@Article{DomingosPradMora:2013:StBeAv,
author = "Domingos, R C and Prado, Antonio Fernando Bertachini de Almeida
and Moraes, R Vilhena de",
affiliation = "{Universidade Faderal de S{\~a}o Paulo (UNIFESP)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and Universidade Federal
de S{\~a}o Paulo (UNIFESP), S{\~a}o Jos{\'e} dos Campos, SP,
Brazil",
title = "Studying the behaviour of averaged models in the third body
perturbation problem",
journal = "Journal of Physics: Conference Series",
year = "2013",
volume = "465",
number = "1",
pages = "Article number 012017",
note = "16th Brazilian Colloquium on Orbital Dynamics; Serra Negra, Sao
Paulo; Brazil; 26 November 2012 through 30 November 2012",
keywords = "Astrodin{\^a}mica, Mec{\^a}nica Celeste, Perturba{\c{c}}{\~a}o
de Terceiro Corpo.",
abstract = "The main goal of the present paper is to perform a study of the
behaviour of the single and double averaged methods used to study
the third-body perturbation problem in celestial mechanics. Both
models are compared with the full elliptic restricted three-body
problem. The study shows the differences between the values of the
eccentricity and inclination of the satellite predicted by those
models, showing the differences at every instant of time, as well
as the integral over the time of the differences between the
models. This integral is a new way to look at those differences
and can give us a more complete view of the quality of the
approximations, instead of just instantaneous views.",
doi = "10.1088/1742-6596/465/1/012017",
url = "http://dx.doi.org/10.1088/1742-6596/465/1/012017",
issn = "1742-6588",
label = "lattes: 7340081273816424 2 DomingosAlmeMora:2013:StBeAv",
language = "pt",
urlaccessdate = "20 maio 2024"
}