Statement
Every particle of matter in the universe attracts every other particle with a gravitational force that is:
- Directly proportional to the product of their masses
- Inversely proportional to the square of the distance between them
Mathematical Form
The gravitational force F between masses m_{1} and m_{2} separated by distance r is:
F = G × m_{1} × m_{2} /
Key Constants
- G = N
- Dimensional formula of G: [ ]
- G was first measured by Henry Cavendish (1798) using a torsion balance
Properties of Gravitational Force
- Always attractive (no repulsion possible)
- Acts along the line joining the two masses
- Obeys Newton's Third Law: = − (equal magnitude, opposite direction)
- Obeys superposition principle (vector addition of forces from multiple masses)
- Central force (acts along the radius vector) — conserves angular momentum
- Universal — applies to all masses everywhere in the universe
- Conservative — work done is path-independent
Cavendish Experiment
- Torsion balance with known masses
- Tiny angular twist measured by mirror-light lever
- This effectively "weighed the Earth" — once G known, M_Earth = /G
Surface Gravity
From Newton's Law, the gravitational acceleration at Earth's surface:
g = GM/ ≈ 9.8 m
where M = Earth's mass = kg, R = m.