The Thermosphere

The outermost layer of the atmosphere, the thermosphere (THUR moh sfeer), begins at an altitude of about 80 kilometers and extends outward into space. No boundary marks the end of the atmosphere. Instead, the thin air of the thermosphere gradually merges with space. In the thermosphere, temperature increases rapidly with altitude, from about −90°C to more than 1000°C. Recall from physics that temperature is a measure of the average kinetic energy of molecules. Because gas molecules in the thermosphere absorb solar radiation and move very fast, the temperature is quite high.

The Ionosphere

The ionosphere (eye AHN uh sfeer) is not a distinct layer of the atmosphere. Rather, it is a region of charged particles, or ions, that overlaps the lower thermosphere. In the ionosphere, molecules of nitrogen and oxygen lose one or more electrons as they absorb high-energy wavelengths of solar radiation. The molecules become positively charged ions. These ions are most dense between the altitudes of 80 and 400 kilometers. At these high altitudes, certain radio waves sent from Earth's surface, such as AM radio waves, bounce off ions and travel back to Earth. You can often hear AM radio stations from very far away at night because the sun's radiation is blocked by Earth. The ions start to recombine at night, allowing AM radio waves to travel farther.

One of nature's most spectacular displays occurs in the ionosphere. An aurora, shown in Figure 6, is a colorful display of light in the sky, produced when charged particles from the sun are attracted to Earth's magnetic poles. There, these particles cause ions in the ionosphere to glow. In the Northern Hemisphere, these displays are called the aurora borealis, or Northern Lights.

Figure 6 Auroras provide spectacular displays of light in the polar regions. Auroras are produced by glowing ions in the ionosphere.

An aurora shining in a night sky over a tree line.

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Table of Contents

Physical Science CHAPTER 1 Science Skills CHAPTER 2 Properties of Matter CHAPTER 3 States of Matter CHAPTER 4 Atomic Structure CHAPTER 5 The Periodic Table CHAPTER 6 Chemical Bonds CHAPTER 7 Chemical Reactions CHAPTER 8 Solutions, Acids, and Bases CHAPTER 9 Carbon Chemistry CHAPTER 10 Nuclear Chemistry CHAPTER 11 Motion CHAPTER 12 Forces and Motion CHAPTER 13 Forces in Fluids CHAPTER 14 Work, Power, and Machines CHAPTER 15 Energy CHAPTER 16 Thermal Energy and Heat CHAPTER 17 Mechanical Waves and Sound CHAPTER 18 The Electromagnetic Spectrum and Light CHAPTER 19 Optics CHAPTER 20 Electricity CHAPTER 21 Magnetism CHAPTER 22 Earth's Interior CHAPTER 23 Earth's Surface CHAPTER 24 Weather and Climate CHAPTER 25 The Solar System CHAPTER 26 Exploring the Universe Skills and Reference Handbook