pith. sign in

arxiv: gr-qc/0403067 · v2 · submitted 2004-03-15 · 🌀 gr-qc

Deformation of the Planetary Orbits Caused by the Time Dependent Gravitational Potential in the Universe

classification 🌀 gr-qc
keywords dependentpotentialtimecausedgravitationalorbitsplanetaryuniverse
0
0 comments X
read the original abstract

In the paper are studied the deformations of the planetary orbits caused by the time dependent gravitational potential in the universe. It is shown that the orbits are not axially symmetric and the time dependent potential does not cause perihelion precession. It is found a simple formula for the change of the orbit period caused by the time dependent gravitational potential and it is tested for two binary pulsars.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.