Giant Stars and Helium Fusion

Giant Stars and Helium Fusion

9th Grade

10 Qs

quiz-placeholder

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Giant Stars and Helium Fusion

Giant Stars and Helium Fusion

Assessment

Quiz

Chemistry

9th Grade

Medium

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

Standards-aligned

Created by

Phyllis Commisso

Used 4+ times

FREE Resource

10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the primary process generating energy in a main sequence star like our sun?

Helium fusion

Hydrogen fusion

Carbon fusion

Oxygen fusion

Tags

NGSS.HS-ESS1-1

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What happens to a star's core when it runs out of hydrogen fuel?

It expands and cools down

It contracts and heats up

It remains the same

It explodes

Tags

NGSS.HS-ESS1-1

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the term used to describe the process of three helium atoms forming carbon?

Alpha decay

Triple alpha process

Beta decay

Gamma process

Tags

NGSS.HS-ESS1-1

NGSS.HS-ESS1-3

NGSS.HS-PS1-8

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the approximate temperature required for helium fusion to begin in a star's core?

10 million Kelvin

50 million Kelvin

100 million Kelvin

200 million Kelvin

Tags

NGSS.HS-ESS1-1

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

As a star becomes a giant, what happens to its density and temperature?

Density increases, temperature increases

Density decreases, temperature decreases

Density increases, temperature decreases

Density decreases, temperature increases

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the main reason a star like our sun will eventually become a giant star?

It will gain mass from nearby stars

It will run out of hydrogen fuel in its core

It will collide with another star

It will lose its outer layers

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the "helium flash" in the context of giant stars?

The explosion of a star

The ignition of helium fusion in the core

The cooling of the star's surface

The expansion of the star's outer layers

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