Why Stars Shine, Simply
32:25–33:33 · 68s
Using E=mc², Galfard gives a crisp, memorable explainer of nuclear fusion: when atomic nuclei fuse, mass vanishes into energy—why the Sun shines and why Earth is warm.
32:25–33:33 · 68s
Using E=mc², Galfard gives a crisp, memorable explainer of nuclear fusion: when atomic nuclei fuse, mass vanishes into energy—why the Sun shines and why Earth is warm.
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