%0 Journal Article
%4 sid.inpe.br/plutao/2013/12.12.15.39.32
%2 sid.inpe.br/plutao/2013/12.12.15.39.33
%@doi 10.1088/1742-6596/465/1/012017
%@issn 1742-6588
%F lattes: 7340081273816424 2 DomingosAlmeMora:2013:StBeAv
%T Studying the behaviour of averaged models in the third body perturbation problem
%D 2013
%A Domingos, R C,
%A Prado, Antonio Fernando Bertachini de Almeida,
%A Moraes, R Vilhena de,
%@affiliation Universidade Faderal de São Paulo (UNIFESP)
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@affiliation Universidade Federal de São Paulo (UNIFESP), São José dos Campos, SP, Brazil
%@electronicmailaddress
%@electronicmailaddress antonio.prado@inpe.br
%B Journal of Physics: Conference Series
%V 465
%N 1
%P Article number 012017
%K Astrodinâmica, Mecânica Celeste, Perturbação de Terceiro Corpo.
%X 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.
%@language pt
%O 16th Brazilian Colloquium on Orbital Dynamics; Serra Negra, Sao Paulo; Brazil; 26 November 2012 through 30 November 2012