SUMMARY
At the center of the Earth, gravitational force is zero due to the cancellation of forces from surrounding mass. As one moves towards the center, gravitational acceleration decreases, reaching half the surface value at approximately halfway to the center, assuming a constant density model. However, variations in Earth's density complicate this approximation, leading to a maximum gravitational acceleration of about 10.7 m/s² at a depth of 3000 km before tapering off to zero at the center. The discussion highlights the importance of density profiles in accurately calculating gravitational forces within the Earth.
PREREQUISITES
- Understanding of Newtonian gravitation and the formula g = G*M/r²
- Familiarity with Poisson's equation in gravitational contexts
- Knowledge of Earth's density variations and their impact on gravitational calculations
- Basic grasp of gravitational acceleration concepts and units (m/s²)
NEXT STEPS
- Research the effects of varying density on gravitational acceleration within planetary bodies
- Study the implications of Poisson's equation in gravitational field theory
- Explore the relationship between gravitational acceleration and depth in different planetary models
- Learn about gravitational anomalies and their measurement techniques
USEFUL FOR
Students of physics, geophysicists, and anyone interested in understanding gravitational forces and their variations within planetary bodies.