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Current evidence suggests that many massive jovian planets orbit at very close orbital distances to their stars.How do we think these planets ended up on these close orbits?


A) These planets are jovian in nature and were able to form close to their stars because their solar nebulas were very cold in temperature.
B) These planets migrated inward after being born on orbits much farther from their stars.
C) Despite their large masses,these planets are terrestrial in nature and therefore could form in their inner solar systems.
D) These planets were captured from other solar systems.

E) A) and B)
F) C) and D)

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Assuming that our ideas about how "hot Jupiters" ended up on their current orbits are correct,why didn't our own solar system end up with any hot Jupiters?


A) Our solar nebula must have been blown into space shortly after the formation of the jovian planets.
B) Our jovian planets must have migrated outward from inside the orbit of Mercury.
C) Our solar nebula must have stuck around for an unusually long time after the formation of jovian planets.
D) The existence of Earth and the other terrestrial planets prevented the jovian planets from migrating inward.

E) A) and B)
F) A) and C)

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The depth of the dip in a star's brightness due to the transit of a planet depends most directly on


A) the planet's mass.
B) the planet's density.
C) the planet's size.
D) the size of the planet's orbit.
E) the eccentricity of the planet's orbit.

F) B) and D)
G) B) and E)

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Planets detected via the Doppler technique have been mostly


A) Earth-mass,in Earth-like orbits.
B) Jupiter-mass,in Jupiter-like orbits.
C) Jupiter-mass,in very close orbits.
D) Earth-mass,in very close orbits.
E) a wide range of masses,in edge-on orbits.

F) D) and E)
G) None of the above

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The composition of a planet's atmosphere be measured during a transit by analyzing


A) the excess absorption of starlight at specific wavelengths.
B) the excess emission of starlight at specific wavelengths.
C) the length and depth of the dip in light during the transit.
D) the amplitude and period of the star's motion.
E) the wobble in a star's position on the sky.

F) A) and D)
G) B) and D)

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Suppose you are using the Doppler technique to look for planets around another star.What must you do?


A) Compare many spectra of an orbiting planet taken over a period of many months or years.
B) Compare the brightness of the star over a period of many months or years.
C) Carefully examine a single spectrum of an orbiting planet.
D) Compare many spectra of the star taken over a period of many months or years.

E) A) and B)
F) A) and C)

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Describe the impact the discovery of extrasolar planets h as had for understanding the origin of our own Solar System.

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The discovery of extrasolar planets show...

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Amateur astronomers are able to detect extrasolar planets with backyard telescopes using the transit method.

A) True
B) False

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Why do we say that the Doppler technique gives the planet's "minimum mass"?


A) The size of the Doppler shift that we detect depends on whether the planet's orbit is tilted.
B) The size of the Doppler shift that we detect depends on knowing the star's mass,which can be very uncertain.
C) Extrasolar planets are always increasing in mass.
D) Doppler measurements are very difficult,producing noisy data that often cause astronomers to underestimate a planet's mass.

E) All of the above
F) A) and B)

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What would happen to the planets in a solar system where the central star did not have a strong wind?


A) One planet would grow to dominate all the others and gravitationally eject them out of the system.
B) All planets would continue to grow to large sizes but their orbits would be unchanged.
C) The gas in the solar nebula would create a drag on the planets and their orbits would migrate inwards.
D) The gas in the solar nebula would create a drag on the planets and their orbits would migrate outwards.
E) Nothing,the star does not affect the process of planet formation.

F) B) and E)
G) C) and D)

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Because we have not found another planetary system like our own,we can conclude that our Solar System must be quite unusual.

A) True
B) False

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What is an extrasolar planet?


A) a planet that orbits a star that is not our own Sun
B) a planet that is larger than the Sun
C) a planet that is extra large compared to what we'd expect
D) a planet that is considered an "extra," in that it was not needed for the formation of its solar system

E) All of the above
F) C) and D)

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Which planet can we see occasionally transit across the face of the Sun?


A) Mercury
B) Mars
C) Jupiter
D) Uranus
E) all of the above

F) A) and B)
G) A) and C)

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A planet is detected via the Doppler technique.The repeating pattern of the stellar motion tells us


A) the planet's size.
B) the planet's mass.
C) the planet's density.
D) the orbital period of the planet.
E) the orbital eccentricity of the planet.

F) C) and E)
G) A) and D)

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Process of Science: Why did some astronomers think that we would not be able to detect planetary systems around other stars so quickly as we did?

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If we simply extrapolated from our own S...

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Which of the following is a consequence of the discovery of hot Jupiters for the nebular theory of solar system formation?


A) It has been discarded.
B) It has been modified to allow for the formation of gas giants within the frost line.
C) It has been modified to allow for planets to migrate inwards or outwards due to gravitational interactions.
D) Its status is unclear and awaits further observations that will determine whether hot Jupiters are dense Earth like planets or gas giants.
E) It remains unchanged as it only needs to explain our Solar System.

F) B) and C)
G) C) and D)

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When should we know if any extra-solar planetary systems are like ours?


A) in just a few years
B) any day now,thanks to new,large,ground-based telescopes
C) in a decade or two,through our current space missions
D) We have already discovered several systems just like ours,through the Kepler mission.

E) B) and C)
F) B) and D)

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Process of Science: Name a testable hypothesis of nebular theory that was shown to be incorrect in observations of extrasolar planets. Must we throw out the theory and start from scratch, i.e., is the observation completely inconsistent with a nebular formation?

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At face value, the nebular theory predic...

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How much brighter is a Sun-like star than the reflected light from a planet orbiting around it?


A) a hundred times brighter
B) a thousand times brighter
C) ten thousand times brighter
D) a million times brighter
E) a billion times brighter

F) A) and D)
G) B) and C)

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How will TESS build upon the Kepler mission?


A) It will zoom in on the best planet candidates and allow us to confirm whether or not they are actually planets.
B) It will use the same strategy but will cover the whole sky.
C) It will allow us to detect extrasolar planets from the Southern hemisphere instead of just the Northern hemisphere.
D) It will allow us to observe in a different wavelength.

E) A) and C)
F) C) and D)

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