SUMMARY
The gravitational force experienced by an object decreases with the square of the distance from the center of the Earth. If an apple weighs 1 N at the Earth's surface, its weight at a distance three times further from the center of the Earth can be calculated using the formula f = m1m2/d². By substituting the distance into the equation, the weight at three times the distance is determined to be 1/9 N, not 1/3 N. This conclusion emphasizes the importance of correctly applying gravitational equations and understanding the inverse square law.
PREREQUISITES
- Understanding of gravitational force and the inverse square law
- Familiarity with the formula f = m1m2/d²
- Basic algebra for manipulating equations
- Knowledge of the concept of distance in gravitational contexts
NEXT STEPS
- Study the derivation of the gravitational force formula f = G(m1m2)/d²
- Explore the implications of the inverse square law in physics
- Learn about gravitational fields and potential energy
- Investigate real-world applications of gravitational force calculations
USEFUL FOR
Students studying physics, educators teaching gravitational concepts, and anyone interested in understanding the mathematical relationships governing gravitational forces.