Earth & Space Science

Earth & Space Science

  • About This Project
    • Preface/About
    • Author/Contributors
    • For Investors/Donors
    • Teaching Guide
  • Ch 1 – Our Place in the Universe
    • Chapter Introduction
    • 1.1 Our Cosmic Address
    • 1.1.1 Overview
    • 1.1.2 What do we mean when we say “Earth is a planet”?
    • 1.1.3 What is our solar system?
    • 1.1.4 What is a galaxy?
    • 1.1.5 What is the universe?
    • 1.1 Review: Our Cosmic Address
    • 1.2 The Scale of Space
    • 1.2.1 Overview
    • 1.2.2 How Big is the Earth–Moon System?
    • 1.2.3 How Big is our Solar System?
    • 1.2.4 How far are the stars?
    • 1.2.5 How big is the Milky Way Galaxy?
    • 1.2.6 How big is the universe?
    • 1.2 Review: The Scale of the Universe
    • 1.3 Spaceship Earth
    • 1.3.1 How is Earth moving in our solar system?
    • 1.3.2 How is our solar system moving in the Milky Way Galaxy?
    • 1.3.3 How does our galaxy move relative to other galaxies in the universe?
    • 1.3 Review
  • Ch 2 – Understanding the Sky
    • Chapter Introduction
    • 2.1 Our Everyday View of the Universe
    • 2.1.1 What do we see in the local sky?
    • 2.1.2 What is the celestial sphere?
    • 2.1.3 Why do stars rise and set?
    • 2.1.4 Why do we see different constellations at different times of year?
    • 2.1 Review
    • 2.2 Seasons
    • 2.2.1 What causes the seasons?
    • 2.2.2 How do seasons differ around the world?
    • 2.2.3 Does the orientation of Earth’s axis ever change?
    • 2.2 Review
    • 2.3 Viewing the Moon: Phases and Eclipses
    • 2.3.1 Why do we see phases of the Moon?
    • 2.3.2 When do we see different phases of the Moon in our sky?
    • 2.3.3 Why do we always see the same face of the Moon?
    • 2.3.4 What are eclipses?
    • 2.3 Review
    • 2.4 Planets in the Night Sky
    • 2.4.1 How do we recognize planets in the sky?
    • 2.4.2 Why do the planets “wander”?
    • 2.4 Review
  • Ch 3 – How Science Discovered the Earth
    • Chapter Introduction
    • 3.1 The Ancient View of Earth
    • 3.1.1 How did the ancient Greeks learn that Earth is round?
    • 3.1.2 Why didn’t the ancient Greeks realize that Earth orbits the Sun?
    • 3.1 Review
    • 3.2 The Copernican Revolution
    • 3.2.1 How did the idea of Earth as a planet gain favor?
    • 3.2.2 How did Galileo seal the case for Earth as a planet?
    • 3.2 Review
    • 3.3 The Nature of Modern Science
    • 3.3.1 How does science work?
    • 3.3.2 What is a “theory” in science?
    • 3.3.3 What is the value of science?
    • 3.3 Review
    • 3.4 The Fact and Theory of Gravity
    • 3.4.1 What is gravity?
    • 3.4.2 How does gravity hold us to the ground and make objects fall?
    • 3.4.3 Why does gravity make planets round?
    • 3.4.4 How does gravity govern motion in the universe?
    • 3.4 Review
  • Chapter 4 – Planet Earth
    • Chapter Introduction
    • 4.1 A Planetary Overview
    • 4.1.1 What does Earth look like on the outside?
    • 4.1.2 What does Earth look like on the inside?
    • 4.1.3 How has Earth changed through time?
    • 4.1.4 How do we study the Earth?
    • 4.1 Review
    • 4.2 Earth System Science
    • 4.2.1 What are Earth’s four major systems?
    • 4.2.2 What drives Earth system changes?
    • 4.2.3 What IS energy and how do we measure it?
    • 4.2 Review
    • 4.3 Earth In the Context of Other Worlds
    • 4.3.1 How does Earth compare to other worlds of our solar system?
    • 4.3.2 Could there be life on other worlds?
  • Chapter 5 – Earth Through Time
    • Chapter Introduction
    • 5.1 Learning from Rocks and Fossils
    • 5.1.1 How do rocks form?
    • 5.1.2 What are fossils?
    • 5.1.3 How do we learn the ages of rocks and fossils?
    • 5.1 Review
    • 5.2 Shaping Earth’s Surface
    • 5.2.1 How do continents differ from oceans?
    • 5.2.2 What processes shape continents?
    • 5.2.3 What dangers do geological changes pose?
    • 5.2 Review
    • 5.3 Plate Tectonics — The Unifying Theory of Earth’s Geology
    • 5.3.1 What evidence led to the idea that continents move?
    • 5.3.2 How does the theory of plate tectonics explain Earth’s major features?
    • 5.3 Review
    • 5.4 A Brief Geological History of Earth
    • 5.4.1 What major changes mark Earth’s fossil record?
    • 5.4.2 What killed the dinosaurs?
    • 5.4.3 Have we humans started a new geological epoch?
    • 5.4 Review
  • Chapter 6 – Air and Water
    • Chapter Introduction
    • 6.1 Atmosphere and Hydrosphere
    • 6.1.1 What exactly is the atmosphere?
    • 6.1.2 How is water distributed on Earth?
    • 6.1.3 How does water cycle through the hydrosphere and atmosphere?
    • 6.1 Review
    • 6.2 Global Winds and Currents
    • 6.2.1 What drives global winds and currents?
    • 6.2.2 What is the general pattern of winds on Earth?
    • 6.2.3 What is the general pattern of ocean currents?
    • 6.2 Review
    • 6.3 Weather and Climate
    • 6.3.1 What is the difference between weather and climate?
    • 6.3.2 How and why does climate vary around the world?
    • 6.3.3 How do we measure and predict the weather?
  • Chapter 7 – Human Impact on the Climate
    • Chapter Introduction
    • 7.1 The Basic Science of Global Warming
    • 7.1.1 What is the greenhouse effect?
    • 7.1.2 How is human activity strengthening Earth’s greenhouse effect?
    • 7.1.3 How do we know that global warming is really happening and is human-caused?
    • 7.1.4 How does human-caused climate change compare to natural climate change?
    • 7.1 Review
    • 7.2 Consequences of Global Warming
    • 7.2.1 What are the major consequences of global warming?
    • 7.2.2 How do scientists predict future consequences of global warming?
    • 7.2.3 How will climate changes affect you and others around the world?
    • 7.2 Review
    • 7.3 Solutions to Global Warming
    • 7.3.1 What existing technologies could solve the problem of global warming?
    • 7.3.2 What future technologies might help even more?
    • 7.3.3 What does it take to implement a solution?
    • 7.3.4 What will your world look like AFTER we solve global warming?
    • 7.3 Review

