table of contents energy in earths atmosphere ms. de los rios science 6 th grade climate...

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Table of Contents Energy in Earth’s Atmosphere Ms. De Los Rios Science 6 th Grade Climate Interactions

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How Does Energy Travel from the Sun Travel to Earth ? Visible light Visible light includes all the colors of the rainbow. The different colors you see are the result of different wavelengths. ROY G BIV Nonvisible Radiation The direct transfer of energy by electromagnetic waves is called radiation. Infrared radiation, type of E.W., wavelengths longer than red light. It is invisible to humans but can be felt as heat. The sun also gives off ultraviolet radiation, which is an invisible form of energy with wavelengths shorter than violet light.

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Page 1: Table of Contents Energy in Earths Atmosphere Ms. De Los Rios Science 6 th Grade Climate Interactions

Table of Contents

Energy in Earth’s AtmosphereMs. De Los Rios

Science 6th Grade

Climate Interactions

Page 2: Table of Contents Energy in Earths Atmosphere Ms. De Los Rios Science 6 th Grade Climate Interactions

Vocabulary 7.21. Electromagnetic wave- a wave made up of a combination of a changing electric field and

a changing magnetic field.

2. Radiation the transfer of energy by electromagnetic waves (E.W)

3. Infrared Radiation - E.w with wavelengths that are longer than visible lights but shorter than microwaves.

4. Ultraviolet radiation-Electromagnetic waves with wavelength shorter than visible light but longer than X-rays.

5. Scattering-reflection of light in all directions.

6. Greenhouse Effect- The trapping of heat near a planet’s surface by certain gases in planet’s atmosphere.

7. Coriolis Effect- The effect of Earth’s rotation on the direction of winds and currents

Page 3: Table of Contents Energy in Earths Atmosphere Ms. De Los Rios Science 6 th Grade Climate Interactions

How Does Energy Travel from the Sun Travel to

Earth?Visible light Visible light includes all the colors of the rainbow. The different colors you see are the result of different wavelengths. ROY G BIV

Nonvisible Radiation The direct transfer of energy by electromagnetic waves is called radiation.

Infrared radiation, type of E.W., •wavelengths longer than red light. •It is invisible to humans but can be felt as heat. •The sun also gives off ultraviolet radiation, which is an invisible form of energy with wavelengths shorter than violet light.

Page 4: Table of Contents Energy in Earths Atmosphere Ms. De Los Rios Science 6 th Grade Climate Interactions

Radiation From the SunEnergy travels to Earth as electromagnetic waves. What are the types of electromagnetic radiation in

the diagram?

Energy in Earth’s Atmosphere

Page 5: Table of Contents Energy in Earths Atmosphere Ms. De Los Rios Science 6 th Grade Climate Interactions

Mnemonic Device to Memorize the Visible Light Spectrum

ROY G BIV•

R: red O: orange Y: yellow G: green

B: blue I: indigo V: violet

Page 6: Table of Contents Energy in Earths Atmosphere Ms. De Los Rios Science 6 th Grade Climate Interactions

How Does Energy Travel from the Sun Travel to Earth?

Nearly all the energy in Earth’s atmosphere comes from the sun.

This energy travels to Earth as electromagnetic waves

•Most of the energy from the sun travels to Earth in the form of visible light and infrared radiation.

•A smaller amount arrives as ultraviolet radiation.

Page 7: Table of Contents Energy in Earths Atmosphere Ms. De Los Rios Science 6 th Grade Climate Interactions

Electromagnetic Waves

A vacuum is a space that contains no air or gas. All electromagnetic waves travel at the same speed in a vacuum.

All electromagnetic waves have different wavelengths

Electromagnetic waves can be classified according to wavelength or distance between waves.

Page 8: Table of Contents Energy in Earths Atmosphere Ms. De Los Rios Science 6 th Grade Climate Interactions

What Happens to the Sun’s Energy When it Reaches Earth?

Sunlight is:• some of it is absorbed or reflected by the atmosphere before it can reach the surface. •The rest passes through the atmosphere to the surface.

•Upper Atmosphere Different wavelengths of radiation are absorbed by different layers in the atmosphere.

•Some ultraviolet radiation is absorbed by the ozone layer.

•Infrared radiation passes farther before some is absorbed by water vapor and carbon dioxide.

