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Eduqas GCSE Physics (C420P) · Topic 10 — Space physics
Mini-Lesson

Space Physics

This mini-lesson covers the whole of Eduqas Topic 10 — Space physics: the Solar System and our place in the Universe, how gravity keeps things in orbit, the stability of orbits and satellites, and the red-shift evidence for an expanding Universe, the Big Bang and the cosmic microwave background.

Solar System red-shift evidence the Universe is expanding galaxies

Work through each screen, answer the questions as you go (some are reasoning, some are calculations) and collect ⭐ stars. Items marked Higher tier are for the higher paper only. Press Start when you're ready.

The Solar System

Our cosmic address

Our Solar System is held together by gravity acting around the Sun — our nearest star. It contains:

  • the Sun (a star) at the centre;
  • eight planets — four inner rocky planets (Mercury, Venus, Earth, Mars) and four outer gas giants (Jupiter, Saturn, Uranus, Neptune);
  • dwarf planets such as Pluto, which has a small irregular orbit;
  • moons (natural satellites) that orbit planets — Earth has one;
  • asteroids (rocky debris, many in the belt between Mars and Jupiter) and comets (icy bodies on long, very elliptical orbits).

Zoom out: the Sun is just one of hundreds of billions of stars in our galaxy, the Milky Way — and the Milky Way is just one of billions of galaxies in the Universe.

Sort it

Name that body

Tap the word that best describes each member of the Solar System.

Orbital motion

Gravity is the string

A planet, moon, comet or artificial satellite moves in a (near-)circular orbit. Even at constant speed its velocity is always changing, because its direction is always changing. A changing velocity means it is accelerating — so a resultant force must be acting.

That force is gravity, and it always points towards the central body. A force directed to the centre of a circle is called the centripetal force.

central body orbiting body gravity = centripetal force velocity (tangent) radius r
Velocity points along the tangent; gravity (the centripetal force) points to the centre.

Misconception buster: an orbiting body is not "weightless because there's no gravity". It is constantly falling towards the central body — gravity provides the centripetal force — but its sideways (tangential) speed means it keeps missing, so it loops round.

Stable orbits

Smaller orbit, faster speed

For a stable orbit at a given radius, the body must travel at exactly the right speed so that gravity provides the centripetal force needed to curve it round. This links speed to radius:

smaller radius → faster orbita body in a smaller (closer) orbit must move faster; a body in a larger (further) orbit moves more slowly

That is why Mercury races round the Sun far faster than distant Neptune, and why a low satellite zips round the Earth in about 90 minutes while the far-off Moon takes about a month.

Misconception buster: if an orbiting body speeds up, it can no longer stay at the same radius — to stay stable its orbit radius must change. For a given radius there is only one stable orbital speed.

Quick check

Which moon is fastest?

?Two moons orbit the same planet in stable circular orbits. Moon A is close to the planet; Moon B is far away. Which orbits at the greater speed, and why?
Calculate

Speed on a circular orbit

1A satellite travels once around a circular orbit of circumference 42 000 km in a time of 6000 s. Calculate its orbital speed in km/s. (speed = distance ÷ time)
km/s
Hint: speed = 42 000 ÷ 6000.
Red-shift

Stretched light

Hot elements in a star produce a pattern of spectral lines at fixed wavelengths — a fingerprint of the chemicals present. If the source is moving away from us, its light waves are stretched, so every line shifts towards the red (longer-wavelength) end. This is red-shift.

Reference (lab) spectrum Distant galaxy — lines red-shifted → same line pattern, shifted towards the red (longer-wavelength) end
The galaxy's lines sit at the same pattern but shifted towards red — it is moving away.

Misconception buster: the colour of the star doesn't simply "turn red". Red-shift means the whole spectral-line pattern moves towards longer wavelengths because space between us and the galaxy is stretching the light's wavelength.

Expanding Universe

The further, the faster

Light from distant galaxies is red-shifted, so almost every galaxy is moving away from us. Crucially:

more distant galaxy → greater red-shiftthe further away a galaxy is, the faster it is receding from us

This is exactly what you expect if space itself is expanding — every galaxy gets carried away from every other one. So red-shift is strong evidence that the Universe is expanding, which supports the Big Bang theory: the Universe began about 13.8 billion years ago from a tiny, hot, dense point and has been expanding ever since.

Misconception buster: galaxies are not flying through fixed space away from a central explosion. The space between galaxies is stretching, which stretches the light's wavelength — and the more space there is in between (more distant), the faster the recession.

Quick check

What does more red-shift tell us?

?Galaxy X shows a larger red-shift than Galaxy Y. What can we conclude?
Higher tier · Calculate

How much is a line shifted?

2A spectral line measured in the lab at 600 nm appears at 630 nm in a galaxy's spectrum. By how many nm has the line been red-shifted? (change in wavelength = observed − reference)
nm
Hint: 630 − 600. A positive shift to longer wavelength is a red-shift.
Big Bang evidence

The afterglow: CMB

If the Universe really did begin in a hot, dense Big Bang, the radiation released should still be detectable today. It is: the cosmic microwave background (CMB) — faint microwave radiation coming from every direction in space, first detected in 1964.

As the Universe expanded, this radiation was stretched (red-shifted) from short-wavelength, high-energy radiation into the microwaves we detect now. The CMB can only be explained by the Big Bang, so it is powerful supporting evidence.

Two pillars of Big Bang evidence:

1. Red-shift of distant galaxies → the Universe is expanding.

2. Cosmic microwave background → leftover radiation from the hot early Universe.

Quick check

Why does the CMB matter?

?The cosmic microwave background (CMB) is described as evidence for the Big Bang. What makes it such strong evidence?
Quick check

What keeps it in orbit?

?A comet sweeps round the Sun on a long elliptical orbit at constant speed near its furthest point. Which statement is correct?
Sort it

Big Bang evidence — or not?

Tap a statement, then tap the box it belongs in.

✅ Supports the Big Bang

🚫 Not evidence

Recap

The big ideas to know

Solar System: Sun + 8 planets, dwarf planets, moons, asteroids, comets — held by gravity; we sit in the Milky Way galaxy.

Orbits: gravity provides the centripetal force; velocity always changes (direction changes) even at constant speed.

Stable orbits: smaller radius → faster orbital speed; for a given radius there is one stable speed.

Red-shift: distant galaxies' light is stretched to longer wavelengths; more distant → greater red-shift → faster recession.

Expanding Universe + Big Bang: red-shift shows expansion and supports the Big Bang (~13.8 billion years ago).

CMB: microwave afterglow from every direction — further Big Bang evidence.

You've covered both parts of Eduqas Topic 10 — the Solar System & orbital motion, and red-shift, the expanding Universe & the Big Bang. Press Finish to see your score.

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Mini-lesson complete!

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You've worked through Space Physics for Eduqas GCSE Physics. 🎉

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