Evolution of the semimajor axis (top) and disk surface density (bottom) in simulations run-fid for a super-Earth planet of 3 M_⊕ (left), a Saturn-mass planet (middle), and a Jupiter-mass planet (right). In the upper panels the gray circles mark the planet’s position used in Fig. 5, and the cyan area in the top-right panel shows the radial extent between the planet’s pericenter and apocenter. The video can be downloaded from: https://github.com/bbliu-astro/movies/blob/main/hydrodynamic_rebound/superEarth.gif and online.