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AE 351 - Orbital Mechanics
Class Hour(s) 3
Laboratory Hour(s) 0
3 Semester Credit Hour(s)
Newton’s equations and Keplers laws. Use of spherical coordinates to solve for orbital equations. Corrections to basic equations caused by earth’s geometry, the moon and the sun. Other effects depending on orbital parameters. Offered during Fall semester only. Offered during Fall semester only.
Corequisite(s): MA 340
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