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Oct 2007
38m 52s

Lecture 19: Orbits

Richard Pogge
About this episode
Why do Kepler's Laws work? In this lecture I will describe Newton's generalization of Kepler's Laws of Planetary Motion so that they will apply to any two massive bodies orbiting around their common center of mass. I will introduce families of open and closed orbits, the circular and escape speeds, center-of-mass, conservation of angular momentum, and New ... Show More
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Oct 2007
Lecture 18: The Apple and the Moon - Newtonian Gravitation
What is Gravity? Starting with the properties of falling bodies first formulated by Galileo, Newton applied his three laws of motion to the problem of Universal Gravitation. Newtonian Gravity is a mutually attractive force that acts at a distance between any two massive bodies. I ... Show More
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Oct 2007
Lecture 17: On the Shoulders of Giants: Isaac Newton and the Laws of Motion
Copernicus, Kepler, Tycho, and Galileo together gave us a new way of looking at the motions in the heavens, but they could not explain why the planets move they way the do. It was to be the work of Isaac Newton who was to sweep away the last vestiges of the Aristotelian view of t ... Show More
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Oct 2007
Lecture 16: The Starry Messenger - Galileo and the Telescope
Tycho reached the limits of what could be done with the naked eye. A new technology was required to extend our vision: the telescope. This lecture introduces Galileo Galilei, the contemporary of Kepler who was in many ways the first modern astronomer, and describes his many disco ... Show More
41m 48s
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