Long-term motion of resonant satellites with arbitrary eccentricity and inclination

DOI10.1007/BF01228561zbMath0501.70031MaRDI QIDQ3967112

Roger E. Diehl, Paul E. Nacozy

Publication date: 1982

Published in: Celestial Mechanics (Search for Journal in Brave)

zbMATH Keywords

semi-analyticalaveraged Hamiltonianaveraging processthree degrees of freedomthird-body effectslong-term motionany inclinationgeo-synchronous satelliteslocation of libration centersmodified von Zeipel methodtesseral and zonal harmonics

Mathematics Subject Classification ID

Computational methods for problems pertaining to mechanics of particles and systems (70-08) Astronomy and astrophysics (85A99) Celestial mechanics (70F15) Orbital mechanics (70M20) Canonical and symplectic transformations for problems in Hamiltonian and Lagrangian mechanics (70H15)

Related Items (1)

A problem of libration with two degrees of freedom

Cites Work

• Unnamed Item
• The motion of a satellite in resonance with the second-degree sectorial harmonic
• Satellite resonances and librations associated with Tesseral harmonics of the geopotential
• Some useful results on initial node locations for near-equatorial circular satellite orbits
• On the motion of a 24-hour satellite

This page was built for publication: Long-term motion of resonant satellites with arbitrary eccentricity and inclination