
Star Evolution and Fusion Processes
Interactive Video
•
Physics, Chemistry, Science
•
9th - 12th Grade
•
Hard

Amelia Wright
FREE Resource
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10 questions
Show all answers
1.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What prevents a star from collapsing during the main sequence phase?
The presence of dark matter
The rotation of the star
The gravitational pull of nearby stars
The energy released from hydrogen fusion
2.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the main sequence phase of a star characterized by?
The fusion of carbon into iron
The fusion of hydrogen into helium
The fusion of helium into carbon
The fusion of oxygen into silicon
3.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What happens to the core of a star as more helium accumulates?
It expands and becomes less dense
It remains the same size
It shrinks and becomes denser
It explodes
4.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
Why does a star become a red giant?
Because it loses mass
Due to intense hydrogen fusion over a larger radius
Because it stops fusing elements
Due to a decrease in gravitational pull
5.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the primary reason for the cooler surface temperature of a red giant?
The star's core is made of iron
The star is moving away from the observer
The star's core stops producing energy
The energy is dissipated over a larger surface area
6.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the primary factor that causes a star to expand into a red giant?
The decrease in core temperature
The increase in core density
The increase in hydrogen fusion rate
The decrease in gravitational force
7.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
At what temperature does helium start to fuse into heavier elements in a star's core?
200 million Kelvin
50 million Kelvin
10 million Kelvin
100 million Kelvin
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