Aristotle s orbital motion theory
[DOC File]Chapter 2: The Copernican Revolution
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Aristotle . Ptolemy . Heliocentric Models and the Birth of Modern Astronomy. Copernicus . Brahe . Galileo . Kepler’s Laws of Planetary Motion . Isaac Newton . Laws of Motion . Gravity . Explaining Orbits and Kepler’s Laws. Teaching Suggestions and Demonstrations . Section 2.1
[DOC File]History of Science Lecture 3 Galileo Galilei
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Ptolemy’s theory explained the retrograde motion of the planets. Predicted future locations of the planets Copernicus Heliocentric Theory. Copernicus sought to explain the retrograde motion of planets using a heliocentric solar system. He still assumed perfect circles for the orbits of planets (with the Sun at the center of the orbits).
[DOC File]Chapter 1
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The greater an object's mass, the more inertia it has, and the greater is the force needed to change its state of motion. Newton's first law contrasts sharply with the view of Aristotle, who maintained (incorrectly) that the natural state of an object was to be at rest—most probably an opinion based on Aristotle's observations of the effect ...
[DOC File]History of our Conceptualization of the Atom
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Quantum mechanics was initially developed to explain the atom, especially the spectra of light emitted by different atomic species. The quantum theory of the atom developed as an explanation for the electron's staying in its orbital, which could not be explained by Newton's laws of motion and by classical electromagnetism.
[DOCX File]Unit B - DYNAMICS
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Unit 2A – Newton’s 3 Laws of Motion. Isaac Newton and the Principia Mathematica. Dynamics is the study of why things move. Why things move the way they do is because of . forces. and Newton’s 3 Laws of Motion. In 1687, Newton outlined his monumental . 3 Laws of Motion: Law I.
[DOC File]The Cosmic Engine
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Orbital periods could be accurately determined. It explained the difference between the inferior planets (Mercury and Venus) that were always observed close to the Sun and the superior ones (Mars, Jupiter and Saturn). It preserved the concept of uniform circular motion. It preserved Aristotle's concept of real spheres nestled inside one another.
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