Because planets do not move in precisely circular orbits, the computation of the
Chapter 6, Problem 6.2.97(choose chapter or problem)
Because planets do not move in precisely circular orbits, the computation of the position of a planet requires the solution of Keplers equation. Keplers equation cannot be solved algebraically. It has the form M e sin , where M is the mean anomaly, e is the eccentricity of the orbit, and is an angle called the eccentric anomaly. For the specified values of M and e, use graphical techniques to solve Keplers equation for to three decimal places.
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