Part of ME-06 — Gravitation

Newton's Universal Law of Gravitation

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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} / r2r^{2}

Key Constants

  • G = 6.674×10116.674 \times 10^{-11} N m2m^{2} kg2kg^{-2}
  • Dimensional formula of G: [M1M^{-1} L3L^{3} T2T^{-2}]
  • 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: F12F_{12} = −F21F_{21} (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 = gR2gR^{2}/G

Surface Gravity

From Newton's Law, the gravitational acceleration at Earth's surface:

g = GM/R2R^{2} ≈ 9.8 m s2s^{-2}

where M = Earth's mass = 5.97×10245.97 \times 10^{24} kg, R = 6.4×1066.4 \times 10^{6} m.

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