The Sun's life from start to finish

Grade 9 Science Worksheet

NameDate

Circle the best answer.

  1. The Sun is 4.6 billion years into a 10-billion-year main sequence. About what percent has it used, by Bo's math?

    • About 46%
    • About 90%, so it ends soon
    • About 4.6%
    • About 100%, so it is nearly done
  2. If the Sun's 10-billion-year main sequence were one 24-hour day, about how many hours would have passed so far, by Esme's math?

    • About 1 hour
    • About 11 hours
    • About 4.6 hours
    • About 23 hours, near the end
  3. On Jun's timeline, 1 m stands for 1 billion years. How far from the Sun's formation is now?

    • 46 m
    • 4.6 mm
    • 0.46 m
    • 4.6 m
  4. Hydrogen fusing into helium. Why will the Sun leave the main sequence, by Kira's reading (NASA)?

    • It will grow heavy enough to explode
    • Its fuel will run out, so it will go dark at once
    • It will run out of the oxygen it needs to burn
    • Its core will run out of hydrogen to fuse
  5. “Star card cutaway:” When the core runs out of hydrogen, gravity squeezes it. What happens next, by Luz's reading (NASA)?

    • The outer layers cool and shrink
    • The core heats up and the outer layers swell
    • The core explodes as a supernova
    • The whole Sun shrinks and goes completely dark
  6. “sources give 7 to 10” Why will the Sun not end as a supernova, by Milo's reading (NASA)?

    • It already exploded long ago
    • It will explode once it becomes a red giant
    • It has too little mass; only far heavier stars explode
    • It is too hot to explode
  7. The Sun today beside a red giant, with surface colors shown. Compared with the Sun today, how does a red giant's surface compare, by Noah's reading?

    • Exactly the same
    • Hotter and dimmer
    • Cooler and redder, though the star is far brighter
    • Hotter and whiter, since the star becomes so much bigger
  8. What becomes of the Sun's outer layers at the end of its red giant stage, by Tala's reading (NASA)?

    • They collapse into a black hole around the core
    • They explode in a supernova
    • They stay and keep fusing hydrogen
    • They drift away as a planetary nebula
  9. Star card cutaway of a white dwarf. What fuses inside a white dwarf, by Zee's reading (NASA)?

    • Hydrogen into helium
    • Nothing; it glows from stored heat as it cools
    • Carbon into iron
    • Helium into carbon, as in a red giant
  10. Red giant core fusing helium into carbon, then the white dwarf left behind. Mostly what will the Sun's white dwarf be made of, by Ari's reading (NASA)?

    • Mostly carbon, made by helium fusion
    • Iron, from fusion up the periodic table
    • Mostly hydrogen, as the Sun is now
    • Neutrons packed tightly together
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The Sun's life from start to finish

Answer Key - Grade 9 Science Worksheet

Circle the best answer.

  1. The Sun is 4.6 billion years into a 10-billion-year main sequence. About what percent has it used, by Bo's math?

    • About 46%
    • About 90%, so it ends soon
    • About 4.6%
    • About 100%, so it is nearly done
  2. If the Sun's 10-billion-year main sequence were one 24-hour day, about how many hours would have passed so far, by Esme's math?

    • About 1 hour
    • About 11 hours
    • About 4.6 hours
    • About 23 hours, near the end
  3. On Jun's timeline, 1 m stands for 1 billion years. How far from the Sun's formation is now?

    • 46 m
    • 4.6 mm
    • 0.46 m
    • 4.6 m
  4. Hydrogen fusing into helium. Why will the Sun leave the main sequence, by Kira's reading (NASA)?

    • It will grow heavy enough to explode
    • Its fuel will run out, so it will go dark at once
    • It will run out of the oxygen it needs to burn
    • Its core will run out of hydrogen to fuse
  5. “Star card cutaway:” When the core runs out of hydrogen, gravity squeezes it. What happens next, by Luz's reading (NASA)?

    • The outer layers cool and shrink
    • The core heats up and the outer layers swell
    • The core explodes as a supernova
    • The whole Sun shrinks and goes completely dark
  6. “sources give 7 to 10” Why will the Sun not end as a supernova, by Milo's reading (NASA)?

    • It already exploded long ago
    • It will explode once it becomes a red giant
    • It has too little mass; only far heavier stars explode
    • It is too hot to explode
  7. The Sun today beside a red giant, with surface colors shown. Compared with the Sun today, how does a red giant's surface compare, by Noah's reading?

    • Exactly the same
    • Hotter and dimmer
    • Cooler and redder, though the star is far brighter
    • Hotter and whiter, since the star becomes so much bigger
  8. What becomes of the Sun's outer layers at the end of its red giant stage, by Tala's reading (NASA)?

    • They collapse into a black hole around the core
    • They explode in a supernova
    • They stay and keep fusing hydrogen
    • They drift away as a planetary nebula
  9. Star card cutaway of a white dwarf. What fuses inside a white dwarf, by Zee's reading (NASA)?

    • Hydrogen into helium
    • Nothing; it glows from stored heat as it cools
    • Carbon into iron
    • Helium into carbon, as in a red giant
  10. Red giant core fusing helium into carbon, then the white dwarf left behind. Mostly what will the Sun's white dwarf be made of, by Ari's reading (NASA)?

    • Mostly carbon, made by helium fusion
    • Iron, from fusion up the periodic table
    • Mostly hydrogen, as the Sun is now
    • Neutrons packed tightly together