A) period and the length of the semimajor axis.
B) eccentricity and the length of the semimajor axis.
C) period and orbital eccentricity.
D) period and mass.
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Multiple Choice
A) distance at which Earth-Sun distance will subtend an angle of 1 arcsecond.
B) mean distance between the Sun and Earth.
C) radius of the Sun.
D) distance traveled by light in 1 year.
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Multiple Choice
A) inferior conjunction.
B) superior conjunction.
C) opposition.
D) greatest elongation.
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Multiple Choice
A) development of the first mathematical heliocentric model of the solar system.
B) the first model in which planetary orbits are ellipses.
C) use of parallax to prove that Earth moves around the Sun.
D) observation of the satellites (moons) of Jupiter.
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Multiple Choice
A) circle, with the Sun at the center.
B) elliptical orbit, with the Sun at one focus.
C) elliptical orbit, with the Sun on the minor axis of the ellipse.
D) elliptical orbit, with the Sun at the center of the ellipse.
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Multiple Choice
A) about 1048 A.D.
B) 786 B.C.
C) 1054 A.D., of course
D) about 4946 B.C.
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Multiple Choice
A) inferior conjunction.
B) superior conjunction.
C) opposition.
D) greatest elongation.
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Multiple Choice
A) Yes.
B) No. Kepler included the effect of the planet's mass, whereas Newton did not.
C) No. Newton included the effect of the planet's mass, whereas Kepler did not.
D) No. Kepler's equation applied only to the inner planets, whereas Newton's applied to all the planets.
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Multiple Choice
A) full
B) gibbous
C) new
D) None of these are correct; they are all visible.
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Multiple Choice
A) opposition.
B) greatest elongation.
C) superior conjunction.
D) None of these are correct.
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Multiple Choice
A) Earth moves.
B) planet's speed changes along its elliptical orbit.
C) planet rotates about its own axis in addition to its orbital motion.
D) the planet moves.
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Multiple Choice
A) magnetism.
B) gravitation.
C) electrical forces.
D) no underlying physical theory.
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Multiple Choice
A) Earth-centered, with the planets, the Sun, and the stars mounted on crystal spheres, pivoted to allow the correct motions around Earth.
B) Earth-centered, with the planets moving in epicycles around Earth.
C) Sun-centered, with the planets moving in elliptical orbits and the Sun at one focus of the ellipse.
D) Sun-centered, with the planets moving in perfect circles around the Sun.
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Multiple Choice
A) star in our Galaxy
B) asteroid in our solar system
C) artificial satellite orbiting Earth
D) distant galaxy
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Multiple Choice
A) Kepler.
B) Ptolemy.
C) Aristotle.
D) Copernicus.
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Multiple Choice
A) 8.55 au
B) 125 au
C) 1 au
D) 25 au
Correct Answer
verified
Multiple Choice
A) 500 kg-m.
B) 20 W.
C) 20 J.
D) 500 J.
Correct Answer
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Multiple Choice
A) 1314.5 au
B) 24.33 au
C) 25.33 au
D) 23.33 au
Correct Answer
verified
Multiple Choice
A) no allowance for retrograde motion.
B) placement of the planets on epicycles, the centers of which followed orbits around the Sun.
C) the assumption that the planets move in elliptical orbits with constant speeds rather than variable speeds.
D) placement of the planets in circular orbits.
Correct Answer
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Multiple Choice
A) phases like the Moon's
B) nothing because Venus is perpetually cloud-covered
C) four satellites (moons) orbiting Venus
D) a set of rings
Correct Answer
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