N-body simulation showing the consequence of the ejection of a 11 M_J planet through a disk. From left to right, the snapshots have been taken 0, 1000 and 10 000 years after the ejection. The planet starts on an hyperbolic orbit similar to what we observe in the simulations we performed: a = 10 au and e = 1.1 (corresponding to periastron q = 1 au). Above is a spatial representation of the top view of the disk (the planet trajectory is depicted in black), below is the density along the y axis, integrated over the x and z axis.