
TL;DR
This study investigates whether the speed of light has varied over the last century by analyzing planetary perihelion precessions, finding no significant variation and setting constraints on c/cb.
Contribution
It provides the first constraints on the temporal variation of the speed of light using planetary orbital data and perihelion precession measurements.
Findings
c/cb = (0.5 b 7 2) d7 10^{-7} yr^{-1}
Variation of c/cb over the last century is statistically insignificant
Ratios of perihelia for different planet pairs strongly constrain c/cb variations
Abstract
Analytical and numerical calculations show that a putative temporal variation of the speed of light c, with the meaning of space-time structure constant c_ST, assumed to be linear over timescales of about one century, would induce a secular precession of the longitude of the pericenter \varpi of a test particle orbiting a spherically symmetric body. By comparing such a predicted effect to the corrections \Delta\dot\varpi to the usual Newtonian/Einsteinian perihelion precessions of the inner planets of the Solar System, recently estimated by E.V. Pitjeva by fitting about one century of modern astronomical observations with the standard dynamical force models of the EPM epehemerides, we obtained \dot c/c =(0.5 +/- 2)\times 10^-7 yr^-1. Moreover, the possibility that \dot c/c\neq 0 over the last century is ruled out at 3-12\sigma level by taking the ratios of the perihelia for different…
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