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Predicting Mercury's Precession using Simple Relativistic Newtonian Dynamics (1603.02560v1)
Published 29 Feb 2016 in physics.gen-ph and gr-qc
Abstract: We present a new simple relativistic model for planetary motion describing accurately the anomalous precession of the perihelion of Mercury and its origin. The model is based on transforming Newton's classical equation for planetary motion from absolute to real spacetime influenced by the gravitational potential and introducing the concept of influenced direction.
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