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Originally Posted by Nereid
1) You say you are 'using the Newton theory' (presumably the one based on F = Gm1m2/r2). What other theory (or theories) are you using?
2) You say "if a planet does not revolve in the plane of the sun's own rotation and circle the sun counterclockwise, it will not be stable and its course will be deflected". What is the time period in which such an initially clockwise planet would be either expelled from the solar system, collide with the Sun or another planet, or change its orbit to a 'normal' one?
I appreciate that the answer to this question will depend on several factors, perhaps the initial clockwise orbit's radius, ellipticity, and inclination. Please answer the question with reference to the key factors.
3) The equations of motion of bodies under mutual (Newtonian) gravitational attraction are relatively easy to simulate, for a system like our solar system. Indeed, it may be that you can download some such, for free. Have you modeled your idea with such a simulation?
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1) The force that runs the moons and planets is the Gravity Force which was discovered by Newton. In my article, I find no more other Newton's theory is needed.
2)The time period for a initially clockwise palnet to change its orbit to a normal one should meet a function, I believe,though I can not offer it right now. The time should be an infinite parameter in the sense of math, for zero is the infinitesimal limit value for the Coriolis Force to reach while reducing the intersect angle between the orbits of such planets/moons and the sun.In the sense of math, this infinitesimal limit (zero) can never be reached.
The bigger the intersect angle is, the more significant the change will be. A vertically circling moon will make the most significant tilting. The tilting speed should be proportional to the differential coefficient of a function as Sin(the angle) or similar. It's not a constant.
3)I am sorry to say that I haven't. Could you please show me how to get it?