In similar-sized planetary collisions, a significant part of the impactor
often misses the target and continues downrange. We follow the dynamical
evolution of "runners" from giant impacts to determine their ultimate fate.
Surprisingly, runners re-impact their target planets only about half of the
time, for realistic collisional and dynamical scenarios. Otherwise they remain
in orbit for tens of millions of years (the limit of our N-body calculations)
and longer, or sometimes collide with a different planet than the first one.
When the runner does return to collide again with the same arget planet, its
impact velocity is mainly constrained by the outcome of the prior collision.
Impact angle and orientation, however, are unconstrained by the prior
collision.Comment: 24 pages, 14 figures, 4 tables, accepted for publication in Ap
