Publicação:
A numerical study of powered Swing-Bys around the Moon

dc.contributor.authorFerreira, Alessandra Ferraz da Silva
dc.contributor.authorPrado, Antonio Fernando Bertachini de Almeida
dc.contributor.authorWinter, Othon Cabo [UNESP]
dc.contributor.institutionInstituto Nacional de Pesquisas Espaciais (INPE)
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2015-10-21T21:13:17Z
dc.date.available2015-10-21T21:13:17Z
dc.date.issued2015-07-15
dc.description.abstractThe present research studies Swing-By maneuvers combined with the application of an impulse at the spacecraft periapsis passage. The studies were made for different values of r(p) (periapsis distance), delta V (magnitude of the impulse), Psi (angle of approach) and alpha (angle that defines the direction of the impulse). The results show the best direction to apply the impulse for each specific geometry of the passage, maximizing the gains or energy losses. The results show, as an example, that an angle alpha near 20 degrees gives the best solution to maximize the energy gains for the situation where the periapsis distance is 1.1 Moon's radius and Psi = 90 degrees. This value goes to near -20 degrees when Psi = 270 degrees. In the case of maximizing the energy losses, two families with impulses against the direction of the spacecraft motion are found to be the best solutions. Conditions where the impulse generates a capture around the Moon or a collision are also mapped. For values larger than 1.1 Moon's radius for the periapsis distance, the angle that maximizes the energy variation increases. Empirical analytical equations are obtained that express the energy variation as a function of the angle of approach, which replaces well-known equations obtained from the two-body approximation.en
dc.description.affiliationUnespUniversidade Estadual Paulista, Departamento de Matemática, Faculdade de Engenharia de Guaratinguetá
dc.description.sponsorshipConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.description.sponsorshipCoordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)
dc.description.sponsorshipIdCNPq: 473387/2012-3
dc.description.sponsorshipIdCNPq: 304700/2009-6
dc.description.sponsorshipIdCNPq: 312813/2013-9
dc.description.sponsorshipIdFAPESP: 2011/13101-4
dc.description.sponsorshipIdFAPESP: 2011/08171-3
dc.description.sponsorshipIdFAPESP: 2012/21023-6
dc.description.sponsorshipIdFAPESP: 2014/06688-7
dc.format.extent252-272
dc.identifierhttp://www.sciencedirect.com/science/article/pii/S0273117715002756
dc.identifier.citationAdvances In Space Research. Oxford: Elsevier Sci Ltd, v. 56, n. 2, p. 252-272, 2015.
dc.identifier.doi10.1016/j.asr.2015.04.016
dc.identifier.issn0273-1177
dc.identifier.lattes0960024575647258
dc.identifier.orcid0000-0002-4901-3289
dc.identifier.urihttp://hdl.handle.net/11449/129496
dc.identifier.wosWOS:000357244200005
dc.language.isoeng
dc.publisherElsevier B.V.
dc.relation.ispartofAdvances In Space Research
dc.relation.ispartofjcr1.529
dc.relation.ispartofsjr0,569
dc.rights.accessRightsAcesso restrito
dc.sourceWeb of Science
dc.subjectPowered Swing-Byen
dc.subjectAstrodynamicsen
dc.subjectOrbital maneuversen
dc.subjectClose-approach maneuversen
dc.titleA numerical study of powered Swing-Bys around the Moonen
dc.typeArtigo
dcterms.licensehttp://www.elsevier.com/about/open-access/open-access-policies/article-posting-policy
dcterms.rightsHolderElsevier B.V.
dspace.entity.typePublication
unesp.author.lattes0960024575647258[3]
unesp.author.orcid0000-0002-7966-3231[2]
unesp.author.orcid0000-0002-4901-3289[3]
unesp.campusUniversidade Estadual Paulista (UNESP), Faculdade de Engenharia, Guaratinguetápt
unesp.departmentMatemática - FEGpt

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