SUMMARY
The mass of Earth, approximately 10^24 kg, was first estimated through the Cavendish experiment conducted by Henry Cavendish around 1798. In this experiment, a rod was suspended from a thread, and a known mass was placed nearby to observe the rod's movement due to gravitational attraction. By measuring the displacement and knowing the resistance of the thread, Cavendish calculated the gravitational constant (G). Using the formula M=gr^2/G, where g is the acceleration due to gravity (9.81 m/s²) and r is the Earth's radius (6,378,000 m), he derived the mass of the Earth.
PREREQUISITES
- Understanding of gravitational force and its measurement
- Familiarity with the Cavendish experiment methodology
- Knowledge of the gravitational constant (G)
- Basic grasp of physics formulas, specifically M=gr^2/G
NEXT STEPS
- Research the historical context and significance of the Cavendish experiment
- Explore the implications of the gravitational constant (G) in modern physics
- Study the methods used to measure gravitational force in contemporary experiments
- Learn about advancements in geophysics and how they relate to Earth's mass estimation
USEFUL FOR
Students of physics, educators in astronomy, and anyone interested in the historical methods of scientific measurement and gravitational studies.