In simple terms
A friendly intro before the formal notes — no formulas yet.
Energy conservation
Cambridge 9702 Paper 2 — Energy conservation (5.1). Senpai Corner diagram-backed pilot with premium structure and live visuals.
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5.1 Energy conservation.
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In physics, work (W) is the energy transferred to or from an object through the application of force (F) along a displacement (d) 𝑊 = 𝐹 × 𝑑.
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The SI units for work is in Joules.
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The principle of conservation of energy states that energy is neither created nor destroyed. But may transform from one type to another .
What this topic covers
The official Cambridge syllabus points this lesson works through.
- 5.1.1
Understand the concept of work, and recall and use work done = force × displacement in the direction of the force
- 5.1.2
Recall and apply the principle of conservation of energy
- 5.1.3
Recall and understand that the efficiency of a system is the ratio of useful energy output from the system to the total energy input
- 5.1.4
Use the concept of efficiency to solve problems
- 5.1.5
Define power as work done per unit time
- 5.1.6
Solve problems using
- 5.1.7
Derive and use it to solve problems
Explore the concept
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Key formulas
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$GPE = mgh \text{ or } \Delta GPE = mg\Delta h$
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$Efficiency = \frac{\text{Useful Energy Output}}{\text{Total Energy Input}} = \frac{\text{Useful Power Output}}{\text{Total Power Input}}$
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Full topic notes
Formal explanation with the rigour you need for the exam.
The Unbreakable Rule: Conservation of Energy
At its core, the Principle of Conservation of Energy states that energy can neither be created nor destroyed. Instead, it continuously changes from one form to another. In a closed system, where no energy can enter or leave, the total amount of energy always stays constant.
5.1 Energy conservation.
In physics, work (W) is the energy transferred to or from an object through the application of force (F) along a displacement (d) 𝑊 = 𝐹 × 𝑑.
The SI units for work is in Joules.
The principle of conservation of energy states that energy is neither created nor destroyed. But may transform from one type to another .
E.g. work can be transformed to heat (friction!), electric to light.
Not all energy transferred is useful. E.g. when transferring electric to light, some energy is wasted in the form of heat!.
Energy's Many Forms: Kinetic and Gravitational Potential
Two crucial forms of energy we frequently encounter are Kinetic Energy (KE) and Gravitational Potential Energy (GPE). KE is the energy an object possesses due to its motion, while GPE is the energy stored due to its position in a gravitational field.
Kinetic energy depends on an object's mass () and the square of its velocity (). The faster or more massive an object, the more kinetic energy it has.
$GPE = mgh \text{ or } \Delta GPE = mg\Delta h$
Gravitational potential energy depends on mass (), gravitational acceleration (), and vertical height (). You can choose any convenient reference point for 'h', as only the change in height matters for .
Kinetic energy is related to an object's movement.
GPE is energy stored by an object's height in a gravitational field.
KE is proportional to mass and the square of velocity.
GPE depends on mass, gravity, and vertical height change.
The GPE reference height can be set arbitrarily.
Work, Power, and Efficiency: Energy in Action
When energy is transferred, we call it work done. Work is done when a force causes an object to move a certain distance. Think of pushing a box across a floor – you're doing work on it. If the force and displacement are in the same direction, the calculation is simple:
What if the force is not in the same direction as the displacement? For example, pulling a suitcase with a handle at an angle. In this case, only the component of the force that acts in the direction of motion does work. We use the formula:
Here, is the angle between the force vector and the displacement vector. If the force is perpendicular to the displacement (), then , and no work is done. This is why the gravitational force does no work on an object moving horizontally.
Power is how quickly this energy transfer or work happens. A powerful engine can do a lot of work in a short amount of time, indicating a high rate of energy transfer.
The formula is particularly useful for objects moving at a constant velocity against a constant force . It's derived from and knowing that for constant velocity.
Finally, efficiency tells us how effectively a system converts input energy into useful output energy. No real system is 100% efficient because some energy is always 'lost' to unwanted forms, typically heat or sound. For example, an electric motor lifting a mass gains useful GPE, but some input electrical energy is wasted as heat in the motor's coils and sound from its operation.
$Efficiency = \frac{\text{Useful Energy Output}}{\text{Total Energy Input}} = \frac{\text{Useful Power Output}}{\text{Total Power Input}}$
Work done is energy transferred by a force causing displacement.
Use when force and displacement are at an angle .
Power measures the rate of energy transfer or work done.
For constant velocity, power can be calculated as .
Efficiency compares useful output energy/power to total input energy/power.
Real systems always have efficiency less than 100% due to energy losses.
Worked examples
See the formulas applied — reveal one step at a time, like the exam.
A 2.0 kg ball is dropped from a height of 5.0 m. (a) Calculate its gravitational potential energy at the start. (b) Assuming no air resistance, calculate its speed just before hitting the ground. (c) If, due to air resistance, its actual speed just before hitting the ground is 8.5 m/s, calculate the work done against air resistance. (Take ).
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(a) Initial GPE: $GPE = mgh = 2.0 \text{ kg} \times 9.81 \text{ m/s}^2 \times 5.0 \text{ m} = 98.1 \text{ J}$.
A car of mass 1200 kg travels at a constant speed of 18 m/s up a road inclined at 6.0° to the horizontal. The car's engine works at a constant rate of 45 kW. (a) Calculate the work done against the gravitational force in 10 seconds. (b) Calculate the total work done by the engine in 10 seconds. (c) Determine the magnitude of the total resistive force acting on the car. (Take ).
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(a) First, find the vertical height gained in 10 seconds.
How it all connects
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Tap a linked idea to see how it connects back to the main topic — that connection is what examiners reward.
Glossary
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Quick check
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Revision flashcards
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What is the fundamental principle of energy conservation in a closed system?
Energy cannot be created or destroyed, only transformed, so the total energy remains constant.
Key takeaways
Review these before you close the topic — retrieval beats re-reading.
- ✓
5.1 Energy conservation.
- ✓
In physics, work (W) is the energy transferred to or from an object through the application of force (F) along a displacement (d) 𝑊 = 𝐹 × 𝑑.
- ✓
The SI units for work is in Joules.
- ✓
The principle of conservation of energy states that energy is neither created nor destroyed. But may transform from one type to another .
- ✓
E.g. work can be transformed to heat (friction!), electric to light.
- ✓
Not all energy transferred is useful. E.g. when transferring electric to light, some energy is wasted in the form of heat!.
Practice — then mark it
The whole point: a real Cambridge question, marked mark-by-mark.
9702/22 · Q3(b)
The potential difference between the ground and the atmosphere is 3.0 × 10^7 V.
Calculate the average power, in GW, transferred during the lightning strike.
power = ................................................................ GW [2]
9702/23 · Q3(d)
Determine an estimate of the work done on the sample as it is extended from zero extension to its breaking point. Explain your reasoning.
Extra simulations & links
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Frequently asked
Checkpoint
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Reading it isn’t knowing it — prove it.
Before you move on: do 9702/22 · Q3(b) on paper, snap a photo, and get examiner-style feedback on exactly where you win and lose marks.