Abstract
The concept of closest approach is analyzed in Hill’s problem, resulting in a partitioning of the position space. The different behavior between the direct and retrograde motion is explained analytically, resulting in a simple estimate of the variation of Hill’s periodic and quasi-circular orbits as a function of the Jacobi constant. The local behavior of the orbits on the zero velocity surfaces and an analytical definition of local escape and capture in Hill’s problem are also given.
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Villac, B., Scheeres, D. On The Concept Of Periapsis In Hill’s Problem. Celestial Mech Dyn Astr 90, 165–178 (2004). https://doi.org/10.1007/s10569-004-0405-9
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DOI: https://doi.org/10.1007/s10569-004-0405-9