SUMMARY
The gravitational constant, denoted as G and valued at 6.67 x 10-11 m3 kg-1 s-2, is crucial for calculating the gravitational force between two masses using the formula F = G(m1m2/r2). It is important to distinguish between G and the acceleration due to gravity on Earth, represented as little g (9.8 m/s2). The confusion often arises from mixing these two concepts, as G is a constant while little g is an acceleration experienced by objects near Earth's surface. The measurement of G was first accomplished by Henry Cavendish through a torsion balance setup.
PREREQUISITES
- Understanding of Newton's Law of Universal Gravitation
- Familiarity with the concepts of mass and distance in physics
- Knowledge of basic physics formulas, particularly F = G(m1m2/r2)
- Ability to differentiate between gravitational constant (G) and acceleration due to gravity (g)
NEXT STEPS
- Research the historical context and experiments conducted by Henry Cavendish to measure G
- Explore the implications of gravitational constant in astrophysics and cosmology
- Learn about the differences between classical mechanics and general relativity regarding gravity
- Investigate the applications of G in satellite motion and orbital mechanics
USEFUL FOR
Students of physics, educators teaching gravitational concepts, and anyone interested in the fundamental principles of gravity and its measurement.