13 review clickers

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Chapter 13 ReviewClickers © 2014 Pearson Education, Inc. The Cosmic Perspective Seventh Edition Other Planetary Systems: The New Science of Distant Worlds

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© 2014 PearsonEducation, Inc. Chapter 13 Is it easy to photograph of a planet orbiting around another star? a) Yes, but a large telescope because the planet would be faint. b) No, because the brightness of the star would overwhelm the planet. c) Yes, but a space telescope must be used so that the scattered light from the star would be minimized.

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© 2014 PearsonEducation, Inc. Chapter 13 Is it easy to photograph of a planet orbiting around another star? a) Yes, but a large telescope because the planet would be faint. b) No, because the brightness of the star would overwhelm the planet. c) Yes, but a space telescope must be used so that the scattered light from the star would be minimized.

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© 2014 PearsonEducation, Inc. Chapter 13 In order to maximize your chance of seeing a faint, cooler planet next to a brighter, hotter star, you should observe a) in visible light. b) in ultraviolet light. c) in infrared light. d) in X-ray light.

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© 2014 PearsonEducation, Inc. Chapter 13 In order to maximize your chance of seeing a faint, cooler planet next to a brighter, hotter star, you should observe a) in visible light. b) in ultraviolet light. c) in infrared light. d) in X-ray light.

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© 2014 PearsonEducation, Inc. Chapter 13 To detect an extrasolar planet by means of the Doppler shift, you look for a periodic shift of the spectrum lines a) of the star the planet is orbiting. b) of the planet. c) of the star and the planet.

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© 2014 PearsonEducation, Inc. Chapter 13 To detect an extrasolar planet by means of the Doppler shift, you look for a periodic shift of the spectrum lines a) of the star the planet is orbiting. b) of the planet. c) of the star and the planet.

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© 2014 PearsonEducation, Inc. Chapter 13 The orbital period of an unseen planet a) will be the same as period of the star's Doppler shift. b) will be much longer than the star's. c) will be much shorter than the star's.

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© 2014 PearsonEducation, Inc. Chapter 13 The orbital period of an unseen planet a) will be the same as period of the star's Doppler shift. b) will be much longer than the star's. c) will be much shorter than the star's.

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© 2014 PearsonEducation, Inc. Chapter 13 The shorter the period of the Doppler curve, a) the closer the unseen planet is to the star. b) the farther the unseen planet is from the star. c) the greater the mass of the planet. d) the smaller the mass of the planet. e) A and C

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© 2014 PearsonEducation, Inc. Chapter 13 The shorter the period of the Doppler curve, a) the closer the unseen planet is to the star. b) the farther the unseen planet is from the star. c) the greater the mass of the planet. d) the smaller the mass of the planet. e) A and C

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© 2014 PearsonEducation, Inc. Chapter 13 The larger the mass of the unseen planet, a) the larger the Doppler shift of the star. b) the smaller the Doppler shift of the star. c) the faster the period of the star's Doppler shift. d) the slower the period of the star's shift. e) A and C

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© 2014 PearsonEducation, Inc. Chapter 13 The larger the mass of the unseen planet, a) the larger the Doppler shift of the star. b) the smaller the Doppler shift of the star. c) the faster the period of the star's Doppler shift. d) the slower the period of the star's shift. e) A and C

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© 2014 PearsonEducation, Inc. Chapter 13 Suppose you found a star similar to the Sun moving back and forth with a period of 2 years. What could you conclude? a) It has a planet orbiting at less than 1 AU. b) It has a planet orbiting at greater than 1 AU. c) It has a planet orbiting at exactly 1 AU. d) It has a planet, but we don't know its mass so we can't know its orbital distance for sure.

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© 2014 PearsonEducation, Inc. Chapter 13 Suppose you found a star similar to the Sun moving back and forth with a period of 2 years. What could you conclude? a) It has a planet orbiting at less than 1 AU. b) It has a planet orbiting at greater than 1 AU. c) It has a planet orbiting at exactly 1 AU. d) It has a planet, but we don't know its mass so we can't know its orbital distance for sure.

