Three-body-interaction effects on the relativistic perihelion precession for the Sun-Jupiter-Saturn system
Kei Yamada, Hideki Asada

TL;DR
This paper derives the relativistic perihelion precession caused by three-body interactions in hierarchical systems like Sun-Jupiter-Saturn, quantifying effects that are larger than the Lense-Thirring effect but insufficient to explain observed anomalies.
Contribution
The study provides a new analytical expression for relativistic three-body perihelion precession in hierarchical systems, expanding understanding of post-Newtonian effects on planetary orbits.
Findings
Relativistic precession for Sun-Jupiter-Saturn is 7.8e-6 arcsec/cy.
Precession effect exceeds Lense-Thirring effect by Sun.
Cannot fully account for observed Saturn perihelion anomaly.
Abstract
The relativistic perihelion precession due to the three-body interaction is derived. We consider a hierarchical coplanar three-body system, such as the Sun, Jupiter and Saturn, in which both the secondary object as the largest planet corresponding to Jupiter (mass ) and the third one corresponding to Saturn (mass ) orbit around the primary object corresponding to Sun (mass ), where the mean orbital radius of the third body is larger than that of the secondary one (denoted as ). We investigate the post-Newtonian effects on the motion of the third body (semimajor axis a, eccentricity e for the Keplerian orbital elements). Under some assumptions with a certain averaging, the relativistic perihelion precession of the third mass by the post-Newtonian three-body interaction is expressed as , where G…
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Taxonomy
TopicsAstro and Planetary Science · Stellar, planetary, and galactic studies · Solar and Space Plasma Dynamics
