Exam 7: The Birth and Evolution of Planetary Systems

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The Kepler mission is designed to search for extrasolar planets using the _________ method.

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Explain why most of the extrasolar planets that astronomers first detected were so-called "hot Jupiters."

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What sets the temperature of the pocket of gas in a protoplanetary disk?

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Inside a solar nebula,as smaller particles collide and stick together,forming larger particles,their self-gravity prevents them from breaking apart,regardless of the strength of the collision.

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What is the ratio of the orbital angular momentum of the Earth compared to its spin angular momentum? Note that the Earth has a radius of 6 × 106 m,and 1 AU is 1.5 × 1011 m.

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The borderline between the most massive planet and the least massive brown dwarf occurs at:

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Was it ever possible (or is it currently possible)for Jupiter to become a star?

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The primordial atmosphere of the Earth consisted of what type of chemical elements and from where did it originate? What chemical elements did the secondary atmosphere of the Earth consist of and from where did it originate?

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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 ±12 m/s over a period of 12 years,because of:

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Two competing models of the formation of giant gaseous planets suggest they form either from gas accreting onto a rocky core or from:

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What is the age of our Solar System?

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What does conservation of angular momentum mean?

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Explain why there is a significant amount of methane and ammonia in the atmospheres of Uranus and Neptune but not nearly as much in the atmospheres of Jupiter and Saturn.

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Which is NOT a scientific goal of NASA's Kepler mission?

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Which property of an extrasolar planet CANNOT be determined using the Doppler effect?

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What is the most important factor in determining whether or not a planet will be rocky like terrestrial planets or gaseous like giant planets?

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Which of the following is FALSE?

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Explain how astronomers use the Doppler effect to detect the presence of extrasolar planets.

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What happens to the kinetic energy of gas as it falls toward and eventually hits the accretion disk surrounding a protostar?

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Why have astronomers using the radial velocity method found more Jupiter-sized planets at a distance of 1 AU around other stars than Earth-sized planets?

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