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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Main Authors: Pritykin Dmitry, Efimov Sergey, Sidorenko Vladislav
Format: Article
Language:English
Published: De Gruyter 2018-11-01
Series:Open Astronomy
Subjects:
Online Access:https://doi.org/10.1515/astro-2018-0029
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spelling 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
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AT efimovsergey defunctsatellitesinnearlypolarorbitslongtermevolutionofattitudemotion
AT sidorenkovladislav defunctsatellitesinnearlypolarorbitslongtermevolutionofattitudemotion
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