Exam 3: Motion of Astronomical Bodies
Exam 1: Why Learn Astronomy92 Questions
Exam 2: Patterns in the Skymotions of Earth96 Questions
Exam 3: Motion of Astronomical Bodies91 Questions
Exam 4: Gravity and Orbits88 Questions
Exam 5: Light87 Questions
Exam 6: The Tools of the Astronomer94 Questions
Exam 7: The Birth and Evolution of Planetary Systems87 Questions
Exam 8: The Terrestrial Planets and Earths Moon99 Questions
Exam 9: Atmospheres of the Terrestrial Planets92 Questions
Exam 10: Worlds of Gas and Liquid the Giant Planets92 Questions
Exam 11: Planetary Adornmentsmoons and Rings93 Questions
Exam 12: Dwarf Planets and Small Solar System Bodies89 Questions
Exam 13: Taking the Measure of Stars88 Questions
Exam 14: Our Starthe Sun88 Questions
Exam 15: Star Formation and the Interstellar Medium89 Questions
Exam 16: Evolution of Low-Mass Stars90 Questions
Exam 17: Evolution of High-Mass Stars90 Questions
Exam 18: Relativity and Black Holes90 Questions
Exam 19: The Expanding Universe90 Questions
Exam 20: Galaxies95 Questions
Exam 21: The Milky Waya Normal Spiral Galaxy96 Questions
Exam 22: Modern Cosmology92 Questions
Exam 23: Large-Scale Structure in the Universe65 Questions
Exam 24: Life61 Questions
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Based on the figure below, an inferior planet would be farthest from the Sun and therefore most easily visible at: 

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Name the two ways in which an object's motion (meaning its velocity) can experience a nonzero acceleration.
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The object can have a nonzero acceleration if the speed of its velocity changes or if the direction of the velocity changes.
Based on his observations of the planets, Copernicus calculated the relative distance of the planets from the Sun using the heliocentric model, and these distances were:
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Galileo's telescopic observations of _________ led him to conclude that the heliocentric model of the Solar System was correct.
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The natural tendency of an object to resist changes in motion is called:
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What is your acceleration if you go from 0 to 60 mph in 4 seconds?
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Newton's second law says that more massive objects are accelerated more than less massive objects when the same force is applied.
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When the Sun, the Earth, and a planet all lie along a straight line, the planet is at:
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When the Earth catches up to a slower moving outer planet and passes it like a faster runner overtaking a slower runner in an outside lane, the planet:
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Saturn has a semimajor axis of 9.6 AU. How long does it take Saturn to orbit once around the Sun?
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The eccentricity of the majority of the planetary orbits in our Solar System is approximately:
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If a 100-kg astronaut pushes on a 5,000-kg satellite and the satellite experiences an acceleration of 0.1 m/s2, what is the acceleration experienced by the astronaut in the opposite direction?
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In the heliocentric model of the Solar System, does retrograde motion occur for superior or inferior planets? (It might help you to draw some illustrations to answer this question.)
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A comet orbits the Sun with a semimajor axis of 90 AU. Using Kepler's third law, the comet's orbital period is approximately
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Based on the figure shown below, explain why an inferior planet would not be able to be seen at all from Earth when it is in conjunction. 

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If you apply a force of 10 N to a grocery cart and get an acceleration of 0.5 m/s2, then the mass of the grocery cart is:
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Johannes Kepler obtained accurate data on the positions of the planets in the sky over time, which Galileo used to prove that planets revolved around the Sun.
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During a certain comet's orbit around the Sun, its closest distance to the Sun is 0.6 AU, and its farthest distance from the Sun is 35 AU. At what distance will the comet's orbital velocity be the largest?
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A planet travels fastest in its orbit when it is closest to the Sun.
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