A NUMERICAL-ANALYTICAL APPROACH BASED ON CANONICAL TRANSFORMATIONS FOR COMPUTING OPTIMAL LOW-THRUST TRANSFERS
Autor(a) principal: | |
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Data de Publicação: | 2018 |
Outros Autores: | , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNIFESP |
Texto Completo: | https://repositorio.unifesp.br/handle/11600/55719 http://www.astroscu.unam.mx/rmaa/RMxAA..54-1/PDF/RMxAA..54-1_sdasilva-VIII.pdf |
Resumo: | A numerical-analytical procedure based on infinitesimal canonical transformations is developed for computing optimal time-fixed low-thrust limited power transfers (no rendezvous) between coplanar orbits with small eccentricities in an inverse-square force field. The optimization problem is formulated as a Mayer problem with a set of non-singular orbital elements as state variables. Second order terms in eccentricity are considered in the development of the maximum Hamiltonian describing the optimal trajectories. The two-point boundary value problem of going from an initial orbit to a final orbit is solved by means of a two-stage Newton-Raphson algorithm which uses an infinitesimal canonical transformation. Numerical results are presented for some transfers between circular orbits with moderate radius ratio, including a preliminary analysis of Earth-Mars and Earth-Venus missions. |
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Fernandes, Sandro da SilvaCarvalho, Francisco das ChagasRomão, João Victor Bateli [UNIFESP]2020-07-20T16:31:07Z2020-07-20T16:31:07Z2018Revista Mexicana De Astronomia Y Astrofisica. Mexico City, v. 54, n. 1, p. 111-128, 2018.0185-1101https://repositorio.unifesp.br/handle/11600/55719http://www.astroscu.unam.mx/rmaa/RMxAA..54-1/PDF/RMxAA..54-1_sdasilva-VIII.pdfWOS:000429617900008A numerical-analytical procedure based on infinitesimal canonical transformations is developed for computing optimal time-fixed low-thrust limited power transfers (no rendezvous) between coplanar orbits with small eccentricities in an inverse-square force field. The optimization problem is formulated as a Mayer problem with a set of non-singular orbital elements as state variables. Second order terms in eccentricity are considered in the development of the maximum Hamiltonian describing the optimal trajectories. The two-point boundary value problem of going from an initial orbit to a final orbit is solved by means of a two-stage Newton-Raphson algorithm which uses an infinitesimal canonical transformation. Numerical results are presented for some transfers between circular orbits with moderate radius ratio, including a preliminary analysis of Earth-Mars and Earth-Venus missions.CNPqFAPESPInst Tecnol Aeronaut, Dept Matemat, Sao Jose Dos Campos, BrazilUniv Fed Sao Paulo, Inst Ciencia & Tecnol, Sao Paulo, BrazilUniv Fed Sao Paulo, Inst Ciencia & Tecnol, Sao Paulo, BrazilCNPq: 304913/2013-8FAPESP: 2012/21023-6Web of Science111-128engUniv Nacional Autonoma Mexico, Inst De AstronomiaRevista Mexicana De Astronomia Y Astrofisicacelestial mechanicsmethods: analyticalmethods: numericalA NUMERICAL-ANALYTICAL APPROACH BASED ON CANONICAL TRANSFORMATIONS FOR COMPUTING OPTIMAL LOW-THRUST TRANSFERSinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleMexico Cityv. 541info:eu-repo/semantics/openAccessreponame:Repositório Institucional da UNIFESPinstname:Universidade Federal de São Paulo (UNIFESP)instacron:UNIFESP11600/557192021-09-29 09:32:52.437metadata only accessoai:repositorio.unifesp.br:11600/55719Repositório InstitucionalPUBhttp://www.repositorio.unifesp.br/oai/requestopendoar:34652021-09-29T12:32:52Repositório Institucional da UNIFESP - Universidade Federal de São Paulo (UNIFESP)false |
dc.title.en.fl_str_mv |
A NUMERICAL-ANALYTICAL APPROACH BASED ON CANONICAL TRANSFORMATIONS FOR COMPUTING OPTIMAL LOW-THRUST TRANSFERS |
title |
A NUMERICAL-ANALYTICAL APPROACH BASED ON CANONICAL TRANSFORMATIONS FOR COMPUTING OPTIMAL LOW-THRUST TRANSFERS |
spellingShingle |
