Exam 10: Other Planetary Systems: the New Science of Distant Worlds

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Only Earth- size terrestrial planets and Jupiter- size gas giants have been discovered in other planetary systems.

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You have observed the wobble in the velocity curves of two otherwise identical stars. Star A has a period of 6 months and Star B has a period of 1 year. What can you say about these stars?

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Astronomers have discovered more extrasolar planets around other stars than the number of planets in our own Solar System.

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What is astrometry?

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A planet's density can be determined if it is observed to periodically transit in front of its parent star causing eclipses.

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Which of the following methods has led to the most discoveries of extrasolar planet candidates?

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Which of the following methods uses the principle of orbital acceleration to detect planets around another star?

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How can astronomers measure the composition of an extrasolar planet's atmosphere?

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The transit method of planet detection works best for

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What mechanism explains the presence of "hot Jupiters" around many other stars?

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Which of the following methods has led to the most confirmed discoveries of massive planets orbiting near their parent stars?

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The Doppler technique for planet detection has found Earth- like planets around nearby Sun- like stars

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The Doppler technique can be used to estimate the semimajor axis of a planet's orbit by

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Which of the following statements is not true about the planets so far discovered around other stars?

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The planet HAT- P- 32b has more than twice the radius of Jupiter, yet is only the same mass. It orbits its star more than a factor of ten closer than Mercury's orbit around the Sun. Which is the most plausible explanation for its large size?

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You discover that a nearby star, very similar to the Sun, has a velocity curve that has a period of 6 months, induced by the orbit of a planet. You infer that

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What is the chief difficulty in attempting to detect planets around other stars?

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Kepler's Impact: In four years of operation, the Kepler satellite discovered nearly three times as many extrasolar planet candidates as had been discovered in the previous 15 years (since the first discovery of an extrasolar planet). Discuss how these observations changed our understanding of the population of planets and of planet formation.

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What must be true in order for astronomers to be able to use the Doppler technique to determine a planet's mass?

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What are the two main differences between extrasolar planetary systems discovered to date and our Solar System?

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