Lecture 1: The Orbital Velocity Vector and Kepler's Third Law
(Vallado, Sections 1.3.5, 1.3.6)
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Animation of Kepler's second law
Homework 4 Solution:
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Lecture 2: Introduction to Orbital Dynamics,
Solution of the Restricted Two-Body Problem
(Vallado, Sections 1.3.2, 1.3.3, 1.3.6)
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Lecture 3: Orbital Energy and the Vis-Viva Equation
(Vallado, Sections 1.3.2, 1.3.3, 1.3.6)
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Homework 5 Solution:
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