A NUMERICAL-ANALYTICAL APPROACH BASED ON CANONICAL TRANSFORMATIONS FOR COMPUTING OPTIMAL LOW-THRUST TRANSFERS Fernandes, Sandro da Silva celestial mechanics methods: analytical methods: numerical |
title_short |
A NUMERICAL-ANALYTICAL APPROACH BASED ON CANONICAL TRANSFORMATIONS FOR COMPUTING OPTIMAL LOW-THRUST TRANSFERS |
title_full |
A NUMERICAL-ANALYTICAL APPROACH BASED ON CANONICAL TRANSFORMATIONS FOR COMPUTING OPTIMAL LOW-THRUST TRANSFERS |
title_fullStr |
A NUMERICAL-ANALYTICAL APPROACH BASED ON CANONICAL TRANSFORMATIONS FOR COMPUTING OPTIMAL LOW-THRUST TRANSFERS |
title_full_unstemmed |
A NUMERICAL-ANALYTICAL APPROACH BASED ON CANONICAL TRANSFORMATIONS FOR COMPUTING OPTIMAL LOW-THRUST TRANSFERS |
title_sort |
A NUMERICAL-ANALYTICAL APPROACH BASED ON CANONICAL TRANSFORMATIONS FOR COMPUTING OPTIMAL LOW-THRUST TRANSFERS |
author |
Fernandes, Sandro da Silva |
author_facet |
Fernandes, Sandro da Silva Carvalho, Francisco das Chagas Romão, João Victor Bateli [UNIFESP] |
author_role |
author |
author2 |
Carvalho, Francisco das Chagas Romão, João Victor Bateli [UNIFESP] |
author2_role |
author author |
dc.contributor.author.fl_str_mv |
Fernandes, Sandro da Silva Carvalho, Francisco das Chagas Romão, João Victor Bateli [UNIFESP] |
dc.subject.eng.fl_str_mv |
celestial mechanics methods: analytical methods: numerical |
topic |
celestial mechanics methods: analytical methods: numerical |
description |
A numerical-analytical procedure based on infinitesimal canonical transformations is developed for computing optimal time-fixed low-thrust limited power transfers (no rendezvous) between coplanar orbits with small eccentricities in an inverse-square force field. The optimization problem is formulated as a Mayer problem with a set of non-singular orbital elements as state variables. Second order terms in eccentricity are considered in the development of the maximum Hamiltonian describing the optimal trajectories. The two-point boundary value problem of going from an initial orbit to a final orbit is solved by means of a two-stage Newton-Raphson algorithm which uses an infinitesimal canonical transformation. Numerical results are presented for some transfers between circular orbits with moderate radius ratio, including a preliminary analysis of Earth-Mars and Earth-Venus missions. |
publishDate |
2018 |
dc.date.issued.fl_str_mv |
2018 |
dc.date.accessioned.fl_str_mv |
2020-07-20T16:31:07Z |
dc.date.available.fl_str_mv |
2020-07-20T16:31:07Z |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.citation.fl_str_mv |
Revista Mexicana De Astronomia Y Astrofisica. Mexico City, v. 54, n. 1, p. 111-128, 2018. |
dc.identifier.uri.fl_str_mv |
https://repositorio.unifesp.br/handle/11600/55719 http://www.astroscu.unam.mx/rmaa/RMxAA..54-1/PDF/RMxAA..54-1_sdasilva-VIII.pdf |
dc.identifier.issn.none.fl_str_mv |
0185-1101 |
dc.identifier.wos.none.fl_str_mv |
WOS:000429617900008 |
identifier_str_mv |
Revista Mexicana De Astronomia Y Astrofisica. Mexico City, v. 54, n. 1, p. 111-128, 2018. 0185-1101 WOS:000429617900008 |
url |
https://repositorio.unifesp.br/handle/11600/55719 http://www.astroscu.unam.mx/rmaa/RMxAA..54-1/PDF/RMxAA..54-1_sdasilva-VIII.pdf |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.ispartof.none.fl_str_mv |
Revista Mexicana De Astronomia Y Astrofisica |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
111-128 |
dc.coverage.none.fl_str_mv |
Mexico City |
dc.publisher.none.fl_str_mv |
Univ Nacional Autonoma Mexico, Inst De Astronomia |
publisher.none.fl_str_mv |
Univ Nacional Autonoma Mexico, Inst De Astronomia |
dc.source.none.fl_str_mv |
reponame:Repositório Institucional da UNIFESP instname:Universidade Federal de São Paulo (UNIFESP) instacron:UNIFESP |
instname_str |
Universidade Federal de São Paulo (UNIFESP) |
instacron_str |
UNIFESP |
institution |
UNIFESP |
reponame_str |
Repositório Institucional da UNIFESP |
collection |
Repositório Institucional da UNIFESP |
repository.name.fl_str_mv |
Repositório Institucional da UNIFESP - Universidade Federal de São Paulo (UNIFESP) |
repository.mail.fl_str_mv |
|
_version_ |
1802764174842920960 |