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How we can prove (using geomtry and not differential equation) that the orbit of planet have to be a conic section.
The discussion centers on proving that planetary orbits are conic sections using geometric methods rather than differential equations. A reference is made to Halliday and Resnick's textbook, which provides a derivation for circular orbits of two bodies influenced by gravitational attraction. The derivation involves the center of mass and equating centripetal forces, leading to the equation GMm/(R+r)² = mw²r. Additionally, it is noted that Isaac Newton demonstrated this concept geometrically in his work "Principia."
PREREQUISITESStudents of physics, educators teaching gravitational dynamics, and anyone interested in the geometric foundations of celestial mechanics.