We read the actual Pearson Edexcel Physics Paper 1 Higher Tier papers and mark schemes for June 2022 and June 2023, since June 2019 is no longer published on Pearson's own site. Below is what each real topic has actually asked, exactly as it was worded, and a complete worked answer written to the top of the real mark scheme for every sitting we have. Use this to see exactly how full marks are earned, not a generic revision summary.
Questions quoted for analysis. Diagrams and figures described in our own words, not reproduced. Mark scheme content translated into plain English, never copied. PrepWise is independent and not endorsed by Pearson Edexcel.
This slot appeared in June 2022 as a full lens question. It combines a quick multiple choice recall point with two real calculations using given equations.
It wants you to apply the total internal reflection angle rule, read heights off a ray diagram to calculate magnification, and substitute given distances into the lens equation to find focal length.
A ray diagram showing a converging lens used as a magnifying glass, with an object placed inside the focal length, an upright enlarged virtual image formed on the same side as the object, and the two focal points marked.
A converging lens with an object 20cm from the lens on one side and a real image forming on a translucent screen 40cm from the lens on the other side.
Ray diagram B shows total internal reflection at the air and glass boundary. This is because total internal reflection only happens when light travels from a denser material into a less dense material, so the ray must be going from glass into air, and it must reflect back into the glass at the same angle it hit the boundary at, rather than crossing over and bending into the air.
Reading the heights straight off Figure 1, the image height is about 18mm and the object height is about 7mm, so magnification = 18 / 7 = 2.6.
One way to increase the magnification would be to use a different lens with a shorter focal length. A lens with more curved surfaces has a shorter focal length and a higher power, so it bends the light rays more strongly, which produces a bigger virtual image for the same object position.
For the focal length, I substitute a = 20 and b = 40 into 1/f = (a + b) / (a x b), which gives 1/f = 60 / 800 = 0.075. Flipping this gives f = 1 / 0.075 = 13.3cm, which rounds to 13cm.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise lenses and images questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
What does a convex (converging) lens do to parallel rays of light?
Lens questions always mix a quick recall point with real calculations using the given equations, so practise reading ray diagrams and substituting carefully.
Practise lenses and images questionsThis slot appeared in June 2022 combining a recall multiple choice question with a full practical design and a graph description.
It tests whether you know energy is conserved in a closed system, can design a fair insulation comparison using nested copper cans, and can read a graph to describe a non-linear trend in thermal conductivity.
A small copper can nested inside a larger copper can, with sand and sawdust shown as the two insulating materials to be tested.
A graph plotting thermal conductivity of expanded polystyrene, in mW per metre kelvin, against its density, in kg per cubic metre, showing a curve that falls steeply then flattens out.
Conservation of energy in a closed system means that when there are energy transfers, the total amount of energy stays the same, it does not increase or decrease. To compare sand and sawdust as insulators fairly, I would set up two identical small copper cans of hot water, each placed inside a larger copper can, packing sand around one small can and sawdust around the other, with a thermometer in each water sample and a stop clock timing how the temperature falls. To make it a fair test I must control the mass of water used, the mass or volume of insulating material packed around each can, the starting temperature of the water, and the time interval or temperature change I compare between the two set ups.
Reading Figure 4, as the density of expanded polystyrene increases, its thermal conductivity decreases, but not at a steady rate: the graph falls steeply at low densities and then the rate of decrease slows down, until the curve levels off and thermal conductivity becomes almost constant at higher densities.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise heat transfer questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
Which method of thermal energy transfer occurs mainly in solids?
Insulation practicals always test fair test thinking as much as the physics itself, so practise naming genuinely different control variables.
Practise heat transfer questionsThis slot appeared in June 2022 linking road safety reasoning to two real speed and time calculations.
It wants a linked explanation of why wet weather needs lower speeds, a unit conversion to compare two speeds, and a rearrangement of distance = speed x time.
A European motorway speed limit sign showing 130 km/h in dry conditions and a lower 110 km/h limit in wet weather.
Driving slower in wet weather is safer because wet roads give less grip between the tyres and the road, so braking distance increases in the wet compared to dry conditions, meaning a slower speed keeps the overall stopping distance shorter and reduces the risk of skidding or losing control.
To compare 31 m/s with 130 km/h, I convert 130 km/h into metres per second: 130 000 m divided by 3600 s gives about 36.1 m/s. Since 31 m/s is less than 36.1 m/s, this confirms 31 m/s is indeed a lower speed than 130 km/h. For the reaction time, distance travelled = speed multiplied by time, so 46 = 31 multiplied by t, giving t = 46/31 = 1.483 seconds, which rounds to 1.5 seconds to two significant figures.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise stopping distances questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
What is the correct definition of stopping distance?
Stopping distance explanations always want two linked ideas, so practise pairing cause and effect rather than listing single facts.
Practise stopping distances questionsThis half-life reasoning appeared in June 2022 as a medical tracer question, and in June 2023 as a graph plotting question, so both real skills are covered here.
It wants you to know gamma is the radiation type that escapes the body to reach an external detector, and that a suitable tracer's half-life must roughly match how long the scan itself takes.
Gamma radiation is the type that travels from the kidney to the scanner, since gamma can pass out through body tissue, unlike alpha or beta radiation which are absorbed inside the body before they could reach an external detector. A half-life of about 6 minutes is not suitable because the isotope would decay away too quickly to still be giving off enough radiation for readings to be taken throughout the whole 30 minute scan. A half-life of about 6 days is not suitable because the isotope would stay radioactive inside the patient's body for far longer than necessary, giving an unnecessarily high radiation dose long after the scan itself has finished.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise half-life questionsIt is testing whether you understand that activity halves every time one half-life passes, and can apply that repeatedly to plot new points.
