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β’οΈ Nuclear fusion is the process where two light atomic nuclei combine to form a heavier nucleus, releasing tremendous energy in the process.
π The Sun produces energy through nuclear fusion, where hydrogen nuclei fuse to create helium.
βοΈ Fusion reactions require extremely high temperatures, often exceeding 100 million degrees Celsius, to overcome the repulsion between positively charged nuclei.
π One of the fuel sources for fusion is isotopes of hydrogen, such as deuterium and tritium.
π If harnessed for energy, nuclear fusion could provide a nearly limitless, clean energy source with minimal environmental impact.
π Experimental fusion reactors like ITER aim to demonstrate the feasibility of fusion as a commercially viable energy source.
π‘ Unlike nuclear fission, which splits heavy nuclei, fusion combines them, producing less long-lived radioactive waste.
π§ͺ Scientists have achieved controlled fusion in laboratories, but sustained and efficient reactions are still under research.
β³ Fusion reactions occur in stars and are responsible for the creation of heavier elements in the universe through stellar nucleosynthesis.
π The Lawson Criterion determines the conditions necessary for fusion to occur, focusing on temperature, density, and confinement time.
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