SUMMARY
When a ball is dropped into a hole drilled through the center of the Earth, it will initially fall to the center due to gravity, then continue to oscillate back and forth, akin to a pendulum, until it eventually comes to rest at the center. The time taken for this journey is approximately 42 minutes, calculated using the formula T = π * √(r/g), where r is Earth's radius (6,378,100 m) and g is the acceleration due to gravity (9.81 m/s²). This scenario assumes no friction or other forces acting on the ball, which would otherwise prevent it from reaching the opposite side of the Earth.
PREREQUISITES
- Understanding of gravitational forces and motion
- Familiarity with simple harmonic motion (S.H.M.) concepts
- Basic knowledge of physics formulas, particularly those involving time, radius, and gravity
- Awareness of Earth's physical properties, including density variations
NEXT STEPS
- Research the derivation of the formula T = π * √(r/g) in the context of gravitational physics
- Explore the implications of varying Earth's density on gravitational calculations
- Investigate the concept of antipodes and the likelihood of drilling through land versus water
- Learn about the effects of friction and other forces on oscillatory motion in physics
USEFUL FOR
Physics students, educators, and anyone interested in gravitational dynamics and the theoretical implications of drilling through the Earth.