Mentatcurated
▸ Concept

Nuclear fusion

Energy released when light atomic nuclei join under extreme heat and pressure — the same process that powers stars.

In a nutshell

When two light nuclei — typically isotopes of hydrogen — collide at temperatures above 100 million degrees, they fuse into a heavier nucleus and release far more energy than they required to collide. Unlike fission, the fuel (hydrogen from seawater) is abundant and the waste is short-lived helium. The hard part is confinement: no material can touch plasma at those temperatures, so reactors use magnetic fields or laser pulses to hold it long enough to extract net energy. Commercial fusion has been "decades away" for seventy years because sustaining the plasma costs more energy than it yields — that ratio, Q, is the scoreboard.

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