Long period variations of the motion of a satellite due to non-resonant tesseral harmonics of a gravity potential
type: Item
instance of: scholarly article
title: Long period variations of the motion of a satellite due to non-resonant tesseral harmonics of a gravity potential
zbMATH Open document ID: 0785.70022
DOI: 10.1007/BF00692472
author: Gilles Métris
author: Y. Boudon
author: F. Barlier
author: Pierre Exertier
published in: Celestial Mechanics and Dynamical Astronomy
publication date: 1994-04-27T00:00:00Z
Mathematics Subject Classification ID: 70M20
Mathematics Subject Classification ID: 70F15
zbMATH DE Number: 486922
zbMATH Keywords: second order perturbations
zbMATH Keywords: Kaula eccentricity and inclination functions
zbMATH Keywords: Earth's geodetic satellites
zbMATH Keywords: secular effects
zbMATH Keywords: Phobos
MaRDI profile type: Publication
cites work: Canonical transformations depending on a small parameter
cites work: The main problem of artificial satellite theory for small and moderate eccentricities
cites work: Tesseral resonance effects on satellite orbits
cites work: Q4174835
cites work: On the motion of a satellite in resonance with its rotating planet
cites work: Tesseral harmonic perturbations for high order and degree harmonics
cites work: Tesseral harmonic perturbations in radial transverse and binormal components
full work available at URL: https://doi.org/10.1007/bf00692472
OpenAlex ID: W4233080858
description: scientific article; zbMATH DE number 486922