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 4.6%
- About 100%, so it is nearly done
- About 90%, so it ends soon
- 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 4.6 hours
- About 11 hours
- About 23 hours, near the end
- 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 - 0.46 m
- 4.6 mm
- 4.6 m
- 46 m
“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 core explodes as a supernova
- The whole Sun shrinks and goes completely dark
- The core heats up and the outer layers swell
- The outer layers cool and shrink
“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 will explode once it becomes a red giant
- It has too little mass; only far heavier stars explode
- It is too hot to explode
- It already exploded long ago
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?
- Exactly the same
- Cooler and redder, though the star is far brighter
- Hotter and whiter, since the star becomes so much bigger
- Hotter and dimmer
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 huge surface area gives off a lot of light
- Its surface is the hottest of any stage
- It reflects light from nearby planets
- Its surface is hotter than the Sun's is now
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
- It is still fusing, but slowly
- 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 drift away as a planetary nebula
- They collapse into a black hole around the core
- They stay and keep fusing hydrogen
- They explode in a supernova
Star card cutaway of a white dwarf. What fuses inside a white dwarf, by Zee's reading (NASA)?
- Hydrogen into helium
- Carbon into iron
- Helium into carbon, as in a red giant
- Nothing; it glows from stored heat as it cools