The Gravitational Constant
The gravitational constant (G) is a key figure in the universal law of gravitation, signifying the proportionality factor that relates the gravitational force between two masses to the product of their masses and the inverse of the square of the distance between them. The value of G was first determined through experiments conducted by Henry Cavendish in 1798, making use of a torsion balance to measure the tiny gravitational forces between lead spheres.
Cavendish’s Experiment
Cavendish's apparatus involved a horizontal bar suspended from a wire, with small lead spheres attached at each end. Large lead spheres were then placed near the smaller ones. Due to gravitational attraction, the bar rotated slightly, and the angle of rotation could be measured. This experiment allowed Cavendish to not only measure G accurately but also estimate the mass of the Earth, confirming the efficacy of the gravitational theory.
Current Value
The currently accepted value of the gravitational constant is:
G = 6.67 × 10^(-11) N m²/kg²
This value is fundamental for calculations involving gravitational forces in astrophysics and cosmology.