PTE · Listening: Fill in the Blanks

The Origin of the Moon: PTE Listening: Fill in the Blanks practice questions

3 original Listening: Fill in the Blanks questions. Answer every question, then check them for your score and the answers. It is free with no login; create a free account to save your score and get a BandLadder AI score for speaking and writing.
  • 3 questions
  • Free, with answers
  • PTE Academic and PTE Core
  • Updated Oct 2026

You will hear a recording. Type the missing word in each gap.

1

Giant Impact Hypothesis

Speaker: Indian English

Plays once, as in the test: no pausing or replay

0:00 / 0:42

For many decades astronomers struggled to explain how the Earth acquired such a large satellite. The leading model today suggests that a Mars sized protoplanet collided with the infant Earth around four and a half billion years ago. This violent collision released an amount of energy, vaporising outer rock layers and ejecting molten debris into orbit. Over several thousand years, gravity pulled this orbiting together to form a solid body. Computer simulations indicate that this catastrophic event explains both the angular momentum of our planetary system and the relatively small metallic core found inside the lunar today, supporting the idea of a shared history.

2

Lunar Magma Ocean Evolution

Speaker: British English

Plays once, as in the test: no pausing or replay

0:00 / 0:47

Shortly after its formation from colliding debris, the infant Moon was likely enveloped by a global ocean of molten rock. As this deep layer began to cool, mineral crystals separated based on their relative within the liquid melt. Denser iron rich minerals sank downward toward the developing mantle, while lighter plagioclase feldspar floated toward the surface. This continuous flotation created the bright anorthosite crust that remains visible across the lunar highlands. Geochemists analyse returned surface samples to reconstruct the rate of this ancient ocean, which provides critical regarding early planetary and internal thermal history across the inner solar system.

3

Isotopic Composition and Planetary Mixing

Speaker: American English

Plays once, as in the test: no pausing or replay

0:00 / 0:39

One of the greatest challenges facing scientists studying lunar origins is the remarkable geochemical similarity between terrestrial and lunar samples. When researchers examine the of oxygen and titanium isotopes in Apollo rocks, they find values nearly identical to those on Earth. If a foreign impacting body had contributed most of the material, subtle chemical differences should be clearly today. This paradox has led theorists to propose models involving extreme high energy impacts that produced complete vaporisation and thorough between the early planet and the colliding body, thereby the isotopic signatures across the entire system.

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