Abstract
We statistically investigate the final stage of terrestrial planet formation from protoplanets by using N-body simulations. As the initial conditions, we adopt the oligarchic growth model of protoplanets. We systematically change the total mass, the mass distribution, and the orbital separation of the initial protoplanet system. For a parameter set of the initial condition, we perform 20 runs. We show the dependence of the mass and orbital properties of the planets on the parameters of the initial protoplanet system.
