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Physics Pathways

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A gravitational force causes a freely falling object to accelerate and keeps a

satellite moving in a
circular path. Clearly a force can change the speed or direction of travel of an
object. A force can
also change the shape or size of an object. If you stand on an empty paper
carton it will change its
shape and if you pull on a spiral spring it will stretch. Several forces may act
on an object at once and
it is useful to calculate a resultant force to predict their combined effect;
both the size and direction
of the forces are needed for this. Friction between a moving object and its
surroundings is also
important as it acts to reduce the speed of the object and produce heat. You
have already learnt how
to quantify some of these changes and in this topic you will encounter more
ways to do so.
Title Slide
 Title: Understanding Mechanics in Physics
 Subtitle: The Fundamentals of Motion and Forces

Introduction to Mechanics
 Definition: Mechanics is the branch of physics that deals with the motion
of objects and the forces that act upon them.
 Importance: Fundamental to understanding the physical world, from the
motion of planets to the dynamics of everyday objects.

Slide 3: Types of Mechanics


 1. Classical Mechanics:
 Definition: Describes the motion of objects that are much larger
than atoms and move at speeds much slower than the speed of
light.
 Example: Newton's laws of motion.
 2. Quantum Mechanics:
 Definition: Deals with the behavior of particles at the atomic and
subatomic levels.
 Example: Wave-particle duality.
 3. Relativistic Mechanics:
 Definition: Applies to objects moving at speeds close to the speed
of light.
 Example: Einstein's theory of relativity.

Slide 4: Newton's Laws of Motion


 1. First Law (Law of Inertia):
 Definition: An object at rest stays at rest, and an object in motion
stays in motion with the same speed and in the same direction
unless acted upon by an external force.
 2. Second Law (Force and Acceleration):
 Definition: The acceleration of an object is directly proportional to
the net force acting upon it and inversely proportional to its mass.
 3. Third Law (Action and Reaction):
 Definition: For every action, there is an equal and opposite
reaction.

Slide 5: Applications of Mechanics


 1. Projectile Motion:
 Definition: The motion of an object thrown or projected into the
air subject to gravity.
 Example: Throwing a ball, launching a rocket.
 2. Circular Motion:
 Definition: The motion of an object in a circular path.
 Example: A car navigating a curve, a planet orbiting the sun.
 3. Friction:
 Definition: The force resisting the relative motion of solid surfaces,
fluid layers, and material elements sliding against each other.
 Example: Sliding a book on a table.

Slide 6: Forces in Mechanics


 1. Gravitational Force:
 Definition: The force of attraction between two masses.
 Example: Earth's gravitational pull.
 2. Electromagnetic Force:
 Definition: The force between charged particles.
 Example: Attraction or repulsion between magnets.
 3. Strong and Weak Nuclear Forces:
 Definition: Forces that act at the atomic and subatomic levels.
 Example: Binding protons and neutrons in an atomic nucleus.

Slide 7: Conclusion
 Recap of key points: Mechanics is a fundamental branch of physics,
encompassing classical, quantum, and relativistic mechanics.
 Importance: Essential for understanding and predicting the motion of
objects, from the microscopic to the cosmic scales.

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