Science
Discover nuclear fusion, the process that powers stars. Learn why this clean, powerful energy source is a major focus of scientific research today.
Nuclear fusion is the cosmic process that powers the sun and all other stars. It occurs when two light atomic nuclei, such as hydrogen, are forced together under extreme pressure and temperature, fusing to form a single heavier nucleus. This process releases a tremendous amount of energy—far more than nuclear fission (the splitting of atoms). On Earth, scientists use hydrogen isotopes like deuterium and tritium as fuel in experimental reactors called tokamaks or stellarators to try and replicate these stellar conditions in a controlled, sustainable way.
Nuclear fusion is trending due to significant scientific breakthroughs. Recently, researchers at facilities like the National Ignition Facility (NIF) in the United States have achieved 'net energy gain' for the first time, meaning the fusion reaction produced more energy than was used to initiate it. This milestone has reignited hope and investment in fusion as a viable future energy source. Global projects like ITER in France are also pushing the boundaries of fusion science, aiming to demonstrate the technology's large-scale potential.
If successfully harnessed, nuclear fusion could revolutionize life on Earth. It promises a virtually limitless source of clean, safe, and carbon-free energy. Unlike fossil fuels, it produces no greenhouse gases. Unlike nuclear fission, it generates no long-lived radioactive waste and carries no risk of meltdown. This could solve the climate crisis, provide energy security for all nations, power space exploration, and usher in a new era of technological advancement and human prosperity. It represents one of humanity's greatest hopes for a sustainable future.