A blank grid with activity in Bq on the vertical axis up to 140 and time in seconds on the horizontal axis up to 80, with the starting point at 128 Bq already plotted at time zero.
Starting at 128 Bq at time zero, one half-life of 17s later the activity halves to 64 Bq, so I plot a point at 17 seconds, 64 Bq. After another 17s, at 34s, the activity halves again to 32 Bq, giving a point at 34 seconds, 32 Bq. After a third half-life, at 51s, the activity halves once more to 16 Bq, giving a point at 51 seconds, 16 Bq, and I would join these points with a smoothly decaying curve rather than straight lines.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise half-life questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
What is the definition of half-life?
Half-life questions test both the words, why a half-life suits a use, and the maths, halving activity again and again, so practise both.
Practise half-life questionsThis appeared in June 2022 as a short two-method recall question about protecting the technician carrying out the scan.
It wants two genuinely different, named ways of protecting a radiation worker.
Two ways of reducing the technician's radiation risk are using shielding, such as standing behind a lead barrier or lead screen, and limiting the time spent close to the radioactive source, for example by leaving the room during the scan or using tongs to keep the source at a distance rather than holding it directly.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise uses and hazards of radiation questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
Which type of radiation is used in smoke detectors?
Radiation safety questions always want two named, genuinely different methods, so practise the time, distance and shielding framework.
Practise uses and hazards of radiation questionsA shorter version of this reasoning appeared in June 2022 as a 6 mark reactor mechanics question, then in June 2023 the same core idea became the paper's full 6 mark Level of Response question, alongside a separate mass and energy calculation.
It wants an explanation of how control rods reduce fission rate, a straightforward percentage calculation, and a description of the energy pathway from fission to the next stage of electricity generation.
A labelled diagram of a nuclear reactor showing control rods, a shield, nuclear fuel, a moderator, a reactor vessel and coolant flowing in and out.
Pushing the control rods further into the reactor slows the chain reaction because the rods absorb neutrons, so fewer neutrons are left available to go on and cause further fission reactions in the uranium fuel. For the percentage calculation, I divide the slow neutron speed by the fast neutron speed and multiply by 100: (4.0 x 10^3 divided by 3.0 x 10^7) multiplied by 100 = 0.013%, showing the slow neutrons move only a tiny fraction as fast as the fast ones. Energy is transferred from the nuclear reaction as kinetic energy of the fission fragments, which is then transferred as thermal energy to the coolant flowing through the reactor, ready to be carried on to boil water and drive a turbine.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise nuclear fission and fusion questionsIt is testing rearranging energy released = change in mass x (speed of light) squared to find the tiny mass converted to energy in one fission.
A diagram of nuclear fission showing a free neutron striking a uranium nucleus, which splits into two smaller nuclei while releasing three free neutrons.
Rearranging energy released = change in mass multiplied by the speed of light squared gives change in mass = energy released divided by the speed of light squared, so change in mass = 1.49 x 10^-10 divided by (3.00 x 10^8)^2 = 1.49 x 10^-10 divided by 9 x 10^16, which evaluates to about 1.66 x 10^-27 kg, an extremely small mass converted straight into the energy released.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise nuclear fission and fusion questionsIt wants a full explanation of how one fission's released neutrons build into a chain reaction, and how control rods and the moderator between them let operators manage exactly how much energy is released.
A single uranium fission only releases a tiny amount of energy, but each fission also releases two or three free neutrons, and it is these neutrons that let the reactor produce large amounts of energy overall. If a released neutron goes on to hit another uranium nucleus, it can cause that nucleus to split as well, releasing more neutrons in turn, and this becomes a self sustaining chain reaction where the number of fissions happening every second keeps building, so instead of one isolated fission the reactor has millions of fissions happening continuously, and it is this huge number of fissions, not the size of any single one, that produces enough energy to supply thousands of homes.
Left completely uncontrolled, this chain reaction would keep accelerating, so the reactor uses control rods to manage exactly how many fissions happen each second. The control rods are made of a material that absorbs neutrons, so when they are pushed further into the reactor core they capture more of the free neutrons released by fission before those neutrons can reach another uranium nucleus. This directly reduces the number of fissions taking place, which slows the rate of energy release, and pulling the control rods back out allows more neutrons through to cause fissions, increasing the rate of energy release again. This is exactly how the reactor is able to track changing demand for electricity, since operators can raise or lower the control rods to increase or decrease power output as needed.
The reactor also contains a moderator, usually water or graphite, which plays a different role from the control rods. Neutrons released directly from fission travel too fast to reliably cause another fission, so the moderator slows these fast neutrons down through collisions, and slower neutrons are far more likely to be captured by a uranium nucleus and cause it to split. Without the moderator the chain reaction would not sustain itself efficiently even with the control rods withdrawn, so the moderator and the control rods work together, one making fission likely, the other limiting how often it is allowed to happen.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise nuclear fission and fusion questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
What is nuclear fission?
Reactor control questions always want chain reaction, control rods and moderator explained together, not just named, so practise linking all three.
Practise nuclear fission and fusion questionsThe equations of motion recur across both sittings, in an aircraft take-off calculation in 2022, a falling stone calculation in 2023, and a full velocity time graph question in 2023.
It wants acceleration from a change in velocity over time, then distance from the equations of motion, then a sensible real-world reason for a safety margin.
