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Principles of Mechanics

Newton's Laws of Motion

Physics I 312 words Free to read

The Laws of Motion

Steady motion needs no force at all; forces only explain changes in motion. The second law runs both ways: ask what net force acts to find acceleration, or see acceleration to know the net force.

Newton's three laws form classical mechanics:

LawCore RuleStatement
First (Inertia)Zero Net ForceA body stays at rest or in uniform motion unless acted on by a net external force.
SecondFnet=ma\vec{F}_{\text{net}} = m\vec{a}Only the vector sum of all forces determines acceleration.
ThirdAction-ReactionIf body A exerts a force on body B, B exerts an equal and opposite force on A.

Common pitfall: Action-reaction pairs never cancel because they act on different bodies. The book's weight and the table's normal force on it are NOT a third-law pair; both act on the book itself.

Free-Body Diagrams & Forces

Free-body diagrams are the essential tool for applying Newton's laws: isolate the object, draw all forces acting on it, choose coordinate axes, and apply Fx=max\sum F_x = ma_x and Fy=may\sum F_y = ma_y.

Common forces quantify these interactions:

ForceFormulaDirectionMeaning
WeightW=mgW = mgDownwardGravitational pull (mm is mass, gg is gravity).
NormalNNPerpendicularSupport force from a surface.
Kinetic frictionfk=μkNf_k = \mu_k NOpposing motionFriction during sliding (μk\mu_k is kinetic coefficient).
Static frictionfsμsNf_s \leq \mu_s NOpposing tendencyFriction before sliding starts (μs\mu_s is static coefficient).
TensionTTAlong stringPulling force exerted by a taut rope or string.
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Principles of Mechanics