Exam 7: The Birth and Evolution of Planetary Systems

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The solid form of a volatile material is generally referred to as a(n):

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Comets and asteroids are:

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According to the conservation of angular momentum, if an ice skater starts spinning with her arms out wide, then slowly pulls them close to her body, this will cause her to:

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How do astronomers explain the basic difference in composition between the inner planets and the outer planets?

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What evidence do we have that the accretion disk that formed the Solar System was initially very centrally condensed?

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How much material in an accretion disk goes into forming the planets, moons, and smaller objects?

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The difference in composition between the giant planets and the terrestrial planets is most likely caused by the fact that:

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Explain the nebular hypothesis, and describe two observations that support it.

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Why do the outer giant planets have massive gaseous atmospheres of hydrogen and helium while the inner planets do not?

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The atmosphere of which of these Solar System bodies is primary, as opposed to secondary, in origin?

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An observer located outside our Solar System, who monitors the velocity of our Sun over time, will find that its velocity varies by ±\pm 12 m/s over a period of 12 years, because of:

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What is the age of our Solar System?

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Whether or not a planet is composed mostly of rock or gas is set by:

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What prevented the Moon from maintaining any atmosphere with which it originally formed?

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Our Solar System is the only planetary system in our galaxy.

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The figure below shows data from Doppler effect studies of three different stars: A, B, and C. Assume that all the stars are similar in mass to the Sun. Which star has the planet with the smallest semimajor axis? The figure below shows data from Doppler effect studies of three different stars: A, B, and C. Assume that all the stars are similar in mass to the Sun. Which star has the planet with the smallest semimajor axis?

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What is the ratio of the orbital angular momentum of Jupiter to its spin angular momentum? Jupiter's orbit has a semimajor axis of 5 AU and period of 12 years, and Jupiter has a rotation period of 0.4 day and a radius of 70,000 km.

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In protoplanetary environments, the plane of an accretion disk is perpendicular to the axis of rotation of the interstellar cloud out of which it forms.

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  Figure 1 -Using the Doppler effect data shown in Figure 1, determine the approximate orbital period of the extrasolar planet. Figure 1 -Using the Doppler effect data shown in Figure 1, determine the approximate orbital period of the extrasolar planet.

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Conservation of angular momentum slows a cloud's collapse:

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