Mars's Atmosphere

Mars has a very thin atmosphere, which allows astronomers to see its surface with a telescope. The thin Martian atmosphere and its distance from the sun make the surface very cold. Temperatures vary from − 140°C to 20°C. Mars's atmosphere is more than 95 percent carbon dioxide, similar to the atmosphere of Venus, but much thinner.

Water on Mars

Mars shows evidence of once having a great deal of liquid surface water. Some geologists think Mars's northern lowlands were once covered by an ocean. Features shown in Figure 16C may have been stream channels and gullies. In fact, changes in surface features over the past several years indicate that water may still flow on the surface, if only for brief periods of time.

Why is liquid water rare on Mars's surface? Some water vapor has escaped into space. Some water is stored, along with frozen carbon dioxide, in ice caps at the north and south poles. Some water is frozen underground, just below the Martian surface.

Because Mars had large amounts of liquid water on its surface in the past, many scientists wonder if life once existed there. Robotic probes have carried out experiments on the Martian surface to look for signs of life. None of these probes found clear evidence for the existence of life on Mars.

Martian Seasons

Like Earth, Mars has distinct seasons. Mars's seasons are caused by the tilt of its axis. Over the course of a Martian year, Mars's ice caps grow and shrink. The change in seasons also causes large dust storms that occasionally rage across the surface.

Figure 16 Mars has a thin atmosphere that permits a clear view of its surface from space. A Mars has ice caps at both poles. BOlympus Mons is the largest volcano in the solar system. CThese Martian valleys are thought to have been formed at least in part by large flows of liquid water in the distant past.

Image of Mars displaying (A) its ice caps to north (B) Olympus Mons as largest volcano in Solar System (C) valleys formed by water in past.

Figure 17 This photo of a dark boulder on Martian sand was taken by the Mars Exploration Rover Spirit in 2006. Spirit found rocks and minerals that formed in, or were altered by, water.

Sandy surface of Mars with scattered rocks and dark boulders.

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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