Round 1
Round 2
Round 3
Round 4
Round 5
100

What shape do planetary orbits take?

Ellipses (oval-shaped orbits).

100

What is a moon?

A natural satellite that orbits a planet.

100

Name the five planets visible without a telescope.

Mercury, Venus, Mars, Jupiter, and Saturn.

100

Which model places Earth at the centre of the universe?

The geocentric model.

100

What causes the phases of the Moon?

We see different amounts of the Moon’s lit side as it orbits Earth.

200

Who discovered that planets move in elliptical orbits?

Johannes Kepler.

200

Name a planet that has no moons.

Mercury or Venus.

200

Why didn’t ancient astronomers include Earth in this list?

They thought Earth was the centre (geocentric model) and we cannot see Earth move from Earth.

200

Which scientist first proposed the heliocentric model?

Nicolaus Copernicus.

200

Why is there a “new moon” phase even though the Moon is still there?

During a new moon, the side facing Earth is dark because sunlight is hitting the far side only.

300

Why do planets move faster when closer to the Sun?

The Sun’s gravity is stronger at closer distances, pulling harder → greater acceleration → higher orbital speed.

300

Why do gas giants tend to have many more moons than rocky planets?

They have much stronger gravity, so they can capture and hold more moons.

300

Why can’t Uranus or Neptune be seen with the naked eye?

They are too far away and too dim to be seen without telescopes.

300

Give one piece of evidence that proved the geocentric model wrong.

Galileo saw moons orbiting Jupiter.

300

Why don’t we get a solar eclipse every new moon?

The Moon’s orbit is tilted, so its shadow usually misses Earth.

400

What does the word “orbit” mean?

The curved path an object follows as it moves around another object due to gravity.

400

Why doesn’t the Moon fly off into space even though Earth is moving?

Earth’s gravity keeps the Moon in orbit;

400

List all five visible planets in order from the Sun.

  1. Mercury

  2. Venus

  3. Mars

  4. Jupiter

  5. Saturn

400

Why did the geocentric model seem correct to early astronomers?

Because the Sun and stars appear to move around Earth, and Earth feels still.

400

What is the difference between waxing and waning?

  • Waxing = the lit part seen from Earth is increasing.

  • Waning = the lit part seen from Earth is decreasing.

500

Explain why gravity alone cannot produce a circular orbit for most planets.

  • Distances from the Sun vary slightly as planets move.

  • Their speed changes depending on distance.

  • These variations create ellipses rather than circles.

500

Explain the difference between a moon’s orbital period and a planet’s rotation period.

  • Orbital period = time the Moon takes to go around Earth.

  • Rotation period = time the Moon or a planet takes to spin once on its axis.

500

Explain why these planets were called “wandering stars.”

They appear to move across the night sky differently from stars (change position relative to stars), so ancient astronomers thought they wandered.

500

State two variables that the gravitational force between two objects depends on. 

Distance between the two objects and the mass between the two objects. 

500

Explain in detail why we always see the same side of the Moon from Earth.

Its rotation period equals its orbital period, so the same side always faces Earth.

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