SUMMARY
The speed of gravity is a complex topic, with discussions indicating that changes in the gravitational field propagate at the speed of light (c), while some simulations assume instantaneous gravity for stability. Solar system simulators, like those found at orbitsimulator.com, demonstrate this by showing stable orbits under the assumption of instantaneous gravity, although this is not entirely accurate. The modified effective potential in General Relativity (GR) accounts for phenomena such as the perihelion precession of Mercury, which cannot be explained by Newtonian gravity alone. The relationship between gravitational influence and mass remains a fundamental question in physics, with current theories well-supported by experimental evidence.
PREREQUISITES
- Understanding of General Relativity (GR) principles
- Familiarity with Newtonian gravity concepts
- Knowledge of gravitational waves and their propagation
- Basic grasp of orbital mechanics and simulations
NEXT STEPS
- Research the perihelion precession of Mercury in General Relativity
- Explore the concept of gravitational waves and their speed
- Learn about the Lienard-Wiechert potentials in relation to gravity
- Investigate the differences between Newtonian and relativistic orbital mechanics
USEFUL FOR
Physicists, astronomy enthusiasts, students of gravitational theory, and anyone interested in the dynamics of gravitational fields and their implications in astrophysics.