Acceleration = change in velocity divided by time, so a = (82 minus 0) divided by 36 = 2.3 m/s^2, which is about 2 m/s^2 as the question asks me to show. Using v squared minus u squared = 2 times a times x, I rearrange to x = (82 squared minus 0 squared) divided by (2 multiplied by 2.3), giving a distance of about 1500 m. The actual runway is always longer than this calculated distance because it needs a safety margin, for example in case the take-off has to be aborted or the aircraft is carrying a heavier load or worse weather conditions on another flight.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise forces and effects questionsAnother equations of motion question, this time using acceleration due to gravity for a falling object starting from rest.
Using v squared minus u squared = 2ax with the stone's acceleration equal to gravity, 10 m/s^2, I substitute 17 squared minus 0 squared = 2 multiplied by 10 multiplied by distance, giving distance = 289 divided by 20 = 14.45 m, which rounds to 14.5 m.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise forces and effects questionsIt is entirely about reading a velocity time graph: identifying a flat zero section, reading a peak value, finding a gradient for acceleration, and finding an area for distance.
A velocity time graph for a lift, rising to 4 m/s then flat, falling to zero, resting, rising again to a higher plateau of about 4.6 m/s, then falling back to zero just before 16 s.
The lift is at rest, meaning its velocity is zero, for 3.0 s during the first 16 s. I get this by reading the length of the flat section of the line that sits exactly on the time axis, where the graph shows no rise or fall in velocity at all.
Using the graph in Figure 8, the maximum velocity during the first 16 s is 4.6 m/s. I read this straight off the height of the second, higher flat section of the line, which sits above the first plateau.
For the acceleration during the first 1.4 s, I read the data point where the line reaches 4 m/s at 1.4 s, starting from (0, 0) where the lift begins moving. Acceleration is the gradient of a velocity time graph, so acceleration equals change in velocity divided by time, which is 4 divided by 1.4, giving 2.9 m/s squared.
To find the distance travelled in the first 6.0 s, I worked out the area under the graph up to that point. I split the shape into a rising triangle, a flat rectangle and a falling triangle: half of 1.4 multiplied by 4, plus 3.6 multiplied by 4, plus half of 1 multiplied by 4. That gives 2.8 plus 14.4 plus 2.0, which is 19.2 m, rounding to 19 m.
At 18 s the lift starts to move downwards. I would sketch a straight line starting exactly at the point (18, 0) on the graph and sloping downward from there into negative velocity values, showing the speed building up gradually rather than dropping instantly. I would not draw a vertical line down at 18 s, and I would not extend this new line back to before 18 s, since the lift is still shown at rest right up until that point.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise forces and effects questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
What is a force?
Motion equation and graph questions reward showing every step of working, so practise rearranging before substituting every time.
Practise forces and effects questionsThis exact calculation appeared in both sittings, once for a landing aircraft and once for a kicked football.
A direct substitution into the kinetic energy equation, followed by naming a real transfer pathway for that energy.
Kinetic energy = half multiplied by mass multiplied by velocity squared, so KE = 0.5 multiplied by 3.6 x 10^5 multiplied by 71 squared, which evaluates to about 9.1 x 10^8 J. As the aircraft comes to a stop, this kinetic energy is transferred to the surroundings mechanically through friction in the brakes and tyres, and thermally as heating due to air resistance.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise kinetic energy questionsA repeat of the same equation with different numbers, for a kicked football.
Kinetic energy = half multiplied by mass multiplied by velocity squared, so KE = 0.5 multiplied by 0.42 multiplied by 12 squared, which evaluates to 30 J.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise kinetic energy questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
Which of the following objects has kinetic energy stored in its kinetic energy store?
Kinetic energy calculations are near guaranteed marks if you square the velocity first, so practise this exact substitution until it is automatic.
Practise kinetic energy questionsRed shift and Big Bang evidence appeared as a full multi-part question in June 2022 and returned as two shorter linked parts in June 2023.
It wants recall of which theory each piece of evidence supports, two calculations using the red shift and recession velocity equations, and an explanation of why satellite telescopes avoid the limitations of ground based ones.
Two hydrogen spectra shown as bands from blue to red, one measured on Earth and one from a distant galaxy, with a labelled spectral line X shifted further towards the red end in the galaxy's spectrum.
Both red shift and cosmic microwave background radiation are explained by the Big Bang theory, since the Steady State theory cannot account for the cosmic microwave background at all, so the correct row of the table links Big Bang to both pieces of evidence. Using z = (wavelength from galaxy minus wavelength on Earth) divided by wavelength on Earth, z = (6.72 x 10^-7 minus 6.56 x 10^-7) divided by 6.56 x 10^-7, which evaluates to about 0.024, close to the 0.025 the question asks me to show. Using recession velocity = z multiplied by speed of light, v = 0.024 multiplied by 3.00 x 10^8, giving a recession velocity of about 7.2 x 10^6 m/s.
The more distant galaxy has an even longer measured wavelength, 6.92 x 10^-7 m, giving a bigger red shift value, which means that galaxy is moving away from Earth at an even higher recession velocity. Since more distant galaxies show larger red shifts and higher recession velocities, this shows that the further away a galaxy is, the faster it is moving away from us, which is exactly the pattern you would expect if the whole Universe is expanding in every direction. Some telescopes are placed on satellites in orbit because, above the Earth's atmosphere, there is no interference from dust, clouds or light pollution, and satellites can detect wavelengths such as infrared, ultraviolet and X-rays that are absorbed by the Earth's atmosphere before they would ever reach a ground based telescope.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise space topic questionsIt wants the same red shift reasoning applied without a numerical calculation, plus reading a typical wavelength value straight from a table.
