The Sun's life from start to finish

Grade 9 Science Worksheet

NameDate

Circle the best answer.

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

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

    • It will grow heavy enough to explode
    • It will run out of the oxygen it needs to burn
    • Its core will run out of hydrogen to fuse
    • Its fuel will run out, so it will go dark at once
  4. “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
  5. “sources give 7 to 10” Why will the Sun not end as a supernova, by Milo's reading (NASA)?

    • It has too little mass; only far heavier stars explode
    • It already exploded long ago
    • It will explode once it becomes a red giant
    • It is too hot to explode
  6. 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?

    • Cooler and redder, though the star is far brighter
    • Hotter and whiter, since the star becomes so much bigger
    • Hotter and dimmer
    • Exactly the same
  7. Drawing of a huge red giant beside a small yellow star. Why is a red giant so bright if its surface is cool, by Pia's reading?

    • Its surface is hotter than the Sun's is now
    • Its surface is the hottest of any stage
    • Its huge surface area gives off a lot of light
    • It reflects light from nearby planets
  8. A young white dwarf has a hotter surface than the Sun today but is far dimmer. Why, by Ren's reading?

    • It fuses hydrogen at its surface
    • It is tiny, about Earth's size, with little surface
    • Its surface is colder than ice
    • It is still fusing, but slowly
  9. 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 drift away as a planetary nebula
    • They explode in a supernova
    • They stay and keep fusing hydrogen
  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 hydrogen, as the Sun is now
    • Iron, from fusion up the periodic table
    • Mostly carbon, made by helium fusion
    • 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. 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 23 hours, near the end
    • About 11 hours
    • About 4.6 hours
  2. On Jun's timeline, 1 m stands for 1 billion years. How far from the Sun's formation is now?

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

    • It will grow heavy enough to explode
    • It will run out of the oxygen it needs to burn
    • Its core will run out of hydrogen to fuse
    • Its fuel will run out, so it will go dark at once
  4. “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
  5. “sources give 7 to 10” Why will the Sun not end as a supernova, by Milo's reading (NASA)?

    • It has too little mass; only far heavier stars explode
    • It already exploded long ago
    • It will explode once it becomes a red giant
    • It is too hot to explode
  6. 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?

    • Cooler and redder, though the star is far brighter
    • Hotter and whiter, since the star becomes so much bigger
    • Hotter and dimmer
    • Exactly the same
  7. Drawing of a huge red giant beside a small yellow star. Why is a red giant so bright if its surface is cool, by Pia's reading?

    • Its surface is hotter than the Sun's is now
    • Its surface is the hottest of any stage
    • Its huge surface area gives off a lot of light
    • It reflects light from nearby planets
  8. A young white dwarf has a hotter surface than the Sun today but is far dimmer. Why, by Ren's reading?

    • It fuses hydrogen at its surface
    • It is tiny, about Earth's size, with little surface
    • Its surface is colder than ice
    • It is still fusing, but slowly
  9. 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 drift away as a planetary nebula
    • They explode in a supernova
    • They stay and keep fusing hydrogen
  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 hydrogen, as the Sun is now
    • Iron, from fusion up the periodic table
    • Mostly carbon, made by helium fusion
    • Neutrons packed tightly together