Newton's Laws and Forces

The three laws

Kinematics described motion; dynamics explains it through forces. Newton’s three laws are the foundation ¹:

1. Law of inertia. An object at rest stays at rest, and one in motion continues at constant velocity, unless acted on by a net external force. Equilibrium means \(\vec F_{net} = 0\), not “no forces.”
2. \(\vec F_{net} = m\vec a\). The net force equals mass times acceleration. This vector equation is the workhorse of mechanics: sum the forces, divide by mass, get the acceleration.
3. Action–reaction. For every force there is an equal and opposite force on the other body: \(\vec F_{AB} = -\vec F_{BA}\). The two forces act on different objects, which is why they do not simply cancel.

Common forces

A handful of forces recur throughout engineering statics and dynamics ¹:

• Weight, the gravitational pull, \(W = mg\), directed downward.
• Normal force \(N\), the push a surface exerts perpendicular to itself.
• Friction \(f\), resisting sliding along a surface, modeled as \(f \le \mu N\) (with \(f = \mu N\) at the point of slipping, where \(\mu\) is the coefficient of friction).
• Tension in ropes and cables, and applied/contact forces.

Free-body diagrams

The single most important problem-solving habit is the free-body diagram: isolate one object, draw every force acting on it as an arrow, and nothing else. Then apply \(\vec F_{net} = m\vec a\) along convenient axes.

The inclined-plane case in the figure is the canonical example, and the trick is choosing axes along and perpendicular to the incline rather than horizontal and vertical. Resolving the weight into those axes gives a component \(mg\sin\theta\) directed down the slope and \(mg\cos\theta\) pressing into it ¹. Perpendicular to the surface there is no acceleration, so the normal force balances the perpendicular weight component:

Along the surface, the net force sets the acceleration. If the block is in equilibrium, friction balances the downhill pull, \(f = mg\sin\theta\); if it slides, the net force is \(mg\sin\theta - \mu N\) and Newton’s second law gives the acceleration. This decomposition — pick smart axes, resolve forces, apply \(\vec F_{net} = m\vec a\) per axis — is exactly the method the Statics course builds on for structures in equilibrium.