Icarus's Orbit as the Ultimate Test for the Vulcan Hypothesis and General Relativity
Souren Petik Pogossian

TL;DR
This paper compares methods for calculating perihelion precession, finds that Icarus's orbit challenges classical and relativistic models, and explores a hypothetical Vulcan planet's influence on planetary orbits to test gravitational theories.
Contribution
It introduces a novel comparison of perihelion calculation methods and assesses Vulcan's potential effects, providing a new approach to testing gravitational theories using Icarus's orbit.
Findings
Laplace-Runge-Lenz vector method aligns with observations for Icarus.
Vulcan's hypothetical parameters can mimic relativistic perihelion effects.
Precise Icarus data can confirm or refute Vulcan hypothesis.
Abstract
General Relativity (GR) quantitatively accounts for the anomalous perihelion precession observed in several planets' orbits, with Mercury exhibiting the most significant deviation from Newtonian predictions. In the present work, I carry out an in-depth study comparing methods for calculating perihelion advance of inner planets using two methods, one based on the rotation of the Laplace-Runge-Lentz vector and the other on the evolution of the perihelion longitude. I show that, although the two methods predict almost identical perihelion advances for inner planets according to classical gravitational theory and the general relativity model, they give divergent results for the asteroid Icarus. Comparing numerical calculations of Icarus'perihelion advance with those predicted by Einstein's formula leads to the conclusion that only the method based on the Laplace-Runge-Lenz vector offers a…
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Taxonomy
TopicsAstro and Planetary Science · Relativity and Gravitational Theory · Planetary Science and Exploration
