A) orbit an object.
B) overcome the gravitational pull of an object.
C) overtake an object in orbit and pass it.
D) keep from falling out of orbit around an object.
E) maintain a constant distance from an object.
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Multiple Choice
A) the mass of the planet only.
B) the mass of the Sun only.
C) both the mass of the planet and the mass of the Sun.
D) the mass of the planet and its distance from the Sun.
E) the mass of both the planet and the Sun and the distance between the two.
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Multiple Choice
A) Aristotle.
B) Pythagoras.
C) Hipparchus.
D) Ptolemy.
E) Erastothenes.
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A) it had the authority of Aristotle behind it.
B) it was consistent with the doctrines of the Catholic Church.
C) it used perfect circles, which appealed to geometry.
D) it accounted well for Galileo's observations of the phase cycle of Venus.
E) it explain why stellar parallax was not observed by the Greeks.
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Multiple Choice
A) transits of Venus across the Sun
B) radar echo timings
C) measurement of stellar parallaxes.
D) timings of the eclipses of its moons by Jupiter's shadow
E) precise measurements of length of the year with atomic clocks
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True/False
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Multiple Choice
A) Artificial satellites could be put into orbit about the Earth.
B) The Sun's gravity is greatest on a planet at perihelion, so the planet must speed up.
C) The Moon pulls as strongly on us as we do on it.
D) His differential calculus lets us calculate planetary motions more accurately.
E) All of these were due to Newton's work.
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Multiple Choice
A) The Moon orbits the Earth.
B) The Earth orbits the Sun.
C) Retrograde motion occurs when one planet overtakes another.
D) The orbits of the planets are ellipses, with one focus at the Sun.
E) Venus will appear as a crescent when she retrogrades between us and the Sun.
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