1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m16.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 6qtX3pFwXQZsFDuKxG/EphGu |
Repository | sid.inpe.br/marciana/2004/12.08.10.42 (restricted access) |
Last Update | 2004:12.10.02.00.00 (UTC) administrator |
Metadata Repository | sid.inpe.br/marciana/2004/12.08.10.42.03 |
Metadata Last Update | 2021:02.11.18.10.20 (UTC) administrator |
Secondary Key | INPE-11809-PRE/7163 |
ISSN | 0273-1177 |
Citation Key | CelestinoWintPrad:2004:ReVeAc |
Title | Debris perturbed by radiation pressure: relative velocities across circular orbits |
Year | 2004 |
Access Date | 2024, May 13 |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 450 KiB |
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2. Context | |
Author | 1 Celestino, C. C. 2 Winter, O. C. 3 Prado, Antonio Fernando Bertachini de Almeida |
Resume Identifier | 1 2 3 8JMKD3MGP5W/3C9JGJA |
Group | 1 DMC-INPE-MCT-BR |
Affiliation | 1 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 |
Journal | Advances in Space Research |
Volume | 34 |
Number | 5 |
Pages | 1177-1180 |
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 |
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3. Content and structure | |
Is the master or a copy? | is the master |
Content Stage | completed |
Transferable | 1 |
Content Type | External Contribution |
Keywords | space debris radiation pressure geostationary orbit |
Abstract | In 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. |
Area | ETES |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDMC > Debris perturbed by... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | there are no files |
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4. Conditions of access and use | |
Language | en |
Target File | sdarticle.pdf |
User Group | administrator sergio |
Visibility | shown |
Copy Holder | SID/SCD |
Archiving Policy | denypublisher denyfinaldraft24 |
Read Permission | deny from all and allow from 150.163 |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/446AF4B |
Dissemination | WEBSCI; PORTALCAPES; MGA; COMPENDEX. |
Host Collection | sid.inpe.br/banon/2003/08.15.17.40 |
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6. Notes | |
Empty Fields | alternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype |
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7. Description control | |
e-Mail (login) | marciana |
update | |
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