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@Article{MerguizoSanchezPrad:2018:UsMeMo,
               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 = "On the use of mean motion resonances to explore the Haumea 
                         system",
              journal = "Advances in the Astronautical Sciences",
                 year = "2018",
               volume = "162",
                pages = "1507--1524",
                 note = "AAS/AIAA Astrodynamics Specialist Conference, 2017; Stevenson; 
                         United States; 20 August 2017 through 24 August 2017",
             abstract = "In this work, Mean Motion Resonances (MMR) are used to create 
                         highly eccentric co-orbital orbits with Namaka, the inner moon of 
                         the dwarf planet Haumea. We found a region of instability nearby 
                         Namaka, caused by the quasi-super position of the critical 
                         semi-major axis of Haumea-Namaka (23,576.573 km) and Haumea-Hiiaka 
                         (22,422.929 km). These orbits need to be retrograde, since 
                         prograde orbits cross the region of instability due to the 
                         variation of their semi-major axis. We used the method of the 
                         integral of the disturbing acceleration to analyze the region of 
                         instability.",
                 issn = "0065-3438.",
             language = "en",
           targetfile = "StevensonFinal2.pdf",
        urlaccessdate = "25 nov. 2020"
}


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