%0 Journal Article
%@resumeid
%@resumeid 8JMKD3MGP5W/3C9JGJA
%X 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.
%9 conference paper
%T On the use of mean motion resonances to explore the Haumea system
%@electronicmailaddress diogo.sanchez@inpe.br
%@electronicmailaddress antonio.prado@inpe.br
%@nexthigherunit 8JMKD3MGPCW/3F2UALS
%@nexthigherunit 8JMKD3MGPCW/446AF4B
%@secondarytype PRE PI
%@usergroup self-uploading-INPE-MCTI-GOV-BR
%@usergroup simone
%@group CMC-ETES-SESPG-INPE-MCTIC-GOV-BR
%@group DIDMC-CGETE-INPE-MCTIC-GOV-BR
%@tertiarymark 8JMKD3MGP3W34P/3HQHJ72
%@issn 0065-3438.
%2 sid.inpe.br/mtc-m21c/2018/08.06.15.18.29
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%B Advances in the Astronautical Sciences
%@versiontype publisher
%P 1507-1524
%4 sid.inpe.br/mtc-m21c/2018/08.06.15.18
%@documentstage not transferred
%D 2018
%V 162
%O AAS/AIAA Astrodynamics Specialist Conference, 2017; Stevenson; United States; 20 August 2017 through 24 August 2017
%A Merguizo Sanchez, Diogo,
%A Prado, Antonio Fernando Bertachini de Almeida,
%@dissemination WEBSCI; PORTALCAPES; MGA; COMPENDEX.
%@area ETES
%@holdercode {isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S}
%3 StevensonFinal2.pdf