SUMMARY
The universal gravitational constant, denoted as 'G', is a proportionality constant in Newton's law of gravitation, defined by the equation F ∝ (m1 * m2) / r². Its value was first determined experimentally by Henry Cavendish, who faced challenges due to measurement errors. G is not a fundamental parameter of the universe but rather a reflection of the units used to express it; in Planck units, G equals 1. The historical measurement of G involved experiments such as the deflection of a pendulum near Schieallion mountain in Scotland in 1774.
PREREQUISITES
- Understanding of Newton's law of gravitation
- Familiarity with experimental physics and measurement techniques
- Knowledge of unit systems, particularly SI and Planck units
- Basic grasp of dimensionless constants in physics
NEXT STEPS
- Research the Cavendish experiment and its significance in measuring G
- Explore the concept of dimensionless constants, such as the fine-structure constant
- Learn about the historical context of gravitational measurements, including the Schieallion experiment
- Investigate the implications of changing unit definitions on physical constants
USEFUL FOR
Physics students, researchers in gravitational studies, and anyone interested in the foundational constants of the universe and their measurement techniques.