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© 2014 PearsonEducation, Inc. Chapter 13 Jupiter is about 1/10 the diameter of the Sun. If it transited, how much would the Sun's light dim? a) about 10% (it would be 90% of its regular brightness) b) about 1% (it would be about 99% its regular brightness) c) about 30 % (it would be about 70% of its regular brightness) d) about 50% (it would be about half its regular brightness)

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© 2014 PearsonEducation, Inc. Chapter 13 Jupiter is about 1/10 the diameter of the Sun. If it transited, how much would the Sun's light dim? a) about 10% (it would be 90% of its regular brightness) b) about 1% (it would be about 99% its regular brightness) c) about 30 % (it would be about 70% of its regular brightness) d) about 50% (it would be about half its regular brightness)

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© 2014 PearsonEducation, Inc. Chapter 13 Most known extrasolar planets have larger masses than Jupiter. This means that a) our solar system is special in having many terrestrial planets, including Earth. b) all stars have smaller planets, but we just can't detect them yet. c) we won't know how many smaller planets are out there until our searches become more sensitive.

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© 2014 PearsonEducation, Inc. Chapter 13 Most known extrasolar planets have larger masses than Jupiter. This means that a) our solar system is special in having many terrestrial planets, including Earth. b) all stars have smaller planets, but we just can't detect them yet. c) we won't know how many smaller planets are out there until our searches become more sensitive.

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© 2014 PearsonEducation, Inc. Chapter 13 Most known extrasolar planets have periods of less than a few years, but are more massive than Jupiter. This means that a) our solar system has planets with unusually long orbits. b) the planets we've discovered so far follow this trend, but we may still discover longer-period extrasolar planets. c) other planetary systems do not have the same layout as our own. d) all of the above e) B and C

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© 2014 PearsonEducation, Inc. Chapter 13 Most known extrasolar planets have periods of less than a few years, but are more massive than Jupiter. This means that a) our solar system has planets with unusually long orbits. b) the planets we've discovered so far follow this trend, but we may still discover longer-period extrasolar planets. c) other planetary systems do not have the same layout as our own. d) all of the above e) B and C

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© 2014 PearsonEducation, Inc. Chapter 13 Our theory of solar system formation predicts that large, gaseous planets form far from their star. How can we explain the extrasolar hot Jupiters that are close to their stars? a) Our theory is wrong. b) Large planets do form far from their star, but their orbits can change due to gravitational encounters with other objects. c) Large planets do form far from their star, but waves of material can pull on planets and alter orbits. d) B and C

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© 2014 PearsonEducation, Inc. Chapter 13 Our theory of solar system formation predicts that large, gaseous planets form far from their star. How can we explain the extrasolar hot Jupiters that are close to their stars? a) Our theory is wrong. b) Large planets do form far from their star, but their orbits can change due to gravitational encounters with other objects. c) Large planets do form far from their star, but waves of material can pull on planets and alter orbits. d) B and C

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© 2014 PearsonEducation, Inc. Chapter 13 Space missions are currently underway to a) search for Earth-sized planets transiting stars. b) search for wobbles in stars caused by planets much less massive than Jupiter. c) attempt to take direct images of extrasolar planets. d) all of the above

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© 2014 PearsonEducation, Inc. Chapter 13 Space missions are currently underway to a) search for Earth-sized planets transiting stars. b) search for wobbles in stars caused by planets much less massive than Jupiter. c) attempt to take direct images of extrasolar planets. d) all of the above

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© 2014 PearsonEducation, Inc. Chapter 13 How can the Doppler shift be used to search for planets around other stars? a) Astronomers look for a periodic, red-then-blue shift in the spectrum of the planet. b) Astronomers look for a periodic, red-then-blue shift in the spectrum of the star. c) Astronomers look to see if the star "wobbles" in the sky, shifting slightly back and forth.

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© 2014 PearsonEducation, Inc. Chapter 13 How can the Doppler shift be used to search for planets around other stars? a) Astronomers look for a periodic, red-then-blue shift in the spectrum of the planet. b) Astronomers look for a periodic, red-then-blue shift in the spectrum of the star. c) Astronomers look to see if the star "wobbles" in the sky, shifting slightly back and forth.

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© 2014 PearsonEducation, Inc. Chapter 13 How do astronomers look for planets whose orbits might cause them to pass in front of a star outside our solar system? a) They look for a small black dot passing in front of the star. b) The look to see if the star's position shifts or "wobbles" slightly in the sky. c) The measure the star's brightness, and look for periodic dimming (transits).

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© 2014 PearsonEducation, Inc. Chapter 13 How do astronomers look for planets whose orbits might cause them to pass in front of a star outside our solar system? a) They look for a small black dot passing in front of the star. b) The look to see if the star's position shifts or "wobbles" slightly in the sky. c) The measure the star's brightness, and look for periodic dimming (transits).

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