Determination of the Preliminary Orbit in the Coplanar Case
摘要
Abstract—
An algorithm for finding a solution to determine a preliminary orbit with a very small inclination to the ecliptic plane is proposed. The method proposed by the author is based on solving a system of transcendental equations for three variables. Solutions to the system are found by searching for the minima of the objective function using the Nelder–Mead method for a simplex. As an example, the results of determining the orbit of asteroid 255 447 (2005 YN24) are given.