OCR GCSE Physics A (Gateway)

OCR GCSE Physics A P8.3 Beyond Earth Exam Questions

Free OCR GCSE Physics A exam questions for P8.3 Beyond Earth, with a mark scheme for every pack. Covers the solar system, orbits, satellites, the life cycle of stars, red-shift, the Big Bang and cosmic microwave background radiation.

P8.3 Beyond Earth exam questions

1 question pack of real past exam questions, each with its mark scheme. Do not stop after a few: answer as many as you can without notes, then mark every answer with the mark scheme. The more questions you do, the more quickly you will spot how examiners ask about each idea.

P8.3 Beyond earth exam questions for OCR GCSE Physics A (Gateway)QuestionsMark scheme
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About OCR GCSE Physics A P8.3 Beyond Earth

P8.3 is the final topic of the P8 Global challenges chapter of OCR Gateway Physics A and is separate physics content. It covers the formation and structure of the solar system, how gravity provides the force for circular orbits, and why the speed of an orbiting body depends on its distance. You learn the life cycle of stars, which depends on their mass, how red-shift of distant galaxies shows the universe is expanding, and why cosmic microwave background radiation supports the Big Bang model. It draws on P2 Forces, P5 Waves and P6 fusion. Examiners like star life cycle sequences and explanations of evidence for the Big Bang.

What you need to know

  • Solar system Formed from a cloud of dust and gas pulled together by gravity. It contains the Sun, planets, dwarf planets, moons, asteroids and comets, and is part of the Milky Way galaxy.
  • Orbits Gravity provides the centripetal force for circular orbits. A body in orbit is accelerating because its direction changes. For a stable orbit, closer objects must move faster.
  • Satellites Artificial satellites are used for communication, weather monitoring, navigation and observing the universe. Geostationary satellites orbit once per day above the equator.
  • Life cycle of stars Nebula, protostar, main sequence (fusion pressure balances gravity). Sun-like stars: red giant, white dwarf. Much more massive stars: red supergiant, supernova, then neutron star or black hole.
  • Red-shift Light from distant galaxies has longer wavelengths than expected. Greater red-shift for more distant galaxies shows they are receding faster, so the universe is expanding.
  • Big Bang and CMB The universe began from a very small, hot, dense region and has expanded since. Cosmic microwave background radiation is evidence for this model.
  • Observing space Telescopes using different parts of the EM spectrum, and space telescopes above the atmosphere, reveal more than visible light alone.

Common mistakes in P8.3 Beyond Earth

  • Saying there is no gravity in space. Gravity keeps satellites and planets in orbit.
  • Saying a satellite at constant speed is not accelerating. Its direction changes, so its velocity changes.
  • Saying all stars end as black holes. Only very massive stars do.
  • Describing red-shift as galaxies looking redder. It is an increase in observed wavelength.
  • Saying a main sequence star is stable because fusion stops. It is stable because outward pressure from fusion balances gravity.

Try three P8.3 Beyond Earth exam-style questions

1. Describe the life cycle of a star with a similar mass to the Sun. (4 marks)

Show the mark scheme answer

Nebula of dust and gas collapses under gravity to form a protostar; fusion starts and it becomes a main sequence star; it expands into a red giant when hydrogen runs out in the core; it ends as a white dwarf.

2. Explain how red-shift provides evidence for the Big Bang. (3 marks)

Show the mark scheme answer

Light from distant galaxies is red-shifted, so they are moving away; more distant galaxies have greater red-shift, so are moving faster; this shows the universe is expanding from a single point.

3. Explain why a satellite in a circular orbit is accelerating even though its speed is constant. (2 marks)

Show the mark scheme answer

Its direction is continually changing so its velocity changes; gravity provides a resultant force towards the centre of the orbit.

P8.3 Beyond Earth FAQs

What does OCR GCSE Physics A (Gateway Science) P8.3 Beyond Earth cover?

It covers the solar system, orbits and satellites, the life cycle of stars, red-shift, the Big Bang and cosmic microwave background radiation.

Which paper is P8.3 examined on?

Topics P5 to P8 are assessed on Paper 2 (Foundation) or Paper 4 (Higher), which can also draw on knowledge from P1 to P4 and practical skills.

What evidence for the Big Bang should I learn?

Learn red-shift of distant galaxies, including the link between distance and recession speed, and cosmic microwave background radiation, and be able to explain how each supports the model.