Study of collision probability considering a non-uniform cloud of space debris
Autor(a) principal: | |
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Data de Publicação: | 2019 |
Outros Autores: | , , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1007/s40314-019-0997-z http://hdl.handle.net/11449/198156 |
Resumo: | The present paper aims to study the cumulative collision probability of a target that crosses a cloud of particles that has the orbital parameters of each individual element modified by a close approach with the Earth. Clouds of this type are formed when natural or man-made bodies explode for some reason. After an explosion like that, the individual particles have different trajectories. The clouds are specified by a non-uniform distribution of semi-major axis and eccentricity of their particles which are assumed to pass close to the Earth, making a close approach that modifies the trajectory of every single particle that belongs to the cloud. This study makes simulations considering separately two different clouds based on the patched conics model to obtain the new trajectories of each particle and to analyze the density of the whole cloud. Then it is possible to map the new distribution of the orbital elements of the fragments that constituted the cloud, using the distribution as initial conditions. After calculating the spatial density for the whole cloud, it is possible to obtain the cumulative collision probability for one space vehicle that crosses the cloud. These pieces of information are important when planning satellite missions where a spacecraft passes close to a cloud of this type, because we can determine values to study the risks of collision and the possible maneuvers that need to be made to avoid them. |
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Repositório Institucional da UNESP |
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Study of collision probability considering a non-uniform cloud of space debrisClose approachOrbital maneuverSpace debrisSpace trajectoriesThe present paper aims to study the cumulative collision probability of a target that crosses a cloud of particles that has the orbital parameters of each individual element modified by a close approach with the Earth. Clouds of this type are formed when natural or man-made bodies explode for some reason. After an explosion like that, the individual particles have different trajectories. The clouds are specified by a non-uniform distribution of semi-major axis and eccentricity of their particles which are assumed to pass close to the Earth, making a close approach that modifies the trajectory of every single particle that belongs to the cloud. This study makes simulations considering separately two different clouds based on the patched conics model to obtain the new trajectories of each particle and to analyze the density of the whole cloud. Then it is possible to map the new distribution of the orbital elements of the fragments that constituted the cloud, using the distribution as initial conditions. After calculating the spatial density for the whole cloud, it is possible to obtain the cumulative collision probability for one space vehicle that crosses the cloud. These pieces of information are important when planning satellite missions where a spacecraft passes close to a cloud of this type, because we can determine values to study the risks of collision and the possible maneuvers that need to be made to avoid them.Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Institute of Science and Technology São Paulo State University (UNESP)São Paulo State University (UNESP)Federal University of So Paulo (UNIFESP)SNational Institute for Space Research(INPE)Institute of Science and Technology São Paulo State University (UNESP)São Paulo State University (UNESP)FAPESP: 2016/15675-1FAPESP: 2017/04643-4Universidade Estadual Paulista (Unesp)Universidade Federal de São Paulo (UNIFESP)National Institute for Space Research(INPE)Formiga, Jorge Kennety Silva [UNESP]Santos, Denilson Paulo Souza dos [UNESP]Fiore, Fabiana A. [UNESP]de Moraes, Rodolpho VilhenaPrado, Antonio Fernando Bertachini A.2020-12-12T01:00:43Z2020-12-12T01:00:43Z2019-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1007/s40314-019-0997-zComputational and Applied Mathematics, v. 39, n. 1, 2019.1807-03022238-3603http://hdl.handle.net/11449/19815610.1007/s40314-019-0997-z2-s2.0-85075175658990553971561964577409171447574100000-0002-2430-82400000-0003-1289-8332Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengComputational and Applied Mathematicsinfo:eu-repo/semantics/openAccess2021-10-23T10:26:19Zoai:repositorio.unesp.br:11449/198156Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T20:16:36.710485Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Study of collision probability considering a non-uniform cloud of space debris |