A Brief Review

The Many Forms of Light

Show Teacher Notes

This box is a “Review” because most students will already have learned about the spectrum and the different forms of light in a Physical Science unit (NGSS standard MS-PS4B). However, it will almost certainly be worth spending a little time to review the ideas, and you may have some students for whom this material is new.



You’ve probably learned before that there are many forms of light besides the “visible light” that our eyes can see. To understand the many forms of light, it’s helpful to start by reviewing exactly what light is.

Light is a form of energy that travels through space at the speed of light (about 300,000 kilometers per second) and is characterized by rapidly changing electric and magnetic fields. For this reason, we often say that light is an electromagnetic wave. Like any wave, electromagnetic waves are characterized by a wavelength .

We refer to the full range of wavelengths as the electromagnetic spectrum , and Figure 1 shows the names we give to different sets of wavelength. Let’s start at the rainbow in the middle of Figure 1:

  • The light that our eyes can see is called visible light . The rainbow shows how the color that we see depends on wavelength: On the short-wavelength side of the rainbow, visible light is blue or violet. On the long-wavelength side, it is red. Note that visible light represents only a very small part of the full spectrum of light. (Visible light is the narrow rainbow with wavelengths ranging from about 400 to 700 nanometers.)
  • Light with wavelengths slightly longer than those of visible light is called infrared light . It gets this name because infra means “further on” or “beyond” and this light is beyond the red end of the visible light spectrum.
  • The longest wavelength forms of light (beyond the infrared) are called radio waves , or just “radio” for short. In other words, radio is a form of light, not sound. However, sound signals can be electronically encoded in radio waves, which is why we often talk about “listening to the radio” even though the radio waves themselves are a form of light.

    Note that microwaves (like those used in your microwave oven) are an alternative name for the wavelengths in parts of the infrared and radio regions of the spectrum.

  • Going in the other direction from visible light (to the left in Figure 1), ultraviolet light lies beyond the violet end of the visible light spectrum, meaning it represents slightly shorter wavelengths than visible light.
  • Light with even shorter wavelengths represents what we call x-rays . In other words, the “rays” in x-rays refer to light waves (electromagnetic waves).
  • The shortest wavelength forms of light are called gamma rays .
Figure 1 – This illustration represents the full spectrum of light, called the electromagnetic spectrum. Short wavelengths are on the left and long wavelengths are on the right. Notice the names given to different wavelength bands.

The basic names above (radio waves, infrared light, visible light, ultraviolet light, x-rays, gamma rays) are pretty easy to remember, but there are a few more ideas that you should also keep in mind and that will help you when you hear people talking about light:

  • The term radiation is often uses as a synonym for light. For example, you may hear infrared light being called “infrared radiation” or ultraviolet light referred to as “ultraviolet (uv) radiation.” More generally, light is sometimes called “electromagnetic radiation.”
  • In addition to a wavelength, waves also have a frequency that describes how many waves pass some point each second. Frequencies are always higher for short wavelengths and lower for long wavelengths, which means that gamma rays and x-rays have very high frequencies and radio waves have very low frequencies.
  • When studied carefully, the behavior of light can seem rather strange: Sometimes it behaves like waves, which are spread out over some distance (like ocean waves or waves on a string), and sometimes it behaves like individual particles. For this reason, we often talk about individual “pieces” of light, which we call photons . For example, we might talk about “x-ray photons,” meaning individual x-rays, each characterized by its wavelength (and frequency).

The following video reviews these ideas in a little more detail.

https://grade8science.com/wp-content/uploads/2021/01/EMSPectrum.mp4

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