Topic: Newton’s Laws of Motion
1. Introduction
Newton's laws of motion describe the relationship between the motion of an object and the
forces acting on it. These laws are fundamental to understanding classical mechanics.
2. Newton's First Law of Motion (Law of Inertia)
Definition: An object will remain at rest or in uniform motion in a straight line unless
acted upon by an external force.
Key Concept: Inertia – The tendency of an object to resist a change in its state of motion.
Examples:
A book lying on a table remains at rest until pushed.
A passenger in a moving car tends to move forward when brakes are applied suddenly.
Formula:
Fnet=0(No external force)F_{\text{net}} = 0 \quad \text{(No external force)}
3. Newton's Second Law of Motion
Definition: The acceleration of an object is directly proportional to the net force acting
on it and inversely proportional to its mass.
Key Concept: Explains how force causes changes in motion.
Formula:
F=m⋅aF = m \cdot a
Where:
FF = Net force (in Newtons)
mm = Mass of the object (in kilograms)
aa = Acceleration (in m/s²)
Example Problem:
If a 5 kg object experiences a net force of 20 N, what is its acceleration?
a=Fm=205=4 m/s2a = \frac{F}{m} = \frac{20}{5} = 4 \, \text{m/s}^2
4. Newton's Third Law of Motion
Definition: For every action, there is an equal and opposite reaction.
Key Concept: Forces always occur in pairs.
Examples:
A rocket launching: The exhaust gases push downward (action), and the rocket moves
upward (reaction).