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The Triple Challenge: Temperature, Density, Time

Learn why achieving fusion requires balancing three impossible conditions simultaneously

Part of Build A Star: The Nuclear Fusion Revolution

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The Three-Way Problem

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The Three-Way Problem

To achieve fusion, you need three conditions simultaneously:

1. Temperature: ~100-150 million Kelvin

  • Atoms must move fast enough to overcome repulsion

2. Density: Enough particles colliding per second

  • Need ~10²⁰ particles per cubic meter

3. Confinement Time: Hold plasma stable long enough

  • Need >1 second for magnetic, nanoseconds for inertial

The Lawson Criterion: n × τ × T ≥ 3×10²¹

Miss any one condition = no fusion power. This is why fusion is so hard.

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Quiz: 3 Questions

Test your understanding with this quiz.

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Why can't we just use the Sun's temperature (15 million K) for Earth-based fusion?

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Choose Your Reactor Strategy

Complete this exercise and get AI-powered feedback.

Choose Your Reactor Strategy

You're leading a fusion startup. Choose between magnetic confinement or inertial confinement, understanding the Lawson criterion trade-offs.

Think about: Risk vs reward, cost, timeline, technical challenges, and market timing.

Key insight: In breakthrough innovation, there's rarely one "right" answer—it's about choosing which constraints to optimize for.