Lecture 1 | Modern Physics: Special Relativity (Stanford)
Lecture 1 of Leonard Susskind's Modern Physics course concentrating on Special Relativity. Recorded April 14, 2008 at Stanford University. This Stanford Continuing Studies course is the third of a six-quarter sequence of classes exploring the essential theoretical foundations of modern physics. The topics covered in this course focus on classical mechanics. Leonard Susskind is the Felix Bloch Professor of Physics at Stanford University. Complete Playlist for the Course: http://www.youtube.com/view_play_list... Stanford Continuing Studies: http://continuingstudies.stanford.edu/ About Leonard Susskind: http://www.stanford.edu/dept/physics/... Stanford University Channel on YouTube: http://www.youtube.com/stanford Category: Education Tags: Physics math calculus geometry algebra theoretical minimum special relativity classical field theory reference frame uniform velocity Newton Laws of nature speed light wave maxwell space time Einstein hyperbolic functions cos
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We conclude our study by proving, with mathematical rigour as always, Kepler's Third Law - the square of the period of a planet moving around its elliptical orbit is proportional to the cube of its semimajor axis of that orbit. Check out www.gaussianmath.com for an indepth study or more calculus related content.
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We shall prove Kepler's First Law: A planet revolves in an elliptical orbit with the sun at one of its focus. This simple looking law actually turns out to be the hardest one to derive.
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Keplers Laws - Preliminaries pt1
Before we prove Kepler's Laws, we need to formulate some preliminaries namely setting up the coordinate axis. Check out www.gaussianmath.com for a more indepth explanation and more calculus-related content.
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