← Back to subjects
0
OCR Gateway GCSE Physics A (J249) · P8 — Global challenges
Mini-Lesson

Global Challenges

This mini-lesson covers the whole of OCR Gateway Topic P8 — Global challenges, all three parts: P8.1 Physics on the move, P8.2 Powering Earth and P8.3 Beyond Earth.

P8.1 Physics on the move P8.2 Powering Earth P8.3 Beyond Earth

Work through each screen, answer the questions as you go (some wordy, some calculations) and collect ⭐ stars. Items marked Higher are Higher-tier only. Press Start when you're ready.

P8.1 · Physics on the move

Stopping distance

The total distance a vehicle travels from the moment a hazard appears until it is fully stopped is the stopping distance. It splits into two parts:

stopping = thinking + brakingstopping distance = thinking distance + braking distance
thinking distance braking distance driver reacts brakes do work stopping distance
Thinking distance = distance travelled during the driver's reaction time. Braking distance = distance travelled once the brakes are applied.

Watch out: a common mix-up is which factors change which part. Tiredness, alcohol, drugs and distraction increase the driver's reaction time, so they increase the thinking distance — not the braking distance.

P8.1 · Physics on the move

What changes each distance?

Thinking distance depends on the driver's reaction time and the speed:

  • Longer reaction time → longer thinking distance: caused by tiredness, alcohol, drugs, or distraction (e.g. a phone).
  • Higher speed → more distance covered before the brakes even come on.

Braking distance depends on the braking force, the mass and the speed, and on the road and vehicle:

  • Wet or icy road, or worn tyres / brakes → less grip → longer braking distance.
  • Higher speed → far longer braking distance (it grows much faster than thinking distance, because the kinetic energy ∝ v²).
  • A heavier or faster vehicle needs a larger braking force to stop in the same distance.

Reaction time is typically 0.2 s – 0.9 s. You can measure it with the ruler-drop experiment.

Quick calculation

Thinking distance

1A car travels at 30 m/s. The driver's reaction time is 0.7 s. Calculate the thinking distance (distance travelled during the reaction time). Use distance = speed × time.
m
Hint: 30 × 0.7.
P8.1 · Physics on the move

Large decelerations are dangerous

In a crash a vehicle stops in a very short time. A large deceleration means a large force on the occupants — enough to cause serious injury.

Safety features work by making the collision take longer, so the deceleration — and therefore the force — is smaller:

  • Crumple zones fold and squash, extending the stopping time.
  • Seatbelts stretch slightly and stop you being thrown forward; they spread the force and lengthen the stop.
  • Airbags inflate and let the head and chest decelerate over a longer time and area.
wall crumple crumple zone folds → collision time ↑ deceleration ↓ force on people ↓
All three features lengthen the collision time. A longer time means a smaller rate of change of momentum, so a smaller force.

Misconception: longer collision time does not mean a bigger force — it means a smaller force, because the same momentum change is spread over more time.

P8.1 · Physics on the move

Momentum & its conservation

Momentum is mass × velocity. It is a vector (it has direction).

p = m vmomentum (kg m/s) = mass (kg) × velocity (m/s)

In a closed system (no external forces) momentum is conserved: the total momentum before a collision or explosion equals the total momentum after.

Example — collision

A 2 kg trolley at 3 m/s hits a stationary 1 kg trolley and they stick together.

Before: p = (2 × 3) + (1 × 0) = 6 kg m/s.

After: total mass 3 kg, so 3 × v = 6 → v = 2 m/s.

Higher tier

Force equals the rate of change of momentum:

F = Δ(mv) / tforce (N) = change in momentum (kg m/s) ÷ time (s)

For the same change in momentum, a longer time t gives a smaller force F. That is exactly how crumple zones, seatbelts and airbags protect you.

Higher · Quick calculation

Force from momentum change

2In a crash a 900 kg car moving at 20 m/s is brought to rest. (a) Without a crumple zone it stops in 0.10 s. Calculate the force. Use F = Δ(mv) ÷ t.
N
Hint: Δp = 900 × 20 = 18000 kg m/s, then divide by 0.10.

Now show the safety effect:

3(b) A crumple zone extends the stop to 0.50 s. Calculate the new force (same Δp = 18000 kg m/s).
N
Hint: 18000 ÷ 0.50. Notice the force is 5× smaller — the collision lasted 5× longer.
P8.1 · Physics on the move

Terminal velocity

When an object falls through a fluid (e.g. a skydiver in air) two forces act: weight pulling down and air resistance (drag) pushing up.

weight drag Start: weight > drag → speeds up Faster: drag grows → acceleration falls drag = weight → terminal velocity (constant)
At first weight > drag so the object accelerates. As it speeds up, drag grows until drag = weight: the resultant force is zero, so the object falls at a steady terminal velocity.

At terminal velocity the forces are balanced, the resultant force is zero, acceleration is zero, and the speed is constant.

