← Back to subjects
0
Edexcel GCSE Astronomy (1AS0) · Exploring the Moon
Mini-Lesson

Exploring the Moon

Topic 9 opens Paper 2. It covers what the Moon is like to visit, how we have explored it with robots and astronauts, what the rock samples told us, and the giant impact theory of how the Moon formed.

no atmosphere no sound, no weather, no erosion, black sky gravity ≈ 1/6 g 1.62 m/s² — an 80 kg astronaut weighs 130 N extreme temperatures about +120 °C by day, −150 °C at night

Work through each screen, answer the questions as you go (some are wordy, some are calculations) and collect ⭐ stars. Press Start when you're ready.

Exploring the Moon · conditions

What it is like on the Moon

The Moon is a hostile place, and almost everything about it follows from one fact: it has essentially no atmosphere (its gravity is too weak to hold gas).

  • No air → no sound, no wind, no weather, no erosion, and a black sky even in daylight (no scattering).
  • Surface gravity 1.62 m/s², about 1/6 of Earth's. Astronauts bounce; a dropped hammer and feather fall together.
  • Temperature swings from roughly +120 °C in sunlight to −150 °C at night — and the lunar night lasts about a fortnight.
  • No global magnetic field and no atmosphere → the surface is fully exposed to the solar wind, cosmic rays and micrometeorites.
  • Regolith — sharp, abrasive dust that clung to Apollo suits, jammed seals and abraded visors.

Water ice has been detected in permanently shadowed craters near the lunar poles — a huge deal, because it could supply drinking water, oxygen and rocket fuel to a future base.

Calculate

Your turn — weight on the Moon

1Lunar surface gravity is 1.62 N/kg. Calculate the weight of an 80 kg astronaut standing on the Moon.
N
Hint: weight = mass × gravitational field strength = 80 × 1.62. (On Earth the same astronaut weighs about 784 N.)
Quick check

A black daytime sky

?Apollo photographs taken in bright sunlight show a completely black sky with no stars visible. Why is the sky black?
Exploring the Moon · missions

Robots and astronauts

The Moon has been explored in two very different ways.

  • Robotic probesLuna 3 photographed the far side (1959); Surveyor landers proved the surface would take a spacecraft's weight; the Lunar Reconnaissance Orbiter has mapped the whole Moon in fine detail; Lunokhod and Yutu rovers drove across it; Luna 16 and Chang'e 5 returned samples automatically.
  • Crewed landings — six Apollo missions landed between 1969 and 1972. Apollo 11 touched down in the Sea of Tranquillity (Mare Tranquillitatis) in July 1969. Later crews drove the Lunar Roving Vehicle and left experiment packages — including retroreflectors still used today to laser-range the Moon to a few centimetres.
Apollo brought back 382 kg of lunar rockthe single most valuable scientific result of the programme

The trade-off — a classic 6-marker. Robots: far cheaper, no risk to life, can survive years and go anywhere. Astronauts: adaptable, can choose the best samples, do field geology, fix things — but need life support, cost billions and can die.

Calculate

Your turn — radio delay

2The Moon is 384 400 km away and radio waves travel at 300 000 km/s. Calculate the time for a radio signal to travel one way from Earth to the Moon, in seconds (1 decimal place).
s
Hint: time = distance ÷ speed = 384 400 ÷ 300 000. (A round trip — question and answer — takes about 2.6 s.)
Exploring the Moon · origin

Where did the Moon come from?

The Apollo samples were the key evidence. They showed lunar rock is:

  • Chemically very like the Earth's mantle — in particular the oxygen isotope ratios match the Earth's almost exactly, which is not true of meteorites from elsewhere.
  • Completely dry — no water-bearing minerals — and depleted in iron and other dense metals.
  • Very old, and once molten (the surface was a magma ocean).

The theory that fits all of this is the giant impact hypothesis: about 4.5 billion years ago a Mars-sized body struck the young Earth a glancing blow. Debris blasted from the mantles of both bodies went into orbit and coalesced into the Moon. That explains the matching isotopes (same material), the missing iron (the impactor's core sank into the Earth) and the bone-dry rock (volatiles boiled away).

Rejected rivals: capture (hard to slow a passing body down, and the isotopes would not match), co-formation (would give the Moon an iron core like the Earth's), and fission (the Earth would have to spin impossibly fast).

Quick check

The best evidence

?Which piece of evidence most strongly supports the giant impact theory over the idea that the Moon was captured?
Quick check

Robot or human?

?Which is a genuine scientific advantage of sending astronauts rather than robots to the Moon?
Sort it

Sort the statements

Tap a statement, then tap where it belongs.

🤖 Robotic advantage

👩‍🚀 Crewed advantage

🌑 Lunar condition

Match it

Match the description to the term

Tap a description on the left, then its matching term on the right.

Description
Term
Quick check

Why go back?

?Why is the discovery of water ice in permanently shadowed polar craters so important for a future lunar base?
Exploring the Moon · lunar science

What the experiments revealed

Apollo did far more than plant flags. Each crew left an ALSEP experiment package behind:

  • Seismometers detected "moonquakes" and let scientists work out the Moon's internal structure — a thick crust (thicker on the far side), a deep mantle and a small, partly molten iron core. That small core is exactly what the giant impact theory predicts.
  • Retroreflectors — corner-cube mirrors that bounce a laser pulse straight back. By timing the round trip, the Earth-Moon distance is now known to a few centimetres. The result: the Moon is drifting away from us at about 3.8 cm per year, and the Earth's day is very slowly lengthening (tidal friction).
  • Solar wind collectors — foil sheets exposed to trap solar wind particles for analysis back on Earth.

Why the Moon has no magnetic field: its core is small and has largely solidified, so it cannot sustain a dynamo. With no magnetic field and no atmosphere, the surface is left utterly unprotected from the solar wind and cosmic rays.

Calculate

Your turn — a retreating Moon

3Laser ranging shows the Moon recedes from the Earth by 3.8 cm each year. How much further away, in km, would it be after 1 000 000 years, if the rate stayed the same?
km
Hint: 3.8 cm × 1 000 000 = 3 800 000 cm. There are 100 000 cm in a km, so divide by 100 000.
Quick check

Why no magnetic field?

?Why does the Moon have no global magnetic field today?
Recap

The big ideas to know

Conditions: no atmosphere, ~1/6 Earth gravity, huge temperature range, no magnetic field, unshielded radiation, abrasive regolith

Apollo: six crewed landings 1969-72; Apollo 11 landed in the Sea of Tranquillity in July 1969

Samples: 382 kg of Moon rock; identical oxygen isotopes to Earth rock, but bone dry and iron-poor

Giant impact theory: a Mars-sized body struck the young Earth; debris from the mantle formed the Moon

Robotic probes: cheaper, no risk to life, can last for years — but slow to react

Crewed missions: flexible, can select samples and react to surprises — but hugely expensive and dangerous

Radio delay: the Moon is 384 400 km away, so a signal takes about 1.3 s each way

That is Exploring the Moon covered for Edexcel GCSE Astronomy. Press Finish to see your score.

🏆

Mini-lesson complete!

⭐⭐⭐

You have worked through Exploring the Moon for Edexcel GCSE Astronomy. 🎉

Your stars: 0 / 0

Next: test yourself in the Evaluate stage Confidence Quiz, then lock it in with Verify.

📣 Smashed it? Share your score

Challenge a mate to beat your stars, or show a parent how you got on.

→ Back to all subjects