SUMMARY
The acceleration of free fall at the equator is defined by the equation a = g - v²/R, where g is the gravitational force, v is the tangential velocity of the Earth's surface (approximately 465 m/s), and R is the Earth's radius (approximately 6400 km). This equation illustrates that the observed acceleration of free fall is reduced by the centripetal acceleration due to Earth's rotation. At the poles, the centripetal acceleration is negligible, resulting in free fall acceleration equating to the gravitational field strength of 9.81 m/s². The centrifugal force, while a pseudo-force, is essential for understanding the difference in free fall acceleration between the equator and the poles.
PREREQUISITES
- Newton's Second Law of Motion
- Understanding of gravitational force and centripetal acceleration
- Basic knowledge of physics concepts related to motion
- Familiarity with the Earth's rotation and its effects on gravity
NEXT STEPS
- Study the derivation of gravitational force using GM/r²
- Learn about the effects of Earth's rotation on gravitational measurements
- Explore the concept of pseudo-forces in rotating reference frames
- Investigate the differences in gravitational acceleration at various latitudes
USEFUL FOR
Students studying physics, educators teaching mechanics, and anyone interested in the effects of Earth's rotation on gravitational forces.