Exam 6: The Solar System: Comparative Planetology and Formation Models

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Describe how the observable properties of the solar system are related to its process offormation.

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For what reasons do we consider the planets of the solar system to be of two fundamentallydifferent types?

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Which of the following are the jovian planets?

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Accretion occurred sooner in the inner part of the solar system than it did in the outerregions.

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Discuss the role that gravity assist played in Voyager 2 and its Grand Tour.

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Name three properties of the solar nebula still seen in planet orbits.

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One possible way that future scientists may determine whether the core-accretion model orthe gravitational instability theory better explains the formation of the jovian planet is:

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The principal difference between the terrestrial and jovian planets is the absence of ________and helium close to the Sun.

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All the planets orbit the Sun in the ________ plane.

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A successful theory of the formation of the solar system must explain:

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According to the planetary migration model, the jovian planets are thought to have formed:

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How do the atmospheres of terrestrial worlds compare with the jovians?

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In composition and density, the asteroids most resemble:

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Briefly outline the theory or hypothesis which best explains the origin of the solar system.

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In composition, mass, and density, Jupiter is most like:

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Asteroids are the densest form of interplanetary debris.

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What support for the solar nebula theory has come from observations of nearby young stars?

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What form of interplanetary debris did humans discover first? Why?

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At what point does the accretion process turn a clump of debris into a planetesimal?

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Our solar system contains more than 100 Kuiper Belt objects larger than 300 km in diameter.

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