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PDF document - Orbital and Celestial Mechanics Website

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wheremsc iis the initial spacecraft mass, <strong>and</strong> piis the semiparameter of the initial orbit <strong>and</strong>pfis thesemiparameter of the final orbit. The upper bound on true longitude L allows for a maximum of 200complete orbits during the transfer.Finally, the components of the unit thrust vector are constrained as follows:Technical discussion1.1 u 1.11.1 u 1.11.1 u 1.1The modified equinoctial orbital elements are a set of orbital elements that are useful for trajectoryanalysis <strong>and</strong> optimization. They are valid for circular, elliptic, <strong>and</strong> hyperbolic orbits. These equationsexhibit no singularity for zero eccentricity <strong>and</strong> orbital inclinations equal to 0 <strong>and</strong> 90 degrees. However,two components of the orbital element set are singular for an orbital inclination of 180 degrees.The relationship between direct modified equinoctial <strong>and</strong> classical orbital elements is defined by thefollowing definitionsrtn21 cosp a e f e g esin h tan i 2 cosk tan i 2 sin L wherep a e i L semiparametersemimajor axisorbital eccentricityorbital inclinationargument of periapsisright ascension of the ascending nodetrue anomalytrue longitudeThe relationship between classical <strong>and</strong> modified equinoctial orbital elements is:psemimajor axis a 2 21 f gorbital eccentricity2 2e f gorbital inclination i 2 tan 1 h 2 k2page 16

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