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How did the Solar System and stars form, and what is the evidence for the Big Bang?

The structure of the Solar System, the life cycle of stars, red-shift of light from distant galaxies, and how red-shift provides evidence for an expanding universe and the Big Bang theory.

A focused answer to OCR Gateway GCSE Physics A topic P8 Beyond Earth, covering the structure of the Solar System, the life cycle of stars, the red-shift of light from distant galaxies, and how red-shift provides evidence for an expanding universe and the Big Bang theory.

Generated by Claude Opus 4.89 min answer

Reviewed by: AI editorial process; not yet individually human-reviewed

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  1. What this topic is asking
  2. The Solar System
  3. The life cycle of stars
  4. Red-shift
  5. Evidence for the expanding universe and the Big Bang
  6. Try this

What this topic is asking

OCR wants you to describe the structure of the Solar System, describe the life cycle of stars, explain red-shift, and explain how red-shift provides evidence for an expanding universe and the Big Bang. This is topic P8.3 (Beyond Earth) of the OCR Gateway Physics A (J249) specification.

The Solar System

Planets orbit the Sun, and moons orbit planets; the gravitational force provides the centripetal force that keeps each body in its orbit.

The life cycle of stars

Supernovae also scatter the heavier elements (made by fusion in massive stars and in the explosion itself) into space, where they can form new stars and planets.

Red-shift

Astronomers measure red-shift by looking at the dark lines in a galaxy's spectrum, which are shifted towards longer (redder) wavelengths compared with the same lines measured on Earth.

Evidence for the expanding universe and the Big Bang

Try this

Q1. State what holds the planets in orbit around the Sun. [1 mark]

  • Cue. The gravitational attraction (force) of the Sun.

Q2. State what the red-shift of distant galaxies tells us about the universe. [2 marks]

  • Cue. The galaxies are moving away (and more distant ones move away faster), which shows the universe is expanding.

Exam-style practice questions

Practice questions written in the style of OCR exam questions on this dot point, with worked answer explainers. The year tag is the paper they imitate, not the source.

OCR 20184 marksDescribe the life cycle of a star about the same size as the Sun, from its formation to its final stage.
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A P8 Describe question worth four marks. A star forms when a cloud of dust and gas (a nebula) is pulled together by gravity, heating up until nuclear fusion of hydrogen into helium begins; this stable phase is the main sequence (2 marks for the nebula collapsing under gravity and fusion starting). When the hydrogen runs low, a Sun-sized star swells into a red giant (1 mark). Finally it sheds its outer layers (forming a planetary nebula) and the core is left as a hot, dense white dwarf (1 mark). Markers reward the nebula-to-main-sequence formation, the red giant stage, and the white dwarf end point for a Sun-sized star. A common error is to give the high-mass route (supernova, neutron star or black hole) for a Sun-sized star.

OCR 20214 marksExplain what is meant by red-shift, and explain how observations of red-shift provide evidence for the Big Bang theory.
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A P8 question worth four marks. Red-shift is the increase in the wavelength of light from distant galaxies, shifting it towards the red end of the spectrum, which happens because the galaxies are moving away from us (2 marks for the increase in wavelength caused by galaxies moving away). Observations show that more distant galaxies have a greater red-shift, so they are moving away faster, which means the whole universe is expanding (1 mark). Tracing this expansion backwards suggests everything began from a single, very hot, dense point: this is the Big Bang theory (1 mark). Markers reward red-shift as increasing wavelength from receding galaxies, the link to an expanding universe, and the Big Bang as the implied origin. A common error is to describe red-shift as a colour change of the galaxy itself rather than a stretch in wavelength.

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