A table listing typical wavelengths for each region of the electromagnetic spectrum, from gamma rays at 1.0 x 10^-12 m up to radio waves at 50 m, including microwaves at 1.0 mm.
| Type of radiation | Typical wavelength |
|---|---|
| Gamma rays | 1.0 × 10⁻¹² m |
| X-rays | 3.0 × 10⁻¹¹ m |
| Ultraviolet | 200 nm |
| Visible | 600 nm |
| Infrared | 4.0 μm |
| Microwaves | 1.0 mm |
| Radio waves | 50 m |
The wavelength of light detected on Earth from distant galaxies is longer, red shifted, than the wavelength that was actually emitted, and this stretching of the wavelength shows that the galaxies emitting that light are moving away from Earth, which is only possible if the space between galaxies is itself expanding. Using the table of typical radiation wavelengths, cosmic microwave background radiation has a typical wavelength of about 1.0 mm, since it falls within the microwave part of the electromagnetic spectrum.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise space topic questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
What is the orbital period of a geostationary satellite?
Red shift questions always want the wavelength change linked all the way through to universal expansion, so practise the full chain of reasoning, not just the calculation.
Practise space topic questionsThis life cycle of stars reasoning appeared in June 2023 as a two part recall question.
It wants gravity named as the cause of collapse, then a linked explanation of how nuclear fusion starting balances that gravity and stabilises the star.
A nebula collapses because of the gravitational attraction pulling its particles of gas and dust together. As the nebula keeps collapsing, the increasing gravity raises the temperature and pressure at the centre until it becomes hot enough for nuclear fusion to begin, turning hydrogen into helium. Once fusion starts, the outward push from the energy released by fusion balances the inward pull of gravity, and it is this balance that stops the star collapsing any further, keeping it stable as a main sequence star.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise space topic questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
The light from a distant galaxy is red-shifted. What does this tell us about the galaxy?
Star formation questions want gravity and fusion linked together as a balance, so practise explaining the whole cycle, not just naming the two forces.
Practise space topic questionsJune 2022 asked for a full investigation design testing conservation of momentum, while June 2023 tested the same equation directly as a calculation.
It wants the correct unit of momentum, a logically ordered investigation measuring momentum before and after a sticky collision, and the reason a sloped runway compensates for friction.
Two identical trolleys on a sloped runway, trolley A carrying a card and fitted with sticky pads facing trolley B, ready to collide and stick together.
The unit of momentum is kg m/s, since momentum is mass multiplied by velocity. To investigate conservation of momentum, I would first weigh both trolleys, then use a light gate connected to a data logger to measure the velocity of trolley A as it travels down the runway on its own before the collision. The trolleys are fitted with sticky pads so that when trolley A hits trolley B they stick together, and a second light gate further down the runway measures the combined velocity of both trolleys straight after the collision. I would then calculate the total momentum before the collision, mass of A multiplied by its velocity, and the total momentum after, the combined mass multiplied by the combined velocity, and check whether these two values are equal. I would repeat this several times and take an average to reduce the effect of timing errors.
The runway is set at a slope to compensate for friction, so that trolley A travels at a constant speed before reaching trolley B rather than gradually slowing down, which would make the momentum comparison inaccurate.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise momentum questionsA direct substitution into momentum = mass x velocity, this time with a very small atomic mass.
Momentum = mass multiplied by velocity, so momentum = 6.6 x 10^-26 multiplied by 480, which evaluates to about 3.2 x 10^-23 kg m/s.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise momentum questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
What is the equation for momentum?
Momentum questions swing between full investigation designs and direct calculations, so practise both the words and the maths.
Practise momentum questionsBoth sittings tested exactly the same reasoning: a collision where the object reverses direction, so the change in momentum adds the two magnitudes together rather than subtracting them.
It wants force = change in momentum divided by time, applied carefully to a ball that reverses direction on impact.
A tennis racket with the ball shown travelling towards it at 8.2 m/s and travelling away from it at 15 m/s after being hit.
Taking the direction the ball is hit back in as positive, F = (mass multiplied by final velocity minus mass multiplied by initial velocity) divided by time = (0.075 multiplied by 15 minus 0.075 multiplied by negative 8.2) divided by 0.012, which evaluates to about 145 N, since the ball's velocity has reversed direction the two momentum terms add together rather than cancel out.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise impulse and collisions questionsThe same reversed direction reasoning as the racket question, applied to a ball bouncing off a wall.
A ball travelling towards a wall before the collision and travelling away from the wall in the opposite direction after the collision.
Since the ball's momentum reverses direction, the change in momentum is the sum of the two magnitudes rather than their difference: change in momentum = 0.80 plus 0.60 = 1.4 kg m/s. Using force = change in momentum divided by time, with 70 ms converted to 0.070 s, force = 1.4 divided by 0.070 = 20 N.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise impulse and collisions questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
Which equation correctly defines impulse?
Force from momentum change questions almost always involve a reversal of direction, so practise spotting when to add rather than subtract.
Practise impulse and collisions questionsJune 2022 tested a short Newton's third law application, while June 2023 turned Newton's second law into the paper's full 6 mark Level of Response investigation question.
It wants Newton's third law force pair features applied specifically to the racket and ball, not a generic statement of the law.
Newton's third law applies here because the force the racket exerts on the ball and the force the ball exerts back on the racket are equal in size and opposite in direction, and they act on two different objects, the racket and the ball, rather than both acting on the same object, with both forces being the same type of contact force.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise Newton's laws questionsIt wants a full, ordered procedure showing how to change the force on a trolley while keeping mass constant, and how to measure acceleration accurately for each force.
