Cosmology and the Universe

Cosmology and the Universe

Assessment

Interactive Video

Physics, Science

10th Grade - University

Hard

Created by

Olivia Brooks

FREE Resource

The video explores the composition and evolution of the universe, highlighting that visible matter constitutes only 5% of the universe, with dark matter and dark energy making up the rest. It explains the Big Bang Theory and cosmological inflation, which describe the universe's expansion and the uniformity of cosmic microwave background radiation. The video also discusses the future of the universe, where dark energy will dominate, leading to an ever-expanding, largely empty universe.

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10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What percentage of the universe is made up of visible matter?

50%

75%

5%

25%

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How does dark matter differ from visible matter?

It does not have gravitational effects

It is visible

It clumps together

It interacts with light

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is a unique property of dark energy?

It clumps together

It dilutes as the universe expands

It does not clump or dilute

It is associated with particles

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What does the Big Bang Theory primarily explain?

The properties of dark matter

The end of the universe

The evolution of the universe from a hot, dense state

The initial creation of the universe

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What evidence supports the Big Bang Theory?

The presence of dark matter

The cosmic microwave background radiation

The uniformity of dark energy

The universe is contracting

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What problem does cosmological inflation solve?

The lack of dark matter

The abundance of visible matter

The uniformity of the cosmic microwave background

The presence of black holes

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the main idea behind cosmological inflation?

A slow expansion of the universe

A rapid exponential expansion early in the universe's history

The constant size of the universe

The contraction of the universe

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