SUMMARY
The radial acceleration of Earth at the equator is calculated using the formula a = v²/r, where v is the tangential velocity and r is the radius of the Earth. The correct calculation yields a radial acceleration of approximately 169.9 m/s², based on a tangential velocity of 1041 m/s and a radius of 6378 km. This value accurately reflects the acceleration experienced by an object due to the Earth's rotation at the equator, although it may vary slightly based on geographic factors.
PREREQUISITES
- Understanding of basic physics concepts, specifically circular motion
- Familiarity with the formula for radial acceleration
- Knowledge of Earth's radius and rotational speed
- Basic mathematical skills for performing calculations
NEXT STEPS
- Research the effects of Earth's shape on radial acceleration
- Learn about the variations in gravitational acceleration at different latitudes
- Explore the relationship between tangential velocity and radial acceleration
- Investigate the impact of Earth's rotation on satellite orbits
USEFUL FOR
Students of physics, engineers working on geophysical projects, and anyone interested in understanding the dynamics of Earth's rotation and its effects on objects at the equator.