The possible motions of a satellite about an oblate planet |
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| Authors: | K Zare |
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| Institution: | 1. System Analysis Department, Ford Aerospace and Communication Corporation, 94303, Palo Alto, CA, USA
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| Abstract: | The regions of motions of a satellite for given values of energy and angular momentum about polar axes are shown. Special attention is paid to the circular equatorial orbits which have been shown to be Hill stable. The anomalistic and the nodal period for the motions near to the circular equatorial orbits have been found. |
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