The accelerated longitude drift regimes of eccentric 12-hr orbits are considered, due to the resonant geopotential. These quasi-stationary orbits are under investigation at NASA for large payload earth surveillance spacecraft in the small applications technology satellite (SATS) program. Inclinations near 'critical' are especially attractive because of their possible long term stability, and these are examined in detail. 'Stable' equator crossing longitudes for these satellites are found as functions of the argument of perigee. As long as the argument of perigee is between plus or minus 100 deg, these stable longitudes lie within a narrow range. Maximum 'east-west' stationkeeping requirements for these satellites at nonequilibrium positions are in the range of 0.3 to 3 m/sec/yr.
Stable longitudes for 12-hr eccentric orbit satellites.
01.10.1972
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Stable longitudes for 12-hr eccentric orbit satellites.
AIAA | 1972
|Stable Longitudes for 12 Hour Eccentric Orbit Satellites
NTIS | 1971
|Equilibrium longitudes of geostationary satellites.
AIAA | 1968
|British Library Online Contents | 2002
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