• Mercury has cratered highlands, much like the moon, and vast smooth terrains that resemble maria.
• Mercury has the greatest temperature extremes of any planet.
Surface Features
Surface Temperatures
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23.2 The Terrestrial Planets
• The surface temperature of Venus reaches 475oC, and its atmosphere is 97 percent carbon dioxide.
Surface Temperatures
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23.2 The Terrestrial Planets
Venus is similar to Earth in size, density, mass, and location in the solar system. Thus, it has been referred to as “Earth’s twin.”
• Venus is covered in thick clouds that visible light cannot penetrate.
Surface Features
• About 80 percent of Venus’s surface consists of plains covered by volcanic flow.
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23.2 The Terrestrial Planets
The Martian Atmosphere
• The Martian atmosphere has only 1 percent of the density of Earth’s.
Surface Features
• Most Martian surface features are old by Earth standards. The highly cratered southern hemisphere is probably 3.5 billion to 4.5 billion years old.
• Although the atmosphere of Mars is very thin, extensive dust storms occur and may cause the color changes observed from Earth.
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23.2 The Terrestrial Planets
Water on Mars
• Some areas of Mars exhibit drainage patterns similar to those created by streams on Earth.
• Images from the Mars Global Surveyor indicate that groundwater has recently migrated to the surface.
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23.3 The Outer Planets
Jupiter has a mass that is 2 1/2 times greater than the mass of all the other planets and moons combined.
• Jupiter’s hydrogen-helium atmosphere also contains small amounts of methane, ammonia, water, and sulfur compounds.
Structure of Jupiter
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