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1. Identity statement
Reference TypeBook Section
Sitemarte3.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3r59YCT/H3K3V
Repositorysid.inpe.br/iris@1905/2005/08.04.02.10   (restricted access)
Last Update2019:01.18.16.43.40 (UTC) simone
Metadata Repositorysid.inpe.br/iris@1905/2005/08.04.02.10.27
Metadata Last Update2021:02.11.18.10.11 (UTC) administrator
Secondary KeyINPE-9541-PRE/5194
Label10469
Citation KeyDomingosWint:2002:CrEaOf
TitleThe cross-section of the Earth and of the Moon
FormatISBN 85-17-00005-6
Year2002
Secondary Date20021213
Access Date2024, May 05
Secondary TypePRE LN
Number of Files1
Size1932 KiB
2. Context
Author1 Domingos, Rita de Cássia
2 Winter, Othon
Group1 DMC-INPE-MCT-BR
EditorWinter, Othon Cabo
Prado, Antonio Fernando Bertachini de Almeida.
Book TitleAdvances in space dynamics 2: applications in astronomy
PublisherINPE
CitySão José dos Campos
Pages25-31
Series TitleAdvances in space dynamics 2: applications in astronomy
History (UTC)2008-06-09 21:41:16 :: administrator -> jefferson ::
2012-08-02 17:55:11 :: jefferson -> administrator ::
2019-01-18 16:42:04 :: administrator -> simone :: 2002
2019-01-18 16:43:41 :: simone -> administrator :: 2002
2021-02-11 18:10:11 :: administrator -> :: 2002
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
KeywordsENGENHARIA E TECNOLOGIA ESPACIAL
cross-section
three-body problem
AbstractThe extension of the gravity fields of the Earth and of the Moon affect the impact probabilities of celestial bodies with them. The gravitational attraction can imply on a cross-section larger than the a of the maximum geometrical circle formed by the earth (or Moon). However, this effect depends on the velocity of the body relative to the Earth (or Moon). Following the work of Tatum (1997)we present an analytical model based on the definition of gravity assisted trajectories. The results of this analytical study were compared to fall numerical integration of the planar circular restricted three-body problem. The cross- section from the analytical model are in good agreement with the numerical results,, but always overestimating its radius. From the numerical results we found that for low relative velocities , V, the effective cross-section radius is a few times the geometric cross-section radius. For V=3 km/s the effective radius of Earth's cross-section increases by a factor of 4. In the case of the Moon, for V=1 km/s, the factor is about 2.5.
AreaETES
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDMC > The cross-section of...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Target FileINPE-9541.pdf
User Groupadministrator
Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/446AF4B
Host Collectionsid.inpe.br/banon/2001/04.03.15.36
6. Notes
Empty Fieldsaffiliation archivingpolicy archivist callnumber contenttype copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition electronicmailaddress isbn issn language lineage mark mirrorrepository nextedition notes numberofvolumes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarymark serieseditor session shorttitle sponsor subject tertiarymark tertiarytype translator url versiontype volume


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