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9th grade The Sun's layers and the fusion that powers it worksheet

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The Sun's layers and the fusion that powers it

Grade 9 Science Worksheet - Challenge Me

NameDate

Circle the best answer.

  1. Power about 3.8 × 10^26 W; c² ≈ 9.0 × 10^16 m²/s². The Sun gives off about 3.8 × 10^26 W (IAU). With E = mc² and c² ≈ 9.0 × 10^16 m²/s², about how much mass becomes energy each second, by Esme's math?

    • About 4 million metric tons
    • About 4 kilograms
    • Zero, since mass is conserved
    • About 4 billion metric tons
  2. Why does the Sun become very slightly less massive over time, by Kira's reading?

    • It burns and loses smoke into space
    • It does not; its mass stays exactly the same
    • Fusion turns some of its mass into energy that leaves as light
    • Fission splits off pieces of the Sun
  3. Luz's friend says the Sun is a giant ball of burning gas, like a campfire. Which response is best?

    • Agree: fire and fusion are the same process
    • Disagree: its energy comes from nuclear fusion in the core
    • Disagree: the Sun runs on fission of uranium
    • Agree: the Sun burns hydrogen with oxygen
  4. A path from the core labeled about 170,000 years, then to Earth labeled about 8 minutes. Milo's cousin says the energy in today's sunlight was released in the core just 8 minutes ago. Which response is best (NASA)?

    • Agree: the radiative zone is empty space
    • Agree: light leaves the core at once
    • Disagree: it took about 170,000 years to leave the Sun first
    • Disagree: it was released 8 hours ago
  5. Noah's friend says the Sun's surface must be its hottest part, since that is where the light comes from. Which response is best?

    • Agree: the core is cold and dark
    • Disagree: the 15 million °C core is far hotter
    • Disagree: the convection zone is the hottest part
    • Agree: light comes from the hottest part
  6. Read this first

    Sun temperatures (NASA)

    LayerTemperature
    coreabout 15 million °C
    photosphereabout 5,500 °C
  7. Using kelvins (°C + 273), about how many times hotter is the Sun's core (15 million °C) than its photosphere (5,500 °C), by Pia's math?

    • The photosphere is the hotter one
    • About 2,700 times
    • About 3 times
    • About 2,600 times
  8. NASA lists the photosphere at about 5,500 °C and the corona, the Sun's outer atmosphere, at up to 2 million °C. Which statement is true, by Ren's reading?

    • The photosphere is the hottest layer outside the core
    • The corona is where fusion happens
    • The corona is cooler, since it is farther from the core
    • The corona is far hotter than the photosphere
  9. Sun surface temperature

    SourceValue
    H-R cardabout 5,800 K
    NASAabout 5,500 °C
  10. The H-R card puts the Sun at about 5,800 K, and NASA lists its surface at about 5,500 °C. Do they agree, by Tala's math?

    • No: they differ by 300 degrees
    • Yes: 5,500 + 273 is about 5,800 K
    • No: 5,800 K must be the core temperature
    • Yes: kelvins and degrees Celsius are the same numbers
  11. Why does fusion need the core's temperature of about 15 million °C, by Zee's reading?

    • Heat lights the hydrogen, as a match lights wood
    • Heat splits helium back into hydrogen
    • Positive nuclei repel; only very fast ones get close enough to fuse
    • Fusion needs oxygen, which only the core has
  12. Core density about 150 g/cm³. NASA gives the core's density as about 150 g/cm³. Why does such high density help fusion, by Ari's reading?

    • Dense matter burns for longer
    • High density splits nuclei apart
    • High density lets light escape the core at once
    • Packed nuclei collide more often
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9th grade The Sun's layers and the fusion that powers it worksheet – printable
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About this worksheet

The Sun's layers and the fusion that powers it. Every version has 10 questions, and the answer key prints on the second page.

What your child will learn

  • I can name the Sun's layers in order and say how energy crosses each one.
  • I can explain fusion (4 hydrogen-1 → helium-4 + energy), tell it from fission and from burning, and use the 0.7% mass loss with E = mc².
  • I can work out light travel times and read the Sun's place on an H-R diagram.

Standard: HS-ESS1-1

Words to know

nuclear fusion: Light nuclei joining into a heavier nucleus, releasing energy

nuclear fission: A heavy nucleus splitting into smaller ones

radiative zone: Inner layer where energy travels as light

convection zone: Outer layer where hot plasma rises and cooler plasma sinks

photosphere: The Sun's visible surface, about 5,500 °C

H-R diagram: A graph of star brightness against surface temperature, hot on the left

Common mistakes

Your child described the Sun as burning like a fire. The Sun's energy comes from nuclear fusion in its core, not from chemical burning, which needs oxygen.

Your child mixed up fusion and fission. Fusion joins light nuclei such as hydrogen into heavier ones; fission splits heavy nuclei such as uranium.

Your child thought the glowing surface is the Sun's hottest part. The core is hottest, about 15 million °C; the photosphere is about 5,500 °C (NASA).

Questions parents ask

What is the most common mistake with the sun's layers and the fusion that powers it?

Your child described the Sun as burning like a fire. The Sun's energy comes from nuclear fusion in its core, not from chemical burning, which needs oxygen.

Are these 9th grade science worksheets free to print?

Yes. All 6 printable versions at each level are free to print, with the answer key, and no account is needed.

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