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<p>than that of four atoms of hydrogen, and that the <a href="page.php?w=mass-energy_equivalence">mass-energy equivalence</a> of Einstein implies that the nuclear fusion (4 H -> He) could liberate sufficient energy to make stars shine for billions of years. A similar theory was first proposed by American chemist <a href="page.php?w=William_Draper_Harkins">William Draper Harkins</a> in 1915. It remained for <a href="page.php?w=Hans_Bethe">Hans Bethe</a> and <a href="page.php?w=Carl_Friedrich_von_Weizs%C3%A4cker">Carl Friedrich von Weizsäcker</a> to</p><p>
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