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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentifierJ8LNKAN8RW/3C63L2E
Repositorydpi.inpe.br/plutao/2012/06.21.18.29
Last Update2012:08.21.14.57.37 (UTC) secretaria.cpa@dir.inpe.br
Metadata Repositorydpi.inpe.br/plutao/2012/06.21.18.29.11
Metadata Last Update2021:02.11.18.16.03 (UTC) administrator
ISBN9781618040
Labellattes: 6880903376164690 1 GomesPrad:2012:ClApCl
Citation KeyGomesPrad:2012:ClApCl
TitleClose approaches for a cloud of particles with the moon
FormatPapel
Year2012
Access Date2024, Apr. 19
Secondary TypePRE CI
Number of Files1
Size2086 KiB
2. Context
Author1 Gomes, Vivian Martins
2 Prado, Antonio Fernando Bertachini de Almeida
Group1
2 DMC-ETE-INPE-MCTI-GOV-BR
Affiliation1
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 vivian.gomes@uol.com.br
2 abertachini@terra.com.br
e-Mail Addressvivian.gomes@uol.com.br
Conference NameWorld Congress on Applied Computing Conference, 5.
Conference LocationFaro
Date2012
Pages84-89
Book TitleProceedings
Tertiary TypePaper
History (UTC)2012-06-22 00:10:59 :: lattes -> secretaria.cpa@dir.inpe.br :: 2012
2012-08-21 14:58:46 :: secretaria.cpa@dir.inpe.br -> administrator :: 2012
2021-02-11 18:16:03 :: administrator -> marciana :: 2012
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsAstrodynamics
Orbital maneuvers
Swing-By
Gravity assisted maneuvers
Orbital motion
AbstractThe goal of this research is to study close approaches between the Moon and a cloud of particles. The system is formed by two main bodies (the Earth and the Moon) and it is assumed that they are in circular orbits. The cloud of particles is moving under their gravitational attraction. The motion is assumed to be planar for all the particles and the dynamics given by the patched-conic approximation is used, which means that a series of two-body problems are used to generate analytical equations that describe the problem. The main obejctive is to understand the change of the orbit of this cloud of particles after the close approach with the Moon. It is assumed that all the particles that belong to the cloud have semi-major axis a ± da and eccentricity e ± de before the close approach with the Moon, such that the particles are inside a circle (in the semi-major axis-eccentricity plane) with center in the center of mass of the cloud. It is desired to known those values after the close approach.
AreaETES
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDMC > Close approaches for...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
data URLhttp://urlib.net/ibi/J8LNKAN8RW/3C63L2E
zipped data URLhttp://urlib.net/zip/J8LNKAN8RW/3C63L2E
Languageen
Target FileBICA-13.pdf
User Grouplattes
secretaria.cpa@dir.inpe.br
Visibilityshown
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/446AF4B
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
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7. Description control
e-Mail (login)marciana
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