@Article{SolórzanoPrad:2007:ApNoVa,
author = "Sol{\'o}rzano, Carlos Renato Huaura and Prado, Antonio Fernando
Bertachini de Almeida",
title = "Third-Body Perturbation Using a Single Averaged Model: Application
in Nonsingular Variables",
journal = "Mathematical Problems in Engineering",
year = "2007",
volume = "Article ID 40475",
abstract = "The Lagranges planetary equations written in terms of the
classical orbital elements have the disadvantage of singularities
in eccentricity and inclination. These singularities are due to
the mathematical model used and do not have physical reasons. In
this paper, we studied the third-body perturbation using a single
averaged model in nonsingular variables. The goal is to develop a
semianalytical study of the perturbation caused in a spacecraft by
a third body using a single averaged model to eliminate
short-period terms caused by themotion of the spacecraft. This is
valid if no resonance occurs with themoon or the sun. Several
plots show the time histories of the Keplerian elements of
equatorial and circular orbits, which are the situations with
singularities. In this paper, the expansions are limited only to
second order in eccentricity and for the ratio of the semimajor
axis of the perturbing and perturbed bodies and to the fourth
order for the inclination.",
doi = "10.1155/2007/40475",
url = "http://dx.doi.org/10.1155/2007/40475",
issn = "1024-123X and 1563-5147",
language = "en",
targetfile = "S1024123X07404756[1].pdf",
urlaccessdate = "21 maio 2024"
}