The Sun's layers and the fusion that powers it
Grade 9 Science Worksheet - Challenge Me

Circle the best answer.
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?
- Zero, since mass is conserved
- About 4 kilograms
- About 4 billion metric tons
- About 4 million metric tons
Fusion turns about 0.7% of hydrogen's mass into energy. If 1 kg of hydrogen fuses into helium, about how much mass becomes energy, by Jun's math?
- About 7 g
- About 0.7 g
- 0 g, since mass is conserved
- About 70 g
Why does the Sun become very slightly less massive over time, by Kira's reading?
Star card cutaway with energy arrows leaving the surface. Star card cutaway with energy arrows leaving the surface. energy Star - Fusion turns some of its mass into energy that leaves as light
- It burns and loses smoke into space
- Fission splits off pieces of the Sun
- It does not; its mass stays exactly the same
Luz's friend says the Sun is a giant ball of burning gas, like a campfire. Which response is best?
Two panels: a campfire; the Sun's core with nuclei joining. Two panels: a campfire; the Sun's core with nuclei joining. campfire Sun's core - Disagree: its energy comes from nuclear fusion in the core
- Agree: the Sun burns hydrogen with oxygen
- Disagree: the Sun runs on fission of uranium
- Agree: fire and fusion are the same process
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: 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
- Agree: the radiative zone is empty space
Read this first
Sun temperatures (NASA)
Layer Temperature core about 15 million °C photosphere about 5,500 °C 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?
- About 3 times
- About 2,600 times
- The photosphere is the hotter one
- About 2,700 times
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 corona is far hotter than the photosphere
- The corona is cooler, since it is farther from the core
- The corona is where fusion happens
- The photosphere is the hottest layer outside the core
Sun surface temperature
Source Value H-R card about 5,800 K NASA about 5,500 °C 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
- No: 5,800 K must be the core temperature
- Yes: kelvins and degrees Celsius are the same numbers
- Yes: 5,500 + 273 is about 5,800 K
Why does fusion need the core's temperature of about 15 million °C, by Zee's reading?
Two positive nuclei moving fast toward each other, with repelling arrows between them. Two positive nuclei moving fast toward each other, with repelling arrows between them. positive nuclei + + - Positive nuclei repel; only very fast ones get close enough to fuse
- Fusion needs oxygen, which only the core has
- Heat splits helium back into hydrogen
- Heat lights the hydrogen, as a match lights wood
What keeps the Sun from collapsing under its own gravity, by Bo's reading (NASA)?
Star card cutaway with gravity arrows pointing in and pressure arrows pointing out. Star card cutaway with gravity arrows pointing in and pressure arrows pointing out. gravity - Burning gases push outward like exhaust from a rocket engine
- Nothing; the Sun is collapsing quickly
- Fission blasts push it apart
- Outward pressure from fusion-heated gas balances gravity