The Sun's life from start to finish
Grade 9 Science Worksheet

Circle the best answer.
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 90%, so it ends soon
- About 4.6%
- About 100%, so it is nearly done
- About 46%
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?
Clock face for a 24-hour day beside the timeline ruler: now at 4.6 of 10 billion years. Clock face for a 24-hour day beside the timeline ruler: now at 4.6 of 10 billion years. 24-hour day 0 6 12 18 now 0 10 billion years 4.6 billion years - About 11 hours
- About 23 hours, near the end
- About 4.6 hours
- About 1 hour
On Jun's timeline, 1 m stands for 1 billion years. How far from the Sun's formation is now?
Timeline ruler: 1 m = 1 billion years; now at 4.6 billion years. Timeline ruler: 1 m = 1 billion years; now at 4.6 billion years. 1 m = 1 billion years 0 1 2 3 4 4.6 4.6: now - 46 m
- 4.6 mm
- 0.46 m
- 4.6 m
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
- Its core will run out of hydrogen to fuse
- It will run out of the oxygen it needs to burn
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
- Exactly the same
- Hotter and dimmer
- Hotter and whiter, since the star becomes so much bigger
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 the hottest of any stage
- Its surface is hotter than the Sun's is now
- Its huge surface area gives off a lot of light
- It reflects light from nearby planets
A young white dwarf has a hotter surface than the Sun today but is far dimmer. Why, by Ren's reading?
Size bars, not to scale: the Sun and an Earth-sized white dwarf. Size bars, not to scale: the Sun and an Earth-sized white dwarf. Size bars, not to scale 0 2 4 6 8 10 10 Sun 1 Earth-sized white dwarf - It fuses hydrogen at its surface
- It is still fusing, but slowly
- It is tiny, about Earth's size, with little surface
- Its surface is colder than ice
What becomes of the Sun's outer layers at the end of its red giant stage, by Tala's reading (NASA)?
Drawing of a red giant with its outer layers drifting away. Drawing of a red giant with its outer layers drifting away. red giant outer layers - They explode in a supernova
- They collapse into a black hole around the core
- They stay and keep fusing hydrogen
- They drift away as a planetary nebula
Star card cutaway of a white dwarf. What fuses inside a white dwarf, by Zee's reading (NASA)?
- Carbon into iron
- Helium into carbon, as in a red giant
- Nothing; it glows from stored heat as it cools
- Hydrogen into helium
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
- Neutrons packed tightly together
- Mostly hydrogen, as the Sun is now
- Iron, from fusion up the periodic table