Jeremie Vaubaillon, IMCCE, 77 Av. Denfert Rochereau, Paris F-75014, France
The study of the dynamics of 2008TC3 is the first step in understanding its origin. I will show how we examined the present, past and future motion of 2008TC3-like clones as well as other F-type asteroids. The closest object in terms of dynamical behavior is found to be 1998KU2.