A trolley on a runway resting on a bench, with a pulley implied at the end of the runway for attaching a hanging weight.
First I would set up the runway on a slight slope and let the trolley run down it on its own with no weights attached, adjusting the angle of the slope until the trolley travels at a constant speed. This step compensates for friction, so that any acceleration I measure later is caused only by the force I add, not by friction slowing the trolley down. I would then attach a length of string over a pulley at the end of the runway, with a weight hanger hanging from the other end, and place some slotted weights both on the hanger and on the trolley itself, since I need a way of changing the accelerating force without changing the total mass of the whole system.
To measure the acceleration, I would attach a card of known length to the trolley and set up two light gates connected to a data logger at fixed points along the runway, which record the time the card takes to pass through each gate and the time between the two gates. From these readings the data logger can calculate the trolley's velocity at each gate and the time taken to travel between them, and I can use acceleration = change in velocity divided by time to find the acceleration for that run.
For each reading I would move one or more slotted weights from the trolley onto the hanger, one at a time, which increases the accelerating force while keeping the total mass of the trolley and weights system exactly the same, and repeat the timing for each new force. I would repeat every measurement at least twice more and take an average of the acceleration at each force, to reduce the effect of random timing errors, then finally plot a graph of force against acceleration for all my results.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise Newton's laws questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
According to Newton's First Law, what happens to an object when there is no resultant force acting on it?
Newton's second law investigations always need friction compensated first and total mass kept constant, so drill this exact sequence.
Practise Newton's laws questionsThis full alpha scattering question appeared in June 2022, combining an estimation calculation, a graph ratio, the full nuclear model explanation, and an evaluation of a marble analogy model.
It wants an estimate calculation, a ratio read from a log scale graph, the full reasoning link from scattering pattern to nuclear model, and evaluation of a marble analogy model.
The Rutherford scattering apparatus: an alpha particle source firing a beam through thin gold foil at the centre of a circular fluorescent detector screen, with most particles detected straight ahead.
A graph on a logarithmic vertical scale showing the number of scattered particles detected falling steeply from around 10 to the 7th at small scattering angles down to around 10 squared at large angles.
A marble rolled down a slope towards a fixed circular weight sitting on a large sheet of paper marked with a grid of lines one centimetre apart.
To estimate how many gold atoms fit across the foil, I divide the foil thickness by the diameter of one atom: 4.0 x 10^-7 divided by 0.15 nm, which is 4.0 x 10^-7 divided by 1.5 x 10^-10, giving about 2700 atoms. Reading the graph, at 5 degrees roughly 10 to the power 6.5 particles were detected and at 100 degrees only about 10 squared were detected, giving a ratio of around 10 to the power 4.5 to 1, somewhere between 10 000 to 1 and 100 000 to 1.
This huge difference in scattering is the key evidence for the nuclear model of the atom. Most alpha particles pass straight through the gold foil with little or no deflection, which shows that atoms are mostly empty space. A small number are scattered through small angles, showing there must be something inside the atom that can repel a positively charged alpha particle. A very small number, matching that low count at 100 degrees, are scattered through large angles or even bounce straight back, which can only happen if they hit something small, dense and positively charged concentrated at the centre of the atom, the nucleus.
To model this scattering, the students could roll marbles down the slope towards the fixed circular weight on the sheet of paper, and record where each marble ends up or measure the angle each marble deflects through, comparing the pattern to the real alpha scattering data. One real limitation of this marble model is that the marble carries no electrical charge, so it cannot represent the electrostatic repulsion between the positive alpha particle and the positive nucleus that actually causes the deflection in the real experiment.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise atomic structure questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
What does the atomic number of an element tell you?
Alpha scattering questions want every observation linked to its own conclusion about atomic structure, so practise the three way link, not just describing the results.
Practise atomic structure questionsJune 2022 built a full multi-part electromagnetic spectrum question ending in the paper's other 6 mark Level of Response question, while June 2023 asked for two more brief examples of waves transferring energy.
It wants recall linking frequency to danger, two straightforward calculations, and a full comparison of X-rays and radio waves covering both their uses and how each is actually produced.
The potential danger from waves in the electromagnetic spectrum increases as frequency increases, since higher frequency waves such as ultraviolet, X-rays and gamma rays carry more energy and become ionising, unlike the low frequency, low energy waves such as radio waves and microwaves.
For the microwave oven's wavelength, using wave speed = frequency multiplied by wavelength, wavelength = speed divided by frequency = 3.00 x 10^8 divided by 2.45 x 10^9, which evaluates to about 0.12 m. For the total energy supplied, using efficiency = useful energy transferred divided by total energy supplied, total energy supplied = 42 000 divided by 0.55, which evaluates to about 76 000 J.
X-rays sit at the high frequency, short wavelength end of the electromagnetic spectrum, which makes them highly ionising and high in energy. Because of this, hospitals use X-rays to image broken bones and damaged lungs, since X-rays pass through soft tissue but are absorbed more by dense bone, producing a shadow picture on a detector. The same high energy lets X-rays treat cancer directly in radiotherapy, and airport security scanners use them to see through luggage. Radio waves sit at the opposite end of the spectrum, with low frequency, long wavelength and low energy, so they are not ionising. This makes them safe for everyday use in broadcasting television and radio, in mobile phone communication, in satellite transmissions and in radar.
