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

Circle the best answer.
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
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 m
- 4.6 mm
- 0.46 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
- 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
“Star card cutaway:” When the core runs out of hydrogen, gravity squeezes it. What happens next, by Luz's reading (NASA)?
Star card cutaway: the core shrinking, arrows pointing in. Star card cutaway: the core shrinking, arrows pointing in. core shrinking - 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
“sources give 7 to 10” Why will the Sun not end as a supernova, by Milo's reading (NASA)?
Two paths: stars up to about 8 times the Sun's mass (sources give 7 to 10) end as white dwarfs; heavier stars explode. Two paths: stars up to about 8 times the Sun's mass (sources give 7 to 10) end as white dwarfs; heavier stars explode. stars up to about 8 times the Sun's mass white dwarfs heavier stars explode - 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
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
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
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 tiny, about Earth's size, with little surface
- Its surface is colder than ice
- It is still fusing, but slowly
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 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
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