Stellar Evolution Review

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Across
  1. 6. the sun is categorized as this type of star
  2. 11. Supernovae are the only natural way that elements heavier than ______ are created
  3. 13. type 2 supernovae require _________ star(s)
  4. 14. this is the order of the letters for stellar classifications
  5. 15. in order to fuse hydrogen into helium, the core of a star needs to reach 15 _______ Kelvin
  6. 16. this type of star changes in brightness
  7. 18. this area of the H-R Diagram is where most stars fall.
  8. 21. after hydrogen, the most common element in stars is
  9. 22. given a fixed volume, if pressure increases then ___________ increases
  10. 23. a star will fuse helium much _____________ than hydrogen
  11. 24. fusing helium produces more ____________ than fusing hydrogen
  12. 25. A blue star is typically ___________ than a red star
  13. 28. this section of the Hertzsprung-Russell Diagram is below the main sequence
  14. 32. The energy of fusing in the core of stars is the only thing preventing a star from dying due to its own ______________
  15. 33. The Sun’s stellar classification is _______
  16. 34. type 2 supernovae that create black holes must start with a mass of _________________ times more than the Sun
  17. 35. stars with more mass live much _________ lives than low mass stars
Down
  1. 1. over half of the stars in the night sky are in a ___________ system (they have a companion)
  2. 2. K type stars are typically what color?
  3. 3. this is the stage of a low mass star after the red giant phase
  4. 4. there are _________ high mass stars than there are low mass stars
  5. 5. fusing iron (or in some cases, carbon) causes this to happen
  6. 7. this type of supernova is the result of one star accreting mass from a companion
  7. 8. Given a fixed temperature, if pressure increases then _______________ decreases
  8. 9. a magnitude 2.5 star is ____________ than a magnitude 3.5 star
  9. 10. Compared to other stars, the Sun is relatively _________ in size
  10. 12. The Sun will ends its life cycle as a white dwarf with carbon and _________ as the only remaining elements
  11. 17. Betelgeuse is this type of star (color and size)
  12. 19. the force that keeps white dwarfs from collapsing is called electron ___________ pressure which occurs because electrons don’t like being near each other
  13. 20. O type stars are typically what color?
  14. 26. type 1a supernovae require _________ star(s)
  15. 27. there are about 200 ________ stars in the Milky Way
  16. 29. In a massive star, it takes a single _____ to fuse all silicon into iron
  17. 30. this is the name of the stage of a star before it starts fusing hydrogen
  18. 31. Hot stars are typically brighter or more ____________ than cooler stars