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

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The Kuiper Belt is located beyond the orbit of ________.

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Masses of the planets are easiest to determine if:

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Our solar system contains only 65 moons (as of Summer 2007).

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As a result of the ejection of planetesimals into the Oort Cloud,simulations indicate that Uranus and Neptune moved:

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A meteorite is:

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All jovian planets have rings around their equators and at least eight moons.

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

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Conservation of angular momentum explains why the contracting solar nebula's rotation rate increased as it contracted.

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As the solar nebula contracts due to gravitation,the cloud:

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An alternative to the core-accretion theory that explains the formation of the jovian planets is the:

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

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What is the goal of comparative planetology?

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Any model of solar system formation must explain why every planet is relatively isolated in space.

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All jovians have at least eight moons and equatorial rings.

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What physical characteristics of Mercury distinguish it among all the planets in our solar system?

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The Pioneer and Voyager space probes passed near the jovian planets without landing or crashing into them.

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While all planet orbits are ellipses,the eight large planets have fairly ________ eccentricities.

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The least dense form of interplanetary debris are ________.

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In terms of ________,all the terrestrials are greater than any of the jovians.

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Which of the characteristics below describes the terrestrial planets?

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