Location and stability of distant retrograde orbits around the Moon

Registro completo de metadados
MetadadosDescriçãoIdioma
Autor(es): dc.contributorUniversidade do Estado do Rio de Janeiro (UERJ)-
Autor(es): dc.contributorUniversidade Estadual Paulista (Unesp)-
Autor(es): dc.creatorPires, P.-
Autor(es): dc.creatorWinter, O. C. [UNESP]-
Data de aceite: dc.date.accessioned2022-02-22T00:20:46Z-
Data de disponibilização: dc.date.available2022-02-22T00:20:46Z-
Data de envio: dc.date.issued2020-12-10-
Data de envio: dc.date.issued2020-12-10-
Data de envio: dc.date.issued2020-05-01-
Fonte completa do material: dc.identifierhttp://dx.doi.org/10.1093/mnras/staa887-
Fonte completa do material: dc.identifierhttp://hdl.handle.net/11449/197795-
Fonte: dc.identifier.urihttp://educapes.capes.gov.br/handle/11449/197795-
Descrição: dc.descriptionRecently has grown the interest of placing natural or artificial objects in the neighbourhood of the Moon. We numerically investigate a region of retrograde orbits around the Moon associated with the C Family of periodic orbits and the quasi-periodic orbits that oscillate around them (Broucke 1968; Winter 2000). We have given continuity to Winter (2000) investigations by introducing a more realistic dynamical scenario, one based on the four-body Sun-Earth-Moon-particle problem. Our results showed that the region of stability diminished to approximately 4 per cent, the original size encountered for the circular-restricted three-body problem (CRTBP), mainly due to the Sun's gravitational perturbations. None the less, the size of the region continues to be significant and we were able to found distant retrograde orbits (DROs) around the Moon with eccentricity following e = 2.259 63 x 10(-6) a + 0.238 45 (standard error of 1 per cent) and semimajor axis values of the initial osculating orbits, varying between 110 000 and 185 000 km, remaining stable for a time span of 10(4) lunar periods. This set of distant orbits from the Moon are characterized by a narrow range of acceptable initial positions (0.8-0.83) and velocities of similar to 0.5, in the rotating Earth-Moon frame. The out of plane amplitude oscillations of +/- 15 000 km presented by these DROs are a natural outcome of the significant Moon's inclination of 5.15 degrees. Some results presented on this work can be useful for lunar missions, such as the ones that would require prolonged stays around the satellite and use stable distant orbits as 'parking' orbits, such as the advanced concepts of NASA's Asteroid Redirect Mission, proposed a few years ago.-
Descrição: dc.descriptionCoordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)-
Descrição: dc.descriptionFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)-
Descrição: dc.descriptionConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)-
Descrição: dc.descriptionUniv Estado Rio De Janeiro, UERJ, BR-27537000 Resende, RJ, Brazil-
Descrição: dc.descriptionSao Paulo State Univ, UNESP, Grp Dinam Orbital & Planetol, BR-12516410 Guaratingueta, SP, Brazil-
Descrição: dc.descriptionSao Paulo State Univ, UNESP, Grp Dinam Orbital & Planetol, BR-12516410 Guaratingueta, SP, Brazil-
Descrição: dc.descriptionCAPES: 001-
Descrição: dc.descriptionFAPESP: 2016/24561-0-
Descrição: dc.descriptionCNPq: 305210/2018-1-
Formato: dc.format2727-2735-
Idioma: dc.languageen-
Publicador: dc.publisherOxford Univ Press-
Relação: dc.relationMonthly Notices Of The Royal Astronomical Society-
???dc.source???: dc.sourceWeb of Science-
Palavras-chave: dc.subjectmethods: numerical-
Palavras-chave: dc.subjectEarth-
Palavras-chave: dc.subjectMoon-
Título: dc.titleLocation and stability of distant retrograde orbits around the Moon-
Tipo de arquivo: dc.typelivro digital-
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