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Flashcards · J249 · Topic 8
Global challenges flashcards
32 cards on Topic 8, subtopics P8.1 to P8.3. Pick a subtopic or study them all.
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P8.1 Physics on the move
- Typical speeds: walking, cycling, car in town, car on a motorway, sound in air
- Walking ~1.5 m/s, cycling ~6 m/s, car in town ~13 m/s, motorway ~30 m/s, sound in air ~340 m/s.
- Typical accelerations: car pulling away, emergency braking, free fall
- Car pulling away: 2 to 3 m/s². Emergency braking: 6 to 8 m/s². Free fall: about 10 m/s².
- How do you measure reaction time with a ruler drop?
- Drop the ruler without warning between the person’s thumb and finger, read the distance fallen when caught, convert it to a time, repeat and take the mean. A typical value is about 0.2 s.
- Thinking distance and braking distance: what affects each?
- Thinking (speed × reaction time): speed, tiredness, alcohol, drugs, distraction. Braking: speed, wet or icy roads, worn tyres or brakes, greater mass.
- A driver at 90 km/h has a reaction time of 0.60 s. Thinking distance?
- 90 ÷ 3.6 = 25 m/s, so 25 × 0.60 = 15 m
- Why is a large deceleration dangerous?
- F = ma, so a large deceleration means a large force on the body, which can cause broken bones and internal injuries.
- How do crumple zones, seat belts and airbags reduce injury?
- They make the stop take a longer time (or distance), so the deceleration and the force on the person are smaller. Airbags also spread the force over a larger area.
- Estimate the stopping distance at 25 m/s (reaction time 0.7 s, deceleration 5.0 m/s²).
- Thinking: 25 × 0.7 = 17.5 m Braking: 25² ÷ (2 × 5.0) = 62.5 m Total ≈ 80 m
- A 1000 kg car at 20 m/s stops in 40 m. Estimate the braking force.Higher
- Kinetic energy = ½ × 1000 × 20² = 200 000 J. Force = 200 000 ÷ 40 = 5000 N.
P8.2 Powering Earth
- Renewable vs non-renewable energy resource
- Renewable: replaced as fast as it is used (wind, tides, the Sun, hydroelectricity, biofuel). Non-renewable: used faster than it forms, so it will run out (coal, oil, gas, nuclear fuel).
- How do fossil-fuel and nuclear power stations generate electricity?
- The fuel’s energy heats water to make steam, the steam turns a turbine, and the turbine turns a generator.
- Compare gas and wind for generating electricity
- Gas: reliable on demand, but burning it releases carbon dioxide and it needs a continuing fuel supply. Wind: no fuel and no carbon dioxide, but output depends on the weather.
- National grid
- The network of cables and transformers linking power stations to users.
- Step-up transformer
- Raises the potential difference, at the power station end of the grid.
- Step-down transformer
- Lowers the potential difference near where the power is used, so homes get a safe, usable supply.
- Why is high-voltage transmission efficient?
- For a fixed power, P = VI, so a high pd means a low current. Wasted power is I²R, so a lower current means much less heating in the cables.
- Does a transformer increase power?
- No. A transformer changes the potential difference. It does not increase power.
- How do the turns on a step-up transformer compare?Higher
- More turns on the secondary coil than the primary (Vp / Vs = Np / Ns), so the secondary pd is higher and, for the same power, the current is lower.
- UK domestic electricity supply
- Alternating current, 50 Hz, about 230 V. One cycle lasts 1 ÷ 50 = 0.02 s.
- Live, neutral and earth wires: colours and potential differences
- Live: brown, about 230 V. Neutral: blue, about 0 V, completes the circuit. Earth: green and yellow, 0 V, safety wire joined to the metal case.
- What does the earth wire do if the live wire touches a metal case?
- A large current flows through the earth wire instead of through the user. Without an earth wire the case would be at about 230 V and could give a shock.
P8.3 Beyond Earth
- How does the radiation from a body change as it gets hotter?
- The intensity (energy emitted per second per square metre) increases, and the strongest emission moves to a shorter wavelength.
- Order of the planets from the Sun
- Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune.
- Geostationary vs polar orbit
- Geostationary: about 36 000 km up, period 24 hours, above the equator, appears fixed (communications). Polar: low, period around 1.5 hours, passes over both poles (mapping, monitoring, weather).
- In a circular orbit, which stay constant: speed, velocity, size of the resultant force?Higher
- Speed and the size of the resultant force stay constant. The velocity changes because the direction changes; gravity acts towards the centre.
- How are orbit radius and speed linked for a stable orbit?Higher
- A lower orbit needs a faster speed (and has a shorter period). If the speed changes, the radius must change.
- What determines whether a body warms, cools or stays at a constant temperature?Higher
- Absorbed more than emitted: it warms. Emitted more than absorbed: it cools. Equal: constant temperature (equilibrium).
- Red-shift
- Light from a receding source is observed at a longer wavelength and lower frequency than it was emitted. A bigger shift means a faster recession.
- How does red-shift data support an expanding universe?
- Nearly every galaxy is red-shifted, and more distant galaxies have bigger red-shifts, so they move away faster: space itself is expanding.
- How does the CMBR support the Big Bang model?
- The early universe was very hot and dense and full of radiation. Expansion stretched its wavelengths, so it is now seen from all directions as microwaves.
- How does a star form and become stable?
- Gravity pulls a cloud of dust and gas together; it heats up until hydrogen nuclei fuse to helium, releasing energy. Inward gravitational collapse is then balanced by outward expansion from the fusion energy.
- Life cycle of a star much more massive than the Sun
- Cloud → protostar → stable star → red supergiant → supernova → neutron star or black hole.
Revise Global challenges further
- Study guideOCR GCSE Physics A: Energy resources, trends in use and mains electricity (J249)
- Revision notesOCR GCSE Physics A: Energy resources, trends in use and mains electricity (J249) – Revision Notes
- Practice questionsOCR GCSE Physics A: Energy resources, trends in use and mains electricity (J249) – Practice Questions