Evolution of Stars from Youth to Old Age

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Across
  1. 1. A star fusing hydrogen into helium in its core
  2. 4. The anti-particle of an electron
  3. 6. When the triple-alpha process results in a quick burst of helium fusion in the core
  4. 8. The largest stars turn into this when the radiative pressure from the core becomes so great that it causes the star to expand
  5. 11. The very small, mysterious particle emitted by nuclear processes that does not interact with normal matter
  6. 12. The positively charged particles in the nucleus of an atom
  7. 14. The next phase of the Sun's life. It will get much bigger and cool down
  8. 15. An area of spacetime so dense that nothing can escape it. Created by the core collapse of the largest stars
  9. 18. The clouds of gas and dust in space that form stars
  10. 19. When the radiative pressure in a red giant's core becomes so great that it begins to shed off the outer layers of its atmosphere
  11. 21. The Sun is technically a yellow __________________
  12. 22. The neutral particle in the nucleus of an atom
  13. 23. The very high energy light produced by nuclear fusion and other high energy processes
Down
  1. 2. Once the core of a red supergiant becomes iron-56, the body of the star collapses then rebounds off of the core, creating this explosion
  2. 3. An incredibly dense left-over of large stars. Only made of neutrons
  3. 5. The leftover core of a red giant that becomes revealed after the production of a planetary nebula
  4. 7. The diagram that plots a star's luminosity against its temperature. Used to organize stars into different categories
  5. 9. A very young star that is still gathering mass from its parent nebula
  6. 10. The nuclear fusion process that involves fusing hydrogen into helium
  7. 13. The end stage of sun-like stars. The universe isn't old enough for these to exist yet
  8. 16. The end product of the triple-alpha process
  9. 17. The most abundant element in the universe. Used by stars as the base of nuclear fusion processes
  10. 20. The negatively charged subatomic particles that orbit the nuclei of atoms