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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3RJMHK5
Repositorysid.inpe.br/mtc-m21c/2018/08.06.15.23   (restricted access)
Last Update2019:01.10.16.19.34 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21c/2018/08.06.15.23.48
Metadata Last Update2021:02.11.18.10.43 (UTC) administrator
ISSN0065-3438.
Citation KeyMurciaPinerosPrad:2018:ImAeAs
TitleImpulsive aero-gravity assisted maneuvers in Venus and Mars to change the inclination of a spacecraft
Year2018
Access Date2024, May 08
Type of Workconference paper
Secondary TypePRE PI
Number of Files1
Size1947 KiB
2. Context
Author1 Murcia Pineros, Jhonathan Orlando
2 Prado, Antonio Fernando Bertachini de Almeida
Resume Identifier1
2 8JMKD3MGP5W/3C9JGJA
Group1 CMC-ETES-SESPG-INPE-MCTIC-GOV-BR
2 DIDMC-CGETE-INPE-MCTIC-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 jhonathan.pineros@inpe.br
2 antonio.prado@inpe.br
JournalAdvances in the Astronautical Sciences
Volume162
Pages3921-3936
History (UTC)2018-08-06 15:23:58 :: simone -> administrator :: 2018
2019-01-04 16:57:07 :: administrator -> simone :: 2018
2019-01-07 10:11:40 :: simone -> administrator :: 2018
2021-02-11 18:10:43 :: administrator -> simone :: 2018
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractThe impulsive or powered aero-gravity-assisted is an orbital maneuver that combines three basic components: A gravity-assisted with a passage by the atmosphere of the planet during the close approach and the application of an impulse during this passage. The mathematical model used to simulate the trajectories is the Restricted Three-Body Problem including aerodynamic forces. The present paper uses this type of maneuver considering atmospheric drag and lift forces. The lift is applied orthogonal to the initial orbital plane to generate an inclination change in the trajectory of the spacecraft, which are very expensive maneuvers. The lift to drag ratio selected goes up to 9.0, because there are vehicles, like waveriders, designed to have these values. When the spacecraft is located at the periapsis the impulse is applied to increase or decrease the variation of energy given by the aero-gravity-assisted maneuver. The planets Venus and Mars are selected to be the secondary bodies for the maneuver, due to their atmospheric density and strategic location to provide possible use for future missions in the solar system. Results of the numerical simulations show the maximum changes in the inclination obtained by the maneuvers as a function of approach angle and direction of the impulse, lift to drag ratio and ballistic coefficient. In the case of Mars, inclination change can be larger than 13°, and for Venus higher than 21°. The energy and inclination variations are shown for several selected orbits.
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4. Conditions of access and use
Languageen
Target FileAAS 17-752.pdf
User Groupself-uploading-INPE-MCTI-GOV-BR
simone
Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
LinkingTrabalho não Vinculado à Tese/Dissertação
Next Higher Units8JMKD3MGPCW/3F2UALS
8JMKD3MGPCW/446AF4B
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
NotesAAS/AIAA Astrodynamics Specialist Conference, 2017; Stevenson; United States; 20 August 2017 through 24 August 2017.
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