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Lesson 5.2 – The Expanding Universe

16 Dec 2025 Module 5: Galaxies and the Universe
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Part of a Module

This lesson is part of Module 5: Galaxies and the Universe. Take it in course mode for progress tracking and the end-of-module exam.

The Big Bang Theory

The Big Bang describes how the universe began 13.8 billion years ago in an extremely hot, dense state and has been expanding ever since.

Importantly:

  • The Big Bang was not an explosion in space

  • It was an expansion of space itself


Evidence for the Big Bang

Three major observations support this model:

  1. Galaxy redshift
    Distant galaxies are moving away from us — the farther they are, the faster they recede.

  2. Cosmic Microwave Background (CMB)
    Faint radiation left over from the early universe, visible in all directions.

  3. Element abundance
    The observed amounts of hydrogen and helium match predictions.


What Does “Expansion” Mean?

Expansion does not mean galaxies are moving through space away from a central point. Instead:

  • Space itself is stretching

  • Distances between galaxies increase

  • No centre or edge exists

A common analogy is dots on the surface of a balloon as it inflates.


The Observable Universe

Because light travels at a finite speed, we can only see part of the universe. This region is called the observable universe.

Beyond it, space may continue — but we cannot observe it yet.


Key Takeaways

  • The universe is expanding

  • The Big Bang explains cosmic origins

  • Expansion affects all large-scale distances

  • We can only observe part of the universe

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