Work & Energy

Module 6, Lesson 1 | PHYS-1315 Physical Science I
"Energy cannot be created or destroyed, only transformed from one form to another."
— First Law of Thermodynamics

Understanding Work & Energy

Energy is one of the most fundamental concepts in all of physics. It provides an alternative way to analyze motion that doesn't require vectors and offers powerful insights into the behavior of physical systems. Work and energy concepts allow us to solve complex problems with elegant simplicity and understand the deep conservation principles that govern our universe.

This lesson builds upon your knowledge of forces to discover how work changes a system's energy. We'll explore the work-energy theorem, different forms of energy storage, and the principle of energy conservation that underlies everything from roller coasters to power plants.

Energy Analysis Advantage

Unlike force analysis which requires vector calculations, energy analysis uses scalar quantities. This often makes complex problems much simpler to solve, especially when dealing with curved paths or changing forces.

Learning Objectives

Course Competency CC6.1

Solve problems related to the work done by forces and changes in energy

LO6.1.1

Calculate work from displacement and net force using W = F·d = Fd cos θ

LO6.1.2

Distinguish between conservative and non-conservative forces and their effects

LO6.1.3

Compute kinetic energy (½mv²) and gravitational potential energy (mgh)

LO6.1.4

Identify different ways in which energy is stored in physical systems

LO6.1.5

Compute the total energy and changes in energy of a system using conservation principles

Required Readings

Primary Reading

Equation Sheet

Supplementary Resources

Interactive Activity 1: Energy Problem-Solving Sequence

Instructions: Arrange the following steps in the correct order for solving work and energy problems. This systematic approach ensures you apply conservation principles correctly and avoid common pitfalls.

Identify the system and states

Define what objects are included and the initial/final states to analyze

Identify all forces acting

List conservative forces (gravity, springs) and non-conservative forces (friction, air resistance)

Choose reference points

Set zero potential energy level and establish coordinate system

Calculate initial energy

Find KE₁ + PE₁ for the initial state of the system

Calculate work by non-conservative forces

Find work done by friction, air resistance, or other dissipative forces

Apply work-energy theorem

Use E₁ + W_nc = E₂ or ΔKE = W_net to find final state

Verify solution makes physical sense

Check units, signs, and whether answer is reasonable for the scenario

Energy Analysis Key: Always distinguish between conservative and non-conservative forces. Conservative forces (gravity, springs) store energy as potential energy, while non-conservative forces (friction) dissipate energy. The work-energy theorem connects force analysis to energy conservation.

Interactive Activity 2: Work and Energy Concepts Classification

Instructions: Sort the following concepts related to work and energy into their correct categories. Understanding these classifications is essential for choosing the right approach to energy problems.

Kinetic Energy

Energy of motion and movement

Potential Energy

Stored energy due to position or configuration

Work & Forces

Force applications and work calculations

Conservation Laws

Fundamental conservation principles

KE = ½mv²
Translational motion energy
Rotational motion energy
Energy increases with speed squared
PE = mgh (gravitational)
PE = ½kx² (elastic/spring)
Energy stored at height
Energy in compressed/stretched spring
W = F·d = Fd cos θ
Conservative forces (gravity, springs)
Non-conservative forces (friction, air resistance)
Work-energy theorem: W_net = ΔKE
Total mechanical energy conserved
E_initial = E_final (no friction)
Energy transformed, never destroyed
KE + PE = constant (conservative systems)

Energy Classification: Kinetic energy depends on motion (speed), potential energy depends on position (height, compression). Conservative forces allow energy conversion between KE and PE, while non-conservative forces dissipate mechanical energy. Conservation laws are fundamental - energy is always conserved, though it may change forms.

Interactive Activity 3: Work and Energy Principles

Instructions: Click each card to reveal detailed information about fundamental work and energy concepts, conservation laws, and problem-solving strategies. These principles form the foundation of energy analysis.