Quick check

At terminal velocity…

?A skydiver is falling at a steady terminal velocity. What is true about the forces on her?
P8.2 · Powering Earth

Energy resources

We generate most electricity by spinning a turbine connected to a generator. Resources are renewable (won't run out) or non-renewable (finite).

Renewable 💨 wind☀️ solar 💧 hydro🌊 tidal ♨️ geothermal🌱 biomass Non-renewable ⛽ coal⛽ oil 🔥 gas☢️ nuclear
Renewables: wind, solar, hydroelectric, tidal, geothermal, biomass. Non-renewables: fossil fuels (coal, oil, gas) and nuclear fuel.

Trade-offs: fossil fuels are reliable and high-output but release CO₂ (climate change) and other pollutants. Nuclear is reliable and CO₂-free in use but produces radioactive waste. Renewables are clean but many (wind, solar, tidal) are intermittent or depend on weather/location.

Trend: over time the UK is shifting away from coal and increasingly towards gas and renewables — renewables make up a growing share of electricity generation.

Mini-game · Sort it

Renewable or non-renewable?

Tap a resource, then tap the box you think it belongs in. Sort all eight.

♻️ Renewable

⛽ Non-renewable

P8.2 · Powering Earth

Mains electricity & the plug

The UK mains supply is a.c. (alternating current) at 50 Hz and about 230 V. a.c. repeatedly changes direction; a battery gives d.c. (direct current) which flows one way only.

E N L fuse Live (brown): carries 230 V a.c. Neutral (blue): completes the circuit, ~0 V Earth (green/yellow): safety wire, 0 V
Live (brown) carries the supply p.d. Neutral (blue) completes the circuit. Earth (green-and-yellow) is a safety wire connected to the metal case.

A live wire is dangerous even when the switch is off, because it stays at 230 V relative to earth — touching it gives a path to earth and a shock.

P8.2 · Powering Earth

Fuses, earthing & double insulation

  • Fuse — a thin wire in the live side. A fault makes the current rise; the fuse heats up and melts, breaking the circuit before the cable overheats.
  • Earthing — an earth wire connects a metal case to earth. If a fault makes the case live, a large current flows to earth and blows the fuse, so the case can't stay live.
  • Double insulation — appliances with plastic cases have no exposed metal to become live, so they need no earth wire (shown by the ⧈ symbol).

Electrical power links to current and p.d.:

P = V × Ipower (W) = potential difference (V) × current (A)
Why fuse rating matters

A 230 V appliance rated 690 W draws I = P ÷ V = 690 ÷ 230 = 3 A, so a 5 A fuse is suitable (next size up).

Quick check

Mains safety

?Why is the live wire dangerous even when an appliance is switched off at the wall?
P8.2 · Powering Earth

The National Grid

The National Grid moves electricity from power stations to homes. It transmits at very high voltage (hundreds of kV) and low current.

power station step-UP V↑ I↓ high V, low I (small I²R loss) step-DOWN V↓ I↑ homes station → step-up → pylons (high V) → step-down → homes (230 V)
A step-up transformer raises the voltage for transmission; a step-down transformer lowers it again for safe use in homes.

Why high voltage? Power lines have resistance R. The power wasted as heat is I²R. Transmitting at high V means a low current I (since P = VI), and because the loss depends on I², a small current means a much smaller energy loss. This makes transmission efficient.

Misconception: the high voltage is across the lines relative to earth, not "extra current". Higher V → lower I → lower I²R heating loss.

P8.2 · Powering Earth

Transformers

A transformer has two coils on an iron core. The turns ratio sets how the p.d. changes:

Vp / Vs = Np / Nsprimary p.d. ÷ secondary p.d. = primary turns ÷ secondary turns
  • Step-up: more turns on the secondary (Ns > Np) → V goes up.
  • Step-down: fewer turns on the secondary → V goes down.

Higher tier

An ideal transformer wastes no power, so power in = power out:

Vp Ip = Vs Isprimary p.d. × primary current = secondary p.d. × secondary current

Misconception: transformers only work with a.c. They rely on a changing magnetic field to induce a voltage in the second coil — a steady d.c. current would not work. This is one reason the grid uses a.c.

Quick calculation

Transformer ratio

4A step-up transformer has a primary coil of 1000 turns at 230 V and a secondary coil of 100000 turns. Calculate the secondary voltage Vs. Use Vp/Vs = Np/Ns.
V
Hint: Vs = Vp × (Ns ÷ Np) = 230 × (100000 ÷ 1000).
P8.3 · Beyond Earth

The Solar System & our galaxy

Our Solar System contains the Sun (a star) at the centre, the 8 planets and their moons, plus dwarf planets (e.g. Pluto), asteroids and comets. The Sun and everything orbiting it sit within the Milky Way galaxy — billions of stars bound by gravity.

