long-term stability of solar system planetary motion. for readers who have more specific and deeper interests in our numerical results， we have prepared a webpage (access )， where we show raw orbital elements， their low-pass filtered results， variation of delaunay elements and angular momentum deficit， and results of our simple time–frequency analysis on all of our integrations.
in section 2 we briefly explain our dynamical model， numerical method and initial conditions used in our integrations. section 3 is devoted to a description of the quick results of the numerical integrations. very long-term stability of solar system planetary motion is a
对火星轨道变化问题的最后解释(12/49)