.