Predicting Mercury's Precession using Simple Relativistic Newtonian Dynamics

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.

5 pages

References in corpus (1)

• A new relativistic kinematics of accelerated systems

Cited by in corpus (7)

• Bounds on graviton mass using weak lensing and SZ effect in galaxy clusters
• Gravitational Deflection in Relativistic Newtonian Dynamics
• Predicting the relativistic periastron advance of a binary without curving spacetime
• A unifying physically meaningful relativistic action
• Relativistic Newtonian Dynamics
• Relativistic Newtonian Dynamics for Objects and Particles
• Relativity from the Geometrization of Newtonian Dynamics