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An important perturbation affecting low planetary satellites is the planet’s oblateness, approximated mathematically by the second zonal harmonic J2, discussed in Sect. 11.10 The problem of motion in such a potential field is often referred to as the main problem in artificial satellite theory, and has been the subject of many studies over the years ...
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Collision orbits in the oblate planet problem
Celestial Mechanics, 1984Summary: Some of the properties of the oblate planet problem are derived. We use the technique of blowing up the singularity to study the collision orbits.
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