Stellar Evolution and Nuclear Fusion Quiz

Stellar Evolution and Nuclear Fusion Quiz

9th Grade

23 Qs

quiz-placeholder

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Stellar Evolution and Nuclear Fusion Quiz

Stellar Evolution and Nuclear Fusion Quiz

Assessment

Quiz

Science

9th Grade

Hard

NGSS
HS-ESS1-3, HS-ESS1-1, HS-PS1-8

Standards-aligned

Created by

Mark Bate

Used 4+ times

FREE Resource

23 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the primary source of energy in a main-sequence star like our Sun?

Gravitational potential energy

Nuclear fusion of hydrogen into helium

Convection currents

Solar winds

Tags

NGSS.HS-ESS1-1

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

During which stage of a star's life does nuclear fusion of helium into heavier elements typically occur?

Protostar

Red giant

White dwarf

Main sequence

Tags

NGSS.HS-ESS1-3

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which of the following elements is primarily formed through nuclear fusion in the core of massive stars?

Iron

Carbon

Helium

Oxygen

Tags

NGSS.HS-ESS1-1

NGSS.HS-ESS1-3

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What happens to a star when it exhausts its nuclear fuel in the core?

It becomes a neutron star

It collapses into a black hole

It expands into a red giant

It sheds its outer layers and becomes a white dwarf

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which of the following stages of stellar evolution comes after the red giant phase for a Sun-like star?

Main sequence

Supernova explosion

Planetary nebula

Neutron star formation

Tags

NGSS.HS-ESS1-3

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

In the core of a star, what temperature and pressure conditions are necessary for nuclear fusion to occur?

Low temperature and high pressure

High temperature and high pressure

Low temperature and low pressure

High temperature and low pressure

Tags

NGSS.HS-ESS1-1

NGSS.HS-PS1-8

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What role does the Chandrasekhar limit play in the evolution of massive stars?

It marks the end of the main sequence phase.

It determines the size of a star's habitable zone.

It limits the mass of a white dwarf that can form.

It triggers the formation of a black hole.

Tags

NGSS.HS-ESS1-3

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