Session XP: 0
P7 SpaceAQA GCSE Physics · 8463 (Triple)

Solar System and the Universe

Structure of the solar system and universe, life cycle of stars, formation of planets.

Best score
Last attempt
Best attempt progress
0
XP earned
Watch first
CognitoSolar system and the universe
Key facts & equations

Structure of the Solar System

  • Sun (a star) at the centre. Eight planets orbit the Sun in elliptical orbits.
  • In order from Sun: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune.
  • Inner planets (rocky): Mercury, Venus, Earth, Mars.
  • Outer planets (gas giants): Jupiter, Saturn. Ice giants: Uranus, Neptune.
  • Also: dwarf planets (Pluto), asteroids (asteroid belt between Mars/Jupiter), comets (eccentric orbits).
  • Moons orbit planets. Earth has one Moon. Jupiter has 95 known moons.

Scale of the universe

  • Units of distance: AU (astronomical unit = Earth-Sun distance = 1.5 × 10¹¹ m).
  • Light-year: distance light travels in one year ≈ 9.5 × 10¹⁵ m.
  • Our galaxy: the Milky Way — contains ~300 billion stars. Diameter ~100,000 light-years.
  • Observable universe: ~93 billion light-years across. Contains ~2 trillion galaxies.
  • Nearest star to Sun: Proxima Centauri — 4.2 light-years away.

Life cycle of stars

  • All stars: formed from clouds of gas and dust (nebula) → gravitational collapse → protostar → main sequence star (hydrogen fusion, balance of gravity vs radiation pressure).
  • Small stars (like Sun): main sequence → red giant (He fusion) → planetary nebula → white dwarf → black dwarf.
  • Large stars: main sequence → red supergiant → supernova (explosive collapse) → neutron star OR black hole (if very massive).
  • Supernova: heavy elements (beyond iron) formed and dispersed through universe.
  • Our Sun: currently main sequence (~halfway through its ~10 billion year life).

Formation of the Solar System

  • Formed ~4.6 billion years ago from a rotating cloud of gas and dust (solar nebula).
  • Gravity caused collapse → most mass collected at centre → Sun formed.
  • Remaining material flattened into a disc. Material clumped (accretion) → planets.
  • Rocky (inner) planets: formed close to Sun where temperatures were too high for gas to remain.
  • Gas giants: formed further out where ices and gases could also accrete.
Exam questions — 4 questions · 11 marks · AQA 8463 style
Show all working — the AI marks against the AQA mark scheme. Method marks awarded for correct working even if the final answer is wrong.
1 markMain sequence starAQA 8463 style

What process releases energy in a main sequence star like the Sun?

A Nuclear fission of uranium in the core
B Combustion of hydrogen in the core
C Nuclear fusion of hydrogen into helium in the core
D Gravitational collapse continuously releasing energy
4 marksStellar life cycleAQA 8463 P2 style

Describe the life cycle of a star similar to our Sun, from nebula to final state. (4 marks)

Hint: Five stages in order: nebula → protostar → main sequence → red giant → planetary nebula → white dwarf. Give brief explanation of each transition.
+40 XP
1 markLarge star endpointAQA 8463 style

A star much more massive than the Sun will eventually become a:

A White dwarf
B Red giant then planetary nebula
C Supernova, then either a neutron star or black hole
D Double star system
3 marksFormation of solar systemAQA 8463 style

Explain why the inner planets are rocky and the outer planets are gas giants. (3 marks)

Hint: Key concept: temperature gradient. Close to Sun = too hot for gases/ices to stay → rocky planets. Far from Sun = cold enough for gases/ices → gas giants.
+30 XP

Module complete! 🎉

Score loading...

+10 XP