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Lesson 5.3 – Dark Matter & Dark Energy

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 Invisible Majority

Everything we can see — stars, planets, gas — makes up less than 5% of the universe.

The rest is:

  • Dark matter (~27%)

  • Dark energy (~68%)


What Is Dark Matter?

Dark matter:

  • Does not emit or reflect light

  • Interacts via gravity

  • Holds galaxies together

Without dark matter, galaxies would spin so fast that stars would fly apart.

Evidence includes:

  • Galaxy rotation curves

  • Gravitational lensing

  • Large-scale structure of the universe


What Is Dark Energy?

Dark energy is even more mysterious. It appears to:

  • Drive the accelerated expansion of the universe

  • Act opposite to gravity on cosmic scales

We don’t know what dark energy is — only how it behaves.


Why This Matters

Dark matter shapes galaxies.
Dark energy controls the universe’s fate.

Understanding them is one of the greatest challenges in modern physics.


Key Takeaways

  • Most of the universe is invisible

  • Dark matter binds galaxies

  • Dark energy accelerates expansion

  • Major mysteries remain unsolved

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