Life and Death of Stars

Life and Death of Stars

Assessment

Interactive Video

Physics

9th - 10th Grade

Hard

Created by

Liam Anderson

FREE Resource

The video explores the potential for human survival in the universe, focusing on the life cycle of stars and the formation of white dwarfs. It discusses the possibility of white dwarfs serving as future habitats due to their longevity and stable energy output. The video also delves into the eventual end of the universe, highlighting the transition from white dwarfs to black dwarfs and the concept of heat death. Despite the distant and dark future, the video concludes on a hopeful note, emphasizing the current opportunity to explore and appreciate the universe.

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10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the primary reason humans can survive in the universe?

Existence of planets

Presence of an energy source

Abundance of oxygen

Availability of water

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What percentage of stars end their existence as white dwarfs?

50%

100%

75%

97%

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What happens to the Sun when it exhausts its hydrogen core?

It becomes a black hole

It starts burning helium into heavier elements

It explodes in a supernova

It turns into a red giant

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How dense is a white dwarf compared to Earth?

As dense as a feather

As dense as a teaspoon of water

As dense as a mountain

As dense as a car

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is a significant challenge for life around a white dwarf?

Absence of water

Lack of atmosphere

Extreme surface gravity

High radiation levels

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Why do white dwarfs shine longer than other star types?

They are extremely hot and inefficient at losing heat

They have a stable energy output

They are closer to other stars

They are larger in size

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the estimated lifespan of a white dwarf's shine?

100 billion billion years

10 million years

Forever

1 trillion years

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