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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Siteplutao.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W/474NTRP
Repositóriosid.inpe.br/plutao/2022/06.15.12.28.42   (acesso restrito)
Última Atualização2022:06.20.13.55.18 (UTC) administrator
Repositório de Metadadossid.inpe.br/plutao/2022/06.15.12.28.43
Última Atualização dos Metadados2022:07.17.01.14.41 (UTC) administrator
DOI10.1016/j.asr.2022.04.014
ISSN0273-1177
Rótulolattes: 7340081273816424 3 CarvalhoVilhPrad:2022:AnOrEv
Chave de CitaçãoCarvalhoVilhPrad:2022:AnOrEv
TítuloAnalysis of the orbital evolution of space debris using a solar sail and natural forces
Ano2022
Data de Acesso11 maio 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho2339 KiB
2. Contextualização
Autor1 Carvalho, Jean Paulo dos Santos
2 Vilhena de Moraes, Rodolpho
3 Prado, Antonio Fernando Bertachini de Almeida
Identificador de Curriculo1
2
3 8JMKD3MGP5W/3C9JGJA
Grupo1
2
3 DIMEC-CGCE-INPE-MCTI-GOV-BR
Afiliação1 Universidade Federal do Recôncavo da Bahia (URFB)
2 Universidade Federal de São Paulo (UNIFESP)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 jean.carvalho@ufrb.edu.br
2 rodolpho.vilhena@gmail.com
3 antonio.prado@inpe.br
RevistaAdvances In Space Research
Volume70
Páginas125-143
Nota SecundáriaB1_INTERDISCIPLINAR B1_GEOCIÊNCIAS B1_ENGENHARIAS_IV B1_ENGENHARIAS_III B1_BIODIVERSIDADE B3_CIÊNCIA_DA_COMPUTAÇÃO B4_ASTRONOMIA_/_FÍSICA C_CIÊNCIAS_BIOLÓGICAS_I
Histórico (UTC)2022-06-15 12:28:43 :: lattes -> administrator ::
2022-06-20 13:53:36 :: administrator -> lattes :: 2022
2022-06-20 13:55:20 :: lattes -> administrator :: 2022
2022-07-17 01:14:41 :: administrator -> simone :: 2022
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
Palavras-ChaveAstrodinâmica
Astrodynamics
Space Debris
Space debris
Solar radiation pressure
Solar sail
Sustainability
Astrodynamics
ResumoSince the launch of the first artificial satellite around the Earth up to the present date, various non-functional objects are orbiting the Earth, such as deactivated satellites, satellite components, rocket bodies, among others. These objects can collide with operational satel- lites or other debris, generating a cloud of smaller particles. Space agencies are concerned about the current scenario of the space envi- ronment. If we continue as we are the number of objects in orbit will make it difficult to operate safely in the space environment. So space exploration may become unsustainable (ESA (2020)). In this work, the orbital evolution of these objects that are located in the geosta- tionary orbit (GEO) is analyzed. In the mathematical model we consider the main disturbing forces, such as the direct solar radiation pressure (SRP), the perturbation of the third body (Sun and Moon) and the Earth oblateness. The SRP is the most relevant perturbation for objects with larger area-mass ratio. Knowing this, the possibility of using a solar sail is considered to help to clean the space envi- ronment. The main natural environmental perturbations that act in the orbit of the debris are considered in the dynamics. Such forces acting in the solar sail can force the growth of the eccentricity of these objects in the GEO orbit. Several authors have presented models of the solar radiation pressure considering the single-averaged model. But, doing a literature research, we found that the authors consider the Earth around the Sun in a circular and inclined orbit. Our contribution to the SRP model is in developing a different approach from other authors, where we consider the Sun in an elliptical and inclined orbit, which is valid for other bodies in the solar system when the eccentricity cannot be neglected. The expression of the SRP is developed up to the second order. We found that the first-order term is much superior to the second-order term, so the quadrupole term can be neglected. Another contribution is the approach to identify the initial conditions of the perigee argument (g) and the longitude of the ascending node (h), where some values of the (g; h) plane contribute to amplify the eccentricity growth. In the numerical simulations we consider real data from space debris removed from the site Stuff in Space. The solar sail helps to clean up the space environment using a propulsion system that uses the Sun itself, a clean and abundant energy source, unlike chemical propellants, to contribute to the sustainability of space exploration. Ó 2022 Published by Elsevier B.V. on behalf of COSPAR.
ÁreaETES
Arranjourlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Analysis of the...
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreementnão têm arquivos
4. Condições de acesso e uso
Idiomaen
Grupo de Usuárioslattes
self-uploading-INPE-MCTI-GOV-BR
Visibilidadeshown
Política de Arquivamentodenypublisher denyfinaldraft24
Permissão de Leituradeny from all and allow from 150.163
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
VinculaçãoTrabalho não Vinculado à Tese/Dissertação
Unidades Imediatamente Superiores8JMKD3MGPCW/46KTFK8
DivulgaçãoWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Acervo Hospedeirodpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn lineage mark mirrorrepository month nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject targetfile tertiarytype url
7. Controle da descrição
e-Mail (login)simone
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