Work Definition

W = F·d cos θ

Force Applied Through Distance

  • • Work = force × displacement × cos(angle)
  • • Only force component parallel to motion does work
  • Units: Joules (J) = N⋅m
  • • Positive work: force helps motion
  • • Negative work: force opposes motion
  • • Zero work: force perpendicular to motion

Kinetic Energy

KE = ½mv²

Energy of Motion

  • • Energy possessed by moving objects
  • • Depends on mass and speed squared
  • • Always positive (speed squared)
  • Units: Joules (J)
  • • Doubling speed quadruples kinetic energy
  • • Related to momentum: KE = p²/(2m)

Gravitational PE

PE = mgh

Energy Stored by Height

  • • Energy stored due to position in gravity field
  • • Depends on mass, gravity, and height
  • • Reference level can be chosen arbitrarily
  • g = 9.8 m/s² on Earth's surface
  • • Converts to kinetic energy when falling
  • • Conservative force - path independent

Elastic PE

PE = ½kx²

Energy Stored in Springs

  • • Energy stored in compressed or stretched springs
  • k: spring constant (N/m)
  • x: displacement from equilibrium
  • • Quadratic relationship with displacement
  • • Applies to any elastic deformation
  • • Conservative force - energy recoverable

Work-Energy Theorem

W_net = ΔKE

Net Work Equals Change in Kinetic Energy

  • • Total work done equals change in kinetic energy
  • • W_net = KE_final - KE_initial
  • • Alternative to Newton's 2nd Law
  • • Useful for variable forces
  • • Links force analysis to energy analysis
  • • Works for curved paths and complex motions

Conservative Forces

Path Independent

Forces That Store Energy

  • • Work depends only on start and end points
  • • Work around closed loop = zero
  • • Examples: gravity, spring force, electric force
  • • Can convert KE ↔ PE reversibly
  • • Allow mechanical energy conservation
  • • Have associated potential energy functions

Non-Conservative Forces

Path Dependent

Forces That Dissipate Energy

  • • Work depends on path taken
  • • Examples: friction, air resistance, tension
  • • Convert mechanical energy to heat
  • • Mechanical energy not conserved
  • • Usually oppose motion (negative work)
  • • Cause energy "losses" from mechanical system

Energy Conservation

E_total = constant

Fundamental Conservation Principle

  • • Energy cannot be created or destroyed
  • • Energy can be transformed between forms
  • Mechanical energy: E = KE + PE
  • • E₁ + W_nc = E₂ (general form)
  • • E₁ = E₂ (conservative forces only)
  • • Basis for analyzing complex systems

Energy Conservation and Work Laws

Work Definition

Force Applied Through Distance
W = F⋅d = Fd cos θ

Work is the energy transfer that occurs when a force is applied through a distance. Only the component of force parallel to the displacement contributes to work.

Key Insight: Work is a scalar quantity measured in Joules (J).

Applications: Lifting objects, pushing boxes, climbing stairs

Work-Energy Theorem

Net Work Changes Kinetic Energy
W_net = ΔKE = ½mv₂² - ½mv₁²

The net work done on an object equals its change in kinetic energy. This powerful theorem connects force analysis with energy analysis.

Key Insight: Alternative approach to Newton's 2nd Law for complex problems.

Applications: Variable forces, curved paths, collision analysis

Energy Conservation

Mechanical Energy Conservation
KE₁ + PE₁ = KE₂ + PE₂

In the absence of non-conservative forces, the total mechanical energy (kinetic + potential) remains constant. Energy converts between forms but total amount is preserved.

Key Insight: Most powerful tool for solving energy problems efficiently.

Applications: Roller coasters, pendulums, planetary motion

Forms of Energy

Kinetic Energy

Translational KE (½mv²): Energy of linear motion; depends on mass and speed squared.

Rotational KE: Energy of spinning objects; depends on moment of inertia and angular velocity.