title |
Study of collision probability considering a non-uniform cloud of space debris |
spellingShingle |
Study of collision probability considering a non-uniform cloud of space debris Formiga, Jorge Kennety Silva [UNESP] Close approach Orbital maneuver Space debris Space trajectories |
title_short |
Study of collision probability considering a non-uniform cloud of space debris |
title_full |
Study of collision probability considering a non-uniform cloud of space debris |
title_fullStr |
Study of collision probability considering a non-uniform cloud of space debris |
title_full_unstemmed |
Study of collision probability considering a non-uniform cloud of space debris |
title_sort |
Study of collision probability considering a non-uniform cloud of space debris |
author |
Formiga, Jorge Kennety Silva [UNESP] |
author_facet |
Formiga, Jorge Kennety Silva [UNESP] Santos, Denilson Paulo Souza dos [UNESP] Fiore, Fabiana A. [UNESP] de Moraes, Rodolpho Vilhena Prado, Antonio Fernando Bertachini A. |
author_role |
author |
author2 |
Santos, Denilson Paulo Souza dos [UNESP] Fiore, Fabiana A. [UNESP] de Moraes, Rodolpho Vilhena Prado, Antonio Fernando Bertachini A. |
author2_role |
author author author author |
dc.contributor.none.fl_str_mv |
Universidade Estadual Paulista (Unesp) Universidade Federal de São Paulo (UNIFESP) National Institute for Space Research(INPE) |
dc.contributor.author.fl_str_mv |
Formiga, Jorge Kennety Silva [UNESP] Santos, Denilson Paulo Souza dos [UNESP] Fiore, Fabiana A. [UNESP] de Moraes, Rodolpho Vilhena Prado, Antonio Fernando Bertachini A. |
dc.subject.por.fl_str_mv |
Close approach Orbital maneuver Space debris Space trajectories |
topic |
Close approach Orbital maneuver Space debris Space trajectories |
description |
The present paper aims to study the cumulative collision probability of a target that crosses a cloud of particles that has the orbital parameters of each individual element modified by a close approach with the Earth. Clouds of this type are formed when natural or man-made bodies explode for some reason. After an explosion like that, the individual particles have different trajectories. The clouds are specified by a non-uniform distribution of semi-major axis and eccentricity of their particles which are assumed to pass close to the Earth, making a close approach that modifies the trajectory of every single particle that belongs to the cloud. This study makes simulations considering separately two different clouds based on the patched conics model to obtain the new trajectories of each particle and to analyze the density of the whole cloud. Then it is possible to map the new distribution of the orbital elements of the fragments that constituted the cloud, using the distribution as initial conditions. After calculating the spatial density for the whole cloud, it is possible to obtain the cumulative collision probability for one space vehicle that crosses the cloud. These pieces of information are important when planning satellite missions where a spacecraft passes close to a cloud of this type, because we can determine values to study the risks of collision and the possible maneuvers that need to be made to avoid them. |
publishDate |
2019 |
dc.date.none.fl_str_mv |
2019-01-01 2020-12-12T01:00:43Z 2020-12-12T01:00:43Z |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://dx.doi.org/10.1007/s40314-019-0997-z Computational and Applied Mathematics, v. 39, n. 1, 2019. 1807-0302 2238-3603 http://hdl.handle.net/11449/198156 10.1007/s40314-019-0997-z 2-s2.0-85075175658 9905539715619645 7740917144757410 0000-0002-2430-8240 0000-0003-1289-8332 |
url |
http://dx.doi.org/10.1007/s40314-019-0997-z http://hdl.handle.net/11449/198156 |
identifier_str_mv |
Computational and Applied Mathematics, v. 39, n. 1, 2019. 1807-0302 2238-3603 10.1007/s40314-019-0997-z 2-s2.0-85075175658 9905539715619645 7740917144757410 0000-0002-2430-8240 0000-0003-1289-8332 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Computational and Applied Mathematics |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.source.none.fl_str_mv |
Scopus reponame:Repositório Institucional da UNESP instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
instname_str |
Universidade Estadual Paulista (UNESP) |
instacron_str |
UNESP |
institution |
UNESP |
reponame_str |
Repositório Institucional da UNESP |
collection |
Repositório Institucional da UNESP |
repository.name.fl_str_mv |
Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
repository.mail.fl_str_mv |
|
_version_ |
1808129182414143488 |