The classical Laplace plane as a stable disposal orbit for geostationary satellites |
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Authors: | Aaron J. Rosengren Daniel J. Scheeres Jay W. McMahon |
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Affiliation: | Department of Aerospace Engineering Sciences, University of Colorado at Boulder, Boulder, CO 80309, USA |
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Abstract: | ![]() The classical Laplace plane is a frozen orbit, or equilibrium solution for the averaged dynamics arising from Earth oblateness and lunisolar gravitational perturbations. The pole of the orbital plane of uncontrolled GEO satellites regress around the pole of the Laplace plane at nearly constant inclination and rate. In accordance with Friesen et al. (1993), we show how this stable plane can be used as a robust long-term disposal orbit. The current graveyard regions for end-of-life retirement of GEO payloads, which is several hundred kilometers above GEO depending on the spacecraft characteristics, cannot contain the newly discovered high area-to-mass ratio debris population. Such objects are highly susceptible to the effects of solar radiation pressure exhibiting dramatic variations in eccentricity and inclination over short periods of time. The Laplace plane graveyard, on the contrary, would trap this debris and would not allow these objects to rain down through GEO. Since placing a satellite in this inclined orbit can be expensive, we discuss some alternative disposal schemes that have acceptable cost-to-benefit ratios. |
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Keywords: | Geosynchronous orbit High area-to-mass ratio objects Space debris Disposal orbits Celestial mechanics Dynamical evolution and stability |
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