The possible motions of a satellite about an oblate planet
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Publication:3667988
DOI10.1007/BF01231101zbMath0518.70014OpenAlexW1996719939MaRDI QIDQ3667988
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Publication date: 1983
Published in: Celestial Mechanics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/bf01231101
two degrees of freedomenergy integralequilibrium solutionstopological propertiesconservativecircular equatorial orbitsHill stableregions of motions of satellite around oblate planet
Dynamical aspects of finite-dimensional Hamiltonian and Lagrangian systems (37J99) Celestial mechanics (70F15) Orbital mechanics (70M20)
Related Items (2)
Numerical integration of periodic orbits in the main problem of artificial satellite theory ⋮ Collision orbits in the oblate planet problem
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