Grade 11 Physics • Energy

Analyze Energy Using Conservation Laws — Analyze energy changes using conservation laws

Learn how energy transforms but never disappears, and use conservation laws to solve real-world physics problems.

Grade 11 Physics emblem with an atom, orbital path, and measurement gauge
Inside this lesson 10 sections 5 questions 10 figures

SECTION 1

Historical Context & Motivation

For centuries, people wondered what made things move, heat up, or slow down. Early thinkers believed in mysterious substances like "caloric" — an invisible fluid they thought flowed from hot objects to cold ones. It took generations of careful experimentation before scientists realized that motion, heat, light, and sound are all different faces of one underlying quantity: energy. The discovery that energy can change forms but never be created or destroyed became one of the most powerful ideas in all of science.

1676 • Leibniz and vis viva

Gottfried Wilhelm Leibniz proposed vis viva ("living force"), a quantity proportional to mass times velocity squared. This was an early precursor to our modern concept of kinetic energy.

1843 • Joule's Mechanical Equivalent of Heat

James Prescott Joule showed that mechanical work could be precisely converted into heat. His paddle-wheel experiment demonstrated that a specific amount of work always produced the same amount of heat, linking mechanics and thermodynamics.

1847 • Helmholtz Formalizes Conservation of Energy

Hermann von Helmholtz published a landmark paper proving that energy is conserved across all physical processes. This established the First Law of Thermodynamics and unified mechanics, electricity, and heat under one principle.

1918 • Noether's Theorem

Mathematician Emmy Noether proved that conservation of energy arises from the fact that the laws of physics do not change over time. Her theorem connected symmetry in nature to conservation laws, deepening our understanding of why energy is conserved.

The central question that these discoveries address is deceptively simple: if energy never vanishes, how can we track it as it transforms from one type to another? The law of conservation of energy gives us the tool to do exactly that. By accounting for all energy entering, leaving, and transforming within a system, we can predict speeds, heights, temperatures, and much more — often without needing to know every detail of the forces involved.

SECTION 2

Core Principles & Definitions

Before we can analyze energy changes, we need a clear vocabulary. Energy comes in many forms, but in a typical Grade 11 Physics course, the three you will encounter most often are kinetic energy, gravitational potential energy, and elastic potential energy. Understanding what each one represents and how they relate to conservation of energy is the foundation for solving every problem in this unit.

1

Kinetic Energy (KE)

The energy an object possesses due to its motion. It depends on mass and the square of velocity: KE = ½mv². A car moving at 60 km/h has four times the KE of the same car at 30 km/h.
2

Gravitational Potential Energy (PEgPE_g)

The energy stored in an object because of its height above a reference point. Calculated as PE = mgh, where h is the vertical height. Choosing a consistent reference level (often the ground) is essential.
3

Elastic Potential Energy (PEePE_e)

Energy stored in a stretched or compressed spring. Given by PE = ½kx², where k is the spring constant and x is the displacement from the natural length. The farther you stretch it, the more energy it stores.
4

Conservation of Mechanical Energy

In an isolated system with no friction or air resistance, the total mechanical energy (KE + PE) remains constant. Energy may shift between kinetic and potential forms, but the sum never changes.
5

Work Done by Non-Conservative Forces

When friction or applied forces act, mechanical energy is not conserved by itself. The work-energy theorem accounts for energy added or removed: E_initial + W_non-conservative = E_final.
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KEY TAKEAWAY

Think of energy like money in a bank account with multiple sub-accounts. You can transfer money from savings (potential energy) to checking (kinetic energy), but the total balance stays the same — unless you make a deposit or withdrawal (work by external or friction forces). Conservation of energy is just bookkeeping: if one account goes down, another must go up by exactly the same amount.

SECTION 3

Visual Explanation — Energy on a Roller Coaster

Energy Transformation on a Roller Coasterh = 0 (ref)ABCDPE: maxKE: 0PE: lowKE: highPE: maxKE: ≈0PE: minKE: max
At point A, the coaster starts at the top with maximum PE and zero KE. As it descends to point B, PE converts to KE and the speed increases. At point C (another peak), KE converts back to PE. At the lowest point D, nearly all energy is kinetic, and the coaster reaches its maximum speed. The total mechanical energy at every point remains constant (in the absence of friction).

This diagram captures the essence of conservation of energy in a mechanical system. At any point along the track, you could draw a bar chart showing how the total energy is split between PE and KE, and the total bar height would always be the same. The roller coaster is a perfect classroom example because you can feel the physics: you slow down going up (KE → PE) and speed up going down (PE → KE). Notice that the second hill (point C) cannot be taller than the first hill (point A) if the coaster starts from rest, because there is simply not enough total energy to reach a greater height.

