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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZsFDuKxG/EphGu
Repositorysid.inpe.br/marciana/2004/12.08.10.42   (restricted access)
Last Update2004:12.10.02.00.00 (UTC) administrator
Metadata Repositorysid.inpe.br/marciana/2004/12.08.10.42.03
Metadata Last Update2021:02.11.18.10.20 (UTC) administrator
Secondary KeyINPE-11809-PRE/7163
ISSN0273-1177
Citation KeyCelestinoWintPrad:2004:ReVeAc
TitleDebris perturbed by radiation pressure: relative velocities across circular orbits
Year2004
Access Date2024, Apr. 28
Secondary TypePRE PI
Number of Files1
Size450 KiB
2. Context
Author1 Celestino, C. C.
2 Winter, O. C.
3 Prado, Antonio Fernando Bertachini de Almeida
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JGJA
Group1 DMC-INPE-MCT-BR
Affiliation1 Winter OC (reprint author), UNESP, Grupo Dinam Orbital & Planetol, CP 205, Guaratingueta, SP BR-12500000 Brazil
2 UNESP, Grupo Dinam Orbital & Planetol, Guaratingueta, SP BR-12500000 Brazil
3 INPE, Div Mecan Espacial & Controle, Sao Jose Dos Campos, SP BR-12227010 Brazil
JournalAdvances in Space Research
Volume34
Number5
Pages1177-1180
History (UTC)2004-12-10 16:24:38 :: sergio -> administrator ::
2006-09-28 22:28:19 :: administrator -> sergio ::
2008-01-07 12:53:39 :: sergio -> administrator ::
2021-02-11 18:10:20 :: administrator -> marciana :: 2004
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Keywordsspace debris
radiation pressure
geostationary orbit
AbstractIn the present work we consider a dynamical system of mum size particles around the Earth subject to the effects of radiation pressure. Our main goal is to study the evolution of its relative velocity with respect to the co-planar circular orbits that it crosses. The particles were initially in a circular geostationary orbit, and the particles size were in the range between 1 and 100 mum. The radiation pressure produces variations in its eccentricity, resulting in a change in its orbital velocity. The results indicated the maximum linear momentum and kinetic energy increases as the particle size increases. For a particle of 1 mum the kinetic energy is approximately 1.56 x 10(-7) J and the momentum is 6.27 x 10(-11) kg m/s and for 100 mum the energy is approximately 1.82 x 10(-4) J and the momentum is 2.14 x 10(-6) kg m/s. (C) 2004 COSPAR. Published by Elsevier Ltd. All rights reserved.
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Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDMC > Debris perturbed by...
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4. Conditions of access and use
Languageen
Target Filesdarticle.pdf
User Groupadministrator
sergio
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/446AF4B
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
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