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1. Identity statement
Reference TypeJournal Article
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentifierJ8LNKAN8RW/34BER8B
Repositorydpi.inpe.br/plutao@80/2008/12.04.12.20.06   (restricted access)
Last Update2013:02.06.15.59.17 (UTC) marciana
Metadata Repositorydpi.inpe.br/plutao@80/2008/12.04.12.20.07
Metadata Last Update2021:02.11.18.11.17 (UTC) administrator
DOI10.1016/j.actaastro.2008.05.005
ISSN0094-5765
Labellattes: 7340081273816424 2 CabettePrad:2008:TrOrTo
Citation KeySantosCabettePrad:2008:TrOrTo
TitleTransfer orbits to/from the Lagrangian points in the restricted four-body problem
Year2008
Access Date2024, May 06
Secondary TypePRE PI
Number of Files1
Size489 KiB
2. Context
Author1 Santos Cabette, Regina Elaine
2 Prado, Antonio Fernando Bertachini de Almeida
Group1
2 DMC-ETE-INPE-MCT-BR
Affiliation1
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2 abertachini@terra.com.br
e-Mail Addressabertachini@terra.com.br
JournalActa Astronautica
Volume63
Number11-12
Pages1221-1232
Secondary MarkB_ENGENHARIAS_I B_ENGENHARIAS_II B_ENGENHARIAS_III B_ENGENHARIAS_IV C_GEOCIÊNCIAS C_INTERDISCIPLINAR
History (UTC)2008-12-04 16:12:41 :: lattes -> simone ::
2010-07-07 18:38:51 :: simone -> marciana ::
2013-02-06 15:59:18 :: marciana -> administrator :: 2008
2021-02-11 18:11:17 :: administrator -> marciana :: 2008
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsAstrodinamica
Abstracthe well-known Lagrangian points that appear in the planar restricted three-body problem are very important for astronautical applications. They are five points of equilibrium in the equations of motion, what means that a particle located at one of those points with zero velocity will remain there indefinitely. The collinear points (L-1, L-2 and L-3) are always unstable and the triangular points (L-4 and L-5) are stable in the present case studied (Earth-Sun system). They are all very good points to locate a space-station, since they require a small amount of AV (and fuel), the control to be used, for station-keeping. The triangular points are especially good for this purpose, since they are stable equilibrium points. In this paper, the planar restricted four-body problem applied to the Sun-Earth-Moon-Spacecraft is combined with numerical integration and gradient methods to solve the two-point boundary value problem. This combination is applied to the search of families of transfer orbits between the Lagrangian points and the Earth, in the Earth-Sun system, with the minimum possible cost of the control used. So, the final goal of this paper is to find the magnitude of the two impulses to be applied in the spacecraft to complete the transfer: the first one when leaving/arriving at the Lagrangian point and the second one when arriving/living at the Earth. The dynamics given by the restricted four-body problem is used to obtain the trajectory of the spacecraft, but not the position of the equilibrium points. Their position is taken from the restricted three-body model. The goal to use this model is to evaluate the perturbation of the Sun in those important trajectories, in terms of fuel consumption and time of flight. The solutions will also show how to apply the impulses to accomplish the transfers under this force model. The results showed a large collection of transfers, and that there are initial conditions (position of the Sun with respect to the other bodies) where the force of the Sun can be used to reduce the cost of the transfers.
AreaETES
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDMC > Transfer orbits to/from...
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4. Conditions of access and use
Languageen
User Grouplattes
marciana
Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/446AF4B
DisseminationWEBSCI; PORTALCAPES; COMPENDEX.
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
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