Abstract
From the historical perspective, the derivation of three Kepler’s laws in Classical Mechanics is one of the most relevant calculations which were ever done. We shall present this calculation in details and also give a simple treatment of the effect of Precession of Perihelion for a nearly circular orbit for a weakly non-Newtonian gravitational force. This problem has very special importance in General Relativity due to the Precession of Perihelion for the Mercury and some other relativistic tests.
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- 1.
Let us remember that a central force field is characterized by the spherical symmetry about the origin (force acts in the radial direction and its modulus is independent of angular coordinates). The gravitational field generated by a spherically symmetric distribution is a central field.
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Shapiro, I.L., de Berredo-Peixoto, G. (2013). Central Forces and Kepler’s Laws. In: Lecture Notes on Newtonian Mechanics. Undergraduate Lecture Notes in Physics. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-7825-6_9
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