Sun 8 planets ☄️ comets · 🪨 asteroids · 🌑 moons · dwarf planets
Bodies in the Solar System: the Sun, 8 planets, their moons, dwarf planets, asteroids and comets — all part of the Milky Way.

Misconception: "the Sun is not a star." It is a star — an ordinary main-sequence star that happens to be close to us.

P8.3 · Beyond Earth

Orbital motion

Planets orbit the Sun, and satellites (natural moons and artificial ones) orbit planets. The force that holds an object in orbit is gravity, pulling it toward the central body.

central gravity (toward centre) velocity
Gravity always points toward the central body and provides the centripetal force. The velocity is along the orbit — at right angles to the force.

Higher tier

In a circular orbit the speed is constant but the velocity is always changing (its direction changes). The inward gravitational pull constantly changes the direction of motion without changing the speed. For a stable orbit, if the orbital speed changes the radius must change: a satellite moving faster needs a smaller orbit radius, and a slower one needs a larger radius.

Misconception: orbiting objects are not "force-free." Gravity provides the centripetal force — without it they would fly off in a straight line.

Higher · Quick check

Reasoning about orbits

?A satellite is in a stable circular orbit. Which statement is correct?
P8.3 · Beyond Earth

The life cycle of a star

A star is born when gravity pulls a cloud of dust and gas (a nebula) together into a protostar. When it is hot and dense enough, nuclear fusion of hydrogen begins and it becomes a stable main-sequence star like the Sun.

Stability comes from a balance: the outward pressure from fusion energy exactly balances the inward pull of gravity. What happens at the end depends on the star's mass:

nebula proto-star main-sequence redgiant whitedwarf low / medium mass (like Sun) redsupergiant supernova neutronstar blackhole massive star
Both paths start nebula → protostar → main sequence. A Sun-like star ends as red giant → white dwarf. A massive star ends as red supergiant → supernova → neutron star or, if massive enough, a black hole.
Mini-game · Put it in order

Order a Sun-like star's life

Tap the stages in the correct order, earliest first, for a star like our Sun.

P8.3 · Beyond Earth

Red-shift & the Big Bang

Light from distant galaxies is shifted toward the red (longer wavelength, lower frequency) end of the spectrum. The further away a galaxy is, the greater its red-shift — so more distant galaxies are receding faster.

blue red → nearby distant lines moved toward red
The same spectral lines appear at longer (redder) wavelengths for more distant galaxies. More distant = greater red-shift.

This is strong evidence that the universe is expanding — space itself is stretching, carrying galaxies apart. Running the expansion backwards points to the Big Bang: the universe began from a tiny, hot, dense point. The leftover heat is detected today as the cosmic microwave background radiation (CMB), the strongest evidence for the Big Bang.

Misconception: red-shift is not galaxies moving "through" space like cars. It is space itself stretching, so the wavelengths of the light are stretched too.

Quick check

What red-shift tells us

?Astronomers find that more distant galaxies show greater red-shift. What does this provide evidence for?
P8.3 · Beyond Earth · Higher

Seismic waves & Earth's structure

Earthquakes send seismic waves through the Earth. Differences in how they travel reveal the hidden internal structure:

  • P waves (primary) are longitudinal. They travel through solids and liquids.
  • S waves (secondary) are transverse. They travel through solids only — they cannot pass through liquids.
mantle liquid outer core solid inner core earthquake P (all layers) S (solids only) S-wave shadow → liquid outer core
S waves are blocked by the liquid outer core, creating an S-wave "shadow." This tells us the outer core is liquid; the way P waves refract reveals the layered structure.

Because S waves don't reach the far side of the Earth (an S-wave shadow zone), scientists deduced the outer core is liquid. P-wave refraction at boundaries reveals the crust, mantle and core.

Recap

Key equations & ideas — P8

Stopping: stopping distance = thinking + braking distance

Momentum: p = m v  (conserved in collisions)

Force (HT): F = Δ(mv) ÷ t  → longer time, smaller force

Power: P = V × I

Transformer: Vp/Vs = Np/Ns  (HT: VpIp = VsIs)

Grid: high V → low I → small I²R loss

Orbits: gravity provides the centripetal force

Stars: nebula → protostar → main sequence → (Sun) red giant → white dwarf / (massive) red supergiant → supernova → neutron star or black hole

Cosmology: more distant = greater red-shift → expanding universe → Big Bang + CMB

Earth: P waves (solid+liquid), S waves (solid only) → liquid outer core

You've covered all three parts of OCR Gateway P8 — Physics on the move, Powering Earth and Beyond Earth. Press Finish to see your score.

🏆

Mini-lesson complete!

⭐⭐⭐

You've worked through Global Challenges for OCR Gateway GCSE Physics A. 🎉

Your stars: 0 / 0

Next: test yourself in the Evaluate stage Confidence Quiz, then lock it in with Verify.

📣 Smashed it? Share your score

Challenge a mate to beat your stars, or show a parent how you got on.

→ Back to all subjects