SECTION 4

Mathematical Framework

Now let's put numbers to the concepts. The conservation of energy can be expressed mathematically in different forms depending on whether non-conservative forces (like friction) are present. We'll start with the ideal case and then generalize.

KINETIC ENERGY

KE=½mv2KE = ½mv²

where m is mass in kilograms (kg) and v is speed in metres per second (m/s). Energy is measured in joules (J).

GRAVITATIONAL POTENTIAL ENERGY

PEg=mghPE_g = mgh

where g is the acceleration due to gravity (9.8 m/s²) and h is the vertical height above the chosen reference level.

ELASTIC POTENTIAL ENERGY

PEe=½kx2PE_e = ½kx²

where k is the spring constant in N/m and x is the compression or extension from the spring's natural (equilibrium) length.

CONSERVATION OF MECHANICAL ENERGY (NO FRICTION)

KEi+PEi=KEf+PEfKE_i + PE_i = KE_f + PE_f

The total mechanical energy at the initial state equals the total at the final state. This is valid only when no non-conservative forces do work on the system.

GENERALIZED ENERGY EQUATION (WITH FRICTION OR APPLIED FORCES)

KEi+PEi+Wnc=KEf+PEfKE_i + PE_i + W_nc = KE_f + PE_f

Here W_nc is the net work done by all non-conservative forces. If friction removes energy, Wnc is negative. If an engine adds energy, Wnc is positive.

💡

Choosing a Reference Level

Gravitational PE depends on height, but height is always measured from a reference level that you choose. The reference level is where h = 0. Common choices include the ground, the bottom of a ramp, or the lowest point of a pendulum's swing. The actual choice doesn't matter as long as you use the same reference for every point in the problem — the change in PE is always the same.

SECTION 5

Energy Bar Charts — Tracking Every Joule

One of the most useful tools for analyzing energy is the energy bar chart (sometimes called a LOL chart — "Left, Operator, Left" — because it resembles two bar charts flanking a system description). Energy bar charts let you visualize how each form of energy changes between an initial and a final state. They enforce the conservation principle: the bars on the left plus or minus any work must equal the bars on the right.

Energy Bar Chart: Ball Dropped from 20 mINITIAL STATE (top)FINAL STATE (ground)W_nc = 0KEPE_gPE_eKEPE_gPE_e01960 J01960 J00=Ball at rest, h = 20 mBall at ground, h = 0 mmax0
A 10 kg ball is dropped from 20 m. Initially, all 1960 J of energy is stored as gravitational PE (tall purple bar). At the ground, all of that energy has been converted to kinetic energy (tall cyan bar). The total bar height stays the same because Wnc = 0 (no friction).

Energy bar charts are powerful because they make the conservation law visible. If you add friction, the final total bars would be shorter than the initial total bars, and the difference equals the energy removed by friction (shown as negative Wnc). This visual approach prevents common mistakes like accidentally "creating" energy that was never there in the first place.

SituationEnergy ConversionsW_nc
Ball falling freelyPE → KE0
Skier sliding down with frictionPE → KE + thermal energyNegative (friction removes energy)
Spring launching a ball upwardPE_e → KE → PE_g0 (ideal)
Car braking to a stopKE → thermal energyNegative (brakes remove KE)
Engine accelerating a car up a hillChemical → KE + PEPositive (engine adds energy)

Common energy transformation scenarios and the role of non-conservative work

SECTION 6

Worked Example — Speed at the Bottom of a Ramp

A 5.0 kg box starts from rest at the top of a frictionless ramp that is 3.0 m high. What is the speed of the box when it reaches the bottom of the ramp?

Finding the Speed at the Bottom of a Frictionless Ramp

  1. 1

    Step 1 — Identify Given Values and Define States

    Mass: m = 5.0 kg. Height of ramp: h = 3.0 m. Initial speed: vi = 0 m/s (starts from rest). We set the reference level at the bottom of the ramp, so hf = 0. The ramp is frictionless, so Wnc = 0.
    m = 5.0 kg, h = 3.0 m, vi = 0, Wnc = 0
  2. 2

    Step 2 — Write the Conservation of Energy Equation

    Since there are no non-conservative forces, we use: KEi + PEi = KEf + PEf. Substituting the formulas: ½mvi² + mghi = ½mvf² + mghf.
    ½mv²i + mghi = ½mv²f + mghf
  3. 3