The key difference the question is really testing is how these two radiations are actually produced, not just where they sit in the spectrum. X-rays are emitted when electrons inside an atom absorb energy and jump up to a higher energy level, then almost immediately fall back down to a lower energy level. As an electron drops back down it has to lose a large amount of energy, and because atoms can only lose energy in fixed amounts, that lost energy is released as a single high energy photon, which is an X-ray. Radio waves are produced completely differently, through electrons oscillating in an electrical circuit rather than jumping between fixed energy levels inside an atom. An alternating current makes electrons flow back and forth up and down a transmitting aerial, and this oscillating movement of charge generates radio waves in the space around the aerial, with the frequency of the radio wave produced matching the frequency at which the electrons oscillate in the circuit.
So although X-rays and radio waves are both electromagnetic waves that travel at the speed of light and transfer energy without needing a medium, they sit at opposite extremes of frequency and energy, they are used for very different purposes because of that energy difference, and critically they come from two entirely different electron behaviours: energy level transitions inside atoms for X-rays, against oscillating current in a circuit for radio waves.
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Practise electromagnetic spectrum questionsIt wants two named electromagnetic waves other than light, each with a genuine, specific description of how they transfer energy.
Microwaves transfer energy by increasing the kinetic energy of vibration of water molecules, which is how a microwave oven heats food. Infrared radiation transfers energy by heating the skin, which is how a thermal imaging camera or an electric heater works, and can also cause skin burns at high enough intensity.
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Practise electromagnetic spectrum questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
What is the speed of all electromagnetic waves in a vacuum?
X-rays versus radio waves questions always want both uses and both production mechanisms, so practise explaining electrons in atoms versus electrons in circuits.
Practise electromagnetic spectrum questionsSound wave content recurred heavily across both sittings: hearing range and ultrasound cracks in 2022, bat echolocation in 2023, and speed of sound plus refraction in a separate 2023 question.
It wants the standard human hearing range, two genuinely different reasons for its limits, and reasoning linking reflection timing and amplitude loss to a crack in the metal.
An ultrasound emitter and receiver on a crack-free metal bar, showing one emitted signal and one reflected signal, P, on an oscilloscope trace.
The same emitter and receiver on a metal bar containing a crack partway down, showing the emitted signal followed by two separate reflected signals, Q and R, arriving at different times.
The human ear detects roughly 20 Hz to 20 kHz. Two reasons there are limits to this range are the fixed size and stiffness of the parts of the inner ear, such as the cochlea, which are only built to respond to a limited range of vibration frequencies, and the fact that the eardrum itself is not sensitive enough to vibrate in response to frequencies far outside this range.
In Figure 13b, an extra reflected signal, Q, arrives back at the emitter in a shorter time than the signal reflected from the base of the bar, R, and a shorter time means a shorter distance travelled, so signal Q must be reflecting off a crack partway through the bar rather than the far end. Signal R has a smaller amplitude than signal P in the crack free bar because some of the original pulse's energy is already reflected or absorbed by the crack, so less of the signal reaches the base of the bar to be reflected back as R.
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Practise sound wave questionsIt wants a rearrangement of the wave speed equation for frequency, then an echo distance calculation remembering the pulse travels there and back.
A bat shown emitting a sound pulse towards its prey, a moth, drawn not to scale.
Rearranging v = f multiplied by lambda for frequency gives f = v divided by lambda = 330 divided by 0.011, which evaluates to 30 000 Hz. For the distance, the pulse has to travel to the prey and back again in 18 ms, so the total distance travelled is speed multiplied by time = 330 multiplied by 0.018 = 5.94 m, and the distance to the prey itself is half of this, about 3.0 m.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise sound wave questionsIt wants a percentage calculation comparing reaction time to travel time, the correct way to reduce that error's effect, and an explanation of why sound and light refract in opposite ways entering water.
Two technicians, L and M, standing 120 m apart, with L firing a starting pistol and M timing from seeing the smoke to hearing the bang.
Two ray diagrams showing a sound wave and a light wave both travelling from air into water, bending in opposite directions relative to the normal at the boundary.
The time for sound to travel 120 m is distance divided by speed = 120 divided by 330 = 0.364 s. M's reaction time as a percentage of this is (0.23 divided by 0.364) multiplied by 100, which evaluates to about 63%. This shows the technicians' measurement would be improved by increasing the distance between L and M, since a longer travel time makes the fixed 0.23 s reaction time a much smaller proportion of the overall measurement, reducing its effect on the result.
The refraction of the sound wave is different from the light wave because refraction is caused by a change in speed at the boundary, and sound actually speeds up when it travels from air into water, while light slows down when it travels from air into water, so the two waves bend in opposite ways relative to the normal even though both are refracting.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise sound wave questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
What type of wave is sound?
Sound wave questions mix echo timing calculations with reasoning about hearing limits and refraction, so practise both the maths and the explanations.
Practise sound wave questionsThis was June 2022's other 6 mark Level of Response question, asking students to interpret a full seismic wave diagram covering three separate regions of the Earth's surface.
It wants a full interpretation of three regions of detected waves around the Earth, using the properties of P and S waves to argue for a solid mantle, a liquid outer core and a solid inner core.
A table comparing S waves and P waves: S waves are transverse, slow moving and only travel through solids, P waves are longitudinal, fast moving and travel through both liquids and solids.
| Wave type | Wave category | Relative speed | Travels through |
|---|---|---|---|
| S waves | Transverse | Slow moving | Solids only |
| P waves | Longitudinal | Fast moving | Liquids and solids |
A cross section of the Earth showing curved wave paths from a surface earthquake, with region A detecting both P and S waves, region B detecting no waves at all, and region C on the far side detecting only P waves.
