“Fusion Confusion: A Star’s Guide to Burning Bright”

“Fusion Confusion: A Star’s Guide to Burning Bright”

12th Grade

25 Qs

quiz-placeholder

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“Fusion Confusion: A Star’s Guide to Burning Bright”

“Fusion Confusion: A Star’s Guide to Burning Bright”

Assessment

Quiz

Physics

12th Grade

Easy

Created by

HOD Sciences

Used 2+ times

FREE Resource

25 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Why are stars called the “element factories” of the universe?

They cook elements in their hot cores by fusion

They recycle planets into gas

They shine brighter than galaxies

They make atoms disappear

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

The collapse of a gas cloud into a protostar (baby star born) is mainly caused by:

Pressure from planets nearby

Gravity overpowering pressure

Supernova shockwaves only

Magnetic fields twisting the gas

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What keeps a main-sequence star (like our sun) stable?

Gravity pulling in balanced by radiation pressure pushing out

Strong nuclear force pulling everything together

Magnetic attraction from galaxies

Rotation of the star

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

The Sun shines because:

Hydrogen fuses into helium in its core

Helium splits into hydrogen

Carbon is burned like coal

 It reflects light from the Milky Way

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which condition is most critical for starting nuclear fusion?

Large amounts of oxygen

Freezing cold vacuum

Planetary magnetic fields

 Very high core temperature and pressure

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Why can’t stars fuse elements heavier than iron in their cores?

 Iron nuclei are too heavy to move

Fusion beyond iron absorbs energy instead of releasing it

 Iron is unstable in stars

Stars cool down iron immediately

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which process forms gold and uranium in the universe?

Hydrogen burning in stars

Helium fusion in red giants (old age stars)

Supernova explosions and neutron star mergers

White dwarf cooling

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