Page 9: Table of Contents Energy in Earths Atmosphere Ms. De Los Rios Science 6 th Grade Climate Interactions

Energy in the AtmosphereSome wavelengths reach Earth’s surface. Other wavelengths are

completely or partially absorbed in the atmosphere.

Energy in Earth’s Atmosphere

Page 10: Table of Contents Energy in Earths Atmosphere Ms. De Los Rios Science 6 th Grade Climate Interactions

What Happens to the Sun’s Energy When it Reaches Earth?

Troposphere

In the troposphere, clouds reflect some sunlight back into space. Dust-sized particles and gases in the atmosphere disperse light in all directions in a process called scattering.

Earth’s Surface

About 50 percent of the sun’s energy that reaches Earth’s surface is absorbed.

The result of this is: It heats land and water.

Page 11: Table of Contents Energy in Earths Atmosphere Ms. De Los Rios Science 6 th Grade Climate Interactions

Use the higher percentages below to show a bar graph. Give it a title.

Energy in Earth’s AtmosphereEnergy in Earth’s Atmosphere

Page 12: Table of Contents Energy in Earths Atmosphere Ms. De Los Rios Science 6 th Grade Climate Interactions

Energy at Earth’s Surface

Complete each sentence with a word from the Word Bank to learn what is happening to the energy at Earth's surface and in the lower atmosphere.

Energy in Earth’s Atmosphere

Page 13: Table of Contents Energy in Earths Atmosphere Ms. De Los Rios Science 6 th Grade Climate Interactions

What Happens to the Sun’s Energy When it Reaches Earth?

Earth’s Energy Budget

•Earth’s surface radiates some energy back into the atmosphere as infrared radiation.• Some travels all the way back into space, but much is absorbed by water vapor, carbon dioxide and other gases in the atmosphere, heating them.

The greenhouse effect is when these gases heat in the atmosphere.

•These gases hold in a process called The greenhouse effect keeps Earth’s atmosphere at a comfortable temperature.

•But scientists have evidence that human activities may be altering this process.

Page 14: Table of Contents Energy in Earths Atmosphere Ms. De Los Rios Science 6 th Grade Climate Interactions

Greenhouse EffectThe greenhouse effect is a natural heat-trapping process. What is the sequence of events that causes it to occur?

Energy in Earth’s Atmosphere

Page 15: Table of Contents Energy in Earths Atmosphere Ms. De Los Rios Science 6 th Grade Climate Interactions

How Does the Sun’s Energy affect Global Winds?

Energy provided by the sun influences global winds and creates temperature differences among Earth’s air, water, and land. Global winds are created by the unequal heating of Earth’s surface over a large area. Because of Earth’s spherical shape, rays from the sun strike directly at the equator but hit the poles at a lower angle. As a result, temperatures near the poles are much lower than near the equator. The differences between the equator and the two poles produce giant convection currents in the atmosphere. Surface winds blow from the poles toward the equator. Higher in the atmosphere, winds flow from equator to poles. The way Earth’s rotations make winds curve is called the Coriolis effect. Because of the Coriolis effect, global winds in the Northern Hemisphere gradually turn toward the right.

Page 16: Table of Contents Energy in Earths Atmosphere Ms. De Los Rios Science 6 th Grade Climate Interactions

Heating of Earth’s SurfaceThe angle of the sun's rays causes temperature differences at Earth's surface. Which areas on Earth receives the most direct light from the sun, and which

areas receive the least?

Energy in Earth’s Atmosphere

Page 17: Table of Contents Energy in Earths Atmosphere Ms. De Los Rios Science 6 th Grade Climate Interactions

The Coriolis EffectThe Coriolis effect determines the direction of global winds.

Energy in Earth’s Atmosphere

Page 18: Table of Contents Energy in Earths Atmosphere Ms. De Los Rios Science 6 th Grade Climate Interactions

How Does the Sun’s Energy affect Global Winds?

Land’s Heating

•Land heats and cools more rapidly than water. •Also, land can heat to higher temperatures than water can. •Land can also cool to lower temperatures than water can.

Heating and cooling of Earth’s land and water directly affect the air temperature above these surfaces.

This process helps create winds.

Page 19: Table of Contents Energy in Earths Atmosphere Ms. De Los Rios Science 6 th Grade Climate Interactions

Global Wind BeltsThe Coriolis effect and other factors combine to produce a pattern of wind belts and calm areas around Earth. Match the descriptions of the global winds with their location on the globe.

Energy in Earth’s Atmosphere