At region A, both P and S waves are detected. Since S waves are transverse and can only travel through solids, the fact that S waves reach A at all proves that the material directly beneath the crust, the mantle, must behave as a solid. The paths of both waves also curve as they travel deeper into the Earth, which means the waves are being refracted, and a wave only refracts when it moves into a material where its speed changes. Since the paths bend gradually rather than sharply, the mantle's density must increase gradually with depth rather than changing all at once.
At region B, neither P nor S waves are detected at all, creating a shadow zone. S waves cannot travel through a liquid, so their total absence confirms that whatever lies at the centre of the Earth blocking them must be liquid rather than solid. P waves can travel through both liquids and solids, so their absence at B cannot be explained by the same reason. Instead, P waves must be refracted so strongly at the boundary between the solid mantle and this liquid layer that they bend away from region B entirely, missing it, which is only possible if there is a sudden, large change in density at that boundary.
At region C, only P waves are detected, and they arrive at slightly different times from each other rather than as one clean signal. This can only happen if the P waves have travelled through more than one distinct material on their way to C, each with a different density and therefore a different wave speed. Since the outer part of the core has already been shown to be liquid, the fact that some P waves arrive faster than others at C suggests part of their journey passed through a denser, solid region right at the very centre of the Earth, meaning the Earth has both a liquid outer core and a solid inner core.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise seismic waves questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
What type of wave is a P-wave (primary seismic wave)?
Seismic wave questions always want you to interpret all three regions of the shadow zone diagram, so practise linking each region to a specific structural conclusion.
Practise seismic waves questionsThis full terminal velocity investigation appeared in June 2023, combining a scalar and vector MCQ with a complete practical design and force reasoning.
It combines a scalar and vector MCQ with a full terminal velocity investigation design, a weight calculation, and understanding that constant velocity means balanced forces.
A single paper cupcake case, and then a nested stack of several cupcake cases about to be dropped base first.
A cupcake case shown falling with a single downward weight arrow drawn beneath it, falling at a constant velocity.
Distance is the scalar quantity. Acceleration, force and weight all need a direction as well as a size to describe them fully, so they are vectors, but distance only has a magnitude, which is what makes it a scalar.
To investigate how the falling speed depends on the number of cupcake cases in the stack, I would use the metre rule to measure a fixed height and drop the stack from that same height each time. I would use the stop clock to measure the time of fall for that stack, then work out the average speed using speed equals distance divided by time. I would then repeat the whole process using stacks with a different number of nested cupcake cases, and for each stack size I would repeat the drop several times and average the time to reduce the effect of my reaction time on the stopwatch. Finally I would plot a graph of falling speed against the number of cupcake cases in the stack to show the pattern.
The weight of the stack is found using weight equals mass multiplied by gravitational field strength, so W = 0.005 multiplied by 10, which gives 0.05 N.
On Figure 4 I draw a single straight vertical arrow starting at the cupcake case and pointing directly upward, the same rough length as the downward weight arrow already shown: uparrow. This arrow shows the force due to air resistance acting on the cupcake case.
The acceleration of the cupcake case when it is falling at a constant velocity is zero, since the upward air resistance force is now equal in size to the downward weight force, so the resultant force on it is zero.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise terminal velocity questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
An object reaches terminal velocity when falling through air. Which statement correctly describes the forces at terminal velocity?
Terminal velocity investigations always need the changed variable repeated at multiple values, so practise designing around that specific structure.
Practise terminal velocity questionsThis appeared in June 2023 as a height calculation from a given change in gravitational potential energy for a kicked football.
A direct rearrangement of the GPE equation to find height, using given mass and gravitational field strength.
A football kicked from the ground and rising towards a solid wall, with its path shown curving upward before hitting the wall.
Rearranging change in GPE = mass multiplied by gravitational field strength multiplied by change in height gives change in height = change in GPE divided by (mass multiplied by g), so delta h = 11 divided by (0.42 multiplied by 10), which evaluates to about 2.6 m.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise gravitational potential energy questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
What is the value of gravitational field strength (g) on Earth?
GPE calculations reward rearranging cleanly before substituting, so practise this exact sequence of steps.
Practise gravitational potential energy questionsThis short energy stores description appeared in June 2023 immediately after the GPE and kinetic energy calculations on the same football scenario.
It wants the kinetic energy store named as the starting point, and one genuine destination store on impact.
When the ball hits the wall, energy in the kinetic energy store of the ball is transferred to another store, either the elastic potential energy store as the ball briefly compresses, or the thermal energy store of the ball, wall and surroundings as some energy is dissipated as heat and sound on impact.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise energy stores and systems questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
Which energy store is associated with an object that is moving?
Energy transfer descriptions want a named starting store and a named finishing store, so practise naming both rather than just describing motion.
Practise energy stores and systems questionsThis full set of radioactive decay recall and equation balancing questions appeared in June 2023.
It wants recognising isotopes by proton number, recall of alpha range in air, balancing a full decay equation, and describing what happens inside a nucleus during positron emission.
The nuclear notation for americium-241, showing mass number 241 and proton number 95.
An incomplete decay equation showing americium-241 decaying into an alpha particle plus neptunium, with the mass and proton numbers of the alpha particle and neptunium left blank.
Another isotope of americium must have the same proton number, 95, but a different mass number, so 245 over 95 Am is the correct answer, since the other options change the proton number and so are not isotopes of americium at all. Alpha particles can travel about 5 cm in air at normal atmospheric pressure before being stopped.
Completing the decay equation, an alpha particle has a mass number of 4 and proton number of 2, so subtracting these from americium's 241 and 95 gives neptunium as 237 over 93 Np, balancing both the mass numbers, 241 equals 4 plus 237, and the proton numbers, 95 equals 2 plus 93, on both sides. When a positron is emitted from a nucleus, a proton inside the nucleus changes into a neutron, releasing the positron in the process.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise radioactive decay questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
An alpha particle consists of which particles?
