
High-Mass Star Fusion Processes

Interactive Video
•
Physics
•
9th - 12th Grade
•
Hard

Patricia Brown
FREE Resource
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10 questions
Show all answers
1.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the primary difference in hydrogen fusion between high-mass and low-mass stars?
High-mass stars use the proton-proton chain.
Low-mass stars use the CNO cycle.
Low-mass stars do not fuse hydrogen.
High-mass stars use the CNO cycle.
2.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the CNO cycle in high-mass stars?
A process that fuses hydrogen into helium using carbon, nitrogen, and oxygen as catalysts.
A process that fuses carbon into oxygen.
A process that fuses helium into carbon.
A process that fuses silicon into iron.
3.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What happens to a high-mass star when its core hydrogen is depleted?
It becomes a white dwarf.
It turns into a red supergiant.
It explodes immediately.
It stops shining.
4.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What happens to the core of a high-mass star after it runs out of helium?
It shrinks and heats up.
It expands and cools.
It stops nuclear reactions.
It becomes a black hole.
5.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
Which process allows high-mass stars to fuse heavier elements?
Helium capture reactions
Proton-proton chain
Electron capture reactions
Neutron capture reactions
6.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the role of helium capture reactions in high-mass stars?
They create a new hydrogen shell.
They cool down the star's core.
They prevent the star from collapsing.
They convert helium into heavier elements.
7.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
Why can't elements heavier than iron generate energy through fusion?
They are too rare.
They have a lower mass per nuclear particle.
They are too unstable.
They have a higher mass per nuclear particle.
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