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Newton's Laws of Motion

Newton's three laws of motion with formulas, explanations, and real-world examples.
Foundation of classical mechanics.

Newton's First Law (Law of Inertia)

An object at rest stays at rest, and an object in motion stays in motion at constant velocity, unless acted upon by a net external force.

If ΣF = 0, then v = constant

In simple terms: things keep doing what they are doing unless a force changes that. A ball rolling on a frictionless surface would roll forever.

Newton's Second Law

F = m × a

ΣF = m × a

The net force on an object equals its mass times its acceleration. This is the most used equation in classical mechanics.

Variables

SymbolMeaningUnit
FForceNewtons (N)
mMassKilograms (kg)
aAccelerationm/s²
ΣFNet (total) forceNewtons (N)
vVelocitym/s

Newton's Third Law

For every action, there is an equal and opposite reaction.

F₁₂ = −F₂₁

When object A exerts a force on object B, object B exerts an equal force back on object A in the opposite direction. When you push a wall, the wall pushes back on you with the same force.

Example 1 — Second Law

A 5 kg box is pushed with a force of 20 N. What is the acceleration?

F = m × a → a = F / m

a = 20 N / 5 kg

a = 4 m/s²

Example 2 — Weight Force

What is the weight (force of gravity) on a 70 kg person?

Weight = m × g (where g = 9.81 m/s²)

W = 70 × 9.81

W = 686.7 N (about 154.3 lbs of force)

Example 3 — Third Law

A swimmer pushes water backward with 50 N of force. What happens?

By Newton's third law, the water pushes the swimmer forward with 50 N.

The swimmer accelerates forward (F = 50 N in the forward direction).

When to Use Them

  • First law: Understanding why objects resist changes in motion (inertia, seatbelts, etc.)
  • Second law: Calculating force, mass, or acceleration when two of the three are known
  • Third law: Analyzing interactions between objects (rockets, swimming, walking)

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