Greenhouse Gases and Energy Concepts

Greenhouse Gases and Energy Concepts

Assessment

Interactive Video

Physics

9th - 12th Grade

Hard

Created by

Patricia Brown

FREE Resource

This video tutorial covers the greenhouse effect, focusing on key physics concepts such as conservation of energy, emissivity, and albedo. It explains how these concepts relate to real-world phenomena like energy loss, temperature changes, and the solar constant. The video also discusses the greenhouse effect and its impact on Earth's climate, highlighting the role of major greenhouse gases.

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10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What does the law of conservation of energy state?

Energy can only be transferred from one form to another.

Energy can be created and destroyed.

Energy is only present in living organisms.

Energy is always increasing in the universe.

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which of the following best describes emissivity?

A measure of the color of an object.

A measure of the temperature of an object.

A measure of how well an object emits electromagnetic waves.

A measure of how well an object reflects light.

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the albedo of a very light-colored object?

Exactly zero

Close to zero

Exactly one

Close to one

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How are albedo and emissivity related for opaque objects?

They are directly proportional.

They are inversely proportional.

They are equal.

They are unrelated.

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What happens to the power emitted by an object when its temperature decreases from 800K to 500K?

It increases.

It remains the same.

It decreases.

It doubles.

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the solar constant?

The energy reflected by the Earth's surface.

The total energy emitted by the Sun.

The average intensity of solar energy at the top of Earth's atmosphere.

The energy received by the Earth at its surface.

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How is the average intensity of solar energy reaching Earth calculated?

By adding the solar constant to Earth's albedo.

By subtracting Earth's emissivity from the solar constant.

By multiplying the solar constant by Earth's surface area.

By dividing the two-dimensional area of Earth by the three-dimensional surface area of Earth.

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