Compute equal and opposite force pairs, relate masses and accelerations using m₁·a₁ = – m₂·a₂. Visualize action-reaction vectors on two interacting objects.
Newton's third law states: For every action, there is an equal and opposite reaction. When one object exerts a force on a second object, the second object simultaneously exerts a force equal in magnitude and opposite in direction on the first object. These forces always occur in pairs and act on different bodies. Mathematically: F₁→₂ = – F₂→₁.
F₁ = –F₂ ⟹ m₁·a₁ = – m₂·a₂
The product mass × acceleration for two interacting objects are equal in magnitude and opposite in direction.
From Newton's second law, F = dp/dt. For two isolated interacting objects, the total momentum is constant: p₁ + p₂ = constant. Thus dp₁/dt + dp₂/dt = 0 ⇒ F₁ + F₂ = 0 ⇒ F₂ = –F₁. For constant masses, m₁·a₁ = – m₂·a₂. Our calculator uses this relationship. When solving for a₂: a₂ = – (m₁·a₁)/m₂. Note that negative sign indicates opposite direction.
| Scenario | Action Force | Reaction Force | Key insight |
|---|---|---|---|
| Rocket thrust | Exhaust gases pushed backward | Rocket pushed forward | Rocket moves without pushing against ground |
| Gun recoil | Bullet accelerated forward | Gun moves backward | m_bullet·a_bullet = – m_gun·a_gun |
| Swimming | Swimmer pushes water backward | Water pushes swimmer forward | Propulsion in fluids |
| Walking | Foot pushes ground backward | Ground pushes foot forward | Friction enables motion |
A rocket of mass 500 kg ejects exhaust at a rate producing acceleration of 5 m/s² upward. The exhaust gases experience an equal downward force. Using m₁·a₁ = – m₂·a₂, if the exhaust mass flow rate corresponds to an effective mass of 200 kg, then the exhaust acceleration a₂ = – (500×5)/200 = –12.5 m/s² (downward). Our calculator instantly verifies thrust and recoil effects, crucial for aerospace engineering.
Newton’s third law is the foundation of momentum conservation in isolated systems. It also implies that internal forces cannot change the total momentum of a system. This principle governs collisions, explosions, and even celestial mechanics.