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Lesson 3.3 – Space Weather & Auroras

16 Dec 2025 Module 3: Earth and Space
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Part of a Module

This lesson is part of Module 3: Earth and Space. Take it in course mode for progress tracking and the end-of-module exam.

What Is Space Weather?

Space weather refers to conditions in space driven by the Sun’s activity, particularly:

  • Solar flares

  • Coronal mass ejections (CMEs)

  • Solar wind

These events send charged particles toward Earth.


Earth’s Magnetic Field

Earth is surrounded by a magnetosphere, generated by its molten iron core. This magnetic field:

  • Deflects charged particles

  • Protects the atmosphere

  • Guides particles toward the poles


How Auroras Form

When solar particles collide with atmospheric gases near the poles, they release energy as light.

  • Oxygen → green/red

  • Nitrogen → blue/purple

This creates the Aurora Borealis and Aurora Australis.


Why Space Weather Matters

Strong solar storms can:

  • Disrupt satellites

  • Knock out power grids

  • Interfere with radio communication

Understanding space weather helps protect modern technology.


Key Takeaways

  • Space weather comes from the Sun

  • Earth’s magnetic field protects us

  • Auroras are a visible result of solar activity

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