SUMMARY
The gravity constant, denoted as G, was famously measured by Henry Cavendish using a torsion balance, a device originally invented by Charles-Augustin de Coulomb. Newton's theory of gravitation allows for the calculation of planetary masses based on their orbital radius and period, particularly when the orbiting object is significantly lighter than the central mass, such as planets around the Sun. Historical experiments, including one conducted on Schiehallion Mountain in the 18th Century, provided early estimates of Earth's density, contributing to the understanding of G and the masses of celestial bodies. Current values for GM for Earth are known to a higher precision than those for G or M individually.
PREREQUISITES
- Understanding of Newton's law of universal gravitation
- Familiarity with the concept of orbital mechanics
- Knowledge of the torsion balance and its application in physics
- Basic grasp of significant figures and measurement accuracy
NEXT STEPS
- Research the historical context and methodology of Henry Cavendish's experiment
- Explore the principles of orbital mechanics and how they relate to mass calculations
- Learn about the significance of the torsion balance in modern physics
- Investigate the methods used to measure the gravitational constant G in contemporary experiments
USEFUL FOR
Students of physics, researchers in gravitational studies, and anyone interested in the historical and scientific methods used to measure gravitational forces and planetary masses.