Exam 9: Planetary Geology: Earth and the Other Terrestrial Worlds

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The core,mantle,and crust of a planet are defined by differences in their

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Explain how we can estimate the geological age of a planetary surface from its number of impact craters.

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Even though impacts still occur today,the vast majority of craters formed during the bombardment period that ended around 3.8 billion years ago.A surface region that is still saturated with craters must have remained essentially undisturbed for the last 3.8 billion years.In contrast,a surface region that has few craters indicates that the original craters must have been somehow "erased" since then.

In general,which things below are affected by a magnetic field?

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Spacecraft have landed on all the terrestrial worlds except

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Why is continental crust lower in density than seafloor crust?

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In the inner solar system,the largest surface features are found on the largest planets.

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Shallow-sloped shield volcanoes are made from lava that

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From center to surface,which of the following correctly lists the interior layers of a terrestrial world?

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Which of the following worlds have the thinnest lithospheres?

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Based on all we know about the terrestrial worlds,what single factor appears to play the most important role in a terrestrial planet's geological destiny?

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The cores of the terrestrial worlds are made mostly of metal because

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Describe the three sources of internal heat of the terrestrial planets?

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Much of the land on the west coast of North America began as volcanic islands in the Pacific.

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Which internal energy source is the most important in continuing to heat the terrestrial planets today?

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Olympus Mons is

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Briefly explain why Mercury,Venus,and the Moon do not have significant erosion.Relate erosional activity to the four planetary formation properties.

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Spacecraft have landed on all of the terrestrial worlds.

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What observational evidence supports the idea that Mercury once shrank by some 20 kilometers in radius?

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Erosion is the most important geological process on Venus.

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Which of the following best describes the geological histories of the Moon and Mercury?

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