Physics › Mechanics › Conservation of energy
Conservation of energy
Energy is never made and never destroyed, only moved between stores, and two stores dominate mechanics: kinetic and gravitational potential. Add the work done against resistive forces and every mechanics energy problem becomes one and the same calculation.
Pick your board and the few notes written for the other boards quietly fold away, here and in the practice players. Nothing is deleted: every folded piece reopens on a tap.
Builds on Work, energy and power.
IN THIS TOPIC
- State the principle of conservation of energy and use it as an accounting identity.
- Calculate kinetic energy and changes in gravitational potential energy.
- Derive ΔEp = mgΔh from W = Fs, and Ek = ½mv2 from the equations of motion.
- Balance energy budgets that include work done against friction or drag.
COMMON MISCONCEPTION
Energy gets used up.
The principle, and the two big stores
The principle of conservation of energy says energy cannot be created or destroyed, only transferred from one store to another. “Using” energy means moving it somewhere less useful. The total never drops. Mechanics runs almost entirely on two stores, the first being kinetic energy, the energy of motion.
The second is the change in gravitational potential energy when a mass moves through a height.
Respect the square in Ek. Double the speed and the kinetic energy goes up four times, which is the physics sitting underneath every stopping-distance table you were shown at GCSE.
Where the two formulas come from
Neither equation is handed down from nowhere. Both are the work done by a force, , worked through to its destination, and both derivations are short enough to be worth carrying rather than trusting.
Take the potential energy first. To raise a mass m through a height Δh without giving it any speed, you pull upward with a force equal to its weight, mg, and that force acts along the displacement, so W = Fs becomes W = mg × Δh with no angle to worry about. The work you put in is held in the gravitational field and returned in full if the mass is released, so the store gains exactly the work done, . One condition hides inside treating g as a single number, which is that the field must be uniform over the height climbed. Near the Earth's surface it is, and over the height of a mountain it is not quite.
Kinetic energy needs one extra ingredient, the equations of motion. Push a mass m from rest with a constant resultant force F through a distance s. The work done on it is , and Newton's second law turns the F into ma, so W = mas. Now bring in with u = 0, which leaves , so the product as on its own is . Put that back in place of as, and the work done comes out as W = m × ½v2 = ½mv2.
Nothing was lifted and nothing was rubbed, so every joule of that work went into the motion. The energy a mass m carries by virtue of moving at speed v is therefore . The ½ has a definite source, and it is the 2 in 2as. It is not a fudge factor, and a student who has watched it arrive can rebuild the formula when memory fails.
Frictionless exchanges
With no resistive forces, the two stores simply trade. A pendulum converts potential to kinetic on the way down and back again on the way up; a thrown ball does the same in one exchange.
That exchange opens a fast route through problems which would be tedious with forces. Equate mgΔh to ½mv2 and the speeds and heights follow with no force diagram at all. The mass usually cancels, so a heavy pendulum and a light one released from the same height reach the bottom at identical speed.
WORKED EXAMPLE
A pendulum's speed at the bottom
A pendulum bob is pulled aside until it sits 0.20 m higher than its lowest point, then released. Find its speed at the bottom.
Take the energy route. The tension is always perpendicular to the motion and does no work, so every joule of gravitational potential energy becomes kinetic energy.
mgh = ½mv2, and the mass cancels, leaving v = the square root of 2 × 9.81 × 0.20 = 2.0 m s−1.
No mass was given because none was needed. Noticing that before you go hunting for one is the mark of a student who has understood the energy method.
GUIDED PRACTICE
Thrown from a cliff, any direction
A ball is thrown at 12 m s−1 from the top of a 15 m cliff. Using energy conservation, find its speed just before landing, and say why the throwing angle never entered.
Show the working
½mv2 = ½mu2 + mgh, and the mass cancels, leaving v2 = 122 + 2 × 9.81 × 15 = 438.
v = 21 m s−1. Energy is a scalar, so the drop in height fixes the gain in speed whatever direction the throw took. Proving the same thing with projectile SUVAT takes three lines and an angle you were never given.
When friction dissipates energy
Real systems leak, and the leak has a name, work done against resistive forces. Nothing is destroyed. The energy goes to internal energy of the surfaces and the air, warming both. Conservation then reads as a budget with three lines in it.
Energy in equals useful energy out plus energy to the resistive forces, every joule accounted for. Questions run both ways. Give you two lines and ask for the third, or give you all three and ask whether the energy balances. One sentence handles either. Write the stores at the start, write the stores at the end, and let the difference be the work done against resistance.
INDEPENDENT PRACTICE
A braking distance from energy
A 1000 kg car at 25 m s−1 brakes with a constant resistive force of 6.0 kN. Find the stopping distance using the energy route.
Show the working
Work done against the braking force takes all of the kinetic energy, so ½mv2 = Fd.
d = (½ × 1000 × 252)/6000 = 312 500/6000 = 52 m.
Because kinetic energy is proportional to v2, doubling the speed quadruples the initial kinetic energy and, with the same constant braking force, quadruples the stopping distance. Motorway crashes differ from town crashes for exactly that reason.
ASSESSMENT FOCUS
- Open energy questions with the accounting sentence. Energy at the start = energy at the end + work done against resistive forces. That structure carries method marks on its own, before a number appears.
- ΔEp uses the vertical height change. On a slope that is the drop, never the distance travelled along the surface, and it catches people every year.
- “Where did the energy go?” has one acceptable answer, which is transferred to internal energy of the object and its surroundings by the resistive force. “Lost as heat” is tolerated. “Lost” on its own is not.
- The mass often cancels in a pure Ep-to-Ek exchange. Asked why two different masses land at the same speed, that cancellation is the answer.
- CIE examines both derivations by name. For ΔEp, lift at constant speed so the force is mg and quote W = Fs. For Ek, start from W = Fs, put F = ma, then use v2 = u2 + 2as with u = 0 to replace as by ½v2.
CHECK YOURSELF
A child of mass 30 kg starts from rest at the top of a slide 2.5 m high and reaches the bottom at 5.0 m s−1. How much energy was transferred to the surroundings by friction?
Show a hint
Write the budget out. Potential in, kinetic out, and friction takes the difference.
Show the answer
Potential energy given up is = 30 × 9.81 × 2.5 = 736 J.
Kinetic energy gained is = ½ × 30 × 5.02 = 375 J.
The energy has to balance, so friction accounted for 736 − 375 = 361 J, which is 360 J to two significant figures. It is now internal energy in the slide, the child and the air.
Energy is never used up.
It is moved, and you can always audit the move.
WORKBOOK
Printable practice for this topic: original exam-style questions with room to work, and a fully worked answer book. Free to use; please do not redistribute or sell.
Or read them with their mark schemes on the conservation of energy questions page.
CHECK YOUR PROGRESS
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- State the principle of conservation of energy and use it as an accounting identity.
- Calculate kinetic energy and changes in gravitational potential energy.
- Derive ΔEp = mgΔh from W = Fs, and Ek = ½mv2 from the equations of motion.
- Balance energy budgets that include work done against friction or drag.
Open the full revision checklist to track your progress across the whole unit.