Key Features:

  • Always positive (speed squared)
  • Increases rapidly with speed
  • Converts to potential energy and back
  • Related to momentum and temperature

Potential Energy

Gravitational PE (mgh): Energy stored due to position in a gravitational field; increases with height.

Elastic PE (½kx²): Energy stored in springs, rubber bands, and deformed materials.

Key Features:

  • Depends on position or configuration
  • Can be negative (below reference level)
  • Converts to kinetic energy when released
  • Associated with conservative forces

Work & Power

Work (W = F⋅d): Energy transfer when force acts through distance; can be positive or negative.

Power (P = W/t): Rate of energy transfer or work done; measured in Watts.

Key Features:

  • Work changes energy of system
  • Power indicates how quickly work is done
  • Positive work increases energy
  • Negative work decreases energy

Energy Storage & Transfer

Chemical Energy: Stored in molecular bonds; released in reactions (food, fuel, batteries).

Thermal Energy: Random kinetic energy of molecules; related to temperature.

Other Forms: Nuclear, electromagnetic, sound, electrical energy.

Key Features:

  • Energy can be stored in many forms
  • Conversions between forms are common
  • Total energy always conserved
  • Efficiency measures useful energy transfer

Video Lectures

Work and Energy Introduction

Duration: 6:29 | Topic: Work definition, force-displacement relationship

ASL Version available

Work-Energy Theorem, Potential Energy, and Non-Conservative Forces

Duration: 9:36 | Topic: W-KE theorem, conservative vs non-conservative forces, energy diagrams

ASL Version available

Total Energy & Energy Conservation

Duration: 8:56 | Topic: Energy conservation, total mechanical energy, bonus problems

Key Lessons and Appendix

Duration: 9:00 | Topic: Module summary and key concepts review

ASL Version available

Problem Solving Examples

Energy Problem-Solving Strategy

  1. Identify system: What objects and energy forms are involved?
  2. Choose reference levels: Set PE = 0 level conveniently
  3. List initial and final states: Identify speeds, heights, compressions
  4. Identify forces: Conservative vs non-conservative forces
  5. Apply energy conservation: E₁ + W_nc = E₂
  6. Solve and check: Units, signs, reasonable magnitude

Example: Roller Coaster Energy

Problem: A 500 kg roller coaster car starts from rest at a height of 30 m. What is its speed when it reaches a height of 10 m? (Ignore friction)

Click to reveal solution

Given: m = 500 kg, h₁ = 30 m, v₁ = 0 m/s, h₂ = 10 m

Initial energy: E₁ = KE₁ + PE₁ = 0 + mgh₁ = 500 × 9.8 × 30 = 147,000 J

Final energy: E₂ = ½mv₂² + mgh₂ = ½(500)v₂² + 500 × 9.8 × 10

Energy conservation: E₁ = E₂ → 147,000 = 250v₂² + 49,000

Solve: 250v₂² = 98,000 → v₂² = 392 → v₂ = 19.8 m/s

Example: Work Against Friction

Problem: A 2 kg block slides 4 m up a 30° incline with friction coefficient μ = 0.3. If it starts with speed 8 m/s, what is its final speed?

Click to reveal solution

Given: m = 2 kg, d = 4 m, θ = 30°, μ = 0.3, v₁ = 8 m/s

Initial energy: E₁ = ½mv₁² = ½(2)(8²) = 64 J

Final energy: E₂ = ½mv₂² + mgh = ½(2)v₂² + 2 × 9.8 × 4 sin(30°) = v₂² + 39.2 J

Work by friction: W_f = -μmg cos(30°) × d = -0.3 × 2 × 9.8 × cos(30°) × 4 = -20.4 J

Apply W-E theorem: E₁ + W_f = E₂ → 64 - 20.4 = v₂² + 39.2 → v₂ = 2.2 m/s

PHYS-1315 Physical Science I | Module 6, Lesson 1

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