CH 1 – Space – Flashcards

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In Ptolemy's geocentric model, retrograde motion occurs when the planet is closest to us, on the inside portion of the
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epicycle
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According to Copernicus, retrograde motion for Venus must occur around
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inferior conjunction, when it passes between us and the Sun.
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Which of these observations of Galileo refuted Ptolemy's epicycles?
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the complete cycle of Venus' phases
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The force of gravity varies with
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both product of the two masses and inverse square of the distance separating the two bodies.
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A planet whose distance from the Sun is 3 A.U. would have an orbital period of how many Earth-years?
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square root 27
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How much stronger is the gravitational pull of the Sun on Earth, at 1 AU, than it is on Saturn at 10 AU?
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100x
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According to Newton's second law, if you double the force acting on a body, the acceleration will double.
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true
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According to Newton's first law, an object traveling in a circle does not have a force acting on it.
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False
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Kepler relied heavily on the telescopic observations of Galileo in developing his laws of planetary motion.
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false
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Kepler found the orbits of planets are ellipses, not circles.
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True
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A planet (or comet) will speed up as it approaches the Sun
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True
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Copernicus believed the Earth was the center of all celestial motion.
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false
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According to Copernicus, retrograde motion occurs at opposition for the outer planets.
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True
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In Ptolemy's geocentric model, the planet's motion along its deferent is all that is needed to understand retrograde motion.
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False
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The place in a planet's orbit that is closest to the Sun is called
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perihelion
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geocentric
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-model is earth centered -retrograde motion is explained by epicycles
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heliocentric
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-this model is sun-centered -retrograde motion is explained by the orbital speeds of planets
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both geocentric and heliocentric
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-epicycles and deferents help explain planetary motion -planets move in circular orbits and with uniform motion -brightness of a planet increases when the planet is closest to earth
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heliocentric advantage
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explained planetary motions and brightness changes most simply
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geocentric advantage
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rooted in widely accepted religious beliefs regarding Earth's place in the universe
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both heliocentric and geocentric advantages
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-predicted planetary positions accurately over relatively short time periods -planetary orbits and motions based on Greek idealogies of perfect form motion
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The geocentric model, in all of its complexity, survived scientific scrutiny for almost 1400 years. However, in modern astronomy, scientists seek to explain the natural and physical world we live in as simply as possible. The complexity of Ptolemy's model was an indicator that his theory was inherently flawed. Why, then, was the geocentric model the leading theory for such a long time, even though the heliocentric model more simply explained the observed motions and brightness of the planets?
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-The geocentric model conformed to both the philosophical and religious doctrines of the time. -Ancient astronomers did not observe stellar parallax, which would have provided evidence in favor of the heliocentric model. -From Earth, all heavenly bodies appeared to circle around Earth, while Earth remained still. -The heliocentric model did not make noticeably better predictions than the geocentric model.
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Galileo Galilei was the first scientist to perform experiments in order to test his ideas. He was also the first astronomer to systematically observe the skies with a telescope. Galileo made four key observations that challenged the widely accepted philosophical beliefs on which the geocentric model was based, thus providing support for the heliocentric model. From the following list of observations, which are the key observations made by Galileo that challenged widespread philosophical beliefs about the solar system?
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-The Moon has mountains, valleys, and craters. -Jupiter has orbiting moons. -The Sun has sunspots and rotates on its axis. -Venus goes through a full set of phases.
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Johannes Kepler used decades of Tycho Brahe's observational data to formulate an accurate description of planetary motion. Kepler spent almost 30 years of his life trying to develop a simple description of planetary motion based on a heliocentric model that fit Tycho's data. What conclusion did Kepler eventually come to that revolutionized the heliocentric model of the solar system?
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Kepler determined that the planetary orbits are elliptical.
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Astronomers have made many observations since the days of Galileo and Kepler to confirm that the Sun really is at the center of the solar system, and that the planets revolve around the Sun in elliptical orbits. Which observation(s) could you make today that Galileo and Kepler could not have made to confirm that the heliocentric model is correct?
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-Stellar parallax in nearby stars -Transit of an extrasolar planet -Doppler shifts in stellar spectra of nearby stars
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