Yu Yi
Abstract
Based on the Schwarzs Child Gauge, the moving orbital equation of the planets round the sun is derived, from directly finding the solution of the three geodefic equations relevant to r, φ and t. The whole derivative process differs obviously from those of Landau's and Weber's.
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Based on the Schwarzs Child Gauge, the moving orbital equation of the planets round the sun is derived, from directly finding the solution of the three geodefic equations relevant to r, φ and t. The whole derivative process differs obviously from those of Landau's and Weber's.
Key concepts: Planet, Physics, General relativity, Theory of relativity, Mathematical physics, Classical mechanics, Astrophysics