Apply Newton's three laws to systems of objects, analyse forces on inclined planes, and solve problems involving friction, tension and connected objects.
An object remains at rest or moves in a straight line at constant velocity unless acted upon by a net (resultant) external force.
This property is called inertia — the tendency of an object to resist changes to its state of motion. Inertia is directly proportional to mass.
When a net force acts on an object, it accelerates in the direction of the net force. The acceleration is directly proportional to the net force and inversely proportional to the mass.
| Symbol | Meaning | Unit |
|---|---|---|
| Fnet | Net (resultant) force | N |
| m | Mass of object | kg |
| a | Acceleration | m·s⁻² |
For every action force, there is an equal and opposite reaction force. These forces:
An FBD shows all forces acting on a single object as arrows from or through the object's centre. Rules:
The normal force N is perpendicular to the contact surface. On a flat surface: N = mg. On an incline at angle θ: N = mg cosθ.
Static friction prevents sliding: fs ≤ μsN. It equals the applied force up to a maximum of μsN (maximum static friction = μsN).
Kinetic friction acts while sliding: fk = μkN. Note: μk < μs always.
Resolve the weight into components parallel and perpendicular to the slope:
Apply Fnet = ma along the slope: if the block slides down, take down-the-slope as positive.
For two blocks connected by a string: treat the whole system for acceleration, then isolate one block for tension.
The apparent weight is the normal force N from the scale in a lift:
In an ideal Atwood machine, two masses hang over a massless, frictionless pulley. IEB may introduce a pulley with mass (moment of inertia), or friction in the pulley bearing. Qualitatively: a massive pulley slows the acceleration because energy is used to spin the pulley. The tension on each side of a massive pulley is different (unlike an ideal pulley where tensions are equal for a stationary pulley problem).
An inertial frame is one that is not accelerating. Newton's Laws hold exactly in inertial frames. In a non-inertial (accelerating) frame (e.g., a rotating carousel), a fictitious force appears — the centrifugal force. It is not a real force; it arises because the observer is accelerating. The Coriolis effect (deflection of moving objects on Earth) is another fictitious force in Earth's rotating frame.
| Time (s) | 0 | 1 | 2 | 3 | 4 | 5 |
|---|---|---|---|---|---|---|
| Velocity (m·s⁻¹) | 24 | 20 | 16 | 12 | 8 | 4 |