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4. LAWS OF MOTION
The chapter discusses the laws of motion, emphasizing the concepts introduced by Galileo and Newton. It explains the significance of forces in motion, defining inertia, momentum, and the three laws of motion. Through examples and illustrations, it explores how these principles apply in various real-life scenarios, including the effects of friction, circular motion, and equilibrium.
Sections
The introduction discusses the fundamental concepts of motion, emphasizing the necessity of external forces to initiate or alter motion.
Inertia is the resistance of a body to change its state of motion, defined by Newton's first law.
The second law of motion relates the force applied to an object to its mass and acceleration, encapsulated in the equation F = ma.
The third law of motion states that for every action, there is an equal and opposite reaction.
Inertia
The property of a body to resist changes to its state of rest or uniform motion unless acted upon by an external force.
Momentum
The product of an object's mass and its velocity, represented mathematically as p = mv.
Newton's First Law of Motion
A body at rest stays at rest, and a body in motion continues in uniform motion unless acted upon by an external force.
Newton's Second Law of Motion
The acceleration of an object is directly proportional to the net external force acting on it and inversely proportional to its mass.
Newton's Third Law of Motion
For every action, there is an equal and opposite reaction; forces always occur in pairs.
Friction
The force that opposes the relative motion of two surfaces in contact.
Equilibrium
A state in which the net external force acting on a body is zero, resulting in the body being at rest or in uniform motion.
Practice Exercises
Total Questions
5
Estimated Time
10 min
Passing Score
70%
Instructions
- Read each question carefully
- You can use hints if you need help
- Complete all questions before submitting