Decay equations always balance both mass number and proton number, so practise checking both totals every time.
Practise radioactive decay questionsThis critical angle investigation appeared in June 2023 as a two part question combining recall and a graph extrapolation method.
It wants the specific reason normal incidence does not bend, and a described method of extrapolating a graph to find the critical angle where r reaches 90 degrees.
A semicircular glass block with a ray of light entering the curved edge at point X along the normal, then hitting the flat face and refracting, with angles i and r both marked from the normal.
A graph of angle r against angle i, curving upward and levelling off, plotted only up to about 40 degrees of i and 80 degrees of r.
The ray does not change direction entering at point X because it enters along the normal to the curved edge of the block, and light travelling along a normal always passes straight through a boundary without bending, even though it does still change speed. To find the critical angle from the graph, I would extend or extrapolate the curve until it reaches an angle of refraction, r, of 90 degrees, then read off the corresponding value of angle i at that point, since the critical angle is defined as the angle of incidence that produces a 90 degree angle of refraction.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise reflection and refraction questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
According to the law of reflection, the angle of incidence is:
Critical angle graph questions always want the curve extended to r = 90 degrees, so practise describing that exact method.
Practise reflection and refraction questionsThis black body radiation reasoning appeared in June 2023 comparing a black and a white sphere near a radiant heater.
It wants a colour based explanation of why absorption rates differ, then a full account of why a sphere absorbing radiation eventually stops rising in temperature.
Two identical iron spheres near a radiant heater, one drawn solid black, the other drawn white with an outline only.
A temperature against time graph for sphere P, rising quickly at first then curving to level off at a constant temperature.
Sphere P heats up faster than sphere Q because a black surface is a better absorber of radiation than a white surface, while a white surface is a better reflector, so the different colours of the two spheres absorb the same incoming radiation at different rates, with the black sphere P taking in far more of the radiation reaching it.
P is absorbing radiation from the heater, but P is also emitting its own radiation as it gets hotter, and the rate of emission increases as temperature rises. The temperature stops rising and becomes constant once the rate at which P emits radiation exactly equals the rate at which it absorbs radiation from the heater, since at that point there is no longer a net gain of thermal energy even though the heater is still switched on.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise black body radiation questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
What is a perfect black body?
Black body equilibrium questions always want absorption and emission both mentioned, so practise explaining the balance, not just the colour effect.
Practise black body radiation questionsThis RTG efficiency question appeared in June 2023, combining a percentage rearrangement with a reasoned property choice.
It wants the efficiency equation rearranged for useful energy, then a genuinely justified isotope property linked to the rover's actual mission.
A photograph of a Mars rover, a wheeled exploration vehicle with instruments mounted on top, shown on the rocky surface of Mars.
Rearranging efficiency = (useful energy transferred divided by total energy supplied) multiplied by 100% gives useful energy transferred = (efficiency multiplied by total energy supplied) divided by 100, so useful energy transferred = (7 multiplied by 1300) divided by 100, which evaluates to 91 J, accepted to the nearest ten joules as 90 J. The isotope used must have a long half-life, since the rover needs to keep operating on Mars for a long time after its long journey there, and once on Mars the RTG cannot simply be replaced or refuelled.
Could you have written this? Every fact in this answer is drilled in our quizzes — the writing is the easy part once the evidence is automatic.
Practise efficiency questionsThe topic changes by sitting — the mark scheme never does. Learn this once, then open your question above for that sitting’s sources and a full worked answer.
Which equation correctly defines efficiency?
Efficiency rearrangements are easy marks once you have the percentage handling right, so drill the rearrangement until it is automatic.
Practise efficiency questionsAcross the June 2022 and June 2023 sittings we have full papers for, these are the topics with real questions in both sittings, so they carry the most weight to prepare for.
Moments and levers as a standalone calculation · Work done and energy transfer calculations · Specific heat capacity calculations · Power calculations · Comparing wave properties across the spectrum · Background radiation sources · Radiation detection methods · Our Solar System · Orbits
This page focuses on question types with a genuinely comparable, real structure across two or more sittings, or a single strong recent example. Several other topics on the specification appear in the two real papers we analysed but are not yet built out here in this recurring-structure format.
The stems are quoted from the real Pearson Edexcel papers, the diagrams and figures are described in our own words, and every worked answer is written entirely by us, aimed at the top of the real mark scheme for each question. Nothing here is copied from Pearson's own exemplar material, since that would breach copyright, but each answer is built to hit exactly what the real mark scheme rewarded. PrepWise is independent of Pearson Edexcel and not endorsed by them.
Pearson no longer hosts the June 2019 Paper 1H files on their own live filestore, so we have not built anything from that sitting rather than invent content from a paper we cannot verify. Everything on this page is built directly from the real June 2022 and June 2023 papers and mark schemes.
Sometimes a very similar calculation reappears with different numbers, and topics like momentum, sound waves, forces and reactor control return in some form almost every sitting. But you cannot rely on exact repeats, so use this page to learn which TOPICS keep returning and practise the underlying method, since the specific numbers in the question will very likely change.
Across the two sittings we have, there are three extended, Level of Response questions worth 6 marks each, graded against three named bands rather than simple point marking, not one per paper. June 2022 has one: comparing X-rays with radio waves. June 2023 has two: explaining a Newton's second law investigation, and separately explaining nuclear reactor control. These need a genuinely detailed, logically structured answer covering every strand the mark scheme asks for, not just a list of isolated facts.
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