

Neutron Stars: The Extreme End of Stellar Evolution
Interactive Video
•
Physics, Chemistry, Science
•
9th - 12th Grade
•
Practice Problem
•
Hard
Patricia Brown
FREE Resource
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10 questions
Show all answers
1.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What causes the initial balance in a star that allows it to remain stable?
The balance between nuclear fusion and magnetic fields
The balance between radiation and magnetic fields
The balance between magnetic fields and gravitational forces
The balance between nuclear fusion and gravitational forces
2.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What happens to a star when it exhausts its hydrogen supply?
It becomes a black hole immediately
It turns into a neutron star immediately
It goes through a giant phase and eventually becomes a white dwarf
It explodes into a supernova immediately
3.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the result of a supernova explosion?
The star becomes a red giant
The star becomes a white dwarf
The star becomes a black hole
The star becomes a neutron star
4.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
How dense is neutron star matter compared to everyday objects?
As dense as a mountain
As dense as a sugar cube
As dense as a cup of coffee
As dense as a billion tons in a sugar cube
5.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is nucleopasta?
A type of star
A dense material found in the crust of neutron stars
A type of black hole
A type of pasta found in space
6.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What happens to protons and neutrons in the core of a neutron star?
They turn into electrons
They remain unchanged
They form a new type of element
They dissolve into an ocean of quarks
7.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What causes neutron stars to spin rapidly?
Their magnetic fields
Their collapse and conservation of angular momentum
Their interaction with other stars
Their large size
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