@Article{MerguizoSanchezPrad:2020:StHiIn,
               author = "Merguizo Sanchez, Diogo and Prado, Antonio Fernando Bertachini de 
                         Almeida",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)}",
                title = "Stability of highly inclined orbits around the asteroid (153591) 
                         2001 sn263",
              journal = "Advances in the Astronautical Sciences",
                 year = "2020",
               volume = "171",
                pages = "1075--1093",
             abstract = "In this work perturbation maps are used to measure the stability 
                         of highly inclined orbits around the triple asteroid 2001 SN263, 
                         target of the Brazilian ASTER mission. The perturbation maps also 
                         provide the delta-v required to keep a spacecraft as close as 
                         possible to a reference orbit through orbital maneuvers. In our 
                         case the reference orbit is a Keplerian orbit. However, the 
                         reference orbit can be any, depending on the objectives of the 
                         mission. We compare the orbital stability of the spacecraft with 
                         three values area-to-mass ratio, to show the effect of the solar 
                         radiation pressure on the dynamical structure of the system. The 
                         results of this work can be used for the planning of the ASTER 
                         mission and for the planning of any space mission.",
                 issn = "0065-3438.",
             language = "en",
        urlaccessdate = "19 abr. 2024"
}