CH-1020 Chapter 21: Textbook Notes

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Throughout this book we have seen that the identities of atoms remain unchanged. The rapid transformation of energy into matter described by einstein"s famous. 21. 1 changing the identities of atoms in chemical reactions, in keeping with the law of conservation of mass. Now we turn to nuclear reactions, in which atoms" identities do change because their nuclei change. The magnitude of the speed of light (squared) means that nuclear reactions that result in minor changes in mass are accompanied by enormous changes in energy, much greater than those that accompany chemical reactions. Primordial nucleosynthesis created an early universe mainly composed of two elements: hydrogen and helium. More massive nuclei containing up to 26 protons in each nucleus formed later in the cores of the giant stars that populated the first generation of galaxies. Even more massive nuclei formed during the enormous releases of energy that mark the deaths of giant stars, events we know as supernovae.

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