SUMMARY
When reaching the center of the Earth, a person would experience weightlessness due to the gravitational forces from all sides canceling each other out. If positioned slightly off-center, oscillatory motion would occur, allowing one to bounce from one end of the Earth to the other in approximately 43 minutes. The gravitational pull experienced at any distance from the center is determined by the mass within that radius, following the formula αM, where α is the fraction of mass within a spherical shell. The discussion also highlights that external gravitational influences, such as the Moon and Sun, affect the perceived center of gravity, making the exact center not the true neutral point.
PREREQUISITES
- Understanding of Newtonian gravity principles
- Familiarity with gravitational formulas and concepts
- Basic knowledge of oscillatory motion and its calculations
- Awareness of the Earth-Moon system dynamics
NEXT STEPS
- Research the implications of gravitational forces in spherical shells
- Study the effects of the Earth-Moon system on gravitational balance
- Explore the differences between Newtonian gravity and general relativity
- Investigate the concept of barycenter in celestial mechanics
USEFUL FOR
Physicists, students of mechanics, and anyone interested in gravitational theories and the dynamics of celestial bodies will benefit from this discussion.