    Step 3 — Substitute Known Values

    Since vi = 0 and hf = 0, the equation simplifies to: 0 + mghi = ½mvf² + 0. Notice that mass m cancels from both sides: gh = ½vf².
    gh = ½vf² → mass cancels!
  4. 4

    Step 4 — Solve for vfv_f

    Rearranging: vf² = 2gh = 2 × 9.8 × 3.0 = 58.8. Taking the square root: vf = √58.8 ≈ 7.67 m/s.
    vfv_f ≈ 7.7 m/s
  5. 5

    Step 5 — Check the Answer

    The answer is independent of mass, which makes physical sense — on a frictionless ramp, all objects reach the same speed at the bottom regardless of mass (just like Galileo's insight). The speed is also reasonable for a 3 m drop. Additionally, the final KE = ½(5.0)(7.67)² ≈ 147 J, which equals the initial PE = (5.0)(9.8)(3.0) = 147 J. ✓ Energy is conserved.
    KEf = PEi = 147 J ✓
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Why Mass Cancels

In problems where only gravity does work and the object starts from rest, the final speed depends only on the height dropped, not on the mass. This is because both KE (½mv²) and PE (mgh) are proportional to mass. This is a powerful shortcut: for any frictionless fall from height h, the speed at the bottom is always v = √(2gh).

SECTION 7

Strengths & Limitations of the Energy Approach

Using conservation of energy is one of the most powerful problem-solving strategies in physics, but like any tool, it has ideal use cases and limitations. Understanding when to use the energy approach versus a force-based (Newton's Laws) approach is an important skill.

FeatureEnergy ApproachForce (Newton's Laws) Approach
Best for finding…Speeds, heights, distances — scalar quantitiesAccelerations, forces, time — vector quantities
Path dependenceWorks regardless of the path taken (for conservative forces)Requires knowing the exact path and forces at each point
Curved or complex pathsEasily handles curved ramps, pendulums, loopsRequires calculus or component analysis on curves
Finding timeCannot directly find time of travelCan determine time using kinematics
Friction / non-conservative forcesHandled by adding W_nc term, but need to know friction force and distanceDirectly calculated through free body diagrams
Mathematical complexityOften simpler — avoids vector componentsCan involve multiple equations and unknowns

Comparing energy and force approaches to problem solving

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WHEN TO USE ENERGY

Use conservation of energy whenever you know something about the starting and ending positions (heights, compressions, speeds) and you want to find an unknown speed, height, or compression — especially when the path is curved or complicated. Think of it as a teleportation trick: you don't care about the journey, only the departure and arrival. If the problem asks about time or acceleration, however, you'll likely need Newton's Laws or kinematics instead.

SECTION 8

Connection to Advanced Topics

Conservation of energy in mechanics is just the beginning. The same principle extends throughout every branch of physics, from circuits to nuclear reactions. In more advanced courses, you'll encounter situations where energy appears to "disappear" — but it hasn't. It has simply converted into forms that are harder to track, like thermal energy, sound, or electromagnetic radiation.

TopicIn This Course (Grade 11)In Advanced Physics
Types of energyKE, gravitational PE, elastic PEAlso thermal, nuclear, electromagnetic, chemical, mass-energy (E = mc²)
Conservation lawMechanical energy conserved (no friction)Total energy always conserved (1st Law of Thermodynamics)
Non-conservative forcesFriction removes mechanical energyEnergy still conserved — converted to thermal energy (entropy increases)
Mathematical toolsAlgebra, square rootsCalculus-based work integrals, Lagrangian and Hamiltonian mechanics
Related conservation lawsIntroduced alongside momentumConnected via Noether's theorem to time-translation symmetry

How conservation of energy extends to advanced physics

One particularly fascinating extension is Einstein's famous equation E = mc², which reveals that mass itself is a form of energy. In nuclear reactions, tiny amounts of mass are converted into enormous amounts of energy, but the total (mass-energy) is still conserved. The principle you are learning right now — that energy is never created or destroyed, only transformed — is truly universal, and mastering it in mechanics gives you a foundation for all of physics.

SECTION 9

Practice Problems

Question 1: CONCEPTUAL

A pendulum swings from its highest point on the left to its highest point on the right. At which point during the swing is the pendulum's kinetic energy at a maximum? Explain your reasoning in terms of energy conservation.
Show answer
The kinetic energy is at a maximum at the lowest point of the swing (the equilibrium position). At the highest points on either side, the pendulum momentarily stops, so KE = 0 and all mechanical energy is stored as gravitational PE. As it swings down, PE converts to KE. At the bottom, h is at its minimum (if we set the reference there, h = 0), so PE is minimized and KE is maximized. By conservation of energy, KEmax = PEmax = mgh, where h is the height of the endpoints above the lowest point.

