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s8pe-41302-ca 10/28/05 12:38 PM MAZER Page 425 Venus is too hot to have liquid water, and the winds do not seem to move much material. Erosion may be slower on Venus than on Earth. Weathering and Erosion Round craters mark the surface here and there. Older craters have been erased by the other processes. Also, Venus’s thick atmosphere protects the surface from small impacts. Impact Cratering check your reading Why is Venus not covered with craters? Erosion changes the appearance of Mars. Mars is relatively small, with a diameter about half that of Earth. The orange color of some of the surface comes from molecules of iron and oxygen—rust. Mars has two tiny moons. They were probably once asteroids that were pulled into orbit around Mars. Mars The atmosphere of Mars is thin but causes weathering and erosion. Surface of Mars The same processes that affect the other terrestrial planets affect Mars. Valleys and raised areas formed on Mars as the mantle moved. One huge system of valleys, called Valles Marineris, is long enough to stretch across the United States. Tectonics Most of the northern hemisphere has smooth plains of cooled lava. Several volcanoes are higher than any mountain on Earth. The lava must have built up in the same spot for a long time, so scientists have inferred that the crust of Mars has cooled more than Earth’s crust. On Earth, the tectonic plates move, so chains of smaller volcanoes form instead of single larger volcanoes. Mass 11% of Earth’s mass Diameter 53% of Earth’s diameter Average distance from Sun 1.5 AU Orbits in 1.9 Earth years Rotates in 25 hours Volcanism volcanoes Valles Marineris Fast winds carry sand that breaks down rocks. Wind and gravity move the broken material, forming new features such as sand dunes. There are also landforms that look like the results of gigantic flash floods that happened long ago. Weathering and Erosion Round craters cover much of the southern hemisphere of Mars. Many craters are very old and eroded. A few impact craters on the volcanoes make scientists think that the volcanoes have not released lava for a long time. Impact Cratering Chapter 13: Our Solar System 425 PDF