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GCSE/Physics/CCEA

U2.3Space physics — solar system, life cycle of stars, redshift, Big Bang theory

Notes

Space Physics

The Solar System

The Solar System consists of the Sun (a star) and all the objects gravitationally bound to it:

  • 8 planets (in order from the Sun): Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune. Mnemonic: "My Very Eager Mother Just Served Us Nachos."
  • Moons — natural satellites of planets. Earth has one Moon.
  • Asteroids — rocky bodies mostly in the Asteroid Belt between Mars and Jupiter.
  • Comets — icy bodies with elongated orbits; tails point away from the Sun.
  • Dwarf planets (e.g. Pluto, Eris).

Planets orbit the Sun in elliptical paths (approximately circular for inner planets). Gravitational force from the Sun provides the centripetal force keeping planets in orbit.

Units of distance

  • Astronomical unit (AU): average Earth-Sun distance ≈ 1.5 × 10¹¹ m. Used within the Solar System.
  • Light-year (ly): distance light travels in one year ≈ 9.5 × 10¹⁵ m. Used for distances between stars.
  • Parsec (pc): ≈ 3.26 light-years. Used by professional astronomers.

Life cycle of stars

Low/medium mass stars (like the Sun):

  1. Nebula (cloud of gas and dust) → gravity causes collapse.
  2. Protostar → gravitational energy converts to heat; core heats up.
  3. Main sequence star → hydrogen fusion in core; stable for billions of years (Sun: ~10 billion years total).
  4. Red giant → hydrogen in core runs out; star expands; helium fusion begins.
  5. White dwarf → outer layers blown off as planetary nebula; core cools and contracts.
  6. Cools to a black dwarf (very long timescale).

High mass stars:

  1. Nebula → Protostar → Main sequence (shorter life, hotter, more luminous, blue).
  2. Red supergiant (larger than red giant).
  3. Supernova — catastrophic explosion; releases huge energy; can outshine an entire galaxy briefly.
  4. Core collapses to a neutron star or, if very massive, a black hole.

Supernovae are important: they synthesise heavy elements (heavier than iron) and scatter them through space. We are literally made of "star stuff."

Galaxies and the universe

A galaxy is a system of billions of stars bound by gravity. The Milky Way is our galaxy (~200–400 billion stars, ~100,000 light-years across). Galaxies are grouped into clusters; clusters into superclusters.

Redshift and the expanding universe

Redshift: light from distant galaxies is shifted towards longer (red) wavelengths. The further the galaxy, the greater the redshift. This is the Doppler effect for light — galaxies are moving away from us, so their light is stretched.

Hubble's law: recession speed v = H₀ × d, where H₀ is the Hubble constant and d is distance. More distant galaxies recede faster.

Implication: the universe is expanding. Running time backward → everything was once in the same place → the Big Bang theory.

The Big Bang theory

  • The universe began approximately 13.8 billion years ago from an extremely hot, dense state (a singularity).
  • The universe has been expanding and cooling ever since.
  • Evidence: (1) redshift of galaxies; (2) Cosmic Microwave Background CMB radiation — faint microwave radiation coming uniformly from all directions, the "echo" of the hot early universe.
  • The Big Bang was not an explosion into space but an expansion of space itself.

Common mistakes

  1. Confusing red giant and red supergiant — the latter is from a high-mass star.
  2. Saying the Sun will go supernova — it will not; it is too low mass and will become a white dwarf.
  3. Redshift = moving away; blueshift = moving towards — all distant galaxies are redshifted (expanding universe).
  4. Big Bang was not an explosion INTO space — space itself expanded.

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Practice questions

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  1. Question 17 marks

    Life cycle of the Sun

    CCEA Unit 2 Paper

    (a) Describe the stages in the life cycle of a star similar in mass to the Sun, starting from a nebula. (6 marks)
    (b) State one way in which the life cycle of a very massive star differs from that of the Sun. (1 mark)

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  2. Question 25 marks

    Redshift and the expanding universe

    CCEA Unit 2 Paper

    (a) Explain what is meant by redshift of light from distant galaxies. (2 marks)
    (b) Describe the pattern observed in redshift measurements of galaxies at different distances. (2 marks)
    (c) State what these observations tell us about the universe. (1 mark)

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  3. Question 38 marks

    Big Bang theory — evidence

    CCEA Unit 2 Paper

    (a) State two pieces of evidence that support the Big Bang theory. (2 marks)
    (b) Describe the Big Bang theory. (3 marks)
    (c) Explain what is meant by Cosmic Microwave Background CMB radiation and why it supports the Big Bang. (3 marks)

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  4. Question 46 marks

    Solar system — planets and distances

    CCEA Unit 2 Paper

    (a) Name the four inner planets of the Solar System in order from the Sun. (2 marks)
    (b) State what provides the centripetal force for planetary orbits. (1 mark)
    (c) The distance from Earth to the Sun is approximately 1.5 × 10¹¹ m. Light takes approximately 8.3 minutes to travel from the Sun to Earth. Show that this is consistent with the speed of light being 3.0 × 10⁸ m/s. (3 marks)

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  5. Question 56 marks

    Supernova and stellar remnants

    CCEA Unit 2 Paper

    (a) Describe what happens to a very massive star at the end of its main sequence stage. (4 marks)
    (b) Explain the importance of supernovae for the chemical elements found on Earth. (2 marks)

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Flashcards

U2.3 — Space physics — solar system, life cycle of stars, redshift, Big Bang theory

8-card SR deck for CCEA Physics topic U2.3

8 cards · spaced repetition (SM-2)