SUMMARY
Einstein's General Relativity successfully explains the precession of Mercury's orbit around the Sun, which deviates from Newtonian predictions. The observed precession is 5600.7 arc seconds per century, while Newtonian gravity predicts only 5557.6 arc seconds per century, leaving a discrepancy of 43 arc seconds that General Relativity accounts for. The elliptical nature of Mercury's orbit, combined with its proximity to the Sun, intensifies the effects of gravitational perturbations from other planets, particularly Jupiter. This phenomenon is known as the advance of the perihelion of Mercury.
PREREQUISITES
- Understanding of General Relativity principles
- Familiarity with Newtonian gravity and Kepler's laws of planetary motion
- Basic knowledge of orbital mechanics and celestial bodies
- Ability to interpret astronomical measurements like arc seconds
NEXT STEPS
- Study the mathematical foundations of General Relativity
- Explore the concept of gravitational perturbations in multi-body systems
- Learn about the two-body problem in celestial mechanics
- Investigate the implications of precession in other celestial bodies
USEFUL FOR
Astronomers, physicists, students of astrophysics, and anyone interested in the dynamics of planetary motion and gravitational theory.