Physics: Classical Mechanics
Explore Newton's laws of motion, kinematics, and fundamental physics equations with clear mathematical formulations.
Physics: Classical Mechanics
Introduction
Classical mechanics describes the motion of macroscopic objects. From falling apples to orbiting planets, the equations of mechanics govern the physical world around us.
Kinematics: Motion in One Dimension
Position and Displacement
The position of an object is described by , a function of time. Displacement is:
Velocity
Average velocity:
Instantaneous velocity:
Acceleration
Average acceleration:
Instantaneous acceleration:
Kinematic Equations
For constant acceleration , we have the four kinematic equations:
where:
- = initial velocity
- = final velocity
- = acceleration
- = time
- = initial position
- = final position
Interactive: Projectile Motion
The chart below shows position vs. time for an object dropped from rest (no air resistance, ):
And here is the corresponding velocity vs. time graph ():
Newton's Laws of Motion
First Law (Inertia)
An object at rest stays at rest, and an object in motion stays in motion with the same speed and direction, unless acted upon by an unbalanced force.
Second Law (Force and Acceleration)
The net force on an object equals its mass times its acceleration:
This is the fundamental equation of mechanics. From it, we can derive:
Third Law (Action-Reaction)
For every action, there is an equal and opposite reaction:
Types of Forces
Gravitational Force
Newton's law of universal gravitation:
where .
Near Earth's surface:
where .
Normal Force
The normal force acts perpendicular to a surface. For an object on a flat surface:
Friction
Static friction:
Kinetic friction:
where and are the coefficients of static and kinetic friction.
Spring Force (Hooke's Law)
where is the spring constant and is the displacement from equilibrium.
Work and Energy
Work
Work done by a constant force:
where is the angle between the force and displacement vectors.
Kinetic Energy
Potential Energy
Gravitational potential energy:
Elastic potential energy:
Work-Energy Theorem
Conservation of Energy
Momentum and Impulse
Linear Momentum
Impulse
Conservation of Momentum
For an isolated system:
Interactive Simulation: Forces and Motion
Experiment with the simulation below to see Newton's laws in action. Apply different forces to objects and observe how they accelerate.
Try applying different forces to the objects. Notice how heavier objects accelerate more slowly for the same force — this is Newton's Second Law in action!
3D Molecular Viewer
Explore the 3D structure of Crambin (PDB: 1CRN), a small plant protein with 46 amino acids. Drag to rotate, scroll to zoom, and right-click to pan.
Molecular structures are loaded from the RCSB Protein Data Bank. You can replace 1CRN with any valid PDB ID (e.g., 4HHB for hemoglobin, 1IGT for an antibody).
Practice Questions
A car accelerates from rest at 2 m/s² for 5 seconds. What is its final velocity?
According to Newton's Second Law, if you double the force on an object, what happens to its acceleration?
A 5 kg object is lifted 3 meters. What is its gravitational potential energy? (g = 10 m/s²)
Interactive Exercises
Drag-and-Drop: Order the Kinematic Steps
Put these steps in the correct order for solving a kinematics problem:
Order these steps for solving a kinematics problem:
Matching: Newton's Laws
Match each law of motion with its correct statement:
Match each law of motion with its statement:
Drag answers from here:
Fill in the Blanks: Energy Conservation
Complete the conservation of energy equation:
The total blank energy equals the total blank energy: KE_i + PE_i = KE_f + PE_f. Kinetic energy is blankmv² and gravitational potential energy is blank.
Word Bank — drag words into the blanks above:
Key Takeaways
- Kinematics equations describe motion with constant acceleration: and
- Newton's Second Law:
- Work: ; Kinetic Energy:
- Energy is conserved:
- Momentum is conserved in isolated systems