The fifth-order analytical solution of the equations of motion of a satellite in orbit around a non-spherical planet

DOI10.1007/BF00051893zbMath0852.70013OpenAlexW2083532970MaRDI QIDQ1894305

Sergej M. Kudryavtsev

Publication date: 16 December 1996

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00051893

zbMATH Keywords

secular perturbationsplanetary potential expansionPoisson's small parameter methodshort-periodic perturbations

Mathematics Subject Classification ID

Celestial mechanics (70F15) Orbital mechanics (70M20)

Related Items (2)

Position and velocity perturbations for the determination of geopotential from space geodetic measurements ⋮ Analytic orbit theory with any arbitrary spherical harmonic as the dominant perturbation

Uses Software

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Cites Work

• [https://portal.mardi4nfdi.de/wiki/Publication:4058271 Th�orie analytique programm�e du mouvement des satellites artificiels sous l'action gravitationnelle de la terre]
• The main problem of artificial satellite theory for small and moderate eccentricities
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