これの和訳を教えてください。
In order to understand precisely the formation process of planets it is important to study extensively the two-body encounters between planetesimals taking fully into account the influence of the solar gravity. Some authors have tried to simulate numerically the growth process of N-planetesimals to the present planets, taking into account the influence of the Sun. But before executing the simulation of the N-bodies’ encountering process numerically, it is necessary to know more detailes of the fundamental features of the two-body encounters between Keplerian particles. Furthermore, according to Hayashi, the ratio of the collisional rate to the scattering rate as well as the collisional rate itself is one of the important parameters which determine essentially the time scale of the planetary growth.
