Defunct Satellites in Nearly Polar Orbits: Long-term Evolution of Attitude Motion
Low Earth orbits (LEO) are known as a region of high space activity and, consequently, space debris highest density. Launcher upper stages and defunct satellites are the largest space debris objects, whose collisions can result in still greater pollution, rendering further space missions in LEO impo...
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Online Access: | https://doi.org/10.1515/astro-2018-0029 |
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doaj-990c40bbb89f49858b0053d8826434452021-09-06T19:40:14ZengDe GruyterOpen Astronomy2543-63762018-11-0127126427710.1515/astro-2018-0029astro-2018-0029Defunct Satellites in Nearly Polar Orbits: Long-term Evolution of Attitude MotionPritykin Dmitry0Efimov Sergey1Sidorenko Vladislav2Skolkovo Institute of Science and Technology,Skolkovo, RussiaMoscow Institute of Physics and Technology,Moscow, RussiaKeldysh Institute of Applied Mathematics, Russian Academy of Sciences,Keldysh, RussiaLow Earth orbits (LEO) are known as a region of high space activity and, consequently, space debris highest density. Launcher upper stages and defunct satellites are the largest space debris objects, whose collisions can result in still greater pollution, rendering further space missions in LEO impossible. Thus, space debris remediation is necessary, and the LEO region is a primary target of active debris removal (ADR) projects. However, ADR planning requires at least an approximate idea of the candidate objects’ attitude dynamics, which is one of the incentives for our study. This paper is mainly focused on modeling and simulating the attitude dynamics of defunct satellites. We consider a “boxwing” configuration satellite with an ellipsoid of inertia close to an oblate ellipsoid of revolution. The dynamical model takes into account the gravity-gradient torque, the torque due to the residual magnetic moment, and the torque due to eddy currents induced by the interaction of conductive materials with the geomagnetic field. A better understanding of the intermediate phase of the exponential deceleration and existing final regimes is achieved owing to a more accurate model of the eddy-current torque than in most prior research.We also show the importance of orbital precession, which contributes to the overall attitude motion evolution.https://doi.org/10.1515/astro-2018-0029space debrisattitude dynamicseddy-current torqueresidual magnetic moment |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Pritykin Dmitry Efimov Sergey Sidorenko Vladislav |
spellingShingle |
Pritykin Dmitry Efimov Sergey Sidorenko Vladislav Defunct Satellites in Nearly Polar Orbits: Long-term Evolution of Attitude Motion Open Astronomy space debris attitude dynamics eddy-current torque residual magnetic moment |
author_facet |
Pritykin Dmitry Efimov Sergey Sidorenko Vladislav |
author_sort |
Pritykin Dmitry |
title |
Defunct Satellites in Nearly Polar Orbits: Long-term Evolution of Attitude Motion |
title_short |
Defunct Satellites in Nearly Polar Orbits: Long-term Evolution of Attitude Motion |
title_full |
Defunct Satellites in Nearly Polar Orbits: Long-term Evolution of Attitude Motion |
title_fullStr |
Defunct Satellites in Nearly Polar Orbits: Long-term Evolution of Attitude Motion |
title_full_unstemmed |
Defunct Satellites in Nearly Polar Orbits: Long-term Evolution of Attitude Motion |
title_sort |
defunct satellites in nearly polar orbits: long-term evolution of attitude motion |
publisher |
De Gruyter |
series |
Open Astronomy |
issn |
2543-6376 |
publishDate |
2018-11-01 |
description |
Low Earth orbits (LEO) are known as a region of high space activity and, consequently, space debris highest density. Launcher upper stages and defunct satellites are the largest space debris objects, whose collisions can result in still greater pollution, rendering further space missions in LEO impossible. Thus, space debris remediation is necessary, and the LEO region is a primary target of active debris removal (ADR) projects. However, ADR planning requires at least an approximate idea of the candidate objects’ attitude dynamics, which is one of the incentives for our study. This paper is mainly focused on modeling and simulating the attitude dynamics of defunct satellites. We consider a “boxwing” configuration satellite with an ellipsoid of inertia close to an oblate ellipsoid of revolution. The dynamical model takes into account the gravity-gradient torque, the torque due to the residual magnetic moment, and the torque due to eddy currents induced by the interaction of conductive materials with the geomagnetic field. A better understanding of the intermediate phase of the exponential deceleration and existing final regimes is achieved owing to a more accurate model of the eddy-current torque than in most prior research.We also show the importance of orbital precession, which contributes to the overall attitude motion evolution. |
topic |
space debris attitude dynamics eddy-current torque residual magnetic moment |
url |
https://doi.org/10.1515/astro-2018-0029 |
work_keys_str_mv |
AT pritykindmitry defunctsatellitesinnearlypolarorbitslongtermevolutionofattitudemotion AT efimovsergey defunctsatellitesinnearlypolarorbitslongtermevolutionofattitudemotion AT sidorenkovladislav defunctsatellitesinnearlypolarorbitslongtermevolutionofattitudemotion |
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1717769036440272896 |