Question 2: BASIC CALCULATION

A 2.0 kg ball is dropped from rest from a height of 10.0 m. Using conservation of energy (and ignoring air resistance), find the speed of the ball just before it hits the ground. Use g = 9.8 m/s².
Show answer
Using conservation of energy: mgh = ½mv². Mass cancels: gh = ½v², so v² = 2gh = 2 × 9.8 × 10.0 = 196. Therefore v = √196 = 14.0 m/s. The ball strikes the ground at 14.0 m/s. Notice that the 2.0 kg mass did not affect the answer — any object dropped from 10.0 m on a frictionless path reaches the same speed.

Question 3: INTERMEDIATE

A 0.50 kg block slides down a frictionless ramp from a height of 4.0 m. At the bottom of the ramp, it encounters a horizontal surface where friction (μk = 0.40) brings it to a stop. How far does the block slide on the horizontal surface before stopping? Use g = 9.8 m/s².
Show answer
First, find the speed at the bottom of the ramp using conservation of energy: v = √(2gh) = √(2 × 9.8 × 4.0) = √78.4 ≈ 8.85 m/s. Now on the flat surface, the friction force is f = μkmg = 0.40 × 0.50 × 9.8 = 1.96 N. Using the work-energy theorem: the work done by friction equals the loss in KE. So f × d = ½mv², giving d = ½mv² / f = ½(0.50)(8.85)² / 1.96 = 19.6 / 1.96 = 10.0 m. Alternatively, mgh = μkmgd gives d = h / μk = 4.0 / 0.40 = 10.0 m. The block slides 10.0 m.

Question 4: APPLIED

A spring-powered toy launcher has a spring constant of k = 800 N/m. The spring is compressed by 0.15 m and launches a 0.060 kg ball straight up. Ignoring air resistance, how high does the ball rise above the launch point?
Show answer
At the compressed position, the ball has elastic PE = ½kx² = ½(800)(0.15)² = ½(800)(0.0225) = 9.0 J. At the highest point, all this energy has converted to gravitational PE: mgh = 9.0 J. Solving for h: h = 9.0 / (mg) = 9.0 / (0.060 × 9.8) = 9.0 / 0.588 ≈ 15.3 m. The ball rises approximately 15.3 m. This is a great example of energy converting across three forms: elastic PE → KE (during launch) → gravitational PE (at peak), but we only need to compare the first and last states.

Question 5: CRITICAL THINKING

A roller coaster car (mass 600 kg) starts from rest at the top of a 40 m hill. It then goes through a circular loop of radius 10 m (so the top of the loop is 20 m above the ground). (a) Using conservation of energy, find the speed at the top of the loop. (b) Is this speed fast enough to maintain contact with the track? (Hint: at the top of the loop, gravity must provide at least the centripetal force: mg ≤ mv²/r.) (c) What does this tell you about the minimum starting height for a safe loop?
Show answer
(a) Using conservation of energy from the top of the hill (h = 40 m) to the top of the loop (h = 20 m): mgh₁ = ½mv² + mgh₂. Mass cancels: g(40) = ½v² + g(20), so ½v² = g(20) = 196, giving v² = 392, v ≈ 19.8 m/s. (b) At the top of the loop, gravity provides centripetal force. The minimum condition is mg = mv²/r, which means v²min = gr = 9.8 × 10 = 98 m²/s². Since the actual v² = 392 > 98, the car is fast enough and stays on the track. (c) Setting the minimum: g × hmin = ½gr + g(2r) gives hmin = ½r + 2r = 2.5r = 25 m. Any starting height below 25 m would be unsafe because the car would not have enough speed at the top of the loop to maintain contact.

SUMMARY

Summary

Summary

The law of conservation of energy states that energy cannot be created or destroyed — it can only be transformed from one form to another. In mechanics, the three key forms are kinetic energy (KE = ½mv²), gravitational potential energy (PE = mgh), and elastic potential energy (PE = ½kx²). When no non-conservative forces (like friction) act on a system, the total mechanical energy remains constant: KEi + PEi = KEf + PEf.

When friction or applied forces are present, use the generalized equation: KEi + PEi + Wnc = KEf + PEf. The energy approach is especially powerful for problems involving curved paths and variable forces, where Newton's Laws would require complex calculations. Always define a reference level for height, draw an energy bar chart to visualize transformations, and verify your answer by checking that total energy is accounted for.

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