@Article{SantosCarvPradMora:2017:LiMaOr,
               author = "Santos, Josu{\'e} Cardoso dos and Carvalho, Jean P. S. and Prado, 
                         Antonio Fernando Bertachini de Almeida and Moraes, Rodolpho 
                         Vilhena de",
          affiliation = "{Universidade Estadual Paulista (UNESP)} and {Universidade Federal 
                         do Rec{\^o}ncavo da Bahia (UFRB)} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and {Universidade Federal de S{\~a}o 
                         Paulo (UNIFESP)}",
                title = "Lifetime maps for orbits around Callisto using a double-averaged 
                         model",
              journal = "Astrophysics and Space Science",
                 year = "2017",
               volume = "362",
               number = "12",
                pages = "227",
             keywords = "Lifetime of orbits · Double-average · Third-body perturbation · 
                         Orbital perturbations · Moons, perturbation maps.",
             abstract = "The present paper studies the lifetime of orbits around a moon 
                         that is in orbit around its mother planet. In the context of the 
                         inner restricted three-body problem, the dynamical model 
                         considered in the present study uses the double-averaged dynamics 
                         of a spacecraft moving around a moon under the gravitational 
                         pulling of a disturbing third body in an elliptical orbit. The 
                         non-uniform distribution of the mass of the moon is also 
                         considered. Applications are performed using numerical experiments 
                         for the Callisto spacecraftJupiter system, and lifetime maps for 
                         different values of the eccentricity of the disturbing body 
                         (Jupiter) are presented, in order to investigate the role of this 
                         parameter in these maps. The idea is to simulate a system with the 
                         same physical parameters as the JupiterCallisto system, but with 
                         larger eccentricities. These maps are also useful for validation 
                         and improvements in the results available in the literature, such 
                         as to find conditions to extend the available time for a massless 
                         orbiting body to be in highly inclined orbits under gravitational 
                         disturbances coming from the other bodies of the system.",
                  doi = "10.1007/s10509-017-3200-2",
                  url = "http://dx.doi.org/10.1007/s10509-017-3200-2",
                 issn = "0004-640X",
                label = "lattes: 7340081273816424 3 
                         CardosodosSantosCarvPradVilh:2017:LiMaOr",
             language = "en",
           targetfile = "santos_lifetime.pdf",
        urlaccessdate = "03 maio 2024"
}