Exam 4: The Origin of Modern Astronomy

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____________________ is a description of the Ptolemaic model of the solar system.

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Once a theory has been tested thoroughly and is confidently believed by scientists, it becomes a ____________________.

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What is the circular velocity of an object orbiting Earth at a distance of 100,000 km from Earth's center? What is the circular velocity of an object orbiting Earth at a distance of 100,000 km from Earth's center?   G = 6.67*10<sup>-</sup><sup>11</sup> m<sup>3</sup>.kg<sup>-</sup><sup>1</sup>.s<sup>-</sup><sup>2</sup>; M<sub>Earth</sub> = 5.98*10<sup>24</sup>kg G = 6.67*10-11 m3.kg-1.s-2; MEarth = 5.98*1024kg

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The orbit of the planet Jupiter is an ellipse with the sun at one focus. What is located at the other focus?

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Ptolemy's model of the universe

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How did Tycho Brahe's model of the universe differ from that of Ptolemy? How did Tycho Brahe's model of the universe differ from that of Copernicus?

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The neap tides can only occur when the moon's position is at or near one of its orbital nodes.

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Which of the following people did NOT accept a heliocentric model for the universe?

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The first observations of objects in the solar system that orbited neither the sun nor Earth were made by ____________________.

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The book "De Revolutionibus Orbium Coelestium"

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The ____________________ Tables were based on a heliocentric model of the universe and used elliptical orbits for the planets.

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The semimajor axis of an ellipse is

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The purpose of using epicycles and deferents to explain the motion of the planets in the night sky was to account for

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The greatest inaccuracy in Copernicus's model of the solar system was that the planets

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Describe one observation that would disprove the Ptolemaic model and explain why it would conflict with the model.

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Parallax is the apparent change in location of an object due to the motion of the observer.

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Why were Galileo's telescopic observations of the phases of Venus critical evidence in favor of the Copernican theory?

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Kepler's second law implies that

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The force of gravity from one object extends to infinity never going to zero. When we say that gravitation is universal we mean that

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How can tidal forces affect the rotation of celestial bodies and their orbital motion? Hint: Consider Earth and the moon.

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