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The average density of a planet can be obtained from


A) the Doppler method only
B) a combination of the Doppler and transit methods
C) the transit method only
D) a combination of the astrometric and Doppler methods

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

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The wavelengths of radiation from a star that is moving toward us


A) can be longer or shorter depending on the distance to the star
B) are shorter than if the star were not moving
C) are longer than if the star were not moving
D) are the same as if the star were not moving

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

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All stars on the main sequence


A) are in the process of forming
B) are mature stars that are fusing hydrogen into helium in their cores
C) are dead stars
D) have exhausted their nuclear fuel and are in the process of dying

E) None of the above
F) B) and C)

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Orphan planets will most likely be found using which method used for finding exoplanets?


A) Doppler
B) transit
C) microlensing
D) astrometric

E) B) and C)
F) None of the above

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Which space mission is searching for extrasolar planets using the astrometric method?


A) Kepler
B) GAIA
C) CoRoT
D) Spitzer

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

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Stars only exhibit a Doppler shift if they are moving


A) away from us along the line of sight
B) perpendicular to our line of sight
C) in a circular motion about us
D) toward or away from us along the line of sight

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

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What is the simplest way we might detect life on an extrasolar planet?


A) listen for radio signals coming from an advanced civilization on the planet
B) wait for aliens from the planet to visit us
C) analyze the spectrum of reflected light from the planet
D) send an interstellar probe to the planetary system

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

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The Hertzprung-Russell diagram is a plot of


A) radial velocity against distance
B) apparent brightness against time
C) luminosity against distance
D) luminosity against surface temperature

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

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White dwarfs


A) are dead stars
B) are in the process of forming
C) are mature stars that are fusing hydrogen into helium in their cores
D) have exhausted their nuclear fuel and are in the process of dying

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

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When we measure the mass of a planet using the Doppler shift method, we know that it is mass


A) could well be smaller
B) could be larger or smaller
C) is exactly as measured
D) could well be larger

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

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Which of the following could be a stable planetary orbit in a binary system?


A) a large orbit around both stars in a close binary system
B) a "figure-of-eight" orbit about both stars in a close binary system
C) an orbit close to one of the stars in a close binary system
D) a large orbit around both stars in a wide binary system

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

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What is the spectral type of the Sun?


A) K9
B) G2
C) F7
D) A2

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

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B-type stars have lifetimes


A) long enough for advanced life to evolve
B) too short for planet formation
C) long enough for planets to form but not for life to appear
D) long enough for planets to form and for simple life to appear, but not long enough for advanced life to develop

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

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The center of mass of the solar system is


A) midway between the Sun and Jupiter
B) exactly at the center of the Sun
C) just outside the orbit of Mercury
D) close to but not exactly at the center of the Sun

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

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What is a major limitation in the Doppler method for detecting extrasolar planets?


A) it is better at finding massive planets like Jupiter rather than small planets like the Earth
B) it is best suited to finding planets which orbit relatively close to their star
C) it requires the use of fairly large telescopes and long exposures which limits the number of star that can be studied
D) all of these are major limitations

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

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The radial velocity curve of a star with an extrasolar planet is a plot of


A) radial velocity against luminosity
B) radial velocity against brightness
C) radial velocity against distance
D) radial velocity against time

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

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Studies of multiplanet exoplanet systems have shown us that other planetary systems can sometimes differ from ours by


A) having their planets packed much closer to each other than our solar system's planets
B) exist in binary star systems
C) containing planets with much lower masses
D) two of these

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

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What is the minimum possible mass for a star?


A) 0.01 solar masses
B) 0.008 solar masses
C) 0.1 solar masses
D) 0.08 solar masses

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

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M-type stars in our galaxy are


A) fairly common (several percent)
B) the most common type of stars in our galaxy (75% or more)
C) very common, making up about 50% of the total
D) very rare (less than 1%)

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

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A planet with a density comparable to the Earth but several times more massive is described as a


A) mini-Neptune
B) super-Earth
C) mega-Earth
D) super-Jovian

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

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